JUPITER AFTER THE 2009 IMPACT: HUBBLE SPACE TELESCOPE IMAGING OF THE IMPACT-GENERATED DEBRIS AND ITS TEMPORAL EVOLUTION

We report Hubble Space Telescope images of Jupiter during the aftermath of an impact by an unknown object in 2009 July. The 2009 impact-created debris field evolved more slowly than those created in 1994 by the collision of the tidally disrupted comet D/Shoemaker-Levy 9 (SL9). The slower evolution, in conjunction with the isolated nature of this single impact, permits a more detailed assessment of the altitudes and meridional motion of the debris than was possible with SL9. The color of the 2009 debris was markedly similar to that seen in 1994, thus this dark debris is likely to be Jovian material that is highly thermally processed. The 2009 impact site differed from the 1994 SL9 sites in UV morphology and contrast lifetime; both are suggestive of the impacting body being asteroidal rather than cometary. Transport of the 2009 Jovian debris as imaged by Hubble shared similarities with transport of volcanic aerosols in Earth's atmosphere after major eruptions.

[1]  J. Burns,et al.  Cassini Imaging of Jupiter's Atmosphere, Satellites, and Rings , 2003, Science.

[2]  Paul Pellegrino,et al.  Monitoring the Mt. Pinatubo aerosol layer with NOAA/11 AVHRR data , 1992 .

[3]  R. Clark,et al.  Storm clouds on Saturn: Lightning-induced chemistry and associated materials consistent with Cassini/VIMS spectra , 2009 .

[4]  O. Toon,et al.  Radiatively forced dispersion of the Mt. Pinatubo volcanic cloud and induced temperature perturbations in the stratosphere during the first few months following the eruption , 1994 .

[5]  H. Hammel The Collision of Comet Shoemaker-Levy 9 and Jupiter: HST imaging of Jupiter shortly after each impact: Plumes & fresh sites , 1996 .

[6]  R. West,et al.  Transport and Mixing in Jupiter's Stratosphere Inferred from Comet S-L9 Dust Migration , 1999 .

[7]  Richard C. Puetter,et al.  THE IMPACT OF A LARGE OBJECT ON JUPITER IN 2009 JULY , 2010, 1005.2312.

[8]  E. Karkoschka Spectrophotometry of the Jovian Planets and Titan at 300- to 1000-nm Wavelength: The Methane Spectrum , 1994 .

[9]  T. Dowling,et al.  HST imaging of atmospheric phenomena created by the impact of comet Shoemaker-Levy 9 , 1995, Science.

[10]  C. Barnet,et al.  HST spectroscopic observations of Jupiter after the collision of comet Shoemaker-Levy 9 , 1995, Science.

[11]  M. Patrick McCormick,et al.  The poleward dispersal of Mount Pinatubo volcanic aerosol , 1993 .

[12]  C. Moutou,et al.  Detection of atmospheric haze on an extrasolar planet: the 0.55–1.05 μm transmission spectrum of HD 189733b with the Hubble Space Telescope , 2007, 0712.1374.

[13]  M. Ádámkovics,et al.  Discovery of Fog at the South Pole of Titan , 2009, 0908.4087.

[14]  R. West,et al.  Impact debris particles in Jupiter's stratosphere , 1995, Science.

[15]  R Prange,et al.  HST far-ultraviolet imaging of Jupiter during the impacts of comet Shoemaker-Levy 9 , 1995, Science.

[16]  A. Simon The Structure and Temporal Stability of Jupiter's Zonal Winds: A Study of the North Tropical Region , 1999 .

[17]  A. Sánchez-Lavega,et al.  A Study of the Stability of Jovian Zonal Winds from HST Images: 1995–2000 , 2001 .

[18]  L. Bernstein,et al.  Mid-Infrared Ethane Emission on Neptune and Uranus* , 2006, astro-ph/0602546.

[19]  S. Pérez-Hoyos,et al.  Brightness power spectral distribution and waves in Jupiter's upper cloud and hazes , 2009 .

[20]  David A. Crawford,et al.  Comet Shoemaker‐Levy 9 Fragment Size Estimates: How Big Was the Parent Body? a , 1995 .