[astro-ph.EP] Planet formation requires growth over 12 orders of magnitude in size, from micron-sized dust grains to fully formed planets.
astrochemistry
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 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 […]
![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 […]
![(Top row:) Composite images on three dates (Table 1) shown with a common display range from -0.01 to 0.02 adu pixel−1 . (Bottom row:) Same images from the top row contoured from 0.0004 adu pixel−1 in steps of 0.002 adu pixel−1 . Contours are smoothed over 8×8 pixel boxes. Yellow arrows show the projected antisolar direction while white arrows show the projected negative heliocentric velocity vector, from Table 1. The two directions are overlapping in the 2023 data. A 1′′ scale is common to all panels.-- [astro-ph.EP]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/10/Hubble-Space-.png?resize=1200%2C725&ssl=1)
Posted inComets and Asteroids
Hubble Space Telescope Observations of Active Asteroid (101955) Bennu
[astro-ph.EP] Measurements from NASA’s OSIRIS-REx spacecraft revealed (101955) Bennu as a member of the active asteroid class.
![First detection of fully deuterated methanol in interstellar space This composite image shows the Perseus molecular cloud, which is located about 1,000 light-years from Earth. A rare form of the organic alcohol methanol has been observed around at least one of the very young stars still embedded within it. This is the first time this molecule has been detected in space, as shared by the ALMA COMPASS Large Program (Complex Organic Molecules in Protostars with ALMA Spectral Surveys). Credit: Ekaterina Moerova / MPIfR; Background: NASA, CXC, SSC, NOAO, DSS; and 3D image of methanol fromPubChem [Internet]. Bethesda (MD): National Library of Medicine (US), National Center for Biotechnology Information; 2004-. PubChem Compound Summary for CID 887, Methanol; [cited 2026 July 16]. -- [NRAO]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/10/Exotic.png?resize=1200%2C724&ssl=1)
Posted inAstrochemistry
Exotic Methanol Discovered In Planet-Building Zones
[NRAO] An international team of astronomers using the Atacama Large Millimeter/submillimeter Array (ALMA), of which the U.S. National Science Foundation National Radio Astronomy Observatory is a partner (NSF NRAO), has […]
Posted inBrown Dwarfs
First Detection Of Variable Water Clouds Outside Of Our Solar System
[University Of Arizona]. A Jupiter-sized world just 7.5 light-years away is cloudy, chemically complex, and, it turns out, more like home than anyone expected.
Posted inAstrochemistry
Complex Organic Molecules in Protostars with ALMA Spectral Surveys (COMPASS) II. Approach To Data Reduction And Products For Line-rich Broadband (sub)millimeter Spectra
[astro-ph.SR] Studying the chemical composition of the warm gas surrounding embedded solar-type protostars is one of the areas for which the Atacama Large Millimeter/submillimeter Array (ALMA) is particularly well suited.
![Column density maps of 13CO2, CO and OCN− ice (panel I, II and III, respectively). 12CO2 column densities are derived from 13CO2 column densities. Panel IV shows the ratio between the 4.38 µm and 4.39 µm peak of the 13CO2 ice feature. A higher ratio indicates higher degree of CO2 ice segregation. The axes are shown on astronomical unit scales. Pixelated areas especially in the north and south of the maps as well as the edges are caused by low signal-to-noise levels. -- [astro-ph.SR]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/10/Mapping.png?resize=1200%2C718&ssl=1)
Posted inAstrochemistry
Mapping Of Interstellar Ices With JWST In Protostellar Envelopes: Spatial Variations Of 13CO2, 12CO2, CO, OCN− and H2O ice
[astro-ph.SR] The composition of planets and their atmospheres is largely determined by the formation environment of the planet. This environment is pre-determined during early stages when the protostar is still […]