International audienceJupiter’s Great Red Spot (GRS) is the largest atmospheric vortex in the Solar System and has been observed for at least two centuries. It has been unclear how deep the vortex extends beneath its visible cloud tops. We examined the gravity signature of the GRS using data from 12 encounters of the Juno spacecraft with the planet, including two direct overflights of the vortex. Localized density anomalies due to the presence of the GRS caused a shift in the spacecraft line-of-sight velocity. Using two different approaches to infer the GRS depth, which yielded consistent results, we conclude that the GRS is contained within the upper 500 kilometers of Jupiter’s atmosphere
Jupiter's Great Red Spot (GRS) is one of its most distinct and enduring features. Since the advent o...
The observed zonal winds at Jupiter's cloud tops have been shown to be closely linked to the asymmet...
We have produced mosaics of the Great Red Spot (GRS) using images taken by the Galileo spacecraft in...
Jupiter’s Great Red Spot (GRS) is the largest atmospheric vortex in the Solar System and has been ob...
Jupiter’s Great Red Spot (GRS) is the most dominant and long-lived feature in Jupiter’s atmosphere. ...
One of Jupiter's most prominent atmospheric features, the Great Red Spot (GRS), has been observed fo...
International audienceMeasuring the depth of Jupiter’s storms The atmosphere of Jupiter consists of ...
Jupiter’s atmosphere has a system of zones and belts punctuated by small and large vortices, the lar...
Jupiter’s fast rotation- one rotation over 10 hours- creates strong jet streams, smearing its clouds...
The depth to which Jupiter’s observed east–west jet streams extend has been a long-standing question...
Jupiter’s Great Red Spot (GRS) is one of its most distinct and enduring features. Since the advent o...
The Little Red Spot (LRS) in Jupiter's atmosphere was investigated in unprecedented detail by the Ne...
On 27 August 2016, the Juno spacecraft acquired science observations of Jupiter, passing less than ...
Most current models of Jupiter's Great Red Spot (GRS) are cast in terms of a two-layer model, where ...
In this paper, Jupiter’s Great Red Spot (GRS) is used to determine properties of the Jovian atmosphe...
Jupiter's Great Red Spot (GRS) is one of its most distinct and enduring features. Since the advent o...
The observed zonal winds at Jupiter's cloud tops have been shown to be closely linked to the asymmet...
We have produced mosaics of the Great Red Spot (GRS) using images taken by the Galileo spacecraft in...
Jupiter’s Great Red Spot (GRS) is the largest atmospheric vortex in the Solar System and has been ob...
Jupiter’s Great Red Spot (GRS) is the most dominant and long-lived feature in Jupiter’s atmosphere. ...
One of Jupiter's most prominent atmospheric features, the Great Red Spot (GRS), has been observed fo...
International audienceMeasuring the depth of Jupiter’s storms The atmosphere of Jupiter consists of ...
Jupiter’s atmosphere has a system of zones and belts punctuated by small and large vortices, the lar...
Jupiter’s fast rotation- one rotation over 10 hours- creates strong jet streams, smearing its clouds...
The depth to which Jupiter’s observed east–west jet streams extend has been a long-standing question...
Jupiter’s Great Red Spot (GRS) is one of its most distinct and enduring features. Since the advent o...
The Little Red Spot (LRS) in Jupiter's atmosphere was investigated in unprecedented detail by the Ne...
On 27 August 2016, the Juno spacecraft acquired science observations of Jupiter, passing less than ...
Most current models of Jupiter's Great Red Spot (GRS) are cast in terms of a two-layer model, where ...
In this paper, Jupiter’s Great Red Spot (GRS) is used to determine properties of the Jovian atmosphe...
Jupiter's Great Red Spot (GRS) is one of its most distinct and enduring features. Since the advent o...
The observed zonal winds at Jupiter's cloud tops have been shown to be closely linked to the asymmet...
We have produced mosaics of the Great Red Spot (GRS) using images taken by the Galileo spacecraft in...