Observations of Disintegrating Long-period Comet C/2019 Y4 (ATLAS): A Sibling of C/1844 Y1 (Great Comet)

摘要

We present a study of C/2019 Y4 (ATLAS) using Sloan gri observations from 2020 mid-January to early April. During this time span, the comet brightened with a growth in the effective cross-section of 2.0 0.1 10 ? ′ 2 ( ) m2 s ?1 from the beginning to ～70 days preperihelion in late 2020 March, 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 (g ? r ≈ 0.2) 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, =+ ? ′ - A1 2.25 0.13 10 7 ( ) au day?2 in the heliocentric motion of the comet. Taking all of these findings into consideration, we conclude that the comet has disintegrated since 2020 mid-March. 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 ?1ms?1 . 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 μm (assuming a dust bulk density of 0.5 g cm?3 ) with an ejection speed of ～30 m s?1 in early 2020 March and increased to ～80 m s?1 toward the end of the month for grains of ～10 μm.