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Gliese 784

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Thome, Juan M. (1900). "Zonas de exploracion : Brillantez y posicion de todas las estrellas fijas hasta la decima magnitud comprendidas EN la faja del cielo entre 42 y 52 grados de declinacion sud".
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of roughly 48 days. The star has 58% of the mass and 58% of the radius of the Sun. It is radiating just 6% of the luminosity of the Sun from its
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Byrne, P. B.; Doyle, J. G. (January 1989). "Activity in late-type dwarfs. III. Chromospheric and transition region line fluxes for two dM stars".
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Torres, C. A. O.; et al. (December 2006). "Search for associations containing young stars (SACY). I. Sample and searching method".
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Brems, Stefan S.; et al. (2019), "Radial-velocity jitter of stars as a function of observational timescale and stellar age",
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Bailer-Jones, C.A.L.; et al. (2018). "New stellar encounters discovered in the second Gaia data release".
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of −33.5 km/s. The system is predicted to come as close as 11.4 light-years in ~121,700 years time.
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Tuomi, M.; et al. (2019-06-11). "Frequency of planets orbiting M dwarfs in the Solar neighbourhood".
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Hojjatpanah, S.; et al. (2019). "Catalog for the ESPRESSO blind radial velocity exoplanet survey".
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Tanner, Angelle; et al. (2020), "Herschel Observations of Disks around Late-type Stars",
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Anderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation".
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In June 2019 one planet candidate was reported in orbit around Gliese 784. An
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0.4 billion years. Despite this, it appears to be rotating slowly with a
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companion. The star was catalogued in 1900, when it was included in the
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Early Data Release 3: Summary of the contents and survey properties"
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was detected in 2020 that could suggest the presence of a
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of 7.96. Gliese 784 is located at a distance of 20.1 
1278:(1900). "Cordoba Durchmusterung declination -42 to -52". 1100: 1098: 1096: 1013:. Research Consortium On Nearby Stars. January 1, 2012. 1425:
Publications of the Astronomical Society of the Pacific
