Coma morphology of comet 67P controlled by insolation over irregular nucleus - INSU - Institut national des sciences de l'Univers Access content directly
Journal Articles Nature Astronomy Year : 2018

Coma morphology of comet 67P controlled by insolation over irregular nucleus

Marco Fulle
  • Function : Author
  • PersonId : 980748
Maurizio Pajola
  • Function : Author
  • PersonId : 987591
Dennis Bodewits
  • Function : Author
  • PersonId : 991882
Philippe L. Lamy
Jean-Loup Bertaux
  • Function : Author
  • PersonId : 914210
Gabriele Cremonese
  • Function : Author
  • PersonId : 1005814
Stefano Debei
  • Function : Author
  • PersonId : 1002201
Olivier Groussin
  • Function : Author
  • PersonId : 837612
Pedro J. Gutiérrez
  • Function : Author
  • PersonId : 880386
Wing-Huen Ip
Laurent Jorda
Michael Küppers
Nilda Oklay
  • Function : Author
  • PersonId : 976656
Imre Toth
  • Function : Author
Jean-Baptiste Vincent
  • Function : Author
  • PersonId : 992874


While the structural complexity of cometary comae is already recognizable from telescopic observations1, the innermost region, within a few radii of the nucleus, was not resolved until spacecraft exploration became a reality2,3. The dust coma displays jet-like features of enhanced brightness superposed on a diffuse background1,4,5. Some features can be traced to specific areas on the nucleus, and result conceivably from locally enhanced outgassing and/or dust emission6-8. However, diffuse or even uniform activity over topographic concavity can converge to produce jet-like features9,10. Therefore, linking observed coma morphology to the distribution of activity on the nucleus is difficult11,12. Here, we study the emergence of dust activity at sunrise on comet 67P/Churyumov-Gerasimenko using high-resolution, stereo images from the OSIRIS camera onboard the Rosetta spacecraft, where the sources and formation of the jet-like features are resolved. We perform numerical simulations to show that the ambient dust coma is driven by pervasive but non-uniform water outgassing from the homogeneous surface layer. Physical collimations of gas and dust flows occur at local maxima of insolation and also via topographic focusing. Coma structures are projected to exhibit jet-like features that vary with the perspective of the observer. For an irregular comet such as 67P/Churyumov-Gerasimenko, near-nucleus coma structures can be concealed in the shadow of the nucleus, which further complicates the picture.
No file

Dates and versions

insu-01806355 , version 1 (02-06-2018)



Xian Shi, Xuanyu Hu, Sefano Mottola, Holger Sierks, Horst Uwe Keller, et al.. Coma morphology of comet 67P controlled by insolation over irregular nucleus. Nature Astronomy, 2018, 2, pp.562-567. ⟨10.1038/s41550-018-0481-5⟩. ⟨insu-01806355⟩
208 View
0 Download



Gmail Facebook X LinkedIn More