In this article, we want to focus on List of coolest stars , a topic that has captured the attention of many people in recent times. As the world advances, List of coolest stars has become a point of interest for researchers, professionals and enthusiasts alike. Through this article, we will seek to explore various facets of List of coolest stars and its impact on society, economy, culture, and more. Different perspectives and opinions will be addressed to offer a complete overview of List of coolest stars and delve into its relevance today. With a critical and analytical eye, we hope to provide our readers with a more complete understanding of List of coolest stars and its importance in the modern world.
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.
Kirkpatrick et al. 2021 has a more complete list of nearby objects with a temperature below 2,400 K. Objects with a temperature below 500 K from this paper were included in this list.
List
Star name
Temperature
(K )
Spectral type
Distance (light years )
Notes
WISE 0855–0714
285
Y4
7.426± 0.039
WISE 0336-0143B
295± 10
Y1?
32.7
spectral 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.
WISEA 0830+2837
300-350
>Y1
26.87
uncertain parallax and spectral type is an estimate
CWISEP 0238-1332
367± 79
>Y1
58.66
uncertain parallax and spectral type is an estimate
CWISEP 0402-2651
367± 79
>Y1
39.53
uncertain parallax and spectral type is an estimate
WISEU 0503-5648
367± 79
>Y1
33.18
spectral type is an estimate
CWISEP 0940+5233
367± 79
>Y1
43.49
uncertain parallax and spectral type is an estimate
WISEA 1257+7153
367± 79
>Y1
54.18
spectral type is an estimate
CWISEP 1446-2317
367± 79
>Y1
37.75
uncertain parallax and spectral type is an estimate
WISEA 1930-2059
367± 79
>Y1
30.67
spectral type is an estimate
CWISEP 1935-1546
367± 79
>Y1
47.06
spectral type is an estimate
CWISEP 2230+2549
367± 79
>Y1
52.44
uncertain parallax and spectral type is an estimate
CWISEP 2256+4002
367± 79
>Y1
32.04
spectral type is an estimate
CFBDSIR 1458+10B
370
Y0
104
WISE 0825+2805
376± 88
Y0.5
21.37
WD 0806-661B
377± 88
Y1
62.80
spectral type is an estimate
WISE 0350-5658
388± 88
Y1
18.49
WISEA 2354+0240
388± 88
Y1
24.97
WISE 2209+2711
389± 88
Y0:
20.17
WISE 0647-6232
393± 88
Y1
32.78
WISEPA 1541-2250
395± 88
Y1
19.54
WISE 1828+2650
406± 88
Y2V
32.5
Temperature could be lower. If it is a binary, its components could be as cold as about 275-350 K.
WISE 0535-7500
410± 88
>=Y1:
47.48
WISE 1405+5534
411± 88
Y0.5(pec?)
20.62
CWISEP 0321+6932
412± 79
Y0.5
47.61
spectral type is an estimate
WISE 1639-6847
412± 88
Y0pec
14.85
CWISEP 2356-4814
412± 79
Y0.5
56.62
spectral type is an estimate
WISE 0336-0143A
440± 24
Y0
32.7
WISEPA 1738+2732
450± 88
Y0
24.92
WISEPA 0410+1502
451± 88
Y0
21.56
WISE 2220-3628
452± 88
Y0
34.15
WISE 1534-1043
453± 77
sdY?
