573:). Analysis of the data revealed that, of the two-component stars in the Kepler-14 system, both stars are of nearly equal magnitude, although one of the stars was fainter. The brighter star was designated the "A" component, and the fainter star received the "B" designation. The transit signal was observed in orbit around the A component of the system, meaning that the planetary candidate would be in orbit of the primary star of Kepler-14. This was confirmed on August 7, 2010, when the Infrared Array Camera on the
494:
481:. The star system was identified by Kepler as a possible planetary host, but when imaging revealed that Kepler-14 was a binary star system and not a single star, the confirmation process became protracted. The stars are separated by at least 280 AU, and the stars complete an orbit around a common center of mass every 2800 years. Both stars are larger than the Sun. They are of similar
589:
that the assumed characteristics of the stars and their planets may be incorrect. As a result of their studies into Kepler-14, the Kepler team suggested the implementation of a high-resolution imaging campaign to re-examine transiting planet hosts, an effort that would require only a modest amount of telescope time.
588:
Kepler-14's nature as a close binary star was almost missed by the astronomers, and would not have been known if high-resolution imaging of the star had not been undertaken. The Kepler team acknowledged that a number of transiting planets' host stars may have actually been close visual binaries and
628:
Because Kepler-14 is so close-knit as seen from Earth, it was impossible for the discovery team to separate the two stars and analyze their characteristics as separate stars. The Kepler team analyzed their characteristics under the assumption that Kepler-14 was a single star. If Kepler-14 were a
509:
launched the satellite in April 2009. Kepler-14 was provisionally designated KOI-98. Because Kepler-14's transit signal seemed to imply that the possible planet had a short orbit and a clear effect on Kepler-14's brightness, the Kepler science team forwarded the candidate to the
1039:
Eylen, Vincent Van; Albrecht, Simon; Huang, Xu; MacDonald, Mariah G.; Dawson, Rebekah I.; Cai, Maxwell X.; Foreman-Mackey, Daniel; Lundkvist, Mia S.; Aguirre, Victor Silva; Snellen, Ignas; Winn, Joshua N. (2019), "The
Orbital Eccentricity of Small Planet Systems",
553:, something that radial velocity data alone could not recognize. Because of this new discovery, further investigation of Kepler-14 was postponed until after the publishing of the first five new Kepler planets (the ones orbiting
2144:
1797:
605:
of the Kepler-14 binary system is approximated at 2800 years. The two stars are of nearly equal brightness, but the primary component is slightly brighter as it has a more visible
2629:
581:
data. Analysis of both the
Spitzer photometric data and the radial velocity data confirmed the idea of a planet as the source of the transit signal. The planet was designated
1011:
2619:
2624:
458:
895:
28:
1165:
715:
649:
would be 0.12, or 132% the amount found in the Sun. Assuming that Kepler-14's two stars formed at about the same time, their
419:
347:
900:
2121:
1338:
1190:
403:
518:
511:
574:
2634:
1764:
630:
578:
161:
2614:
2437:
1536:
1310:
1185:
650:
638:
526:
320:
1117:
1059:
1016:
972:
864:
837:
741:
688:
452:
407:
132:
41:
613:, and the secondary has an estimated mass of 1.39 times the Sun's mass. The Kepler-14 system is 980
2390:
746:
542:
502:
474:
1158:
1107:
1077:
1049:
962:
687:. Kepler-14b completes an orbit every 6.79 days with a slightly irregular orbit indicated by its
622:
606:
482:
415:
73:
1995:
1975:
1965:
1960:
1945:
1526:
1521:
1516:
1511:
1506:
1501:
1496:
1491:
1481:
1476:
1471:
675:, the equivalent of 2670 times Earth's mass. The planet is slightly larger than Jupiter at 1.14
1930:
1925:
1920:
1905:
1895:
1875:
1754:
1749:
1744:
1739:
1734:
1729:
1719:
1714:
1699:
1684:
1679:
1654:
1644:
1639:
1634:
1604:
1599:
1594:
1589:
1584:
1579:
1569:
1559:
1554:
2565:
2560:
2550:
2545:
2540:
2535:
2530:
2525:
2520:
2515:
2510:
2505:
2495:
2485:
2480:
2475:
2470:
2465:
2460:
2455:
2450:
2445:
1466:
1461:
1446:
1436:
1431:
1421:
1416:
1411:
1406:
1401:
1396:
1391:
1386:
1381:
1376:
1209:
721:
598:
411:
368:
225:
24:
2076:
1366:
1361:
1356:
1351:
1127:
1067:
982:
868:
694:
Radial velocity measurements of host star did not reveal any additional planets as in 2018.
