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.
| Original language | English (US) |
|---|---|
| Pages (from-to) | 265-269 |
| Number of pages | 5 |
| Journal | Science |
| Volume | 310 |
| Issue number | 5746 |
| DOIs | |
| State | Published - Oct 14 2005 |
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Deep Impact : Observation from a worldwide earth-based campaign. / Meech, K. J.; Ageorges, N.; A'Hearn, M. F.; Arpigny, C.; Ates, A.; Aycock, J.; Bagnulo, S.; Bailey, J.; Barber, R.; Barrera, L.; Barrena, R.; Bauer, J. M.; Belton, M. J S; Bensch, F.; Bhattacharya, B.; Biver, N.; Blake, G.; Bockelée-Morvan, D.; Boehnhardt, H.; Bonev, B. P.; Bonev, T.; Buie, M. W.; Burton, M. G.; Butner, H. M.; Cabanac, R.; Campbell, R.; Campins, H.; Capria, M. T.; Carroll, T.; Chaffee, F.; Charnley, S. B.; Cleis, R.; Coates, A.; Cochran, A.; Colom, P.; Conrad, A.; Coulson, I. M.; Crovisier, J.; DeBuizer, J.; Dekany, R.; De Léon, J.; Dello Russo, N.; Delsanti, A.; DiSanti, M.; Drummond, J.; Dundon, L.; Etzel, P. B.; Farnham, T. L.; Feldman, P.; Fernández, Y. R.; Filipovic, M. D.; Fisher, S.; Fitzsimmons, A.; Fong, D.; Fugate, R.; Fujiwara, H.; Fujiyoshi, T.; Furusho, R.; Fuse, T.; Gibb, E.; Groussin, O.; Gulkis, S.; Gurwell, M.; Hadamcik, E.; Hainaut, O.; Harker, D.; Harrington, D.; Harwit, M.; Hasegawa, S.; Hergenrother, C. W.; Hirst, P.; Hodapp, K.; Honda, M.; Howell, E. S.; Hutsemékers, D.; Iono, O.; Ip, W. H.; Jackson, W.; Jehin, E.; Jiang, Z. J.; Jones, G. H.; Jones, P. A.; Kadono, T.; Kamath, U. W.; Käufl, H. U.; Kasuga, T.; Kawakita, H.; Kelley, M. S.; Kerber, F.; Kidger, M.; Kinoshita, D.; Knight, M.; Lara, L.; Larson, S. M.; Lederer, S.; Lee, C. F.; Levasseur-Regourd, A. C.; Li, J. Y.; Li, Q. S.; Licandro, J.; Lin, Z. Y.; Lisse, C. M.; LoCurto, G.; Lovell, A. J.; Lowry, S. C.; Lyke, J.; Lynch, D.; Ma, J.; Magee-Sauer, K.; Maheswar, G.; Manfroid, J.; Marco, O.; Martin, P.; Melnick, G.; Miller, S.; Miyata, T.; Moriarty-Schieven, G. H.; Moskovitz, N.; Mueller, B. E A; Mumma, M. J.; Muneer, S.; Neufeld, D. A.; Ootsubo, T.; Osip, D.; Pandea, S. K.; Pantin, E.; Paterno-Mahler, R.; Patten, B.; Penprase, B. E.; Peck, A.; Petitas, G.; Pinilla-Alonso, N.; Pittichova, J.; Pompei, E.; Prabhu, T. P.; Qi, C.; Rao, R.; Rauer, H.; Reitsema, H.; Rodgers, S. D.; Rodriguez, P.; Ruane, R.; Ruch, G.; Rujopakarn, W.; Sahu, D. K.; Sako, S.; Sakon, I.; Samarasinha, N.; Sarkissian, J. M.; Saviane, I.; Schirmer, M.; Schultz, P.; Schulz, R.; Seitzer, P.; Sekiguchi, T.; Selman, F.; Serra-Ricart, M.; Sharp, R.; Snell, R. L.; Snodgrass, C.; Stallard, T.; Stecklein, G.; Sterken, C.; Stüwe, J. A.; Sugita, S.; Sumner, M.; Suntzeff, N.; Swaters, R.; Takakuwa, S.; Takato, N.; Thomas-Osip, J.; Thompson, E.; Tokunaga, A. T.; Tozzi, G. P.; Tran, H.; Troy, M.; Trujillo, C.; Van Cleve, J.; Vasundhara, R.; Vazquez, R.; Vilas, F.; Villanueva, G.; Von Braun, K.; Vora, P.; Wainscoat, R. J.; Walsh, K.; Watanabe, J.; Weaver, H. A.; Weaver, W.; Weiler, M.; Weissman, P. R.; Welsh, W. F.; Wilner, D.; Wolk, S.; Womack, M.; Wooden, D.; Woodney, L. M.; Woodward, C.; Wu, Z. Y.; Wu, J. H.; Yamashita, T.; Yang, B.; Yang, Y. B.; Yokogawa, S.; Zook, A. C.; Zauderer, A.; Zhao, X.; Zhou, X.; Zucconi, J. M.
