Observational Consequences of Shallow-water Magnetohydrodynamics on Hot Jupiters

A. W. Hindle, P. J. Bushby, T. M. Rogers

Research output: Contribution to journalArticlepeer-review

3 Scopus citations

Abstract

We use results of shallow-water magnetohydrodynamics to place estimates on the minimum magnetic field strengths required to cause atmospheric wind variations (and therefore westward-venturing hotspots) for a data set of hot Jupiters (HJs), including HAT-P-7b, CoRoT-2b, Kepler-76, WASP-12b, and WASP-33b, on which westward hotspots have been observationally inferred. For HAT-P-7b and CoRoT-2b our estimates agree with past results; for Kepler-76b we find that the critical dipolar magnetic field strength, over which the observed wind variations can be explained by magnetism, lies between 4 G and 19 G; for WASP-12b and WASP-33b westward hotspots can be explained by 1 G and 2 G dipolar fields, respectively. Additionally, to guide future observational missions, we identify 61 further HJs that are likely to exhibit magnetically driven atmospheric wind variations and predict these variations are highly likely in ∼40 of the hottest HJs.

Original languageEnglish (US)
Article numberL8
JournalAstrophysical Journal Letters
Volume916
Issue number1
DOIs
StatePublished - Jul 20 2021
Externally publishedYes

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Fingerprint

Dive into the research topics of 'Observational Consequences of Shallow-water Magnetohydrodynamics on Hot Jupiters'. Together they form a unique fingerprint.

Cite this