Observations of Disintegrating Long-Period Comet C/2019 Y4 (ATLAS) -- A Sibling of C/1844 Y1 (Great Comet)
arXiv:2004.10990 · doi:10.3847/1538-3881/ab9d81
Abstract
We present a study of C/2019 Y4 (ATLAS) using Sloan observations from mid-January to early April 2020. During this timespan, the comet brightened with a growth in the effective cross-section of m s from the beginning to 70 d preperihelion in late March 2020, followed by a brightness fade and the comet gradually losing the central condensation. Meanwhile, the comet became progressively bluer, and was even bluer than the Sun () when the brightness peaked, likely due to activation of subterranean fresh volatiles exposed to sunlight. With the tailward-bias corrected astrometry we found an enormous radial nongravitational parameter, au d in the heliocentric motion of the comet. Taking all of these finds into consideration, we conclude that the comet has disintegrated since mid-March 2020. By no means was the split new to the comet, as we quantified that the comet had undergone another split event around last perihelion 5 kyr ago, during which its sibling C/1844 Y1 (Great Comet) was produced, with the in-plane component of the separation velocity 1 m s. We constrained that the nucleus of C/2019 Y4 before disintegration was 60 m in radius, and has been protractedly ejecting dust grains of 10-40 m (assuming dust bulk density 0.5 g cm) with ejection speed 30 m s in early March 2020 and increased to 80 m s towards the end of the month for grains of 10 m.
Accepted to Astronomical Journal; 9 figures, 4 tables
References in corpus (3)
Cited by in corpus (6)
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