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 WELCOME

NEWS Last Update:  2007/Oct/03

IMPACT IN JUPITER

Images obtained by Anthony Wesley from Australia on 19th July 2009 show a new dark spot in Jupiter’s South Polar Region whose morphology differs from “normal features” in Jupiter, strongly suggesting that it was caused by a cometary or asteroidal impact. This seems confirmed by later observations in the infrarred range that indicate a warming in the upper troposphere and lower stratosphere of Jupiter.
We urge observations of this spot in any spectral range in order to follow its evolution. Since NEW IMPACTS can occur, we strongly suggest obtaining Jupiter images in any longitude.

See the initial report and ephemeris of the impact spot visibility for planning observations in the News section

The International Outer Planets Watch (IOPW) is an informal organization of astronomers and planetary scientists who are interested in the study of the Solar System's giant planets, their atmospheres, satellites, rings, magnetospheres, aurorae, and other phenomena. For this purpose, the International Outer Planets Watch has a Steering Committee and six discipline groups.

The Atmosphere Discipline of the IOPW is devoted to coordinate and encourage observations of the atmospheres of the giant planets and their satellites, from the Earth and from space, with an emphasis on time-variable phenomena.

Discipline Leader:
Ricardo Hueso Alonso

Grupo de Ciencias Planetarias
Escuela Superior de Ingenieros
Universidad del Pais Vasco
Alameda Urquijo s/n
48013 BILBAO (Spain)

Tel: (34) 946 014 262
Fax: (34) 946 014 178
e-mail:
  Web Site Manager:
Jon J. Legarreta Etxagibel

Grupo de Ciencias Planetarias
E.U.I.T.I.
Universidad del Pais Vasco
Plaza La Casilla 3
48012 BILBAO (Basque Country)

Tel: (34) 946 014 357
Fax: (34) 946 014 300
e-mail:
 

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 Our logo is a composition of images from Voyager and Hubble Space Telescope.


International Outer Planets Watch - Atmosphere Discipline
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Discipline Leader
Web Site Manager
Web Page Designer
Ricardo Hueso Alonso
Jon J. Legarreta Etxagibel
Irma T. Flores Mendoza
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Euskal Herriko Unibertsitatea