TY - JOUR
T1 - Contemporaneous multiwavelength and precovery observations of the active centaur P/2019 LD2 (ATLAS)
AU - Kareta, Theodore
AU - Woodney, Laura M.
AU - Schambeau, Charles
AU - Fernandez, Yanga
AU - Pinto, Olga Harrington
AU - Wierzchos, Kacper
AU - Womack, M.
AU - Bus, S. J.
AU - Steckloff, Jordan
AU - Sarid, Gal
AU - Volk, Kathryn
AU - Harris, Walter M.
AU - Reddy Kanupuru, Vishnu V
N1 - Publisher Copyright:
© 2021. The Author(s). Published by the American Astronomical Society.
PY - 2021/4
Y1 - 2021/4
N2 - The Gateway Centaur and Jupiter co-orbital P/2019 LD2 (ATLAS) provides the first opportunity to observe the migration of a solar system small body from a Centaur orbit to a Jupiter Family Comet (JFC) four decades from now. The Gateway transition region is beyond where water ice can power cometary activity, and coma production there is as poorly understood as in all Centaurs. We present contemporaneous multiwavelength observations of LD2 from 2020 July 2–4: Gemini North visible imaging, NASA IRTF near-infrared spectroscopy, and ARO Submillimeter Telescope millimeter-wavelength spectroscopy. Precovery DECam images limit the nucleus’s effective radius to ≤1.2 km and no large outbursts were seen in archival Catalina Sky Survey observations. LD2's coma has g¢ - r¢ = 0.70 ± 0.07, r¢ - i¢ = 0.26 ± 0.07, a dust-production rate of ∼10–20 kg s-1, and an outflow velocity between v ∼ 0.6–3.3 m s-1. We did not detect CO toward LD2 on 2020 July 2–3, with a 3σ upper limit of Q(CO) < 4.4 × 1027 mol s-1 (≲ 200 kg s-1). Near-infrared spectra show evidence for water ice at the 1%–10% level depending on grain size. Spatial profiles and archival data are consistent with sustained activity. The evidence supports the hypothesis that LD2 is a typical small Centaur that will become a typical JFC, and thus, it is critical to understanding the transition between these two populations. Finally, we discuss potential strategies for a community-wide, long-baseline monitoring effort.
AB - The Gateway Centaur and Jupiter co-orbital P/2019 LD2 (ATLAS) provides the first opportunity to observe the migration of a solar system small body from a Centaur orbit to a Jupiter Family Comet (JFC) four decades from now. The Gateway transition region is beyond where water ice can power cometary activity, and coma production there is as poorly understood as in all Centaurs. We present contemporaneous multiwavelength observations of LD2 from 2020 July 2–4: Gemini North visible imaging, NASA IRTF near-infrared spectroscopy, and ARO Submillimeter Telescope millimeter-wavelength spectroscopy. Precovery DECam images limit the nucleus’s effective radius to ≤1.2 km and no large outbursts were seen in archival Catalina Sky Survey observations. LD2's coma has g¢ - r¢ = 0.70 ± 0.07, r¢ - i¢ = 0.26 ± 0.07, a dust-production rate of ∼10–20 kg s-1, and an outflow velocity between v ∼ 0.6–3.3 m s-1. We did not detect CO toward LD2 on 2020 July 2–3, with a 3σ upper limit of Q(CO) < 4.4 × 1027 mol s-1 (≲ 200 kg s-1). Near-infrared spectra show evidence for water ice at the 1%–10% level depending on grain size. Spatial profiles and archival data are consistent with sustained activity. The evidence supports the hypothesis that LD2 is a typical small Centaur that will become a typical JFC, and thus, it is critical to understanding the transition between these two populations. Finally, we discuss potential strategies for a community-wide, long-baseline monitoring effort.
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U2 - 10.3847/PSJ/abe23d
DO - 10.3847/PSJ/abe23d
M3 - Review article
AN - SCOPUS:85114730016
SN - 2632-3338
VL - 2
JO - Planetary Science Journal
JF - Planetary Science Journal
IS - 2
M1 - abe23d
ER -