Curiosity's rover environmental monitoring station: Overview of the first 100 sols

Javier Gómez‐Elvira(Centro de Astrobiología), Carlos Armiens(Centro de Astrobiología), I. Carrasco(Centro de Astrobiología), M. Genzer(Finnish Meteorological Institute), Felipe Gómez(Centro de Astrobiología), R. M. Haberle(Ames Research Center), V. E. Hamilton(Southwest Research Institute), Ari‐Matti Harri(Finnish Meteorological Institute), Henrik Kahanpää(Finnish Meteorological Institute), Osku Kemppinen(Finnish Meteorological Institute), A. Lepinette(Centro de Astrobiología), Javier Martín Soler(Centro de Astrobiología), Javier Martín‐Torres(Instituto Andaluz de Ciencias de la Tierra), Jesús Martínez‐Frías(Centro de Astrobiología), M. A. Mischna(Jet Propulsion Laboratory), Luis Mora‐Sotomayor(Centro de Astrobiología), Sara Navarro(Centro de Astrobiología), Claire Newman(Ashima Group (United States)), M. A. de Pablo(Universidad de Alcalá), V. Peinado(Centro de Astrobiología), Jouni Polkko(Finnish Meteorological Institute), Scot Rafkin(Southwest Research Institute), Miguel Ramos(Universidad de Alcalá), N. O. Rennó(University of Michigan), M. I. Richardson(Ashima Group (United States)), J. A. Rodríguez‐Manfredi(Centro de Astrobiología), Julio José Romeral-Planelló(Centro de Astrobiología), Eduardo Sebastián(Centro de Astrobiología), Manuel de la Torre Juárez(Jet Propulsion Laboratory), J. Torres(Centro de Astrobiología), R. Urquí(Ingeniería de Sistemas para la Defensa de España), A. R. Vasavada(Jet Propulsion Laboratory), J. Verdasca(Centro de Astrobiología), María‐Paz Zorzano(Centro de Astrobiología)
Journal of Geophysical Research Planets
May 22, 2014
Cited by 139Open Access
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Abstract

In the first 100 Martian solar days (sols) of the Mars Science Laboratory mission, the Rover Environmental Monitoring Station (REMS) measured the seasonally evolving diurnal cycles of ultraviolet radiation, atmospheric pressure, air temperature, ground temperature, relative humidity, and wind within Gale Crater on Mars. As an introduction to several REMS-based articles in this issue, we provide an overview of the design and performance of the REMS sensors and discuss our approach to mitigating some of the difficulties we encountered following landing, including the loss of one of the two wind sensors. We discuss the REMS data set in the context of other Mars Science Laboratory instruments and observations and describe how an enhanced observing strategy greatly increased the amount of REMS data returned in the first 100 sols, providing complete coverage of the diurnal cycle every 4 to 6 sols. Finally, we provide a brief overview of key science results from the first 100 sols. We found Gale to be very dry, never reaching saturation relative humidities, subject to larger diurnal surface pressure variations than seen by any previous lander on Mars, air temperatures consistent with model predictions and abundant short timescale variability, and surface temperatures responsive to changes in surface properties and suggestive of subsurface layering.


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