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| dc.contributor.author | Burton, M. G | |
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| dc.contributor.author | Cabanac, R | |
| dc.contributor.author | Campbell, R | |
| dc.contributor.author | Campins, H | |
| dc.contributor.author | Capria, M. T | |
| dc.contributor.author | Jackson, W | |
| dc.contributor.author | Carroll, T | |
| dc.contributor.author | Chaffee, F | |
| dc.contributor.author | Charnley, S. B | |
| dc.contributor.author | Lovell, A. J | |
| dc.contributor.author | Cleis, R | |
| dc.contributor.author | Coates, A | |
| dc.contributor.author | Cochran, A | |
| dc.contributor.author | Colom, P | |
| dc.contributor.author | Conrad, A | |
| dc.contributor.author | Coulson, I. M | |
| dc.contributor.author | Jehin, E | |
| dc.contributor.author | Crovisier, J | |
| dc.contributor.author | deBuizer, J | |
| dc.contributor.author | Dekany, R | |
| dc.contributor.author | de Léon, J | |
| dc.contributor.author | Lowry, S. C | |
| dc.contributor.author | Dello Russo, N | |
| dc.contributor.author | Delsanti, A | |
| dc.contributor.author | DiSanti, M | |
| dc.contributor.author | Drummond, J | |
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| dc.contributor.author | Etzel, P. B | |
| 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 |