In: Science, Vol. 310, No. 5746, 14.10.2005, p. 265-269.Research output: Contribution to journal › Article › peer-review
}
TY - JOUR
T1 - Deep Impact
T2 - Observation from a worldwide earth-based campaign
AU - Meech, K. J.
AU - Ageorges, N.
AU - A'Hearn, M. F.
AU - Arpigny, C.
AU - Ates, A.
AU - Aycock, J.
AU - Bagnulo, S.
AU - Bailey, J.
AU - Barber, R.
AU - Barrera, L.
AU - Barrena, R.
AU - Bauer, J. M.
AU - Belton, M. J S
AU - Bensch, F.
AU - Bhattacharya, B.
AU - Biver, N.
AU - Blake, G.
AU - Bockelée-Morvan, D.
AU - Boehnhardt, H.
AU - Bonev, B. P.
AU - Bonev, T.
AU - Buie, M. W.
AU - Burton, M. G.
AU - Butner, H. M.
AU - Cabanac, R.
AU - Campbell, R.
AU - Campins, H.
AU - Capria, M. T.
AU - Carroll, T.
AU - Chaffee, F.
AU - Charnley, S. B.
AU - Cleis, R.
AU - Coates, A.
AU - Cochran, A.
AU - Colom, P.
AU - Conrad, A.
AU - Coulson, I. M.
AU - Crovisier, J.
AU - DeBuizer, J.
AU - Dekany, R.
AU - De Léon, J.
AU - Dello Russo, N.
AU - Delsanti, A.
AU - DiSanti, M.
AU - Drummond, J.
AU - Dundon, L.
AU - Etzel, P. B.
AU - Farnham, T. L.
AU - Feldman, P.
AU - Fernández, Y. R.
AU - Filipovic, M. D.
AU - Fisher, S.
AU - Fitzsimmons, A.
AU - Fong, D.
AU - Fugate, R.
AU - Fujiwara, H.
AU - Fujiyoshi, T.
AU - Furusho, R.
AU - Fuse, T.
AU - Gibb, E.
AU - Groussin, O.
AU - Gulkis, S.
AU - Gurwell, M.
AU - Hadamcik, E.
AU - Hainaut, O.
AU - Harker, D.
AU - Harrington, D.
AU - Harwit, M.
AU - Hasegawa, S.
AU - Hergenrother, C. W.
AU - Hirst, P.
AU - Hodapp, K.
AU - Honda, M.
AU - Howell, E. S.
AU - Hutsemékers, D.
AU - Iono, O.
AU - Ip, W. H.
AU - Jackson, W.
AU - Jehin, E.
AU - Jiang, Z. J.
AU - Jones, G. H.
AU - Jones, P. A.
AU - Kadono, T.
AU - Kamath, U. W.
AU - Käufl, H. U.
AU - Kasuga, T.
AU - Kawakita, H.
AU - Kelley, M. S.
AU - Kerber, F.
AU - Kidger, M.
AU - Kinoshita, D.
AU - Knight, M.
AU - Lara, L.
