In the first 300 days of the Mars Science Laboratory surface mission, the Curiosity rover cruised around the planet’s Gale Crater, collecting soil samples and investigating rock structures while the onboard Radiation Assessment Detector made detailed measurements of the radiation environment on the surface of Mars.
SwRI scientists published radiation surface dose rates from the first 300 days on Mars in Science online Dec. 9. Curiosity’s Radiation Assessment Detector observed a spike in the radiation dose associated with one hard solar energetic particle event and three dips in radiation associated with soft interplanetary coronal mass ejections, which provided magnetic shielding against galactic cosmic rays. Occasional brief gaps are typically when RAD was powered off to minimize interference with other activities.
“Our measurements provide crucial information for human missions to Mars,” said Dr. Don Hassler, a Southwest Research Institute program director and RAD principal investigator. Hassler is the lead author of “Mars’ Surface Radiation Environment Measured with the Mars Science Laboratory’s Curiosity Rover,” scheduled for publication in the journal Science online on December 9, 2013. “We’re continuing to monitor the radiation environment, and seeing the effects of major solar storms on the surface and at different times in the solar cycle will give additional important data. Our measurements also tie into Curiosity’s investigations about habitability. The radiation sources that are of concern for human health also affect microbial survival as well as the preservation of organic chemicals.”
Two forms of radiation pose potential health risks to astronauts: a chronic low dose of galactic cosmic rays (GCRs) and the possibility of short-term exposures to the solar energetic particles (SEPs) associated with solar flares and coronal mass ejections. The radiation on Mars is much harsher than on Earth for two reasons: Mars lacks a global magnetic field and the Martian atmosphere is much thinner than Earth’s, providing little shielding to the surface.
This environmental factor poses a challenge for future human exploration of Mars and is also important in understanding both geological and potential biological evolution on Mars. Both GCRs and SEPs interact with the atmosphere and, if energetic enough, penetrate into the Martian soil, or regolith, where they produce secondary particles that contribute to the complex radiation environment on the Martian surface, which is unlike anything on Earth.
“The RAD surface radiation data show an average GCR dose equivalent rate of 0.67 millisieverts per day from August 2012 to June 2013 on the Martian surface,” said Hassler. Radiation dose is measured in units of sievert (Sv) or millisievert (1/1000 Sv). “In comparison, RAD data show an average GCR dose equivalent rate of 1.8 millisieverts per day on the journey to Mars, when RAD measured the radiation inside the spaceship.”
Using the data collected by SwRI’s Radiation Assessment Detector onboard the Curiosity rover, this chart compares the radiation dose equivalent for a 500-day stay on Mars to the dose associated with a 180-day journey to Mars, a six-month stay on the International Space Station and several Earth-based sources of radiation.
According to RAD data, most mission radiation exposure will be during outbound and return travel, when the astronauts will be exposed to the radiation environment in interplanetary space, shielded only by the spacecraft itself. The total during just the transit phases of a Mars mission would be approximately 0.66 Sv for a round trip with current propulsion systems and during similar solar activity. A 500-day mission on the surface would bring the total exposure to around 1 Sv.
Long-term population studies have shown that exposure to radiation increases a person’s lifetime cancer risk; exposure to a dose of 1 Sv is associated with a five percent increase in fatal cancer risk. Although NASA has generally established a three percent increased risk of fatal cancer as an acceptable career limit for astronauts in low earth orbit, it does not currently have a limit for deep space missions, and is working with the National Academies Institute of Medicine to determine appropriate limits for deep space missions, such as a mission to Mars in the 2030s.
SwRI, together with Christian Albrechts University in Kiel, Germany, built RAD with funding from the NASA Human Exploration and Operations Mission Directorate and Germany’s national aerospace research center, Deutsches Zentrum für Luft- und Raumfahrt.
NASA’s Jet Propulsion Laboratory, a division of the California Institute of Technology, Pasadena, Calif., manages the Mars Science Laboratory Project. The NASA Science Mission Directorate, at NASA Headquarters in Washington, manages the Mars Exploration Program.
“Mars’ Surface Radiation Environment Measured with the Mars Science Laboratory’s Curiosity Rover,” published in Science online December 9, was written by Hassler, Cary Zeitlin of SwRI, Robert F. Wimmer-Schweingruber of Christian Albrechts University, Bent Ehresmann of SwRI, Scot Rafkin of SwRI, Jennifer L. Eigenbrode of NASA’s Goddard Space Flight Center, David E. Brinza of JPL, Gerald Weigle of SwRI, Stephan Böttcher of Christian Albrechts University , Eckart Böhm of Christian Albrechts University, Soenke Burmeister of Christian Albrechts University, Jingnan Guo of Christian Albrechts University, Jan Köhler of Christian Albrechts University, Cesar Martin of Christian Albrechts University, Guenther Reitz of German Aerospace Center in Cologne, Germany, Francis A. Cucinotta of University of Nevada Las Vegas, Myung-Hee Kim of Universities Space Research Association, David Grinspoon of the Denver Museum of Nature and Science, Mark A. Bullock of SwRI, Arik Posner of NASA, Javier Gómez-Elvira of Centro de Astrobiología in Madrid, Spain, Ashwin Vasavada of JPL, and John P.Grotzinger of JPL, and the MSL Science Team.
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