Radiation assessment detector
Radiation Assessment Detector (RAD) was the first of ten instruments in the Mars Science Laboratory (MSL) to be turned on.
The first role of RAD was to characterize the broad spectrum of radiation environment found inside the spacecraft during the cruise phase. These measurements have never been done before from the inside of a spacecraft in interplanetary space. Its primary purpose is to determine the viability and shielding needs for potential human travelers on a manned mission to Mars, as well as to characterize the radiation environment on the surface of Mars, which it started doing immediately after MSL landed in August 2012. Turned on after launch, the RAD recorded several radiation spikes caused by the Sun.
RAD is funded by the Exploration Systems Mission Directorate at NASA Headquarters and Germany's Space Agency (DLR), and developed by the Southwest Research Institute (SwRI) and the extraterrestrial physics group at Christian-Albrechts-Universität zu Kiel, Germany.
On 31 May 2013, NASA scientists reported the results obtained during cruise, and stated that the equivalent dose radiation for even the shortest round-trip with current propulsion systems and comparable shielding is found to be 0.66 ± 0.12 sievert. This implies a great health risk caused by energetic particle radiation for any manned mission to Mars.
The radiation sources that are of concern for human health also affect microbial survival as well as the preservation of organic chemicals and biomolecules. The RAD is currently quantifying the flux of biologically hazardous radiation at the surface of Mars today, and will help determine how these fluxes vary on diurnal, seasonal, solar cycle and episodic (flare, storm) timescales. These measurements will allow calculations of the depth in rock or soil to which this flux, when integrated over long timescales, provides a lethal dose for known terrestrial microorganisms. Through such measurements, scientists can learn how deep below the surface life would have to be, or have been in the past, to be protected.
Research published in January 2014 of data from RAD, state that "ionizing radiation strongly influences chemical compositions and structures, especially for water, salts, and redox-sensitive components such as organic matter." The report concludes that the in situ "surface measurements —and subsurface estimates— constrain the preservation window for Martian organic matter following exhumation and exposure to ionizing radiation in the top few meters of the Martian surface.
- Cosmic ray
- Effect of spaceflight on the human body
- Exploration of Mars
- Health threat from cosmic rays
- Manned mission to Mars
- Spaceflight radiation carcinogenesis
- Space medicine
- Timeline of Mars Science Laboratory
- "SwRI Radiation Assessment Detector (RAD) Homepage". Southwest Research Institute. Retrieved 19 January 2011.
- NASA – RAD
- Kerr, Richard (31 May 2013). "Radiation Will Make Astronauts' Trip to Mars Even Riskier". Science 340 (6136): 1031. doi:10.1126/science.340.6136.1031. Retrieved 31 May 2013.
- Zeitlin, C. et al. (31 May 2013). "Measurements of Energetic Particle Radiation in Transit to Mars on the Mars Science Laboratory". Science 340 (6136): 1080–1084. doi:10.1126/science.1235989. Retrieved 31 May 2013.
- Chang, Kenneth (30 May 2013). "Data Point to Radiation Risk for Travelers to Mars". New York Times. Retrieved 31 May 2013.
- First radiation measurements from the surface of Mars. (9 December 2013). Southwest Research Institute. Science Daily.
- Hassler, Donald M.; Zeitlin, Cary; Wimmer-Schweingruber, Robert F.; Ehresmann, Bent; Rafkin, Scot; Martin, Cesar; Boettcher, Stephan; Koehler, Jan; Guo, Jingnan; Brinza, David E. Reitz, Guenther; Posner, Arik; the MSL Science Team (7-12 April 2013), "The Radiation Environment on the Martian Surface and during MSL's Cruise to Mars", EGU General Assembly 2013, Ads Labs, retrieved 23 June 2013
- Hassler, Donald M.; et al (24 January 2014). "Mars’ Surface Radiation Environment Measured with the Mars ScienceLaboratory’s Curiosity Rover" (PDF). Science 343 (6169). doi: 10.1126/science.1244797. Retrieved 2014-01-27.