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Robert M. Haberle
Researcher at Ames Research Center
Publications - 195
Citations - 13491
Robert M. Haberle is an academic researcher from Ames Research Center. The author has contributed to research in topics: Mars Exploration Program & Atmosphere of Mars. The author has an hindex of 58, co-authored 192 publications receiving 12240 citations. Previous affiliations of Robert M. Haberle include California Institute of Technology & University of Washington.
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Journal ArticleDOI
Context Camera Investigation on board the Mars Reconnaissance Orbiter
Michael C. Malin,James F. Bell,Bruce A. Cantor,Michael Caplinger,Wendy M. Calvin,R. Todd Clancy,Kenneth S. Edgett,Lawrence Edwards,Robert M. Haberle,P. B. James,Steven W. Lee,Michael A. Ravine,Peter C. Thomas,Michael J. Wolff +13 more
TL;DR: The Context Camera (CTX) on the Mars Reconnaissance Orbiter (MRO) is a Facility Instrument (i.e., government-furnished equipment operated by a science team not responsible for design and fabrication) designed, built, and operated by Malin Space Science Systems and the MRO Mars Color Imager team (MARCI) as mentioned in this paper.
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The Mars Pathfinder atmospheric structure investigation/meteorology (ASI/MET) experiment
John T. Schofield,Jeffrey R. Barnes,David Crisp,Robert M. Haberle,Søren Ejling Larsen,Julio A. Magalhães,James R. Murphy,Alvin Seiff,Greg W. Wilson +8 more
TL;DR: The Mars Pathfinder atmospheric structure investigation/meteorology (ASI/MET) experiment measured the vertical density, pressure, and temperature structure of the martian atmosphere from the surface to 160 km, and monitored surface meteorology and climate for 83 sols.
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Simulations of the Atmospheres of Synchronously Rotating Terrestrial Planets Orbiting M Dwarfs: Conditions for Atmospheric Collapse and the Implications for Habitability☆
TL;DR: In this article, the authors present results of three-dimensional simulations of the atmospheres of such planets, and comment on their possible habitability, concluding that these planets orbiting M stars can support atmospheres over a large range of conditions and, despite constraints such as stellar activity, are very likely to be habitable.
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Formation of Glaciers on Mars by Atmospheric Precipitation at High Obliquity
TL;DR: High-resolution climate simulations performed with a model designed to simulate the present-day Mars water cycle but assuming a 45° obliquity points to an atmospheric origin for the ice and reveals how precipitation could have formed glaciers on Mars.
Journal ArticleDOI
A reappraisal of the habitability of planets around M dwarf stars.
Jill Tarter,Peter Backus,Rocco L. Mancinelli,Jonathan M. Aurnou,Dana E. Backman,Gibor Basri,Alan P. Boss,Andrew Clarke,Drake Deming,Laurance R. Doyle,Eric D. Feigelson,Friedmann Freund,David Grinspoon,Robert M. Haberle,Steven A. Hauck,Martin J. Heath,Todd J. Henry,Jeffery L. Hollingsworth,Manoj Joshi,Steven Kilston,Michael C. Liu,Eric Meikle,I. Neill Reid,Lynn J. Rothschild,John Scalo,Antígona Segura,Carol M. Tang,James M. Tiedje,Margaret C. Turnbull,Lucianne M. Walkowicz,Arthur L. Weber,Richard E. Young +31 more
TL;DR: It is concluded that M dwarf stars may indeed be viable hosts for planets on which the origin and evolution of life can occur and it makes sense to include M dwarfs in programs that seek to find habitable worlds and evidence of life.