A circumplanetary disk (or circumplanetary disc, short CPD) is a torus, pancake or ring-shaped accumulation of matter composed of gas, dust, planetesimals, asteroids or collision fragments in orbit around a planet. They are reservoirs of material out of which moons (or exomoons or subsatellites) may form.[1] Such a disk can manifest itself in various ways.
In August 2018, astronomers reported the probable detection of a circumplanetary disk around CS Cha B.[2] The authors state that "The CS Cha system is the only system in which a circumplanetary disc is likely present as well as a resolved circumstellar disc."[3] In 2020 though, the parameters of CS Cha B were revised, making it an accreting red dwarf star, and making the disk circumstellar.[4]
^Parks, Jake (8 November 2021). "Snapshot: ALMA spots moon-forming disk around distant exoplanet - This stellar shot serves as the first unambiguous detection of a circumplanetary disk capable of brewing its own moon". Astronomy. Retrieved 9 November 2021.
^Ginski, Christian (August 2018). "First direct detection of a polarized companion outside a resolved circumbinary disk around CS Chamaeleonis". Astronomy & Astrophysics. 616 (79): 18. arXiv:1805.02261. Bibcode:2018A&A...616A..79G. doi:10.1051/0004-6361/201732417.
^Starr, Michelle. "Astronomers Have Accidentally Taken a Direct Photo of a Possible Baby Exoplanet". Retrieved 10 October 2019.
^Haffert, S. Y.; Van Holstein, R. G.; Ginski, C.; Brinchmann, J.; Snellen, I. A. G.; Milli, J.; Stolker, T.; Keller, C. U.; Girard, J. (2020), "CS Cha B: A disc-obscured M-type star mimicking a polarised planetary companion", Astronomy & Astrophysics, 640: L12, arXiv:2007.07831, Bibcode:2020A&A...640L..12H, doi:10.1051/0004-6361/202038706, S2CID 220525346
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A circumplanetarydisk (or circumplanetary disc, short CPD) is a torus, pancake or ring-shaped accumulation of matter composed of gas, dust, planetesimals...
a moon-forming circumplanetarydisk. The disk was detected around PDS 70 c, with a potential disk observed around PDS 70 b. The disk was confirmed by...
of satellite systems around giant planets such as of Saturn, or circumplanetarydisks. But they can also be galactic rings and circumstellar discs, belts...
the disk. Excretion disks are formed when stars merge. Accretion Astrophysical jet Blandford–Znajek process Circumstellar disc Circumplanetarydisk Dynamo...
smaller, circumplanetary analogs of the protoplanetary disks. The formation of planets and moons in geometrically thin, gas- and dust-rich disks is the...
planet formation observationally. The flux from HD 100546 b and its circumplanetarydisk (CPD) are superimposed, leaving its properties such the radius and...
protostellar jets, and inclined orbits of circumplanetary objects (as seen in the eclipsing binary TY CrA). For disks orbiting a low secondary-to-primary mass...
aligned with the giant planet's equator because these formed in circumplanetarydisks. Planets close to their stars on circular orbits will tend to despin...
out of a nebula to create a young protostar orbited by a protoplanetary disk. There are eight planets within the Solar System; planets outside of the...
in the literature on roundness are italicized in the table below. Circumplanetarydisk – Accumulation of matter around a planet Co-orbital moon – Configuration...
1 AU. Accretion disk Asteroid belt Circumplanetarydisk – Accumulation of matter around a planet Exoasteroid belt Protoplanetary disk Wang, Z.; Chakrabarty...
aligned with the giant planet's equator, because these formed in circumplanetarydisks. Strictly speaking, this applies only to regular satellites. Captured...
into interstellar space. Following the dissipation of the protoplanetary disk, the Nice model proposes that gravitational encounters between planetisimals...
nebula to create a young protostar orbited by a protoplanetary disk. Planets grow in this disk by the gradual accumulation of material driven by gravity,...
believed to have formed from a circumplanetarydisk, a ring of accreting gas and solid debris analogous to a protoplanetary disk. They may be the remnants...
self-gravitating, spherically symmetric polytropic fluid Synestia Circumplanetarydisk – Accumulation of matter around a planet Second Borel–Cantelli Lemma...
planet. They considered two models to explain the SED: (1) a large circumplanetarydisk around a massive, but unseen, planet and (2) the aftermath of a collision...
Wars, the moon Ajan Kloss has two moons of its own. Binary asteroid Circumplanetarydisk – Accumulation of matter around a planet Minor-planet moon Moons...
ALMA at Planet-forming Scales (MAPS): A CircumplanetaryDisk Candidate in Molecular-line Emission in the AS 209 Disk". The Astrophysical Journal Letters....
eventually surround the parent star in the form of a circumstellar disk or debris disk. As a consequence, the orbiting debris field may be an "uneven ring...
ISBN 978-0-14-341421-6. Joshua Rapp Learn (May 11, 2021). "The Nebra Sky Disk: Is the world's oldest star map really a map at all?". Astronomy Today. Retrieved...
believed to have formed from a circumplanetarydisk, a ring of accreting gas and solid debris analogous to a protoplanetary disk. They may be the remnants...
Chronology of the universe – History and future of the universe Circumplanetarydisk – Accumulation of matter around a planet Cosmology – Scientific study...