|
|
Line 1: |
Line 1: |
| {{Lists of Solar System objects}}
| | == New Balance Dame 420 hvis du er en marketingmedarbejder == |
| In 2006, the [[International Astronomical Union]] (IAU) defined a [[planet]] as a body in orbit around the [[Sun]] that was large enough to have achieved [[hydrostatic equilibrium]] and to have [[Clearing the neighbourhood|cleared the neighbourhood around its orbit]].<ref name=IAU0603>{{cite press release
| |
| |date=2006-08-24
| |
| |publisher=International Astronomical Union (News Release – IAU0603)
| |
| |title=IAU 2006 General Assembly: Result of the IAU Resolution votes
| |
| |url=http://www.iau.org/public_press/news/release/iau0603/
| |
| |accessdate=2007-12-31}} ([http://www.iau.org/iau0603.414.0.html orig link])</ref> An object in hydrostatic equilibrium is one that is large enough for its gravity to have overcome its internal rigidity, and so relax into a rounded ([[ellipsoid]]al) shape. The practical meaning of "cleared the neighborhood" is that a planet is comparatively massive enough for its gravitation to control the orbits of all objects in its vicinity. By the IAU's definition, there are eight planets in the [[Solar System]]. Those objects in orbit around the Sun that have achieved hydrostatic equilibrium but have not cleared their neighborhoods are called [[dwarf planet]]s, and the remainder are termed [[small Solar System body|small Solar System bodies]]. In addition, the Sun itself and a dozen or so [[natural satellite]]s are also massive enough to have achieved hydrostatic equilibrium.<ref name=mike/> Apart from the Sun, these bodies are included in the term ''planetary-mass object'', or ''planemo''. All known planetary-mass objects in the Solar System, as well as the Sun, are listed below, along with a sample of the largest objects whose shape has yet to be accurately determined. The Sun's orbital characteristics are listed in relation to the [[Galactic Center]]. All other objects are listed in order of their distance from the Sun. | |
|
| |
|
| == Sun ==
| | Men mange foodies ikke så store fans. Vi har alle denne bitre søde holdning lige nu om semesteret komme til en ende. Indsatsen for at genvinde resterne af Peking Man er blevet hånet af Fang Zhouzi, skriver i siderne i Beijing SciTech rapporten, en ugentlig tillæg på Beijing Youth Daily. <br><br>Vi har brug for svar på ovenstående spørgsmål. Producere backlinks vil give dig højere placeringer på søgemaskinen resultat sider og consenquently mere synlighed, men hvis din strategi består [http://www.jyskgenbrug.dk/images/file.asp?d=77-New-Balance-Dame-420 New Balance Dame 420] i [http://www.cuthouse.dk/new_backup/new/img/head/define.asp?g=27 Mbt Sko Slagelse] blot at indsende en artikel eller to hver uge, vil resultaterne sandsynligvis være ubetydelig, det er derfor du absolut bør investere [http://www.trykpaatoej.dk/content/frame.asp?rayban=66 Køb Ray Ban New Wayfarer] nogle penge i artiklen indsendelse tjenester . <br><br>"For deres vedkommende, har mange små virksomheder set deres kassekredit reduceres eller elimineres, eller de har været i stand til at opnå kredit kun på betydeligt mere restriktive vilkår," Bernanke sagde. Jeg iagttog indgående hits til virksomhedens websted på min Google Analytics-rapporten, og var nysgerrig efter at se den stigende hits fra en Google-søgning for mit firma navn. <br><br>Da jeg første gang stødte på Fluxbox, var jeg kommer fra den forkerte vinkel. Der er bogstaveligt talt et ubegrænset antal andre social networking websites som du kan deltage [http://www.trykpaatoej.dk/content/frame.asp?rayban=58 Ray Ban Solbriller Aviator] .... Få 2 eller flere hold linet op foran tavle. N form af sidevisninger, er vi næsten tre gange større, at dem. <br><br>Denne løsning var en succes på grund af standardisering, men yderst begrænset i den måde oplysninger kan hentes og bruges.. Hvis du interesseret i at lære mere om sociale medier og marketing, dette er artiklen for dig! Prøv at bruge YouTube som del af markedsføringen, du bruger til sociale medier, for at hjælpe tiltrække særlige seerne til din hjemmeside. <br><br>Men dette var langt mere end en dårligt valgt Twitter indlæg og indlæg var detaljeret, langvarige og talrige .. Med pædiatrisk eksklusivitet dette at tage kreatin Korrekt Castro til magten tusinder. Ulempen er, at der er en setup gebyr på omkring 10,00, men for hvad du får det er vel det værd. <br><br>Hey, ethvert websted med en bopæl klummeskribent, der går af Bunches er fint med mig. Der er nogle særlige bøger og leksika, som du kan tænke på. Næsten alle kender nogen, der bygger hjemmesider og nogle af dem er meget gode til hvad de gør. De forventer højere kvalitet artikler. <br><br>I dag har vi afsløret Konverteringsoptimering vores nye værktøj til at gennemføre flerdimensionale og A / B-test. Nu, hvis du er en marketingmedarbejder, og du vil have dem til at købe dit produkt efter at have læst artiklen, så kan du ikke give væk i butikken i selve artiklen.<ul> |
| The Sun is a [[G-type main-sequence star]]. It contains almost 99.9 percent of all the mass in the Solar System.<ref>{{cite journal |author=M Woolfson |title=The origin and evolution of the solar system | doi= 10.1046/j.1468-4004.2000.00012.x |year=2000 |journal=Astronomy & Geophysics |volume=41 |issue=1 |pages=1.12 |bibcode = 2000A&G....41a..12W }}</ref>
| | |
| {| class="wikitable" border="1" style="text-align: center;"
| | <li>[http://www.k8383.com/news/html/?669666.html http://www.k8383.com/news/html/?669666.html]</li> |
| |-
| | |
| ! colspan="2" style="background: #fffdd0;" |
| | <li>[http://galleri.kjerringoy.no/displayimage.php?album=155&pos=46 http://galleri.kjerringoy.no/displayimage.php?album=155&pos=46]</li> |
| ! style="background: yellow;" | [[Sun]]<ref>[http://solarsystem.nasa.gov/planets/profile.cfm?Object=Sun&Display=Facts&System=Metric NASA Solar System exploration Sun factsheet] and [http://nssdc.gsfc.nasa.gov/planetary/factsheet/sunfact.html NASA Sun factsheet] ''NASA'' Retrieved on 2008-11-17 (unless otherwise cited)</ref>
| | |
| |-
| | <li>[http://www.163sy.com/home.php?mod=spacecp&ac=blog&blogid= http://www.163sy.com/home.php?mod=spacecp&ac=blog&blogid=]</li> |
| | colspan="2" style="background: #fffdd0;" |
| | |
| | style="background: yellow;" | [[File:The Sun by the Atmospheric Imaging Assembly of NASA's Solar Dynamics Observatory - 20100801.jpg|70px]]
| | <li>[http://hablaameno.com/index.php/ http://hablaameno.com/index.php/]</li> |
| |-
| | |
| | colspan="2" style="background: #fffdd0;" | [[Astronomical symbol|Astronomical symbol]]{{ref label|Q|q|none}}
| | <li>[http://www.metransparent.com/spip.php?article9653&lang=ar&id_forum=11085/ http://www.metransparent.com/spip.php?article9653&lang=ar&id_forum=11085/]</li> |
| | style="background: yellow;" | [[File:Sun symbol.svg|20px|Sun]]
| | |
| |-
| | </ul> |
| | style="background: #fffdd0;" | Mean distance <br /> from [[Galactic Center]]
| |
| | style="background: #fffdd0;" | km <br /> [[light years]]
| |
| | style="background: yellow;" | ~2.5{{e|17}} <br /> ~26,000
| |
| |-
| |
| | style="background: #fffdd0;" | Mean [[radius]]
| |
| | style="background: #fffdd0;" | km <br /> :E{{ref label|F|f|none}}
| |
| | style="background: yellow;" | 696,000 <br /> 109
| |
| |-
| |
| | style="background: #fffdd0;" | [[Surface area]]
| |
| | style="background: #fffdd0;" | km<sup>2</sup> <br /> :E{{ref label|F|f|none}}
| |
| | style="background: yellow;" | 6.0877{{e|12}} <br /> 11,990
| |
| |-
| |
| | style="background: #fffdd0;" | [[Volume]]
| |
| | style="background: #fffdd0;" | km<sup>3</sup> <br /> :E{{ref label|F|f|none}}
| |
| | style="background: yellow;" | 1.4122{{e|18}} <br /> 1,300,000
| |
| |-
| |
| | style="background: #fffdd0;" | [[Mass]]
| |
| | style="background: #fffdd0;" | [[Kilogram|kg]] <br /> :E{{ref label|F|f|none}}
| |
| | style="background: yellow;" | 1.9891{{e|30}} <br /> 332,946
| |
| |-
| |
| | style="background: #fffdd0;" | [[Density]]
| |
| | style="background: #fffdd0;" | [[Gram|g]]/cm<sup>3</sup>
| |
| | style="background: yellow;" | 1.409
| |
| |-
| |
| | style="background: #fffdd0;" | [[Equator]]ial [[gravity]]
| |
| | style="background: #fffdd0;" | [[Acceleration|m/s<sup>2</sup>]]
| |
| | style="background: yellow;" | 274.0
| |
| |-
| |
| | style="background: #fffdd0;" | [[Escape velocity]]
| |
| | style="background: #fffdd0;" | [[Speed|km/s]]
| |
| | style="background: yellow;" | 617.7
| |
| |-
| |
| | style="background: #fffdd0;" | Rotation period
| |
| | style="background: #fffdd0;" | days{{ref label|G|g|none}}
| |
| | style="background: yellow;" | 25.38
| |
| |-
| |
| | style="background: #fffdd0;" | [[Galactic year|Orbital period]] about Galactic Center<ref name=sun>{{cite web | url=http://hypertextbook.com/facts/2002/StacyLeong.shtml|work=[http://hypertextbook.com/facts/ The Physics Factbook] (self-published)| author=Stacy Leong| editor=Glenn Elert (ed.) | year=2002|title=Period of the Sun's Orbit around the Galaxy (Cosmic Year) | accessdate=2008-06-26}}</ref>
| |
| | style="background: #fffdd0;" | million years
| |
| | style="background: yellow;" | 225–250
| |
| |-
| |
| | style="background: #fffdd0;" | Mean orbital speed<ref name=sun/>
| |
| | style="background: #fffdd0;" | [[Speed|km/s]]
| |
| | style="background: yellow;" | ~220
| |
| |-
| |
| | style="background: #fffdd0;" | [[Axial tilt]]{{ref label|I|i|none}} to the ecliptic
| |
| | style="background: #fffdd0;" | [[Degree (angle)|deg.]]
| |
| | style="background: yellow;" | 7.25
| |
| |-
| |
| | style="background: #fffdd0;" | [[Axial tilt]]{{ref label|I|i|none}} to the galactic plane
| |
| | style="background: #fffdd0;" | [[Degree (angle)|deg.]]
| |
| | style="background: yellow;" | 67.23
| |
| |-
| |
| | style="background: #fffdd0;" | Mean surface [[temperature]]
| |
| | style="background: #fffdd0;" | [[Kelvin|K]]
| |
| | style="background: yellow;" | 5,778
| |
| |-
| |
| | style="background: #fffdd0;" | Mean [[corona]]l [[temperature]]<ref>{{cite book|title=Encyclopedia of the Solar System|editor=Lucy Ann McFadden, Paul R. Weissman, Torrence V. Johnsson|chapter=The Sun|page=80|author=Markus J. Aschwanden|year=2007|publisher=Academic Press}}</ref>
| |
| | style="background: #fffdd0;" | [[Kelvin|K]]
| |
| | style="background: yellow;" | 1–2{{e|6}}
| |
| |-
| |
| | colspan="2" style="background: #fffdd0;" | [[Photosphere|Photospheric]] composition
| |
| | style="background: yellow;" | [[Hydrogen|H]], [[Helium|He]], [[Oxygen|O]], [[Carbon|C]], [[Iron|Fe]], [[Sulphur|S]]
| |
| |}
| |
|
| |
|
| == Planets == | | == New Balance 574 Børn dage i en uge == |
| <div style="float: right; margin: 5px;">
| |
| {| class="wikitable" border="1"
| |
| |-
| |
| ! style="background: #eaeaea" colspan="6" | Key
| |
| |-
| |
| | bgcolor="#eeffee" width=50 style="text-align: left" |* <br /> [[terrestrial planet]]
| |
| | bgcolor="#fffAee" width=50 style="text-align: left" |° <br /> [[gas giant]]
| |
| |}</div>
| |
| [[Planet]]s are both large enough to have achieved [[hydrostatic equilibrium]] and have [[cleared their neighborhood]]s of similar objects. There are four [[terrestrial planet]]s and four [[gas giant]]s in the Solar System. The latter combined comprise more than 99 percent of the mass in the Solar System excluding that of the Sun.
| |
| {| class="wikitable" border="1" style="text-align: center;"
| |
| |-
| |
| ! colspan="2" style="background: #fffdd0;" |
| |
| ! style="background: #efe;" | *[[Mercury (planet)|Mercury]]<ref>[http://nssdc.gsfc.nasa.gov/planetary/factsheet/mercuryfact.html NASA Mercury Fact Sheet] and [http://solarsystem.nasa.gov/planets/profile.cfm?Object=Mercury&Display=Facts NASA Solar System Exploration Factsheet] ''NASA'' Retrieved on 2008-11-17 (unless otherwise cited)</ref>
| |
| ! style="background: #efe;" | *[[Venus]]<ref>[http://nssdc.gsfc.nasa.gov/planetary/factsheet/venusfact.html NASA Venus Factsheet] and [http://sse.jpl.nasa.gov/planets/profile.cfm?Object=Venus&Display=Facts&System=Metric NASA Solar System Exploration Factsheet] ''NASA'' Retrieved on 2008-11-17 (unless otherwise cited)</ref>
| |
| ! style="background: #efe;" | *[[Earth]]<ref name=Earth>[http://nssdc.gsfc.nasa.gov/planetary/factsheet/earthfact.html NASA Earth factsheet] and [http://sse.jpl.nasa.gov/planets/profile.cfm?Object=Earth&Display=Facts&System=Metric NASA Solar System Exploration Factsheet] ''NASA'' Retrieved on 2008-11-17 (unless otherwise cited)</ref>
| |
| ! style="background: #efe;" | *[[Mars]]<ref>[http://nssdc.gsfc.nasa.gov/planetary/factsheet/marsfact.html NASA Mars Factsheet] and [http://solarsystem.jpl.nasa.gov/planets/profile.cfm?Object=Mars&Display=Facts&System=Metric NASA Mars Solar System Exploration Factsheet] ''NASA'' Retrieved on 2008-11-17 (unless otherwise cited)</ref>
| |
| ! style="background: #fffaee;" | °[[Jupiter]]<ref>[http://nssdc.gsfc.nasa.gov/planetary/factsheet/jupiterfact.html NASA Jupiter factsheet] and [http://solarsystem.nasa.gov/planets/profile.cfm?Object=Jupiter&Display=Facts NASA Solar System Exploration Factsheet] ''NASA'' Retrieved on 2008-11-17 (unless otherwise cited)</ref>
| |
| ! style="background: #fffaee;" | °[[Saturn]]<ref>[http://nssdc.gsfc.nasa.gov/planetary/factsheet/saturnfact.html NASA Saturn factsheet] and [http://solarsystem.nasa.gov/planets/profile.cfm?Object=Saturn&Display=Facts NASA Solar System Exploration Saturn Factsheet] ''NASA'' Retrieved on 2008-11-17 (unless otherwise cited)</ref>
| |
| ! style="background: #fffaee;" | °[[Uranus]]<ref>[http://nssdc.gsfc.nasa.gov/planetary/factsheet/uranusfact.html NASA Uranus factsheet] and [http://solarsystem.nasa.gov/planets/profile.cfm?Object=Uranus&Display=Facts NASA Solar System Exploration Uranus Factsheet] ''NASA'' Retrieved on 2008-11-17 (unless otherwise cited)</ref>
| |
| ! style="background: #fffaee;" | °[[Neptune]]<ref>[http://nssdc.gsfc.nasa.gov/planetary/factsheet/neptunefact.html NASA Neptune factsheet] and [http://solarsystem.nasa.gov/planets/profile.cfm?Object=Neptune&Display=Facts NASA Solar System Exploration Neptune Factsheet] ''NASA'' Retrieved on 2008-11-17 (unless otherwise cited)</ref>
| |
| |-
| |
| | colspan="2" style="background: #fffdd0;" |
| |
| | style="background: #efe;" | [[File:Reprocessed Mariner 10 image of Mercury.jpg|75px]]
| |
| | style="background: #efe;" | [[File:Venus globe.jpg|70px]]
| |
| | style="background: #efe;" | [[File:The Earth seen from Apollo 17.jpg|70px]]
| |
| | style="background: #efe;" | [[File:Mars Valles Marineris.jpeg|70px]]
| |
| | style="background: #fffaee;" | [[File:Jupiter.jpg|70px]]
| |
| | style="background: #fffaee;" | [[File:Saturn (planet) large.jpg|70px]]
| |
| | style="background: #fffaee;" | [[File:Uranus2.jpg|70px]]
| |
| | style="background: #fffaee;" | [[File:Neptune.jpg|70px]]
| |
| |-
| |
| | colspan="2" style="background: #fffdd0;" | [[Astronomical symbol|Astronomical symbol]]{{ref label|Q|q|none}}
| |
| | style="background: #efe;" | [[File:Mercury symbol.svg|20px|Mercury]]
| |
| | style="background: #efe;" | [[File:Venus symbol.svg|20px|Venus]]
| |
| | style="background: #efe;" | [[File:Earth symbol.svg|20px|Earth]]
| |
| | style="background: #efe;" | [[File:Mars symbol.svg|20px|Mars]]
| |
| | style="background: #fffaee;" | [[File:Jupiter symbol.svg|20px|Jupiter]]
| |
| | style="background: #fffaee;" | [[File:Saturn symbol.svg|20 px|Saturn]]
| |
| | style="background: #fffaee;" | [[File:Uranus symbol.svg|20px|Uranus]]
| |
| | style="background: #fffaee;" | [[File:Neptune symbol.svg|20px|Neptune]]
| |
| |-
| |
| | style="background: #fffdd0;" | [[Semimajor axis|Mean distance]] <br /> from [[Sun]]
