List of coolest stars


This is a list of coolest stars and brown dwarfs discovered, arranged by decreasing temperature. The stars with temperatures lower than 2,000 K are included.

Coolest [main sequence] stars

Include stars with temperatures lower than 2,500 Kelvin.
Star nameTemperature
Spectral typeDistance Notes
CWISE J1249+36211,715-2,320sdL1408
2MASS J0523-14031,939L2.5V41.62The coolest main sequence star known as of 2023.

Coolest [giant star]s

Include giants with temperatures lower than 2,000 Kelvin.
Star nameTemperature
Spectral typeDistance Notes
S Cassiopeiae1,800S3,4–S5,8
LL Pegasi1,800C4,200
RW Leonis Minoris1,800C4,31,053
1,800C6,2e_MS3
V384 Persei1,820N
T Draconis1,850C6,2e
V346 Puppis1,875C
Leo A 221,900C2,600,000
S Aurigae1,940C-N5+
V1426 Cygni1,975C7,2e-
Sextans A 202,000C4,310,000
Leo A 2262,000C2,600,000
Sextans A 1002,000C4,310,000
IRC +303742,000C3,900
IRC +601442,000C3,400
CZ Hydrae2,000C7,200
SS Virginis2,000C-N4.52,100

Coolest brown dwarfs and rogue planets

Include brown dwarfs with temperatures lower than 500 Kelvin.
Star nameTemperature
Spectral typeDistance Notes
285Y4
WISE 0336-0143BY1?32.7spectral type is not yet published, but should be around Y1 if we assume MIRI F480M is similar to W2 and by using Figure 13 from Kirkpatrick et al. 2012 Might be a later spectral type.
WISE J0830+2837300-350>Y126.87uncertain parallax and spectral type is an estimate
CWISEP 0238-1332>Y158.66uncertain parallax and spectral type is an estimate
CWISEP 0402-2651>Y139.53uncertain parallax and spectral type is an estimate
WISEU 0503-5648>Y133.18spectral type is an estimate
CWISEP 0940+5233>Y143.49uncertain parallax and spectral type is an estimate
WISEA 1257+7153>Y154.18spectral type is an estimate
CWISEP J1446−2317>Y137.75uncertain parallax and spectral type is an estimate
WISEA 1930-2059>Y130.67spectral type is an estimate
CWISEP 1935-1546>Y147.06spectral type is an estimate
CWISEP 2230+2549>Y152.44uncertain parallax and spectral type is an estimate
CWISEP 2256+4002>Y132.04spectral type is an estimate
WISE 0825+2805Y0.521.37
WD 0806-661BY162.80spectral type is an estimate
WISE 0350-5658Y118.49
WISE J2354+0240Y124.97
WISE 2209+2711Y0:20.17
WISE 0647-6232Y132.78
WISEPA 1541-2250Y119.54
WISE 1828+2650Y2V32.5Temperature could be lower. If it is a binary, its components could be as cold as about 275-350 K.
WISE 0535-7500>=Y1:47.48
WISE 1405+5534Y0.520.62
CWISEP 0321+6932Y0.547.61spectral type is an estimate
WISE 1639-6847Y0pec14.85
CWISEP 2356-4814Y0.556.62spectral type is an estimate
WISE 0336-0143AY032.7
WISEPA 1738+2732Y024.92
WISEPA 0410+1502Y021.56
WISE 2220-3628Y034.15
WISE 1534-1043sdY?53possibly halo brown dwarf
WISE J1206+8401Y038.51
WISE 0146+4234BY063.09
WISEA 0302-5817Y0:54.45
CWISEP 0634+5049Y052.61spectral type is an estimate
CWISEP 0859+5349Y060.62spectral type is an estimate
CWISE 0925-4720Y034.96spectral type is an estimate
CWISEP 0938+0634Y061.31uncertain parallax and spectral type is an estimate
CWISEP J1047+5457Y043.37spectral type is an estimate
CWISE 1121-6232Y033.69spectral type is an estimate
WISEA J1141−3326Y031.36
WISE 1217+1626 BY0-0.533
CWISE 1531-3306Y055.37spectral type is an estimate
WISENF 1936+0408Y028.64spectral type is an estimate
CWISEP 2011-4812Y045.94spectral type is an estimate
WISEA 2243-1458Y047,75spectral type is an estimate
WISE 1112-3857T931.79
WISE 0734-7157Y043.78
WISE 0713-2917Y029.84
WISEPC 2056+1459Y023.16
WISE J0304−2705Y0~pec44.62
WISE 0359-5401Y044.31
WISE 0943+3607T9.533.59
WISE 0833+0052T940.92possible subdwarf
WISE 1542+2230T9.538.69
WISE 0811-8051T9.5:32.91
WISEPA 2134-7137T9~pec29.73possible subdwarf
WISE 2212-6931T940.47
WISEPA 0751-7634T933.32
WISE 0335+4310T938.46