Double coset
<imagemap> Image:Scale one to thousand spheres no labels.svg|right|Click on the small very purple bottom-left sphere for volumes smaller than 1 E+30 m³, on the next larger sphere for 1 E+31 m³ to 1 E+32 m³, the next larger sphere for 1 E+32 m³ to 1 E+33 m³ units, and the largest sphere for 1 E+33 m³ to 1 E+34 m³ poly 0 230 28 230 28 198 0 198 smaller than 1 E+30 m³ poly 0 216 56 216 56 172 0 172 1 E+30 m³ to 1 E+31 m³ poly 20 214 106 214 106 124 20 124 1 E+31 m³ to 1 E+32 m³ poly 32 201 220 201 220 14 32 14 1 E+32 m³ to 1 E+33 m³ default Click here for volumes 1 E+33 m³ and larger, or click on one of the spheres for the desired volume desc top-left </imagemap>
To help compare different orders of magnitudes this page lists volumes between one thousand cubic gigametres and ten thousand cubic terametres ( to cubic metres). See also volumes or capacities of other orders of magnitude.
- Volumes smaller than 1 nonillion (a million5) cubic metres
- Volume of Alcyone, brightest star in the Pleiades = ~1Template:E m³[1]
- Volume of Arcturus, brightest star in Boötes = ~1.7Template:E m³[2]
1 E+33 m³ and larger
<imagemap> Image:Scale one to thousand spheres no labels.svg|right|Click on the small very purple bottom-left sphere for volumes smaller than 1 E+33 m³, on the next larger sphere for 1 E+34 m³ to 1 E+35 m³, the next larger sphere for 1 E+35 m³ to 1 E+36 m³ units, and the largest sphere for 1 E+36 m³ to 1 E+37 m³ poly 0 230 28 230 28 198 0 198 smaller than 1 E+33 m³ poly 0 216 56 216 56 172 0 172 1 E+33 m³ to 1 E+31 m³ poly 20 214 106 214 106 124 20 124 1 E+34 m³ to 1 E+35 m³ poly 32 201 220 201 220 14 32 14 1 E+35 m³ to 1 E+36 m³ default Click here for volumes 1 E+36 m³ and larger, or click on one of the spheres for the desired volume desc top-left </imagemap>
- ~1 * 1034 m³ = volume of Deneb, a white supergiant in Cygnus[5]
- 6.4 * 1034 m³ = volume of η Carinae, a white supergiant in Cygnus[6]
- 1.3Template:E m³ = estimated volume of S Orionis[7]
- 1.5Template:E m³ = volume of Antares, a Mira variable in Orion[8]
1 E+36 m³ and larger
<imagemap> Image:Scale one to thousand spheres no labels.svg|right|Click on the small very purple bottom-left sphere for volumes smaller than 1 E+36 m³, on the next larger sphere for 1 E+37 m³ to 1 E+38 m³, the next larger sphere for 1 E+38 m³ to 1 E+39 m³ units, and the largest sphere for 1 E+39 m³ to 1 E+40 m³ poly 0 230 28 230 28 198 0 198 smaller than 1 E+36 m³ poly 0 216 56 216 56 172 0 172 1 E+36 m³ to 1 E+37 m³ poly 20 214 106 214 106 124 20 124 1 E+37 m³ to 1 E+38 m³ poly 32 201 220 201 220 14 32 14 1 E+38 m³ to 1 E+39 m³ default Click here for volumes 1 E+39 m³ and larger, or click on one of the spheres for the desired volume desc top-left </imagemap>
- 4Template:E m³ = possible volume of µ Cephei (estimates vary)
- 8Template:E m³ = estimated volume of VY Canis Majoris, a red hypergiant star[9]
- 3.9Template:E m³ = 390 undecillion m³ = volume of a sphere which would enclose the orbit of Neptune
1 E+39 m³ and larger
<imagemap> Image:Scale one to thousand spheres no labels.svg|right|Click on the small very purple bottom-left sphere for volumes smaller than 1 E+39 m³, on the next larger sphere for 1 E+40 m³ to 1 E+41 m³, the next larger sphere for 1 E+41 m³ to 1 E+42 m³ units, and the largest sphere for 1 E+42 m³ to 1 E+43 m³ poly 0 230 28 230 28 198 0 198 smaller than 1 E+39 m³ poly 0 216 56 216 56 172 0 172 1 E+39 m³ to 1 E+40 m³ poly 20 214 106 214 106 124 20 124 1 E+40 m³ to 1 E+41 m³ poly 32 201 220 201 220 14 32 14 1 E+41 m³ to 1 E+42 m³ default Click here for volumes 1 E+42 m³ and larger, or click on one of the spheres for the desired volume desc top-left </imagemap>
- 6Template:E m³ = possible volume of the Heliosphere inside the Termination shock
- Volumes larger than or equal to 10 duodecillion (ten thousand million6) cubic metres
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One other major development concerning concurrent HDB ownership concerns private property owners who are actually successfully banned from buying HDB resale flats for investment purposes. HDB has carried out a new rule requiring non-public property owners who purchase a HDB flat to dispose of their non-public property inside six months. Similarly, buyers of HDB flats who didn't obtain any subsidies may not purchase personal property throughout the minimum occupation interval (MOP), which has now been extended from three to 5 years. Other than prolonging the "upgrading" cycle, these new restrictions will considerably impression funding demand, significantly in the non-public housing sector. Extension of Holding Interval on Seller's Stamp Duty
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One factor we've got on this country is a big group of "economists," and "market analysts." What's interesting about this group of real property market-watchers is that there are two very different ways through which they predict Boomers will influence housing markets over the next decade. Let's check out those two opposites and see how each can change the way in which real property buyers method their markets. Quiet Enjoyment 19. The Landlord covenants that on paying the Hire and performing the covenants contained in this Settlement, the Tenant will peacefully and quietly have, hold, and benefit from the Property for the agreed time period. Register now for VIP preview quickly this Might and be the 1st toselect your selection unit at particular Preview Worth. No overseas income tax
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Notes
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- ↑ Kaler, Jim, Alcyone, retrieved 2008-11-18: "radius nearly 10 solar"
- ↑ Mozurkewich, David; Armstrong, J. Thomas; Hindsley, Robert B.; Quirrenbach, Andreas; Hummel, Christian A.; Hutter, Donald J.; Johnston, Kenneth J.; Hajian, Arsen R.; Elias II, Nicholas M.; Buscher, David F.; and Simon, Richard S.; Angular diameters of stars from the Mark III optical interferometer, Astronomical Journal, 126, 2502-2520 (2003)
- ↑ Its radius is 70 times the Sun's
- ↑ Its radius is 113 times the Sun's
- ↑ Its radius is estimated to be 200 to 300 times the Sun's
- ↑ Its radius is estimated to be 200 to 300 times the Sun's
- ↑ VizeR page for Antares, retrieved 2009-11-18: "5.1e+02 solRad"
- ↑ VizeR page for S Orionis, retrieved 2009-11-18: "5.3e+02 solRad"
- ↑ Humphreys, Roberta M.; VY Canis Majoris: The Astrophysical Basis of its Luminosity, arxiv.org, 13 October 2006, page 3, retrieved 2009-11-18: "1800 to 2100 R⊙"