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Presentation
Asteroid sample return missions: Sample Analysis of Returned Sample by OSIRIS-REx
Japan Geoscience Union - American Geophysical Union Joint Meeting 2017 (2017)
  • Harold C. Connolly, Rowan University
  • Scott Messenger, Washington University in St. Louis
  • Shogo Tachibana, University of Tokyo
  • Dante S. Lauretta, University of Arizona
Abstract
The Origins Spectral Interpretation, Resource Identification, and Security-Regolith Explorer (OSIRIS-REx) spacecraft launched flawlessly on September 8, 2016, as NASA's third New Frontiers mission. The primary requirement of the OSIRIS-REx mission is to collect and return a pristine sample from the surface of a near-Earth asteroid. OSIRIS-REx will arrive at B-type asteroid (101955) Bennu [1] in August 2018. This asteroid was targeted owing to its spectral similarity to carbonaceous chondrites, appropriate size, and favorable orbit. After detailed geological and spectral mapping, OSIRIS-REx will collect up to 2 kg of surface regolith samples from a carefully-selected site in mid-2020. The surface regolith from Bennu will be pristine samples with a record of the entire history of Bennu from the interstellar medium to the recent dynamical evolution and surface geological processes [2]. The sample return capsule will deliver these samples to the Earth in September 2023.
Publication Date
May 20, 2017
Location
Japan
Citation Information
Harold C. Connolly, Scott Messenger, Shogo Tachibana and Dante S. Lauretta. "Asteroid sample return missions: Sample Analysis of Returned Sample by OSIRIS-REx" Japan Geoscience Union - American Geophysical Union Joint Meeting 2017 (2017)
Available at: http://works.bepress.com/harold-connolly/32/