From Wikipedia, the free encyclopedia
The following are lists of stars .
Stars are
astronomical objects that spend some portion of their existence generating
energy through
thermonuclear fusion .
By physical characteristic
By variability or other factor
The following is a list of particularly notable actual or hypothetical
stars that have their own articles in Wikipedia, but are not included in the lists above.
Specific
International Astronomical Union:
IAU
Sol Station — information on nearby and bright stars.
Primary member
type
Celestial objects by systems. Secondary members are listed in small print.
Main-sequence stars
G-type
Tau Ceti (11.9118± 0.0074 ly)
4 (8?) planets: (b), (c), (d), e, f, g, h, (i)
K-type
M-type(red dwarfs)
Ross 248 (10.3057± 0.0014 ly)
Lacaille 9352 (10.7241± 0.0007 ly)
2 (3?) planets: b, c, d?
Ross 128 (11.0074± 0.0011 ly)
planet
b
EZ Aquarii (11.109± 0.034 ly)
2 red dwarfs: B, C
Struve 2398 (11.4908± 0.0009 ly)
red dwarf B
2? planets: Bb?, Bc?
Groombridge 34 (11.6191± 0.0008 ly)
red dwarf B
2 planets:
Ab ,
Ac
DX Cancri (11.6797± 0.0027 ly)
GJ 1061 (11.9839± 0.0014 ly)
3 planets: b, c, d
YZ Ceti (12.1222± 0.0015 ly)
3 planets: b, c, d
Luyten's Star (12.3485± 0.0019 ly)
2 (4?) planets:
b , c, d?, e?
Teegarden's Star (12.4970± 0.0045 ly)
2 planets:
b ,
c
Kapteyn's Star (12.8308± 0.0008 ly)
Lacaille 8760 (12.9472± 0.0018 ly)
SCR 1845−6357 (13.0638± 0.0070 ly)
T-type brown dwarf B
Kruger 60 (13.0724± 0.0052 ly)
red dwarf B
DENIS J1048−3956 (13.1932± 0.0027 ly)
Ross 614 (13.363± 0.040 ly)
red dwarf B
Wolf 1061 (14.0500± 0.0016 ly)
3 planets:
b ,
c ,
d
Gliese 1 (14.1747± 0.0022 ly)
TZ Arietis (14.5780± 0.0046 ly)
planet b
Wolf 424 (14.595± 0.031 ly)
red dwarf B
Gliese 687 (14.8395± 0.0014 ly)
2 planets: b, c
Gliese 674 (14.8492± 0.0018 ly)
planet
b
LHS 292 (14.8706± 0.0041 ly)