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(2016). 33:       1017:from the original on March 26, 2012 171: 523: 14: 194:162.2171 ± 0.0225  2050: 2049: 1519:Telescopium in Chinese astronomy 871:Gaia EDR3 record for this source 650:The Gliese 784 planetary system 522: 515: 2104:Henry Draper Catalogue objects 2079:Hypothetical planetary systems 1: 557:star located in the southern 1514:List of stars in Telescopium 1503:Constellation of Telescopium 1348:Astronomy & Astrophysics 1195:Astronomy & Astrophysics 1107:Astronomy & Astrophysics 865:10.1051/0004-6361/202039657e 813:Astronomy & Astrophysics 702: 697: 692: 679: 666: 661: 654: 1378:10.1051/0004-6361/201833456 1225:10.1051/0004-6361/201935520 1137:10.1051/0004-6361/201834729 1078:10.3847/0004-637X/826/2/171 845:10.1051/0004-6361/202039657 572:Cordoba Durchmusterung (CD) 2125: 2074:M-type main-sequence stars 1163:Astronomy and Astrophysics 932:10.1051/0004-6361:20065602 901:Astronomy and Astrophysics 2047: 1969: 1928: 1509: 1047:The Astrophysical Journal 985:10.1134/S1063773712050015 608:M-type main-sequence star 585:apparent visual magnitude 510: 491: 417: 410: 406: 248: 243: 239: 125: 118: 92: 24: 1455:10.1088/1538-3873/ab895f 1329:"Page 206 (CD-45 13677)" 1370:2018A&A...616A..37B 1217:2019A&A...632A..37B 1175:1989A&A...208..159B 1129:2019A&A...629A..80H 924:2006A&A...460..695T 836:2021A&A...649A...1G 225:Absolute magnitude 82:Apparent magnitude 2094:Durchmusterung objects 612:stellar classification 214:(6.1646 ± 0.0009  2099:Gliese and GJ objects 628:effective temperature 579:with the designation 658:(in order from star) 445: 20 1196, 209:20.106 ± 0.003  174: -159.939  1447:2020PASP..132h4401T 1323:1900RNAO...18.....T 1304:1900RNAO...18....1. 1069:2016ApJ...826..171G 977:2012AstL...38..331A 651: 595:as determined from 492:Database references 369:Rotational velocity 162: 778.331  21: 649: 644:circumstellar disk 473: 20103-4519, 412:Other designations 99:Spectral type 19: 2109:Hipparcos objects 2061: 2060: 2043: 2042: 1991: 1990: 1965: 1964: 1924: 1923: 955:Astronomy Letters 772: 771: 715: 690: 677: 659: 630:of 3,754 K. 565:that may host an 548: 547: 485:J20135335-4509506 478: 8392-2673-1 2116: 2053: 2052: 2002: 1971: 1930: 1534: 1496: 1489: 1482: 1473: 1466: 1465: 1440: 1431:(1014): 084401, 1420: 1414: 1413: 1411: 1399: 1390: 1389: 1363: 1343: 1337: 1336: 1331:. Archived from 1326: 1306: 1287: 1272: 1266: 1265: 1263: 1262: 1242: 1236: 1235: 1210: 1190: 1179: 1178: 1158: 1149: 1148: 1122: 1102: 1091: 1090: 1080: 1062: 1038: 1027: 1026: 1024: 1022: 1003: 997: 996: 970: 950: 944: 943: 917: 915:astro-ph/0609258 895: 878: 868: 857: 847: 829: 796: 762: 761: 760: 750: 749: 748: 727: 726: 725: 713: 684: 671: 657: 652: 634:Planetary system 617: 606:This is a small 526: 525: 519: 486: 479: 424: 398: 361: 342: 323: 173: 161: 145: 93:Characteristics 85: 65: 60: 25:Observation data 22: 2124: 2123: 2119: 2118: 2117: 2115: 2114: 2113: 2064: 2063: 2062: 2057: 2039: 2023: 1987: 1961: 1920: 1889: 1856: 1688: 1615: 1523: 1505: 1500: 1470: 1469: 1422: 1421: 1417: 1401: 1400: 1393: 1345: 1344: 1340: 1327: 1307: 1289: 1274: 1273: 1269: 1260: 1258: 1244: 1243: 1239: 1192: 1191: 1182: 1160: 1159: 1152: 1104: 1103: 1094: 1040: 1039: 1030: 1020: 1018: 1005: 1004: 1000: 952: 951: 947: 897: 896: 881: 859:(Erratum:  858: 800:Brown, A. G. A. 798: 797: 782: 777: 758: 756: 755: 753: 746: 744: 743: 741: 734: 723: 721: 720: 718: 683: 670: 656: 640:infrared excess 636: 615: 601:radial velocity 544: 543: 542: 541: 540: 534: 533: 532: 531: 527: 487: 481: 474: 419: 396: 375: sin  359: 340: 321: 307: 304: 287: 284: 267: 264: 230: 213: 170: 143: 137: 132:Radial velocity 80: 63: 58:Right ascension 56: 