[astro-ph.EP] Motivated by recent observations suggesting rings found in debris disks are wider than those in protoplanetary disks, we consider a picture in which planetesimals formed in radially narrow dust […]
Rings
Neptune’s Inner Moons and Rings Are Exposed Icy Body Interiors
[astro-ph.EP] Neptune’s single large moon, Triton, is accompanied by a set of dusty rings and small moons whose composition and origin are uncertain.
Saturn’s Moon Titan Could Have Formed in a Merger of Two Old Moons
Recent research suggests that Saturn’s bright rings and its largest moon, Titan, may have both originated in collisions among its moons.
On The Applicability of Ring-Moon Cycles to Exoplanets
The presence of rings and moons around exoplanets is likely to be one of the next great discoveries in exoplanet research.
Water-group Ion Irradiation Studies Of Enceladus Ice Analogues: Can Radiolysis Account For Material In And Around The South Polar Plume?
Saturn’s magnetosphere contains trapped plasma and energetic charged particles which constantly irradiate the surface of Enceladus.
Fomalhaut’s Warped Ring Is Shaped By Evolving Planets
Astronomers using the Atacama Large Millimeter/submillimeter Array (ALMA) have made the highest resolution image to date, revealing new insights into the unusual and mysterious architecture of the debris disk encircling […]
Search For Exoplanetary Ring Systems With TESS
Photometric surveys for exoplanetary ring systems have not confirmed any object with Saturn-sized ring.
Peculiar Rainbows in Saturn’s E Ring: Uncovering Luminious Bands Near Enceladus
We report observations of stripe-like features in Enceladus’ plumes captured simultaneously by Cassini’s VIMS-IR and ISS NAC instruments during flyby E17, with similar patterns seen in VIMS-IR data from flyby […]
Triton Atmospheric Pressure: A New Value Is Obtained
The observation of a stellar occultation by a Solar System object is a very powerful method for measuring its dimensions, as well as possibly detecting rings, revealing an atmosphere and […]
Validating the Orbital Periods of the Coolest TESS Exoplanet Candidates
When an exoplanet passes in front of its host star, the resulting eclipse causes an observable decrease in stellar flux, and when multiple such transits are detected, the orbital period […]
