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WISE 1828+2650

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1550:; 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)". 1382: 28: 1899:; 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". 474:
presented discovery of seven brown dwarfs – one of T9.5 type, and six of Y-type – first members of the Y spectral class, ever discovered and spectroscopically confirmed, including "archetypal member" of the Y spectral class – WISE 1828+2650. These seven objects are also the faintest seven of 98 brown
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Cushing, 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.;
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Lew, Ben W.P.; Roellig, Thomas; Batalha, Natasha E.; Line, Michael; Greene, Thomas; Murkherjee, Sagnick; Freedman, Richard; Meyer, Michael; Beichman, Charles; De Oliveira, Catarina Alves; De Furio, Matthew; Johnstone, Doug; Greenbaum, Alexandra Z.; Marley, Mark; J. Fortney, Jonathan (8 Feb 2024).
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These 98 brown dwarf systems are only among first, not all brown dwarf systems, discovered from data, collected by WISE: 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
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low resolution prism observations cannot be explained with existing Sonora Bobcat models of planetary objects, neither single nor multiple. The binary model fails to provide an improved fit for the existing photometric data. A newer analysis of the NIRSpec data compared radius determined with
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De Furio, Matthew; Lew, Ben; Beichman, Charles; Roellig, Thomas; Bryden, Geoffrey; Ciardi, David; Meyer, Michael; Rieke, Marcia; Greenbaum, Alexandra; Leisenring, Jarron; Llop-Sayson, Jorge; Ygouf, Marie; Albert, Loic; Boyer, Martha; Eisenstein, Daniel (2023-05-01).
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Beichman, Charles; De Furio, Matthew; Roellig, Thomas; Lew, Ben; Greene, Thomas; Leisenring, Jarron; Misselt, Karl; Stansberry, John; Boyer, Martha; Rieke, Marcia; Meyer, Michael; Albert, Loic; Kelly, Douglas; Greenbaum, Alexendra; Bryden, Geoffrey (2023-01-01).
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bearing species in the atmosphere of WISE 1828+2650. The carbon-to-oxygen ratio (C/O ratio) is with 0.45±0.01 close to the solar ratio. The abundance of carbon, oxygen and sulfur is higher than the sun, but the abundance of nitrogen is likely similar to the sun.
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Beichman, Charles A.; Gelino, Christopher R.; Kirkpatrick, J. Davy; Cushing, Michael C.; Dodson-Robinson, Sally; Marley, Mark S.; Morley, Caroline V.; Wright, Edward L. (2014). "WISE Y Dwarfs As Probes of the Brown Dwarf-Exoplanet Connection".
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Beichman, Charles A.; Gelino, Christopher R.; Kirkpatrick, J. Davy; Barman, Travis S.; Marsh, Kenneth A.; Cushing, Michael C.; Wright, Edward L. (2013). "The Coldest Brown Dwarf (or Free-floating Planet)?: The Y Dwarf WISE 1828+2650".
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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).
972:(it is not currently known if it is a brown dwarf or a free-floating planet). It has a temperature in the range 250–400 K (−23–127 °C; −10–260 °F) and was initially estimated below 300 449:
at infrared wavelength. WISE 1828+2650 has two discovery papers: Kirkpatrick et al. (2011) and Cushing et al. (2011), however, basically with the same authors and published nearly simultaneously.
3310: 2963: 1263:, and no direct evidence for binarity yet exists. However, the spectrum of the system best fits a pair of brown dwarfs, each with an effective temperature of about 325 K and a mass of about 2145:"High-precision atmospheric characterization of a Y dwarf with JWST NIRSpec G395H spectroscopy: isotopologue, C/O ratio, metallicity, and the abundances of six molecular species" 1459: 3787: 1711: 1320:) is too large for its age, which might be an indication that WISE 1828+2650 is an equal mass binary with both objects having a radius of 0.87 1244:
Comparison between WISE 1828+2650 and WD 0806-661 B may suggest that WISE 1828+2650 is a system of two equal-mass objects. Observations with
1552: 1021:. This suggests that WISE 1828+2650 may be a free-floating planet rather than a brown dwarf, since it is below the lower mass limit for 442: 368: 363: 358: 353: 348: 41: 2077: 62: 2331: 1957:
Dupuy, Trent J.; Kraus, Adam L. (2013). "Distances, Luminosities, and Temperatures of the Coldest Known Substellar Objects".
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of WISE 1828+2650, characteristic of an old disk population, indicates a possible age of WISE 1828+2650 in the range 2–4
3777: 1369:) when using the temperature and gravity from Sonora Elf Owl atmospheric model grid. Future observations could look for 1103: 1043:. WD 0806-661 B could have formed as a planet close to its primary, WD 0806-661 A, and later, when the primary became a 1051:, and similarity between WD 0806-661 B and WISE 1828+2650 may indicate that WISE 1828+2650 had formed in the same way. 1780:
Wright, Edward L. (2011). "The Discovery of Y Dwarfs using Data from the Wide-field Infrared Survey Explorer (WISE)".
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atmospheric retrieval framework CHIMERA and evolutionary model Sonora Bobcat. The CHIMERA radius for a single object (
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system had not revealed binarity, suggesting that if any such companion exists, it would have an orbit less than 0.5
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Barrado, David; Mollière, Paul; et al. (November 2023). "15NH3 in the atmosphere of a cool brown dwarf".
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in 2014, WISE 1828+2650 was considered as the coldest currently known brown dwarf or the first example of
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imaging observations did not find a companion at a separation larger than 0.5 astronomical units.
