GAIA DATA RELEASE 3: ANALYSIS OF REFLECTANCE SPECTRA OF NEAR-EARTH ASTEROIDS AND MARS-CROSSERS
Authors:
1.
Sternberg Astronomical Institute, Moscow State University
Institute of Astronomy (INASAN)
Institute of Astronomy (INASAN)
2.
Institute of Astronomy (INASAN)
Type:
Сonference article
Published:
27.12.2024
Subject area:
52
53
520
521
523
524
52-1
52-6
41.00
29.35
29.31
29.33
29.27
29.05
03.06.01
03.05.01
03.04.03
2
223
614
6135
SCI004000
SCI005000
53
520
521
523
524
52-1
52-6
41.00
29.35
29.31
29.33
29.27
29.05
03.06.01
03.05.01
03.04.03
2
223
614
6135
SCI004000
SCI005000
Language:
English
Keywords:
astronomical databases: Gaia Data Release 3; asteroids: Near-Earth Asteroids, Mars-crossers
Abstract (English):
Since July 2014, the European Space Agency (ESA) Gaia mission has been observing objects in the Solar System as part of its various scientific missions. The third data release (DR3) includes observations of more than 150,000 objects, including asteroids. Analysis of Gaia asteroid reflectance spectra has allowed for the first time to determine spectral types for many objects and to confirm or refine previously determined classes. The distribution of spectral groups coincides with the analysis of ground-based observations performed by other authors, with a sample overlap of less than 20 %. The main groups include the S-group ($\sim$60 %) and the C-group ($\sim$20—25 %). Mars-crossing objects are slightly more likely to have mixed mineralogy. This distribution remains constant over different ranges of object diameters. Analysis of the distribution of spectral groups by semi-major axis and perihelion distance may serve as indirect evidence for the prevalence of sublimation-dust activity in primitive asteroids.
Since July 2014, the European Space Agency (ESA) Gaia mission has been observing objects in the Solar System as part of its various scientific missions. The third data release (DR3) includes observations of more than 150,000 objects, including asteroids. Analysis of Gaia asteroid reflectance spectra has allowed for the first time to determine spectral types for many objects and to confirm or refine previously determined classes. The distribution of spectral groups coincides with the analysis of ground-based observations performed by other authors, with a sample overlap of less than 20 %. The main groups include the S-group ($\sim$60 %) and the C-group ($\sim$20—25 %). Mars-crossing objects are slightly more likely to have mixed mineralogy. This distribution remains constant over different ranges of object diameters. Analysis of the distribution of spectral groups by semi-major axis and perihelion distance may serve as indirect evidence for the prevalence of sublimation-dust activity in primitive asteroids.
Keywords:
astronomical databases: Gaia Data Release 3; asteroids: Near-Earth Asteroids, Mars-crossers
astronomical databases: Gaia Data Release 3; asteroids: Near-Earth Asteroids, Mars-crossers
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