Clare Fletcher , Martin Van Kranendonk , Carol Oliver
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引用次数: 0
Abstract
Of the planets in our solar system, Mars may be the most likely place to find evidence of life and learn about planetary evolution. However, in exploring Mars, we risk damaging sites of possible outstanding universal geoheritage value due to a lack of legal frameworks or practical guidelines. This study sought to develop practical exogeoconservation methods and test these at the Mars Desert Research Station (MDRS) over two crew rotations, totalling one month. However, there were several unanticipated challenges both in pre-mission planning and on-site, in-person exploration, making effective, practical exogeoconservation extremely challenging. This analogue study has implications for continued Mars exploration, as without practical exogeoconservation methods, we may risk the destruction of sites of possible outstanding universal geoheritage value on Mars. We find that exogeoconservation of Mars will require significantly more detailed information and study than is currently available. A key implication of this study is that sampling of potentially important outcrops should be reserved until after a whole area has been explored in-depth, to ensure the samples taken are both exceptional and common enough to allow for their removal. We also find that there is a role for geoconservation experts on Mars exploration teams to bring exogeoconservation principles to the forefront of Mars missions.
期刊介绍:
Planetary and Space Science publishes original articles as well as short communications (letters). Ground-based and space-borne instrumentation and laboratory simulation of solar system processes are included. The following fields of planetary and solar system research are covered:
• Celestial mechanics, including dynamical evolution of the solar system, gravitational captures and resonances, relativistic effects, tracking and dynamics
• Cosmochemistry and origin, including all aspects of the formation and initial physical and chemical evolution of the solar system
• Terrestrial planets and satellites, including the physics of the interiors, geology and morphology of the surfaces, tectonics, mineralogy and dating
• Outer planets and satellites, including formation and evolution, remote sensing at all wavelengths and in situ measurements
• Planetary atmospheres, including formation and evolution, circulation and meteorology, boundary layers, remote sensing and laboratory simulation
• Planetary magnetospheres and ionospheres, including origin of magnetic fields, magnetospheric plasma and radiation belts, and their interaction with the sun, the solar wind and satellites
• Small bodies, dust and rings, including asteroids, comets and zodiacal light and their interaction with the solar radiation and the solar wind
• Exobiology, including origin of life, detection of planetary ecosystems and pre-biological phenomena in the solar system and laboratory simulations
• Extrasolar systems, including the detection and/or the detectability of exoplanets and planetary systems, their formation and evolution, the physical and chemical properties of the exoplanets
• History of planetary and space research