585:, and this was published alongside the data and research on Kepler-14 in a June 2011 paper.
534:
307:
444:
2116:
2101:
2081:
546:
538:
530:
522:
216:
49:
855:
Høg, E.; et al. (2000). "The Tycho-2 catalogue of the 2.5 million brightest stars".
1122:
1063:
977:
841:
501:
Kepler-14 was identified as a possible host to a planet during the first four months of
798:
792:
728:
676:
609:, or its brightness as seen from Earth. The primary star has an estimated mass of 1.51
602:
497:
The
Palomar Observatory confirmed findings suggesting that Kepler-14 was a binary star.
395:
199:
120:
108:
2609:
2603:
1247:
1242:
1151:
1081:
832:
Zacharias, N. (2009). "Third U.S. Naval
Observatory CCD Astrograph Catalog (UCAC3)".
97:
36:
987:
950:
671:-like planet in the orbit of the primary star of Kepler-14. The planet is 8.4 times
2382:
2363:
1282:
1237:
1232:
1096:"Revisiting the Kepler field with TESS: Improved ephemerides using TESS 2 min data"
766:
672:
642:
634:
278:
242:
493:
951:"Kepler-14b: A Massive Hot Jupiter Transiting an F Star in a Close Visual Binary"
2418:
2358:
2337:
2332:
2327:
2322:
2317:
2312:
2307:
2055:
1277:
1267:
1257:
1252:
1227:
646:
550:
470:
335:
62:
1072:
2395:
2302:
2297:
2292:
2287:
2282:
2277:
2272:
2267:
2262:
2257:
2252:
2247:
2242:
2237:
2232:
2227:
2222:
2217:
2212:
2207:
2202:
2197:
2192:
2187:
2182:
2177:
2071:
2050:
2045:
2040:
2035:
2030:
2025:
2020:
2015:
2010:
2005:
2000:
1990:
1985:
1980:
1970:
1955:
1950:
1940:
1935:
1486:
1272:
1222:
759:
684:
662:
633:
star with a mass of 1.512 times the Sun's, and a size that is 2.048 times the
618:
610:
597:
Kepler-14 is a binary star whose two components are separated by at least 280
582:
478:
291:
249:
139:
85:
2172:
2167:
2162:
2157:
2152:
2135:
1915:
1910:
1900:
1890:
1885:
1880:
1870:
1865:
1860:
1855:
1850:
1845:
1840:
1835:
1830:
1820:
1787:
1782:
1777:
1772:
1724:
1709:
1704:
1694:
1689:
1674:
1669:
1664:
1659:
1649:
1629:
1624:
1619:
1614:
1609:
1574:
1564:
1549:
1544:
1300:
1295:
1262:
1132:
1095:
890:
2555:
2500:
2490:
2400:
2353:
2096:
1815:
1810:
1805:
1456:
1451:
1441:
1426:
1371:
1328:
1323:
1318:
1287:
570:
566:
562:
558:
554:
525:
in
October 2009. Other radial velocity measurements were collected using
384:
1143:
2581:
2368:
2111:
2086:
1346:
668:
2428:
2410:
2106:
2091:
751:
683:, the second densest planet confirmed by the Kepler spacecraft after
614:
438:
327:
262:
144:
1112:
1054:
1200:
967:
492:
423:
171:
1217:
1174:
710:
506:
207:
124:
112:
1147:
734:
477:
spacecraft. It is host to one known planet: the
Jupiter-like
485:; however, the primary star is brighter as seen from Earth.
601:, or the distance between the Earth and Sun. The estimated
517:
625:
of 12.12, and thus cannot be seen with the unaided eye.
949:
Buchhave, Lars A.; et al. (28 September 2011).
2574:
2436:
2427:
2409:
2381:
2346:
2143:
2134:
2064:
1796:
1763:
1535:
1337:
1309:
1208:
1199:
1100:Monthly Notices of the Royal Astronomical Society
1094:Battley, Matthew P; et al. (10 March 2021).
944:
942:
940:
938:
549:, revealed that Kepler-14 was actually a close
936:
934:
932:
930:
928:
926:
924:
922:
920:
918:
1159:
8:
2630:Planetary systems with one confirmed planet
1006:
1004:
1002:
1000:
998:
955:The Astrophysical Journal Supplement Series
645:, much hotter than the Sun, and the star's
67:+47° 19′ 58.87″
2433:
2140:
1205:
1166:
1152:
1144:
653:would be approximately 2.2 billion years.
