Debris disks contain the solid remnants of planet formation that are in collisional cascade, with particles ranging from kilometre - sized planetesimals down to micron - sized dust grains.
Not exact matches
Yet icy grains evaporate and collisions produce both gas and dust, so at some level all
debris disks must
contain some amount of gas.
Rieke notes that our solar system
contains a faint
debris disk of its own — micrometer - size dust particles slowly spiraling in toward the sun.
His calculations were the first to demonstrate that
debris disks around the nearby stars Vega and β Pictoris are newly - formed planetary systems
containing planets at least as large as Pluto and Mars.
In particular, I will focus on planets on eccentric orbits, not only because typical exoplanetary systems have been found to
contain these, but also because their interactions with
debris disks theoretically facilitates the transport of icy bodies within the habitable zone of planetary systems.
When researchers observed star systems
containing debris disks with giant exoplanets in distant orbits, they noted that the star systems had similar dual dust
disks analogous to the Solar System's two zones — the asteroid belt (between Mars and Jupiter) and the Kuiper Belt (beyond the orbit of Neptune).
Most galaxies in the observable universe
contain a supermassive black hole at their center, one that is either active and surrounded by an accretion
disk of dust, gas and other
debris, or is dormant — lurking at the center, patiently awaiting its next meal.
This large
debris disk is similar to the Kuiper Belt, which encircles the solar system and
contains a range of icy bodies from dust grains to objects the size of dwarf planets, such as Pluto.