Cassini Archives

An artist’s rendition of Saturn’s moon Enceladus depicts hydrothermal activity on the seafloor and cracks in the moon’s icy crust that allow material from the watery interior to be ejected into space. New research shows that instruments destined for the next missions could find traces of a single cell in a single ice grain contained in a plume. NASA/JPL-Caltech

Astrochemistry, Astrogeology, Biogeochemical Cycles & Geobiology, Biosignatures & Paleobiology, Enceladus, Habitable Zones, Icy Worlds, Status Report

Tidal Rock Grinding As A Source Of H2 On Enceladus

by Keith CowingJune 16, 2026June 16, 2026

The Solar System hosts multiple potentially habitable environments, including the subsurface ocean beneath the icy crust of Saturn’s moon Enceladus.

Example of altimeter echo received from plains. This waveform was recorded during flyby T30 from an altitude of 1964.9 km at an incidence angle 0.0137°. Panel (a) shows a context map. Section of the T30 altimeter track observing the plains from point A to C. The waveform resulting from the integration of three echoes (Burst ID 131027162/4) located at point B is shown in panel (b) the altimetric model is used to fit the echo, resulting in an estimated RMS height of 4 m over the 115 square km footprints. The fitting error is indicated as a percentage by the mean integral relative error (MIRE). Panel (c) shows the large-scale topography of the plains using three elevation trackers, Maximum Likelihood, Threshold, and First Moment. All three trackers agree that the overall surface height changes less than 50 m over 50 km. -- JGR Planets

Atmospheres, Climate, Weather, Biochemistry & Organic Chemistry, Biogeochemical Cycles & Geobiology, Habitable Zones, Icy Worlds, Mapping, Geodesy, Cartography, Bathymetry, Status Report, Titan

Titan’s Plains Revealed: Evidence For A Layered Surface

by Keith CowingApril 10, 2026April 10, 2026

Undifferentiated plains are the most common terrain type on Titan, yet their composition and geologic history remain poorly understood.

Namib Sand Sea, Ground Penetrating Radar, Yardang, Lut desert,

Analog Studies, Arctic / Antarctic / Alpine, Away Teams & Field Reports, Caves, Craters, Mountains, Subsurface, Lava Tubes, Desert Worlds, Exploration Gear & Tech, Icy Worlds, Lava / magma ocean / Volcanic Worlds, Mapping, Geodesy, Cartography, Bathymetry, Planetary Protection & Biosafety, Polar / Alpine Expeditions, Robotics/Rovers/UAVs, Sample Return, Status Report, Titan, Tricorders & Sensors, Water/Hycean Worlds & Oceanography

Terrestrial Analogs To Titan For Geophysical Research

by Keith CowingFebruary 20, 2026February 20, 2026

Saturn’s moon Titan exhibits remarkable parallels to the Earth in many geophysical and geological processes not found elsewhere in the solar system at the present day.

This view was taken from above the ringplane and looks toward the unlit side of the rings. Here, the probe gazes upon Titan in the distance beyond Saturn and its dark and graceful rings -- NASA/JPL/SSI

Astrogeology, Atmospheres, Climate, Weather, Biochemistry & Organic Chemistry, Hyperion, Impact events, Press Release, Saturn, Titan

Saturn’s Moon Titan Could Have Formed in a Merger of Two Old Moons

by Keith CowingFebruary 11, 2026

Recent research suggests that Saturn’s bright rings and its largest moon, Titan, may have both originated in collisions among its moons.

Illustration of the electrodynamic interaction between Enceladus and Saturn. The primary Alfvén wing is shown in blue, and the reflected Alfvén wings in magenta. The arrow indicates the corotation direction of the Enceladus plasma torus. Relative sizes of Saturn and Enceladus are not to scale. Design & Animation: Fabrice Etifier - École Polytechnique.

