Fragmentation modelling of the 2019 August impact on Jupiter

Author:

Sankar Ramanakumar1ORCID,Palotai Csaba1ORCID,Hueso Ricardo2,Delcroix Marc3,Chappel Ethan4,Sánchez-Lavega Agustin2

Affiliation:

1. Department of Aerospace, Physics and Space Sciences, Florida Institute of Technology, 150 W University Blvd, Melbourne, FL 32901, USA

2. Depto. Física Aplicada I, Escuela de Ingeniería de Bilbao, UPV/EHU, Bilbao 48013, Spain

3. Commission des Observations planétaires, Sociéte Astronomique de France, 75016 Paris, France

4. Department of Computer Science, University of Texas at San Antonio, 1 UTSA Circle, San Antonio, TX 78249, USA

Abstract

Abstract On 2019 August 7, an impact flash lasting ∼1 s was observed on Jupiter. The video of this event was analysed to obtain the light curve, and determine the energy release and initial mass. We find that the impactor released a total energy of 96–151 kilotons of TNT, corresponding to an initial mass between 190 and 260 metric tonnes with a diameter between 4 and 10 m. We developed a fragmentation model to simulate the atmospheric breakup of the object and reproduce the light curve. We model three different materials: cometary, stony, and metallic at speeds of 60, 65, and 70 km s−1, respectively, to determine the material make-up of the impacting object. The slower cases are best fitted by a strong, metallic object while the faster cases require a weaker material.

Funder

MINECO

FEDER

Horizon 2020

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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