53
possibly halo brown dwarf
WISE 1206+8401
454± 88
Y0
38.51
WISE 0146+4234B
460± 79
Y0
63.09
WISEA 0302-5817
460± 79
Y0:
54.45
CWISEP 0634+5049
460± 79
Y0
52.61
spectral type is an estimate
CWISEP 0859+5349
460± 79
Y0
60.62
spectral type is an estimate
CWISE 0925-4720
460± 79
Y0
34.96
spectral type is an estimate
CWISEP 0938+0634
460± 79
Y0
61.31
uncertain parallax and spectral type is an estimate
CWISEP 1047+5457
460± 79
Y0
43.37
spectral type is an estimate
CWISE 1121-6232
460± 79
Y0
33.69
spectral type is an estimate
WISEA 1141-3326
460± 79
Y0
31.36
WISE 1217+1626 B
460± 79
Y0-0.5
33
CWISE 1531-3306
460± 79
Y0
55.37
spectral type is an estimate
WISENF 1936+0408
460± 79
Y0
28.64
spectral type is an estimate
CWISEP 2011-4812
460± 79
Y0
45.94
spectral type is an estimate
WISEA 2243-1458
460± 79
Y0
47,75
spectral type is an estimate
WISE 1112-3857
461± 88
T9
31.79
WISE 0734-7157
462± 88
Y0
43.78
WISE 0713-2917
464± 88
Y0
29.84
WISEPC 2056+1459
464± 88
Y0
23.16
WISE 0304-2705
465± 88
Y0~pec
44.62
WISE 0359-5401
467+16 −18
Y0
44.31
WISE 0943+3607
468± 88
T9.5
33.59
WISE 0833+0052
472± 88
(sd)T9
40.92
possible subdwarf
WISE 1542+2230
472± 88
T9.5
38.69
WISE 0811-8051
479± 88
T9.5:
32.91
WISEPA 2134-7137
481± 88
T9~pec
29.73
possible subdwarf
WISE 2212-6931
487± 88
T9
40.47
WISEPA 0751-7634
492± 88
T9
33.32
WISE 0335+4310
492± 88
T9
38.46
WISE 1217+1626 A
575
T8.5-9
33
UGPS J0521+3640
600–650
T8.5
26.7
2MASS 0939-2448 A/B
650
T8
17.4± 0.4
2MASS 0415-0935
764
T8V
18.6± 0.2
54 Piscium B
810 ± 50
T7.5V
36.32± 0.02
2M 1237+6526
850
T6.5
46
2MASS J0348−6022
880
T7
27.2
SCR 1845-6357B
950
T6
13.050± 0.008
Epsilon Indi Bb
993
T6
12.05
2MASS 0243-2453
1,050
T6
35± 1
Cha 110913-773444
1,350
M9.5
529
Epsilon Indi Ba
1,353
T1-1.5
12.05
2MASS 0036+1821
1,650
L3.5
28.51± 0.05
2MASS 1507-1627
1,650
L5
24.12± 0.06
OTS 44
1,700
M9.5
554
GD 165 B
1,755
L4
109
S Cassiopeiae
1,800
S3,4–S5,8
3,100± 300
V384 Persei
1,820
N
DENIS-P J1058.7−1548
1,850
L3
49
T Draconis
1,850
C6,2e
V346 Puppis
1,875
C
2MASS J0523-1403
1,939
L2.5V
41.62
The coolest main sequence star known as of 2023.
S Aurigae
1,940
C-N5+
V1426 Cygni
1,975
C7,2e
See also
References
^ a b c d e f g h i j k l m n o p q r s t u v w x y z aa ab ac ad ae af ag ah ai aj ak al am an ao ap aq ar as at au av aw ax ay az ba bb bc bd be bf bg bh bi bj bk Kirkpatrick, J. Davy; Gelino, Christopher R.; Faherty, Jacqueline K.; Meisner, Aaron M.; Caselden, Dan; Schneider, Adam C.; Marocco, Federico; Cayago, Alfred J.; Smart, R. L.; Eisenhardt, Peter R.; Kuchner, Marc J.; Wright, Edward L.; Cushing, Michael C.; Allers, Katelyn N.; Gagliuffi, Daniella C. Bardalez (2021-03-01). "The Field Substellar Mass Function Based on the Full-sky 20-pc Census of 525 L, T, and Y Dwarfs" . The Astrophysical Journal Supplement Series . 253 (1): 7. arXiv :2011.11616 . Bibcode :2021ApJS..253....7K . doi :10.3847/1538-4365/abd107 . ISSN 0067-0049 . S2CID 227126954 .
^ Luhman, K. L.; Tremblin, P.; Alves de Oliveira, C.; Birkmann, S. M.; Baraffe, I.; Chabrier, G.; Manjavacas, E.; Parker, R. J.; Valenti, J. (2023-12-05). "JWST/NIRSpec Observations of the Coldest Known Brown Dwarf*" . The Astronomical Journal . 167 (1): 5. arXiv :2311.17316 . doi :10.3847/1538-3881/ad0b72 . ISSN 0004-6256 .
^ a b Calissendorff, Per; De Furio, Matthew; Meyer, Michael; Albert, Loïc; Aganze, Christian; Ali-Dib, Mohamad; Bardalez Gagliuffi, Daniella C.; Baron, Frederique; Beichman, Charles A.; Burgasser, Adam J.; Cushing, Michael C.; Faherty, Jacqueline Kelly; Fontanive, Clémence; Gelino, Christopher R.; Gizis, John E. (2023-04-01). "JWST/NIRCam Discovery of the First Y+Y Brown Dwarf Binary: WISE J033605.05-014350.4" . The Astrophysical Journal . 947 (2): L30. arXiv :2303.16923 . Bibcode :2023ApJ...947L..30C . doi :10.3847/2041-8213/acc86d . ISSN 0004-637X .
^ Leggett, S. K.; Tremblin, Pascal (25 Sep 2023). "The First Y Dwarf Data From JWST Show That Dynamic and Diabatic Processes Regulate Cold Brown Dwarf Atmospheres" . ApJ . 959 (2): 86. arXiv :2309.14567 . Bibcode :2023ApJ...959...86L . doi :10.3847/1538-4357/acfdad .
