Active Asteroid P/2017 S5 (ATLAS)
Active Asteroid P/2017 S5 (ATLAS)
复制标题
活跃小行星 P/2017 S5 (ATLAS)
DOI:
10.3847/1538-3881/aaf563
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发表时间:
2018
期刊:
影响因子:
--
通讯作者:
S. Larson
中科院分区:
文献类型:
--
作者:
D. Jewitt;Yoonyoung Kim;J. Rajagopal;S. Ridgway;R. Kotulla;Wilson M. Liu;M. Mutchler;Jing Li;H. Weaver;S. Larson
Observations of active asteroid P/2017 S5 when near perihelion reveal the ejection of large (102–104 μm) particles at 0.2–2 m s−1 speeds, with estimated mass-loss rates of a few kg s−1. The protracted nature of the mass loss (continuous over ∼150 days) is compatible with a sublimation origin, meaning that this object is likely an ice-bearing main-belt comet. Equilibrium sublimation of exposed water ice covering as little as 0.1 km2 can match the data. Observations a year after perihelion show the object in an inactive state from which we deduce a nucleus effective radius (albedo 0.06 ± 0.02 assumed). The gravitational escape speed from a body of this size is just ∼0.3 m s−1, comparable to the inferred ejection speed of the dust. Time-series photometry provides tentative evidence for rapid rotation (lightcurve period 1.4 hr) that may also play a role in the loss of mass and which, if real, is a likely consequence of spin-up by sublimation torques. P/2017 S5 shares both physical and orbital similarities with the split active asteroid pair P/2016 J1-A and J1-B, and all three objects are likely members of the ∼7 Myr old, collisionally produced, Theobalda family.
影响因子:
5.3
作者:
Hsieh, Henry H.;Jewitt, David;Ishiguro, Masateru
通讯作者:
Ishiguro, Masateru
影响因子:
5.3
作者:
Blanton, Michael R.;Bershady, Matthew A.;Zou, Hu
通讯作者:
Zou, Hu