Jupiter's interior as revealed by Juno
DJ Stevenson - Annual Review of Earth and Planetary Sciences, 2020 - annualreviews.org
Jupiter is in the class of planets that we call gas giants, not because they consist of gas but
because they were primarily made from hydrogen-helium gas, which upon gravitational …
because they were primarily made from hydrogen-helium gas, which upon gravitational …
MWR: Microwave radiometer for the Juno mission to Jupiter
MA Janssen, JE Oswald, ST Brown, S Gulkis… - Space Science …, 2017 - Springer
Abstract The Juno Microwave Radiometer (MWR) is a six-frequency scientific instrument
designed and built to investigate the deep atmosphere of Jupiter. It is one of a suite of …
designed and built to investigate the deep atmosphere of Jupiter. It is one of a suite of …
The water abundance in Jupiter's equatorial zone
Oxygen is the most common element after hydrogen and helium in Jupiter's atmosphere,
and may have been the primary condensable (as water ice) in the protoplanetary disk. Prior …
and may have been the primary condensable (as water ice) in the protoplanetary disk. Prior …
Let the great world spin: revealing the stormy, turbulent nature of young giant exoplanet analogs with the Spitzer Space Telescope
We present a survey for photometric variability in young, low-mass brown dwarfs with the
Spitzer Space Telescope. The 23 objects in our sample show robust signatures of youth and …
Spitzer Space Telescope. The 23 objects in our sample show robust signatures of youth and …
The distribution of ammonia on Jupiter from a preliminary inversion of Juno microwave radiometer data
The Juno microwave radiometer measured the thermal emission from Jupiter's atmosphere
from the cloud tops at about 1 bar to as deep as a hundred bars of pressure during its first …
from the cloud tops at about 1 bar to as deep as a hundred bars of pressure during its first …
Microwave observations reveal the deep extent and structure of Jupiter's atmospheric vortices
Jupiter's atmosphere has a system of zones and belts punctuated by small and large
vortices, the largest being the Great Red Spot. How these features change with depth is …
vortices, the largest being the Great Red Spot. How these features change with depth is …
Weather on Other Worlds. V. The Three Most Rapidly Rotating Ultra-cool Dwarfs
ME Tannock, S Metchev, A Heinze… - The Astronomical …, 2021 - iopscience.iop.org
Weather on Other Worlds. V. The Three Most Rapidly Rotating Ultra-cool Dwarfs - IOPscience
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This site uses cookies. By continuing to use this site you agree to our use of cookies. To find …
Changes in Jupiter's zonal wind profile preceding and during the Juno mission
We present five epochs of WFC3 HST Jupiter observations taken between 2009–2016 and
extract global zonal wind profiles for each epoch. Jupiter's zonal wind field is globally stable …
extract global zonal wind profiles for each epoch. Jupiter's zonal wind field is globally stable …
How well do we understand the belt/zone circulation of giant planet atmospheres?
The atmospheres of the four giant planets of our Solar System share a common and well-
observed characteristic: they each display patterns of planetary banding, with regions of …
observed characteristic: they each display patterns of planetary banding, with regions of …
[HTML][HTML] A review of radio observations of the giant planets: Probing the composition, structure, and dynamics of their deep atmospheres
I de Pater, EM Molter, CM Moeckel - Remote Sensing, 2023 - mdpi.com
Radio observations of the atmospheres of the giant planets Jupiter, Saturn, Uranus, and
Neptune have provided invaluable constraints on atmospheric dynamics, physics/chemistry …
Neptune have provided invaluable constraints on atmospheric dynamics, physics/chemistry …