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{{Sky|11|33|25.4408|-|70|11|41.239|1000000000}}
This is a preview for the new '''MathML rendering mode''' (with SVG fallback), which is availble in production for registered users.
{{Starbox begin
| name = HD 100546
}}
{{Starbox observe
| epoch = [[J2000.0]]<ref name=SIMBAD/>
| constell = [[Musca]]
| ra = {{RA|11|33|25.4408}}<ref name=SIMBAD>{{Cite web | title = SIMBAD Object query: HD 100546 | url = http://simbad.u-strasbg.fr/simbad/sim-id?protocol=html&Ident=HD+100546}}</ref>
| dec = {{DEC|-70|11|41.239}}<ref name=SIMBAD/>
| appmag_v = 6.698<ref name=SIMBAD/>
}}
{{Starbox character
| class = B9Vne<ref name=SIMBAD/>
}}
{{Starbox detail
| age = >10<sup>6</sup><ref name=herbig/>
| luminosity =
}}
{{Starbox astrometry
| prop_mo_ra = -38.78<ref name=SIMBAD/>
| prop_mo_dec = -0.05<ref name=SIMBAD/>
| parallax = 9.67<ref name=SIMBAD/>
| p_error = 0.60<ref name=SIMBAD/>
| dist_ly = 337.3<ref name=EPO>{{cite web | title = The Extrasolar Planets Encyclopaedia | url = http://exoplanet.eu/star.php?st=HD+100546}}</ref>
| dist_pc = 103.4<ref name=EPO/>
| absmag_v =
}}
{{Starbox catalog
| names = V* KR Mus, SAO 251457, CD-69 893, [[Hipparcos catalogue|HIP]] 56379, [[Henry Draper catalogue|HD]] 100546.<ref name=SIMBAD/>
}}
{{Starbox end}}


{{Planetbox begin
If you would like use the '''MathML''' rendering mode, you need a wikipedia user account that can be registered here [[https://en.wikipedia.org/wiki/Special:UserLogin/signup]]
| name = HD 100546 B
* Only registered users will be able to execute this rendering mode.
}}|
* Note: you need not enter a email address (nor any other private information). Please do not use a password that you use elsewhere.
{{Planetbox star
| star = HD 100546
| RA =  {{RA|11|33|25.4408}}<ref name=SIMBAD/>
| DEC =  {{DEC|-70|11|41.239}}<ref name=SIMBAD/>
| class = B9Vne<ref name=SIMBAD/>
}}
{{Planetbox character
| mass = ~20<ref name=planet-1/>
}}
{{Planetbox orbit
| semimajor = 6.5<ref name=planet-1/>
}}
{{Planetbox end}}


'''HD 100546''' is a star 337.3 [[Light year|LY]] from [[Earth]]. It is orbited by an approximately 20 [[Jupiter|M<sub>j</sub>]] [[planet]] at 6.5 [[Astronomical unit|AU]].<ref name=planet-1>{{Cite journal | title = Resolving the disk rotation of HD 97048 and HD 100546 in the <nowiki>[O I]</nowiki> 6300A line: evidence for a giant planet orbiting HD 100546 | last = Acke | first = B. | coauthors = van der Ancker; M. | journal = Astronomy and Astrophysics | date = November 2005 | volume = 449 | issue = 267 | arxiv = astro-ph/0512562|doi = 10.1051/0004-6361:20054330 | bibcode=2006A&A...449..267A | pages = 267}}</ref>
Registered users will be able to choose between the following three rendering modes:  


==HD 100546 B==
'''MathML'''
Evidence for a planetary companion to HD 100546 was gathered using the UVES [[Echelle grating|echelle spectrograph]] at the [[Very Large Telescope|VLT]] in [[Chile]].<ref name=planet-1/> This confirms other data indicating a planetary companion.  The planet's size puts it near the border between a giant planet and a [[brown dwarf]].<ref name=planet-1/>
:<math forcemathmode="mathml">E=mc^2</math>


==Protoplanetary material==
<!--'''PNG'''  (currently default in production)
Spectroscopic analysis of mid-IR data taken from OSCIR on the 4 m [[Victor M. Blanco Telescope|Blanco Telescope]] at [[Cerro Tololo Inter-American Observatory]] indicates the presence of a small particles (10 - 18 <math>\mu  m</math>) containing [[silicates]].<ref name=herbig>{{Cite journal | title = The Disk and Environment of the Herbig Be Star HD 100546 | first = C. A. | last = Grady | date = December 2001 | journal = The Astronomical Journal | volume = 122 | issue = 6 | pages = 3396–3406 | doi = 10.1086/324447 | url = http://www.iop.org/EJ/article/1538-3881/122/6/3396/201085.html | last2 = Polomski | first2 = E. F. | last3 = Henning | first3 = Th. | last4 = Stecklum | first4 = B. | last5 = Woodgate | first5 = B. E. | last6 = Telesco | first6 = C. M. | last7 = Piña | first7 = R. K. | last8 = Gull | first8 = T. R. | last9 = Boggess | first9 = A. | bibcode=2001AJ....122.3396G}}</ref>  The material is found at distances out to 17 [[Astronomical unit|AU]] away from the star and has a temperature of approximately 227 [[Kelvin|K]].<ref name=herbig/>
:<math forcemathmode="png">E=mc^2</math>


