posted on 2019-10-21, 10:28authored byA Sanchez-Lavega, A Wesley, G Orton, R Hueso, S Perez-Hoyos, LN Fletcher, P Yanamandra-Fisher, J Legarreta, I de Pater, H Hammel, A Simon-Miller, JM Gomez-Forrellad, JL Ortiz, E Garcia-Melendo, RC Puetter, P Chodas
On 2009 July 19, we observed a single, large impact on Jupiter at a planetocentric latitude of 55°S. 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.
Funding
This work was supported by the Spanish MEC AYA2006-07735 and MICIIN AYA2009-10701 with FEDER and Grupos Gobierno Vasco IT-464-07. G.O. and P.Y.F. acknowledge support from NASA grants to JPL. L.N.F. was supported by NASA Postdoctoral Program at the Jet Propulsion Laboratory (Caltech, USA). J.L.O. acknowledges AYA2008-06202-C03-01.
History
Citation
Astrophysical Journal Letters, 2010, 715 (2), pp. L155-L159 (5)
Author affiliation
/Organisation/COLLEGE OF SCIENCE AND ENGINEERING/Department of Physics and Astronomy