Comet 67P/Churyumov-Gerasimenko sheds dust coat accumulated over the past four years - INSU - Institut national des sciences de l'Univers Access content directly
Journal Articles Nature Year : 2015

Comet 67P/Churyumov-Gerasimenko sheds dust coat accumulated over the past four years

Rita Schulz
  • Function : Author
Jochen Kissel
  • Function : Author
Johan Silen
  • Function : Author
Klaus Hornung
  • Function : Author
Anaïs Bardyn
  • Function : Author
Henning Fischer
  • Function : Author
Harry Lehto
  • Function : Author
Léna Le Roy
Jouni Rynö
Sandra Siljeström
  • Function : Author
Kurt Varmuza
  • Function : Author
Boris Zaprudin
  • Function : Author


Comets are composed of dust and frozen gases. The ices are mixed with the refractory material either as an icy conglomerate1, or as an aggregate of pre-solar grains (grains that existed prior to the formation of the Solar System), mantled by an ice layer2, 3. The presence of water-ice grains in periodic comets is now well established4, 5, 6. Modelling of infrared spectra obtained about ten kilometres from the nucleus of comet Hartley 2 suggests that larger dust particles are being physically decoupled from fine-grained water-ice particles that may be aggregates7, which supports the icy-conglomerate model. It is known that comets build up crusts of dust that are subsequently shed as they approach perihelion8, 9, 10. Micrometre-sized interplanetary dust particles collected in the Earth’s stratosphere and certain micrometeorites are assumed to be of cometary origin11, 12, 13. Here we report that grains collected from the Jupiter-family comet 67P/Churyumov-Gerasimenko come from a dusty crust that quenches the material outflow activity at the comet surface14. The larger grains (exceeding 50 micrometres across) are fluffy (with porosity over 50 per cent), and many shattered when collected on the target plate, suggesting that they are agglomerates of entities in the size range of interplanetary dust particles. Their surfaces are generally rich in sodium, which explains the high sodium abundance in cometary meteoroids15. The particles collected to date therefore probably represent parent material of interplanetary dust particles. This argues against comet dust being composed of a silicate core mantled by organic refractory material and then by a mixture of water-dominated ices2, 3. At its previous recurrence (orbital period 6.5 years), the comet’s dust production doubled when it was between 2.7 and 2.5 astronomical units from the Sun14, indicating that this was when the nucleus shed its mantle. Once the mantle is shed, unprocessed material starts to supply the developing coma, radically changing its dust component, which then also contains icy grains, as detected during encounters with other comets closer to the Sun4, 5.
No file

Dates and versions

insu-01182128 , version 1 (30-07-2015)



Rita Schulz, Martin Hilchenbach, Yves Langevin, Jochen Kissel, Johan Silen, et al.. Comet 67P/Churyumov-Gerasimenko sheds dust coat accumulated over the past four years. Nature, 2015, 518 (7538), pp.216-218. ⟨10.1038/nature14159⟩. ⟨insu-01182128⟩
295 View
0 Download



Gmail Facebook X LinkedIn More