CFHTWIR-Oph 98 b explained

CFHTWIR-Oph 98 B
Discovery Method:Direct imaging
Discovered:2020
Discoverer:Fontanive et al.
Extrasolarplanet:yes
Semimajor: AU (mean separation)
Star:CFHTWIR-Oph 98 A
Spectral Type:L2-L6

CFHTWIR-Oph 98 B is a substellar object, either an exoplanet or a sub-brown dwarf that orbits CFHTWIR-Oph 98 A, a M-type brown dwarf.[1] The pair form a binary system.

Formation

It orbits a star but its formation as an exoplanet is challenging or impossible.[2] If its formation scenario is known, it may explain the formation of Planet Nine. Planetary migration may explain its formation, or it may be a brown dwarf.

See also

Notes

  1. Encyclopedia: The Extrasolar Planet Encyclopaedia — CFHTWIR-Oph 98 b . . 11 September 2023.
  2. Fontanive . Clémence . Allers . Katelyn N. . Pantoja . Blake . Biller . Beth . Dubber . Sophie . Zhang . Zhoujian . Dupuy . Trent . Liu . Michael C. . Albert . Loïc . 2020-12-01 . A Wide Planetary-mass Companion to a Young Low-mass Brown Dwarf in Ophiuchus . The Astrophysical Journal . 905 . 2 . L14 . 10.3847/2041-8213/abcaf8 . 0004-637X. free . 2011.08871 . 2020ApJ...905L..14F .