4.7 Article

Evaluating possible spectroscopic variation of Bennu's sampling site

Journal

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume 519, Issue 1, Pages 1464-1475

Publisher

OXFORD UNIV PRESS
DOI: 10.1093/mnras/stac2969

Keywords

solid state: volatile; space vehicles; techniques: spectroscopic; minor planets, asteroids: individual: Bennu, OSIRIS-REx; planets and satellites: surfaces

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The OSIRIS-REx spacecraft successfully sampled and stored the surface of asteroid Bennu. The sampling maneuver altered the morphology of the sampling site, providing an opportunity to study the subsurface of Bennu in detail. Analysis of the infrared spectrum showed no significant variations in the near-infrared bands, but the sampling site appeared redder and possible modifications were observed in the hydrated band.
The OSIRIS-REx spacecraft completed the first part of the primary objective by successfully sampling the surface of asteroid (101955) Bennu and storing the acquired sample in the re-entry capsule. The sampling 'Touch-And-Go' (TAG) maneuver was performed nominally at the primary sampling site, Nightingale, in Bennu's Northern hemisphere. As a consequence of the TAG, material at the sampling site was mobilized and the morphology of the area was altered. This event offered a unique opportunity to investigate, in detail, the subsurface of asteroid Bennu giving access to fine grained and less altered material from Nightingale crater. We performed a detailed study on the infrared spectrum in the Nightingale region to search for modification resulting from the sampling event by analysing different features: slope, the H2O-OH- related absorption band in the 2.7 mu m region, and other possible features. Our results show that, despite visible alteration of the TAG location detected by cameras, no strong variations are observed in the near-infrared bands and their quantitative evaluation is not possible beyond all the instrumental effects, although some changes may have occurred. We confirm that the infrared spectrum of the sampling site becomes redder with respect to the pre-TAG observations, conceivably due to fine material mobilization and exposure of less altered material, as confirmed by decreased spectral convexity. We identify possible modification of hydrated band at 2.7 mu m but with some concerns due to data quality. However, our results place new constraints on the nature of Bennu's subsurface material and the sample collected by OSIRIS-REx.

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