Published June 1, 2010 | Version v1
Journal article

THE IMPACT OF A LARGE OBJECT ON JUPITER IN 2009 JULY

  • 1. Dpto. FIsica Aplicada I, Escuela Superior de Ingenieros, Universidad del PaIs Vasco, Alameda Urquijo s/n, 48013 Bilbao (Spain)
  • 2. Acquerra Pty. Ltd., 82 Merryville Drive, Murrumbateman, NSW 2582 (Australia)
  • 3. Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive Pasadena, California, 91109 (United States)
  • 4. Atmospheric, Oceanic and Planetary Physics, Clarendon Laboratory, Parks Road, Oxford OX1 3PU (United Kingdom)
  • 5. Escuela Universitaria Ingenieria Tecnica Industrial, Plaza de la Casilla 3, 48012 Bilbao (Spain)
  • 6. University of California, 601 Campbell Hall, Berkeley CA 94720 (United States)
  • 7. Space Science Institute, 4750 Walnut Avenue, Suite 205, Boulder, CO 80301 (United States)
  • 8. NASA Goddard Space Flight Center, Greenbelt, MD 20771 (United States)
  • 9. Fundacio Observatori Esteve Duran, Montseny 46 - Urb. El Montanya, 08553 Seva, Barcelona (Spain)
  • 10. Instituto de AstrofIsica de Andalucia, CSIC, Apt. 3004, 18080 Granada (Spain)
  • 11. Center for Astrophysics and Space Science, 9500 Gilman Drive, La Jolla, CA 92093 (United States)

Description

On 2009 July 19, we observed a single, large impact on Jupiter at a planetocentric latitude of 550S. This and the Shoemaker-Levy 9 (SL9) impacts on Jupiter in 1994 are the only planetary-scale impacts ever observed. The 2009 impact had an entry trajectory in the opposite direction and with a lower incidence angle than that of SL9. Comparison of the initial aerosol cloud debris properties, spanning 4800 km east-west and 2500 km north-south, with those produced by the SL9 fragments and dynamical calculations of pre-impact orbit indicates that the impactor was most probably an icy body with a size of 0.5-1 km. The collision rate of events of this magnitude may be five to ten times more frequent than previously thought. The search for unpredicted impacts, such as the current one, could be best performed in 890 nm and K (2.03-2.36 μm) filters in strong gaseous absorption, where the high-altitude aerosols are more reflective than Jupiter's primary clouds.

Availability note (English)

Available from http://dx.doi.org/10.1088/2041-8205/715/2/L155

Additional details

Identifiers

Publishing Information

Journal Title
Astrophysical Journal Letters
Journal Volume
715
Journal Issue
2
Journal Page Range
p. L155-L159
ISSN
2041-8205

INIS

Country of Publication
United States
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
42043489
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
AEROSOLS; COLLISIONS; INCIDENCE ANGLE; JUPITER PLANET; PLANETARY ATMOSPHERES
Descriptors DEC
ATMOSPHERES; COLLOIDS; DISPERSIONS; PLANETS; SOLS