Difference between revisions of "Template:GeoTemplate/venus"
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== See also == | == See also == | ||
* [[commons:Category:Surface features of Venus|Surface features of Venus]] {{icon|Commons}} | * [[commons:Category:Surface features of Venus|Surface features of Venus]] {{icon|Commons}} | ||
| + | Venus has many craters and the surface temperature is over 800 degrees Fahrenheit and is unable to be inhabitable | ||
== External links == | == External links == | ||
Revision as of 19:27, 8 April 2019
| Coordinates on Venus | {latdegabs}° {latminint}′ {latsecdec}″ {latNS}, {londegabs}° {lonminint}′ {lonsecdec}″ {lonEW} ({latdegdec}°, {londegdec}°) | Type | {type} |
|---|---|---|---|
View the location above by selecting a mapping provider:
- WikiMiniAtlas Wikipedia links and Commons thumbnails on an interactive radar map
- World Wind
Longitude
Longitudes on Venus are measured eastward from its prime meridian. The original prime meridian passed through the radar-bright spot at the center of the oval feature Eve, located south of Alpha Regio.[1] After the Venera missions were completed, the prime meridian was redefined to pass through the central peak in the crater Ariadne.[2][3]
- ↑ Davies, M.E.; et al. (1994), "Report of the IAU Working Group on Cartographic Coordinates and Rotational Elements of the Planets and Satellites", Celestial Mechanics and Dynamical Astronomy, 63 (2): 127, Bibcode:1996CeMDA..63..127D, doi:10.1007/BF00693410
- ↑ "USGS Astrogeology: Rotation and pole position for the Sun and planets (IAU WGCCRE)". Retrieved 22 October 2009.
- ↑ "The Magellan Venus Explorer's Guide". Retrieved 22 October 2009.
See also
Venus has many craters and the surface temperature is over 800 degrees Fahrenheit and is unable to be inhabitable
