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dc.date.accessioned |
2008-09-06T11:02:22Z |
|
dc.date.available |
2008-09-06T11:02:22Z |
|
dc.date.issued |
2005-10 |
|
dc.identifier.citation |
Science, Vol. 310, No. 5746, pp. 265 - 269 |
en |
dc.identifier.issn |
0036-8075 |
|
dc.identifier.uri |
http://hdl.handle.net/2248/3415 |
|
dc.description |
Restricted Access |
en |
dc.description.abstract |
On 4 July 2005, many observatories around the world and in space observed the collision of Deep Impact with comet 9P/Tempel 1 or its aftermath. This was an unprecedented coordinated observational campaign. These data show that (i) there was new material after impact that was compositionally different from that seen before impact; (ii) the ratio of dust mass to gas mass in the ejecta was much larger than before impact; (iii) the new activity did not last more than a few days, and by 9 July the comet's behavior was indistinguishable from its pre-impact behavior; and (iv) there were interesting transient phenomena that may be correlated with cratering physics. |
en |
dc.language.iso |
en |
en |
dc.publisher |
Science |
en |
dc.relation.uri |
http://dx.doi.org/10.1126/science.1118978 |
en |
dc.subject |
Deep Impact |
en |
dc.subject |
Comet |
en |
dc.subject |
Dust Mass |
en |
dc.subject |
Cratering Physics |
en |
dc.title |
Deep Impact: Observations from a Worldwide Earth-Based Campaign |
en |
dc.type |
Article |
en |