Moons and jupiter imaging spectrometer (MAJIS) on jupiter icy moons explorer (JUICE)
F Poulet, G Piccioni, Y Langevin, C Dumesnil… - Space Science …, 2024 - Springer
Abstract The MAJIS (Moons And Jupiter Imaging Spectrometer) instrument on board the
ESA JUICE (JUpiter ICy moon Explorer) mission is an imaging spectrometer operating in the …
ESA JUICE (JUpiter ICy moon Explorer) mission is an imaging spectrometer operating in the …
Jupiter science enabled by ESA's Jupiter icy moons explorer
Abstract ESA's Jupiter Icy Moons Explorer (JUICE) will provide a detailed investigation of the
Jovian system in the 2030s, combining a suite of state-of-the-art instruments with an orbital …
Jovian system in the 2030s, combining a suite of state-of-the-art instruments with an orbital …
A new window into planet formation and migration: refractory-to-volatile elemental ratios in ultra-hot Jupiters
A primary goal of exoplanet characterization is to use a planet's current composition to
understand how that planet formed. For example, the C/O ratio has long been recognized as …
understand how that planet formed. For example, the C/O ratio has long been recognized as …
A subsolar oxygen abundance or a radiative region deep in Jupiter revealed by thermochemical modelling
Jupiter's deep abundances help to constrain the formation history of the planet and the
environment of the protoplanetary nebula. Juno recently measured Jupiter's deep oxygen …
environment of the protoplanetary nebula. Juno recently measured Jupiter's deep oxygen …
Oxygen depletion in giant planets with different formation histories
S Fonte, D Turrini, E Pacetti, E Schisano… - Monthly Notices of …, 2023 - academic.oup.com
The atmospheric C/O ratio of exoplanets is widely used to constrain their formation. To
guarantee that the C/O ratio provides robust information, we need to accurately quantify the …
guarantee that the C/O ratio provides robust information, we need to accurately quantify the …
H2, He, and CO2 Pressure-induced Parameters for the HITRAN Database. II. Line Lists of CO2, N2O, CO, SO2, OH, OCS, H2CO, HCN, PH3, H2S, and GeH4
Y Tan, FM Skinner, S Samuels… - The Astrophysical …, 2022 - iopscience.iop.org
In recent years, extended efforts have been made to increase the potential for modeling and
interpreting the spectra of planetary atmospheres using the HITRAN database. A significant …
interpreting the spectra of planetary atmospheres using the HITRAN database. A significant …
Evidence for multiple Ferrel‐like cells on Jupiter
Jupiter's atmosphere is dominated by multiple jet streams which are strongly tied to its 3D
atmospheric circulation. Lacking a rigid bottom boundary, several models exist for how the …
atmospheric circulation. Lacking a rigid bottom boundary, several models exist for how the …
Storms and the depletion of ammonia in Jupiter: II. Explaining the Juno observations
Observations of Jupiter's deep atmosphere by the Juno spacecraft have revealed several
puzzling facts: The concentration of ammonia is variable down to pressures of tens of bars …
puzzling facts: The concentration of ammonia is variable down to pressures of tens of bars …
Jupiter's temperate belt/zone contrasts revealed at depth by Juno microwave observations
LN Fletcher, FA Oyafuso, M Allison… - Journal of …, 2021 - Wiley Online Library
Juno microwave radiometer (MWR) observations of Jupiter's midlatitudes reveal a strong
correlation between brightness temperature contrasts and zonal winds, confirming that the …
correlation between brightness temperature contrasts and zonal winds, confirming that the …
Giant planets from the inside-out
Giant planets acquire gas, ices and rocks during the early formation stages of planetary
systems and thus inform us on the formation process itself. Proceeding from inside out …
systems and thus inform us on the formation process itself. Proceeding from inside out …