NASA International Space Apps Time: October 4th – 5th, 2025 On October 4-5, 2025, NASA and 14 Space Agency Partners invite scientists, technologists, and storytellers to participate in the 2025
NASA International Space Apps Time: October 4th – 5th, 2025 On October 4-5, 2025, NASA and 14 Space Agency Partners invite scientists, technologists, and storytellers to participate in the 2025
LIFE RCN Workshop Time: September 11th, 8AM PDT/11AM EDT Join the 2025 LIFE NASA RCN Seminar Series This month’s speakers are Prof. Jennifer Macalady and Dr. Alta Howells. Dr. Jennifer
ASGSR 2025 The American Society for Gravitational and Space Research (ASGSR) Fellows Committee is now accepting nominations for the ASGSR Fellows Program. The distinction of Fellow is awarded by the
Exoplanet Travel Posters from NASA Looking for the perfect vacation? Do you crave late-night fun? PSO J318.5−22, the planet with no star where nightlife never ends, is perfect for you!
Exoplanets under consideration for the Rocky Worlds DDT. Planets above the cosmic shoreline are expected to have lost their atmosphere. The circled exoplanets have already been observed in emission during
Tricorders & Sensors Status Report biorxiv.org September 3, 2025 Heterogeneous degree distributions. a) The Hot Jupiter chemical reaction network’s degree distributions are represented by its complementary cumulative density function (CCDF)
3I/ATLAS Trajectory — SwRI Southwest Research Institute (SwRI) has completed a mission study detailing how a proposed spacecraft could fly by an interstellar comet, providing remarkable insights into the properties
Schematic showing the distribution of the modeled volatile gas (e.g., water vapor) disk and water ice disk around a WD. The rocky dust disk and their observationally inferred properties are
Range of best-fit phase curve and eclipse models for TRAPPIST-1 b and c. The detrended data are shown with gray dots and binned data with black dots. Red curves show
Distribution of the derived planetary radii as a function of insolation, along with the associated KDE. — astro-ph.EP Planetary radii are derived for 218 exoplanets orbiting 161 M dwarf stars.






