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[1] 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 J0855-0714 | 225–260[2] | Y4 | 7.27±0.13 | |
WISE 0336-0143B[3] | 295±10[4] | Y1? | 32.7[1] | 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[5] Might be a later spectral type. |
WISEA 0830+2837 | 300-350[6] | >Y1[1] | 26.87[1] | uncertain parallax and spectral type is an estimate |
CWISEP 0238-1332[1] | 367±79 | >Y1 | 58.66 | uncertain parallax and spectral type is an estimate |
CWISEP 0402-2651[1] | 367±79 | >Y1 | 39.53 | uncertain parallax and spectral type is an estimate |
WISEU 0503-5648[1] | 367±79 | >Y1 | 33.18 | spectral type is an estimate |
CWISEP 0940+5233[1] | 367±79 | >Y1 | 43.49 | uncertain parallax and spectral type is an estimate |
WISEA 1257+7153[1] | 367±79 | >Y1 | 54.18 | spectral type is an estimate |
CWISEP 1446-2317[1] | 367±79 | >Y1 | 37.75 | uncertain parallax and spectral type is an estimate |
WISEA 1930-2059[1] | 367±79 | >Y1 | 30.67 | spectral type is an estimate |
CWISEP 1935-1546[1] | 367±79 | >Y1 | 47.06 | spectral type is an estimate |
CWISEP 2230+2549[1] | 367±79 | >Y1 | 52.44 | uncertain parallax and spectral type is an estimate |
CWISEP 2256+4002[1] | 367±79 | >Y1 | 32.04 | spectral type is an estimate |
CFBDSIR 1458+10B | 370 | Y0 | 104 | |
WISE 0825+2805[1] | 376±88 | Y0.5 | 21.37 | |
WD 0806-661B[1] | 377±88 | Y1 | 62.80 | spectral type is an estimate |
WISE 0350-5658[1] | 388±88 | Y1 | 18.49 | |
WISEA 2354+0240[1] | 388±88 | Y1 | 24.97 | |
WISE 2209+2711[1] | 389±88 | Y0: | 20.17 | |
WISE 0647-6232[1] | 393±88 | Y1 | 32.78 | |
WISEPA 1541-2250[1] | 395±88 | Y1 | 19.54 | |
WISE 1828+2650 | 406±88[1] | Y2V[7] | 32.5 | Temperature could be lower. If it is a binary, its components could be as cold as about 275-350 K.[8] |
WISE 0535-7500[1] | 410±88 | >=Y1: | 47.48 | |
WISE 1405+5534 | 411±88[1] | Y0.5(pec?)[1] | 20.62 | |
CWISEP 0321+6932[1] | 412±79 | Y0.5 | 47.61 | spectral type is an estimate |
WISE 1639-6847[1] | 412±88 | Y0pec | 14.85 | |
CWISEP 2356-4814[1] | 412±79 | Y0.5 | 56.62 | spectral type is an estimate |
WISE 0336-0143A[3] | 440±24[9] | Y0[1] | 32.7[1] | |
WISEPA 1738+2732[1] | 450±88 | Y0 | 24.92 | |
WISEPA 0410+1502[1] | 451±88 | Y0 | 21.56 | |
WISE 2220-3628[1] | 452±88 | Y0 | 34.15 | |
WISE 1534-1043 | 453±77[10] | sdY? | 53 | possibly halo brown dwarf |
WISE 1206+8401[1] | 454±88 | Y0 | 38.51 | |
WISE 0146+4234B[1] | 460±79 | Y0 | 63.09 | |
WISEA 0302-5817[1] | 460±79 | Y0: | 54.45 | |
CWISEP 0634+5049[1] | 460±79 | Y0 | 52.61 | spectral type is an estimate |
CWISEP 0859+5349[1] | 460±79 | Y0 | 60.62 | spectral type is an estimate |
CWISE 0925-4720[1] | 460±79 | Y0 | 34.96 | spectral type is an estimate |
CWISEP 0938+0634[1] | 460±79 | Y0 | 61.31 | uncertain parallax and spectral type is an estimate |
CWISEP 1047+5457[1] | 460±79 | Y0 | 43.37 | spectral type is an estimate |
CWISE 1121-6232[1] | 460±79 | Y0 | 33.69 | spectral type is an estimate |
WISEA 1141-3326[1] | 460±79 | Y0 | 31.36 | |
WISE 1217+1626 B | 460±79[1] | Y0-0.5 | 33 | |
CWISE 1531-3306[1] | 460±79 | Y0 | 55.37 | spectral type is an estimate |
WISENF 1936+0408[1] | 460±79 | Y0 | 28.64 | spectral type is an estimate |
CWISEP 2011-4812[1] | 460±79 | Y0 | 45.94 | spectral type is an estimate |
WISEA 2243-1458[1] | 460±79 | Y0 | 47,75 | spectral type is an estimate |
WISE 1112-3857[1] | 461±88 | T9 | 31.79 | |
WISE 0734-7157[1] | 462±88 | Y0 | 43.78 | |
WISE 0713-2917[1] | 464±88 | Y0 | 29.84 | |
WISEPC 2056+1459[1] | 464±88 | Y0 | 23.16 | |
WISE 0304-2705[1] | 465±88 | Y0~pec | 44.62 | |
WISE 0359-5401 | 467+16 −18[11] |
Y0[1] | 44.31[1] | |
WISE 0943+3607[1] | 468±88 | T9.5 | 33.59 | |
WISE 0833+0052[1] | 472±88 | (sd)T9 | 40.92 | possible subdwarf |
WISE 1542+2230[1] | 472±88 | T9.5 | 38.69 | |
WISE 0811-8051[1] | 479±88 | T9.5: | 32.91 | |
WISEPA 2134-7137[1] | 481±88 | T9~pec | 29.73 | possible subdwarf |
WISE 2212-6931[1] | 487±88 | T9 | 40.47 | |
WISEPA 0751-7634[1] | 492±88 | T9 | 33.32 | |
WISE 0335+4310[1] | 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[12] | 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 | [13] |
2M 1237+6526 | 850[14] | T6.5 | 46 | |
2MASS J0348−6022 | 880 | T7[15] | 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[16] | L4[17] | 109 | |
S Cassiopeiae | 1,800 | S3,4–S5,8 | 3,100±300 | |
V384 Persei | 1,820[18] | N | ||
DENIS-P J1058.7−1548 | 1,850[19] | L3 | 49 | |
T Draconis | 1,850[18] | C6,2e | ||
V346 Puppis | 1,875[18] | C | ||
2MASS J0523-1403 | 1,939[20] | L2.5V | 41.62 | The coolest main sequence star known as of 2023. |
S Aurigae | 1,940[18] | C-N5+ | ||
V1426 Cygni | 1,975[18] | C7,2e |
See also
References
- 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 26 27 28 29 30 31 32 33 34 35 36 37 38 39 40 41 42 43 44 45 46 47 48 49 50 51 52 53 54 55 56 57 58 59 60 61 62 63 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.
- ↑ Clavin, Whitney; Harrington, J. D. (25 April 2014). "NASA's Spitzer and WISE Telescopes Find Close, Cold Neighbor of Sun". NASA.gov. Archived from the original on 26 April 2014.
- 1 2 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. arXiv:2309.14567.
- ↑ 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. arXiv:2309.14567.
- ↑ 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. 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.
- 1 2 3 4 5 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. doi:10.1088/0004-637X/810/2/158. ISSN 1538-4357.
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