| |
| | style="background: #fffdd0;" | km <br /> [[Astronomical unit|AU]]
| |
| | style="background: #efe;" | 57,909,175 <br /> 0.38709893
| |
| | style="background: #efe;" | 108,208,930 <br /> 0.72333199
| |
| | style="background: #efe;" | 149,597,890 <br /> 1.00000011
| |
| | style="background: #efe;" | 227,936,640 <br /> 1.52366231
| |
| | style="background: #fffaee;" | 778,412,010 <br /> 5.20336301
| |
| | style="background: #fffaee;" | 1,426,725,400 <br /> 9.53707032
| |
| | style="background: #fffaee;" | 2,870,972,200 <br /> 19.19126393
| |
| | style="background: #fffaee;" | 4,498,252,900 <br /> 30.06896348
| |
| |-
| |
| | style="background: #fffdd0;" | Equatorial [[radius]]
| |
| | style="background: #fffdd0;" | km <br /> :E{{ref label|F|f|none}}
| |
| | style="background: #efe;" | 2,439.64 <br /> 0.3825
| |
| | style="background: #efe;" | 6,051.59 <br /> 0.9488
| |
| | style="background: #efe;" | 6,378.1 <br /> 1
| |
| | style="background: #efe;" | 3,397.00 <br /> 0.53226
| |
| | style="background: #fffaee;" | 71,492.68 <br /> 11.209
| |
| | style="background: #fffaee;" | 60,267.14 <br /> 9.449
| |
| | style="background: #fffaee;" | 25,557.25 <br /> 4.007
| |
| | style="background: #fffaee;" | 24,766.36 <br /> 3.883
| |
| |-
| |
| | style="background: #fffdd0;" | [[Surface area]]
| |
| | style="background: #fffdd0;" | km² <br /> :E{{ref label|F|f|none}}
| |
| | style="background: #efe;" | 75,000,000 <br /> 0.1471
| |
| | style="background: #efe;" | 460,000,000 <br /> 0.9010
| |
| | style="background: #efe;" | 510,000,000 <br /> 1
| |
| | style="background: #efe;" | 140,000,000 <br /> 0.2745
| |
| | style="background: #fffaee;" | 64,000,000,000 <br /> 125.5
| |
| | style="background: #fffaee;" | 44,000,000,000 <br /> 86.27
| |
| | style="background: #fffaee;" | 8,100,000,000 <br /> 15.88
| |
| | style="background: #fffaee;" | 7,700,000,000 <br /> 15.10
| |
| |-
| |
| | style="background: #fffdd0;" | [[Volume]]
| |
| | style="background: #fffdd0;" | km<sup>3</sup> <br /> :E{{ref label|F|f|none}}
| |
| | style="background: #efe;" | 6.083{{e|10}} <br /> 0.056
| |
| | style="background: #efe;" | 9.28{{e|11}} <br /> 0.87
| |
| | style="background: #efe;" | 1.083{{e|12}} <br /> 1
| |
| | style="background: #efe;" | 1.6318{{e|11}} <br /> 0.151
| |
| | style="background: #fffaee;" | 1.431{{e|15}} <br /> 1,321.3
| |
| | style="background: #fffaee;" | 8.27{{e|14}} <br /> 763.59
| |
| | style="background: #fffaee;" | 6.834{{e|13}} <br /> 63.086
| |
| | style="background: #fffaee;" | 6.254{{e|13}} <br /> 57.74
| |
| |-
| |
| | style="background: #fffdd0;" | [[Mass]]
| |
| | style="background: #fffdd0;" | [[Kilogram|kg]] <br /> :E{{ref label|F|f|none}}
| |
| | style="background: #efe;" | 3.302{{e|23}} <br /> 0.055
| |
| | style="background: #efe;" | 4.8690{{e|24}} <br /> 0.815
| |
| | style="background: #efe;" | 5.9742{{e|24}} <br /> 1
| |
| | style="background: #efe;" | 6.4191{{e|23}} <br /> 0.107
| |
| | style="background: #fffaee;" | 1.8987{{e|27}} <br /> 318
| |
| | style="background: #fffaee;" | 5.6851{{e|26}} <br /> 95
| |
| | style="background: #fffaee;" | 8.6849{{e|25}} <br /> 14
| |
| | style="background: #fffaee;" | 1.0244{{e|26}} <br /> 17
| |
| |-
| |
| | style="background: #fffdd0;" | [[Density]]
| |
| | style="background: #fffdd0;" | [[Gram|g]]/cm<sup>3</sup>
| |
| | style="background: #efe;" | 5.43
| |
| | style="background: #efe;" | 5.24
| |
| | style="background: #efe;" | 5.515
| |
| | style="background: #efe;" | 3.940
| |
| | style="background: #fffaee;" | 1.33
| |
| | style="background: #fffaee;" | 0.70
| |
| | style="background: #fffaee;" | 1.30
| |
| | style="background: #fffaee;" | 1.76
| |
| |-
| |
| | style="background: #fffdd0;" | [[Equator]]ial [[gravity]]
| |
| | style="background: #fffdd0;" | [[Acceleration|m/s<sup>2</sup>]]
| |
| | style="background: #efe;" | 3.70
| |
| | style="background: #efe;" | 8.87
| |
| | style="background: #efe;" | 9.81
| |
| | style="background: #efe;" | 3.71
| |
| | style="background: #fffaee;" | 23.12
| |
| | style="background: #fffaee;" | 10.44
| |
| | style="background: #fffaee;" | 8.69
| |
| | style="background: #fffaee;" | 11.00
| |
| |-
| |
| | style="background: #fffdd0;" | [[Escape velocity]]
| |
| | style="background: #fffdd0;" | [[Speed|km/s]]
| |
| | style="background: #efe;" | 4.25
| |
| | style="background: #efe;" | 10.36
| |
| | style="background: #efe;" | 11.18
| |
| | style="background: #efe;" | 5.02
| |
| | style="background: #fffaee;" | 59.54
| |
| | style="background: #fffaee;" | 35.49
| |
| | style="background: #fffaee;" | 21.29
| |
| | style="background: #fffaee;" | 23.71
| |
| |-
| |
| | style="background: #fffdd0;" | Rotation period{{ref label|G|g|none}}
| |
| | style="background: #fffdd0;" | days
| |
| | style="background: #efe;" | 58.646225
| |
| | style="background: #efe;" | −243.0187{{ref label|H|h|none}}
| |
| | style="background: #efe;" | 0.99726968
| |
| | style="background: #efe;" | 1.02595675
| |
| | style="background: #fffaee;" | 0.41354
| |
| | style="background: #fffaee;" | 0.44401
| |
| | style="background: #fffaee;" | −0.71833{{ref label|H|h|none}}
| |
| | style="background: #fffaee;" | 0.67125
| |
| |-
| |
| | style="background: #fffdd0;" | Orbital period{{ref label|G|g|none}}
| |
| | style="background: #fffdd0;" | [[Julian year (astronomy)|years]]
| |
| | style="background: #efe;" | 0.2408467
| |
| | style="background: #efe;" | 0.61519726
| |
| | style="background: #efe;" | 1.0000174
| |
| | style="background: #efe;" | 1.8808476
| |
| | style="background: #fffaee;" | 11.862615
| |
| | style="background: #fffaee;" | 29.447498
| |
| | style="background: #fffaee;" | 84.016846
| |
| | style="background: #fffaee;" | 164.79132
| |
| |-
| |
| | style="background: #fffdd0;" | Mean orbital speed
| |
| | style="background: #fffdd0;" | [[Speed|km/s]]
| |
| | style="background: #efe;" | 47.8725
| |
| | style="background: #efe;" | 35.0214
| |
| | style="background: #efe;" | 29.7859
| |
| | style="background: #efe;" | 24.1309
| |
| | style="background: #fffaee;" | 13.0697
| |
| | style="background: #fffaee;" | 9.6724
| |
| | style="background: #fffaee;" | 6.8352
| |
| | style="background: #fffaee;" | 5.4778
| |
| |-
| |
| | colspan="2" style="background: #fffdd0;" | [[Eccentricity (orbit)|Eccentricity]]
| |
| | style="background: #efe;" | 0.20563069
| |
| | style="background: #efe;" | 0.00677323
| |
| | style="background: #efe;" | 0.01671022
| |
| | style="background: #efe;" | 0.09341233
| |
| | style="background: #fffaee;" | 0.04839266
| |
| | style="background: #fffaee;" | 0.05415060
| |
| | style="background: #fffaee;" | 0.04716771
| |
| | style="background: #fffaee;" | 0.00858587
| |
| |-
| |
| | style="background: #fffdd0;" | [[Inclination]]{{ref label|F|f|none}}
| |
| | style="background: #fffdd0;" | [[Degree (angle)|deg.]]
| |
| | style="background: #efe;" | 7.00
| |
| | style="background: #efe;" | 3.39
| |
| | style="background: #efe;" | 0<ref name=Earth/>
| |
| | style="background: #efe;" | 1.85
| |
| | style="background: #fffaee;" | 1.31
| |
| | style="background: #fffaee;" | 2.48
| |
| | style="background: #fffaee;" | 0.76
| |
| | style="background: #fffaee;" | 1.77
| |
| |-
| |
| | style="background: #fffdd0;" | [[Axial tilt]]{{ref label|I|i|none}}
| |
| | style="background: #fffdd0;" | [[Degree (angle)|deg.]]
| |
| | style="background: #efe;" | 0.0
| |
| | style="background: #efe;" | 177.3
| |
| | style="background: #efe;" | 23.44
| |
| | style="background: #efe;" | 25.19
| |
| | style="background: #fffaee;" | 3.12
| |
| | style="background: #fffaee;" | 26.73
| |
| | style="background: #fffaee;" | 97.86
| |
| | style="background: #fffaee;" | 29.58
| |
| |-
| |
| | style="background: #fffdd0;" | Mean surface [[temperature]]
| |
| | style="background: #fffdd0;" | [[Kelvin|K]]
| |
| | style="background: #efe;" | 440–100
| |
| | style="background: #efe;" | 730
| |
| | style="background: #efe;" | 287
| |
| | style="background: #efe;" | 227
| |
| | style="background: #fffaee;" | 152 {{ref label|J|j|none}}
| |
| | style="background: #fffaee;" | 134 {{ref label|J|j|none}}
| |
| | style="background: #fffaee;" | 72 {{ref label|J|j|none}}
| |
| | style="background: #fffaee;" | 76 {{ref label|J|j|none}}
| |
| |-
| |
| | style="background: #fffdd0;" | Mean air [[temperature]]{{ref label|K|k|none}}
| |
| | style="background: #fffdd0;" | [[Kelvin|K]]
| |
| | style="background: #efe;" |
| |
| | style="background: #efe;" |
| |
| | style="background: #efe;" | 288
| |
| | style="background: #efe;" |
| |
| | style="background: #fffaee;" | 165
| |
| | style="background: #fffaee;" | 135
| |
| | style="background: #fffaee;" | 73
| |
| | style="background: #fffaee;" | 76
| |
| |-
| |
| | colspan="2" style="background: #fffdd0;" | [[Atmosphere|Atmospheric]] composition
| |
| | style="background: #efe;" | [[Helium|He]] [[Sodium|Na]]<sup>+</sup> [[Phosphorus|P]]<sup>+</sup>
| |
| | style="background: #efe;" | [[Carbon dioxide|CO<sub>2</sub>]] [[Nitrogen|N<sub>2</sub>]]
| |
| | style="background: #efe;" | [[Nitrogen|N<sub>2</sub>]] [[Oxygen|O<sub>2</sub>]]
| |
| | style="background: #efe;" | CO<sub>2</sub> N<sub>2</sub> [[Argon|Ar]]
| |
| | style="background: #fffaee;" | [[Hydrogen|H<sub>2</sub>]] He
| |
| | style="background: #fffaee;" | H<sub>2</sub> He
| |
| | style="background: #fffaee;" | H<sub>2</sub> He [[Methane|CH<sub>4</sub>]]
| |
| | style="background: #fffaee;" | H<sub>2</sub> He CH<sub>4</sub>
| |
| |-
| |
| | colspan="2" style="background: #fffdd0;" | Number of known [[Natural satellite|moons]]{{ref label|V|v|none}}
| |
| | style="background: #efe;" | 0
| |
| | style="background: #efe;" | 0
| |
| | style="background: #efe;" | [[Moon|1]]
| |
| | style="background: #efe;" | [[Moons of Mars|2]]
| |
| | style="background: #fffaee;" | [[Moons of Jupiter|67]]
| |
| | style="background: #fffaee;" | [[Moons of Saturn|62]]
| |
| | style="background: #fffaee;" | [[Moons of Uranus|27]]
| |
| | style="background: #fffaee;" | [[Moons of Neptune|13]]
| |
| |-
| |
| | colspan="2" style="background: #fffdd0;" | [[Planetary ring|Rings?]]
| |
| | style="background: #efe;" | No
| |
| | style="background: #efe;" | No
| |
| | style="background: #efe;" | No
| |
| | style="background: #efe;" | No
| |
| | style="background: #fffaee;" | [[Rings of Jupiter|Yes]]
| |
| | style="background: #fffaee;" | [[Rings of Saturn|Yes]]
| |
| | style="background: #fffaee;" | [[Rings of Uranus|Yes]]
| |
| | style="background: #fffaee;" | [[Rings of Neptune|Yes]]
| |
| |-
| |
| | colspan="2" style="background: #fffdd0;" | [[Clearing the neighbourhood|Planetary discriminant]]{{ref label|L|l|none}}{{ref label|O|o|none}}
| |
| | style="background: #efe;" | 9.1{{e|4}}
| |
| | style="background: #efe;" | 1.35{{e|6}}
| |
| | style="background: #efe;" | 1.7{{e|6}}
| |
| | style="background: #efe;" | 1.8{{e|5}}
| |
| | style="background: #fffaee;" | 6.25{{e|5}}
| |
| | style="background: #fffaee;" | 1.9{{e|5}}
| |
| | style="background: #fffaee;" | 2.9{{e|4}}
| |
| | style="background: #fffaee;" | 2.4{{e|4}}
| |
| |}
| |
|
| |
|
| == Dwarf planets == | | Sure, satte intheknow Mac fyr Jim Dalrymple kibosh på longrumored endnu marginalt hopedfor dedikeret spil controller til iOS-enheder stor skuffelse for dem af os håb om at opleve glæden ved en fuld iRacing rig hooked op til en 90x50 gitter af iPhones. <br><br>Vælg mellem en række temaer med forskellige scavenger elementer og sjove aktiviteter, som du går.. Hvert 20. Du kan være nødt til at være fleksibel med måltider du forbereder at sørge for dit barn får en afbalanceret kost. EF-rammebestemmelserne. Jeg blev bedt om nogle spørgsmål om C siden sagde jeg til intervieweren, at jeg er mere komfortable med ca. <br><br>Som for løn, optjener deres ansatte inden for området af $ 87550 og fra det øjeblik er der 150 ledige [http://www.jyskgenbrug.dk/images/file.asp?d=34-New-Balance-574-Børn New Balance 574 Børn] job baseret på deres site. I dag, nedlæggelse smerter af faderen fra skilsmisse er en af de vigtigste kilder til mandlig mistillid hos kvinder, der udvikler en ubevidst angst for at blive såret, da de så deres mødre såret af deres fædre.. <br><br>Vi havde også injektioner. Portalen tilbyder 12 uger udfordringer, der sigter på at øge aktiviteten for ActiveLink brugere over tid. Produkt Detaljer Vare Vægt: 3 pounds Vægt: 3 pounds (Se fragtpriser Weight Watchers point list Bare gå til den vigtigste Market Samurai skærmen, starte et nyt projekt, og skriv domænenavnet i stedet for et søgeord sætning derefter gå til... <br><br>"Jeg har personligt været ret trist på industriens adfærd omkring alle disse ting. I modsætning til parring toppe og bunde at udforme et komplet udseende, ligger udfordringen i at vælge en kjole i at vælge en enestående beklædningsgenstand, der symboliserer [http://www.trykpaatoej.dk/content/frame.asp?rayban=52 Ray Ban Solbriller Med Styrke] den lejlighed, indeholder de nuværende tendenser, og oversætter en kvindes unikke kvindelighed til alle.. <br><br>Det er ligegyldigt, hvor mange timer der er på en dag, dage i en uge, måneder i et år, kan vi simpelthen ikke gøre alle de tings, vi gerne vil gøre.. Livet i de besatte områder i Palæstina er blevet reduceret generelt en aldeles forringet form for kollektiv fængsel. <br><br>Når du er blevet abonnent på parabol netværk, vil du ikke have noget at afbryde den fantastiske satellit-tv-programmering, som du hurtigt vil vokse vant til. Piloten, inspireret af virkelige begivenheder, der er skrevet af Chris Black and executiveproduced af Martin Campbell for ABC Studios.. <br><br>Tackle nye fitness udfordringer Ifølge fitness redaktør Martha LoureyBird, hvis du har fem kilo at tabe, det hele handler om at blande tingene op. Hun kiggede på ham i det øjeblik, han vendte [http://www.trykpaatoej.dk/content/frame.asp?rayban=18 Ray Ban Briller Til Børn] at se på hende. Grand Mega Resort Spa. Vi fløj gennem Philadelphia ud af Seattle og fra hvad de lokale fortæller [http://www.trykpaatoej.dk/content/frame.asp?rayban=77 Ray Ban Danmark Priser] os, Philadelphia er berygtet for mistet bagage..<ul> |
| <div style="float: right; margin: 5px;"> | | |
| {| class="wikitable" border="1"
| | <li>[http://www.jamiatou.com/spip.php?article21 http://www.jamiatou.com/spip.php?article21]</li> |
| |-
| | |
| ! style="background: #eaeaea" colspan=6|Key
| | <li>[http://www.cclchinese.com/?action-viewcomment-type-news-itemid-8160 http://www.cclchinese.com/?action-viewcomment-type-news-itemid-8160]</li> |
| |-
| | |
| | bgcolor="#f0dc82" width=50 style="text-align: left" |<sup>†</sup> <br> Ceres
| | <li>[http://www.film-video-dvd-production.com/spip.php?article6/ http://www.film-video-dvd-production.com/spip.php?article6/]</li> |
| | bgcolor="#eeffff" width=50 style="text-align: left" |<sup>‡</sup> <br> [[plutoid]]
| | |
| |}</div>
| | <li>[http://ldsbee.com/index.php?page=item&id=2134763 http://ldsbee.com/index.php?page=item&id=2134763]</li> |
| | |
| | <li>[http://222.243.160.155/forum.php?mod=viewthread&tid=7117293&fromuid=136374 http://222.243.160.155/forum.php?mod=viewthread&tid=7117293&fromuid=136374]</li> |
| | |
| | </ul> |
|
| |
|
| [[Dwarf planet]]s are large enough to have achieved [[hydrostatic equilibrium]], but have not cleared their neighbourhoods of similar objects. There are currently five dwarf planets recognized by the IAU in this category. [[Ceres (dwarf planet)|Ceres]] orbits in the [[asteroid belt]], between the orbits of [[Mars]] and [[Jupiter]]. The others orbit beyond Neptune and are sub-classified as [[plutoid]]s.
