Relative Humidity And Vapor Amount At Jezero Crater
L. K. Tamppari, Jet Propulsion Laboratory/California Institute Of Technology, Pasadena, Ca, Usa
(Leslie.Tamppari@Jpl.Nasa.Gov), G. Martínez, Lunar And Planetary Institute, Houston, Tx, Usa, J. A.
Rodríguez-Manfredi, Centro De Astrobiologia (Inta-Csic), Madrid, Spain, M. De La Torre-Juárez, Jet Propulsion Laboratory/California Institute Of Technology, Pasadena, Ca, Usa, M. Hieta, J. Polkko, I.
Jaakonaho, M. Genzer, A.-M. Harri, Finnish Meteorological Institute, Helsinki, Finland, T. Mcconnochie,
Space Science Institute, Boulder, Co, Usa, F. Montmessin, Latmos, Guyancourt, France, M. Smith, Nasa
Goddard Space Flight Center, Greenbelt, Md, Usa, M. Wolff, Space Science Institute, Boulder, Co, Usa, E.
Fischer, University Of Michigan, Ann Arbor, Mi, Usa, P. Conrad, Carnegie Institution Of Science, Washington,
D.C., Usa, F. Gómez, M.-P. Zorzano, And D. Viudez-Moreiras, Centro De Astrobiologia (Inta-Csic), Madrid, Spain, P. Patel, Jet Propulsion Laboratory/California Institute Of Technology, Pasadena, Ca, Usa, M.
Lemmon, Space Science Institute, Boulder, Co, Usa, And The Meda Team.
Introduction:
Near-Surface Water Content And Relative Humidity
Are Important For Understanding The Overall Column
Distribution Of Water, The Exchange With The Surface
And Near-Subsurface, The Potential For Brine Or Frost
Formation, And General Modern Habitability Potential
Of The Local Environment (See E.G., [1-3]). Humidity
Sensors Have Been Used On Phoenix, Msl, And Now
Perseverance To Gain This Understanding.
The Perseverance Meda Relative Humidity