26: 17: 12: 11: 5: 2122: 2120: 2112: 2111: 2106: 2101: 2096: 2091: 2086: 2081: 2076: 2066: 2065: 2059: 2058: 2048: 2045: 2044: 2041: 2040: 2038: 2037: 2031: 2029: 2025: 2024: 2022: 2021: 2016: 2010: 2008: 1999: 1993: 1992: 1989: 1988: 1986: 1985: 1979: 1977: 1967: 1966: 1963: 1962: 1960: 1959: 1954: 1949: 1944: 1938: 1936: 1926: 1925: 1922: 1921: 1919: 1918: 1913: 1908: 1903: 1897: 1895: 1891: 1890: 1888: 1887: 1882: 1877: 1872: 1866: 1864: 1858: 1857: 1855: 1854: 1849: 1844: 1839: 1834: 1829: 1824: 1819: 1814: 1809: 1804: 1799: 1794: 1789: 1784: 1779: 1774: 1769: 1764: 1759: 1754: 1749: 1744: 1739: 1734: 1729: 1724: 1719: 1714: 1709: 1704: 1698: 1696: 1690: 1689: 1687: 1686: 1681: 1676: 1671: 1666: 1661: 1656: 1651: 1646: 1641: 1636: 1631: 1625: 1623: 1617: 1616: 1614: 1613: 1608: 1603: 1598: 1593: 1588: 1583: 1578: 1573: 1568: 1563: 1558: 1553: 1548: 1542: 1540: 1531: 1525: 1524: 1522: 1521: 1516: 1510: 1507: 1506: 1501: 1499: 1498: 1491: 1484: 1476: 1468: 1467: 1415: 1391: 1338: 1335:on 2019-12-15. 1267: 1237: 1180: 1150: 1092: 1028: 998: 945: 908:(3): 695–708. 879: 779: 778: 776: 773: 770: 769: 766: 763: 751: 739: 738:0.059 ± 0.006 736: 732: 716: 707: 706: 701: 696: 691: 681:Orbital period 678: 668:Semimajor axis 665: 660: 635: 632: 546: 545: 535: 529: 528: 521: 520: 514: 513: 512: 511: 508: 507: 502: 494: 493: 489: 488: 441: 325963, 437: 230110, 429: 191849, 418: 415: 414: 408: 407: 404: 403: 393: 385: 384: 381: 364: 363: 356: 348: 347: 337: 329: 328: 318: 310: 309: 305: 302: 298: 290: 289: 285: 282: 278: 270: 269: 265: 262: 258: 250: 249: 246: 245: 241: 240: 237: 236: 233: 228: 220: 219: 207: 199: 198: 192: 183: 182: 157: 148: 147: 140: 135: 127: 126: 123: 122: 116: 115: 112: 105: 104: 101: 95: 94: 90: 89: 86: 77: 76: 73: 67: 66: 61: 53: 52: 47: 41: 40: 15: 13: 10: 9: 6: 4: 3: 2: 2121: 2110: 2107: 2105: 2102: 2100: 2097: 2095: 2092: 2090: 2089:2MASS objects 2087: 2085: 2082: 2080: 2077: 2075: 2072: 2071: 2069: 2056: 2046: 2036: 2033: 2032: 2030: 2026: 2020: 2017: 2015: 2012: 2011: 2009: 2007: 2003: 2000: 1998: 1994: 1984: 1981: 1980: 1978: 1976: 1975:Star clusters 1972: 1968: 1958: 1955: 1953: 1950: 1948: 1945: 1943: 1940: 1939: 1937: 1935: 1931: 1927: 1917: 1914: 1912: 1909: 1907: 1904: 1902: 1899: 1898: 1896: 1892: 1886: 1883: 1881: 1878: 1876: 1873: 1871: 1868: 1867: 1865: 1863: 1859: 1853: 1850: 1848: 1845: 1843: 1840: 1838: 1835: 1833: 1830: 1828: 1825: 1823: 1820: 1818: 1815: 1813: 1810: 1808: 1805: 1803: 1800: 1798: 1795: 1793: 1790: 1788: 1785: 1783: 1780: 1778: 1775: 1773: 1770: 1768: 1765: 1763: 1760: 1758: 1755: 1753: 1750: 1748: 1745: 1743: 1740: 1738: 1735: 1733: 1730: 1728: 1725: 1723: 1720: 1718: 1715: 1713: 1710: 1708: 1705: 1703: 1700: 1699: 1697: 1695: 1691: 1685: 1682: 1680: 1677: 1675: 1672: 1670: 1667: 1665: 1662: 1660: 1657: 1655: 1652: 1650: 1647: 1645: 1642: 1640: 1637: 1635: 1632: 1630: 1627: 1626: 1624: 1622: 1618: 1612: 1609: 1607: 1604: 1602: 1599: 1597: 1594: 1592: 1589: 1587: 1584: 1582: 1579: 1577: 1574: 1572: 1569: 1567: 1564: 1562: 1559: 1557: 1554: 1552: 1549: 1547: 1544: 1543: 1541: 1539: 1535: 1532: 1530: 1526: 1520: 1517: 1515: 1512: 1511: 1508: 1504: 1497: 1492: 1490: 1485: 1483: 1478: 1477: 1474: 1464: 1460: 1456: 1452: 1448: 1444: 1439: 1434: 1430: 1426: 1419: 1416: 1410: 1405: 