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ดาวศุกร์

File:Venusian_magnetosphere.svg · Wikimedia Commons · See Wikimedia Commons

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ดาวศุกร์

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Also known as , Planet Venus

ดาวเคราะห์ลำดับที่ 2 ในระบบสุริยะ

OverviewAI-generated

Venus is an inner and inferior planet of the Solar System that orbits the Sun. It possesses an atmosphere and is characterized by its orbit and the potential for life on its surface. The planet has a radius of 6051.8 and a mass of 4867.5. Its highest point is Skadi Mons.

Venus has an orbital eccentricity of 0.0068 and a flattening of 0. The semi-major axis of its orbit is 108208930, with an orbital inclination of 3.39471. The argument of periapsis is 131.60246718, and the longitude of the ascending node is 76.67984255. Its orbital period is 19414148, and its synodic period is 583.92. The albedo is 0.689.

The demonym for Venus is Venusian, Venerian, Venusano, or Vénusien. It is described by sources including the Brockhaus and Efron Encyclopedic Dictionary, Gujin Tushu Jicheng, The Nuttall Encyclopædia, and the Encyclopædia Britannica 11th edition. The topic is listed in the Wikipedia:List of articles all languages should have and Wikipedia:Vital articles/Level/4.

Synthesized by Vinony from 29 facts across 4 sources: Wikidata, Firecrawl, PubMed, Vinony graph. Generated from structured data (not the Wikipedia text) and checked against those facts — may still contain errors.

Key facts

Planet.name
Venus
Planet.image
Venus 2 Approach Image.jpg
Planet.symbol
24px|♀|class=skin-invert
Planet.caption
Image of Venus, as captured by MESSENGER. In natural color Venus is a featureless sphere. A cloud layer permanently obscures the surface.
Planet.background
LightSalmon
Planet.epoch
J2000
Planet.eccentricity
0.006772
Planet.synodic_period
583.92 days
Planet.avg_speed
35.02km/s
Planet.asc_node
76.680°
Planet.arg_peri
54.884°
Planet.mean_anomaly
50.115°
Planet.satellites
None
Planet.allsatellites
yes
Planet.flattening
0
Planet.rotation
(retrograde) 1 Venus solar day
Planet.sidereal_day
(retrograde)
Planet.axial_tilt
2.64° (for retrograde rotation)177.36° (to orbit)

via Wikipedia infobox

Research

4,214 papers

via PubMed

Described at

Why is Venus so bright? | Live Science

livescience.com

Link to a page describing this subject · 1,025 chars · not written by Vinony

Wikidata facts

Instance of
inferior planet
Named after
Venus
Demonym
Venusano
Area
460230000
Highest point
Skadi Mons
Parent body
Sun
Child body
Neith
Distance from Earth
108000000
Diameter
12103.6
Radius
6051.8
Mass
4867.5
Orbital period
19414148
Image
PIA23791-Venus-RealAndEnhancedContrastViews-20200608 (cropped).jpg
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Commons category
Venus (planet)
topic's main category
Category:Venus
Commons gallery
Venus
orbital eccentricity
0.0068
flattening
0
semi-major axis of an orbit
0.723332
orbital inclination
2.19
argument of periapsis
131.60246718
longitude of ascending node
76.67984255
albedo
0.59
synodic period
583.92
on focus list of Wikimedia project
Wikipedia:Vital articles/Level/4
has characteristic
life on Venus
periapsis
107476259
apoapsis
108942109
apparent magnitude
-4.8
epoch
J2000.0
surface gravity
8.9
density
5.243
mean anomaly
50.115
volume as quantity
928430000000
temperature
474
angular diameter
66
right ascension
272.76
declination
67.16
different from
Venus
Unicode character
notation
Venus symbol
topic has template
Template:GeoTemplate/venus
IPA transcription
ˈveːnʊs
rotation period
-5832.5
effective temperature
226.6
Sources (9)

via Wikidata · CC0

Gallery (52)

Available in 255 languages

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via Wikidata sitelinks · CC0