Towards a global model of the martian atmosphere [PDF]
In an effort to continuously improve the capabilities of the Martian atmospheric predictions at LMD, the GCM has been extended into thermospheric heights thus creating the first model to self-consistently couple the lower and upper regions of the ...
Angelats i Coll, M.+7 more
core
Abstract Mars may have had an ancient ocean filling its northern lowlands until around 3.5 billion years ago. The existence or lack of such a large body of water would have important implications on the ancient martian climate, landscapes, and habitability.
Zachary J. Baran, Benjamin T. Cardenas
wiley +1 more source
Wind measurements in Mars' middle atmosphere at equinox and solstice: IRAM Plateau de Bure interferometric CO observations [PDF]
Characterizing the Martian atmosphere is an essential objective to understand its meteorology and its climate. The lower atmosphere (< 40 km) and middle atmosphere (40-80 km) of Mars appear dynamically coupled at much higher levels than in the case of the Earth.
arxiv
Non-tidal Coupling of the Orbital and Rotational Motions of Extended Bodies [PDF]
The orbital motions and spin-axis rotations of extended bodies are traditionally considered to be coupled only by tidal mechanisms. The orbit-spin coupling hypothesis supplies an additional mechanism. A reversing torque on rotating extended bodies is identified.
arxiv
Different Faces of the Martian Magnetosphere
Abstract The Martian magnetosphere contains components of the induced and intrinsic magnetospheres. Since we can not get a global snapshot of the magnetosphere we use a statistical picture based on a large number of measurements. Depending on the choice of coordinate system and the data selection we can observe different faces of the Martian ...
E. Dubinin+5 more
wiley +1 more source
An estimation of the mass dragged by the solar wind from Mars’s atmosphere in its geologic history [PDF]
In the past Mars had a denser atmosphere, but it lacks a magnetic field to protect the ionosphere and exosphere from the solar wind. A model for describing the loss of atmosphere in geologic time is presented.
Héctor Javier Durand-Manterola
doaj
Hubble Space Telescope observations of Mars [PDF]
Hubble Space Telescope (HST) afforded the possibility of resolving features as small as 100 km on the Martian surface even when it is at the far point of its orbit. Therefore it is ideally suited for monitoring seasonal changes on the red planet.
Clancy, Todd+6 more
core +1 more source
Nowcasting Solar Energetic Particle Events for Mars Missions
Abstract In addition to the omnipresent Galactic Cosmic Rays, sudden Solar Energetic Particle (SEP) events present considerable health hazards for manned space missions. These events not only contribute to an increased long‐term cancer risk, but can, in extreme cases, cause acute radiation syndromes.
Jan Leo Löwe+10 more
wiley +1 more source
Assessment of the probability of microbial contamination for sample return from Martian moons I: Departure of microbes from Martian surface [PDF]
Potential microbial contamination of Martian moons, Phobos and Deimos, which can be brought about by transportation of Mars ejecta produced by meteoroid impacts on the Martian surface, has been comprehensively assessed in a statistical approach, based on the most probable history of recent major gigantic meteoroid collisions on the Martian surface ...
arxiv
Beyond the horizon: Why space biology is the next great innovation opportunity
Experimental Physiology, EarlyView.
Carina Kern, Keith Siew
wiley +1 more source