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Bertaux, J.-R. Kramm, J. Rynoe, J. Wm. Parker, K. Hornung, L. Jorda, L. Kolokolova, L. M. Feaga, L. M. Lara, M. A. Barucci, M. De Cecco, M. F. A'Hearn, M. Fulle, M. Hilchenbach, M. Hofmann, M. Kueppers, M. Lazzarin, M. Pajola, N. Oklay, N. Thomas, O. Groussin, O. Stenzel, P. D. Feldman, P. Hasselmann, P. J. Gutierrez, P. L. Lamy, R. Rodrigo, S. Boudreault, S. C. Lowry, S. Debei, S. F. Hviid, S. Fornasier, S. Hoefner, S. Ivanovski, S. Merouane, S. Mottola, V. Da Deppo, V. Della Corte, W.-H. Ip, X. Shi, Y. Langevin, Z.-Y. Lin","submitted_at":"2017-10-27T16:39:28Z","abstract_excerpt":"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. 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