Sub-stellar object
A substellar object, sometimes called a substar, is an astronomical object whose mass is smaller than the smallest mass at which hydrogen fusion can be sustained (approximately 0.08 solar masses). This definition includes brown dwarfs, former stars similar to EF Eridani B, and can also include objects of planetary mass, regardless of their formation mechanism and whether or not they are associated with a primary star.
Uses material from the Wikipedia article "Sub-stellar object", which is released under the Creative Commons BY-SA 3.0.Astronomical object | Distance | Wiki | ||
---|---|---|---|---|
Aegir | Extra-solar Planet Candidate, Extra-solar Confirmed Planet | 187 | [x] | |
BD+47 2936 | Extra-solar Planet Candidate | K | 122 | |
HAT-P-15 | Extra-solar Planet Candidate | G | 190 | |
HAT-P-2 | Extra-solar Planet Candidate | F | 373 | [x] |
HAT-P-3 | Extra-solar Planet Candidate | K | 457 | [x] |
OGLE-05-071L | Extra-solar Planet Candidate, Extra-solar Confirmed Planet | 11000 | [x] | |
Osiris | Extra-solar Planet Candidate, Extra-solar Confirmed Planet | 101 | ||
WASP-11 | Extra-solar Planet Candidate | K | 408 | [x] |