Astrochemistry, Astrogeology, Atmospheres, Climate, Weather, Biosignatures & Paleobiology, Enceladus, Icy Worlds, Imaging & Spectroscopy, Press Release, Saturn

Enceladus Trails A Wake Of Electromagnetic Ripples That Extend Over Half A Million Kilometers

by Keith CowingFebruary 9, 2026February 9, 2026

A major study by an international team of researchers using data from the NASA/ESA/ASI Cassini spacecraft has revealed a lattice-like structure of crisscrossing reflected waves that flow downstream behind the […]

One set of images taken by Huygens is pictured here showing the view from 2 km altitude. It is in Mercator projection, so the N–S/E–W directions cross at right angles but surface areas appear distorted. Sky above horizon is modfied for formatting.- ESA/Astrobiology.com Original image

Astrogeology, Atmospheres, Climate, Weather, Biogeochemical Cycles & Geobiology, Biosignatures & Paleobiology, Icy Worlds, Imaging & Spectroscopy, Saturn, Status Report, Titan, Water/Hycean Worlds & Oceanography

Absence Of A Subsurface Ocean On Titan Indicated By Cassini Data

by Keith CowingJanuary 7, 2026January 7, 2026

The Cassini spacecraft orbited Saturn from 2004 to 2017, performing over a hundred flybys of Titan, Saturn’s largest moon.

Histograms and uncertainty ellipse (red) for computed Re(k2) and Im(k2) compared with the observed uncertainty ellipse (black) for the interior models of Titan without (a) and with (b) an ocean. The centre and axes of the ellipses are computed from the covariance matrix of the posterior distributions obtained from the interior inversion (1σ level of uncertainty). -- Nature via PubMed

Astrogeology, Atmospheres, Climate, Weather, Biosignatures & Paleobiology, Icy Worlds, Imaging & Spectroscopy, Missions & Hardware, Status Report, Titan, Water/Hycean Worlds & Oceanography

Titan’s Strong Tidal Dissipation Precludes A Subsurface Ocean

by Keith CowingDecember 24, 2025December 24, 2025

The Cassini mission provided unprecedented insights into Saturn’s largest moon, Titan, from its atmosphere to the deep interior.

This artist’s concept depicts NASA’s Cassini spacecraft performing one of its many close flybys of Titan, Saturn’s largest moon. By analyzing the Doppler shift of radio signals traveling to and from Earth, the mission precisely measured Titan’s gravity field. Credit: NASA/JPL-Caltech

Biosignatures & Paleobiology, Icy Worlds, Imaging & Spectroscopy, Missions & Hardware, Press Release, Saturn, Titan, Water/Hycean Worlds & Oceanography

Titan May Not Have A Global Ocean

by Keith CowingDecember 17, 2025December 17, 2025

A key discovery from NASA’s Cassini mission in 2008 was that Saturn’s largest moon Titan may have a vast water ocean below its hydrocarbon-rich surface. But reanalysis of mission data […]

Plumes on Enceladus (artist concept)– NASA JPL

Astrogeology, Atmospheres, Climate, Weather, Biochemistry & Organic Chemistry, Biogeochemical Cycles & Geobiology, Biosignatures & Paleobiology, Cryobiology, Enceladus, Habitable Zones, Icy Worlds, Imaging & Spectroscopy, Mapping, Geodesy, Cartography, Bathymetry, Missions & Hardware, Press Release, Saturn, Water/Hycean Worlds & Oceanography

Cassini Study Found Organics From An Ocean Inside Enceladus

by Keith CowingNovember 19, 2025November 19, 2025

NASA’s Cassini spacecraft captured dramatic plumes, both large and small, spray water ice out from many locations along the famed ‘tiger stripes’ near the south pole of Saturn’s moon Enceladus.

The new study constrained the Enceladus’ global conductive heat flow by studying its seasonal temperature variations at its north pole (yellow). These results, when combined with existing ones of its highly active south polar region (red) provide the first observational constraint of Enceladus’ energy loss budget (

Atmospheres, Climate, Weather, Enceladus, Icy Worlds, Imaging & Spectroscopy, Mapping, Geodesy, Cartography, Bathymetry, Press Release, Water/Hycean Worlds & Oceanography

Enceladus May Host A Stable Ocean Fit For Life, New Study Finds

by Keith CowingNovember 10, 2025November 10, 2025

A new study led by researchers from Oxford University and Southwest Research Institute and the Planetary Science Institute in Tucson, Arizona has provided the first evidence of significant heat flow […]