965: 2324: 2189: 2152: 2109: 2059: 2033: 2000: 1966: 1936: 1910: 1878: 1850: 1815: 1789: 1748: 1720: 1707:"The Field Substellar Mass Function Based on the Full-sky 20 pc Census of 525 L, T, and Y Dwarfs" 1674: 1648: 1587: 1561: 142: 123: 3161: 3141: 3131: 3126: 3111: 2692: 2687: 2682: 2677: 2672: 2667: 2662: 2657: 2647: 2642: 2637: 2289: 1082:) in the atmosphere of WISE 1828+2650. The work detected a low amount of ammonia containing the 3096: 3091: 3086: 3071: 3061: 3041: 2920: 2915: 2910: 2905: 2900: 2895: 2885: 2880: 2865: 2850: 2845: 2820: 2810: 2805: 2800: 2770: 2765: 2760: 2755: 2750: 2745: 2735: 2725: 2720: 3731: 3726: 3716: 3711: 3706: 3701: 3696: 3691: 3686: 3681: 3676: 3671: 3661: 3651: 3646: 3641: 3636: 3631: 3626: 3621: 3616: 3611: 2632: 2627: 2612: 2602: 2597: 2587: 2582: 2577: 2572: 2567: 2562: 2557: 2552: 2547: 2542: 2375: 2217: 1992: 1342: 1260: 1048: 319: 55: 3242: 2532: 2527: 2522: 2517: 1493:
According to Dupuy & Kraus (2013), this measurement uncertainty is likely underestimated.
2207: 2178:"JWST Observations of the Enigmatic Y-Dwarf WISE 1828+2650. I. Limits to a Binary Companion" 2119: 2104: 2051: 1984: 1928: 1868: 1807: 1738: 1666: 1579: 1464: 1252: 1249: 1131: 441:
WISE 1828+2650 was discovered in 2011 from data collected by NASA's 40 cm (16 in)
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NASA Astronomy Picture of the Day: Infrared image of WISE 1828+2650 (30 August 2011)
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The other six discoveries of brown dwarfs, published by Cushing et al. in 2011:
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and not like a planet. Thus, this provides evidence that the object is a
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Kirkpatrick, J. Davy; Gelino, Christopher R.; et al. (March 2021).
1362:. Sonora Bobcat however predicts a lower age (1.4 Gyrs) and mass (9.982 3747: 3534: 3277: 3252: 2512: 1389: 1286: 1115: 1075: 1067: 3594: 3576: 3272: 3257: 1282: 1151: 1147: 1139: 1047:
and lost most of its mass, have migrated into a larger orbit of 2500
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Currently the most accurate distance estimate of WISE 1828+2650 is a
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M, L, T and Y, among which also was WISE 1828+2650 – coolest of them.
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WISE 1828+2650 is similar in appearance to the other Y-type object
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instrument on JWST and detected water vapor, methane, ammonia,
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and it is an indication that WISE 1828+2650 has formed like a
2238:"JWST Observations of the Enigmatic Y Dwarf WISE 1828+2650" 428:. It is the "archetypal member" of the Y spectral class. 1114:
and not a free-floating planet. Another team used the
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Rogue planet or brown dwarf in the constellation Lyra
3740: 3602: 3593: 3575: 3547: 3512: 3309: 3300: 3230: 2962: 2929: 2701: 2503: 2475: 2374: 2365: 767:Non-trigonometric distance estimates are marked in 2305:Solstation.com (New Objects within 20 light-years) 1542: 1540: 1538: 1700: 1698: 1696: 1694: 1692: 1690: 1688: 1536: 1534: 1532: 1530: 1528: 1526: 1524: 1522: 1520: 1518: 1086:isotope when compared to ammonia containing the 2272:"Y dwarf star? Because they're cool, that's Y!" 2242:American Astronomical Society Meeting Abstracts 2016: 2014: 1631: 1629: 1627: 1625: 1623: 1621: 475:dwarfs, presented in Kirkpatrick et al. (2011). 1619: 1617: 1615: 1613: 1611: 1609: 1607: 1605: 1603: 1601: 2325: 1831: 1829: 1774: 1772: 1770: 1768: 1766: 1764: 1762: 1460:List of star systems within 30–35 light-years 8: 1952: 1950: 1098:ratio was measured as 670. This amount of NH 459:presented discovery of 98 new found by WISE 61:55467.61       1712:The Astrophysical Journal Supplement Series 983:The mass of WISE 1828+2650 is in the range 3599: 3306: 2371: 2332: 2318: 2310: 103:26° 50′ 37.79″ 2211: 2193: 2156: 2113: 2037: 1970: 1914: 1872: 1854: 1793: 1742: 1724: 1652: 1565: 980:(>Y2, initially estimated as >Y0). 