Influence of Mars Topography on Radiation Dose Detected by the Mars Science Laboratory and Assessment of Mars Surface Albedo Radiation
Authors:
- Jingnan GuoJGJingnan Guo
- Gabin CharpentierGCGabin Charpentier
- Robert F. Wimmer‐SchweingruberRWRobert F. Wimmer‐Schweingruber
- Salman KhaksarighiriSKSalman Khaksarighiri
- Lu PanLPLu Pan
- Bent EhresmannBEBent Ehresmann
- Donald M. HasslerDHDonald M. Hassler
- Cary ZeitlinCZCary Zeitlin
- Daniel MatthiäDMDaniel Matthiä
- Thomas BergerTBThomas Berger
Open Access
- 21 April 2026
- journal article
- research article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research: Planets
- Vol. 131 (4)
Abstract
The Radiation Assessment Detector (RAD) on the Curiosity rover has been characterizing the Martian surface radiation field since 2012. The dose observed by RAD is influenced by a variety of factors, including an essential one, the terrain. After parking near Murray Buttes in September 2016 where it first detected a ∼5% decrease in dose rate, the rover has passed a series of other interesting terrains where we find decreases in the dose rate reaching 19%. This radiation reduction is due to extra shielding provided by the nearby surface structure, confirming the potential use of surface structures for radiation protection of humans on Mars. Combining a zenith‐angle‐dependent radiation model and the rover panoramic visibility map we calculate the downward radiation dose that RAD should observe under different topographic shielding conditions. This allows us to further evaluate the terrain‐generated albedo dose at different locations. We finally estimate that on a flat surface the albedo radiation is between ∼18% and 24% of the total surface dose. This study contributes to developing a realistic terrain‐based radiation map which is important for future Mars explorers.Keywords
This publication has 30 references indexed in Scilit:
- Charged particles radiation measurements with Liulin-MO dosimeter of FREND instrument aboard ExoMars Trace Gas Orbiter during the transit and in high elliptic Mars orbitIcarus, 2018
- Detecting Upward Directed Charged Particle Fluxes in the Mars Science Laboratory Radiation Assessment DetectorEarth and Space Science, 2017
- The radiation environment on the surface of Mars – Numerical calculations of the galactic component with GEANT4/PLANETOCOSMICSLife Sciences in Space Research, 2017
- Predictions of space radiation fatality risk for exploration missionsLife Sciences in Space Research, 2017
- MAVEN observations of the solar cycle 24 space weather conditions at MarsJournal of Geophysical Research: Space Physics, 2017
- On determining the zenith angle dependence of the Martian radiation environment at Gale Crater altitudesGeophysical Research Letters, 2015
- Computation of cosmic ray ionization and dose at Mars. I: A comparison of HZETRN and Planetocosmics for proton and alpha particlesAdvances In Space Research, 2015
- Diurnal variations of energetic particle radiation at the surface of Mars as observed by the Mars Science Laboratory Radiation Assessment DetectorJournal of Geophysical Research: Planets, 2014
- Comparison of Martian surface ionizing radiation measurements from MSL‐RAD with Badhwar‐O'Neill 2011/HZETRN model calculationsJournal of Geophysical Research: Planets, 2014
- Preface, Executive Summary and GlossaryAnnals of the ICRP, 2007