Deep Impact: observations from a worldwide Earth-based campaign.

نویسندگان

  • 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
چکیده

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.

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عنوان ژورنال:
  • Science

دوره 310 5746  شماره 

صفحات  -

تاریخ انتشار 2005