| | == Ray Ban Solbriller Til Mænd Jeg ser masser af emner == |
| {| class="wikitable" border="1" style="text-align: center;"
| |
| |-
| |
| ! colspan="2" style="background: #fffdd0;" |
| |
| ! style="background: #f0dc82;" | <sup>†</sup>{{dwarfplanet|Ceres}}<ref>{{cite web|title=NASA Asteroid Factsheet|url=http://nssdc.gsfc.nasa.gov/planetary/factsheet/asteroidfact.html|accessdate=2008-11-17|work=NASA}}</ref>
| |
| ! style="background: #eff;" | <sup>‡</sup>{{dwarfplanet|Pluto}}<ref name=Pluto>[http://nssdc.gsfc.nasa.gov/planetary/factsheet/plutofact.html NASA Pluto factsheet] and [http://solarsystem.nasa.gov/planets/profile.cfm?Object=Pluto&Display=Facts NASA Solar System Exploration Pluto Factsheet] Retrieved on 2008-11-17 (unless otherwise cited)</ref>
| |
| ! style="background: #eff;" | <sup>‡</sup>{{dwarfplanet|Haumea}}<ref>(i){{cite journal|author=D. L. Rabinowitz, K. M. Barkume, M. E. Brown, H. G. Roe, M. Schwartz, S. W. Tourtellotte, C. A. Trujillo|year= 2006|title=Photometric Observations Constraining the Size, Shape, and Albedo of 2003 EL61, a Rapidly Rotating, Pluto-Sized Object in the Kuiper Belt|journal=The Astrophysical Journal|volume= 639|issue=2 |pages=1238–1251| doi=10.1086/499575|bibcode=2006ApJ...639.1238R|arxiv = astro-ph/0509401 }} <br> (ii){{cite web|title=Jet Propulsion Laboratory Small-Body Database Browser: 136108 Haumea|publisher=NASA's Jet Propulsion Laboratory (2008-05-10 last obs)|url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=136108|accessdate=2008-11-13}} (unless otherwise cited)</ref>
| |
| ! style="background: #eff;" | <sup>‡</sup>{{dwarfplanet|Makemake}}<ref>(i){{cite web |author=[[Marc W. Buie]] |date=2008-04-05 |title=Orbit Fit and Astrometric record for 136472 |publisher=SwRI (Space Science Department) |url=http://www.boulder.swri.edu/~buie/kbo/astrom/136472.html |accessdate=2008-07-13}} <br> (ii){{cite web|title=NASA Small Bodies Database Browser: 136472 Makemake (2005 FY9)|url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=136472|publisher=NASA JPL|accessdate=2008-10-03}} (unless otherwise cited)</ref>
| |
| ! style="background: #eff;" | <sup>‡</sup>{{dwarfplanet|Eris}}<ref>{{cite web|title=NASA Small Body Database Browser: Eris|url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=Eris|publisher=NASA JPL|accessdate=2008-11-13}} (unless otherwise cited)</ref>
| |
| |-
| |
| | colspan="2" style="background: #fffdd0;" |
| |
| | style="background: #f0dc82;" | [[File:Ceres color.png|70px]]
| |
| | style="background: #eff;" | [[File:Pluto-map-hs-2010-06-d270.jpg|70px]]
| |
| | style="background: #eff;" | [[File:2003EL61art.jpg|70px]]
| |
| | style="background: #eff;" | [[File:2005FY9art.jpg|70px]]
| |
| | style="background: #eff;" | [[File:Eris and dysnomia2.jpg|70px]]
| |
| |-
| |
| | colspan="2" style="background: #fffdd0;" | [[Astronomical symbol|Astronomical symbol]]{{ref label|Q|q|none}}
| |
| | style="background: #f0dc82;" | [[File:Ceres symbol.svg|20px|Ceres]]
| |
| | style="background: #eff;" | [[File:Pluto symbol.svg|20px|Pluto]]
| |
| | style="background: #eff;" |
| |
| | style="background: #eff;" |
| |
| | style="background: #eff;" |
| |
| |-
| |
| | colspan="2" style="background: #fffdd0;" | [[Minor planet designation|Minor planet number]]
| |
| | style="background: #f0dc82;" | 1
| |
| | style="background: #eff;" | 134340
| |
| | style="background: #eff;" | 136108
| |
| | style="background: #eff;" | 136472
| |
| | style="background: #eff;" | 136199
| |
| |-
| |
| | style="background: #fffdd0;" | Mean distance <br> from [[Sun]]
| |
| | style="background: #fffdd0;" | km <br> [[Astronomical unit|AU]]
| |
| | style="background: #f0dc82;" | 413,700,000 <br> 2.766
| |
| | style="background: #eff;" | 5,906,380,000 <br> 39.482
| |
| | style="background: #eff;" | 6,484,000,000 <br> 43.335
| |
| | style="background: #eff;" | 6,850,000,000 <br> 45.792
| |
| | style="background: #eff;" | 10,210,000,000 <br> 67.668
| |
| |-
| |
| | style="background: #fffdd0;" | Mean [[radius]]
| |
| | style="background: #fffdd0;" | km <br> :E{{ref label|F|f|none}}
| |
| | style="background: #f0dc82;" | 471 <br> 0.0738
| |
| | style="background: #eff;" | 1,148.07 <br> 0.180
| |
| | style="background: #eff;" | 575 <br> 0.1537<ref name="Stansberry 2007">{{cite journal| author = J. Stansberry, W. Grundy, M. Brown, ''et al.''| title=Physical Properties of Kuiper Belt and Centaur Objects: Constraints from Spitzer Space Telescope|arxiv=astro-ph/0702538| journal = The Solar System beyond Neptune| publisher = University of Arizona Press | year=2007|bibcode = 2008ssbn.book..161S| last2 = Grundy| last3 = Brown| last4 = Cruikshank| last5 = Spencer| last6 = Trilling| last7 = Margot| pages = 161 }}</ref>
| |
| | style="background: #eff;" | 715±7 <br> 0.11<ref name="Brown2013Makemake">M.E. Brown, 2013, [http://arxiv.org/abs/1304.1041v1 "On the size, shape, and density of dwarf planet Makemake"]</ref>
| |
| | style="background: #eff;" | 1,200 <br> 0.19<ref name="Stansberry 2007"/>
| |
| |-
| |
| | style="background: #fffdd0;" | [[Volume]]
| |
| | style="background: #fffdd0;" | km<sup>3</sup> <br> :E{{ref label|F|f|none}}
| |
| | style="background: #f0dc82;" | 4.37{{e|8}} <br> 0.0005{{ref label|B|b|none}}
| |
| | style="background: #eff;" | 6.33{{e|9}} <br> 0.007
| |
| | style="background: #eff;" | 1.3–1.6{{e|9}} <br> 0.001{{ref_label|Y|y|none}}
| |
| | style="background: #eff;" | 1.5{{e|9}} <br> 0.001{{ref label|B|b|none}}
| |
| | style="background: #eff;" | 7.23{{e|9}} <br> 0.008{{ref label|B|b|none}}
| |
| |-
| |
| | style="background: #fffdd0;" | [[Surface area]]
| |
| | style="background: #fffdd0;" | km² <br> :E{{ref label|F|f|none}}
| |
| | style="background: #f0dc82;" | 2,800,000 <br> 0.0055{{ref label|A|a|none}}
| |
| | style="background: #eff;" | 17,000,000 <br> 0.0333
| |
| | style="background: #eff;" | 6,800,000 <br> 0.0133{{ref label|Z|z|none}}
| |
| | style="background: #eff;" | 6,400,000 <br> 0.013{{ref label|A|a|none}}
| |
| | style="background: #eff;" | 18,000,000 <br> 0.0353{{ref label|A|a|none}}
| |
| |-
| |
| | style="background: #fffdd0;" | [[Mass]]
| |
| | style="background: #fffdd0;" | [[Kilogram|kg]] <br> :E{{ref label|F|f|none}}
| |
| | style="background: #f0dc82;" | 9.5{{e|20}} <br> 0.00016
| |
| | style="background: #eff;" | 1.3{{e|22}} <br> 0.0022
| |
| | style="background: #eff;" | 4.01 ± 0.04{{e|21}} <br> 0.0007<ref>{{cite journal|author=M. E. Brown, A. H. Bouchez, D. L. Rabinowitz, R. Sari, C. A. Trujillo, M. A. van Dam, R. Campbell, J. Chin, S. Hartman, E. Johansson, R. Lafon, D. LeMignant, P. Stomski, D. Summers, P. L. Wizinowich |date=October 2005|title=Keck Observatory laser guide star adaptive optics discovery and characterization of a satellite to large Kuiper belt object 2003 EL61|journal=The Astrophysical Journal Letters|volume= 632|issue=L45| doi=10.1086/497641|pages=L45|bibcode=2005ApJ...632L..45B}}</ref>
| |
| | style="background: #eff;" | >2.1{{e|21}} <br> >0.0003{{ref label|AD|ad|none}}
| |
| | style="background: #eff;" | 1.7{{e|22}} <br> 0.0028<ref name="Brown Schaller 2007">{{cite doi | 10.1126/science.1139415 }}</ref>
| |
| |-
| |
| | style="background: #fffdd0;" | [[Density]]
| |
| | style="background: #fffdd0;" | [[Gram|g]]/cm<sup>3</sup>
| |
| | style="background: #f0dc82;" | 2.08
| |
| | style="background: #eff;" | 2.0
| |
| | style="background: #eff;" | 2.6–3.3<ref>{{cite journal|author=[[David L. Rabinowitz|D. L. Rabinowitz]], K. M. Barkume, [[Michael E. Brown|M. E. Brown]], H. G. Roe, M. Schwartz, S. W. Tourtellotte, [[Chadwick A. Trujillo|C. A. Trujillo]] |year=2006|title=Photometric Observations Constraining the Size, Shape, and Albedo of {{mp|2003 EL|61}}, a Rapidly Rotating, Pluto-Sized Object in the Kuiper Belt|journal=The Astrophysical Journal|volume=639|issue=2|pages=1238–1251|doi=10.1086/499575|bibcode=2006ApJ...639.1238R|arxiv = astro-ph/0509401 }}</ref>
| |
| | style="background: #eff;" | >1.4<ref name="Brown2013Makemake"/>
| |
| | style="background: #eff;" | 2.25{{ref label|C|c|none}}
| |
| |-
| |
| | style="background: #fffdd0;" | [[Equator]]ial [[gravity]]
| |
| | style="background: #fffdd0;" | [[Acceleration|m/s<sup>2</sup>]]
| |
| | style="background: #f0dc82;" | 0.27{{ref label|D|d|none}}
| |
| | style="background: #eff;" | 0.60
| |
| | style="background: #eff;" | 0.44{{ref label|D|d|none}}
| |
| | style="background: #eff;" | >0.28{{ref label|D|d|none}}
| |
| | style="background: #eff;" | ~0.8{{ref label|D|d|none}}
| |
| |-
| |
| | style="background: #fffdd0;" | [[Escape velocity]]
| |
| | style="background: #fffdd0;" | [[Speed|km/s]]{{ref label|E|e|none}}
| |
| | style="background: #f0dc82;" | 0.51
| |
| | style="background: #eff;" | 1.23
| |
| | style="background: #eff;" | 0.84
| |
| | style="background: #eff;" | >0.6
| |
| | style="background: #eff;" | 1.37
| |
| |-
| |
| | style="background: #fffdd0;" | Rotation period{{ref label|G|g|none}}
| |
| | style="background: #fffdd0;" | days
| |
| | style="background: #f0dc82;" | 0.3781
| |
| | style="background: #eff;" | −6.38718{{ref label|H|h|none}}
| |
| | style="background: #eff;" | 0.167
| |
| | style="background: #eff;" | ?
| |
| | style="background: #eff;" | ?
| |
| |-
| |
| | style="background: #fffdd0;" | Orbital period{{ref label|G|g|none}}
| |
| | style="background: #fffdd0;" | [[Julian year (astronomy)|years]]
| |
| | style="background: #f0dc82;" | 4.599
| |
| | style="background: #eff;" | 247.92065
| |
| | style="background: #eff;" | 285.4
| |
| | style="background: #eff;" | 309.9
| |
| | style="background: #eff;" | 557
| |
| |-
| |
| | style="background: #fffdd0;" | Mean orbital speed
| |
| | style="background: #fffdd0;" | [[Speed|km/s]]
| |
| | style="background: #f0dc82;" | 17.882
| |
| | style="background: #eff;" | 4.7490
| |
| | style="background: #eff;" | 4.484{{ref label|O|o|none}}
| |
| | style="background: #eff;" | 4.4{{ref label|O|o|none}}
| |
| | style="background: #eff;" | 3.436{{ref label|N|n|none}}
| |
| |-
| |
| | colspan="2" style="background: #fffdd0;" | [[Eccentricity (orbit)|Eccentricity]]
| |
| | style="background: #f0dc82;" | 0.080
| |
| | style="background: #eff;" | 0.24880766
| |
| | style="background: #eff;" | 0.18874
| |
| | style="background: #eff;" | 0.159
| |
| | style="background: #eff;" | 0.44177
| |
| |-
| |
| | style="background: #fffdd0;" | [[Inclination]]{{ref label|F|f|none}}
| |
| | style="background: #fffdd0;" | [[Degree (angle)|deg.]]
| |
| | style="background: #f0dc82;" | 10.587
| |
| | style="background: #eff;" | 17.14175
| |
| | style="background: #eff;" | 28.19
| |
| | style="background: #eff;" | 28.96
| |
| | style="background: #eff;" | 44.187
| |
| |-
| |
| | style="background: #fffdd0;" | [[Axial tilt]]{{ref label|I|i|none}}
| |
| | style="background: #fffdd0;" | [[Degree (angle)|deg.]]
| |
| | style="background: #f0dc82;" | 4
| |
| | style="background: #eff;" | 119.61
| |
| | style="background: #eff;" | ?
| |
| | style="background: #eff;" | ?
| |
| | style="background: #eff;" | ?
