In 1984, the first debris disk orbiting another star was observed around Vega. Think of a debris disk as the leftovers from solar system formation, analogous to the asteroid or Kuiper belts.
Using the Keck Planet Imager and Characterizer (KPIC), astronomers have performed high-resolution spectroscopic observations ...
A study analyzed 178 debris-disc systems and found that many of these disks likely require the presence of Neptune- to Saturn-mass planets at distances of 10 to 100 astronomical units (au ...
This image of the dusty debris disk surrounding the young star Fomalhaut is from Webb’s Mid-Infrared Instrument (MIRI). It reveals three nested belts extending out to 14 billion miles (23 ...
As Isabel Rebollido, lead author on the new research, explains, “Beta Pictoris is the debris disk that has it all: It has a really bright, close star that we can study very well, and a complex ...
The architecture of the Fomalhaut debris disk system. We highlight the various features identified ... [+] in the JWST/MIRI observations of the Fomalhaut system in this 25.5 μm image.
HD 206893 is orbited by two exoplanets and also hosts a circumstellar debris disk extending from about 30 to 180 AU from the star. HD 206893 B, estimated to be 26 times more massive than Jupiter ...