Diurnal variation of the surface temperature of Mars with the Emirates Mars Mission: A comparison with Curiosity and Perseverance rover measurements
Dimitra Atri, Nour Abdelmoneim, Dattaraj B. Dhuri, Mathilde Simoni
The Emirates Mars Infrared Spectrometer (EMIRS) instrument on board the Emirates Mars Mission (EMM) “Hope”, for the first time, is providing us with the temperature measurements of Mars at all local times covering most of the planet. It is therefore possible now to compare surface temperature measurements made from orbit with those from the surface by rovers during the same time period. We use data of diurnal temperature variation from the Rover Environmental Monitoring Station (REMS) suite on board the Mars Science Laboratory (MSL) “Curiosity” rover, and the Mars Environmental Dynamics Analyzer (MEDA) suite on board the Mars 2020 “Perseverance” rover, between June and August 2021 and compare them with EMIRS observations. We also compare these measurements with estimates of the Mars Climate Database (MCD) model. We show that although the overall trend of temperature variation is in excellent agreement across missions, EMIRS measurements are systematically lower at night compared to Mars 2020. We describe a number of factors which could lead to this discrepancy. We discuss the implications of these results in improving our understanding of the Martian climate which would lead to better modeling of local weather prediction, useful for future robotic and potentially crewed missions to Mars.
Comments: Submitted
Subjects: Earth and Planetary Astrophysics (astro-ph.EP); Space Physics (physics.space-ph)
Cite as: arXiv:2204.12850 [astro-ph.EP] (or arXiv:2204.12850v1 [astro-ph.EP] for this version)
https://doi.org/10.48550/arXiv.2204.12850
Focus to learn more
Submission history
From: Dimitra Atri
[v1] Wed, 27 Apr 2022 11:29:01 UTC (14,936 KB)
