[astro-ph.EP] The composition of rocky planets depends on the dust in their natal protoplanetary disk (PPD), potentially containing water ice. Crystalline water ice was detected in the PPD d216-0939 in […]
Hubble Space Telescope
Astrometric Reconnaissance of Exoplanetary Systems (ARES). I. Methodology Validation With HST Point-source Images Of Proxima Centauri
We present the first results of the Astrometric Reconnaissance of Exoplanetary Systems (ARES) project, aimed at validating and characterizing candidate exoplanets around the nearest systems using multi-epoch Hubble Space Telescope […]
Direct Imaging For The Debris Disk Around epsilon Eridani With The Cool-Planet Imaging Coronagraph
We analyze the inner debris disk around ϵ Eridani using simulated observations with the Cool-Planet Imaging Coronagraph (CPI-C).
Discovery Of An Icy And Nitrogen-rich Extrasolar Planetesimal
White dwarfs accreting planetary debris provide detailed insight into the bulk composition of rocky exo-planetesimals. However, only one Kuiper-Belt analogue has been identified in that way so far.
Hydrocarbon Hazes On Temperate Sub-Neptune K2-18b Supported By Data From The James Webb Space Telescope
K2-18b, a sub-Neptune orbiting in the habitable zone of an M dwarf, has attracted significant interest following observations with the Hubble Space Telescope (HST) and, more recently, with the James […]
The Moons of Uranus Surprise Scientists
Scientists using NASA’s Hubble Space Telescope went looking for evidence of one phenomenon and found quite another. The research team studied the four largest moons of the ice giant Uranus, […]
Refractory Phosphorus In The HD 100546 Protoplanetary Disk
The phosphorus budget of planets is intertwined with their formation history and is thought to influence their habitability.
Astrochemistry: Webb Investigates A Dusty And Dynamic Disc
Herbig-Haro objects are small nebulae found in star formation regions, marking the locations where gas flowing out from young stars is heated into luminescence by shockwaves. HH 30 is an […]
Exoplanet Ephemerides Change Observations (ExoEcho). I. Transit Timing Analysis of Thirty-Seven Exoplanets using HST/WFC3 Data
The ExoEcho project is designed to study the photodynamics of exoplanets by leveraging high-precision transit timing data from ground- and space-based telescopes.
Astrochemistry: Hubble Studies the Tarantula Nebula’s Outskirts
This NASA/ESA Hubble Space Telescope image features a dusty yet sparkling scene from one of the Milky Way’s satellite galaxies, the Large Magellanic Cloud. The Large Magellanic Cloud is a […]