^ Kirkpatrick, J. Davy; Gelino, Christopher R.; Cushing, Michael C.; Mace, Gregory N.; Griffith, Roger L.; Skrutskie, Michael F.; Marsh, Kenneth A.; Wright, Edward L.; Eisenhardt, Peter R.; McLean, Ian S.; Mainzer, Amanda K.; Burgasser, Adam J.; Tinney, C. G.; Parker, Stephen; Salter, Graeme (2012-07-01). "Further Defining Spectral Type "Y" and Exploring the Low-mass End of the Field Brown Dwarf Mass Function" . The Astrophysical Journal . 753 (2): 156. arXiv :1205.2122 . Bibcode :2012ApJ...753..156K . doi :10.1088/0004-637X/753/2/156 . ISSN 0004-637X .
^ Bardalez Gagliuffi, Daniella C.; Faherty, Jacqueline K.; Schneider, Adam C.; Meisner, Aaron; Caselden, Dan; Colin, Guillaume; Goodman, Sam; Kirkpatrick, J. Davy; Kuchner, Marc; Gagné, Jonathan; Logsdon, Sarah E.; Burgasser, Adam J.; Allers, Katelyn; Debes, John; Wisniewski, John (2020-06-01). "WISEA J083011.95+283716.0: A Missing Link Planetary-mass Object" . The Astrophysical Journal . 895 (2): 145. arXiv :2004.12829 . Bibcode :2020ApJ...895..145B . doi :10.3847/1538-4357/ab8d25 . ISSN 0004-637X .
^ Beichman, Charles A.; Gelino, Christopher R.; Kirkpatrick, J. Davy; Barman, Travis S.; Marsh, Kenneth A.; Cushing, Michael C.; Wright, E. L. (2013-01-29). "The Coldest Brown Dwarf (Or Free Floating Planet)?: The Y Dwarf WISE 1828+2650". The Astrophysical Journal . 764 (1): 101. arXiv :1301.1669 . Bibcode :2013ApJ...764..101B . doi :10.1088/0004-637X/764/1/101 . ISSN 0004-637X . S2CID 118575478 .
^ Cushing, Michael C.; Schneider, Adam C.; Kirkpatrick, J. Davy; Morley, Caroline V.; Marley, Mark S.; Gelino, Christopher R.; Mace, Gregory N.; Wright, Edward L.; Eisenhardt, Peter R.; Skrutskie, Michael F.; Marsh, Kenneth A. (2021-10-01). "An Improved Near-infrared Spectrum of the Archetype Y Dwarf WISEP J182831.08+265037.8" . The Astrophysical Journal . 920 (1): 20. arXiv :2107.00506 . Bibcode :2021ApJ...920...20C . doi :10.3847/1538-4357/ac12cb . ISSN 0004-637X .
^ Leggett, S. K.; Tremblin, Pascal (25 Sep 2023). "The First Y Dwarf Data From JWST Show That Dynamic and Diabatic Processes Regulate Cold Brown Dwarf Atmospheres" . ApJ . 959 (2): 86. arXiv :2309.14567 . Bibcode :2023ApJ...959...86L . doi :10.3847/1538-4357/acfdad .
^ Meisner, Aaron M.; Leggett, S. K.; Logsdon, Sarah E.; Schneider, Adam C.; Tremblin, Pascal; Phillips, Mark (2023-08-01). "Exploring the Extremes: Characterizing a New Population of Old and Cold Brown Dwarfs" . The Astronomical Journal . 166 (2): 57. arXiv :2301.09817 . Bibcode :2023AJ....166...57M . doi :10.3847/1538-3881/acdb68 . ISSN 0004-6256 .
^ Beiler, Samuel A.; Cushing, Michael C.; Kirkpatrick, J. Davy; Schneider, Adam C.; Mukherjee, Sagnick; Marley, Mark S. (2023-07-01). "The First JWST Spectral Energy Distribution of a Y Dwarf" . The Astrophysical Journal . 951 (2): L48. arXiv :2306.11807 . Bibcode :2023ApJ...951L..48B . doi :10.3847/2041-8213/ace32c . ISSN 0004-637X .
^ Leggett, Sandy K.; Cushing, Michael C.; Saumon, Didier; Marley, Mark S.; Roellig, Thomas L.; Warren, Stephen J.; Burningham, Ben; Jones, Hugh R. A.; Kirkpatrick, J. Davy; Lodieu, Nicolas; Lucas, Philip W.; Mainzer, Amy K.; Martín, Eduardo L.; McCaughrean, Mark J.; Pinfield, David J.; Sloan, Gregory C.; Smart, Richard L.; Tamura, Motohide; Van Cleve, Jeffrey E. (2009). "The Physical Properties of Four ~600 K T Dwarfs". The Astrophysical Journal . 695 (2): 1517–1526. arXiv :0901.4093 . Bibcode :2009ApJ...695.1517L . doi :10.1088/0004-637X/695/2/1517 . S2CID 44050900 .