1398: 1396: 1392: 1387: 1383: 1379: 1375: 1371: 1367: 1362: 1357: 1353: 1349: 1342: 1339: 1334: 1330: 1324: 1320: 1316: 1312: 1305: 1301: 1297: 1293: 1285: 1281: 1277: 1271: 1268: 1257: 1253: 1252: 1247: 1241: 1238: 1234: 1230: 1226: 1222: 1218: 1214: 1209: 1204: 1200: 1196: 1189: 1187: 1185: 1181: 1176: 1172: 1168: 1164: 1157: 1155: 1151: 1146: 1142: 1138: 1134: 1130: 1126: 1121: 1116: 1112: 1108: 1101: 1099: 1097: 1093: 1088: 1084: 1079: 1074: 1070: 1066: 1061: 1056: 1052: 1048: 1044: 1037: 1035: 1033: 1029: 1016: 1012: 1008: 1002: 999: 994: 990: 986: 982: 978: 974: 969: 964: 960: 956: 949: 946: 941: 937: 933: 929: 925: 921: 916: 911: 907: 903: 902: 894: 892: 890: 888: 886: 884: 880: 876: 872: 866: 862: 855: 851: 846: 841: 837: 833: 828: 823: 819: 815: 814: 809: 807: 801: 795: 793: 791: 789: 787: 785: 781: 774: 767: 764: 752: 740: 737: 735: 731: 717: 714:(unconfirmed) 712: 709: 708: 705: 700: 695: 688: 682: 675: 669: 664: 653: 647: 645: 641: 633: 631: 629: 625: 621: 613: 609: 604: 602: 598: 594: 590: 586: 582: 578: 577:John M. Thome 574: 573: 568: 564: 560: 559:constellation 556: 552: 539: 518: 509: 506: 503: 501: 500: 496: 495: 490: 484: 477: 472: 468: 465: 48880, 464: 460: 456: 452: 448: 444: 440: 436: 433: 99701, 432: 428: 422: 416: 413: 409: 405: 402: 394: 392: 391: 387: 386: 383:1.0 km/s 382: 380: 378: 374: 370: 366: 365: 357: 355: 354: 350: 349: 346: 338: 336: 335: 331: 330: 327: 319: 317: 316: 312: 311: 308: 299: 297: 296: 292: 291: 288: 279: 277: 276: 272: 271: 268: 259: 257: 256: 252: 251: 247: 242: 238: 234: 232: 226: 222: 221: 217: 212: 208: 206: 205: 201: 200: 197: 193: 191: 189: 185: 184: 181: 177: 169: 165: 158: 156: 154: 153:Proper motion 150: 149: 146:0.5 km/s 141: 139: 133: 129: 128: 124: 121: 117: 113: 111: 107: 106: 102: 100: 97: 96: 91: 87: 83: 79: 78: 74: 72: 69: 68: 62: 59: 55: 54: 51: 48: 46: 45:Constellation 43: 42: 39: 36: 32: 29: 23: 1947:Gliese 784 b 1942:Gliese 754 b 1910: 1428: 1424: 1418: 1409:1906.04644v1 1351: 1347: 1341: 1333:the original 1314: 1310: 1295: 1291: 1283: 1279: 1276:Thome, J. M. 1270: 1259:. Retrieved 1249: 1240: 1198: 1194: 1166: 1162: 1110: 1106: 1050: 1046: 1021:November 23, 1019:. Retrieved 1010: 1001: 958: 954: 948: 905: 899: 817: 811: 805: 729: 710: 694:Eccentricity 637: 605: 580: 570: 567:exoplanetary 553:is a single 550: 549: 497: 469: 4794, 461: 7999, 453: 3531, 449: 1532, 388: 376: 372: 367: 351: 332: 313: 293: 273: 253: 223: 202: 186: 151: 130: 64:20 13 53.396 2084:Telescopium 2035:PKS 2014-55 1298:: 1. 1900. 1246:"HD 191849" 1169:: 159–165. 699:Inclination 624:photosphere 589:light-years 581:CD−45 13677 563:Telescopium 538:Telescopium 457: 730, 334:Metallicity 315:Temperature 110:color index 71:Declination 50:Telescopium 20:Gliese 784 2068:Categories 1934:Exoplanets 1911:Gliese 784 1906:Gliese 754 1438:2004.12597 1361:1805.07581 1288:(See also 1261:2021-11-22 1208:1910.10389 1120:1908.04627 1060:1604.07403 1053:(2): 171. 961:(5): 331. 827:2012.01533 775:References 551:Gliese 784 530:Gliese 784 343:0.06  300:0.06  295:Luminosity 280:0.58  260:0.58  120:Astrometry 1952:GJ 1252 b 1463:216553868 1233:204838030 1145:199552090 1087:119241004 993:119257644 968:1108.4971 854:227254300 655:Companion 591:from the 555:red dwarf 423:−45 13677 399:0.4  84: (V) 2055:Category 1997:Galaxies 1983:NGC 6584 1957:KELT-10b 1621:Variable 1386:56269929 1286:: 1–502. 