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  4. Active Asteroid (6478) Gault: A Blue Q-type Surface below the Dust?
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Active Asteroid (6478) Gault: A Blue Q-type Surface below the Dust?

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sword-2020-04-03T17:22:17.original.xml (130 B)
Original SWORD entry document
Journal
Astrophysical Journal Letters
Publisher
American Astronomical Society
Citation
"Active Asteroid (6478) Gault: A Blue Q-type Surface below the Dust?." Astrophysical Journal Letters, 882 (1).
Version
Author's final manuscript
Abstract
© 2019. The American Astronomical Society. All rights reserved.. We present near-infrared spectroscopy of the sporadically active asteroid (6478)Gault collected on the 3 m NASA/Infrared Telescope Facility observatory in late 2019 March/early April. Long-exposure imaging with the 0.5 m Near Earth Environment Monitoring T05 telescope and previously published data simultaneously monitored the asteroid activity, providing context for our measurements. We confirm that Gault is a silicate-rich (Q- or S-type) object likely linked to the (25)Phocaea collisional family. The asteroid exhibits substantial spectral variability over the 0.75-2.45 μm wavelength range, from unusual blue (s′=-13.5 1.1% μm-1) to typical red (s′=+9.1 1.2% μm-1) spectral slope, that does not seem to correlate with activity. Spectral comparisons with samples of ordinary chondrite meteorites suggest that the blue color relates to the partial loss of the asteroid dust regolith, exposing a fresh, dust-free material at its surface. The existence of asteroids rotating close to rotational break-up limit and having similar spectral properties as Gault further supports this interpretation. Future spectroscopic observations of Gault, when the tails dissipate, will help further testing of our proposed hypothesis.
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Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use.
Persistent DSpace Link
https://hdl.handle.net/1721.1/124492
DOI of Published Version
10.3847/2041-8213/AB32EE
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