| |
| |-
| |
| | style="background: #fffdd0;" | Mean surface [[temperature]]{{ref label|W|w|none}}
| |
| | style="background: #fffdd0;" | [[Kelvin|K]]
| |
| | style="background: #f0dc82;" | 167<ref>{{cite journal
| |
| |author= O. Saint-Pé
| |
| |coauthors=N. Combes, F. Rigaut
| |
| |title=Ceres surface properties by high-resolution imaging from Earth
| |
| |year=1993|volume=105
| |
| |issue= 2|pages=271–281|
| |
| journal=Icarus
| |
| |doi=10.1006/icar.1993.1125
| |
| |bibcode=1993Icar..105..271S }}</ref>
| |
| | style="background: #eff;" | 40<ref>{{cite news
| |
| | url = http://www.cnn.com/2006/TECH/space/01/03/pluto.temp/index.html
| |
| | title = Astronomers: Pluto colder than expected
| |
| | author = T. Ker
| |
| | publisher = Space.com (via CNN.com)
| |
| | year = 2006
| |
| }} Retrieved on 2006-03-05.</ref>
| |
| | style="background: #eff;" | <50<ref>{{cite journal|author=Chadwick A. Trujillo, Michael E. Brown, Kristina Barkume, Emily Shaller, David L. Rabinowitz|date=February 2007|title=The Surface of 2003 EL61 in the Near Infrared|journal=The Astrophysical Journal|volume=655|issue=2|pages=1172–1178|doi=10.1086/509861|bibcode=2007ApJ...655.1172T|arxiv = astro-ph/0601618 }}</ref>
| |
| | style="background: #eff;" | 30
| |
| | style="background: #eff;" | 30
| |
| |-
| |
| | colspan="2" style="background: #fffdd0;" | [[Atmosphere|Atmospheric]] composition
| |
| | style="background: #f0dc82;" | [[Water|H<sub>2</sub>O]], [[Oxygen|O<sub>2</sub>]]
| |
| | style="background: #eff;" | [[Nitrogen|N<sub>2</sub>]], [[Methane|CH<sub>4</sub>]]
| |
| | style="background: #eff;" |
| |
| | style="background: #eff;" | N<sub>2</sub>, CH<sub>4</sub>.<ref name=brown>{{cite journal|title=Methane and Ethane on the Bright Kuiper Belt Object 2005 FY<sub>9</sub>|author=Mike Brown, K. M. Barksume, G. L. Blake, E. L. Schaller, D. L. Rabinowitz, H. G. Roe and C. A. Trujillo |journal= The Astronomical Journal |year=2007|volume=133|issue=1|pages= 284–289| doi= 10.1086/509734|bibcode=2007AJ....133..284B}}</ref>
| |
| | style="background: #eff;" | N<sub>2</sub>, CH<sub>4</sub><ref>
| |
| {{cite journal
| |
| | title = Visible spectroscopy of {{mp|2003 UB|313}}: evidence for N<sub>2</sub> ice on the surface of the largest TNO
| |
| | author = J. Licandro, W. M. Grundy, N. Pinilla-Alonso, P. Leisy
| |
| | journal = Astronomy and Astrophysics
| |
| | year = 2006
| |
| | volume =458
| |
| | issue = 1
| |
| | pages = L5–L8
| |
| | doi = 10.1051/0004-6361:20066028
| |
| | format=PDF
| |
| | url =http://www.aanda.org/index.php?option=article&access=standard&Itemid=129&url=/articles/aa/pdf/2006/40/aa6028-06.pdf
| |
| | bibcode=2006A&A...458L...5L
| |
| |arxiv = astro-ph/0608044 }}</ref>
| |
| |-
| |
| | colspan="2" style="background: #fffdd0;" | Number of known [[Natural satellite|moons]]{{ref label|V|v|none}}
| |
| | style="background: #f0dc82;" | 0
| |
| | style="background: #eff;" | [[Pluto's natural satellites|5]]
| |
| | style="background: #eff;" | [[Haumea's natural satellites|2]]<ref>
| |
| {{cite web
| |
| |author=D. Ragozzine, M. E. Brown, C. A. Trujillo, E. L. Schaller
| |
| |title=Orbits and Masses of the 2003 EL61 Satellite System
| |
| |url=http://www.abstractsonline.com/viewer/viewAbstract.asp?CKey={421E1C09-F75A-4ED0-916C-8C0DDB81754D}&MKey={35A8F7D5-A145-4C52-8514-0B0340308E94}&AKey={AAF9AABA-B0FF-4235-8AEC-74F22FC76386}&SKey={545CAD5F-068B-4FFC-A6E2-1F2A0C6ED978}
| |
| |work=AAS DPS conference 2008
| |
| |accessdate=2008-10-17}}
| |
| </ref>
| |
| | style="background: #eff;" | 0<ref>{{cite doi | 10.1086/501524 }}</ref>
| |
| | style="background: #eff;" | [[Dysnomia (moon)|1]]<ref>
| |
| {{cite journal
| |
| | title = Satellites of the largest Kuiper belt objects
| |
| | author = [[Michael E. Brown|M. E. Brown]], M. A. van Dam, A. H. Bouchez, D. LeMignant, [[Chadwick A. Trujillo|C. A. Trujillo]], R. Campbell, J. Chin, Conrad A., S. Hartman, E. Johansson, R. Lafon, [[David L. Rabinowitz|D. L. Rabinowitz]], P. Stomski, D. Summers, P. L. Wizinowich
| |
| | journal = The Astrophysical Journal
| |
| | year = 2006
| |
| | volume =639
| |
| | issue = 1
| |
| | pages = L43–L46
| |
| | doi = 10.1086/501524
| |
| | arxiv =astro-ph/0510029
| |
| | bibcode=2006ApJ...639L..43B
| |
| }}</ref>
| |
| |-
| |
| | colspan="2" style="background: #fffdd0;" | [[Clearing the neighbourhood|Planetary discriminant]]{{ref label|L|l|none}}{{ref label|O|o|none}}
| |
| | style="background: #f0dc82;" | 0.33
| |
| | style="background: #eff;" | 0.077
| |
| | style="background: #eff;" | 0.023
| |
| | style="background: #eff;" | 0.02
| |
| | style="background: #eff;" | 0.10
| |
| |}
| |
|
| |
|
| == Satellites ==
| | Som journaliststuderende jeg drømte om at rejse rundt i verden og fortælle historier om mennesker og steder (mere Martha Gellhorn end Georgie Anne Geyer). Grunden artikler arbejde så godt for "voksende" links indebærer talrige måder, hvorpå artikler bliver distribueret online, som hver især kan skabe dusinvis, hundredvis, ja tusindvis af forskellige links tilbage til dit websted ved at udgive en enkelt artikel ... <br><br>Være beskyttet mod at høre voksne argumenter og tvister. Siddende i oplandet af Kinta Valley er Ipoh By omgivet 400 millioner mange år alderen kalkstensbakke varierer eksklusionen sider. Lav en sætning, der siger klik her for mere information om "Plænetraktorer." Klikbare del af linket skal være dine søgeord og ikke klik her!.. <br><br>Jeg ser masser af emner, der er lukket uden input fra Google personale, så er de emner, lukkede automatisk over tid eller af personale? Hvis af personale så jeg tror, det er lidt af en pik flytte til at lukke et emne, men ikke svare på emnet.. Loftstykkelse 120 mm, Mål: uden dia. <br><br>Med den jublende sektion, er det på høje finans og dit erotiske liv i fokus. Denne våde damp, når inhaleret giver samme tilfredsstillelse som hvilke af at ryge en [http://www.trykpaatoej.dk/content/frame.asp?rayban=18 Ray Ban Solbriller Til Mænd] ægte cigaret, og det er faktisk den funktion, som har gjort det muligt kunder til at undertrykke deres cigaretrygning vane. <br><br>Alle de sædvanlige faciliteter, du ville forvente af et firestjernet webstedet er til rådighed, herunder elektriske [http://www.hotel-nygaard.dk/log/Gallery/crypt.asp?d=111-Air-Jordan-3 Air Jordan 3] tilslutninger til touring enheder, en moderne, wellequipped toilet blok med gratis varmt brusebad, og en onsite shop, som vil levere dit daglige behov sammen med flaskegas, camping gaz og en række nyttige camping reservedele. <br><br>At overleve en Tsunami, og sidst men ikke mindst, at overleve en Tsunami Ligesom Petra Nemcova. [http://www.asherregaard.dk/delikatesser/umenu/client.asp?h=15 Michael Kors Tasker Forhandler Danmark] Købt papirudgave og så kan [http://www.jyskgenbrug.dk/images/file.asp?d=30-Buy-New-Balance-Online-Us Buy New Balance Online Us] jeg bruge min 20 dollar kredit på enten en anden Wii U spil eller måske den nye Tomb Raider ... Trailrunner7 skriver "The Microsoft Digital Crimes Unit har spydspids botnet takedowns og andre anticybercrime operationer i mange år, og det har haft bemærkelsesværdig succes. <br><br>De fleste virksomheder er ikke på resultaterne, men de har kun vage løfter. Southern skuespillere som Mohanlal delte én procent stemmer hver, og resten af skuespillerne fik mindre end en procent af stemmerne ... Jack fik sine autografer gemt væk sikkert, en enkelt rest af liv fortiden. <br><br>Så uanset om det er dag eller nat, når der er sne, kan du ende på pisterne ... Eventuelle forenklingsforanstaltninger, som kan være effektive, er langt opvejes af andre, der vil tilføre yderligere kompleksitet.. Longboarding er alt hvad vi gør, og vi fastholder det største udvalg af longboard dæk, Longboard færdig, longboard hjul, longboard trucks, longboard lejer, sikkerhed gear og mere året rundt ...<ul> |
| <div style="float: right; margin: 0.5px;">
| | |
| {| class="wikitable" border="1"
| | <li>[http://www.shanghai30p.com/news/html/?98063.html http://www.shanghai30p.com/news/html/?98063.html]</li> |
| |-
| | |
| ! style="background: #eaeaea" colspan=6|Key | | <li>[http://ilivewebsolutions.com/awus/DEV/index.php/forum/2-introductions/152169-nike-lobesko-til-born-og-derefter-forberedt-nojagtigt-som-graeskar-hjem#152169 http://ilivewebsolutions.com/awus/DEV/index.php/forum/2-introductions/152169-nike-lobesko-til-born-og-derefter-forberedt-nojagtigt-som-graeskar-hjem#152169]</li> |
| |-
| | |
| | bgcolor="#B0E0E6" width=50 style="text-align: center" |<sup>€</sup> <br /> [[moon|Satellite of Earth]]
| | <li>[http://www.christophegreffet.fr/blog/index.php?2013/04/17/87-ma-reunion-a-bercy/ http://www.christophegreffet.fr/blog/index.php?2013/04/17/87-ma-reunion-a-bercy/]</li> |
| | bgcolor="#FFA6C9" width=50 style="text-align: center" |<sup>₤</sup> <br /> [[Moons of Jupiter|Satellite of Jupiter]]
| | |
| | bgcolor="#FBEC5D" width=50 style="text-align: center" |<sup>$</sup> <br /> [[Moons of Saturn|Satellite of Saturn]]
| | <li>[http://tvman.comze.com/forum.php?mod=viewthread&tid=1058841 http://tvman.comze.com/forum.php?mod=viewthread&tid=1058841]</li> |
| | bgcolor="#7FFFD4" width=50 style="text-align: center" |<sup>₩</sup> <br /> [[Moons of Uranus|Satellite of Uranus]]
| | |
| | bgcolor="#F0FFFF" width=50 style="text-align: center" |<sup>₦</sup> <br /> [[Moons of Neptune|Satellite of Neptune]]
| | <li>[http://www.ovnprod.com/spip.php?article24/ http://www.ovnprod.com/spip.php?article24/]</li> |
| | bgcolor="#CCCCFF" width=50 style="text-align: center" |<sup>¶</sup> <br /> [[Moons of Pluto|Satellite of Pluto]]
| | |
| |}</div>
| | </ul> |
| {{see also|List of moons}}
| |
| There are 19 [[natural satellites]] in the Solar System that are known to be massive enough to be close to hydrostatic equilibrium, which Alan Stern calls ''satellite planets''. However, several of these were once in equilibrium but are no longer: these include all of the moons listed for Saturn apart from Titan and Rhea. Other moons that were once in equilibrium but are no longer very round, such as Saturn's Phoebe, are not included. Satellites are listed first in order from the Sun, and second in order from their parent body.
| |
|
| |
|
| {| class="wikitable" border="1" style="text-align: center;"
| | == Michael Kors Ipad ikke tager mig væk fra hjemmesiden == |
| |-
| |
| ! colspan="2" style="background: #fffdd0;" |
| |
| ! style="background: #b0e0e6;" | <sup>€</sup>[[Moon]]<ref>[http://nssdc.gsfc.nasa.gov/planetary/factsheet/moonfact.html NASA Moon factsheet] and [http://solarsystem.nasa.gov/planets/profile.cfm?Object=Moon&Display=Facts NASA Solar System Exploration Moon Factsheet] ''NASA'' Retrieved on 2008-11-17 (unless otherwise cited)</ref>
| |
|
| |
|
| ! style="background: #ffa6c9;" | <sup>₤</sup>[[Io (moon)|Io]]<ref>{{cite web|title=NASA Io Factsheet|url=http://www2.jpl.nasa.gov/galileo/io/fact.html#stats|publisher=NASA|accessdate=2008-11-16}} (unless otherwise cited)</ref>
| | Der vælger du? Naruto, fordi han er [http://www.asherregaard.dk/delikatesser/umenu/client.asp?h=30 Michael Kors Ipad] meget sjovt og jeg elsker [http://www.jyskgenbrug.dk/images/file.asp?d=30-Buy-New-Balance-Online-Us Buy New Balance Online Us] hans strittende blond hår.. Så længe annoncen ikke var utiltalende (let lukket, ikke tager mig væk fra hjemmesiden, etc.) Det sidste punkt synes at være de mest relevante i denne sag, men denne synes moden til klik svig.. <br><br>Det blev forkastet, men i 1909 det blev fejret i 46 stater. Der er almindelig gamle trætte og så er der god træt. I samme periode i 2012, det største år i dollar siden finanskrisen 73 selskaber rejst i alt 13,1 mia $ ... Den e-mail invitation udtalte: Vil du gerne komme til et møde og hilse i New York for Susan? Uden tøven, ingen stillede spørgsmål, svarede jeg ja ... <br><br>Alt hvad der er nødvendigt, er at have alle dine oplysninger handy og så bare følge instruktionerne i teksten og følg links som hensigtsmæssigt. Heller burde vi til at tænke, at denne sidstnævnte forbedring i videnskaben om mennesket vil gøre mindre ære til vores fædreland end førstnævnte i naturfilosofi, men burde snarere agtelse det en større herlighed, efter betragtning af den større betydning, at videnskab, samt nødvendigheden det lå under en sådan reformation. <br><br>Så temmelig meget du kan lide mennesker. Og over tid, vil det have den bedste, langsigtede indvirkning på organiske ranking resultater.. Husk bag hver person deres er en smertende hjerte. Efter betler, er den næste kendte overdragelse af titlen, når Guilty Spark rettet sergent Marvin Mobuto i Halo: The Flood. <br><br>Andre emner som kuglepenne, køleskabsmagneter, væg kalendere og lomme kalendere med din virksomheds navn på dem er også værdsat i slutningen af året.. Alene overvældende kompleksitet aminosyre / neurotransmitter aktivitet i den menneskelige krop / brainand den opdelte karakter af biokemien hver forekommer bedst egner sig til en mere funktionel og symptomrelated evaluering.. <br><br>På hurtigste kugle selv og læge maske. Monk, der leverer maskiner til HEB Byggestyrelsens byggepladser, sagde hr. Faktisk har denne retsforfølgning [http://www.trykpaatoej.dk/content/frame.asp?rayban=48 Ray Ban Brillestel] er så absolut korrupt, at det har endda bevidst overtrådt loven i Californien om aflytninger, og det er ikke fordi Geragos siger det. <br><br>Prøv Buzz Buzz, han er en virkelig cool humlebi!. Forvent studerende til at tage tests, varierer indholdet, asesment metode og tid. Håndværk og REAL arbejde fra hjemmet job. Faktisk, at NY Times artikel er knyttet til [http://www.jyskgenbrug.dk/images/file.asp?d=5-New-Balance-1500-Dk New Balance 1500 Dk] som "af en ITU apologet", er næppe, hvad jeg ville beskrive som en forsvarstale. <br><br>Disse samtaler kan fortsætte gennem kommentarer eller e-mail. En dag, kan du se dit barns godtgørelse som en direkte debitering fra din konto.. Af de to pressekonferencer blev telecast leve uden at gøre noget forsøg på at kontrollere sandheden eller rigtigheden af de erklæringer og påstande, der gøres under pressekonferencen..<ul> |
| ! style="background: #ffa6c9;" | <sup>₤</sup>[[Europa (moon)|Europa]]<ref>{{cite web|title=NASA Europa Factsheet|url=http://www2.jpl.nasa.gov/galileo/europa/|publisher=NASA|accessdate=2008-11-16}} (unless otherwise cited)</ref>
| | |
| ! style="background: #ffa6c9;" | <sup>₤</sup>[[Ganymede (moon)|Ganymede]]<ref>{{cite web|title=NASA Ganymede Factsheet|url=http://www2.jpl.nasa.gov/galileo/ganymede/fact.html|publisher=NASA|accessdate=2008-11-16}} (unless otherwise cited)</ref>
| | <li>[http://verdamilio.net/tonio/spip.php?article1/ http://verdamilio.net/tonio/spip.php?article1/]</li> |
| ! style="background: #ffa6c9;" | <sup>₤</sup>[[Callisto (moon)|Callisto]]<ref>{{cite web|title=NASA Callisto Factsheet|publisher=NASA|url=http://www2.jpl.nasa.gov/galileo/callisto/|accessdate=2008-11-16}}</ref>
| | |
| ! style="background: #fbec5d;" | <sup>$</sup>[[Mimas (moon)|Mimas]]{{ref label|P|p|none}}
| | <li>[http://39451.vhost13.cloudvhost.net/upload/forum.php?mod=viewthread&tid=45438&fromuid=17466 http://39451.vhost13.cloudvhost.net/upload/forum.php?mod=viewthread&tid=45438&fromuid=17466]</li> |
| ! style="background: #fbec5d;" | <sup>$</sup>[[Enceladus (moon)|Enceladus]]{{ref label|P|p|none}}
| | |
| ! style="background: #fbec5d;" | <sup>$</sup>[[Tethys (moon)|Tethys]]{{ref label|P|p|none}}