1015:Archived 940:16080025 597:parallax 353:Rotation 324:92  306:☉ 286:☉ 266:☉ 227: (M 204:Distance 188:Parallax 1916:GJ 1252 1901:KELT-10 1443:Bibcode 1366:Bibcode 1354:: A37. 1319:Bibcode 1300:Bibcode 1213:Bibcode 1201:: A37, 1171:Bibcode 1125:Bibcode 1113:: A80. 1065:Bibcode 973:Bibcode 920:Bibcode 869:. 832:Bibcode 747:−0.0038 745:+0.0033 610:with a 244:Details 38:J2000.0 35:Equinox 31:J2000.0 1885:191760 1880:181295 1875:177365 1870:173047 1461:  1384:  1251:SIMBAD 1231:  1143:  1085:  1011:RECONS 991:  938:  875:VizieR 852:  820:: A1. 742:6.6592 704:Radius 626:at an 620:period 499:SIMBAD 275:Radius 2028:Other 1894:Other 1538:Bayer 1529:Stars 1459:S2CID 1433:arXiv 1404:arXiv 1382:S2CID 1356:arXiv 1229:S2CID 1203:arXiv 1141:S2CID 1115:arXiv 1083:S2CID 1055:arXiv 989:S2CID 963:arXiv 936:S2CID 910:arXiv 850:S2CID 822:arXiv 759:−0.05 757:+0.23 483:2MASS 339:−0.07 320:3,754 172:Dec.: 142:−33.5 114:1.45 88:7.96 28:Epoch 2019:6861 2014:6845 1852:7766 1847:7758 1842:7749 1837:7745 1832:7714 1827:7674 1822:7621 1817:7549 1812:7548 1807:7537 1802:7521 1797:7459 1792:7411 1787:7388 1782:7370 1777:7297 1772:7289 1767:7271 1762:7233 1757:7223 1752:7190 1747:7097 1742:7095 1737:7093 1732:7092 1727:7065 1722:6986 1717:6954 1712:6894 1707:6821 1702:6778 1023:2021 806:Gaia 754:0.05 724:−4.1 722:+4.6 687:days 663:Mass 505:data 463:NLTT 395:0.85 255:Mass 235:9.01 108:B−V 103:M0V 2006:NGC 1451:doi 1429:132 1374:doi 1352:616 1221:doi 1199:632 1167:208 1133:doi 1111:629 1073:doi 1051:826 981:doi 928:doi 906:460 873:at 861:doi 840:doi 818:649 719:9.4 593:Sun 575:by 561:of 476:TYC 467:PLX 459:LTT 455:LPM 451:LHS 447:LFT 439:PPM 435:SAO 431:HIP 401:Gyr 390:Age 345:dex 196:mas 190:(π) 176:mas 164:mas 160:RA: 155:(μ) 2070:: 1862:HD 1694:HR 1684:QV 1679:QU 1674:QS 1669:QQ 1664:PZ 1659:PW 1654:PV 1649:HO 1644:BL 1639:RX 1634:RS 1629:RR 1457:, 1449:, 1441:, 1427:, 1394:^ 1380:. 1372:. 1364:. 1350:. 1317:. 1315:18 1313:. 1296:18 1294:. 1284:18 1282:. 1254:. 1248:. 1227:, 1219:, 1211:, 1197:, 1183:^ 1165:. 1153:^ 1139:. 1131:. 1123:. 1109:. 1095:^ 1081:. 1071:. 1063:. 1049:. 1045:. 1031:^ 1009:. 987:. 979:. 971:. 959:38 957:. 934:. 926:. 918:. 904:. 882:^ 848:. 838:. 830:. 816:. 810:. 783:^ 768:— 765:— 733:🜨 674:AU 480:, 471:PM 443:Ci 427:HD 425:, 421:CD 362:12 358:48 216:pc 211:ly 180:yr 168:yr 134:(R 1611:τ 1606:ρ 1601:ξ 1596:ν 1591:μ 1586:λ 1581:κ 1576:ι 1571:η 1566:ζ 1561:ε 1556:δ 1551:δ 1546:α 1495:e 1488:t 1481:v 1453:: 1445:: 1435:: 1412:. 1406:: 1388:. 1376:: 1368:: 1358:: 1325:. 1321:: 1302:: 1264:. 1223:: 1215:: 1205:: 1177:. 1173:: 1147:. 1135:: 1127:: 1117:: 1089:. 1075:: 1067:: 1057:: 1025:. 995:. 983:: 975:: 965:: 942:. 930:: 922:: 912:: 877:. 867:) 863:: 856:. 842:: 834:: 824:: 804:" 730:M 711:b 689:) 685:( 676:) 672:( 616:± 397:± 379:) 377:i 373:v 371:( 360:± 341:± 326:K 322:± 303:L 283:R 263:M 231:) 229:V 218:) 178:/ 166:/ 144:± 138:) 136:v

Index

Epoch
J2000.0
Equinox
J2000.0
Constellation
Telescopium
Right ascension
Declination
Apparent magnitude
Spectral type
color index
Astrometry
Radial velocity
Proper motion
mas
yr
mas
yr
Parallax
mas
Distance
ly
pc
Absolute magnitude
Mass
M
Radius
R
Luminosity
L

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