771:. The most precise estimate is marked in 1157: 796: 598:(according to Kirkpatrick et al. (2012)) 527: 3788:Astronomical objects discovered in 2011 1514: 1476: 1159:Elemental Abundances of WISE 1828+2650 798:WISE 1828+2650 proper motion estimates 180: 33:WISE 1828+2650 is circled in the centre 1008:, leading to a mass estimate of about 786:WISE 1828+2650 has a proper motion of 18: 2170: 2168: 2137: 2135: 2133: 416:>Y2, located in the constellation 7: 2270:Choi, Charles Q. (August 26, 2011). 1553:The Astrophysical Journal Supplement 488:, published in 2021 by Kirkpatrick 443:Wide-field Infrared Survey Explorer 200: 1138:S). These molecules are the major 529:WISE 1828+2650 distance estimates 14: 503:, corresponding to a distance of 2078:"An ammonia trail to exoplanets" 26: 949:The best estimate is marked in 1: 1246:Hubble Space Telescope (HST) 1165:Normalized element abundance 1933:10.1088/0004-637X/753/2/156 1671:10.1088/0004-637X/764/1/101 463:systems with components of 231:100.3 ± 2.0  20:WISEPA J182831.08+265037.8 3809: 2124:10.1038/s41586-023-06813-y 2056:10.1088/0004-637X/783/2/68 1812:10.1088/0004-637X/743/1/50 1584:10.1088/0067-0049/197/2/19 1371:radial velocity variations 921: 902: 883: 864: 794:milliarcseconds per year. 726: 694: 662: 630: 593: 568: 402:WISEPA J182831.08+265037.8 3288:WISEP J190648.47+401106.8 2357:Lyra in Chinese astronomy 2347: 2182:The Astrophysical Journal 2025:The Astrophysical Journal 1902:The Astrophysical Journal 1843:The Astrophysical Journal 1782:The Astrophysical Journal 1640:The Astrophysical Journal 948: 865:Kirkpatrick et al. (2011) 766: 727:Kirkpatrick et al. (2021) 569:Kirkpatrick et al. (2011) 376: 346: 339: 335: 268: 263: 259: 167: 160: 107: 52: 24: 2213:10.3847/1538-4357/acbf1e 2149:The Astronomical Journal 1874:10.3847/1538-4357/ac12cb 1744:10.3847/1538-4365/abd107 903:Dupuy & Kraus (2013) 663:Dupuy & Kraus (2013) 1989:10.1126/science.1241917 1373:to confirm the binary. 964:Until the discovery of 432:History of observations 404:) is a possibly binary 143:Apparent magnitude 1406: 1401:compared to red dwarf 1054:JWST observation with 922:Beichman et al. (2014) 884:Beichman et al. (2013) 695:Beichman et al. (2014) 631:Beichman et al. (2013) 594:Beichman et al. (2013) 486:trigonometric parallax 420:at approximately 32.5 3525:HD 173416 b (Wangshu) 2352:List of stars in Lyra 2341:Constellation of Lyra 1405:, Jupiter and the Sun 1384: 1102:is lower than in any 1897:Kirkpatrick, J. Davy 1548:Kirkpatrick, J. Davy 970:free-floating planet 3778:Y-type brown dwarfs 3520:HAT-P-5b (Kráľomoc) 2254:2023AAS...24134505B 2204:2023ApJ...948...92D 2048:2014ApJ...783...68B 1981:2013Sci...341.1492D 1925:2012ApJ...753..156K 1865:2021ApJ...920...20C 1804:2011ApJ...743...50C 1735:2021ApJS..253....7K 1663:2013ApJ...764..101B 1576:2011ApJS..197...19K 1160: 1002:tangential velocity 996:for ages of 0.1–10 960:Physical properties 799: 530: 377:Database references 356:J182831.08+265037.8 351:J182831.08+265037.8 21: 1502:Relative parallax. 1407: 1343:astronomical units 1331:of this binary is 1158: 797: 528: 400:(full designation 341:Other designations 124:Apparent magnitude 114:Spectral type 19: 3760: 3759: 3756: 3755: 3543: 3542: 3296: 3295: 2290:NASA news release 1240:Possible binarity 1237: 1236: 1220:, might be +0.04 1112:(sub-)brown dwarf 1104:Solar System body 957: 956: 779: 778: 395: 394: 251:(10.0 ± 0.2  3800: 3600: 3307: 3253:HAT-P-5 (Chasoň) 2372: 2334: 2327: 2320: 2311: 2286: 2284: 2282: 2258: 2257: 2232: 2226: 2225: 2215: 2197: 2172: 2163: 2162: 2160: 2139: 2128: 2127: 2117: 2099: 2093: 2092: 2090: 2089: 2082:www.phys.ethz.ch 2074: 2068: 2067: 2041: 2018: 2009: 2008: 1974: 1965:(6153): 1492–5. 1954: 1945: 1944: 1918: 1893: 1887: 1886: 1876: 1858: 1833: 1824: 1823: 1797: 1776: 1757: 1756: 1746: 1728: 1702: 1683: 1682: 1656: 1633: 1596: 1595: 1569: 1544: 1503: 1500: 1494: 1491: 1485: 1484:published later. 