| | <li>[http://box-man.co.uk/ http://box-man.co.uk/]</li> |
| ! style="background: #fbec5d;" | <sup>$</sup>[[Dione (moon)|Dione]]{{ref label|P|p|none}}
| | |
| ! style="background: #fbec5d;" | <sup>$</sup>[[Rhea (moon)|Rhea]]{{ref label|P|p|none}}
| | <li>[http://www.jamiatou.com/spip.php?article21 http://www.jamiatou.com/spip.php?article21]</li> |
| |-
| | |
| | colspan="2" style="background: #fffdd0;" |
| | <li>[http://pw.stxia.com/news/html/?112241.html http://pw.stxia.com/news/html/?112241.html]</li> |
| | style="background: #b0e0e6;" | [[File:Full moon.jpeg|70px]]
| | |
| | style="background: #ffa6c9;" | [[File:Io highest resolution true color.jpg|70px]]
| | </ul> |
| | style="background: #ffa6c9;" | [[File:Europa-moon.jpg|70px]]
| |
| | style="background: #ffa6c9;" | [[File:Ganymede g1 true 2.jpg|70px]]
| |
| | style="background: #ffa6c9;" | [[File:Callisto.jpg|70px]]
| |
| | style="background: #fbec5d;" | [[File:Mimas moon.jpg|70px]]
| |
| | style="background: #fbec5d;" | [[File:Enceladus north.jpg|70 px]]
| |
| | style="background: #fbec5d;" | [[File:Inset-sat tethys-large.jpg|70 px]]
| |
| | style="background: #fbec5d;" | [[File:Dione.jpg|70 px]]
| |
| | style="background: #fbec5d;" | [[File:Rhea (moon) thumb.jpg|70 px]]
| |
| |-
| |
| | colspan="2" style="background: #fffdd0;" | [[Astronomical symbol|Astronomical symbol]]{{ref label|Q|q|none}}
| |
| | style="background: #b0e0e6;" | [[File:Moon symbol decrescent.svg|20px|Moon]]
| |
| | style="background: #ffa6c9;" |
| |
| | style="background: #ffa6c9;" |
| |
| | style="background: #ffa6c9;" |
| |
| | style="background: #ffa6c9;" |
| |
| | style="background: #fbec5d;" |
| |
| | style="background: #fbec5d;" |
| |
| | style="background: #fbec5d;" |
| |
| | style="background: #fbec5d;" |
| |
| | style="background: #fbec5d;" |
| |
| |-
| |
| | style="background: #fffdd0;" | Mean distance <br /> from primary:
| |
| | style="background: #fffdd0;" | km
| |
| | style="background: #b0e0e6;" | 384,399
| |
| | style="background: #ffa6c9;" | 421,600
| |
| | style="background: #ffa6c9;" | 670,900
| |
| | style="background: #ffa6c9;" | 1,070,400
| |
| | style="background: #ffa6c9;" | 1,882,700
| |
| | style="background: #fbec5d;" | 185,520
| |
| | style="background: #fbec5d;" | 237,948
| |
| | style="background: #fbec5d;" | 294,619
| |
| | style="background: #fbec5d;" | 377,396
| |
| | style="background: #fbec5d;" | 527,108
| |
| |-
| |
| | style="background: #fffdd0;" | Mean [[radius]]
| |
| | style="background: #fffdd0;" | km <br /> :E{{ref label|F|f|none}}
| |
| | style="background: #b0e0e6;" | 1,737.1 <br /> 0.273
| |
| | style="background: #ffa6c9;" | 1,815 <br /> 0.286
| |
| | style="background: #ffa6c9;" | 1,569 <br /> 0.245
| |
| | style="background: #ffa6c9;" | 2,634.1 <br /> 0.413
| |
| | style="background: #ffa6c9;" | 2,410.3 <br /> 0.378
| |
| | style="background: #fbec5d;" | 198.30 <br /> 0.031
| |
| | style="background: #fbec5d;" | 252.1 <br /> 0.04
| |
| | style="background: #fbec5d;" | 533 <br /> 0.083
| |
| | style="background: #fbec5d;" | 561.7 <br /> 0.088
| |
| | style="background: #fbec5d;" | 764.3 <br /> 0.12
| |
| |-
| |
| | style="background: #fffdd0;" | [[Surface area]]{{ref label|A|a|none}}
| |
| | style="background: #fffdd0;" | km² <br /> :E{{ref label|F|f|none}}
| |
| | style="background: #b0e0e6;" | 37,930,000 <br /> 0.074
| |
| | style="background: #ffa6c9;" | 41,910,000 <br /> 0.082
| |
| | style="background: #ffa6c9;" | 30,900,000 <br /> 0.061
| |
| | style="background: #ffa6c9;" | 87,000,000 <br /> 0.143
| |
| | style="background: #ffa6c9;" | 73,000,000 <br /> 0.143
| |
| | style="background: #fbec5d;" | 490,000 <br /> 0.001
| |
| | style="background: #fbec5d;" | 799,000 <br /> 0.0016
| |
| | style="background: #fbec5d;" | 4,940,000 <br /> 0.01
| |
| | style="background: #fbec5d;" | 3,965,000 <br /> 0.0078
| |
| | style="background: #fbec5d;" | 7,337,000 <br /> 0.0144
| |
| |-
| |
| | style="background: #fffdd0;" | [[Volume]]{{ref label|B|b|none}}
| |
| | style="background: #fffdd0;" | km<sup>3</sup> <br /> :E{{ref label|F|f|none}}
| |
| | style="background: #b0e0e6;" | 2.2{{e|10}} <br /> 0.02
| |
| | style="background: #ffa6c9;" | 2.53{{e|10}} <br /> 0.02
| |
| | style="background: #ffa6c9;" | 1.59{{e|10}} <br /> 0.07
| |
| | style="background: #ffa6c9;" | 7.6{{e|10}} <br /> 0.15
| |
| | style="background: #ffa6c9;" | 5.9{{e|10}} <br /> 0.05
| |
| | style="background: #fbec5d;" | 3.3{{e|7}} <br /> 0.00003
| |
| | style="background: #fbec5d;" | 6.7{{e|7}} <br /> 0.00006
| |
| | style="background: #fbec5d;" | 6.3{{e|8}} <br /> 0.0006
| |
| | style="background: #fbec5d;" | 7.4{{e|8}} <br /> 0.0007
| |
| | style="background: #fbec5d;" | 1.9 {{e|9}} <br /> 0.0017
| |
| |-
| |
| | style="background: #fffdd0;" | [[Mass]]
| |
| | style="background: #fffdd0;" | [[Kilogram|kg]] <br /> :E{{ref label|F|f|none}}
| |
| | style="background: #b0e0e6;" | 7.3477{{e|22}} <br /> 0.0123
| |
| | style="background: #ffa6c9;" | 8.94{{e|22}} <br /> 0.015
| |
| | style="background: #ffa6c9;" | 4.80{{e|22}} <br /> 0.008
| |
| | style="background: #ffa6c9;" | 1.4819{{e|23}} <br /> 0.025
| |
| | style="background: #ffa6c9;" | 1.0758{{e|23}} <br /> 0.018
| |
| | style="background: #fbec5d;" | 3.75{{e|19}} <br /> 0.000006
| |
| | style="background: #fbec5d;" | 1.08{{e|20}} <br /> 0.000018
| |
| | style="background: #fbec5d;" | 6.174{{e|20}} <br /> 0.00132
| |
| | style="background: #fbec5d;" | 1.095{{e|21}} <br /> 0.0003
| |
| | style="background: #fbec5d;" | 2.306{{e|21}} <br /> 0.0004
| |
| |-
| |
| | style="background: #fffdd0;" | [[Density]]{{ref label|C|c|none}}
| |
| | style="background: #fffdd0;" | [[Gram|g]]/cm<sup>3</sup>
| |
| | style="background: #b0e0e6;" | 3.3464
| |
| | style="background: #ffa6c9;" | 3.528
| |
| | style="background: #ffa6c9;" | 3.01
| |
| | style="background: #ffa6c9;" | 1.936
| |
| | style="background: #ffa6c9;" | 1.83
| |
| | style="background: #fbec5d;" | 1.15
| |
| | style="background: #fbec5d;" | 1.61
| |
| | style="background: #fbec5d;" | 0.98
| |
| | style="background: #fbec5d;" | 1.48
| |
| | style="background: #fbec5d;" | 1.23
| |
| |-
| |
| | style="background: #fffdd0;" | [[Equator]]ial [[gravity]]{{ref label|D|d|none}}
| |
| | style="background: #fffdd0;" | [[Acceleration|m/s<sup>2</sup>]]
| |
| | style="background: #b0e0e6;" | 1.622
| |
| | style="background: #ffa6c9;" | 1.796
| |
| | style="background: #ffa6c9;" | 1.314
| |
| | style="background: #ffa6c9;" | 1.428
| |
| | style="background: #ffa6c9;" | 1.235
| |
| | style="background: #fbec5d;" | 0.0636
| |
| | style="background: #fbec5d;" | 0.111
| |
| | style="background: #fbec5d;" | 0.145
| |
| | style="background: #fbec5d;" | 0.231
| |
| | style="background: #fbec5d;" | 0.264
| |
| |-
| |
| | style="background: #fffdd0;" | [[Escape velocity]]{{ref label|E|e|none}}
| |
| | style="background: #fffdd0;" | [[Speed|km/s]]
| |
| | style="background: #b0e0e6;" | 2.38
| |
| | style="background: #ffa6c9;" | 2.56
| |
| | style="background: #ffa6c9;" | 2.025
| |
| | style="background: #ffa6c9;" | 2.741
| |
| | style="background: #ffa6c9;" | 2.440
| |
| | style="background: #fbec5d;" | 0.159
| |
| | style="background: #fbec5d;" | 0.239
| |
| | style="background: #fbec5d;" | 0.393
| |
| | style="background: #fbec5d;" | 0.510
| |
| | style="background: #fbec5d;" | 0.635
| |
| |-
| |
| | style="background: #fffdd0;" | Rotation period
| |
| | style="background: #fffdd0;" | days{{ref label|G|g|none}}
| |
| | style="background: #b0e0e6;" | 27.321582 <br /> (sync){{ref label|M|m|none}}
| |
| | style="background: #ffa6c9;" | 1.7691378 <br /> (sync)
| |
| | style="background: #ffa6c9;" | 3.551181 <br /> (sync)
| |
| | style="background: #ffa6c9;" | 7.154553 <br /> (sync)
| |
| | style="background: #ffa6c9;" | 16.68902 <br /> (sync)
| |
| | style="background: #fbec5d;" | 0.942422 <br /> (sync)
| |
| | style="background: #fbec5d;" | 1.370218 <br /> (sync)
| |
| | style="background: #fbec5d;" | 1.887802 <br /> (sync)
| |
| | style="background: #fbec5d;" | 2.736915 <br /> (sync)
| |
| | style="background: #fbec5d;" | 4.518212 <br /> (sync)
| |
| |-
| |
| | style="background: #fffdd0;" | Orbital period about primary
| |
| | style="background: #fffdd0;" | days{{ref label|G|g|none}}
| |
| | style="background: #b0e0e6;" | 27.32158
| |
| | style="background: #ffa6c9;" | 1.769138
| |
| | style="background: #ffa6c9;" | 3.551181
| |
| | style="background: #ffa6c9;" | 7.154553
| |
| | style="background: #ffa6c9;" | 16.68902
| |
| | style="background: #fbec5d;" | 0.942422
| |
| | style="background: #fbec5d;" | 1.370218
| |
| | style="background: #fbec5d;" | 1.887802
| |
| | style="background: #fbec5d;" | 2.736915
| |
| | style="background: #fbec5d;" | 4.518212
| |
| |-
| |
| | style="background: #fffdd0;" | Mean orbital speed{{ref label|O|o|none}}
| |
| | style="background: #fffdd0;" | [[Speed|km/s]]
| |
| | style="background: #b0e0e6;" | 1.022
| |
| | style="background: #ffa6c9;" | 17.34
| |
| | style="background: #ffa6c9;" | 13.740
| |
| | style="background: #ffa6c9;" | 10.880
| |
| | style="background: #ffa6c9;" | 8.204
| |
| | style="background: #fbec5d;" | 14.32
| |
| | style="background: #fbec5d;" | 12.63
| |
| | style="background: #fbec5d;" | 11.35
| |
| | style="background: #fbec5d;" | 10.03
| |
| | style="background: #fbec5d;" | 8.48
| |
| |-
| |
| | colspan="2" style="background: #fffdd0;" | [[Eccentricity (orbit)|Eccentricity]]
| |
| | style="background: #b0e0e6;" | 0.0549
| |
| | style="background: #ffa6c9;" | 0.0041
| |
| | style="background: #ffa6c9;" | 0.009
| |
| | style="background: #ffa6c9;" | 0.0013
| |
| | style="background: #ffa6c9;" | 0.0074
| |
| | style="background: #fbec5d;" | 0.0202
| |
| | style="background: #fbec5d;" | 0.0047
| |
| | style="background: #fbec5d;" | 0.02
| |
| | style="background: #fbec5d;" | 0.002
| |
| | style="background: #fbec5d;" | 0.001
| |
| |-
| |
| | style="background: #fffdd0;" | [[Inclination]] to primary's equator
| |
| | style="background: #fffdd0;" | [[Degree (angle)|deg.]]
| |
| | style="background: #b0e0e6;" | 18.29–28.58
| |
| | style="background: #ffa6c9;" | 0.04
| |
| | style="background: #ffa6c9;" | 0.47
| |
| | style="background: #ffa6c9;" | 1.85
| |
| | style="background: #ffa6c9;" | 0.2
| |
| | style="background: #fbec5d;" | 1.51
| |
| | style="background: #fbec5d;" | 0.02
| |
| | style="background: #fbec5d;" | 1.51
| |
| | style="background: #fbec5d;" | 0.019
| |
| | style="background: #fbec5d;" | 0.345
| |
| |-
| |
| | style="background: #fffdd0;" | [[Axial tilt]]{{ref label|I|i|none}}{{ref label|U|u|none}}
| |
| | style="background: #fffdd0;" | [[Degree (angle)|deg.]]
| |
| | style="background: #b0e0e6;" | 6.68
| |
| | style="background: #ffa6c9;" | 0
| |
| | style="background: #ffa6c9;" | 0
| |
| | style="background: #ffa6c9;" | 0–0.33<ref>{{cite journal|author=Bruce G. Bills|title=Free and forced obliquities of the Galilean satellites of Jupiter|year=2005|volume=175|issue=1|pages=233–247| doi=10.1016/j.icarus.2004.10.028|bibcode=2005Icar..175..233B | journal = Icarus}}</ref>
| |
| | style="background: #ffa6c9;" | 0
| |
| | style="background: #fbec5d;" | 0
| |
| | style="background: #fbec5d;" | 0
| |
| | style="background: #fbec5d;" | 0
| |
| | style="background: #fbec5d;" | 0
| |
| | style="background: #fbec5d;" | 0
| |
| |-
| |
| | style="background: #fffdd0;" | Mean surface [[temperature]]{{ref label|W|w|none}}
| |
| | style="background: #fffdd0;" | [[Kelvin|K]]
| |
| | style="background: #b0e0e6;" | 220
| |
| | style="background: #ffa6c9;" | 130
| |
| | style="background: #ffa6c9;" | 102
| |
| | style="background: #ffa6c9;" | 110<ref name=Orton1996>{{cite journal|author=GS Orton|coauthors=G.R. Spencer, L.D. Travis, et al.|title=Galileo Photopolarimeter-radiometer observations of Jupiter and the Galilean Satellites|journal=Science|year=1996|volume=274|issue=5286|pages=389–391|bibcode=1996Sci...274..389O|doi=10.1126/science.274.5286.389}}</ref>
| |
| | style="background: #ffa6c9;" | 134
| |
| | style="background: #fbec5d;" | 64
| |
| | style="background: #fbec5d;" | 75
| |
| | style="background: #fbec5d;" | 64
| |
| | style="background: #fbec5d;" | 87
| |
| | style="background: #fbec5d;" | 76
| |
| |-
| |
| | colspan="2" style="background: #fffdd0;" | [[Atmosphere|Atmospheric]] composition
| |
| | style="background: #b0e0e6;" | [[Hydrogen|H]] [[Helium|He]] [[Sodium|Na]]<sup>+</sup> [[Potassium|K]]<sup>+</sup> [[Argon|Ar]]
| |
| | style="background: #ffa6c9;" | [[Sulphur dioxide|SO<sub>2</sub>]]<ref>{{cite journal|authors=JC Pearl, et al.| year=1979| title=Identification of gaseous SO2 and new upper limits for other gases on Io|journal=Nature|volume=288|issue=5725|pages=755| doi=10.1038/280755a0|bibcode=1979Natur.280..755P|last2=Hanel|first2=R.|last3=Kunde|first3=V.|last4=Maguire|first4=W.|last5=Fox|first5=K.|last6=Gupta|first6=S.|last7=Ponnamperuma|first7=C.|last8=Raulin|first8=F.}}</ref>
| |
| | style="background: #ffa6c9;" | [[Oxygen|O<sub>2</sub>]]<ref>D.T. Hall ''et al.''; [http://www.nature.com/nature/journal/v373/n6516/abs/373677a0.html ''Detection of an oxygen atmosphere on Jupiter's moon Europa''], [[Nature (journal)|Nature]], Vol. 373 1995, 677–679 (accessed 2006-15-04)</ref>
| |
| | style="background: #ffa6c9;" | [[Oxygen|O<sub>2</sub>]]<ref>{{cite journal|authors=DT Hall, PD Feldman, MA McGrath, et al.| year=1998|title=The Far-Ultraviolet Oxygen Airglow of Europa and Ganymede|journal=The Astrophysical Journal|volume=499|issue=1| pages=475–481|doi=10.1086/305604|bibcode=1998ApJ...499..475H}} Retrieved on 2008-11-17.</ref>
| |
| | style="background: #ffa6c9;" | [[Oxygen|O<sub>2</sub>]] [[Carbon dioxide|CO<sub>2</sub>]]<ref>{{cite journal|year=2005| title=Atmosphere of Callisto|journal=Journal of Geophysics Research|volume=110|issue=E02003|doi=10.1029/2004JE002322|url=http://yly-mac.gps.caltech.edu/ReprintsYLY/N164Liang_Callisto%2005/Liang_callisto_05.pdf|format=PDF|pages=E02003|bibcode=2005JGRE..11002003L| authors=Mao-Chang Liang, BF Lane, RT Pappalardo, et al.}} Retrieved on 2008-11-17.</ref>
| |
| | style="background: #fbec5d;" |
| |
| | style="background: #fbec5d;" | [[water|H<sub>2</sub>O]], [[Nitrogen|N<sub>2</sub>]], CO<sub>2</sub>, [[Methane|CH<sub>4</sub>]]<ref>{{cite journal|authors=JH Waite, et al.|year=2006|title=Cassini Ion and Neutral Mass Spectrometer: Enceladus Plume Composition and Structure|journal=Science|volume=311|issue=5766| pages=1419–1422|doi=10.1126/science.1121290|pmid=16527970| bibcode=2006Sci...311.1419W|last2=Combi|first2=MR|last3=Ip|first3=WH|last4=Cravens|first4=TE|last5=McNutt Jr|first5=RL| last6=Kasprzak|first6=W|last7=Yelle|first7=R|last8=Luhmann|first8=J|last9=Niemann|first9=H}} Retrieved on 2008-11-17.</ref>
| |
| | style="background: #fbec5d;" |
| |
| | style="background: #fbec5d;" |
| |
| | style="background: #fbec5d;" |
| |
| |-
| |
| | colspan="2" style="background: #fffdd0;" | [[Planetary ring|Rings?]]
| |
| | style="background: #b0e0e6;" | No
| |
| | style="background: #ffa6c9;" | No
| |
| | style="background: #ffa6c9;" | No
| |
| | style="background: #ffa6c9;" | No
| |
| | style="background: #ffa6c9;" | No
| |
| | style="background: #fbec5d;" | No
| |
| | style="background: #fbec5d;" | No
| |
| | style="background: #fbec5d;" | No
| |
| | style="background: #fbec5d;" | No
| |
| | style="background: #fbec5d;" | [[Rings of Rhea|Yes?]]
