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EPOXI at Comet Hartley 2

Authors :
A'Hearn, Michael F
Belton, Michael J. S
Delamere, W. Alan
Feaga, Lori M
Hampton, Donald
Kissel, Jochen
Klaasen, Kenneth P
McFadden, Jessica M
Meech, Karen J
Melosh, H. Jay
Schultz, Peter H
Sunshine, Jessica M
Thomas, Peter C
Veverka, Joseph
Wellnitz, Dennis D
Yeomans, Donald K
Besse, Sebastien
Bodewits, Dennis
Bowling, Timothy J
Carcish, Brian T
Collins, Steven M
Farnham, Tony F
Groussin, Oliver
Hermalyn, Brendan
Kelley, Michael S
Publication Year :
2011
Publisher :
United States: NASA Center for Aerospace Information (CASI), 2011.

Abstract

Understanding how comets work, i,e., what drives their activity, is crucial to using comets to study the early solar system. EPOXI flew past comet 103P/Hartley 2, one with an unusually small but very active nucleus. taking both images and spectra. Unlike large, relatively inactive nuclei, this nncleus is outgassing primarily due to CO2, which drags chnnks of ice out of the nnclens. It also shows significant differences in the relative abundance of volatiles from various parts of the nucleus.

Subjects

Subjects :
Astronomy

Details

Language :
English
Database :
NASA Technical Reports
Notes :
NM0711002, , NNM07AA99C
Publication Type :
Report
Accession number :
edsnas.20110015409
Document Type :
Report