^ Luhman, K. L.; Patten, B. M.; Marengo, M.; Schuster, M. T.; Hora, J. L.; Ellis, R. G.; Stauffer, J. R.; Sonnett, S. M.; Winston, E.; Gutermuth, R. A.; Megeath, S. T.; Backman, D. E.; Henry, T. J.; Werner, M. W.; Fazio, G. G. (January 2007). "Discovery of Two T Dwarf Companions with the Spitzer Space Telescope" . The Astrophysical Journal . 654 (1): 570–579. arXiv :astro-ph/0609464 . Bibcode :2007ApJ...654..570L . doi :10.1086/509073 . ISSN 0004-637X .
^ Liebert & Burgasser (2007). "On the Nature of the Unique Hα-emitting T Dwarf 2MASS J12373919+6526148". Astronomy & Astrophysics . 655 (1): 522–527. arXiv :astro-ph/0609793 . Bibcode :2007ApJ...655..522L . doi :10.1086/509882 . S2CID 18852560 .
^ Tannock, Megan E.; Metchev, Stanimir; Heinze, Aren; Miles-Páez, Paulo A.; Gagné, Jonathan; Burgasser, Adam; Marley, Mark S.; Apai, Dániel; Suárez, Genaro; Plavchan, Peter (2021-05-01). "Weather on Other Worlds. V. The Three Most Rapidly Rotating Ultra-Cool Dwarfs" . The Astronomical Journal . 161 (5): 224. arXiv :2103.01990 . Bibcode :2021AJ....161..224T . doi :10.3847/1538-3881/abeb67 . ISSN 0004-6256 . S2CID 232105126 .
^ Filippazzo, Joseph C.; Rice, Emily L.; Faherty, Jacqueline; Cruz, Kelle L.; Van Gordon, Mollie M.; Looper, Dagny L. (2015-09-10). "Fundamental Parameters and Spectral Energy Distributions of Young and Field Age Objects with Masses Spanning the Stellar to Planetary Regime". The Astrophysical Journal . 810 (2): 158. arXiv :1508.01767 . Bibcode :2015ApJ...810..158F . doi :10.1088/0004-637X/810/2/158 . ISSN 1538-4357 . S2CID 89611607 .
^ Kirkpatrick, J. Davy; Reid, I. Neill; Liebert, James; Cutri, Roc M.; Nelson, Brant; Beichman, Charles A.; Dahn, Conard C.; Monet, David G.; Gizis, John E.; Skrutskie, Michael F. (1999-07-01). "Dwarfs Cooler than M : The Definition of Spectral Type L Using Discoveries from the 2 Micron All-Sky Survey (2MASS)" . The Astrophysical Journal . 519 (2): 802–833. Bibcode :1999ApJ...519..802K . doi :10.1086/307414 . ISSN 0004-637X . S2CID 73569208 .
^ a b c d e Bergeat, J.; Chevallier, L. (2005). "The mass loss of C-rich giants". Astronomy and Astrophysics . 429 : 235–246. arXiv :astro-ph/0601366 . Bibcode :2005A&A...429..235B . doi :10.1051/0004-6361:20041280 . S2CID 56424665 .
^ Heinze, Aren N.; Metchev, Stanimir; Apai, Daniel; Flateau, Davin; Kurtev, Radostin; Marley, Mark; Radigan, Jacqueline; Burgasser, Adam J.; Artigau, Étienne; Plavchan, Peter (2013-04-08). "Weather on Other Worlds I: Detection of Periodic Variability in the L3 Dwarf DENIS-P J1058.7-1548 with Precise Multi-Wavelength Photometry". The Astrophysical Journal . 767 (2): 173. arXiv :1303.2948 . Bibcode :2013ApJ...767..173H . doi :10.1088/0004-637X/767/2/173 . ISSN 0004-637X . S2CID 29406867 .
^ Filippazzo, Joseph C.; Rice, Emily L.; Faherty, Jacqueline; Cruz, Kelle L.; Van Gordon, Mollie M.; Looper, Dagny L. (2015-09-10). "Fundamental Parameters and Spectral Energy Distributions of Young and Field Age Objects with Masses Spanning the Stellar to Planetary Regime". The Astrophysical Journal . 810 (2): 158. arXiv :1508.01767 . Bibcode :2015ApJ...810..158F . doi :10.1088/0004-637X/810/2/158 . ISSN 1538-4357 .