Uranius Tholus
Uranius Tholus is a volcano on Mars located in the Tharsis quadrangle at 26.52° north latitude and 262.43° east longitude. It is 61.4 kilometres (38 mi) across with an elevation of 4,290 metres (14,075 ft)[1] and was named after a classical albedo feature name.[2]
![]() 2001 Mars Odyssey THEMIS mosaic of Uranius Tholus (upper volcano) and Ceraunius Tholus (lower volcano). | |
Feature type | mountain |
---|---|
Coordinates | 26.52°N 262.43°E |
Peak | 4,290 metres (14,075 ft) |
Uranius Tholus is part of the Uranius group of volcanoes and lies north of the larger Ceraunius Tholus.
Volcanoes
Tharsis is a land of great volcanoes. Olympus Mons is the tallest known volcano. "Mons" is a term used for a large raised feature. "Tholus" is about the same, but smaller.
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Wikimedia Commons has media related to Uranius Tholus. |
gollark: Wikipedia says that spider silk has a diameter of "2.5–4 μm", which I approximated to 3μm for convenience, so a strand has a 1.5μm radius. That means that its cross-sectional area (if we assume this long thing of spider silk is a cylinder) is (1.5e-6)², or ~7e-12. Wikipedia also says its density is about 1.3g/cm³, which is 1300kg/m³, and that the observable universe has a diameter of 93 billion light-years (8.8e26 meters). So multiply the length of the strand (the observable universe's diameter) by the density of spider silk by the cross-sectional area of the strand and you get 8e18 kg, while the atmosphere's mass is about 5e18 kg, so close enough really.
gollark: Okay, so by mass it actually seems roughly correct.
gollark: So, spider silk comes in *very* thin strands and is somewhat denser than water, interesting.
gollark: You do that, I'll try and find data on spider silk density.
gollark: Actually, this factoid does seem kind of dubious even if it's meant to say "mass"... hmm.
References
- Peter Grego (1 June 2012). Mars and How to Observe It. Springer. pp. 63. ISBN 978-1-4614-2302-7. Retrieved 10 September 2019.
- "Uranius Tholus". Gazetteer of Planetary Nomenclature. USGS Astrogeology Research Program.
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