[Kyushu University] Planetary systems like our solar system are born within a disk of gas and dust (protoplanetary disk) surrounding a newly formed star. Observations with the ALMA telescope have […]
Spectroscopy
Posted inExoplanets, -moons, -comets
Capture of Interstellar Planetesimals in Protoplanetary Discs in Binary Star Systems
[astro-ph.EP] Planet formation requires growth over 12 orders of magnitude in size, from micron-sized dust grains to fully formed planets.
![Radiogenic dose and the benefit of drilling. (a) GCR dose versus depth for constant-depth and steadily exhuming horizons, compared with the depth-independent radiogenic dose. Shading spans the radiogenic dose of the baseline composition at 3 Ga (0.9 MGy) and that of the regional GRS abundances at 3.9 Ga (5.6 MGy). Where a curve crosses the radiogenic level, the two doses are equal. (b) Total-dose reduction at 100–101 and 199–200 cm versus exposure age; dashed lines are the GCR-only shielding factors. Dotted lines mark effective ages for 10 and 100 nm yr−1 exhumation. -- [astro-ph.EP]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/10/Radiation.png?resize=1200%2C720&ssl=1)
Posted inMars
Radiation Limits On Amino Acid Preservation And Chiral Measurement At Oxia Planum
[astro-ph.EP] Amino acid enantiomeric excess (EE) is a potential biosignature, but its measurement requires sufficient surviving material as well as preserved chirality.
Posted inAstrochemistry
Infrared Spectroscopy Of Cyanonaphthalenes Under Interstellar Relevant Conditions And Their Potential Connection With Astronomical Aromatic Infrared Bands
[Astronomy & Astrophysics] Context. Aromatic infrared bands (AIBs) are widely observed in diverse astrophysical environments and are generally attributed to vibrational emission from polycyclic aromatic hydrocarbons (PAHs). The recent interstellar […]
Posted inAstronomy & Telescopes
ALMA Reveals Planetary Formation Structures In Small Disks
[ALMA] Thanks to the extraordinary sharpness of ALMA’s images, a research team has discovered rings, grooves, and cavities in extremely compact disks surrounding young stars.
Posted inAtmospheres, Climate, Weather
Simulations Of The Evolving Ozone Layer: Implications For The Early Earth, Exoplanets, And The Search For Life
[astro-ph.EP] Over 4 billion years, Earth’s atmosphere has been transformed from a composition devoid of molecular oxygen (O2) to one where O2 is now 21% of our modern atmosphere by […]
Posted inAstrochemistry
VUV And mid-UV Photoabsorption Cross Sections Of Thin Films Of Glycine And Alanine: Application To Their Photochemistry In The Solar System
[Photochemistry and Photobiology] Experiments conducted in Low Earth Orbit (LEO) since the 1990s have investigated the evolution of organic matter in solid-phase (including amino acids) under solar photon irradiation to […]
![Full JWST spectrum of HOPS-68. We indicate the molecular absorption bands of oxygen-bearing molecules as studied in this work (SiO, H2O, CO2 and CO) and of carbon-bearing molecules as studied in paper B, as well as the most notable ice and silicate absorption features. Not indicated are 13CCH2, CS, and CH4 in the 7.3-7.8 µm region, and CH3, C4H2 and C6H2 around ∼ 16 µm, which will all be studied in paper B. Some prominent H2 emission lines are highlighted with a black arrow. HOPS-68 is not detected in continuum at wavelengths lower than 2.2 µm. The inset shows a zoom-in to the 7.8-8.6 µm region, which highlights the detection of SiO. -- [astro-ph.SR]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/10/A-breath.png?resize=1200%2C558&ssl=1)
Posted inAstrochemistry
A Breath Of Fresh Air: Oxygen Enhancement From Silicate Sublimation During Early Protostellar Evolution
[astro-ph.SR] Recently, an analog to the t = 0 moment of our Solar System’s meteoritic record was identified for the first time around the Class I protostar HOPS-315.
![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.
Posted inExoplanets, -moons, -comets
Ultraviolet Reflected-Light Spectroscopy of Modern Earth Analogs with Starshade Observations
[astro-ph.EP] Characterizing rocky, habitable zone planets in reflected light is a key science objective for future direct imaging missions, and the ultraviolet (UV) is uniquely suited for supporting the characterization […]