Tootfinder

Okee!…?
Sone art schlager-hiphop
RAF Camora x Apache 207 - JUPITER
https://www.youtube.com/watch?v=3RvBj77W9sQ
> JUPITER” hier streamen: http…

Coupled 1D Chemical Kinetic-Transport and 2D Hydrodynamic Modeling Supports a modest 1-1.5x Supersolar Oxygen Abundance in Jupiter's Atmosphere
Jeehyun Yang, Ali Hyder, Renyu Hu, Jonathan I. Lunine
https://arxiv.org/abs/2508.05007

Coupled 1D Chemical Kinetic-Transport and 2D Hydrodynamic Modeling Supports a modest 1-1.5x Supersolar Oxygen Abundance in Jupiter's Atmosphere
Understanding the deep atmospheric composition of Jupiter provides critical constraints on its formation and the chemical evolution of the solar nebula. In this study, we combine one-dimensional thermochemical kinetic-transport modeling with two-dimensional hydrodynamic simulations to constrain Jupiter's deep oxygen abundance using carbon monoxide (CO) as a proxy tracer. Leveraging a comprehensive chemical network generated by Reaction Mechanism Generator (RMG), we assess the impact of updated …

In situ and remote observations of the ultraviolet footprint of the moon Callisto by the Juno spacecraft: #Juno Detected the Final Missing Auroral Signature from Jupiter’s Four Largest Moons: https://science.nasa.gov/missions/juno/juno-detected-the-final-missing-auroral-signature-from-jupiters-four-largest-moons/

Wrote a quick explainer of our new paper, led by Karolina Heyduk, showing that Joshua trees can use water-saving CAM photosynthesis, which should be mighty handy for a desert plant facing hotter summers and more stressful droughts
https://lab.jbyoder.org/2025/09/03…

🇺🇦 #NowPlaying on KEXP's #DriveTime
Sun Ra and His Solar Arkestra:
🎵 On Jupiter
#SunRaandHisSolarArkestra
https://sunrastrut.bandcamp.com/track/on-jupiter-2

German Chancellor Friedrich Merz inaugurates the Jupiter supercomputer, powered by Nvidia chips, the world's fourth-fastest and Europe's first Exascale system (Reuters)
https://www.reuters.com/business/media-telecom/g…

A carbon-rich atmosphere on a windy pulsar planet
Michael Zhang, Maya Beleznay, Timothy D. Brandt, Roger W. Romani, Peter Gao, Hayley Beltz, Matthew Bailes, Matthew C. Nixon, Jacob L. Bean, Thaddeus D. Komacek, Brandon P. Coy, Guangwei Fu, Rafael Luque, Daniel J. Reardon, Emma Carli, Ryan M. Shannon, Jonathan J. Fortney, Anjali A. A. Piette, M. Coleman Miller, Jean-Michel Desert

A carbon-rich atmosphere on a windy pulsar planet
A handful of enigmatic Jupiter-mass objects have been discovered orbiting pulsars. One such object, PSR J2322-2650b, uniquely resembles a hot Jupiter exoplanet due to its minimum density of 1.8 g/cm^3 and its ~1900 K equilibrium temperature. We use JWST to observe its emission spectrum across an entire orbit. In stark contrast to every known exoplanet orbiting a main-sequence star, we find an atmosphere rich in molecular carbon (C3, C2) with strong westward winds. Our observations open up a new…

On the meaning of the dynamo radius in giant planets with stable layers
Paula N. Wulff, Hao Cao, Jonathan M. Aurnou
https://arxiv.org/abs/2508.03861 https://

On the meaning of the dynamo radius in giant planets with stable layers
Current structure models of Jupiter and Saturn suggest that helium becomes immiscible in hydrogen in the outer part of the planets' electrically conducting regions. This likely leads to a layer in which overturning convection is inhibited due to a stabilizing compositional gradient. The presence of such a stably stratified layer impacts the location and mechanism of convectively-driven dynamo action. Juno's measurements of Jupiter's magnetic field enabled an estimate of its dynamo radius based …