1481: 1465:List of Y-dwarfs 1392: 1355: 1354: 1353: 1341: 1340: 1339: 1327:. The estimated 1297: 1295: 1266: 1233: 1231: 1219: 1217: 1205: 1204: 1203: 1188: 1187: 1186: 1161: 1132:hydrogen sulfide 1028: 1011: 986: 800: 793: 791: 759: 757: 748: 746: 737: 735: 720: 719: 709: 708: 688: 687: 677: 676: 656: 655: 645: 644: 624: 623: 613: 612: 599: 574: 531: 524: 519: 513: 508: 502: 497: 327: 309: 307: 282: 246:32.5 ± 0.6  210: 208: 202: 190: 188: 182: 152: 133: 108:Characteristics 93: 88: 53:Observation data 44:space telescope) 30: 22: 3808: 3807: 3803: 3802: 3801: 3799: 3798: 3797: 3763: 3762: 3761: 3752: 3736: 3589: 3571: 3557:δ Lyrae cluster 3539: 3508: 3292: 3248:GSC 02652-01324 3226: 2958: 2925: 2697: 2499: 2471: 2361: 2343: 2338: 2280: 2278: 2269: 2266: 2261: 2234: 2233: 2229: 2174: 2173: 2166: 2141: 2140: 2131: 2101: 2100: 2096: 2087: 2085: 2076: 2075: 2071: 2020: 2019: 2012: 1956: 1955: 1948: 1895: 1894: 1890: 1835: 1834: 1827: 1778: 1777: 1760: 1704: 1703: 1686: 1635: 1634: 1599: 1546: 1545: 1516: 1512: 1507: 1506: 1501: 1497: 1492: 1488: 1482: 1478: 1473: 1412: 1388: 1379: 1368: 1365: 1361: 1358: 1351: 1349: 1348: 1346: 1337: 1335: 1334: 1332: 1329:semi-major axis 1326: 1323: 1319: 1316: 1312: 1309: 1304: 1301: 1293: 1291: 1274: 1271: 1264: 1242: 1229: 1227: 1215: 1213: 1201: 1199: 1198: 1196: 1184: 1182: 1181: 1179: 1137: 1129: 1120:carbon monoxide 1101: 1097: 1093: 1090:isotope. The NH 1081: 1073: 1065: 1035: 1032: 1026: 1019: 1016: 1009: 994: 991: 984: 962: 850: 849: 834: 833: 822: 809: 789: 787: 784: 755: 753: 744: 742: 733: 731: 718: 715: 714: 713: 707: 704: 703: 702: 686: 683: 682: 681: 675: 672: 671: 670: 654: 651: 650: 649: 643: 640: 639: 638: 622: 619: 618: 617: 611: 608: 607: 606: 597: 595: 572: 570: 556: 547: 538: 517: 515: 506: 504: 495: 493: 482: 447:space telescope 439: 434: 372: 367: 362: 357: 352: 325: 305: 303: 290: 280: 250: 206: 204: 199: 186: 184: 146: 127: 91: 86:Right ascension 84: 54: 48: 47: 40:image from the 34: 31: 17: 12: 11: 5: 3806: 3804: 3796: 3795: 3790: 3785: 3780: 3775: 3765: 3764: 3758: 3757: 3754: 3753: 3751: 3750: 3744: 3742: 3738: 3737: 3735: 3734: 3729: 3724: 3719: 3714: 3709: 3704: 3699: 3694: 3689: 3684: 3679: 3674: 3669: 3664: 3659: 3654: 3649: 3644: 3639: 3634: 3629: 3624: 3619: 3614: 3608: 3606: 3597: 3591: 3590: 3588: 3587: 3581: 3579: 3573: 3572: 3570: 3569: 3564: 3559: 3553: 3551: 3545: 3544: 3541: 3540: 3538: 3537: 3532: 3527: 3522: 3516: 3514: 3510: 3509: 3507: 3506: 3501: 3496: 3491: 3486: 3481: 3476: 3471: 3466: 3461: 3456: 3451: 3446: 3441: 3436: 3431: 3426: 3421: 3416: 3411: 3406: 3401: 3396: 3391: 3386: 3381: 3376: 3371: 3366: 3361: 3356: 3351: 3346: 3341: 3336: 3331: 3326: 3321: 3315: 3313: 3304: 3298: 3297: 3294: 3293: 3291: 3290: 3285: 3283:WISE 1828+2650 3280: 3275: 3270: 3268:LSR J1835+3259 3265: 3260: 3255: 3250: 3245: 3240: 3234: 3232: 3228: 3227: 3225: 3224: 3219: 3214: 3209: 3204: 3199: 3194: 3189: 3184: 3179: 3174: 3169: 3164: 3159: 3154: 3149: 3144: 3139: 3134: 3129: 3124: 3119: 3114: 3109: 3104: 3099: 3094: 3089: 3084: 3079: 3074: 3069: 3064: 3059: 3054: 3049: 3044: 3039: 3034: 3029: 3024: 3019: 3014: 3009: 3004: 2999: 2994: 2989: 2984: 2979: 2974: 2968: 2966: 2960: 2959: 2957: 2956: 2951: 2946: 2941: 2935: 2933: 2927: 2926: 2924: 2923: 2918: 2913: 2908: 2903: 2898: 2893: 2888: 2883: 2878: 2873: 2868: 2863: 2858: 2853: 2848: 2843: 2838: 2833: 2828: 2823: 2818: 2813: 2808: 2803: 2798: 2793: 2788: 2783: 2778: 2773: 2768: 2763: 2758: 2753: 2748: 2743: 2738: 2733: 2728: 2723: 2718: 2713: 2707: 2705: 2699: 2698: 2696: 2695: 2690: 2685: 2680: 2675: 2670: 2665: 2660: 2655: 2650: 2645: 2640: 2635: 2630: 2625: 2620: 2615: 2610: 2605: 2600: 2595: 2590: 2585: 2580: 2575: 2570: 2565: 2560: 2555: 2550: 2545: 2540: 2535: 2530: 2525: 2520: 2515: 2509: 2507: 2501: 2500: 2498: 2497: 2492: 2487: 2481: 2479: 2473: 2472: 2470: 2469: 2464: 2459: 2451: 2446: 2441: 2436: 2431: 2426: 2421: 2416: 2411: 2406: 2401: 2396: 2391: 2386: 2380: 2378: 2369: 2363: 2362: 2360: 2359: 2354: 2348: 2345: 2344: 2339: 2337: 2336: 2329: 2322: 2314: 2308: 2307: 2302: 2297: 2292: 2287: 2265: 2264:External links 2262: 