TY - JOUR
T1 - Characterization of Temporarily Captured Minimoon 2020 CD3by Keck Time-resolved Spectrophotometry
AU - Bolin, Bryce T.
AU - Fremling, Christoffer
AU - Holt, Timothy R.
AU - Hankins, Matthew J.
AU - Ahumada, Tomás
AU - Anand, Shreya
AU - Bhalerao, Varun
AU - Burdge, Kevin B.
AU - Copperwheat, Chris M.
AU - Coughlin, Michael
AU - Deshmukh, Kunal P.
AU - De, Kishalay
AU - Kasliwal, Mansi M.
AU - Morbidelli, Alessandro
AU - Purdum, Josiah N.
AU - Quimby, Robert
AU - Bodewits, Dennis
AU - Chang, Chan Kao
AU - Ip, Wing Huen
AU - Hsu, Chen Yen
AU - Laher, Russ R.
AU - Lin, Zhong Yi
AU - Lisse, Carey M.
AU - Masci, Frank J.
AU - Ngeow, Chow Choong
AU - Tan, Hanjie
AU - Zhai, Chengxing
AU - Burruss, Rick
AU - Dekany, Richard
AU - Delacroix, Alexandre
AU - Duev, Dmitry A.
AU - Graham, Matthew
AU - Hale, David
AU - Kulkarni, Shrinivas R.
AU - Kupfer, Thomas
AU - Mahabal, Ashish
AU - Mróz, Przemyslaw J.
AU - Neill, James D.
AU - Riddle, Reed
AU - Rodriguez, Hector
AU - Smith, Roger M.
AU - Soumagnac, Maayane T.
AU - Walters, Richard
AU - Yan, Lin
AU - Zolkower, Jeffry
N1 - Publisher Copyright:
© 2020. The American Astronomical Society. All rights reserved.
PY - 2020/9/10
Y1 - 2020/9/10
N2 - We present time-resolved visible spectrophotometry of 2020 CD3, the second known minimoon. The spectrophotometry was taken with the Keck I/Low Resolution Imaging Spectrometer between wavelengths 434 and 912 nm in the B, g, V, R, I, and RG850 filters as it was leaving the Earth-Moon system on 2020 March 23 UTC. The spectrum of 2020 CD3 resembles V-type asteroids and some lunar rock samples with a 434-761 nm reddish slope of ∼18%/100 nm (g-r = 0.62 ± 0.08 and r-i = 0.21 ± 0.06) with an absorption band at ∼900 nm corresponding to i-z = -0.54 ± 0.10. Combining our measured H of 31.9 ± 0.1 with an albedo of 0.35 typical for V-type asteroids, we determine 2020 CD3's diameter to be ∼0.9 ± 0.1 m, making it the first minimoon and one of the smallest asteroids to be spectrally studied. We use our time-series photometry to detect significant periodic light-curve variations with a period of ∼573 s and amplitude of ∼1. In addition, we extend the observational arc of 2020 CD3 to 37 days, to 2020 March 23 UTC. From the improved orbital solution for 2020 CD3, we estimate the likely duration of its capture to be ∼2 yr and the nongravitational perturbation on its orbit due to radiation pressure with an area-to-mass ratio of (6.9 ± 2.4) × 10-4 m2 kg-1 implying a density of 2.3 ± 0.8 g cm-3, broadly compatible with other meter-scale asteroids and lunar rock. We searched for prediscovery detections of 2020 CD3 in the Zwicky Transient Facility archive as far back as 2018 October but were unable to locate any positive detections.
AB - We present time-resolved visible spectrophotometry of 2020 CD3, the second known minimoon. The spectrophotometry was taken with the Keck I/Low Resolution Imaging Spectrometer between wavelengths 434 and 912 nm in the B, g, V, R, I, and RG850 filters as it was leaving the Earth-Moon system on 2020 March 23 UTC. The spectrum of 2020 CD3 resembles V-type asteroids and some lunar rock samples with a 434-761 nm reddish slope of ∼18%/100 nm (g-r = 0.62 ± 0.08 and r-i = 0.21 ± 0.06) with an absorption band at ∼900 nm corresponding to i-z = -0.54 ± 0.10. Combining our measured H of 31.9 ± 0.1 with an albedo of 0.35 typical for V-type asteroids, we determine 2020 CD3's diameter to be ∼0.9 ± 0.1 m, making it the first minimoon and one of the smallest asteroids to be spectrally studied. We use our time-series photometry to detect significant periodic light-curve variations with a period of ∼573 s and amplitude of ∼1. In addition, we extend the observational arc of 2020 CD3 to 37 days, to 2020 March 23 UTC. From the improved orbital solution for 2020 CD3, we estimate the likely duration of its capture to be ∼2 yr and the nongravitational perturbation on its orbit due to radiation pressure with an area-to-mass ratio of (6.9 ± 2.4) × 10-4 m2 kg-1 implying a density of 2.3 ± 0.8 g cm-3, broadly compatible with other meter-scale asteroids and lunar rock. We searched for prediscovery detections of 2020 CD3 in the Zwicky Transient Facility archive as far back as 2018 October but were unable to locate any positive detections.
UR - http://www.scopus.com/inward/record.url?scp=85091827843&partnerID=8YFLogxK
U2 - 10.3847/2041-8213/abae69
DO - 10.3847/2041-8213/abae69
M3 - 期刊論文
AN - SCOPUS:85091827843
SN - 2041-8205
VL - 900
JO - Astrophysical Journal Letters
JF - Astrophysical Journal Letters
IS - 2
M1 - L45
ER -