Recent Hotspot Volcanism on Venus from VIRTIS Emissivity Data

• DOI: 10.1126/science.1186785
• Publication Date: 2010-04-09T02:37:49Z
• Authors: Suzanne E. Smrekar; Ellen R. Stofan; Nils Mueller; Allan Treiman; Linda Elkins-Tanton; Joern Helbert; Giuseppe Piccioni; Pierre Drossart
• Keywords: Venus Express; 550; 500; Hotspot Volcanism; VIRTIS; Vulkanismus; Venus; 01 natural sciences; 13. Climate action; VenusExpress; 0103 physical sciences; [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]; [PHYS.ASTR] Physics [physics]/Astrophysics [astro-ph]

Hotspots on Venus

The surface of Venus shows clear signs of volcanism, but are there active volcanoes on Venus today? The answer to this question will bear on our understanding of the planet's climate evolution and interior dynamics. Using surface thermal emissivity data returned by the Venus Express spacecraft,

Smrekar et al.

(p. 605 , published online 8 April) looked at three hotspots on Venus. These places were identified by analogy with terrestrial hotspots like Hawaii, which are believed to overlie mantle plumes and to be the most likely sites for current volcanic activity. Lava flows at the three hotspots have anomalously high thermal emissions when compared with their surroundings. Low emissivity is generally interpreted as the result of surface alteration by the corrosive atmosphere of Venus. High emissivity implies that not much alteration took place and thus that the hotspots must represent recently active volcanoes younger than 2.5 million years.