A Comet Active Beyond the Crystallization Zone
arXiv:1709.10079 · doi:10.3847/2041-8213/aa88b4
Abstract
We present observations showing in-bound long-period comet C/2017 K2 (PANSTARRS) to be active at record heliocentric distance. Nucleus temperatures are too low (60 K to 70 K) either for water ice to sublimate or for amorphous ice to crystallize, requiring another source for the observed activity. Using the Hubble Space Telescope we find a sharply-bounded, circularly symmetric dust coma 10 km in radius, with a total scattering cross section of 10 km. The coma has a logarithmic surface brightness gradient -1 over much of its surface, indicating sustained, steady-state dust production. A lack of clear evidence for the action of solar radiation pressure suggests that the dust particles are large, with a mean size 0.1 mm. Using a coma convolution model, we find a limit to the apparent magnitude of the nucleus 25.2 (absolute magnitude 12.9). With assumed geometric albedo = 0.04, the limit to the nucleus circular equivalent radius is 9 km. Pre-discovery observations from 2013 show that the comet was also active at 23.7 AU heliocentric distance. While neither water ice sublimation nor exothermic crystallization can account for the observed distant activity, the measured properties are consistent with activity driven by sublimating supervolatile ices such as CO, CO, O and N. Survival of supervolatiles at the nucleus surface is likely a result of the comet's recent arrival from the frigid Oort cloud.
20 pages, 3 figures, 2 tables, published on Astrophysical Journal Letters, 847:L19 (5pp), 2017 October 1
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