New insights into martian atmospheric chemistry
نویسندگان
چکیده
منابع مشابه
New Insights on Martian Atmospheric Neon from Martian Meteorite, Dhofar
Introduction: Martian space probe, Viking landers could not measure Ne isotopic ratios, but only had the concentration of Ne as 2.5 ppm (error +3.5, -1.5) in Martian atmosphere [1]. After that, there have been many efforts to determine Ne isotopic composition of Martian atmosphere, by examining the Martian atmospheric gases trapped in impact glasses of the EET 79001 and other shergottites [2-6]...
متن کاملLaboratory simulation of Martian atmospheric chemistry
Measurements of the yield of important trace gas species such as ozone, evolved during photolytic reactions have been made under Martian environmental conditions in one of the The Open University’s Mars simulation chambers. The simulation chamber can mimic Martian temperatures and pressures and a UV solar simulator can be added to irradiate a Marslike gas mixture within the chamber to drive che...
متن کاملNew Insights into Source Craters for the Martian Meteorites
C. D. K. Herd1, L. L. Tornabene2, T. J. Bowling3, E. L. Walton1,4, T. G. Sharp5, and H. J. Melosh6, 1Department of Earth and Atmospheric Sciences, 1-26 Earth Sciences Building, University of Alberta, Edmonton, AB, T6G 2E3, [email protected], 2Centre for Planetary Science and Exploration/Department of Earth Sciences, University of Western Ontario, London, ON. 3Department of the Geophysical Scienc...
متن کاملNew Insights Into the Dynamics of Martian Gullies
Mangold, D. Mège, F. Bouchut, Institut de Physique du Globe de Paris, Université Paris-Diderot, CNRS, 4 place Jussieu, 75005 Paris, France, Laboratoire de Planétologie et de Géodynamique, Université de Nantes, CNRS, 2 rue de la Houssinière, 44000 Nantes, France, 3 Département de Mathématiques et Applications, École Normale Supérieure, CNRS, 45 rue d’Ulm, 75005 Paris, France Contact: [email protected].
متن کاملIntroduction to New Martian Chemistry Workshop: "follow the Chemistry"
In the post-Viking era, Mars was defined largely in terms of geomorphology and the planet-wide cycles of water, dust, and CO2. In the 21 century, we have increasingly come to understand Mars in terms of chemical processes. Soil chemistry has become a key to understanding geological, astrobiological, and even atmospheric processes. What the future holds for our understanding of Mars will be dete...
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ژورنال
عنوان ژورنال: Icarus
سال: 2014
ISSN: 0019-1035
DOI: 10.1016/j.icarus.2014.07.023