==References==
'''source'''
{{Reflist}}
:<math forcemathmode="source">E=mc^2</math> -->


==Further reading==
<span style="color: red">Follow this [https://en.wikipedia.org/wiki/Special:Preferences#mw-prefsection-rendering link] to change your Math rendering settings.</span> You can also add a [https://en.wikipedia.org/wiki/Special:Preferences#mw-prefsection-rendering-skin Custom CSS] to force the MathML/SVG rendering or select different font families. See [https://www.mediawiki.org/wiki/Extension:Math#CSS_for_the_MathML_with_SVG_fallback_mode these examples].
*{{Cite journal | title = Catalog of Nearby Exoplanets | last = Butler | first = P. | coauthors = Wright, J.; Marcy, G.; Fischer, D.; Vogt, S.; Tinney, Ch.; Jones, H.; Carter, B.; Penny, A | journal = The Astrophysical Journal | volume = 646 | issue = 505 | pages = 505–522 | date = March 2006 | arxiv = astro-ph/0607493 | doi = 10.1086/504701 | bibcode=2006ApJ...646..505B}}


*{{Cite journal | title = Kinematics of planet-host stars and their relation to dynamical streams in the solar neighbourhood | last = Ecuvillon | first = A. | coauthors = Israelian, G.; Pont, F.; Santos, N.; Mayor, M. | journal = Astronomy and Astrophysics | date = August 2006 | volume = 461 | issue = 171 | arxiv = astro-ph/0608669|doi = 10.1051/0004-6361:20065872 | pages = 171–182 | bibcode=2007A&A...461..171E}}
==Demos==


*{{Cite journal | title = Habitability of known exoplanetary systems based on measured stellar properties | last = Jones | first = B. | coauthors = Sleep, P.; Underwood, D. | journal = The Astrophysical Journal | date = June 2006 | volume = 649 | issue = 1010 | arxiv = astro-ph/0603200|bibcode = 2006ApJ...649.1010J |doi = 10.1086/506557 | pages = 1010–1019 }}
Here are some [https://commons.wikimedia.org/w/index.php?title=Special:ListFiles/Frederic.wang demos]:


*{{Cite journal | title = Formation of Earth-like Planets During and After Giant Planet Migration | last = Mandell, A.; Raymond, S.; Sigurdsson, S | date = | journal = The Astrophysical Journal | volume = 660 | issue =  | arxiv = astro-ph/0701048 |bibcode =  2007ApJ...660..823M|doi = 10.1086/512759 | first1 = Avi M. | last2 = Raymond | first2 = Sean N. | last3 = Sigurdsson | first3 = Steinn | pages = 823–844 }}


*{{Cite journal | title = Extrasolar planet taxonomy: a new statistical approach | last = Marchi | first = S. | date = May 2007 | journal = The Astrophysical Journal | volume = 666 | issue =  | arxiv = 0705.0910|bibcode = 2007ApJ...666..475M |doi = 10.1086/519760 | pages = 475–485 }}
* accessibility:
** Safari + VoiceOver: [https://commons.wikimedia.org/wiki/File:VoiceOver-Mac-Safari.ogv video only], [[File:Voiceover-mathml-example-1.wav|thumb|Voiceover-mathml-example-1]], [[File:Voiceover-mathml-example-2.wav|thumb|Voiceover-mathml-example-2]], [[File:Voiceover-mathml-example-3.wav|thumb|Voiceover-mathml-example-3]], [[File:Voiceover-mathml-example-4.wav|thumb|Voiceover-mathml-example-4]], [[File:Voiceover-mathml-example-5.wav|thumb|Voiceover-mathml-example-5]], [[File:Voiceover-mathml-example-6.wav|thumb|Voiceover-mathml-example-6]], [[File:Voiceover-mathml-example-7.wav|thumb|Voiceover-mathml-example-7]]
** [https://commons.wikimedia.org/wiki/File:MathPlayer-Audio-Windows7-InternetExplorer.ogg Internet Explorer + MathPlayer (audio)]
** [https://commons.wikimedia.org/wiki/File:MathPlayer-SynchronizedHighlighting-WIndows7-InternetExplorer.png Internet Explorer + MathPlayer (synchronized highlighting)]
** [https://commons.wikimedia.org/wiki/File:MathPlayer-Braille-Windows7-InternetExplorer.png Internet Explorer + MathPlayer (braille)]
** NVDA+MathPlayer: [[File:Nvda-mathml-example-1.wav|thumb|Nvda-mathml-example-1]], [[File:Nvda-mathml-example-2.wav|thumb|Nvda-mathml-example-2]], [[File:Nvda-mathml-example-3.wav|thumb|Nvda-mathml-example-3]], [[File:Nvda-mathml-example-4.wav|thumb|Nvda-mathml-example-4]], [[File:Nvda-mathml-example-5.wav|thumb|Nvda-mathml-example-5]], [[File:Nvda-mathml-example-6.wav|thumb|Nvda-mathml-example-6]], [[File:Nvda-mathml-example-7.wav|thumb|Nvda-mathml-example-7]].
** Orca: There is ongoing work, but no support at all at the moment [[File:Orca-mathml-example-1.wav|thumb|Orca-mathml-example-1]], [[File:Orca-mathml-example-2.wav|thumb|Orca-mathml-example-2]], [[File:Orca-mathml-example-3.wav|thumb|Orca-mathml-example-3]], [[File:Orca-mathml-example-4.wav|thumb|Orca-mathml-example-4]], [[File:Orca-mathml-example-5.wav|thumb|Orca-mathml-example-5]], [[File:Orca-mathml-example-6.wav|thumb|Orca-mathml-example-6]], [[File:Orca-mathml-example-7.wav|thumb|Orca-mathml-example-7]].
** From our testing, ChromeVox and JAWS are not able to read the formulas generated by the MathML mode.


