DENSITY AND CHARGE OF PRISTINE FLUFFY PARTICLES FROM COMET 67P/CHURYUMOV–GERASIMENKO
By M. Fulle, V. Corte, A. Rotundi, P. Weissman, A. Juhász, K. Szego, R. Sordini, M. Ferrari, S. Ivanovski, F. Lucarelli and 31 more. 2015
144 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics
View Paper: https://www.semanticscholar.org/paper/f82745851f95d0bb681e431282a2d2ef1fbe44ad
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In Astronomy and Astrophysics
- Anders Johansen
- B. Gundlach
- J. Blum
- Jean-Loup Bertaux
- Stefano Mottola
- Gabriele Cremonese
- H. Rickman
- F. Rietmeijer
Citations in the corpus
- EVOLUTION OF THE DUST SIZE DISTRIBUTION OF COMET 67P/CHURYUMOV–GERASIMENKO FROM 2.2 au TO PERIHELION (2016, background): “…density between the two populations: fluffy particles have densities even lower than 1 kg m−3, and have always been detected as short-lasting showers of single detections, resulting from the fragmentation of fragile parents that interact with the spacecraft’s electric field (Fulle et al. 2015).”
- Evidence for the formation of comet 67P/Churyumov-Gerasimenko through gravitational collapse of a bound clump of pebbles (2017, methodology): “0.001 (comprising ∼1% of the total mass, but consequently a much larger share of the volume of the comet nucleus) by the Rosetta/GIADA instrument (Fulle et al. 2015) and the discovery of a fractal particle by the Rosetta/MIDAS instrument (Mannel et al. 2016) unambiguously show that the comet never…”