2260: 2259: 2227: 2164: 2129: 2094: 2069: 2010: 1946: 1888: 1825: 1758: 1684: 1597: 1513: 1511: 1508: 1505: 1504: 1495: 1486: 1475: 1474: 1472: 1469: 1468: 1467: 1462: 1453: 1452: 1449:WISE 2056+1459 1446: 1443:WISE 1738+2732 1440: 1437:WISE 1541−2250 1434: 1431:WISE 1405+5534 1428: 1425:WISE 0410+1502 1422: 1419:WISE 0148−7202 1411: 1408: 1399:WISE 1828+2650 1378: 1375: 1366: 1363: 1359: 1356: 1324: 1321: 1317: 1314: 1310: 1307: 1302: 1299: 1272: 1269: 1241: 1238: 1235: 1234: 1225: 1222: 1221: 1210: 1207: 1206: 1193: 1190: 1189: 1177: 1174: 1173: 1171:(=0 is solar) 1167: 1135: 1127: 1124:carbon dioxide 1099: 1095: 1091: 1079: 1071: 1063: 1033: 1030: 1017: 1014: 992: 989: 978:spectral class 966:WISE 0855−0714 961: 958: 955: 954: 946: 945: 943: 938: 933: 928: 923: 919: 918: 916: 913: 910: 907: 904: 900: 899: 897: 894: 891: 888: 885: 881: 880: 878: 875: 872: 869: 866: 862: 861: 858: 847: 842: 831: 826: 817: 804: 783: 780: 777: 776: 764: 763: 761: 750: 739: 728: 724: 723: 721: 716: 710: 705: 699: 696: 692: 691: 689: 684: 678: 673: 667: 664: 660: 659: 657: 652: 646: 641: 635: 632: 628: 627: 625: 620: 614: 609: 603: 600: 591: 590: 588: 583: 578: 575: 566: 565: 562: 553: 544: 535: 481: 478: 477: 476: 468: 465:spectral types 438: 435: 433: 430: 414:spectral class 398:WISE 1828+2650 393: 392: 387: 379: 378: 374: 373: 347: 344: 343: 337: 336: 333: 332: 323: 315: 314: 301: 293: 292: 288: 278: 270: 269: 266: 265: 261: 260: 257: 256: 244: 236: 235: 229: 220: 219: 178: 169: 168: 165: 164: 158: 157: 154: 151:filter system) 139: 138: 135: 132:filter system) 120: 119: 116: 110: 109: 105: 104: 101: 95: 94: 89: 81: 80: 75: 69: 68: 50: 49: 32: 25: 15: 13: 10: 9: 6: 4: 3: 2: 3805: 3794: 3791: 3789: 3786: 3784: 3781: 3779: 3776: 3774: 3773:Rogue planets 3771: 3770: 3768: 3749: 3746: 3745: 3743: 3739: 3733: 3730: 3728: 3725: 3723: 3720: 3718: 3715: 3713: 3710: 3708: 3705: 3703: 3700: 3698: 3695: 3693: 3690: 3688: 3685: 3683: 3680: 3678: 3675: 3673: 3670: 3668: 3665: 3663: 3660: 3658: 3655: 3653: 3650: 3648: 3645: 3643: 3640: 3638: 3635: 3633: 3630: 3628: 3625: 3623: 3620: 3618: 3615: 3613: 3610: 3609: 3607: 3605: 3601: 3598: 3596: 3592: 3586: 3583: 3582: 3580: 3578: 3574: 3568: 3565: 3563: 3560: 3558: 3555: 3554: 3552: 3550: 3549:Star clusters 3546: 3536: 3533: 3531: 3528: 3526: 3523: 3521: 3518: 3517: 3515: 3511: 3505: 3502: 3500: 3497: 3495: 3492: 3490: 3487: 3485: 3482: 3480: 3477: 3475: 3472: 3470: 3467: 3465: 3462: 3460: 3457: 3455: 3452: 3450: 3447: 3445: 3442: 3440: 3437: 3435: 3432: 3430: 3427: 3425: 3422: 3420: 3417: 3415: 3412: 3410: 3407: 3405: 3402: 3400: 3397: 3395: 3392: 3390: 3387: 3385: 3382: 3380: 3377: 3375: 3372: 3370: 3367: 3365: 3362: 3360: 3357: 3355: 3352: 3350: 3347: 3345: 3342: 3340: 3337: 3335: 3332: 3330: 3327: 3325: 3322: 3320: 3317: 3316: 3314: 3312: 3308: 3305: 3303: 3299: 3289: 3286: 3284: 3281: 3279: 3276: 3274: 3271: 3269: 3266: 3264: 3261: 3259: 3256: 3254: 3251: 3249: 3246: 3244: 3241: 3239: 3236: 3235: 3233: 3229: 3223: 3220: 3218: 3215: 3213: 3210: 3208: 3205: 3203: 3200: 3198: 3195: 3193: 3190: 3188: 3185: 3183: 3180: 3178: 3175: 3173: 3170: 3168: 3165: 3163: 3160: 3158: 3155: 3153: 3150: 3148: 3145: 3143: 3140: 3138: 3135: 3133: 3130: 3128: 3125: 3123: 3120: 3118: 3115: 3113: 3110: 3108: 3105: 3103: 3100: 3098: 3095: 3093: 3090: 3088: 3085: 3083: 3080: 3078: 3075: 3073: 3070: 3068: 3065: 3063: 3060: 3058: 3055: 3053: 3050: 3048: 3045: 3043: 3040: 3038: 3035: 3033: 3030: 3028: 3025: 3023: 3020: 3018: 3015: 3013: 3010: 3008: 3005: 3003: 3000: 2998: 2995: 2993: 2990: 2988: 2985: 2983: 2980: 2978: 2975: 2973: 2970: 2969: 2967: 2965: 2961: 2955: 2952: 2950: 2947: 2945: 2942: 2940: 2937: 2936: 2934: 2932: 2928: 2922: 2919: 2917: 2914: 2912: 2909: 2907: 2904: 2902: 2899: 2897: 2894: 2892: 2889: 2887: 2884: 2882: 2879: 2877: 2874: 2872: 2869: 2867: 2864: 2862: 2859: 2857: 2854: 2852: 2849: 2847: 2844: 2842: 2839: 2837: 2834: 2832: 2829: 2827: 2824: 2822: 2819: 2817: 2814: 2812: 2809: 2807: 2804: 2802: 2799: 2797: 2794: 2792: 2789: 2787: 2784: 2782: 2779: 2777: 