The Origin of Jupiter's Great Red Spot

Author:

Sánchez‐Lavega Agustín1ORCID,García‐Melendo Enrique2ORCID,Legarreta Jon1ORCID,Miró Arnau3ORCID,Soria Manel2ORCID,Ahrens‐Velásquez Kevin2ORCID

Affiliation:

1. Escuela de Ingeniería de Bilbao Universidad del País Vasco UPV/EHU Bilbao Spain

2. Escola Superior d’Enginyeries Industrial Aeroespacial i Audiovisual de Terrassa Universitat Politècnica de Catalunya Terrassa/Barcelona Spain

3. Barcelona Supercomputing Center Barcelona Spain

Abstract

AbstractJupiter's Great Red Spot (GRS) is the largest and longest‐lived known vortex of all solar system planets but its lifetime is debated and its formation mechanism remains hidden. G. D. Cassini discovered in 1665 the presence of a dark oval at the GRS latitude, known as the “Permanent Spot” (PS) that was observed until 1713. We show from historical observations of its size evolution and motions that PS is unlikely to correspond to the current GRS, that was first observed in 1831. Numerical simulations rule out that the GRS formed by the merging of vortices or by a superstorm, but most likely formed from a flow disturbance between the two opposed Jovian zonal jets north and south of it. If so, the early GRS should have had a low tangential velocity so that its rotation velocity has increased over time as it has shrunk.

Funder

Eusko Jaurlaritza

Ministerio de Ciencia, Innovación y Universidades

Barcelona Supercomputing Center

Publisher

American Geophysical Union (AGU)

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