Agarwal, J., Della Corte, V., Feldman, P. D., Geiger, B., Merouane, S., Bertini, I., Bodewits, D., Fornasier, S., Grün, E., Hasselmann, P., and others. (2017) Evidence of sub-surface energy storage in comet 67P from the outburst of 2016 July 03. Monthly Notices of the Royal Astronomical Society, 469 (sup2). s606-s625. ISSN 0035-8711. (doi:10.1093/mnras/stx2386) (KAR id:65125)
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| Official URL https://doi.org/10.1093/mnras/stx2386 |
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Abstract
On 3 July 2016, several instruments on board ESA’s Rosetta spacecraft detected signs of an outburst event on comet 67P, at a heliocentric distance of 3.32 AU from the sun, outbound from perihelion. We here report on the inferred properties of the ejected dust and the surface change at the site of the outburst. The activity coincided with the local sunrise and continued over a time interval of 14 – 68 minutes. It left a 10m-sized icy patch on the surface. The ejected material comprised refractory grains of several hundred microns in size, and sub-micron-sized water ice grains. The high dust mass production rate is incompatible with the free sublimation of crystalline water ice under solar illumination as the only acceleration process. Additional energy stored near the surface must have increased the gas density. We suggest a pressurized sub-surface gas reservoir, or the crystallization of amorphous water ice as possible causes.
| Item Type: | Article |
|---|---|
| DOI/Identification number: | 10.1093/mnras/stx2386 |
| Subjects: | Q Science > QB Astronomy > QB651 Planets, Minor |
| Divisions: | Faculties > Sciences > School of Physical Sciences > Centre for Astrophysics and Planetary Sciences |
| Depositing User: | Stephen Lowry |
| Date Deposited: | 08 Dec 2017 11:33 UTC |
| Last Modified: | 05 Oct 2020 10:03 UTC |
| Resource URI: | https://kar.kent.ac.uk/id/eprint/65125 (The current URI for this page, for reference purposes) |
| Lowry, S. C.: |  https://orcid.org/0000-0002-5605-4329 |
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