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 © 2010 by the American Geophysical Union.

HARMONI: a single-field wide-band integral-field spectrograph for the European ELT

Proceedings of SPIE--the International Society for Optical Engineering SPIE, the international society for optics and photonics 7735 (2010) 77352i-77352i-11

Authors:

Niranjan Thatte, Mathias Tecza, Fraser Clarke, Roger L Davies, Alban Remillieux, Roland Bacon, David Lunney, Santiago Arribas, Evencio Mediavilla, Fernando Gago, Naidu Bezawada, Pierre Ferruit, Ana Fragoso, David Freeman, Javier Fuentes, Thierry Fusco, Angus Gallie, Adolfo Garcia, Timothy Goodsall, Felix Gracia, Aurelien Jarno, Johan Kosmalski, James Lynn, Stuart McLay, David Montgomery, Arlette Pecontal, Hermine Schnetler, Harry Smith, Dario Sosa, Giuseppina Battaglia, Neil Bowles, Luis Colina, Eric Emsellem, Ana Garcia-Perez, Szymon Gladysz, Isobel Hook, Patrick Irwin, Matt Jarvis, Robert Kennicutt, Andrew Levan, Andy Longmore, John Magorrian, Mark McCaughrean, Livia Origlia, Rafael Rebolo, Dimitra Rigopoulou, Sean Ryan, Mark Swinbank, Nial Tanvir, Eline Tolstoy, Aprajita Verma

The future of planetary geophysics

Astronomy & Geophysics Oxford University Press (OUP) 51:2 (2010) 2.22-2.25

Authors:

Nick Teanby, Neil Bowles

Thermal inertia and bolometric Bond albedo values for Mimas, Enceladus, Tethys, Dione, Rhea and Iapetus as derived from Cassini/CIRS measurements

Icarus Elsevier 206:2 (2010) 573-593

Authors:

CJA Howett, JR Spencer, J Pearl, M Segura

Structure and dynamics of the Martian lower and middle atmosphere as observed by the Mars Climate Sounder: Seasonal variations in zonal mean temperature, dust, and water ice aerosols

Journal of Geophysical Research: Planets 115:12 (2010)

Authors:

DJ McCleese, NG Heavens, JT Schofield, WA Abdou, JL Bandfield, SB Calcutt, PGJ Irwin, DM Kass, A Kleinböhl, SR Lewis, DA Paige, PL Read, MI Richardson, JH Shirley, FW Taylor, N Teanby, RW Zurek

Abstract:

The first Martian year and a half of observations by the Mars Climate Sounder aboard the Mars Reconnaissance Orbiter has revealed new details of the thermal structure and distributions of dust and water ice in the atmosphere. The Martian atmosphere is shown in the observations by the Mars Climate Sounder to vary seasonally between two modes: a symmetrical equinoctial structure with middle atmosphere polar warming and a solstitial structure with an intense middle atmosphere polar warming overlying a deep winter polar vortex. The dust distribution, in particular, is more complex than appreciated before the advent of these high (∼5 km) vertical resolution observations, which extend from near the surface to above 80 km and yield 13 dayside and 13 nightside pole-to-pole cross sections each day. Among the new features noted is a persistent maximum in dust mass mixing ratio at 15-25 km above the surface (at least on the nightside) during northern spring and summer. The water ice distribution is very sensitive to the diurnal and seasonal variation of temperature and is a good tracer of the vertically propagating tide. Copyright 2010 by the American Geophysical Union.