Bolin, BT, Fernandez, YR, Lisse, CM, Holt, TR, Lin, Z-Y, Purdum, JN, Deshmukh, KP, Bauer, JM, Bellm, EC, Bodewits, D, Burdge, KB, Carey, SJ, Copperwheat, CM, Helou, G, Ho, AYQ, Horner, J, van Roestel, J, Bhalerao, V, Chang, C-K, Chen, C et al, Hsu, C-Y, Ip, W-H, Kasliwal, MM, Masci, FJ, Ngeow, C-C, Quimby, R, Burruss, R, Coughlin, M, Dekany, R, Delacroix, A, Drake, A, Duev, DA, Graham, M, Hale, D, Kupfer, T, Laher, RR, Mahabal, A, Mroz, PJ, Neill, JD, Riddle, R, Rodriguez, H, Smith, RM, Soumagnac, MT, Walters, R, Yan, L and Zolkower, J (2021) Initial Characterization of Active Transitioning Centaur, P/2019 LD2 (ATLAS), Using Hubble, Spitzer, ZTF, Keck, Apache Point Observatory, and GROWTH Visible and Infrared Imaging and Spectroscopy. ASTRONOMICAL JOURNAL, 161 (3). ISSN 0004-6256

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Abstract

We present visible and mid-infrared imagery and photometry of temporary Jovian co-orbital comet P/2019 LD2 taken with Hubble Space Telescope/Wide Field Camera 3 (HST/WFC3), Spitzer Space Telescope/Infrared Array Camera (Spitzer/IRAC), and the GROWTH telescope network, visible spectroscopy from Keck/Low-Resolution Imaging Spectrometer (LRIS), and archival Zwicky Transient Facility observations taken between 2019 April and 2020 August. Our observations indicate that the nucleus of LD2 has a radius between 0.2 and 1.8 km assuming a 0.08 albedo and a coma dominated by ∼100 μm-scale dust ejected at ∼1 m s−1 speeds with a ∼1′ jet pointing in the southwest direction. LD2 experienced a total dust mass loss of ∼108 kg at a loss rate of ∼6 kg s−1 with Afρ/cross section varying between ∼85 cm/125 km2 and ∼200 cm/310 km2 from 2019 April 9 to 2019 November 8. If the increase in Afρ/cross section remained constant, it implies LD2's activity began ∼2018 November when within 4.8 au of the Sun, implying the onset of H2O sublimation. We measure CO/CO2 gas production of ≲1027 mol s−1/≲1026 mol s−1 from our 4.5 μm Spitzer observations; g–r = 0.59 ± 0.03, r–i = 0.18 ± 0.05, and i–z = 0.01 ± 0.07 from GROWTH observations; and H2O gas production of ≲80 kg s−1 scaling from our estimated C2 production of ${Q}_{{C}_{2}}\lesssim 7.5\times {10}^{24}$ mol s−1 from Keck/LRIS spectroscopy. We determine that the long-term orbit of LD2 is similar to Jupiter-family comets having close encounters with Jupiter within ∼0.5 Hill radius in the last ∼3 y and within 0.8 Hill radius in ∼9 y. Additionally, 78.8% of our orbital clones are ejected from the solar system within 1 × 106 yr, having a dynamical half-life of 3.4 × 105 yr.

Item Type:	Article
Uncontrolled Keywords:	Astronomy & Astrophysics; Physical Sciences; Science & Technology; Science & Technology; Physical Sciences; Astronomy & Astrophysics; Astronomy & Astrophysics; 0201 Astronomical and Space Sciences
Subjects:	Q Science > QB Astronomy
Divisions:	Astrophysics Research Institute
Publisher:	IOP PUBLISHING LTD
SWORD Depositor:	A Symplectic
Date Deposited:	31 Oct 2022 16:29
Last Modified:	31 Oct 2022 16:30
DOI or ID number:	10.3847/1538-3881/abd94b
URI:	https://researchonline.ljmu.ac.uk/id/eprint/17982

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