*{{Cite journal | title = The Geneva-Copenhagen survey of the Solar neighbourhood. Ages, metallicities, and kinematic properties of ~14000 F and G dwarfs | last = Nortdstrom, R.; Mayor, M.; Andersen, J.; Holmberg, J; Pont, F.; Jorgenson, B.; Olsen, E.; Udry, S.; Mowlavi, N | journal = Astronomy and Astrophysics | volume = 418 | issue = 989 | arxiv = astro-ph/0405198|bibcode = 2004A&A...418..989N |doi = 10.1051/0004-6361:20035959 | year = 2004  | pages = 989–1019 | first1 = B. | last2 = Mayor | first2 = M. | last3 = Andersen | first3 = J. | last4 = Holmberg | first4 = J. | last5 = Pont | first5 = F. | last6 = j�Rgensen | first6 = B. R. | last7 = Olsen | first7 = E. H. | last8 = Udry | first8 = S. | last9 = Mowlavi | first9 = N. }}
==Test pages ==


*{{Cite journal | title = The Circumstellar Dust Disk of HD 100546 | last = Hedrick | first = C. H. | coauthors =  Doering, R.; Lee, K.-G.; Sosey, M.; Meixner, M.; Ardila, D. | journal = American Astronomical Society | date = January 2006 | volume = 37 | issue = 4 | url = http://www.aas.org/publications/baas/v37n4/aas207/1013.htm}}
To test the '''MathML''', '''PNG''', and '''source''' rendering modes, please go to one of the following test pages:
*[[Displaystyle]]
*[[MathAxisAlignment]]
*[[Styling]]
*[[Linebreaking]]
*[[Unique Ids]]
*[[Help:Formula]]


==External links==
*[[Inputtypes|Inputtypes (private Wikis only)]]
*[http://zuserver2.star.ucl.ac.uk/~apod/apod/ap010502.html Astronomy picture of the day] - May 2, 2001
*[[Url2Image|Url2Image (private Wikis only)]]
 
==Bug reporting==
[[Category:Extrasolar planets]]
If you find any bugs, please report them at [https://bugzilla.wikimedia.org/enter_bug.cgi?product=MediaWiki%20extensions&component=Math&version=master&short_desc=Math-preview%20rendering%20problem Bugzilla], or write an email to math_bugs (at) ckurs (dot) de .
 
 
{{star-stub}}
{{extrasolar-planet-stub}}
 
[[fa:اچ‌دی ۱۰۰۵۴۶]]
[[ru:HD 100546]]

Latest revision as of 22:52, 15 September 2019

This is a preview for the new MathML rendering mode (with SVG fallback), which is availble in production for registered users.

If you would like use the MathML rendering mode, you need a wikipedia user account that can be registered here [[1]]

  • Only registered users will be able to execute this rendering mode.
  • Note: you need not enter a email address (nor any other private information). Please do not use a password that you use elsewhere.

Registered users will be able to choose between the following three rendering modes:

MathML

E=mc2


Follow this link to change your Math rendering settings. You can also add a Custom CSS to force the MathML/SVG rendering or select different font families. See these examples.

Demos

Here are some demos:


Test pages

To test the MathML, PNG, and source rendering modes, please go to one of the following test pages:

Bug reporting

If you find any bugs, please report them at Bugzilla, or write an email to math_bugs (at) ckurs (dot) de .

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