| |
| |}
| |
|
| |
|
| {| class="wikitable" border="1" style="text-align: center;"
| | == Nike Blazer Low Dame farve og grafik omhyggeligt == |
| |-
| |
| ! colspan="2" style="background: #fffdd0;" |
| |
| ! style="background: #fbec5d;" | <sup>$</sup>[[Titan (moon)|Titan]]{{ref label|P|p|none}}
| |
| ! style="background: #fbec5d;" | <sup>$</sup>[[Iapetus (moon)|Iapetus]]{{ref label|P|p|none}}
| |
| ! style="background: #7fffd4;" | <sup>₩</sup>[[Miranda (moon)|Miranda]]{{ref label|R|r|none}}
| |
| ! style="background: #7fffd4;" | <sup>₩</sup>[[Ariel (moon)|Ariel]]{{ref label|R|r|none}}
| |
| ! style="background: #7fffd4;" | <sup>₩</sup>[[Umbriel (moon)|Umbriel]]{{ref label|R|r|none}}
| |
| ! style="background: #7fffd4;" | <sup>₩</sup>[[Titania (moon)|Titania]]{{ref label|R|r|none}}
| |
| ! style="background: #7fffd4;" | <sup>₩</sup>[[Oberon (moon)|Oberon]]{{ref label|R|r|none}}
| |
| ! style="background: azure;" | <sup>₦</sup>[[Triton (moon)|Triton]]<ref name=nep>Triton info taken from [http://nssdc.gsfc.nasa.gov/planetary/factsheet/neptuniansatfact.html NASA Neptunian Satellite Fact Sheet] ''NASA'' Retrieved on 2009-01-18 (unless otherwise cited)</ref>
| |
| ! style="background: #ccf;" | <sup>¶</sup>[[Charon (moon)|Charon]]<ref name=Pluto/>
| |
| |-
| |
| | colspan="2" style="background: #fffdd0;" |
| |
| | style="background: #fbec5d;" | [[File:Titan in natural color Cassini.jpg|70px]]
| |
| | style="background: #fbec5d;" | [[File:Iapetus by Voyager 2 - enhanced.jpg|70px]]
| |
| | style="background: #7fffd4;" | [[File:Miranda.jpg|70px]]
| |
| | style="background: #7fffd4;" | [[File:Ariel (moon).jpg|70px]]
| |
| | style="background: #7fffd4;" | [[File:Umbriel moon 1.gif|70px]]
| |
| | style="background: #7fffd4;" | [[File:Titania (moon) color cropped.jpg|70px]]
| |
| | style="background: #7fffd4;" | [[File:Voyager 2 picture of Oberon.jpg|70 px]]
| |
| | style="background: azure;" | [[File:Triton Voyager 2.jpg|70 px]]
| |
| | style="background: #ccf;" | [[File:Charon.png|70 px]]
| |
| |-
| |
| | style="background: #fffdd0;" | Mean distance <br /> from primary:
| |
| | style="background: #fffdd0;" | km
| |
| | style="background: #fbec5d;" | 1,221,870
| |
| | style="background: #fbec5d;" | 3,560,820
| |
| | style="background: #7fffd4;" | 129,390
| |
| | style="background: #7fffd4;" | 190,900
| |
| | style="background: #7fffd4;" | 266,000
| |
| | style="background: #7fffd4;" | 436,300
| |
| | style="background: #7fffd4;" | 583,519
| |
| | style="background: azure;" | 354,759
| |
| | style="background: #ccf;" | 17,536
| |
| |-
| |
| | style="background: #fffdd0;" | Mean [[radius]]
| |
| | style="background: #fffdd0;" | km <br /> :E{{ref label|F|f|none}}
| |
| | style="background: #fbec5d;" | 2,576 <br /> 0.404
| |
| | style="background: #fbec5d;" | 735.60 <br /> 0.115
| |
| | style="background: #7fffd4;" | 235.8 <br /> 0.037
| |
| | style="background: #7fffd4;" | 578.9 <br /> 0.091
| |
| | style="background: #7fffd4;" | 584.7 <br /> 0.092
| |
| | style="background: #7fffd4;" | 788.9 <br /> 0.124
| |
| | style="background: #7fffd4;" | 761.4 <br /> 0.119
| |
| | style="background: azure;" | 1353.4 <br /> 0.212
| |
| | style="background: #ccf;" | 603.5 <br /> 0.095
| |
| |-
| |
| | style="background: #fffdd0;" | [[Surface area]]{{ref label|A|a|none}}
| |
| | style="background: #fffdd0;" | km² <br /> :E{{ref label|F|f|none}}
| |
| | style="background: #fbec5d;" | 83,000,000 <br /> 0.163
| |
| | style="background: #fbec5d;" | 6,700,000 <br /> 0.013
| |
| | style="background: #7fffd4;" | 700,000 <br /> 0.0014
| |
| | style="background: #7fffd4;" | 4,211,300 <br /> 0.008
| |
| | style="background: #7fffd4;" | 4,296,000 <br /> 0.008
| |
| | style="background: #7fffd4;" | 7,820,000 <br /> 0.015
| |
| | style="background: #7fffd4;" | 7,285,000 <br /> 0.014
| |
| | style="background: azure;" | 23,018,000 <br /> 0.045
| |
| | style="background: #ccf;" | 4,580,000 <br /> 0.009
| |
| |-
| |
| | style="background: #fffdd0;" | [[Volume]]{{ref label|B|b|none}}
| |
| | style="background: #fffdd0;" | km<sup>3</sup> <br /> :E{{ref label|F|f|none}}
| |
| | style="background: #fbec5d;" | 7.16{{e|10}} <br /> 0.066
| |
| | style="background: #fbec5d;" | 1.67{{e|9}} <br /> 0.0015
| |
| | style="background: #7fffd4;" | 5.5{{e|7}} <br /> 0.00005
| |
| | style="background: #7fffd4;" | 8.1{{e|8}} <br /> 0.0008
| |
| | style="background: #7fffd4;" | 8.4{{e|8}} <br /> 0.0008
| |
| | style="background: #7fffd4;" | 2.06{{e|9}} <br /> 0.0019
| |
| | style="background: #7fffd4;" | 1.85{{e|9}} <br /> 0.0017
| |
| | style="background: azure;" | 1{{e|10}} <br /> 0.00958
| |
| | style="background: #ccf;" | 9.2{{e|8}} <br /> 0.00085
| |
| |-
| |
| | style="background: #fffdd0;" | [[Mass]]
| |
| | style="background: #fffdd0;" | [[Kilogram|kg]] <br /> :E{{ref label|F|f|none}}
| |
| | style="background: #fbec5d;" | 1.3452{{e|23}} <br /> 0.023
| |
| | style="background: #fbec5d;" | 1.8053{{e|21}} <br /> 0.0003
| |
| | style="background: #7fffd4;" | 6.59{{e|19}} <br /> 0.00001
| |
| | style="background: #7fffd4;" | 1.35{{e|21}} <br /> 0.00022
| |
| | style="background: #7fffd4;" | 1.2{{e|21}} <br /> 0.0002
| |
| | style="background: #7fffd4;" | 3.5{{e|21}} <br /> 0.0006
| |
| | style="background: #7fffd4;" | 3.014{{e|21}} <br /> 0.00046
| |
| | style="background: azure;" | 2.14{{e|22}} <br /> 0.00358
| |
| | style="background: #ccf;" | 1.52{{e|21}} <br /> 0.00025
| |
| |-
| |
| | style="background: #fffdd0;" | [[Density]]{{ref label|C|c|none}}
| |
| | style="background: #fffdd0;" | [[Gram|g]]/cm<sup>3</sup>
| |
| | style="background: #fbec5d;" | 1.88
| |
| | style="background: #fbec5d;" | 1.08
| |
| | style="background: #7fffd4;" | 1.20
| |
| | style="background: #7fffd4;" | 1.67
| |
| | style="background: #7fffd4;" | 1.40
| |
| | style="background: #7fffd4;" | 1.72
| |
| | style="background: #7fffd4;" | 1.63
| |
| | style="background: azure;" | 2.061
| |
| | style="background: #ccf;" | 1.65
| |
| |-
| |
| | style="background: #fffdd0;" | [[Equator]]ial [[gravity]]{{ref label|D|d|none}}
| |
| | style="background: #fffdd0;" | [[Acceleration|m/s<sup>2</sup>]]
| |
| | style="background: #fbec5d;" | 1.35
| |
| | style="background: #fbec5d;" | 0.22
| |
| | style="background: #7fffd4;" | 0.08
| |
| | style="background: #7fffd4;" | 0.27
| |
| | style="background: #7fffd4;" | 0.23
| |
| | style="background: #7fffd4;" | 0.39
| |
| | style="background: #7fffd4;" | 0.35
| |
| | style="background: azure;" | 0.78
| |
| | style="background: #ccf;" | 0.28
| |
| |-
| |
| | style="background: #fffdd0;" | [[Escape velocity]]{{ref label|E|e|none}}
| |
| | style="background: #fffdd0;" | [[Speed|km/s]]
| |
| | style="background: #fbec5d;" | 2.64
| |
| | style="background: #fbec5d;" | 0.57
| |
| | style="background: #7fffd4;" | 0.19
| |
| | style="background: #7fffd4;" | 0.56
| |
| | style="background: #7fffd4;" | 0.52
| |
| | style="background: #7fffd4;" | 0.77
| |
| | style="background: #7fffd4;" | 0.73
| |
| | style="background: azure;" | 1.46
| |
| | style="background: #ccf;" | 0.58
| |
| |-
| |
| | style="background: #fffdd0;" | Rotation period
| |
| | style="background: #fffdd0;" | days{{ref label|G|g|none}}
| |
| | style="background: #fbec5d;" | 15.945 <br /> (sync){{ref label|M|m|none}}
| |
| | style="background: #fbec5d;" | 79.322 <br /> (sync)
| |
| | style="background: #7fffd4;" | 1.414 <br /> (sync)
| |
| | style="background: #7fffd4;" | 2.52 <br /> (sync)
| |
| | style="background: #7fffd4;" | 4.144 <br /> (sync)
| |
| | style="background: #7fffd4;" | 8.706 <br /> (sync)
| |
| | style="background: #7fffd4;" | 13.46 <br /> (sync)
| |
| | style="background: azure;" | 5.877 <br /> (sync)
| |
| | style="background: #ccf;" | 6.387 <br /> (sync)
| |
| |-
| |
| | style="background: #fffdd0;" | Orbital period about primary
| |
| | style="background: #fffdd0;" | days
| |
| | style="background: #fbec5d;" | 15.945
| |
| | style="background: #fbec5d;" | 79.322
| |
| | style="background: #7fffd4;" | 1.4135
| |
| | style="background: #7fffd4;" | 2.520
| |
| | style="background: #7fffd4;" | 4.144
| |
| | style="background: #7fffd4;" | 8.706
| |
| | style="background: #7fffd4;" | 13.46
| |
| | style="background: azure;" | −5.877{{ref label|H|h|none}}
| |
| | style="background: #ccf;" | 6.387
| |
| |-
| |
| | style="background: #fffdd0;" | Mean orbital speed{{ref label|O|o|none}}
| |
| | style="background: #fffdd0;" | [[Speed|km/s]]
| |
| | style="background: #fbec5d;" | 5.57
| |
| | style="background: #fbec5d;" | 3.265
| |
| | style="background: #7fffd4;" | 6.657
| |
| | style="background: #7fffd4;" | 5.50898
| |
| | style="background: #7fffd4;" | 4.66797
| |
| | style="background: #7fffd4;" | 3.644
| |
| | style="background: #7fffd4;" | 3.152
| |
| | style="background: azure;" | 4.39
| |
| | style="background: #ccf;" | 0.2
| |
| |-
| |
| | colspan="2" style="background: #fffdd0;" | [[Eccentricity (orbit)|Eccentricity]]
| |
| | style="background: #fbec5d;" | 0.0288
| |
| | style="background: #fbec5d;" | 0.0286
| |
| | style="background: #7fffd4;" | 0.0013
| |
| | style="background: #7fffd4;" | 0.0012
| |
| | style="background: #7fffd4;" | 0.005
| |
| | style="background: #7fffd4;" | 0.0011
| |
| | style="background: #7fffd4;" | 0.0014
| |
| | style="background: azure;" | 0.00002
| |
| | style="background: #ccf;" | 0.0022
| |
| |-
| |
| | style="background: #fffdd0;" | [[Inclination]] to primary's equator
| |
| | style="background: #fffdd0;" | [[Degree (angle)|deg.]]
| |
| | style="background: #fbec5d;" | 0.33
| |
| | style="background: #fbec5d;" | 14.72
| |
| | style="background: #7fffd4;" | 4.22
| |
| | style="background: #7fffd4;" | 0.31
| |
| | style="background: #7fffd4;" | 0.36
| |
| | style="background: #7fffd4;" | 0.14
| |
| | style="background: #7fffd4;" | 0.10
| |
| | style="background: azure;" | 157
| |
| | style="background: #ccf;" | ?
| |
| |-
| |
| | style="background: #fffdd0;" | [[Axial tilt]]{{ref label|I|i|none}}{{ref label|U|u|none}}
| |
| | style="background: #fffdd0;" | [[Degree (angle)|deg.]]
| |
| | style="background: #fbec5d;" | 0
| |
| | style="background: #fbec5d;" | 0
| |
| | style="background: #7fffd4;" | 0
| |
| | style="background: #7fffd4;" | 0
| |
| | style="background: #7fffd4;" | 0
| |
| | style="background: #7fffd4;" | 0
| |
| | style="background: #7fffd4;" | 0
| |
| | style="background: azure;" | 0
| |
| | style="background: #ccf;" | ?
| |
| |-
| |
| | style="background: #fffdd0;" | Mean surface [[temperature]]{{ref label|W|w|none}}
| |
| | style="background: #fffdd0;" | [[Kelvin|K]]
| |
| | style="background: #fbec5d;" | 93.7<ref>{{cite web
| |
| |title=Optical Properties of Titan Haze Laboratory Analogs Using Cavity Ring Down Spectroscopy
| |
| |author= C. A. Hasenkopf
| |
| |year=2007
| |
| |work=Workshop on Planetary Atmospheres
| |
| |url=http://webcache.googleusercontent.com/search?q=cache:H1UhAFtLEpEJ:www.lpi.usra.edu/meetings/patm2007/pdf/9034.pdf+titan+anti-greenhouse-effect+2006+OR+2007&hl=en&ct=clnk&cd=3&gl=uk
| |
| |accessdate=2007-10-16
| |
| }}</ref>
| |
| | style="background: #fbec5d;" | 130
| |
| | style="background: #7fffd4;" | 59
| |
| | style="background: #7fffd4;" | 58
| |
| | style="background: #7fffd4;" | 61
| |
| | style="background: #7fffd4;" | 60
| |
| | style="background: #7fffd4;" | 61
| |
| | style="background: azure;" | 38 <ref>{{cite journal
| |
| | title = Spectroscopic Determination of the Phase Composition and Temperature of Nitrogen Ice on Triton
| |
| | author= Kimberly Tryka, Robert Brown, V. Anicich et al.
| |
| | journal = Science
| |
| | volume = 261
| |
| | issue = 5122
| |
| | pages = 751–754
| |
| | bibcode = 1993Sci...261..751T
| |
| |date=August 1993
| |
| | doi = 10.1126/science.261.5122.751
| |
| | pmid = 17757214
| |
| }}</ref>
| |
| | style="background: #ccf;" | 53
| |
| |-
| |
| | colspan="2" style="background: #fffdd0;" | [[Atmosphere|Atmospheric]] composition
| |
| | style="background: #fbec5d;" | [[Nitrogen|N<sub>2</sub>]], [[Methane|CH<sub>4</sub>]]<ref>
| |
| {{cite journal | title= The abundances of constituents of Titan's atmosphere from the GCMS instrument on the Huygens probe |author= H. B. Niemann, et al. |journal= [[Nature (journal)|Nature]] |volume=438 | issue= 7069 |pages=779–784 |year=2005 | pmid= 16319830 |doi=10.1038/nature04122 |bibcode = 2005Natur.438..779N }}</ref>
| |
| | style="background: #fbec5d;" |
| |
| | style="background: #7fffd4;" |
| |
| | style="background: #7fffd4;" |
| |
| | style="background: #7fffd4;" |
| |
| | style="background: #7fffd4;" |
| |
| | style="background: #7fffd4;" |
| |
| | style="background: azure;" | [[Nitrogen|N<sub>2</sub>]], [[Methane|CH<sub>4</sub>]]<ref name=nature2>{{cite journal
| |
| | title = Ultraviolet Spectrometer Observations of Neptune and Triton
| |
| | author = A L Broadfoot, S K Bertaux, J E Dessler et al.
