[NASA]. You may never soar under the clouds or over the organic sands of Saturn’s moon Titan, but your name can. NASA is inviting the public to send their names […]
Saturn
![Global map of Enceladus with color and contours indicating the estimated heat flux (in mWm−2 ) calculated from maps of shell thickness [Hemingway and Mittal, 2019]. Our results (Table 1) are plotted as lines using the same color scale as the background. Green labeled boxes show other estimates [Giese et al., 2008; Bland et al., 2012, 2007; Leonard et al., 2021] of paleo-heat fluxes using similar methods.-- [astro-ph.EP]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/10/Paleoheat.png?resize=1200%2C721&ssl=1)
Posted inEnceladus
Paleo-heat Flux Estimates Across Enceladus Derived From Flexural Response Of The Ice Shell
[astro-ph.EP] Saturn’s moon Enceladus has active plumes suggestive of locally high heat fluxes at present, and the present-day heating is reasonably well characterized. However, the moon’s thermal history is not […]
Posted inTitan
Detection Of Hydrocarbons In Titan Using High-resolution Cross-correlation Spectroscopy
[astro-ph.EP]. High-resolution cross-correlation spectroscopy (HRCCS) is a powerful technique for detecting molecules whose individual spectral lines are too weak to be identified directly, but its sensitivity is limited by the […]
Posted inMissions & Hardware
Using Nuclear Technology To Change How We Explore Icy Ocean Worlds: Examples From Nuclear Powered Mission Concept Designs
[Frontiers] Icy ocean worlds represent some of the most compelling targets in the search for extraterrestrial life, yet their exploration is constrained by significant logistical challenges including long transit times, […]
Posted inTitan
A Review Of The Geochemical Environment at Selk Crater on Titan: Applications to Dragonfly
[Astrobiology (Journal)] This article summarizes the current state of knowledge regarding the destination for NASA’s Dragonfly mission: Titan’s Selk crater.
![Pressures determined by ruby fluorescence measurements at different locations within the sample chamber: (a) during powder compaction, (b) after decompression. No ruby fluorescence spectrum was obtained on the sphere marked with an asterisk, likely due to insufficient Cr doping, resulting in an undetectable fluorescence signal. -- [astro-ph.EP]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/10/Elastic.png?resize=1200%2C720&ssl=1)
Posted inTitan
Elastic Properties of Titan Tholins Revealed by Brillouin Spectroscopy
[astro-ph.EP] Titan tholins, complex organic solids synthesized by simulating photochemical processes in Titan’s atmosphere, are widely regarded as analogs to organic surface materials on the Saturnian moon.
![A heterotrophic ecosystem enabled by fermentation on Enceladus. [astro-ph.EP]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/10/Fermentation.png?resize=1200%2C720&ssl=1)
Posted inEnceladus
Fermentation Heterotrophy Can Reproduce Enceladus’s H2 And CH4 Under Limited Serpentinization
[astro-ph.EP] Saturn’s icy moon Enceladus is a prime target in the search for life beyond Earth. Abundant H2 and CH4 in Enceladus’s south-polar plume have been shown to be consistent […]
Posted inEnceladus
How Enceladus’ Ocean Spray Becomes Chemically Diverse Ice Grains
[Institute of Science Tokyo] Saturn’s icy moon Enceladus hides a global ocean beneath its frozen surface. From fractures near its south pole, material from this ocean is ejected into space […]
Posted inTitan
Dragonfly Gets Wired Up While Titan Landing Area Is Named
[NASA]. Peeking into the clean room at the Johns Hopkins Applied Physics Laboratory (APL) in Laurel, Maryland, it might be one of the first things you notice about NASA’s Dragonfly: […]
![Example weighting functions for selected microwave frequencies (logarithmically spaced between 3 mm - 3 m) corresponding to the model atmospheres for Saturn (top) and Uranus (bottom) from Figure 1. -- [astro-ph.EP]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/08/Microwave-Remote-.png?resize=1200%2C715&ssl=1)
Posted inAtmospheres, Climate, Weather
Microwave Remote Sensing Of Giant Planet Atmospheres: Considerations For Saturn And Uranus Orbiter Missions
[astro-ph.EP] Microwave radiometer instruments are uniquely capable of studying volatile element abundances and heat/mass transport within the deep atmospheres of giant planets.