Mars Sample Return Strategic Approach to Backward Planetary Protection
No abstract provided
Salvo, Chris↗
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Results for “Sample Return”
Search indexed NASA NTRS and DOE OSTI research on propulsion, heat transfer, battery materials and energy systems. Follow report and document links to the original sources.
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Considerations for the Mars Sample Return Containment Facility
No abstract provided
McCubbin, Francis↗
Assessing Relay Communications for Mars Sample Return Surface Mission Concepts
No abstract provided
Lee, Charles↗
Particle Transport Analyses and Testing for the Prevention of Terrestrial-Borne Contamination of the Return Samples on NASA’s Mars 2020 Mission
No abstract provided
Mikellides, Ioannis G.↗
Mars Sample Return (MSR) Campaign Overview and Key Capabilities
No abstract provided
Salvo, Christopher G.↗
3-D Printed Hybrid Propulsion Solutions for SmallSat Lunar Landing and Sample Return
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Stephen A Whitmore↗
Rover Relocalization for Mars Sample Return by Virtual Template Synthesis and Matching
No abstract provided
Detry, Renaud↗
Progress Toward Evaluating Roughness-Resolved Aerothermodynamic Simulations for the Mars Sample Return Earth Entry System
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Ali Reza Mazaheri↗
Rover Relocalization for Mars Sample Return by Virtual Template Synthesis and Matching
No abstract provided
Detry, Renaud↗
The First Returned Samples From A C-Type Asteroid Show Kinship to the Chemically Most Primitive Meteorites
Bulk chemical and isotopic compositions, and mineralogy in the asteroid (162173) Ryugu samples show that Ryugu is mainly composed of materials related to the CI (Ivuna-like) carbonaceous chondrite group. The samples consist predominantly of minerals produced by aqueous alteration in a parent planetesimal from which Ryugu was derived. The 53Mn-53Cr systematics of dolomite suggest that this alteration occurred 5.2 (+0.7/–0.8) million years after formation of Ca-Al-rich inclusions, the first solids formed in the Solar System. The aqueous alteration temperature at the time dolomite and magnetite coprecipitated was 37±10°C. Unlike in CI chondrites, phyllosilicates in Ryugu have lost most of their interlayer water, but retained structural water. This indicates that following aqueous alteration the Ryugu samples avoided heating above ~90°C.
Tetsuya Yokoyama↗
Mars 2020 Perseverance & Mars Sample Return
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George Tahu↗
Mars Sample Return (MSR)
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Jeff Gramling↗
Mars Sample Return - Earth Entry System
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Zion Young↗
Sampling By the NASA Perserverance Rover for Mars Sample Return
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C D K Herd↗