The depth of Jupiter's Great Red Spot constrained by Juno gravity overflights
Utilisation des micro-ondes du vaisseau spatial Juno pour observer la profondeur de la Grande Tache Rouge de Jupiter
Parisi, Marzia ; et al.
<br>The atmosphere of Jupiter consists of bands of winds rotating at different rates, punctuated by giant storms. The largest storm is the Great Red Spot (GRS), which has persisted for more than a century. It has been unclear whether the storms are confined to a thin layer near the top of the atmosphere or if they extend deep into the planet. Bolton et al. used microwave observations from the Juno spacecraft to observe several storms and vortices. They found that the storms extended below the depths at which water and ammonia are expected to condense, implying a connection with the deep atmosphere. Parisi et al. analyzed gravity measurements taken while Juno flew over the GRS. They detected a perturbation in the planet's gravitational field caused by the storm, finding that it was no more than 500 kilometers deep. In combination, these results constrain how Jupiter's meteorology links to its deep interior. -KTS<br></p>
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