In astrogeology, an arachnoid /əˈræknɔɪd/ is a large geological structure resembling a spider web. They are of unknown origin, and have been found only on the surface of the planet Venus. They appear as concentric ovals surrounded by a complex network of fractures, and can span 200 kilometers. Over 90 arachnoids have been identified on Venus.
Arachnoids could be related to volcanos, however it is also possible that different arachnoids are formed by different processes. One possible explanation is that an upwelling of magma from the interior of the planet pushed up on the surface, causing cracks. An alternate theory concerning their origin is that they are a precursor to coronae formation.
Much of what is known about arachnoids is the result of studies performed by C.B. Dawson and L.S. Crumpler.
See also
References
- "Planetary Names: Corona, coronae: Trotula Corona on Venus". planetarynames.wr.usgs.gov. Archived from the original on 1 October 2015. Retrieved 26 January 2022.
- Kostama, V.P. (2002). "The Four Arachnoid Groups of Venus" (PDF). Lunar and Planetary Science Conference: 1115. Bibcode:2002LPI....33.1115K – via lpi.
- This article contains text from the Astronomy Picture of the Day . As a work of the United States Federal Government, it is in the public domain.
- "WTP: Venus: Arachnoids". pds.jpl.nasa.gov. Retrieved 2017-04-06.
- Hamilton, Calvin J. "Arachnoids". solarviews.com. Retrieved 2017-04-06.
- Dawson and Crumpler. "Characteristics of Arachnoids from Magellan Data" (PDF). Lunar and Planetary Institute Conference: 383–384 – via LPSC.
External links
This article incorporates text from a public-domain NASA website.
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