AU - Larson, S. M.
AU - Lederer, S.
AU - Lee, C. F.
AU - Levasseur-Regourd, A. C.
AU - Li, J. Y.
AU - Li, Q. S.
AU - Licandro, J.
AU - Lin, Z. Y.
AU - Lisse, C. M.
AU - LoCurto, G.
AU - Lovell, A. J.
AU - Lowry, S. C.
AU - Lyke, J.
AU - Lynch, D.
AU - Ma, J.
AU - Magee-Sauer, K.
AU - Maheswar, G.
AU - Manfroid, J.
AU - Marco, O.
AU - Martin, P.
AU - Melnick, G.
AU - Miller, S.
AU - Miyata, T.
AU - Moriarty-Schieven, G. H.
AU - Moskovitz, N.
AU - Mueller, B. E A
AU - Mumma, M. J.
AU - Muneer, S.
AU - Neufeld, D. A.
AU - Ootsubo, T.
AU - Osip, D.
AU - Pandea, S. K.
AU - Pantin, E.
AU - Paterno-Mahler, R.
AU - Patten, B.
AU - Penprase, B. E.
AU - Peck, A.
AU - Petitas, G.
AU - Pinilla-Alonso, N.
AU - Pittichova, J.
AU - Pompei, E.
AU - Prabhu, T. P.
AU - Qi, C.
AU - Rao, R.
AU - Rauer, H.
AU - Reitsema, H.
AU - Rodgers, S. D.
AU - Rodriguez, P.
AU - Ruane, R.
AU - Ruch, G.
AU - Rujopakarn, W.
AU - Sahu, D. K.
AU - Sako, S.
AU - Sakon, I.
AU - Samarasinha, N.
AU - Sarkissian, J. M.
AU - Saviane, I.
AU - Schirmer, M.
AU - Schultz, P.
AU - Schulz, R.
AU - Seitzer, P.
AU - Sekiguchi, T.
AU - Selman, F.
AU - Serra-Ricart, M.
AU - Sharp, R.
AU - Snell, R. L.
AU - Snodgrass, C.
AU - Stallard, T.
AU - Stecklein, G.
AU - Sterken, C.
AU - Stüwe, J. A.
AU - Sugita, S.
AU - Sumner, M.
AU - Suntzeff, N.
AU - Swaters, R.
AU - Takakuwa, S.
AU - Takato, N.
AU - Thomas-Osip, J.
AU - Thompson, E.
AU - Tokunaga, A. T.
AU - Tozzi, G. P.
AU - Tran, H.
AU - Troy, M.
AU - Trujillo, C.
AU - Van Cleve, J.
AU - Vasundhara, R.
AU - Vazquez, R.
AU - Vilas, F.
AU - Villanueva, G.
AU - Von Braun, K.
AU - Vora, P.
AU - Wainscoat, R. J.
AU - Walsh, K.
AU - Watanabe, J.
AU - Weaver, H. A.
AU - Weaver, W.
AU - Weiler, M.
AU - Weissman, P. R.
AU - Welsh, W. F.
AU - Wilner, D.
AU - Wolk, S.
AU - Womack, M.
AU - Wooden, D.
AU - Woodney, L. M.
AU - Woodward, C.
AU - Wu, Z. Y.
AU - Wu, J. H.
AU - Yamashita, T.
AU - Yang, B.
AU - Yang, Y. B.
AU - Yokogawa, S.
AU - Zook, A. C.
AU - Zauderer, A.
AU - Zhao, X.
AU - Zhou, X.
AU - Zucconi, J. M.
PY - 2005/10/14
Y1 - 2005/10/14
N2 - 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.
AB - 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.
UR - http://www.scopus.com/inward/record.url?scp=26844468254&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=26844468254&partnerID=8YFLogxK
U2 - 10.1126/science.1118978
DO - 10.1126/science.1118978
M3 - Article
C2 - 16150977
AN - SCOPUS:26844468254
VL - 310
SP - 265
EP - 269
JO - Science
JF - Science
SN - 0036-8075
IS - 5746
ER -