The two largest planets in our Solar System, Jupiter and Saturn, also have the largest satellite systems, or the most moons. At present, Jupiter’s reported moon count stands at more […]
circumplanetary disk
New Insights Into The Potential For Life In The Jovian System
Southwest Research Institute was part of an international team that demonstrated how complex organic molecules (COMs), key chemical precursors to life, could have been incorporated into Jupiter’s Galilean moons during […]
Delivery Of Complex Organic Molecules To The System Of Jupiter
Complex organic molecules are key markers of molecular diversity, and their formation conditions in protoplanetary disks remain an active area of research. These molecules have been detected on a variety […]
Formation and Survival of Complex Organic Molecules in the Jovian Circumplanetary Disk
Europa, Ganymede, and Callisto are key targets in the search for habitability due to the potential presence of subsurface oceans. Detecting complex organic molecules (COMs), essential for prebiotic chemistry, is […]
Circumplanetary Disk Candidate In The Disk of HD 163296 Traced By Localized Emission From Simple Organics
Atacama Large Millimeter/submillimeter Array observations suggest that the disc of HD 163296 is being actively shaped by embedded, yet unseen protoplanets, as indicated by numerous gas and dust substructures consistent […]
JWST-TST High Contrast: Medium-resolution Spectroscopy Reveals a Carbon-rich Circumplanetary Disk Around The Young Accreting Exoplanet Delorme 1 AB b
Young accreting planetary-mass objects are thought to draw material from a circumplanetary disk (CPD) composed of gas and dust.
A Carbon-rich Disk Surrounding A Planetary-mass Companion
During the final assembly of gas giant planets, circumplanetary disks (CPDs) of gas and dust form due to the conservation of angular momentum, providing material to be accreted onto the […]
On the Detection Of Exorings in Reflected Light With JWST NIRCam
When directly imaging a cold giant exoplanet hosting a ring system, the reflected light from the rings can outshine the planet’s thermal emission and reflected-light in the near-infrared.
Studying Protoplanets and Protoplanetary Disks with the Habitable Worlds Observatory
Since the discovery of the first exoplanet orbiting a Sun-like star, the confirmation of nearly 6000 exoplanets to date – and their diversity – has revolutionized our knowledge of planetary […]
Formation Of Habitable Moons Around Giant Planets
Of the few thousand discovered exoplanets, a significant number orbit in the habitable zone of their star.
