Investigating Taxonomic Diversity within Asteroid Families through ATLAS Dual-band Photometry

被引:16
作者
Erasmus, N. [1 ]
Navarro-Meza, S. [2 ,3 ]
McNeill, A. [3 ]
Trilling, D. E. [1 ,3 ]
Sickafoose, A. A. [1 ,4 ,5 ]
Denneau, L. [6 ]
Flewelling, H. [6 ]
Heinze, A. [6 ]
Tonry, J. L. [6 ]
机构
[1] South African Astron Observ, ZA-7925 Cape Town, South Africa
[2] Univ Nacl Autonoma Mexico, Inst Astron, Ensenada 22860, BC, Mexico
[3] No Arizona Univ, Dept Astron & Planetary Sci, Flagstaff, AZ 86001 USA
[4] MIT, Dept Earth Atmospher & Planetary Sci, Cambridge, MA 02139 USA
[5] Planetary Sci Inst, Tucson, AZ 85719 USA
[6] Univ Hawaii, Inst Astron, 2680 Woodlawn Dr, Honolulu, HI 96822 USA
基金
美国国家航空航天局; 新加坡国家研究基金会;
关键词
VESTA;
D O I
10.3847/1538-4365/ab5e88
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present here the c-o colors for identified Flora, Vesta, Nysa-Polana, Themis, and Koronis family members within the historic data set (2015-2018) of the Asteroid Terrestrial-impact Last Alert System (ATLAS). The Themis and Koronis families are known to be relatively pure C- and S-type Bus-DeMeo taxonomic families, respectively, and the extracted color data from the ATLAS broadband c- and o-filters of these two families are used to demonstrate that the ATLAS c-o color is a sufficient parameter to distinguish between the C- and S-type taxonomies. The Vesta and NysaPolana families are known to display a mixture of taxonomies possibly due to Vesta's differentiated parent body origin and Nysa-Polana actually consisting of two nested families with differing taxonomies. Our data show that the Flora family also displays a large degree of taxonomic mixing and the data reveal a substantial H-magnitude dependence on color. We propose and exclude several interpretations for the observed taxonomic mix. Additionally, we extract rotation periods of all of the targets reported here and find good agreement with targets that have previously reported periods.
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页数:7
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