Astrobiology117- Page

Simulated behaviour of L 98-59 b calculated with a semi-analytic toy model for its thermal evolution. Temperature is plotted over time for different initial temperatures 𝑇0 (line style) and tidal

Example of a bipolar outflow in IRAS 15557-5215 region. The top panels show the moment-0 map (left) and moment-1 map (right) of HC3N line. The outflow axis is represented by

Ganymede and Callisto As Seen By Voyager — NASA Analysis of Callisto’s moments of inertia, derived from Galileo’s gravity data, suggests that its structure is not fully differentiated. This possibly

MRS continuum-subtracted spectra of C2H2 (magenta), HCN (green), H2O (blue), and CO2 (brown) emission lines between 13.6-15.3 µm from JDISCS sources with sub-mm dust sizes r > 63 au. ALMA

Biosignatures & Paleobiology Status Report astro-ph.EP May 13, 2025 Schematic diagram of the analytical model (Eq. (11)) we use to understand the effect of cloud height and particle size on

Artist impression of solar system formation. Presolar grains are tiny, solid grains of primitive solar system material that originated before the formation of the Sun. They have been found in

Period-radius injection-recovery map for TOI 2076. Blue points indicate recovered signals, while red points mark signals that were not recovered. Only 20% of injected planets are shown for clarity. The

The abstract in PubMed or at the publisher’s site is linked when available and will open in a new window. Lee SMC, Miller A, Ribeiro LC, Rosenberg M, Miller CA,