a paragraph on venus
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Answer:
it is the second planet on our solar system. except mercury is closer to the sun it is the hottest planet . it has no moon because it is present near to the sun and is too hot. the year length of Venus is 225 earth days . it has longest rotation period
Answer:
Venus is the hottest known planet in the solar system because of its closeness to sun and many hot gases surrounding the atomospehere of Venus. Venus is the second planet from the Sun, orbiting it every 224.7 Earth days.[13] It has the longest rotation period (243 Earth days) of any planet in the Solar System and rotates in the opposite direction to most other planets (meaning the Sun rises in the west and sets in the east).[14] It does not have any natural satellites. It is named after the Roman goddess of love and beauty. It is the second-brightest natural object in the night sky after the Moon, reaching an apparent magnitude of −4.6 – bright enough to cast shadows at night and, rarely, visible to the naked eye in broad daylight.[15][16] Orbiting within Earth's orbit, Venus is an inferior planet and never appears to venture far from the Sun; its maximum angular distance from the Sun (elongation) is 47.8°.
Venus
The Venusian symbol, a circle with a small equal-armed cross beneath it
Venus in approximately true colour, a nearly uniform pale cream, although the image has been processed to bring out details.[1] The planet's disc is about three-quarters illuminated; almost no variation or detail can be seen in the clouds
A real-colour image taken by Mariner 10 processed from two filters, the surface is obscured by thick sulfuric acid clouds
Designations
Pronunciation
/ˈviːnəs/ (About this soundlisten)
Adjectives
Venusian or (rarely) Cytherean, Venerean
Orbital characteristics[3][5]
Epoch J2000
Aphelion
0.728213 AU
108,939,000 km
Perihelion
0.718440 AU
107,477,000 km
Semi-major axis
0.723332 AU
108,208,000 km
Eccentricity
0.006772[2]
Orbital period
224.701 d[3]
0.615198 yr
1.92 Venus solar day
Synodic period
583.92 days[3]
Average orbital speed
35.02 km/s
Mean anomaly
50.115°
Inclination
3.39458° to ecliptic
3.86° to Sun's equator
2.19° to invariable plane[4]
Longitude of ascending node
76.680°[2]
Argument of perihelion
54.884°
Satellites
None
Physical characteristics
Mean radius
6,051.8±1.0 km[6]
0.9499 Earths
Flattening
0[6]
Surface area
4.6023×108 km2
0.902 Earths
Volume
9.2843×1011 km3
0.866 Earths
Mass
4.8675×1024 kg[7]
0.815 Earths
Mean density
5.243 g/cm3
Surface gravity
8.87 m/s2
0.904 g
Escape velocity
10.36 km/s (6.44 mi/s)[8]
Sidereal rotation period
−243.025 d (retrograde)[3]
Equatorial rotation velocity
6.52 km/h (1.81 m/s)
Axial tilt
2.64° (for retrograde rotation)
177.36° (to orbit)[3][note 1]
North pole right ascension
18h 11m 2s
272.76°[9]
North pole declination
67.16°
Albedo
0.689 (geometric)[10]
0.76 (Bond)[11]
Surface temp. min mean max
Kelvin 737 K[3]
Celsius 462 °C
Fahrenheit 864 °F
Apparent magnitude
−4.92 to −2.98[12]
Angular diameter
9.7″–66.0″[3]
Atmosphere[3]
Surface pressure
92 bar (9.2 MPa)
91 atm
Composition by volume
96.5% carbon dioxide
3.5% nitrogen
0.015% sulfur dioxide
0.0070% argon
0.0020% water vapour
0.0017% carbon monoxide
0.0012% helium
0.0007% neon
trace carbonyl sulfide
trace hydrogen chloride
trace hydrogen fluoride
The plains of Venus are outlined in red and gold, with impact craters leaving golden rings across the surface