On The Evolution Of The Dust Emitted By Comet 103P/Hartley 2 And Observed By EPOXI

Details On The Evolution Of The Dust Emitted By Comet 103P/Hartley 2 And Observed By EPOXI On The Evolution Of The Dust Emitted By Comet 103P/Hartley 2 And Observed By EPOXI

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf..870l&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.870

Physics

Scientific paper

The EPOXI close flyby of comet 103P/Hartley 2 at 13:59 UT on 04 Nov 2010 showed clear evidence for a highly active surface emitting refractory dust and solid ice particles into interplanetary space, with multiple jets emanating from localized spots on the surface (Fig. 1). The evidence included a smooth space-filling coma dust distribution shadowed in regions by the nucleus, as well as a distribution of large individual particles detected as discrete spots and streaks.

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