Javascript must be enabled to continue!
Surface temperature of Mars: Exploring diurnal and seasonal variations with the Emirates Mars Mission
View through CrossRef
The ~55 hour orbit of the Emirates Mars Mission (EMM) or the “Hope'" orbiter enables it to achieve a near-global coverage of the planet every 4 orbits, or ~9 sols. The Emirates Mars Infrared Spectrometer (EMIRS) instrument on board EMM is used to retrieve surface temperatures. We study the geographical and temporal variation of surface temperature on diurnal and seasonal timescales. We compare these measurements with NASA’s rover measurements —  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. We also compare these measurements with the Mars Climate Database (MCD), identify anomalies in surface temperature and discuss the role of thermal inertia. We discuss other implications of these findings leading to a better understanding of temperature variation on Mars and its impact on weather and climate.   
Title: Surface temperature of Mars: Exploring diurnal and seasonal variations with the Emirates Mars Mission
Description:
The ~55 hour orbit of the Emirates Mars Mission (EMM) or the “Hope'" orbiter enables it to achieve a near-global coverage of the planet every 4 orbits, or ~9 sols.
The Emirates Mars Infrared Spectrometer (EMIRS) instrument on board EMM is used to retrieve surface temperatures.
We study the geographical and temporal variation of surface temperature on diurnal and seasonal timescales.
We compare these measurements with NASA’s rover measurements —  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.
We also compare these measurements with the Mars Climate Database (MCD), identify anomalies in surface temperature and discuss the role of thermal inertia.
We discuss other implications of these findings leading to a better understanding of temperature variation on Mars and its impact on weather and climate.
  .
Related Results
Study on Urban Thermal Environment based on Diurnal Temperature Range
Study on Urban Thermal Environment based on Diurnal Temperature Range
<p>Diurnal temperature range (includes land surface temperature diurnal range and near surface air temperature diurnal range) is an important meteorological parameter...
Illumination conditions on Phobos for the MMX rover mission
Illumination conditions on Phobos for the MMX rover mission
IntroductionIn preparation of the Phobos Rover experiment as part of JAXA’s Mars Moon eXplorer (MMX) mission, we study the illumination conditions on the Martian moon, fo...
From Reconstructing to Monitoring Martian Dust Storms
From Reconstructing to Monitoring Martian Dust Storms
<p>We have accumulated almost uninterrupted observations of dust from satellites in orbit around Mars for more than 20 years to date.&#160;Such a long-term an...
Companions in the Spirit – Companions in Mission
Companions in the Spirit – Companions in Mission
Introductory RemarksSince Pentecost the Holy Spirit has inspired the church to proclaim Jesus Christ as the Lord and Saviour and we continue to be obedient to the command to preach...
Results from the Emirates Mars Mission (EMM) - Hope Probe
Results from the Emirates Mars Mission (EMM) - Hope Probe
<p>The Emirates Mars Mission (EMM) &#8211; Hope Probe &#8211; has commenced its one-Martian-year science phase on May 23rd 2021. The goals of the miss...
Concept of Operations for Future Mars Helicopters: Accessing Distant Targets with a Pathfinder-Style EDL System
Concept of Operations for Future Mars Helicopters: Accessing Distant Targets with a Pathfinder-Style EDL System
. IntroductionThe highly successful campaign of the Ingenuity Mars helicopter [1] proved the feasibility of powered, controlled flight on Mars and has motivated the development of ...
Investigating Seasonal Variations in Mars' Hydrogen Escape Flux derived by model fitting Lyman Alpha observations from Emirates Mars Ultraviolet Spectrometer (EMUS) onboard the Emirates Mars Mission (EMM).
Investigating Seasonal Variations in Mars' Hydrogen Escape Flux derived by model fitting Lyman Alpha observations from Emirates Mars Ultraviolet Spectrometer (EMUS) onboard the Emirates Mars Mission (EMM).
The Martian atmosphere has undergone significant decay over time, with several factors contributing to this process. It is believed that thermal (Jeans) escape is a significant con...
Modelling very recent ice ages on Mars with the Planetary Climate Model
Modelling very recent ice ages on Mars with the Planetary Climate Model
Protected by centimeters of dry sediments, a planetary-scale mantle of relatively pure water ice covers the entire mid and high latitudes of Mars. Its presence down has been shown ...

