Deep impact: observations from a worldwide earth-based campaign

Meech, K. J.; Ageorges, N.; Hearn, M. F. A.; 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.; Battacharya, B.; Biver, N.; Blake, G.; Bocklee-Morvan, D.; Boehnhardt, H.; Bonev, B. P.; Bonev, T.; Buie, M.V.; 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.; deBuzier, J.; Dekany, R.; de Leon, J.; Dello Russo, N.; Delsanti, A.; DiSanti, M.; Drummond, J.; Dundon, L.; Etzel, P. B.; Farnham, T. L.; Feldman, P.; Fernandez, Y. R.; Filipovic, M. D.; Fisher, S.; Fitzsimmons, A.; Fong, D.; Fugate, R.; Fujiewara, 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.; Hutsemekers, D.; Iono, D.; Ip, W.-H.; Jackson, W.; Jehin, E.; Jiang, Z. J.; Jones, G. H.; Jones, P. A.; Kadono, T.; Kamath, U. W.; Kaufl, 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.; Schultz, R.; Seitzer, P.; Sekiguchi, T.; Selman, F.; Serra-Ricart, M.; Sharp, R.; Snell, R. L.; Snodgrass, C.; Stallard, T.; Stecklein, G.; Sterken, C.; Stuwe, 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. and Zucconi, J.-M. (2005). Deep impact: observations from a worldwide earth-based campaign. Science, 310(5746) pp. 265–269.

DOI: https://doi.org/10.1126/science.1118978

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.

Viewing alternatives

Look up in Google Scholar

Metrics

Public Attention

Altmetrics from Altmetric

Number of Citations

Citations from Dimensions
No digital document available to download for this item

Item Actions

Export

About

CORE (COnnecting REpositories)

Recommendations