Evidence of sub-surface energy storage in comet 67P from the outburst of 2016 July 03

Agarwal, J., Della Corte, V., Feldman, P. D., Geiger, B., Merouane, S., Bertini, I., Bodewits, D., Fornasier, S., Grün, E., Hasselmann, P., and others. Hilchenbach, M., Höfner, S., Ivanovski, S., Kolokolova, L., Pajola, M., Rotundi, A., Sierks, H., Steffl, A. J., Thomas, N., A'Hearn, M. F., Barbieri, C., Barucci, M. A., Bertaux, J.-L., Boudreault, S., Cremonese, G., Da Deppo, V., Davidsson, B., Debei, S., De Cecco, M., Deller, J. F., Feaga, L. M., Fischer, H., Fulle, M., Gicquel, A., Groussin, O., Güttler, C., Gutiérrez, P. J., Hofmann, M., Hornung, K., Hviid, S. F., Ip, W.-H., Jorda, L., Keller, H. U., Kissel, J., Knollenberg, J., Koch, A., Koschny, D., Kramm, J.-R., Kührt, E., Küppers, M., Lamy, P. L., Langevin, Y., Lara, L. M., Lazzarin, M., Lin, Z.-Y., Lopez Moreno, J. J., Lowry, S. C., Marzari, F., Mottola, S., Naletto, G., Oklay, N., Parker, J. Wm., Rodrigo, R., Rynö, J., Shi, X., Stenzel, O., Tubiana, C., Vincent, J.-B., Weaver, H. A., and Zaprudin, B. (hide) (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 . s606-s625. ISSN 0035-8711. (doi:10.1093/mnras/stx2386)

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:	12 Jul 2019 08:37 UTC
Resource URI:	https://kar.kent.ac.uk/id/eprint/65125 (The current URI for this page, for reference purposes)