| |
| | bibcode = 1989Sci...246.1459B
| |
| | date = 1989-12-15
| |
| | journal = Science
| |
| | volume = 246
| |
| | pages = 1459–1466
| |
| | doi = 10.1126/science.246.4936.1459
| |
| | pmid = 17756000
| |
| | issue = 4936 | |
| }}</ref>
| |
| | style="background: #ccf;" |
| |
| |}
| |
|
| |
|
| == Largest likely dwarf planets == | | Af alle de søgemaskiner, Google det bedste job at respektere det. Vellykket er observeret ved anvendelse op billederne med pay begrundelse, et quasi billeder ansøgning op langs pay stemma, vinder du. Didn tror det gav mening, og bedt dem om at kontrollere igen, rep sagde. <br><br>Denne aldersgruppe går fremad ind Junior Rugby ser frem til en lys fremtid ... De unge, som endnu ikke uåbnede, blade blev trukket ud fra opløbet i centrum af palme, og disse var de dele faktisk anvendes. Hvis du ikke har de tekniske færdigheder eller blot tid til at oprette og administrere links, der er virksomheder, der kan give link bygningsteknik. <br><br>Mens træ rør er nyttige og gøre et udmærket supplement til alle samlinger, er der simpelthen ingen slå et glas pibe. Når du strække eller bøje fingeren til pop skank, du forårsager knoglerne i joint at trække fra hinanden. Denne information er også kendt som whois information. <br><br>Hun tæller ned top 10 sundeste, alkalineforming fødevarer, vi skal spise. Vælg tekst, farve og grafik omhyggeligt, de alle bidrager til den side indlæsningstid. Ny polstring og maling har taget denne bil til en solid 2plus bedømmelse på betingelse skalaen ... <br><br>Hun er virkelig god til det må jeg indrømme. Også inkluderet er de talrige stilarter bære dem baseret på en af de episoder af The Oprah Winfrey Show. Selv på Valentinsdag har jeg en begivenhed i aften. Hver CoolSculpting procedure resulterer i en 20% reduktion af fedt Resultater ses over en periode på en til tre måneder. <br><br>Arbejde ud før en stor dato Hver fyr kender det føles fantastisk at snige en løbetur eller endda et par pushups i, før en dato. Bad for SEO Flash design er ikke SEO venlige. Indiens søgen efter missilteknologi har ikke været jævn. Historisk hjem til Kumeyaay folk var San Diego det første websted besøgt af europæere på, hvad er nu det vestkysten af USA. <br><br>Giv det tid, vil flere og flere Adobe CC (CS) produkter være tilgængelige uden for Windows og OS X.. Lyrics: Sekai de ichiban ohimesama Sou iu atsukai Kokoro ete yo ne Sono ichi Itsumo til chigau kamigata ni ki ga tsuku koto Sono ni CHANTO [http://www.hotel-nygaard.dk/log/Gallery/crypt.asp?d=83-Nike-Blazer-Low-Dame Nike Blazer Low Dame] kutsu lavet Miru koto ii ne? Sono san watashi ingen hitokoto ni wa mittsu ingen Kotoba de henji suru koto Wakattara migite ga orusu nano wo nantoka shite Betsu ni wagamama Nante itte nai [http://www.asherregaard.dk/delikatesser/umenu/client.asp?h=28 Michael Kors Tasker Illum] n dakara Kimi ni Kokoro kara omotte hoshii ingen kawaii tte Sekai de ichiban ohimesama Ki ga tsuite nee nee Mataseru Nante Rongai yo Watashi wo dare Dato omotteru nej? Mou Nanda ka Amai mono ga tabetai! Ima Sugu ni yo Ah! Check én, [http://www.asherregaard.dk/delikatesser/umenu/client.asp?h=11 Michael Kors Iphone 4 Covers] to! Aa! Ketten? Kawaii ingen machigai Desho Monku wa yurushimasen ingen Ano ne? Watashi ingen [http://www.jyskgenbrug.dk/images/file.asp?d=30-Buy-New-Balance-Online-Us Buy New Balance Online Us] Hanashi CHANTO kiiteru? Chotto.<ul> |
| {{Main|List of possible dwarf planets}}
| | |
| These [[trans-Neptunian object]]s are theoretically large enough to be dwarf planets. Dozens more could have been included.<ref name=mike>{{cite web|title=The Dwarf Planets |author=Mike Brown|publisher=CalTech|url=http://www.gps.caltech.edu/~mbrown/dwarfplanets/|accessdate=2008-09-25}}</ref> Both [[50000 Quaoar|Quaoar]] and [[90482 Orcus|Orcus]] have known moons that have allowed the mass of the systems to be determined. Both are more massive than the 5{{e|20}} kg recommendation of the [[IAU definition of planet#Draft proposal|IAU 2006 draft proposal]] as sufficient for classification as a dwarf planet.<ref name=IAU-draft2006>{{cite web
| | <li>[http://f1sqg2003.free.fr/forum.php?mod=viewthread&tid=440311 http://f1sqg2003.free.fr/forum.php?mod=viewthread&tid=440311]</li> |
| |title=The Path to Defining Planets
| | |
| |author=O. Gingerich
| | <li>[http://honbbs.com/forum.php?mod=viewthread&tid=2162636 http://honbbs.com/forum.php?mod=viewthread&tid=2162636]</li> |
| |work=Harvard-Smithsonian Center for Astrophysics and IAU EC Planet Definition Committee chair
| | |
| |year=2006
| | <li>[http://4187.n.uuuke.com/news/html/?31945.html http://4187.n.uuuke.com/news/html/?31945.html]</li> |
| |url=http://astro.cas.cz/nuncius/nsiii_03.pdf
| | |
| |accessdate=2007-03-13
| | <li>[http://ldsbee.com/index.php?page=item&id=2407149 http://ldsbee.com/index.php?page=item&id=2407149]</li> |
| |format=PDF}}</ref> | | |
| | <li>[http://www.metransparent.com/spip.php?article21662&lang=ar&id_forum=37102/ http://www.metransparent.com/spip.php?article21662&lang=ar&id_forum=37102/]</li> |
| | |
| | </ul> |
|
| |
|
| {| class="wikitable" border="1" style="text-align: center;"
| | == Michael Kors Pung hvor vi kan se over en kontrakt == |
| |-
| |
| ! colspan="2" style="background: #fffdd0;" |
| |
| ! style="background: #eff;" | [[90482 Orcus|Orcus]]<ref>{{cite web
| |
| |date=2008-02-10 last obs
| |
| |title=JPL Small-Body Database Browser: 90482 Orcus (2004 DW)
| |
| |publisher=NASA JPL
| |
| |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=Orcus
| |
| |accessdate=2008-07-02}} (unless otherwise cited)</ref>
| |
| ! style="background: #eff;" | [[28978 Ixion|Ixion]]<ref>{{cite web
| |
| |date=2007-07-12 last obs
| |
| |publisher=NASA JPL
| |
| |title=JPL Small-Body Database Browser: 28978 Ixion (2001 KX76)
| |
| |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=Ixion
| |
| |accessdate=2008-10-04}} (unless otherwise cited)</ref>
| |
| ! style="background: #eff;" | {{mpl-|307261|2002 MS|4}}<ref>{{cite web
| |
| |date=2009-09-19 last obs
| |
| |title=JPL Small-Body Database Browser: 307261 (2002 MS4)
| |
| |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=307261
| |
| |accessdate=2013-12-23}} (unless otherwise cited)</ref>
| |
| ! style="background: #eff;" | [[120347 Salacia|Salacia]]<ref>{{cite web
| |
| |date=2010-11-05 last obs
| |
| |title=JPL Small-Body Database Browser: 120347 Salacia
| |
| |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=120347
| |
| |accessdate=2013-12-23}} (unless otherwise cited)</ref>
| |
| ! style="background: #eff;" | [[20000 Varuna|Varuna]]<ref>{{cite web
| |
| |date=2007-11-17 last obs
| |
| |title=JPL Small-Body Database Browser: 20000 Varuna (2000 WR106)
| |
| |publisher=NASA JPL
| |
| |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=20000
| |
| |accessdate=2008-07-02}} (unless otherwise cited)</ref>
| |
| ! style="background: #eff;" | {{mpl-|202421|2005 UQ|513}}<ref>{{cite web
| |
| |date=2008-11-29 last obs
| |
| |title=JPL Small-Body Database Browser: (2005 UQ513)
| |
| |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2005UQ513
| |
| |accessdate=2008-07-31}}(unless otherwise cited)</ref>
| |
| ! style="background: #eff;" | [[50000 Quaoar|Quaoar]]<ref>{{cite web|title=NASA JPL Database Browser: 50000 Quaoar|url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=50000|publisher=NASA JPL|accessdate=2008-12-19}} (unless otherwise cited)</ref>
| |
| ! style="background: #eff;" | {{mpl-|225088|2007 OR|10}}<ref>{{cite web|title=NASA Small Bodies Database Browser: 2007 OR10|publisher=NASA JPL|url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2007OR10|accessdate=2008-12-20}} (unless otherwise cited)</ref>
| |
| ! style="background: #eff;" | {{mpl-|229762|2007 UK|126}}<ref>{{cite web
| |
| |date=2009-12-20 last obs
| |
| |title=JPL Small-Body Database Browser: 229762 (2007 UK126)
| |
| |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=229762
| |
| |accessdate=2010-05-02}} (unless otherwise cited)</ref>
| |
| ! style="background: #eff;" | [[90377 Sedna|Sedna]]<ref>{{cite web
| |
| |author=[[Marc W. Buie]]
| |
| |date=2007-08-13
| |
| |title=Orbit Fit and Astrometric record for 90377
| |
| |publisher=[[Deep Ecliptic Survey]]
| |
| |url=http://www.boulder.swri.edu/~buie/kbo/astrom/90377.html
| |
| |accessdate=2006-01-17}} (unless otherwise cited)</ref>
| |
| |-
| |
| | colspan="2" style="background: #fffdd0;" |
| |
| | style="background: #eff;" | [[File:Orcus nasa.jpg|70 px]]
| |
| | style="background: #eff;" | [[File:Ixion planetoid nasa.jpg|70 px]]
| |
| | style="background: #eff;" |
| |
| | style="background: #eff;" |
| |
| | style="background: #eff;" | [[File:Varuna artistic.png|70 px]]
| |
| | style="background: #eff;" |
| |
| | style="background: #eff;" | [[File:Quaoar PRC2002-17e.jpg|70 px]]
| |
| | style="background: #eff;" | [[File:2007 OR10 artist.png|70 px]]
| |
| | style="background: #eff;" | [[File:MinorPlanet-2007uk126-19970930.gif|70 px]]
| |
| | style="background: #eff;" | [[File:Ssc2004-05b.jpg|70 px]]
| |
| |-
| |
| | colspan="2" style="background: #fffdd0;" | [[Minor planet designation|Minor-planet number]]
| |
| | style="background: #eff;" | 90482
| |
| | style="background: #eff;" | 28978
| |
| | style="background: #eff;" | 307361
| |
| | style="background: #eff;" | 120347
| |
| | style="background: #eff;" | 20000
| |
| | style="background: #eff;" | 202421
| |
| | style="background: #eff;" | 50000
| |
| | style="background: #eff;" | 225088
| |
| | style="background: #eff;" | 229762
| |
| | style="background: #eff;" | 90377
| |
| |-
| |
| | style="background: #fffdd0;" | [[Semi-major axis]]
| |
| | style="background: #fffdd0;" | km <br> [[Astronomical unit|AU]]
| |
| | style="background: #eff;" | 5,896,946,000 <br> 39.419
| |
| | style="background: #eff;" | 5,935,999,000 <br> 39.68
| |
| | style="background: #eff;" | 6,273,000,000 <br> 41.93
| |
| | style="background: #eff;" | 6,311,000,000 <br> 42.19
| |
| | style="background: #eff;" | 6,451,398,000 <br> 43.13
| |
| | style="background: #eff;" | 6,479,089,380 <br> 43.31
| |
| | style="background: #eff;" | 6,493,296,000 <br> 43.6
| |
| | style="background: #eff;" | 10,072,433,340 <br> 67.33
| |
| | style="background: #eff;" | 11,032,000,000 <br> 73.74
| |
| | style="background: #eff;" | 78,668,000,000 <br> 525.86
| |
| |-
| |
| | style="background: #fffdd0;" | Mean [[radius]]{{ref label|S|s|none}}
| |
| | style="background: #fffdd0;" | km <br> :E{{ref label|F|f|none}}
| |
| | style="background: #eff;" | 473 <br> 0.0742
| |
| | style="background: #eff;" | 402 <br> 0.063
| |
| | style="background: #eff;" | 467<ref name=TNOsCool6>
| |
| {{cite web
| |
| |title="TNOs are Cool": A survey of the trans-Neptunian region VI. Herschel/PACS observations and thermal modeling of 19 classical Kuiper belt objects
| |
| |author=Vilenius, E., Kiss, C., Mommert, M. et al.
| |
| |date=April 4, 2012
| |
| |url=http://arxiv.org/pdf/1204.0697.pdf
| |
| |accessdate=2012-05-07}}
| |
| </ref> <br> 0.073
| |
| | style="background: #eff;" | 427<ref name=TNOsCool8>S. Fornasier, E. Lellouch, T. Müller, P. Santos-Sanz, P. Panuzzo, C. Kiss, T. Lim, M. Mommert, D. Bockelée-Morvan, E. Vilenius, J. Stansberry, G.P. Tozzi, S. Mottola, A. Delsanti, J. Crovisier, R. Duffard, F. Henry, P. Lacerda, A. Barucci, & A. Gicquel (2013). [http://arxiv.org/pdf/1305.0449v2.pdf TNOs are Cool: A survey of the trans-Neptunian region. VIII. Combined Herschel PACS and SPIRE observations of 9 bright targets at 70–500 ''µ''m.]</ref> <br> 0.067
| |
| | style="background: #eff;" | ~350 <br> 0.055
| |
| | style="background: #eff;" | 460 <br> 0.072{{ref label|AA|aa|none}}
| |
| | style="background: #eff;" | 422 <br> 0.066
| |
| | style="background: #eff;" | ~640 <br> 0.10
| |
| | style="background: #eff;" | 440 <br> 0.07{{ref label|AA|aa|none}}
| |
| | style="background: #eff;" | ~500 <br> 0.08
| |
| |-
| |
| | style="background: #fffdd0;" | [[Surface area]]{{ref label|A|a|none}}
| |
| | style="background: #fffdd0;" | km² <br> :E{{ref label|F|f|none}}
| |
| | style="background: #eff;" | 2,811,462 <br> 0.0055
| |
| | style="background: #eff;" | 2,030,775 <br> 0.00398
| |
| | style="background: #eff;" | ?
| |
| | style="background: #eff;" | ?
| |
| | style="background: #eff;" | 1,091,000 <br> 0.00636
| |
| | style="background: #eff;" | 2,659,044 <br> 0.0052
| |
| | style="background: #eff;" | 2,237,870 <br> 0.00439
| |
| | style="background: #eff;" | 6,157,522 <br> 0.012
| |
| | style="background: #eff;" | 2,432,849 <br> 0.005
| |
| | style="background: #eff;" | 3,000,000 <br> 0.006
| |
| |-
| |
| | style="background: #fffdd0;" | [[Volume]]{{ref label|B|b|none}}
| |
| | style="background: #fffdd0;" | km<sup>3</sup> <br> :E{{ref label|F|f|none}}
| |
| | style="background: #eff;" | 443,273,768 <br> 0.0004
| |
| | style="background: #eff;" | 272,123,951 <br> 0.0002
| |
| | style="background: #eff;" | ?
| |
| | style="background: #eff;" | ?
| |
| | style="background: #eff;" | 549,135,785 <br> 0.0005
| |
| | style="background: #eff;" | 407,720,083 <br> 0.0003
| |
| | style="background: #eff;" | 314,793,649 <br> 0.0002
| |
| | style="background: #eff;" | 1,436,755,040 <br> 0.001
| |
| | style="background: #eff;" | 356,817,905 <br> 0.0002
| |
| | style="background: #eff;" | 500,000,000 <br> 0.0005
| |
| |-
| |
| | style="background: #fffdd0;" | [[Mass]]{{ref label|T|t|none}}
| |
| | style="background: #fffdd0;" | [[Kilogram|kg]] <br> :E{{ref label|F|f|none}}
| |
| | style="background: #eff;" | 6.32{{e|20}}<ref name="Brown2009">{{cite journal
| |
| |last=Brown |first=M.E.
| |
| |coauthors=Ragozzine, D.; Stansberry, J.; Fraser, W.C.
| |
| |title=The size, density, and formation of the Orcus-Vanth system in the Kuiper belt
| |
| |journal=AJ
| |
| |volume= 139|pages= 2700|year=2009
| |
| |doi= 10.1088/0004-6256/139/6/2700
| |
| |arxiv=0910.4784
| |
| |bibcode = 2010AJ....139.2700B
| |
| |issue=6 }}</ref> <br> 0.0001
| |
| | style="background: #eff;" | 5.4{{e|20}} <br> 0.00009
| |
| | style="background: #eff;" | ?
| |
| | style="background: #eff;" | 4.5{{e|20}}<ref name="Stansberry-result">{{cite web
| |
| |title=Physical Properties of Trans-Neptunian Binaries (120347) Salacia–Actaea and (42355) Typhon–Echidna
| |
| |publisher=[[Elsevier]]
| |
| |author=J.A. Stansberry
| |
| |year=2012
| |
| |url=http://www.sciencedirect.com/science/article/pii/S0019103512001224
| |
| |accessdate=2012-04-27}}</ref> <br> 0.000075
| |
| | style="background: #eff;" | 5.5{{e|20}} <br> 0.00009
| |
| | style="background: #eff;" | 8.2{{e|20}} <br> 0.0001
| |
| | style="background: #eff;" | (1.3–1.9){{e|21}}<ref name=weywot>{{cite conference
| |
| |last=Brown |first=M.E. | |
| |coauthors=Fraser, Wesley
| |
| |title=Quaoar: A Rock in the Kuiper Belt
| |
| |conference=DPS meeting #41
| |
| |publisher=American Astronomical Society
| |
| |year=2009
| |
| |bibcode=2009DPS....41.6503F
| |
| }} [http://solarsystemwatch.blogspot.com/2009/10/quaoar-giant-rock-in-icy-kuiper-belt.html (Backup reference)]</ref> <br> 0.0004
| |
| | style="background: #eff;" | 2.9{{e|21}} <br> 0.0005
| |
| | style="background: #eff;" | 7.1{{e|20}} <br> 0.0001
| |
| | style="background: #eff;" | 1{{e|21}} <br> 0.00016
| |
| |-
| |
| | style="background: #fffdd0;" | [[Density]]{{ref label|T|t|none}}
| |
| | style="background: #fffdd0;" | [[Gram|g]]/cm<sup>3</sup>
| |
| | style="background: #eff;" | 1.5±0.3<ref name="Brown2009"/>
| |
| | style="background: #eff;" | 2.0
| |
| | style="background: #eff;" | ?
| |
| | style="background: #eff;" | 1.16<ref name="Stansberry-result"/>
| |
| | style="background: #eff;" | 0.9992<ref name=jewitt/>
| |
| | style="background: #eff;" | 2.0
| |
| | style="background: #eff;" | >2.8<ref name=weywot/>
| |
| | style="background: #eff;" | 2.0
| |
| | style="background: #eff;" | 2.0
| |
| | style="background: #eff;" | 2.0
| |
| |-
| |
| | style="background: #fffdd0;" | [[Equator]]ial [[gravity]]{{ref label|D|d|none}}
| |
| | style="background: #fffdd0;" | [[Acceleration|m/s<sup>2</sup>]]
| |
| | style="background: #eff;" | 0.27
| |
| | style="background: #eff;" | 0.22
| |
| | style="background: #eff;" | ?
| |
| | style="background: #eff;" | {{Gr|1.16|854|2}}
| |
| | style="background: #eff;" | 0.14
| |
| | style="background: #eff;" | 0.26
| |
| | style="background: #eff;" | 0.24
| |
| | style="background: #eff;" | <0.39
| |
| | style="background: #eff;" | 0.25
| |
| | style="background: #eff;" | <0.5
| |
| |-
| |
| | style="background: #fffdd0;" | [[Escape velocity]]{{ref label|E|e|none}}
| |
| | style="background: #fffdd0;" | [[Speed|km/s]]
| |
| | style="background: #eff;" | 0.50
| |
| | style="background: #eff;" | 0.42
| |
| | style="background: #eff;" | ?
| |
| | style="background: #eff;" | {{v2|1.16|854|2}}
| |
| | style="background: #eff;" | 0.38
| |
| | style="background: #eff;" | 0.49
| |
| | style="background: #eff;" | 0.45
| |
| | style="background: #eff;" | <0.74
| |
| | style="background: #eff;" | 0.46
| |
| | style="background: #eff;" | <1.0
| |
| |-
| |
| | style="background: #fffdd0;" | Rotation period{{ref label|G|g|none}}
| |
| | style="background: #fffdd0;" | days
| |
| | style="background: #eff;" | ?
| |
| | style="background: #eff;" | ?
| |
| | style="background: #eff;" | ?
| |
| | style="background: #eff;" | 0.25
| |
| | style="background: #eff;" | 0.13216<ref name=jewitt>{{cite journal|title=Physical Properties of Trans-Neptunian Object (20000) Varuna|author=David C. Jewitt and Scott S. Sheppard |journal=The Astronomical Journal|volume=123|issue=4|pages=2110–2120|year=2002|url=http://www.iop.org/EJ/article/1538-3881/123/4/2110/201498.html|doi=10.1086/339557|bibcode=2002AJ....123.2110J|arxiv = astro-ph/0201082 }} Retrieved on 2008-12-19.</ref>
| |
| | style="background: #eff;" | ?
| |
| | style="background: #eff;" | ?
| |
| | style="background: #eff;" | ?
| |
| | style="background: #eff;" | ?
| |
| | style="background: #eff;" | 0.42<ref>{{cite web|title=Case of Sedna's Missing Moon Solved|publisher=Harvard Smithsonian Center for Astrophysics|year=2005|url=http://www.cfa.harvard.edu/news/2005/pr200510.html|accessdate=2011-07-05}}</ref>
| |
| |-
| |
| | style="background: #fffdd0;" | Orbital period{{ref label|G|g|none}}
| |
| | style="background: #fffdd0;" | [[Julian year (astronomy)|years]]
| |
| | style="background: #eff;" | 247.492
| |
| | style="background: #eff;" | 249.95
| |
| | style="background: #eff;" | 271.53
| |
| | style="background: #eff;" | 274.03
| |
| | style="background: #eff;" | 283.20
| |
| | style="background: #eff;" | 285.12
| |
| | style="background: #eff;" | 287.97
| |
| | style="background: #eff;" | 552.52
| |
| | style="background: #eff;" | 633.28
| |
| | style="background: #eff;" | 12,059.06
| |
| |-
| |
| | style="background: #fffdd0;" | Mean orbital speed
| |
| | style="background: #fffdd0;" | [[Speed|km/s]]
| |
| | style="background: #eff;" | 4.68
| |
| | style="background: #eff;" | 4.66
| |
| | style="background: #eff;" | ?
