The global shape, density and rotation of Comet 67P/Churyumov-Gerasimenko from preperihelion Rosetta/OSIRIS observations
By L. Jorda, R. Gaskell, C. Capanna, S. Hviid, P. Lamy, Josef Durech, G. Faury, O. Groussin, P. Gutiérrez, C. Jackman and 38 more. 2016
274 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/e7bb1fee9915b490906c5ca0859c603caf92ef2e
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In Astronomy and Astrophysics
- Anders Johansen
- B. Gundlach
- J. Blum
- Jean-Loup Bertaux
- G. Kovacs
- Stefano Mottola
- Nicolas Gonzalez Thomas
- Matteo Massironi
In Nuclear and High Energy Physics
Citations in the corpus
- Evidence for the formation of comet 67P/Churyumov-Gerasimenko through gravitational collapse of a bound clump of pebbles (2017, methodology): “We approximated the shape and orientation of 67P by a digital terrain model with 5000 facets (Jorda et al. 2016) and its real obliquity (Acton 1996) as well as by a 1000-facet sphere with an effective radius of 1.65 km and a rotation axis perpendicular to the orbital plane.”
- The primordial nucleus of comet 67P/Churyumov-Gerasimenko (2015, methodology): “The dimensions of the large lobe is 4.10 × 3.52 × 1.63 km and the small lobe measures 2.5×2.14×1.64 km (Jorda et al. 2016).”