World Library  
Flag as Inappropriate
Email this Article

Rahe (crater)

Article Id: WHEBN0036002618
Reproduction Date:

Title: Rahe (crater)  
Author: World Heritage Encyclopedia
Language: English
Subject: Asopus Vallis, Apsus Vallis, Ausonia Montes, Ganges Mensa, Pityusa Patera
Publisher: World Heritage Encyclopedia

Rahe (crater)

2001 Mars Odyssey THEMIS mosaic showing Ceraunius Tholus (below) and Uranius Tholus (above). Rahe crater is at the center.
Feature type crater

Rahe is a crater on the planet Mars in the Tharsis quadrangle, positioned at 25.05° north latitude and 262.52° east longitude,[1] between the volcanoes Ceraunius Tholus and Uranius Tholus. It is named after Jurgen H. Rahe, a German-American astronomer and NASA science program director.[1][2] The crater has an elongated shape measuring 35 km by 18 km and is the result of an oblique impact. A channel connects Rahe crater to the vicinity of the summit caldera of Ceraunius Tholus, with an interesting fan-shaped deposit at the lower end.

Rahe Crater is 1 km deep in places, and was created by a low angle impact which is evident by its elongated shape and ejecta deposit in the shape of a “butterfly.”[3][4] Rahe Crater is believed to once have held a lake. The lake was formed because heat from the nearby volcano Ceraunius Tholus melted glaciers. Melt water first collected in the caldera of Cerunius Tholus, and then spilled over the caldera rim forming a valley and the lake in Rahe Crater. The valley that carried the water was about 200 m wide. A delta formed where the valley entered Rahe Crater.[5] This type of event involving volcanic heat melting glaciers is common in Iceland. Eruptions under glaciers are called jökulhlaups and average two each century.[6] Studies of climate change show that many low-latitude regions accumulated large amounts of snow when the climate was different.[7][8]

See also


  1. ^ a b Blue, Jennifer. "Rahe (crater)". Gazetteer of Planetary Nomenclature. USGS Astrogeology Research Program.
  2. ^
  3. ^ Gault, D. J. Wedekind. 1978. Experimental studies of oblique impact. Proc. Lunar Planet. Sci. Conf. 9, 3843-3875.
  4. ^ Nyquist, L. 1983. Do Oblique Impacts Produce Martian Meteorites? Proc. Lunar Planet. Sci. Conf. 13, pt.2 Geophys. Res. (Supp.) 88S, A785-A798.
  5. ^ Fassett, C. J. Head. 2007. Valley Formation on Martian Volcanoes in the Hesperian: Evidence for Melting of Summit Snowpack, Caldera Lake Formation, Drainage and Erosion on Ceraunis Tholus, Mars. Icarus: 189, 118-135.
  6. ^ Bjornnson, H, F. Palsson, M. Gudmundsson. 2000. Surface and bedrock topography of the Myrdalsjokull ice cap, Iceland: The Katla caldera, eruption sites and routes of jökulhlaups. Jokull: 49, 29-46.
  7. ^ Head, J. et al. 2005. Tropical to mid-latitude snow and ice accumulation, flor and glaciation on Mars. Nature:434,346-351.
  8. ^ Head, J. et al. 2006. Extensive valley glacier deposits in the northern mid-latitudes of Mars: Evidence for Late Amazonian obliquity-driven climate change. Earth Planet. Sci. Lett. 241,663-671.

This article was sourced from Creative Commons Attribution-ShareAlike License; additional terms may apply. World Heritage Encyclopedia content is assembled from numerous content providers, Open Access Publishing, and in compliance with The Fair Access to Science and Technology Research Act (FASTR), Wikimedia Foundation, Inc., Public Library of Science, The Encyclopedia of Life, Open Book Publishers (OBP), PubMed, U.S. National Library of Medicine, National Center for Biotechnology Information, U.S. National Library of Medicine, National Institutes of Health (NIH), U.S. Department of Health & Human Services, and, which sources content from all federal, state, local, tribal, and territorial government publication portals (.gov, .mil, .edu). Funding for and content contributors is made possible from the U.S. Congress, E-Government Act of 2002.
Crowd sourced content that is contributed to World Heritage Encyclopedia is peer reviewed and edited by our editorial staff to ensure quality scholarly research articles.
By using this site, you agree to the Terms of Use and Privacy Policy. World Heritage Encyclopedia™ is a registered trademark of the World Public Library Association, a non-profit organization.

Copyright © World Library Foundation. All rights reserved. eBooks from Hawaii eBook Library are sponsored by the World Library Foundation,
a 501c(4) Member's Support Non-Profit Organization, and is NOT affiliated with any governmental agency or department.