| |
| | style="background: #eff;" | ?
| |
| | style="background: #eff;" | 4.53
| |
| | style="background: #eff;" | 4.52
| |
| | style="background: #eff;" | 4.52
| |
| | style="background: #eff;" | 3.63
| |
| | style="background: #eff;" | 3.25
| |
| | style="background: #eff;" | 1.04
| |
| |-
| |
| | colspan="2" style="background: #fffdd0;" | [[Eccentricity (orbit)|Eccentricity]]
| |
| | style="background: #eff;" | 0.22552
| |
| | style="background: #eff;" | 0.242
| |
| | style="background: #eff;" | 0.148
| |
| | style="background: #eff;" | 0.10312
| |
| | style="background: #eff;" | 0.051
| |
| | style="background: #eff;" | 0.145
| |
| | style="background: #eff;" | 0.038
| |
| | style="background: #eff;" | 0.5
| |
| | style="background: #eff;" | 0.490
| |
| | style="background: #eff;" | 0.855
| |
| |-
| |
| | style="background: #fffdd0;" | [[Inclination]]{{ref label|F|f|none}}
| |
| | style="background: #fffdd0;" | [[Degree (angle)|deg.]]
| |
| | style="background: #eff;" | 22.5
| |
| | style="background: #eff;" | 19.6
| |
| | style="background: #eff;" | 17.693
| |
| | style="background: #eff;" | 23.9396
| |
| | style="background: #eff;" | 17.2
| |
| | style="background: #eff;" | 25.69
| |
| | style="background: #eff;" | 8
| |
| | style="background: #eff;" | 30.7
| |
| | style="background: #eff;" | 23.37
| |
| | style="background: #eff;" | 11.93
| |
| |-
| |
| | style="background: #fffdd0;" | Mean surface [[temperature]]{{ref label|W|w|none}}
| |
| | style="background: #fffdd0;" | [[Kelvin|K]]
| |
| | style="background: #eff;" | ~42
| |
| | style="background: #eff;" | ~43
| |
| | style="background: #eff;" | ?
| |
| | style="background: #eff;" | ?
| |
| | style="background: #eff;" | ~43
| |
| | style="background: #eff;" | ~41
| |
| | style="background: #eff;" | ~41
| |
| | style="background: #eff;" | ~30
| |
| | style="background: #eff;" | ~32
| |
| | style="background: #eff;" | ~12
| |
| |-
| |
| | colspan="2" style="background: #fffdd0;" | Number of known [[Natural satellite|moons]]
| |
| | style="background: #eff;" | 1<ref name="Distant EKO">[http://www.boulder.swri.edu/ekonews/issues/past/n051/html/index.html Distant EKO] The Kuiper Belt Electronic newsletter, March 2007 Retrieved on 2008-11-17</ref>
| |
| | style="background: #eff;" | 0
| |
| | style="background: #eff;" | 0
| |
| | style="background: #eff;" | 1
| |
| | style="background: #eff;" | 0
| |
| | style="background: #eff;" | 0
| |
| | style="background: #eff;" | 1<ref>{{cite web|title=IAUC 8812: Sats OF 2003 AZ_84, (50000), (55637),, (90482); V1281 Sco; V1280 Sco|url=http://www.cbat.eps.harvard.edu/iauc/08800/08812.html|publisher=International Astronomical Union|accessdate=2011-07-05}}</ref>
| |
| | style="background: #eff;" | 0
| |
| | style="background: #eff;" | 0
| |
| | style="background: #eff;" | 0
| |
| |-
| |
| | colspan="2" style="background: #fffdd0;" | [[Clearing the neighbourhood|Planetary discriminant]]{{ref label|L|l|none}}{{ref label|O|o|none}}
| |
| | style="background: #eff;" | 0.003
| |
| | style="background: #eff;" | 0.0027
| |
| | style="background: #eff;" | <0.1
| |
| | style="background: #eff;" | <0.1
| |
| | style="background: #eff;" | 0.0027
| |
| | style="background: #eff;" | 0.003
| |
| | style="background: #eff;" | 0.0015
| |
| | style="background: #eff;" | <0.1
| |
| | style="background: #eff;" | 0.036{{ref label|X|x|none}}
| |
| | style="background: #eff;" | ?{{ref label|X|x|none}}
| |
| |-
| |
| | colspan="2" style="background: #fffdd0;" | [[Absolute magnitude#Solar System bodies (H)|Absolute magnitude (H)]]
| |
| | style="background: #eff;" | 2.30
| |
| | style="background: #eff;" | 3.20
| |
| | style="background: #eff;" | 3.7
| |
| | style="background: #eff;" | 4.2
| |
| | style="background: #eff;" | 3.70
| |
| | style="background: #eff;" | 3.40
| |
| | style="background: #eff;" | 2.71
| |
| | style="background: #eff;" | 1.7
| |
| | style="background: #eff;" | 3.40
| |
| | style="background: #eff;" | 1.58
| |
| |}
| |
|
| |
|
| == See also ==
| | Hvis du har specifikke krav eller har brug for yderligere hjælp, kan du kontakte Student Rådgivningscenter for at tale med et hus rådgiver. Vi tilbyder også en servicekontrakt kontrol, hvor vi kan se over en kontrakt, så tjek det er fair og hjælpe dig med at få mening ud af alle de juridiske vilkår og betingelser. <br><br>Nyd vores Anchorage hotel værelse indkvartering og mange hotel bekvemmeligheder, som du slappe af efter en lang dag med forretninger eller sightseeing. Nyd Anchorage golf, vandreture og fiskeri, herunder restauranter og shopping tæt på vores hotel. Osaka Philharmonic Orchestra var tidligere den vigtigste performer af Osaka Classic og er nu følgeskab af tre professionelle [http://michaelkorstasker.majasolsblog.dk/ Michael Kors Pung] orkestre er baseret i Osaka og Soai Gakuen Orchestra dette år for flere forestillinger end sidste år og større berigelse. Casual programmer invitere folk, der ikke er meget fortrolig med klassisk musik. <br><br>Programmer er vokset i popularitet Stateside over de seneste fem år. Dette format er bedst egnet til dem, der ønsker at fortsætte arbejdet i samme branche, men vil gerne uddybe deres viden og færdigheder på bestemte områder for at flytte [http://vibramsko.majasolsblog.dk/ Vibram Fivefingers Kso] ind i en højere position. <br><br>På den anden side, hvis du er en udholdenhed atlet eller highvolume fyr, vil du drage fordel af at arbejde på din styrke og løfte tunge vægte. Du bør virkelig fokusere på at forsøge at [http://mbtsko.majasolsblog.dk/ Mbt Sko Udsalg] få hele pakken: fleksibilitet, styrke og udholdenhed.. For at få et pålideligt resultat, bedes du svare på alle spørgsmålene. Når du er færdig med at besvare, skal du trykke på kernen It!? Knappen nederst på skærmen. <br><br>Salinas Personlig træning, Fitness Boot Camps Corporate Wellness. Personlig træner uddannelsesmæssige workshops, seminarer og informationsmøder ProductsAbout UsMeet Vores StaffWolf Fitness Systems tilbyder lokale uddannelse i Salinas Valley i Californien og et stigende antal online ressourcer, der støtter folk fitness verdensplan. <br><br>Kendskab mindst én eller nogle få af de kendte sprog som fransk kan hjælpe dig være parat til [http://vibramsko.majasolsblog.dk/ Vibram Sko] at håndtere mennesker. Også, kan du få bedre kant fra andre, når det kommer til at fungere, hvis du ved, hvordan man taler fremmedsprog.. For eksempel billetter til Sunderland væk armaturet vil i første omgang være begrænset til tilhængere, der har 100 eller flere væk loyalitetspoint. Afhængigt af hvordan billetter sælge det antal væk loyalitetspoint pligt til at købe en billet vil blive reduceret, indtil et sådant tidspunkt, at enten alle billetter er solgt eller billetter stadig på hvilket tidspunkt alle sæsonkort indehavere kan købe..<ul> |
| {{Wikipedia books|Solar System}}
| | |
| {{-}}
| | <li>[http://nymcnj.org/blog/2011/06/trials-or-sin-pile/#comments http://nymcnj.org/blog/2011/06/trials-or-sin-pile/#comments]</li> |
| | | |
| *[[Methone (moon)]]
| | <li>[http://www.qymsw.cn/bbs/forum.php?mod=viewthread&tid=43086&fromuid=3642 http://www.qymsw.cn/bbs/forum.php?mod=viewthread&tid=43086&fromuid=3642]</li> |
| | | |
| == Notes ==
| | <li>[http://enseignement-lsf.com/spip.php?article64#forum24844358 http://enseignement-lsf.com/spip.php?article64#forum24844358]</li> |
| <div class="references-small"> | | |
| | | <li>[http://ciarcr.org/spip.php?article310/ http://ciarcr.org/spip.php?article310/]</li> |
| === Unless otherwise cited:{{ref label|AC|ac|none}} ===
| | |
| | | <li>[http://www.snesup-paris13.org/spip.php?article16/ http://www.snesup-paris13.org/spip.php?article16/]</li> |
| <ol type="a"> | | |
| <li value="15">{{note label|O|o|none}} The planetary discriminant for the planets is taken from material published by Stephen Soter.<ref>{{cite journal|title=What is a Planet?|author=Stephen Soter|date=2006-08-16|journal=The Astronomical Journal|volume=132|issue=6|pages=2513–2519|arxiv=astro-ph/0608359|doi=10.1086/508861|bibcode=2006AJ....132.2513S}}</ref> Planetary discriminants for Ceres, Pluto and Eris taken from Soter, 2006. Planetary discriminants of all other bodies calculated from the Kuiper belt mass estimate given by Lorenzo Iorio.<ref>{{cite journal|title=Dynamical determination of the mass of the Kuiper Belt from motions of the inner planets of the Solar system|author=Lorenzo Iorio|journal=Monthly Notices of the Royal Astronomical Society|volume=375|issue=4|pages=1311–1314|bibcode=2007MNRAS.tmp...24I|date=March 2007|doi=10.1111/j.1365-2966.2006.11384.x}}</ref>
| | </ul> |
| <li value="16">{{note label|P|p|none}}Saturn satellite info taken from NASA Saturnian Satellite Fact Sheet.<ref name=Saturn>[http://nssdc.gsfc.nasa.gov/planetary/factsheet/saturniansatfact.html NASA Saturnian Satellite Fact Sheet] ''NASA'' Retrieved on 2008-11-17</ref> | |
| <li value="17">{{note label|Q|q|none}}Astronomical symbols for all listed objects except Ceres taken from NASA Solar System Exploration.<ref>{{cite web|url=http://solarsystem.nasa.gov/multimedia/display.cfm?IM_ID=167|title=NASA Solar System Exploration: Planet Symbols|publisher=NASA|accessdate=2009-01-26}}</ref> Symbol for Ceres was taken from material published by James L. Hilton.<ref>{{cite web | author=James L. Hilton | title=When did asteroids become minor planets? | work=U.S. Naval Observatory | url=http://sd-www.jhuapl.edu/weaver_projects/GPD/Contributed_Talks/hilton_gpd_poster.pdf |format=PDF| accessdate=2008-10-25}}</ref> The Moon is the only natural satellite with an astronomical symbol, and Pluto and Ceres the only dwarf planets. | |
| <li value="18">{{note label|R|r|none}}Uranus satellite info taken from NASA Uranian Satellite Fact Sheet.<ref>{{cite web|url=http://nssdc.gsfc.nasa.gov/planetary/factsheet/uraniansatfact.html|title=NASA Uranian Satellite Fact Sheet|publisher=NASA|accessdate=2008-11-17}}</ref>
| |
| <li value="19">{{note label|S|s|none}}Radii for plutoid candidates taken from material published by John Stansberry et al.<ref name="Stansberry 2007"/>
| |
| <li value="21">{{note label|U|u|none}}Axial tilts for most satellites assumed to be zero in accordance with the Explanatory Supplement to the Astronomical Almanac: "In the absence of other information, the axis of rotation is assumed to be normal to the mean orbital plane."<ref>{{cite book|title=Explanatory Supplement to the Astronomical Almanac|editor=P. Kenneth Seidelmann|publisher=University Science Books|year=1992|page=384}}</ref> | |
| <li value="22">{{note label|V|v|none}}Natural satellite numbers taken from material published by Scott S. Sheppard.<ref>{{cite web |title=The Jupiter Satellite Page |author=Scott S. Sheppard |work=Carnegie Institution for Science, Department of Terrestrial Magnetism |url=http://www.dtm.ciw.edu/users/sheppard/satellites |accessdate=2008-04-02}}</ref>
| |
| </li>
| |
| </ol>
| |
| | |
| === Manual calculations (unless otherwise cited) === | |
| | |
| <ol type="a">
| |
| <li value="1">{{note label|A|a|none}} Surface area ''A'' derived from the radius using <math>\begin{smallmatrix}A=4\pi r^2 \end{smallmatrix}</math>, assuming sphericity.
| |
| <li value="2">{{note label|B|b|none}} Volume ''V'' derived from the radius using <math>\begin{smallmatrix}V=\frac{4}{3}\pi r^3 \end{smallmatrix}</math>, assuming sphericity.
| |
| <li value="3">{{note label|C|c|none}} Density derived from the mass divided by the volume.
| |
| <li value="4">{{note label|D|d|none}} Surface gravity derived from the mass ''m'', the [[gravitational constant]] ''G'' and the radius ''r'': ''G*m/r<sup>2</sup> ''. | |
| <li value="5">{{note label|E|e|none}} Escape velocity derived from the mass ''m'', the [[gravitational constant]] ''G'' and the radius ''r'': ''sqrt((2*G*m)/r).
| |
| <li value="14">{{note label|N|n|none}} Orbital speed is calculated using the mean orbital radius and the orbital period, assuming a circular orbit.
| |
| <li value="20">{{note label|T|t|none}} Assuming Pluto's density of 2.0
| |
| <li value="23">{{note label|W|w|none}} Calculated using the formula <math>\begin{smallmatrix}T\ =\ \frac{T_{\textrm{eff}}(1-qp_{\nu})^{1/4}}{\sqrt{2}}\sqrt{52/r},\end{smallmatrix}</math> where T<sub>eff</sub> =54.8 K at 52 AU, <math>p_{\nu}</math> is the geometric albedo, ''q''=0.8 is the [[phase integral]], and <math>r</math> is the distance from the Sun in AU. This formula is a simplified version of that in section 2.2 of Stansberry, ''et al.'', 2007,<ref name="Stansberry 2007"/> where emissivity and beaming parameter were assumed equal unity, and <math>\pi</math> was replaced with 4 accounting for the difference between circle and sphere. All parameters mentioned above were taken from the same paper.
| |
| <li value="27">{{note label|AA|aa|none}}Calculated using the formula <math>\begin{smallmatrix}D=\frac{1329}{\sqrt{p}}10^{-0.2H}\end{smallmatrix}</math>, where H is the absolute magnitude, p is the geometric albedo and D is the diameter in km, and assuming an albedo of 0.15, as per Dan Bruton.<ref>{{cite web |title=Conversion of Absolute Magnitude to Diameter for Minor Planets |publisher=Department of Physics & Astronomy (Stephen F. Austin State University) |author=Dan Bruton |url=http://www.physics.sfasu.edu/astro/asteroids/sizemagnitude.html |accessdate=2009-01-20}}</ref> | |
| <li value="30">{{note label|AD|ad|none}} Mass derived from the density multipied by the volume.
| |
| </li> | |
| </ol>
| |
| | |
| === Individual calculations ===
| |
| | |
| <ol type="a">
| |
| <li value="25">{{note label|Y|y|none}}Derived from density
| |
| <li value="26">{{note label|Z|z|none}} Surface area was calculated using the formula for a scalene [[ellipsoid]]: | |
| :<math>\begin{smallmatrix}2\pi\left(c^2+b\sqrt{a^2-c^2}E(\alpha,m)+\frac{bc^2}{\sqrt{a^2-c^2}}F(\alpha,m)\right),\,\!\end{smallmatrix}</math> where <math>\begin{smallmatrix}\alpha=\arccos\left(\frac{c}{a}\right)\,\,\!\end{smallmatrix}</math> is the modular angle, or '''[[angular eccentricity]]'''; <math>\begin{smallmatrix}m=\frac{b^2-c^2}{b^2\sin(\alpha)^2}\,\!\end{smallmatrix}</math> and <math>\begin{smallmatrix}F(\alpha,m)\,\!\end{smallmatrix}</math>, <math>\begin{smallmatrix}E(\alpha,m)\,\!\end{smallmatrix}</math> are the incomplete [[elliptic integral]]s of the first and second kind, respectively. The values 980 km, 759 km, and 498 km were used for a, b, and c respectively.
| |
| </li>
| |
| </ol>
| |
| | |
| === Other notes ===
| |
| | |
| <ol type="a">
| |
| <li value="6">{{note label|F|f|none}} Relative to Earth
| |
| <li value="7">{{note label|G|g|none}} [[Orbital period|sidereal]]
| |
| <li value="8">{{note label|H|h|none}} [[Retrograde motion|retrograde]] | |
| <li value="9">{{note label|I|i|none}} The inclination of the body's [[equator]] from its [[orbit]].
| |
| <li value="10">{{note label|J|j|none}} At pressure of 1 bar
| |
| <li value="11">{{note label|K|k|none}} At sea level
| |
| <li value="12">{{note label|L|l|none}} The ratio between the mass of the object and those in its immediate neighborhood. Used to distinguish between a planet and a dwarf planet.
| |
| <li value="13">{{note label|M|m|none}} This object's rotation is synchronous with its orbital period, meaning that it only ever shows one face to its primary.
| |
| <li value="24">{{note label|X|x|none}} Objects' planetary discriminants based on their similar orbits to Eris. Sedna's population is currently too little-known for a planetary discriminant to be determined.
| |
| <li value="28">{{note label|AB|ab|none}}Proteus average diameter: 210 km;<ref name=nep/> Mimas average diameter: 199 km<ref name=Saturn/>
| |
| <li value="29">{{note label|AC|ac|none}} "Unless otherwise cited" means that the information contained in the citation is applicable to an entire line or column of a chart, unless another citation specifically notes otherwise.
| |
| </div> | |
| | |
| == References ==
| |
| {{reflist|2}}
| |
| | |
| {{Solar System}}
| |
| | |
| {{Featured list}}
| |
| | |
| [[Category:Lists of Solar System objects|Hydrostatic equilibrium]]
| |
| [[Category:Planemos|*]]
| |
| | |
| {{Link FL|ja}}
| |
| {{Link FL|ru}}
| |