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Planetary Protection Considerations for Missions to Solar System Small Bodies: Report Series—Committee on Planetary Protection (2023)

Chapter: Appendix B: COSPAR Planetary Protection Requirements for Category I and Category II Missions

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Suggested Citation:"Appendix B: COSPAR Planetary Protection Requirements for Category I and Category II Missions." National Academies of Sciences, Engineering, and Medicine. 2023. Planetary Protection Considerations for Missions to Solar System Small Bodies: Report Series—Committee on Planetary Protection. Washington, DC: The National Academies Press. doi: 10.17226/26714.
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B

COSPAR Planetary Protection Requirements for Category I and Category II Missions

These categorizations are taken from COSPAR’s Planetary Protection Policy.1

Category I includes any mission to a target body which is not of direct interest for understanding the process of chemical evolution or the origin of life. No protection of such bodies is warranted and no planetary protection requirements are imposed by this policy.

Category II missions comprise all types of missions to those target bodies where there is significant interest relative to the process of chemical evolution and the origin of life, but where there is only a remote chance that contamination carried by a spacecraft could compromise future investigations. The requirements are for simple documentation only. Preparation of a short planetary protection plan is required for these flight projects primarily to outline intended or potential impact targets, brief Pre- and Post-launch analyses detailing impact strategies, and a Post-encounter and End-of-Mission Report which will provide the location of impact if such an event occurs. Solar system bodies considered to be classified as Category II are listed in the Appendix to this document.

Category-specific listing of target body/mission types:

Category I: Flyby, Orbiter, Lander: Undifferentiated, metamorphosed asteroids; Io; others to be defined (TBD)

Category II: Flyby, Orbiter, Lander: Venus; Moon (with organic inventory); Comets; Carbonaceous Chondrite Asteroids; Jupiter; Saturn; Uranus; Neptune; Ganymede*; Callisto; Titan*; Triton*; Pluto/Charon*; Ceres; Kuiper Belt objects > half the size of Pluto*; Kuiper Belt objects < half the size of Pluto; others TBD

* The mission-specific assignment of these bodies to Category II must be supported by an analysis of the “remote” potential for contamination of the liquid-water environments that may exist beneath their surfaces (a probability of introducing a single viable terrestrial organism of < 1 × 10−4), addressing both the existence of such environments and the prospects of accessing them.

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1 “COSPAR Policy on Planetary Protection,” prepared by the COSPAR Panel on Planetary Protection and approved by the COSPAR Bureau on June 3, 2021, https://cosparhq.cnes.fr/assets/uploads/2021/07/PPPolicy_2021_3-June.pdf.

Suggested Citation:"Appendix B: COSPAR Planetary Protection Requirements for Category I and Category II Missions." National Academies of Sciences, Engineering, and Medicine. 2023. Planetary Protection Considerations for Missions to Solar System Small Bodies: Report Series—Committee on Planetary Protection. Washington, DC: The National Academies Press. doi: 10.17226/26714.
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The ultimate goal of planetary protection for outbound missions is to prevent harmful contamination that would inhibit future measurements designed to search for evidence of the existence or evolution of extraterrestrial life. Preventing harmful contamination is achieved by following specific guidelines based on existing scientific knowledge about the destination and the type of mission. This report responds to NASA's request for a study on planetary protection categorization of missions to small bodies, including whether there are particular populations of small bodies for which contamination of one object in the population would not be likely to have a tangible effect on the opportunities for scientific investigation using other objects in the population. In addressing NASA's request, the authoring committee considered surface composition of target bodies and their importance for prebiotic chemistry, along with size of the small-body populations, the current state of knowledge on the types of objects, the likelihood of a future scientific mission returning to any specific object, active object surface processes, and the size.

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