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[[he:נוגה]]
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[[hi:शुक्र]]
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[[hr:Venera (planet)]]
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[[ht:Venis (planèt)]]
[[ht:Venis (planèt)]]

Àtúnyẹ̀wò ní 12:00, 23 Oṣù Kẹta 2011

Venus  Venus's symbol, a circle with a small equal-armed cross beneath it
Venus in real color, a nearly uniform pale cream. The planet's disk is about three-quarters illuminated. Almost no variation or detail can be seen in the clouds.
Venus in real color
Ìfúnlọ́rúkọ
Ìpolongo /ˈviːnəs/  ( listen)
Alápèjúwe Venusian or (rarely) Cytherean, Venerean
Àsìkò J2000
Aphelion108,942,109 km
0.728 231 28 AU
Perihelion 107,476,259 km
0.718 432 70 AU
Semi-major axis 108,208,930 km
0.723 332 AU
Eccentricity 0.006 8
Àsìkò ìgbàyípo 224.700 69 day
0.615 197 0 yr
1.92 Venus solar day
Synodic period 583.92 days
Average orbital speed 35.02 km/s
Inclination 3.394 71° to Ecliptic
3.86° to Sun’s equator
2.19° to Invariable plane[1]
Longitude of ascending node 76.670 69°
Argument of perihelion 54.852 29°
Satellites None
Àwọn ìhùwà àdánidá
Iyeìdáméjì ìfẹ̀kiri 6,051.8 ± 1.0 km[2]
0.949 9 Earths
Flattening 0[2]
Ààlà ojúde 4.60 × 108 km²
0.902 Earths
Ìpọ̀sí 9.38 × 1011 km³
0.857 Earths
Àkójọ 4.868 5 × 1024 kg
0.815 Earths
Iyeìdáméjì ìṣùpọ̀ 5.204 g/cm³
Equatorial surface gravity8.87 m/s2
0.904 g
Escape velocity10.46 km/s
Sidereal rotation
period
-243.018 5 day
Equatorial rotation velocity 6.52 km/h (1.81 m/s)
Axial tilt 177.3°
North pole right ascension 18 h 11 min 2 s
272.76°[3]
North pole declination 67.16°
Albedo0.65 (geometric) or 0.75 (bond)
Ìgbónásí ojúde
   Kelvin
   Celsius
minmeanmax
735 K "Venus: Facts & Figures". NASA. Retrieved 2007-04-12. </ref>[4]
461.85 °C
Apparent magnitude up to -4.6 (crescent)
-3.8 (full)
Angular diameter 9.7" – 66.0"
Afẹ́fẹ́àyíká
Ìfúnpá ojúde 93 bar (9.3 MPa)
Ìkósínú ~96.5% Carbon dioxide
~3.5% Nitrogen
0.015% Sulfur dioxide
0.007% Argon
0.002% Water vapor
0.001 7% Carbon monoxide
0.001 2% Helium
0.000 7% Neon
trace Carbonyl sulfide
trace Hydrogen chloride
trace Hydrogen fluoride

Aguala je planeti.



Itokasi

  1. "The MeanPlane (Invariable plane) of the Solar System passing through the barycenter". 2009-04-03. Retrieved 2009-04-10.  (produced with Solex 10 written by Aldo Vitagliano; see also Invariable plane)
  2. 2.0 2.1 Seidelmann, P. Kenneth; Archinal, B. A.; A’hearn, M. F.; et al. (2007). "Report of the IAU/IAGWorking Group on cartographic coordinates and rotational elements: 2006". Celestial Mechanics and Dynamical Astronomy 90: 155–180. doi:10.1007/s10569-007-9072-y. http://adsabs.harvard.edu/doi/10.1007/s10569-007-9072-y. Retrieved 2007-08-28. 
  3. "Report on the IAU/IAG Working Group on cartographic coordinates and rotational elements of the planets and satellites". International Astronomical Union. 2000. Retrieved 2007-04-12. 
  4. "Space Topics: Compare the Planets: Mercury, Venus, Earth, The Moon, and Mars". Planetary Society. Retrieved 2007-04-12.