[astro-ph.EP] Sub-Neptunes are the most common short-period (P<100 d) planets known. A major goal for the field is to build a comprehensive understanding of their compositions and evolutionary histories, and […]
exoplanet
Posted inExoplanets, -moons, -comets
Spectro-polarimetry of HAbitable Planet Earth (SHAPE) on Chandrayaan-3: Instrument Characteristics, Calibration and Onboard Performance
[astro-ph.IM] The orbiter of the Chandrayaan-3 mission of the Indian Space Research Organisation (ISRO) carries an experimental payload called SHAPE (Spectro-polarimetry of HAbitable Planet Earth). This payload makes disc-integrated observations […]
Posted inExoplanets, -moons, -comets
JWST/MIRI Imaging Search for Kinematically Detected Protoplanetary Candidates
[astro-ph.EP] Kinematic perturbations observed with ALMA in CO line emission provide evidence for a population of embedded giant protoplanets shaping the structure of protoplanetary disks.
Posted inExoplanets, -moons, -comets
AstroFetch: AI-powered Exoplanet Assistant
[NASA Exoplanet Archive] We’re excited to announce that AstroFetch, an AI-powered assistant that answers natural-language questions about exoplanets using archive data, is now in open beta.
![Sensitivity of the adopted contrast curves for the newly validated planets, separated by technique. Each pixel gives the fraction of curves sensitive to a companion of the given magnitude contrast (∆mag) at the given angular separation (∆arcsec), shading from white (all curves sensitive) to black (none sensitive). Speckle observations are confined to their ∼ 1.2 ′′ field of view, while the adaptive-optics curves extend to wider separations. Contrasts are in each observation’s native band and are not directly comparable across instruments (cf. Table 2).-- [astro-ph.EP]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/09/Assessing-the.png?resize=1200%2C720&ssl=1)
Posted inExoplanets, -moons, -comets
Assessing the Impact of High-Resolution Imaging on Statistical Validation of TESS Planet Candidates
[astro-ph.EP] High-resolution imaging is widely used to constrain false-positive scenarios in exoplanet validation, but it is a finite follow-up resource that reaches only a subset of candidates, and its population-level […]
![Disk properties [Ri,Rco,Rdust] and exoplanet semimajor axis values are plotted in units of the PMS host stellar radius as a function of host star mass. The plot shows planets are less common inside the disk corotation radius suggesting that planetary inward migration is frequently halted in the vicinity of the corotation radius. Some planets have semimajor axis values < Rdust the dust sublimation radius, implying that planet migration must have occurred to populate the semimajor axis < Rdust region. Ri & Rco (gray diamonds and red squares respectively) are from the Pittman et al. (2025b) survey. -- [astro-ph.EP]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/09/Exoplanet-System.png?resize=1200%2C719&ssl=1)
Posted inExoplanets, -moons, -comets
Exoplanet System Architecture: Sculpting the Inner Regions
[astro-ph.EP] In this study, we seek to improve our understanding of the competing roles of disk-driven and planet-planet dynamical migration in sculpting planetary system architecture in the inner ≲1.5 au […]
Posted inExoplanets, -moons, -comets
Eight New Planets Join The NASA Exoplanet Archive
[NASA Exoplanet Archive]. This week, the archive welcomes eight new planets: CD-35 2722 B b, HD 50554 c & d, KMT-2025-BLG-0975L b, KMT-2025-BLG-1160L b, TOI-3053 b, TOI-3278 b, and TOI-4409 b. We also bid adieu to WASP-126 […]
![Set B latitudinal annual temperature variation of Gl 514 b after 10 Myr evolution for two different orbital configurations. The nearly horizontal contours after ∼5 Myr indicate the model prediction has stabilized. Left panel: surface temperature (in °C) for e = 0.45. Right panel: e = 0.62. Note that the color bar for the right panel is not the same due to the large difference in surface temperature between each simulation.-- [Planetary Science Journal]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/09/Climates.png?resize=1200%2C722&ssl=1)
Posted inHabitable Zones
Climates Of Gl 514 b
[Planetary Science Journal] The continuous discovery of exoplanets, each with distinctive stellar and planetary properties, along with the development of higher resolution ground and space telescopes has positioned climate evolution […]
![Panel (a): HR diagram of the OC members with detections. The blue solid line is the fitting results of MS. green dashed lines represent the upper and lower bounds of the MS fitted with a ±0.5 offset, and the red dashed line is the same sequence shifted upwards by 2. The color bars represent the stellar ages. Panel (b): HR diagram of the field stars with detections. Panel (c): The Galactic distribution of the selected sources from the detected OC members. Panel (d): The Galactic distribution of the selected sources from the detected field stars. -- [astro-ph.SR]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/09/Evolution-of.png?resize=1200%2C720&ssl=1)
Posted inHabitable Zones
Evolution of Stellar Activity and Habitable Zone (EATEN): III. X-ray Activity of Dwarfs in Open Clusters and Field Stars
[astro-ph.SR] Stellar X-ray emission serves as a direct diagnostic of coronal activity, which is fundamentally linked to coronal heating processes. It also strongly influences the atmospheres and long-term habitability of […]
Posted inTRAPPIST-1
Radial Velocity Detection Of The TRAPPIST-1 Planetary System With SPIRou And NIRPS
[astro-ph.EP]. The TRAPPIST-1 system is well-known for its seven transiting Earth-sized exoplanets. It has been extensively studied and characterized, notably with transit timing variations (TTVs) to precisely measure the mass […]