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The EnVision Venus orbiter mission, proposed to ESA

Colin Wilson

Visitor

Research theme

  • Exoplanets and planetary physics

Sub department

  • Atmospheric, Oceanic and Planetary Physics

Research groups

  • Planetary atmosphere observation analysis
  • Planetary surfaces
  • Solar system
  • Space instrumentation
Colin.Wilson@physics.ox.ac.uk
Telephone: 07939202151
Atmospheric Physics Clarendon Laboratory, room 209a
  • About
  • Publications

Venus's Southern Polar Vortex Reveals Precessing Circulation

Science (2011) 1-3

Authors:

D Luz, DL Berry, G Piccioni, P Drossart, R Politi, CF Wilson, S Erard, F Nuccilli

Venus Cloud Properties from Venus Express VIRTIS Observations

AAS/Division for Planetary Sciences Meeting Abstracts #42 42 (2010) 994-994

Authors:

J Barstow, FW Taylor, CCC Tsang, CF Wilson, PGJ Irwin, P Drossart, G Piccioni

Simulating weathering of basalt on Mars and Earth by thermal cycling

Geophysical Research Letters 37:18 (2010)

Authors:

H Viles, B Ehlmann, CF Wilson, T Cebula, M Page, M Bourke

Abstract:

Physical weathering induced by heating and cooling may cause rock breakdown on Mars and Earth. We report results from parallel weathering simulations on basalt blocks exposed to diurnal cycles representing Mars-like (two simulation runs from -55 to +20 oC and -75 to +10 oC, 1-100% relative humidity, 4-8 mbar pressure, CO2 atmosphere) and hot arid Earth (23-72o C, 30-100% relative humidity) conditions. Under Earth conditions, thermally pre-stressed blocks showed measurable strength declines, whilst salt pre-treated blocks showed strength gains. Under Mars-like conditions, pre-stressed blocks recorded greater or similar strength declines and salt pre-treated blocks showed more muted strength declines than under Earth conditions. The results imply that on Earth and Mars diurnal cycling of temperature alone can cause deterioration of basalt with a pre-existing stress history. The type of stress history is important, with salt pre-treatment affecting the response of thermally pre-stressed blocks under both Earth and Mars conditions. Copyright 漏 2010 by the American Geophysical Union.

Correlations between cloud thickness and sub-cloud water abundance on Venus

GEOPHYSICAL RESEARCH LETTERS 37 (2010) ARTN L02202

Authors:

Constantine CC Tsang, Colin F Wilson, Joanna K Barstow, Patrick GJ Irwin, Fredric W Taylor, Kevin McGouldrick, Giuseppe Piccioni, Pierre Drossart, Hakan Svedhem

Determining vertical cloud structure on Venus using near-infrared spectroscopy

European Planetary Science Congress 2009 (2009) 249-249

Authors:

JK Barstow, FW Taylor, CCC Tsang, CF Wilson, PGJ Irwin, P Drossart, G Piccioni

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