Jupiter Archives

The north polar region of Jupiter’s volcanic moon Io was captured by NASA’s Juno during the spacecraft’s 57th close pass of the gas giant on Dec. 30, 2023. Data from that flyby and one on Feb. 3, 2024, is helping scientists understand Io’s interior. Image data: NASA/JPL-Caltech/SwRI/MSSS Image processing by Gerald Eichstädt

Lava World Recon: Juno Studies Io’s Volcanoes

by Keith CowingJuly 23, 2026July 23, 2026

[NASA] NASA’s Juno mission has provided the first measurements of the temperature below the surface of Jupiter’s moon Io, revealing significant heating within the shallow subsurface of the most volcanically […]

Ganymede and Callisto As Seen By Voyager -- NASA

Jupiter

The Recent Crossing Of The 7:3 Resonance Between Ganymede And Callisto

by Keith CowingJuly 10, 2026July 10, 2026

[astro-ph.EP] Io, Europa and Ganymede are locked in the well-known Laplace resonance, while Callisto is not, even though it is very close to the 7:3 mean motion resonance with Ganymede. […]

Pioneer 10 sails past Jupiter - Juno image of Jupiter from NASA and graphic by Grok via Astrobiology.com

Missions & Hardware

Pioneer 10/11 Telemetry Explanatory Almanac

by Keith CowingJuly 9, 2026July 9, 2026

[astro-ph.IM] This document is intended to accompany our first release of edited Pioneer 10/11 telemetry data. The purpose of this data release is to provide a data set for the […]

An artist's rendering of Europa and Jupiter based on images sent by visiting spacecraft. Europa is the closest orbiting of the three Jupiter’s large ‘Galilean’ moons to be visited by Juice – any human astronaut that lands there would receive a lethal radiation dose on a timescale of hours. And spacecraft electronics are almost as susceptible to radiation as human biology. CREDIT NASA/JPL-Caltech

Europa, Meteorites & Asteroids, Origin & Evolution of Life, Panspermia, Planetary Protection & Biosafety, Status Report, Water/Hycean Worlds & Oceanography

Earth As A Potential Source Of Llife For Europa’s Subsurface Ocean

by Keith CowingJune 22, 2026June 21, 2026

The paper discusses the possibility of dust particles containing living bacteria ejected from Earth reaching Europa and landing on its surface.

This artist's impression shows radar waves from the NASA Goldstone Solar System Radar pinging one of Jupiter’s moons, Europa. The radar waves penetrate Europa’s icy surface before bouncing back to be collected by the NSF Green Bank Telescope on Earth. Credit: NSF/AUI/NSF NRAO/P.Vosteen

Callisto, Europa, Ganymede, Habitable Zones, Icy Worlds, Journal articles, Press Release, Water/Hycean Worlds & Oceanography

Radar Echoes From Europa Reveal Secrets Beneath the Ice

by Keith CowingJune 18, 2026June 18, 2026

A team of scientists has used NASA’s Goldstone Solar System Radar and the U.S. National Science Foundation Green Bank Telescope (NSF GBT) to carry out the most extensive radar study […]

An artist's impression of a disk of gas and dust formed during the birth of the sun. Credit: NASA/FUSE/Lynette Cook

Astrochemistry, Astrogeology, Comets and Asteroids, Exoplanets, -moons, -comets, Habitable Zones, Mars, Mercury, Meteorites & Asteroids, Press Release, Venus

New Experiments And Modeling On Iron Meteorites Provide Insight Into Young Solar System And Earth’s Building Blocks

by Keith CowingJune 4, 2026June 4, 2026

Habitable planets require life-essential elements, like nitrogen and phosphorus. Understanding how those elements ended up in a planetary body can give insight into the formation of the solar system and […]

This artist’s illustration shows the magnetic activity around a hot Jupiter exoplanet. Hot Jupiters have one side that is always facing their host star and is scorching hot, whereas the other side is extremely cold. This steep temperature difference creates fast winds that blow from the day side to the night side. The planet’s magnetic field, shown here with blue lines, can slow these winds down. Credit International Gemini Observatory/NOIRLab/NSF/AURA/M. Garlick

Exoplanets, -moons, -comets, Gas Giants, Habitable Zones, Magnetic Fields, Electromagnetism, bioelectricity,, Press Release

Strange Winds Reveal Strongest Hints Yet Of Magnetic Activity In Exoplanets

by Keith CowingJune 3, 2026June 3, 2026

By measuring the strength of the invisible magnetic fields of seven ultra-hot Jupiters, astronomers have taken a major step toward understanding planets beyond our Solar System. A new study published […]

A northern polar projection of Jupiter indicating the latitude and longitude ranges adopted for coaddition of individual spectra. The circumference latitude is 40◦ (planetocentric), enclosed concentric circles are spaced by 4◦ in latitude. The magenta line represents the statistical mean position of the auroral oval (Bonfond et al., 2017). Spatial bins in black represent regions that do not overlap in latitude with the auroral oval, blue and red spatial bins represents areas outside and inside the auroral oval, respectively. TEXES achieves diffraction-limited spatial resolutions of 0.7” to 1.4” over the wavelength range adopted in this study, which corresponds to a latitude-longitude footprint of 5-10◦ at 60◦N. -- astro-ph.EP

Astrochemistry, Atmospheres, Climate, Weather, Biochemistry & Organic Chemistry, Biogeochemical Cycles & Geobiology, Exoplanets, -moons, -comets, Gas Giants, Imaging & Spectroscopy, Jupiter, Status Report

Detection Of Propadiene (CH2CCH2), Propene (C3H6) And Non-detection Of Propane (C3H8) In Jupiter’s Northern Polar Stratosphere

by Keith CowingMay 25, 2026May 25, 2026

We report the first detection of stratospheric propadiene (CH2CCH2) and propene (C3H6) at Jupiter’s mid-to-high northern latitudes using IRTF-TEXES measurements recorded on March 5-6, 2025.

Astrogeology, Callisto, Ganymede, Icy Worlds, Imaging & Spectroscopy, Jupiter, Press Release

Ganymede Might Still Be Forming Its Metal Core Today

by Keith CowingMay 18, 2026May 18, 2026

Jupiter’s moon Ganymede is the largest moon in the solar system; at over 3,200 miles across, it is larger than the planet Mercury. It is also the only moon with […]

Numerical ocean-induction setup for Ganymede in a deep-ocean scenario with REM = 1.77 . Ganymede's internal structure is depicted, featuring the ice crust, the deep ocean with its simulated zonal flow, the internal ice layer, the silicate mantle, and the metallic core. Yellow tubes visualize the magnetic field lines. The bottom-right panel shows how magnetic field lines are sheared by the zonal (east–west) jet flow in the ocean (blue/red denote westward/eastward jets, respectively), thereby reflecting the secondary magnetic field induced by such dynamics. -- Geophysical Research Letters

Astrogeology, Biogeochemical Cycles & Geobiology, Ganymede, Icy Worlds, Jupiter, Magnetic Fields, Electromagnetism, bioelectricity,, Press Release, Water/Hycean Worlds & Oceanography

Motional Induction in Ganymede’s Ocean

by Keith CowingMay 10, 2026May 11, 2026

We investigate the magnetic signature of oceanic circulation in Ganymede’s subsurface ocean using kinematic induction modeling. Our approach couples zonal jet flows from rotating thermal convection simulations with magnetic field […]