2774: 2772: 2769: 2767: 2764: 2762: 2759: 2757: 2754: 2752: 2749: 2747: 2744: 2742: 2739: 2737: 2734: 2732: 2729: 2727: 2724: 2722: 2719: 2717: 2714: 2712: 2709: 2708: 2706: 2704: 2700: 2694: 2691: 2689: 2686: 2684: 2681: 2679: 2676: 2674: 2671: 2669: 2666: 2664: 2661: 2659: 2656: 2654: 2651: 2649: 2646: 2644: 2641: 2639: 2636: 2634: 2631: 2629: 2626: 2624: 2621: 2619: 2616: 2614: 2611: 2609: 2606: 2604: 2601: 2599: 2596: 2594: 2591: 2589: 2586: 2584: 2581: 2579: 2576: 2574: 2571: 2569: 2566: 2564: 2561: 2559: 2556: 2554: 2551: 2549: 2546: 2544: 2541: 2539: 2536: 2534: 2531: 2529: 2526: 2524: 2521: 2519: 2516: 2514: 2511: 2510: 2508: 2506: 2502: 2496: 2493: 2491: 2488: 2486: 2483: 2482: 2480: 2478: 2474: 2468: 2465: 2463: 2460: 2458: 2457: 2452: 2450: 2447: 2445: 2442: 2440: 2437: 2435: 2432: 2430: 2427: 2425: 2422: 2420: 2417: 2415: 2412: 2410: 2407: 2405: 2402: 2400: 2397: 2395: 2392: 2390: 2387: 2385: 2382: 2381: 2379: 2377: 2373: 2370: 2368: 2364: 2358: 2355: 2353: 2350: 2349: 2346: 2342: 2335: 2330: 2328: 2323: 2321: 2316: 2315: 2312: 2306: 2303: 2301: 2298: 2296: 2293: 2291: 2288: 2277: 2273: 2268: 2267: 2263: 2255: 2251: 2248:(2): 345.05. 2247: 2243: 2239: 2231: 2228: 2223: 2219: 2214: 2209: 2205: 2201: 2196: 2191: 2187: 2183: 2179: 2171: 2169: 2165: 2159: 2154: 2150: 2146: 2138: 2136: 2134: 2130: 2125: 2121: 2116: 2111: 2107: 2106: 2098: 2095: 2083: 2079: 2073: 2070: 2065: 2061: 2057: 2053: 2049: 2045: 2040: 2035: 2031: 2027: 2026: 2017: 2015: 2011: 2006: 2002: 1998: 1994: 1990: 1986: 1982: 1978: 1973: 1968: 1964: 1960: 1953: 1951: 1947: 1942: 1938: 1934: 1930: 1926: 1922: 1917: 1912: 1908: 1904: 1903: 1898: 1892: 1889: 1884: 1880: 1875: 1870: 1866: 1862: 1857: 1852: 1848: 1844: 1840: 1832: 1830: 1826: 1821: 1817: 1813: 1809: 1805: 1801: 1796: 1791: 1787: 1783: 1775: 1773: 1771: 1769: 1767: 1765: 1763: 1759: 1754: 1750: 1745: 1740: 1736: 1732: 1727: 1722: 1718: 1714: 1713: 1708: 1701: 1699: 1697: 1695: 1693: 1691: 1689: 1685: 1680: 1676: 1672: 1668: 1664: 1660: 1655: 1650: 1646: 1642: 1641: 1632: 1630: 1628: 1626: 1624: 1622: 1620: 1618: 1616: 1614: 1612: 1610: 1608: 1606: 1604: 1602: 1598: 1593: 1589: 1585: 1581: 1577: 1573: 1568: 1563: 1559: 1555: 1554: 1549: 1543: 1541: 1539: 1537: 1535: 1533: 1531: 1529: 1527: 1525: 1523: 1521: 1519: 1515: 1509: 1499: 1496: 1490: 1487: 1480: 1477: 1470: 1466: 1463: 1461: 1458: 1457: 1456: 1450: 1447: 1444: 1441: 1438: 1435: 1432: 1429: 1426: 1423: 1420: 1417: 1416: 1415: 1409: 1404: 1400: 1396: 1391: 1387: 1383: 1376: 1374: 1372: 1344: 1330: 1305: 1288: 1284: 1281: 1277: 1275: 1262: 1258: 1254: 1251: 1247: 1239: 1226: 1224: 1223: 1211: 1209: 1208: 1194: 1192: 1191: 1178: 1176: 1175: 1172: 1168: 1166: 1163: 1162: 1156: 1153: 1149: 1145: 1141: 1133: 1125: 1121: 1117: 1113: 1109: 1105: 1089: 1085: 1077: 1069: 1061: 1057: 1052: 1050: 1046: 1042: 1041:WD 0806-661 B 1037: 1024: 1020: 1007: 1003: 999: 995: 981: 979: 975: 971: 967: 959: 952: 947: 944: 942: 939: 937: 934: 932: 929: 927: 924: 920: 917: 914: 911: 908: 905: 901: 898: 895: 892: 889: 886: 882: 879: 876: 873: 870: 867: 863: 859: 857: 853: 846: 843: 841: 837: 830: 827: 825: 821: 818: 816: 812: 808: 805: 802: 801: 795: 782:Proper motion 781: 774: 770: 765: 762: 760: 751: 749: 740: 738: 729: 725: 722: 711: 700: 697: 693: 690: 679: 668: 665: 661: 658: 647: 636: 633: 629: 626: 615: 604: 601: 592: 589: 587: 584: 582: 579: 576: 567: 563: 560: 554: 551: 545: 542: 536: 533: 532: 526: 523: 512: 501: 491: 487: 479: 473: 469: 466: 462: 458: 455: 452: 451: 450: 448: 444: 436: 431: 429: 427: 423: 419: 415: 411: 407: 403: 399: 391: 388: 386: 385: 381: 380: 375: 370: 365: 360: 355: 350: 345: 342: 338: 334: 331: 326:2–4 or 0.1–10 324: 322: 321: 317: 316: 313: 302: 300: 299: 295: 294: 291: 287: 281:3–6 or 0.5–20 279: 277: 276: 272: 271: 267: 262: 258: 254: 249: 245: 243: 242: 238: 237: 234: 230: 228: 226: 222: 221: 218: 214: 198: 194: 179: 177: 175: 174:Proper motion 171: 170: 166: 163: 159: 156:22.45 ± 0.08 155: 150: 144: 141: 140: 137:23.57 ± 0.35 136: 131: 125: 122: 121: 117: 115: 112: 111: 106: 102: 100: 97: 96: 90: 87: 83: 82: 79: 76: 74: 73:Constellation 71: 70: 67: 64: 60: 57: 51: 45: 43: 39: 29: 23: 3793:WISE objects 3530:HD 178911 Bb 3282: 2455: 2295:Science news 2279:. Retrieved 2245: 2241: 2230: 2185: 2181: 2148: 2103: 2097: 2086:. Retrieved 2084:. 