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First Earth-based Detection of a Superbolide on Jupiter

Authors :
Mark Boslough
Ricardo Hueso
Leigh N. Fletcher
Amy A. Simon-Miller
Santiago Pérez-Hoyos
Agustín Sánchez-Lavega
S. G. Djorgovski
Heidi B. Hammel
P. A. Yanamandra-Fisher
John Clarke
Glenn S. Orton
C. Go
M. L. Edwards
I. de Pater
Michael H. Wong
A. Wesley
Keith S. Noll
Publication Year :
2010
Publisher :
American Astronomical Society, 2010.

Abstract

Cosmic collisions on planets cause detectable optical flashes that range from terrestrial shooting stars to bright fireballs. On 2010 June 3 a bolide in Jupiter's atmosphere was simultaneously observed from the Earth by two amateur astronomers observing Jupiter in red and blue wavelengths. The bolide appeared as a flash of 2 s duration in video recording data of the planet. The analysis of the light curve of the observations results in an estimated energy of the impact of (0.9-4.0) × 1015 J which corresponds to a colliding body of 8-13 m diameter assuming a mean density of 2 g cm-3. Images acquired a few days later by the Hubble Space Telescope and other large groundbased facilities did not show any signature of aerosol debris, temperature, or chemical composition anomaly, confirming that the body was small and destroyed in Jupiter's upper atmosphere. Several collisions of this size may happen on Jupiter on a yearly basis. A systematic study of the impact rate and size of these bolides can enable an empirical determination of the flux of meteoroids in Jupiter with implications for the populations of small bodies in the outer solar system and may allow a better quantification of the threat of impacting bodies to Earth. The serendipitous recording of this optical flash opens a new window in the observation of Jupiter with small telescopes. © 2010 The American Astronomical Society. All rights reserved.

Details

Language :
English
Database :
OpenAIRE
Accession number :
edsair.doi.dedup.....041bd02dab31c2e03e82cd0b864d9992