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25 April 2024
 
  » pubmed » pmid16150977

 Article overview



Deep Impact: observations from a worldwide Earth-based campaign
K J Meech ; N Ageorges ; M F A’Hearn ; C Arpigny ; A Ates ; J Aycock ; S Bagnulo ; J Bailey ; R Barber ; L Barrera ; R Barrena ; J M Bauer ; M J S Belton ; F Bensch ; B Bhattacharya ; N Biver ; G Blake ; D Bockelée-Morvan ; H Boehnhardt ; B P Bonev ; T Bonev ; M W Buie ; M G Burton ; H M Butner ; R Cabanac ; R Campbell ; H Campins ; M T Capria ; T Carroll ; F Chaffee ; S B Charnley ; R Cleis ; A Coates ; A Cochran ; P Colom ; A Conrad ; I M Coulson ; J Crovisier ; J deBuizer ; R Dekany ; J de Léon ; N Dello Russo ; A Delsanti ; M DiSanti ; J Drummond ; L Dundon ; P B Etzel ; T L Farnham ; P Feldman ; Y R Fernández ; M D Filipovic ; S Fisher ; A Fitzsimmons ; D Fong ; R Fugate ; H Fujiwara ; T Fujiyoshi ; R Furusho ; T Fuse ; E Gibb ; O Groussin ; S Gulkis ; M Gurwell ; E Hadamcik ; O Hainaut ; D Harker ; D Harrington ; M Harwit ; S Hasegawa ; C W Hergenrother ; P Hirst ; K Hodapp ; M Honda ; E S Howell ; D Hutsemékers ; D Iono ; W-H Ip ; W Jackson ; E Jehin ; Z J Jiang ; G H Jones ; P A Jones ; T Kadono ; U W Kamath ; H U Käufl ; T Kasuga ; H Kawakita ; M S Kelley ; F Kerber ; M Kidger ; D Kinoshita ; M Knight ; L Lara ; S M Larson ; S Lederer ; C-F Lee ; A C Levasseur-Regourd ; J Y Li ; Q-S Li ; J Licandro ; Z-Y Lin ; C M Lisse ; G LoCurto ; A J Lovell ; S C Lowry ; J Lyke ; D Lynch ; J Ma ; K Magee-Sauer ; G Maheswar ; J Manfroid ; O Marco ; P Martin ; G Melnick ; S Miller ; T Miyata ; G H Moriarty-Schieven ; N Moskovitz ; B E A Mueller ; M J Mumma ; S Muneer ; D A Neufeld ; T Ootsubo ; D Osip ; S K Pandea ; E Pantin ; R Paterno-Mahler ; B Patten ; B E Penprase ; A Peck ; G Petitas ; N Pinilla-Alonso ; J Pittichova ; E Pompei ; T P Prabhu ; C Qi ; R Rao ; H Rauer ; H Reitsema ; S D Rodgers ; P Rodriguez ; R Ruane ; G Ruch ; W Rujopakarn ; D K Sahu ; S Sako ; I Sakon ; N Samarasinha ; J M Sarkissian ; I Saviane ; M Schirmer ; P Schultz ; R Schulz ; P Seitzer ; T Sekiguchi ; F Selman ; M Serra-Ricart ; R Sharp ; R L Snell ; C Snodgrass ; T Stallard ; G Stecklein ; C Sterken ; J A Stüwe ; S Sugita ; M Sumner ; N Suntzeff ; R Swaters ; S Takakuwa ; N Takato ; J Thomas-Osip ; E Thompson ; A T Tokunaga ; G P Tozzi ; H Tran ; M Troy ; C Trujillo ; J Van Cleve ; R Vasundhara ; R Vazquez ; F Vilas ; G Villanueva ; K von Braun ; P Vora ; R J Wainscoat ; K Walsh ; J Watanabe ; H A Weaver ; W Weaver ; M Weiler ; P R Weissman ; W F Welsh ; D Wilner ; S Wolk ; M Womack ; D Wooden ; L M Woodney ; C Woodward ; Z-Y Wu ; J-H Wu ; T Yamashita ; B Yang ; Y-B Yang ; S Yokogawa ; A C Zook ; A Zauderer ; X Zhao ; X Zhou ; J-M Zucconi ;
Date 14 Oct 2005
Journal Science, 310 (5746), 265-9
AbstractOn 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.
Source PubMed, pmid16150977 doi: 10.1126/science.1118978
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