2023-11-07 2081: 2072: 2029: 2023: 1962: 1958: 1906: 1900: 1891: 1846: 1842: 1785: 1781: 1716: 1710: 1644: 1638: 1557: 1551: 1498: 1489: 1479: 1454: 1413: 1398: 1386:Brown dwarfs 1278: 1243: 1170: 1053: 1038: 982: 963: 950: 940: 935: 930: 925: 785: 772: 768: 752: 741: 730: 585: 580: 489: 483: 471: 456: 440: 410:rogue planet 401: 397: 396: 382: 318: 296: 285: 273: 239: 223: 172: 35: 3585:Ring Nebula 2776:7043 (Xihe) 2429:η (Aladfar) 2394:γ (Sulafat) 2389:β (Sheliak) 2039:1401.1194v2 1567:1108.4677v1 1433:(Y0 (pec?)) 1403:Gliese 229A 1395:Gliese 229B 1060:water vapor 1045:white dwarf 1000:. The high 461:brown dwarf 454:Kirkpatrick 422:light-years 406:brown dwarf 298:Temperature 99:Declination 92:18 28 31.10 3767:Categories 3562:Messier 56 3302:Exoplanets 3238:Gliese 758 2456:(Alathfar) 2281:August 31, 2195:2302.12723 2158:2402.05900 2115:2311.08054 2088:2023-11-07 1909:(2): 156. 1856:2107.00506 1726:2011.11616 1647:(1): 101. 1510:References 1377:Comparison 1169:Abundance 909:80.4 ± 0.9 896:153 ± 12.5 874:1078 ± 327 717:−1.9 706:−0.6 685:−7.8 674:−2.4 653:−3.3 642:−1.0 621:−2.6 610:−0.8 371:1828+2650 366:J1828+2650 361:J1828+2650 162:Astrometry 2477:Flamsteed 2276:Space.com 2222:0004-637X 2188:(2): 92. 2064:119302072 2032:(2): 68. 1972:1309.1422 1941:119279752 1916:1205.2122 1883:235694398 1849:(1): 20. 1795:1108.4678 1788:(1): 50. 1753:227126954 1679:118575478 1654:1301.1669 1560:(2): 19. 1058:detected 1023:deuterium 912:1020 ± 15 906:1034 ± 15 877:118 ± 409 573:(Table 6) 520:0.6  509:0.2  498:2.0  437:Discovery 145: (H 126: (J 3595:Galaxies 3567:NGC 6791 3263:LHS 6343 2505:Variable 2384:α (Vega) 2005:30379513 1997:24009359 1719:(1): 7. 1592:16850733 1410:See also 1144:nitrogen 1025:fusion ( 936:1024 ± 7 915:173 ± 16 893:954 ± 11 634:90 ± 9.5 602:122 ± 13 586:<30.7 555:Distance 546:Distance 537:Parallax 480:Distance 470:Cushing 241:Distance 225:Parallax 118:>Y2V 38:Infrared 3748:IC 1296 3577:Nebulae 3535:TrES-1b 3278:WASP-58 3243:GJ 4063 2250:Bibcode 2200:Bibcode 2044:Bibcode 1977:Bibcode 1959:Science 1921:Bibcode 1861:Bibcode 1800:Bibcode 1731:Bibcode 1659:Bibcode 1572:Bibcode 1455:Lists: 1390:Teide 1 1287:NIRSpec 1250:Keck-II 1116:NIRSpec 1076:ammonia 1068:methane 941:174 ± 6 788:1,030.5 698:106 ± 7 666:70 ± 14 581:<9.4 577:– 445:(WISE) 264:Details 185:1,016.5 63:Equinox 3311:Kepler 3273:WASP-3 3258:KSw 71 2964:Kepler 2954:181068 2949:180314 2944:179070 2939:177830 2513:R (13) 2220:  2105:Nature 2062:  2003:  1995:  1939:  1881:  1820:286881 1818:  1751:  1677:  1590:  1439:(Y0.5) 1421:(T9.5) 1397:, and 1338:−0.006 1336:+0.002 1333:0.0098 1313:,0.87 1283:NIRCam 1267:  1152:sulfur 1150:, and 1148:oxygen 1140:carbon 1130:) and 1122:(CO), 1094:-to-NH 1074:) and 1029:  1012:  987:  985:0.5–20 803:Source 769:italic 596:  571:  534:Source 490:et al. 472:et al. 457:et al. 384:SIMBAD 349:WISEPA 328:  310:  283:  211:  203:  191:  183:  3741:Other 3513:Other 3231:Other 2376:Bayer 2367:Stars 2190:arXiv 2153:arXiv 2110:arXiv 2060:S2CID 2034:arXiv 2001:S2CID 1967:arXiv 1937:S2CID 1911:arXiv 1879:S2CID 1851:arXiv 1816:S2CID 1790:arXiv 1749:S2CID 1721:arXiv 1675:S2CID 1649:arXiv 1588:S2CID 1562:arXiv 1471:Notes 1228:+0.14 1214:−0.31 1212:> 1202:−0.02 1200:+0.01 1197:+0.34 1185:−0.02 1183:+0.01 1180:+0.24 820:P. A. 732:100.3 514:, or 494:100.3 426:Earth 424:from 359:WISEP 354:WISEP 205:169.3 201:Dec.: 66:J2000 56:Epoch 3783:Lyra 3732:6792 3727:6765 3722:6745 3717:6740 3712:6713 3707:6710 3702:6703 3697:6702 3692:6700 3687:6695 3682:6692 3677:6688 3672:6686 3667:6685 3662:6675 3657:6672 3652:6671 3647:6665 3642:6663 3637:6662 3632:6657 3627:6646 3622:6640 3617:6612 3612:6606 3504:705b 3499:453b 3494:422b 3489:440b 3484:438b 3474:277b 3222:1513 2921:7382 2916:7376 2911:7359 2906:7346 2901:7345 2896:7338 2891:7302 2886:7284 