GSTDTAP  > 气候变化
DOI10.1029/2020GL091797
Detection of a bolide in Jupiter's atmosphere with Juno UVS
Rohini S. Giles; Thomas K. Greathouse; Joshua A. Kammer; G. Randall Gladstone; Bertrand Bonfond; Vincent Hue; Denis C. Grodent; Jean‐; Claude Gé; rard; Maarten H. Versteeg; Scott J. Bolton; John E. P. Connerney; Steven M. Levin
2021-02-09
发表期刊Geophysical Research Letters
出版年2021
英文摘要

The UVS instrument on the Juno mission recorded transient bright emission from a point source in Jupiter's atmosphere. The spectrum shows that the emission is consistent with a 9600‐K blackbody located 225 km above the 1‐bar level and the duration of the emission was between 17 ms and 150 s. These characteristics are consistent with a bolide in Jupiter's atmosphere. Based on the energy emitted, we estimate that the impactor had a mass of 250–5000 kg, which corresponds to a diameter of 1–4 m. By considering all observations made with Juno UVS over the first 27 perijoves of the mission, we estimate an impact flux rate of 24,000 per year for impactors with masses greater than 250–5000 kg.

领域气候变化
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文献类型期刊论文
条目标识符http://119.78.100.173/C666/handle/2XK7JSWQ/313873
专题气候变化
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GB/T 7714
Rohini S. Giles,Thomas K. Greathouse,Joshua A. Kammer,et al. Detection of a bolide in Jupiter's atmosphere with Juno UVS[J]. Geophysical Research Letters,2021.
APA Rohini S. Giles.,Thomas K. Greathouse.,Joshua A. Kammer.,G. Randall Gladstone.,Bertrand Bonfond.,...&Steven M. Levin.(2021).Detection of a bolide in Jupiter's atmosphere with Juno UVS.Geophysical Research Letters.
MLA Rohini S. Giles,et al."Detection of a bolide in Jupiter's atmosphere with Juno UVS".Geophysical Research Letters (2021).
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