Location of WISE 1541−2250 in the constellationLibra
Artist's vision of a Y-dwarf
WISE 1541−2250 (full designationWISEPA J154151.66−225025.2) is asub-brown orbrown dwarf ofspectral class Y0.5,[2] located in the constellationLibra at approximately 18.6light-years fromEarth.[5] This object received popular attention when its discovery was announced in 2011 at a distance estimated to be only about 9 light-years, which would have made it the closest brown dwarf known.[6] (For really close brown dwarfs see, for example,Luhman 16,WISE 1506+7027,Epsilon Indi Ba, Bb, orUGPS 0722-05). It is not the farthest known Y-type brown dwarf to Earth.
WISE 1541−2250 was discovered in 2011 from data collected by theWide-field Infrared Survey Explorer (WISE) in the infrared at a wavelength of 40 cm (16 in), whose mission lasted from December 2009 to February 2011. WISE 1541−2250 has two discovery papers: Kirkpatrick et al. (2011) and Cushing et al. (2011) with mostly the same authors and published nearly simultaneously.[1][4]
Cushing and collaborators presented the discovery of seven brown dwarfs, one of the T9.5 type and six of the Y-type, the first members of the Y spectral class discovered and spectroscopically confirmed, including an "archetypal member" of the Y spectral class,WISE 1828+2650, and WISE 1541−2250.[4] These seven objects are also the faintest seven of 98 brown dwarfs presented in Kirkpatrick et al. (2011).[1]
Currently the most accurate distance estimate of WISE 1541−2250 is atrigonometric parallax, published in 2014 by Tinneyet al.: 0.1751 ± 0.0044arcsec, corresponding to a distance 5.71+0.15 −0.14 pc, or 18.6 ± 0.5 ly.[5]
For several months after its discovery, before the publication of its parallax by Kirkpatrick et al. in 2012,[2] WISE 1541−2250 was considered to be the nearest known brown dwarf at approximately 9light-years from the Sun, and the seventh-nearest of all star systems, at slightly more than twice the distance of the nearest known star systemAlpha Centauri. This view existed because of a very rough preliminary parallax with a baseline of 1.2 years, published in the discovery paper: 0.351 ± 0.108arcsec, corresponding to a distance 2.8+1.3 −0.6 pc, or 9.3+4.1 −2.2 ly.[1] Also, there were other estimates: spectrophotometric distance estimate 8.2pc (26.7ly),[1] and photometric distance estimate 1.8+0.2 −0 pc (5.9+0.6 −0 ly).[4]
WISE 1541−2250 is among the first known examples of a Y-class brown dwarf, the coldest spectral class of stars, and has temperature about 350K[4] (about 77 °C / 170 °F). Its spectral class is Y0.5[2] (initially was estimated as Y0).[1][4] Modelling of WISE 1541−2250 has shown that there could be water clouds in the atmosphere of this brown dwarf. Models however struggle to reproduce the spectrum even with water clouds.[7]
^These 98 brown-dwarf systems are among the first brown-dwarf systems discovered in data collected by WISE and six discoveries were published earlier (however, also listed in Kirkpatrick et al. (2011)) in Mainzer et al. (2011) and Burgasser et al. (2011), and the other discoveries were published later.
^abcdefghijklmnoKirkpatrick, J. Davy; Cushing, Michael C.; Gelino, Christopher R.; Griffith, Roger L.; Skrutskie, Michael F.; Marsh, Kenneth A.; Wright, Edward L.; Mainzer, Amy K.; Eisenhardt, Peter R.; McLean, Ian S.; Thompson, Maggie A.; Bauer, James M.; Benford, Dominic J.; Bridge, Carrie R.; Lake, Sean E.; Petty, Sara M.; Stanford, Spencer Adam; Tsai, Chao-Wei; Bailey, Vanessa; Beichman, Charles A.; Bloom, Joshua S.; Bochanski, John J.; Burgasser, Adam J.; Capak, Peter L.; Cruz, Kelle L.; Hinz, Philip M.; Kartaltepe, Jeyhan S.; Knox, Russell P.; Manohar, Swarnima; Masters, Daniel; Morales-Calderon, Maria; Prato, Lisa A.; Rodigas, Timothy J.; Salvato, Mara; Schurr, Steven D.; Scoville, Nicholas Z.; Simcoe, Robert A.; Stapelfeldt, Karl R.; Stern, Daniel; Stock, Nathan D.; Vacca, William D. (2011). "The First Hundred Brown Dwarfs Discovered by the Wide-field Infrared Survey Explorer (WISE)".The Astrophysical Journal Supplement.197 (2): 19.arXiv:1108.4677v1.Bibcode:2011ApJS..197...19K.doi:10.1088/0067-0049/197/2/19.S2CID16850733.
^abcdKirkpatrick, 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, Amy K.; Burgasser, Adam J.; Tinney, Chris G.; Parker, Stephen; Salter, Graeme (2012). "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.S2CID119279752.
^abFontanive, Clémence; Bedin, Luigi R.; Albert, Loïc; Gagliuffi, Daniella C. Bardalez (2024-12-21). "The Y Dwarf Population with HST: unlocking the secrets of our coolest neighbours -- II. Parallaxes and Proper Motions".arXiv:2412.16679 [astro-ph].
^abcdefghijkCushing, Michael C.; Kirkpatrick, J. Davy; Gelino, Christopher R.; Griffith, Roger L.; Skrutskie, Michael F.; Mainzer, Amy K.; Marsh, Kenneth A.; Beichman, Charles A.; Burgasser, Adam J.; Prato, Lisa A.; Simcoe, Robert A.; Marley, Mark S.; Saumon, Didier; Freedman, Richard S.; Eisenhardt, Peter R.; Wright, Edward L. (2011). "The Discovery of Y Dwarfs using Data from the Wide-field Infrared Survey Explorer (WISE)".The Astrophysical Journal.743 (1): 50.arXiv:1108.4678.Bibcode:2011ApJ...743...50C.doi:10.1088/0004-637X/743/1/50.S2CID286881.