2881:7280 2876:7272 2871:7253 2866:7244 2861:7238 2856:7237 2851:7212 2846:7204 2841:7202 2836:7181 2831:7162 2826:7146 2821:7140 2816:7132 2811:7118 2806:7115 2801:7112 2796:7081 2791:7073 2786:7064 2781:7044 2771:7041 2766:7033 2761:7030 2756:7019 2751:7017 2746:7016 2741:6997 2736:6984 2731:6968 2726:6901 2721:6853 2716:6847 2711:6845 2693:V558 2688:V550 2683:V545 2678:V543 2673:V542 2668:V533 2663:V478 2658:V477 2653:V473 2648:V404 2643:V361 2638:V344 2283:2011 2218:ISSN 1993:PMID 1451:(Y0) 1445:(Y0) 1427:(Y0) 1296:0.01 1292:1.23 1280:JWST 1248:and 1232:0.03 1218:0.02 1108:star 1066:O), 1056:MIRI 951:bold 931:80.4 926:1039 868:1084 860:Ref 773:bold 754:32.5 743:10.0 712:30.8 680:46.6 669:14.3 648:36.5 637:11.2 616:26.7 564:Ref 516:32.5 505:10.0 418:Lyra 390:data 369:WISE 364:WISE 275:Mass 78:Lyra 42:WISE 3604:NGC 3469:93b 3464:91b 3439:62b 3434:60d 3429:59b 3414:37b 3409:26e 3399:25b 3379:24b 3349:20b 3344:14b 3217:705 3212:635 3207:444 3202:429 3197:421 3192:410 3187:350 3182:282 3177:279 3172:277 3167:238 3162:177 3157:174 3152:160 3147:138 3142:131 3137:130 3132:128 3127:109 3122:105 3117:104 3112:103 3107:102 3102:100 2208:doi 2186:948 2120:doi 2052:doi 2030:783 1985:doi 1963:341 1929:doi 1907:753 1869:doi 1847:920 1808:doi 1786:743 1739:doi 1717:253 1667:doi 1645:764 1580:doi 1558:197 1352:−12 1345:or 1253:LGS 1126:(CO 1078:(NH 1070:(CH 1036:). 1034:Jup 1027:~13 1018:Jup 1010:3–6 1006:Gyr 998:Gyr 993:Jup 887:966 852:mas 848:DEC 836:mas 811:mas 792:1.1 758:0.6 747:0.2 736:2.0 701:9.4 605:8.2 541:mas 500:mas 412:of 408:or 330:Gyr 320:Age 304:406 289:Jup 233:mas 227:(π) 213:mas 209:0.8 193:mas 189:0.8 181:RA: 176:(μ) 149:MKO 130:MKO 59:MJD 3769:: 3329:9b 3324:8b 3319:7b 3097:98 3092:95 3087:94 3082:93 3077:92 3072:91 3067:88 3062:75 3057:65 3052:62 3047:60 3042:59 3037:46 3032:38 3027:37 3022:30 3017:26 3012:25 3007:24 3002:20 2997:19 2992:14 2987:13 2931:HD 2703:HR 2633:MV 2628:KX 2623:HR 2618:HP 2613:HK 2608:FL 2603:EZ 2598:EP 2593:DM 2588:CY 2583:CN 2578:CC 2573:AY 2568:XY 2563:UZ 2558:TZ 2553:TT 2548:RZ 2543:RV 2538:RR 2495:19 2490:17 2485:16 2454:μ 2274:. 2246:55 2244:. 2240:. 2216:. 2206:. 2198:. 2184:. 2180:. 2167:^ 2151:. 2147:. 2132:^ 2118:. 2108:. 2080:. 2058:. 2050:. 2042:. 2028:. 2013:^ 1999:. 1991:. 1983:. 1975:. 1961:. 1949:^ 1935:. 1927:. 1919:. 1905:. 1877:. 1867:. 1859:. 1845:. 1841:. 1828:^ 1814:. 1806:. 1798:. 1784:. 1761:^ 1747:. 1737:. 1729:. 1715:. 1709:. 1687:^ 1673:. 1665:. 1657:. 1643:. 1600:^ 1586:. 1578:. 1570:. 1556:. 1517:^ 1393:, 1350:+4 1347:20 1276:. 1261:AU 1257:AO 1195:≥ 1146:, 1142:, 1134:(H 1062:(H 1049:AU 953:. 890:81 871:84 856:yr 840:yr 832:RA 815:yr 775:. 559:ly 550:pc 525:. 522:ly 511:pc 492:: 308:88 253:pc 248:ly 217:yr 197:yr 153:) 134:) 3479:c 3459:f 3454:e 3449:d 3444:c 3424:d 3419:c 3404:c 3394:e 3389:d 3384:c 3374:g 3369:f 3364:e 3359:d 3354:c 3339:d 3334:c 2982:9 2977:8 2972:7 2533:W 2528:V 2523:T 2518:S 2467:ν 2462:ν 2449:λ 2444:κ 2439:ι 2434:θ 2424:ζ 2419:ζ 2414:ε 2409:ε 2404:δ 2399:δ 2333:e 2326:t 2319:v 2285:. 2256:. 2252:: 2224:. 2210:: 2202:: 2192:: 2161:. 2155:: 2126:. 2122:: 2112:: 2091:. 2066:. 2054:: 2046:: 2036:: 2007:. 1987:: 1979:: 1969:: 1943:. 1931:: 1923:: 1913:: 1885:. 1871:: 1863:: 1853:: 1822:. 1810:: 1802:: 1792:: 1755:. 1741:: 1733:: 1723:: 1681:. 1669:: 1661:: 1651:: 1594:. 1582:: 1574:: 1564:: 1367:J 1364:M 1360:J 1357:R 1325:J 1322:R 1318:J 1315:R 1311:J 1308:M 1303:J 1300:R 1294:± 1273:J 1270:M 1265:5 1255:- 1230:± 1216:± 1136:2 1128:2 1100:3 1096:3 1092:3 1088:N 1084:N 1080:3 1072:4 1064:2 1031:M 1015:M 990:M 974:K 854:/ 845:μ 838:/ 829:μ 824:° 813:/ 807:μ 790:± 756:± 745:± 734:± 561:) 557:( 552:) 548:( 543:) 539:( 518:± 507:± 496:± 312:K 306:± 286:M 255:) 215:/ 207:± 195:/ 187:± 147:( 128:( 46:. 36:(

Index


Infrared
WISE
Epoch
MJD
Equinox
J2000
Constellation
Lyra
Right ascension
Declination
Spectral type
Apparent magnitude
MKO
Apparent magnitude
MKO
Astrometry
Proper motion
mas
yr
mas
yr
Parallax
mas
Distance
ly
pc
Mass
MJup
Temperature

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