![Left: Orbital separations of inspiralling planets over time. Right: Mass accreted onto planets over time. For each initial planet mass, we show results for 𝜀 ∈ [0.01, 0.1, 0.3, 0.5, 1.0], with an increasing efficiency denoted by an increasing opacity. We also allow the accretion to increase up to 10× the Eddington limit, denoted by the dotted lines. Accretion stops when 𝑅𝐵 < 𝑅Jup (see §2.3). -- [astro-ph.EP]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/08/Atmospheric-Signatures.png?resize=1200%2C722&ssl=1)
[astro-ph.EP] The majority of confirmed exoplanets orbit within 1 au of a main-sequence (MS) star. When their stellar hosts evolve off the MS, many of these planets will be engulfed […]
astronomy
![Top: Hexagonal segmented primary mirror designs with no central obscuration with different number of rings and varying segment sizes (flat-to-flat (m) 1-Hex: 2.64, 2-Hex: 1.45, 3-Hex: 1.19, 4-Hex: 0.85, 5-Hex: 0.66), all designs have an inscribed diameter of ∼6 m. Middle: Binary apodizer masks optimized for their respective aperture design. Bottom: Respective coronagraphic PSFs with an annular dark hole ranging from 3.4λ/D - 12λ/D, and a spatial average contrast floor of ∼4 × 10−11 inside the dark hole. -- [astro-ph.IM]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/08/Segmentlevel.png?resize=1200%2C720&ssl=1)
Posted inAstronomy & Telescopes
Segment-level Thermal Sensitivity Analysis For Exo-Earth Coronagraphy With Segmented Space Telescopes
[astro-ph.IM] Direct imaging and characterization of Earth-like planets require ultra-stable wavefronts to achieve a starlight suppression level of 100 parts per trillion (ppt) in the coronagraphic dark region of the […]
![Retrieved emission spectra (blue regions) plotted with the true planet’s flux from our forward model (red) for each redox state considered (IW-6 to IW+6). The retrieved spectra denser region represents the 1𝜎 confidence level, intermediate region 2𝜎, thin region the 3𝜎 level. The observational noise from LIFEsim is shown as a gray envelope. The retrieved spectra capture most spectral features in observed planets, especially in the more pronounced oxidised cases (bottom row). -- [astro-ph.EP]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/08/Characterizing-the.png?resize=1200%2C720&ssl=1)
Posted inExoplanets, -moons, -comets
Characterizing The Oxidation State Of Rocky Exoplanets With The Large Interferometer For Exoplanets (LIFE)
[astro-ph.EP] The oxidation state of rocky exoplanets is expected to play a fundamental role in shaping the chemical composition of their secondary atmospheres by influencing the chemical composition of volcanically […]
![Schematic diagram of our spectral line stacking and matched filtering procedures. First, (a) shows relevant spectral regions of the (synthetic) observational data (black) and an initial spectral simulation (red). Each spectral window is then weighted based on the signal-to-noise ratio of each region to create a velocity stack of all relevant molecular rotational transitions (b). Finally, the stacked simulation is used as a matched filter and is cross-correlated with the stacked data to visualize the statistical significance of a given detection (c). -- [astro-ph.GA]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/08/Exploring-the-Limits.png?resize=1200%2C720&ssl=1)
Posted inAstrochemistry
Exploring the Limits of Spectral Line Stacking in Spectral Line Data and Application Toward the Detection of Bulk 13C Enrichment of Aromatics in TMC-1
[astro-ph.GA] The formation history of polycyclic aromatic hydrocarbons (PAHs) in the interstellar medium remains a topic of active debate, with proposed mechanisms ranging from high-temperature stellar ejecta processes to low-temperature […]
Posted inSETI & Technosignatures
Nondetection of Narrowband Radio Technosignatures from LHS 1140 b at 1–12 GHz
[Research Notes of the AAS] LHS 1140b, a rocky exoplanet in its host star’s habitable zone, was recently shown to have an escaping helium atmosphere.
![Simulated HARMONI images of the Galilean satellites (Io, Europa, Ganymede, Callisto) compared to current VLT imaging (50 mas), illustrating the gain in spatial resolution (12 mas) enabled by the ELT for surface characterisation of Solar System bodies. Credit : Olivier Groussin for the Solar System Science group. -- [astro-ph.IM]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/07/HARMONI.png?resize=1200%2C720&ssl=1)
Posted inAstronomy & Telescopes
HARMONI@ELT: Instrument Design, Performance, And Science Capabilities
[astro-ph.IM] HARMONI is the integral field spectrograph for the Extremely Large Telescope (ELT). Designed as the primary workhorse near-infrared spectrograph of the ELT, it will deliver spatially resolved spectroscopy at […]
Posted inExoplanets, -moons, -comets
Constraining The Lives And Times Of Exoplanets Through Evolutionary Bayesian Retrievals
[astro-ph.EP] Static retrieval frameworks are leading tools for interpreting exoplanet observations, yet time-independent modelling leaves them prone to degeneracy and unable to resolve exoplanets’ histories.
Posted inSETI & Technosignatures
Breakthrough Listen’s Automated Commensal Technosignature Survey With MeerKAT
[astro-ph.IM] The search for extraterrestrial intelligence (SETI) is an ongoing effort to detect technosignatures, evidence of technologically capable life beyond Earth. Conducting a comprehensive SETI programme requires a large amount […]
![Snapshots of the system 1 ps after the initial contact of the nanograins for different initial velocities. Atom colour key indicates hydrogen: white; carbon: dark gray; oxygen: red; silicon: beige; and magnesium: green. -- [astro-ph.GA]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/07/When-Two-Worlds.png?resize=1200%2C715&ssl=1)
Posted inAstrochemistry
When Two Worlds Collide: How Collisions Between Silicate and Carbonaceous Nanograins can Drive Complex Chemistry
[astro-ph.GA] Our overall objective is to determine how collision velocity governs the interactions between silicate and carbonaceous nanograins. (astrochemistry)
Posted inAstronomy & Telescopes
ANDES, The High-resolution Spectrograph Oof The ELT: Simulated Performance Of The CORO Module And Overview Of The High-contrast Capabilities For Exoplanet Observations
[astro-ph.IM] We present the simulated performance of the coronagraph (CORO) module for ANDES, the Extremely Large Telescope (ELT) high-resolution spectrograph.