Jupiter tagged posts

Glorious, Glowing Jupiter awaits Juno’s arrival

In preparation for the imminent arrival of NASA's Juno spacecraft in July 2016, astronomers used ESO's Very Large Telescope to obtain spectacular new infrared images of Jupiter using the VISIR instrument. They are part of a campaign to create high-resolution maps of the giant planet to inform the work to be undertaken by Juno over the following months, helping astronomers to better understand the gas giant. This false-colour image was created by selecting and combining the best images obtained from many short VISIR exposures at a wavelength of 5 micrometres. Credit: ESO/L. Fletcher

In preparation for the imminent arrival of NASA’s Juno spacecraft in July 2016, astronomers used ESO’s Very Large Telescope to obtain spectacular new infrared images of Jupiter using the VISIR instrument. They are part of a campaign to create high-resolution maps of the giant planet to inform the work to be undertaken by Juno over the following months, helping astronomers to better understand the gas giant. This false-colour image was created by selecting and combining the best images obtained from many short VISIR exposures at a wavelength of 5 micrometres. Credit: ESO/L. Fletcher

Stunning new images and the highest-resolution maps to date of Jupiter at thermal infrared wavelengths give a glowing view of Juno’s target, a week ahead of the NASA mission’s arrival at the giant planet...

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Simulating Jet Streams and Anticyclones of Jupiter and Saturn

Image of Jupiter (L) and Simulation of Jupiter's Deep Atmospheric Flow (R). On the left side is a NASA image of Jupiter taken from Hubble Space Telescope. On the ride side is results of a 3-D simulation of Jupiter's deep atmospheric flow. The image gives global views of the axial vorticity (curl of the fluid velocity) at the outer boundary, the interior boundary, and in a meridional cut. Blue spots are anticyclones, which are predominant on Jupiter and rotate in the direction opposite Earth's cyclonic storms. In the simulation, the anticyclones are ringed by cyclonic filaments, which have also been observed on Jupiter. The image also reveals the vorticity of the zonal shear, which is much weaker than that of vortices. The interior flow is seen in the meridional cut to be strongly shaped by global rotation. Credit: Moritz Heimpel, University of Alberta

Image of Jupiter (L) and Simulation of Jupiter’s Deep Atmospheric Flow (R). On the left side is a NASA image of Jupiter taken from Hubble Space Telescope. On the ride side is results of a 3-D simulation of Jupiter’s deep atmospheric flow. The image gives global views of the axial vorticity (curl of the fluid velocity) at the outer boundary, the interior boundary, and in a meridional cut. Blue spots are anticyclones, which are predominant on Jupiter and rotate in the direction opposite Earth’s cyclonic storms. In the simulation, the anticyclones are ringed by cyclonic filaments, which have also been observed on Jupiter. The image also reveals the vorticity of the zonal shear, which is much weaker than that of vortices...

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Close encounter with Jupiter about 4B yrs ago may have Ejected another Planet from the Solar System

Artist’s impression of a fifth giant planet being ejected from the solar system. Image credit: Southwest Research Institute

Artist’s impression of a fifth giant planet being ejected from the solar system. Image credit: Southwest Research Institute

The existence of a 5th giant gas planet at the time of the Solar System’s formation – in addition to Jupiter, Saturn, Uranus and Neptune that we know of today – was first proposed in 2011. But if it did exist, how did it get pushed out? For years, scientists have suspected the ouster was either Saturn or Jupiter.

“Our evidence points to Jupiter,” said Ryan Cloutier
Planet ejections occur as a result of a close planetary encounter in which one of the objects accelerates so much that it breaks free from the massive gravitational pull of the Sun...

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