1131:
1121:
1111:
1071:
1053:
986:
976:
966:
27:J2000
696:
529:. The FIES and Keck data, combined with
827:
825:
823:
821:
817:
104:
505:'s operational data, which began when
15:
884:
882:
880:
878:
7:
903:from the original on 19 October 2012
116:
14:
1012:"Confimred Planet Overview Page"
896:Extrasolar Planets Encyclopaedia
698:The Kepler-14 planetary system
891:"Notes for Planet Kepler-14 b"
1:
679:The density of Kepler-14b is
577:observed Kepler-14 to gather
750:
745:
740:
727:
714:
709:
702:
629:single star, it would be an
2620:Planetary transit variables
834:VizieR On-line Data Catalog
641:of Kepler-14 would be 6395
2651:
2625:Kepler objects of interest
857:Astronomy and Astrophysics
660:
2122:WISEP J190648.47+401106.8
1191:Lyra in Chinese astronomy
1181:
988:10.1088/0067-0049/197/1/3
431:
401:
394:
390:
236:
231:
170:
155:
151:
91:
84:
21:
1073:10.3847/1538-3881/aaf22f
1042:The Astronomical Journal
637:. As a single star, the
621:) from Earth. It has an
519:Nordic Optical Telescope
512:Kepler Follow-up Program
889:Jean Schneider (2011).
869:2000A&A...355L..27H
575:Spitzer Space Telescope
521:to measure Kepler-14's
473:system targeted by the
74:Apparent magnitude
651:gyrochronological ages
498:
2359:HD 173416 b (Wangshu)
1186:List of stars in Lyra
1175:Constellation of Lyra
1133:10.1093/mnras/stab701
639:effective temperature
611:times that of the Sun
527:W.M. Keck Observatory
496:
489:Observational history
362:7.9 (± 1.0) km/s
248:1.512 (± 0.043)
1017:Ames Research Center
706:(in order from star)
689:orbital eccentricity
2354:HAT-P-5b (Kráľomoc)
1123:2021MNRAS.503.4092B
1064:2019AJ....157...61V
978:2011ApJS..197....3B
842:2009yCat.1315....0Z
699:
543:Palomar Observatory
483:absolute magnitudes
432:Database references
348:Rotational velocity
18:
697:
623:apparent magnitude
607:apparent magnitude
599:astronomical units
537:and near-infrared
499:
426:J19105011+4719589
396:Other designations
162:Spectral type
16:
2594:
2593:
2590:
2589:
2377:
2376:
2130:
2129:
809:
808:
738:
725:
707:
464:
463:
326:6395 (± 60)
119: -10.2
2642:
2434:
2141:
2087:HAT-P-5 (Chasoň)
1206:
1168:
1161:
1154:
1145:
1138:
1137:
1135:
1125:
1115:
1106:(3): 4092–4104.
1091:
1085:
1084:
1075:
1057:
1036:
1030:
1029:
1027:
1025:
1008:
993:
992:
990:
980:
970:
946:
913:
912:
910:
908:
886:
873:
872:
852:
846:
845:
829:
801:
785:
783:
769:
732:
719:
705:
700:
682:
667:Kepler-14b is a
657:Planetary system
541:measurements at
535:WIYN Observatory
382:
381:
305:
304:
276:
275:
221:
156:Characteristics
118:
106:
77:
57:
52:
22:Observation data
19:
2650:
2649:
2645:
2644:
2643:
2641:
2640:
2639:
2600:
2599:
2597:
2595:
2586:
2570:
2423:
2405:
2391:δ Lyrae cluster
2373:
2342:
2126:
2082:GSC 02652-01324
2060:
1792:
1759:
1531:
1333:
1305:
1195:
1177:
1172:
1142:
1141:
1093:
1092:
1088:
1038:
1037:
1033:
1023:
1021:
1010:
1009:
996:
948:
947:
916:
906:
904:
888:
887:
876:
854:
853:
849:
831:
830:
819:
814:
804:
799:
781:
779:
772:
767:
731:
718:
704:
680:
665:
659:
595:
593:Characteristics
547:MMT Observatory
539:adaptive optics
531:speckle imaging
523:radial velocity
491:
427:
422:J19108+4720AB,
380:
377:
376:
375:
354: sin
313:
310:
303:
300:
299:
298:
284:
281:
274:
271:
270:
269:
255:
252:
217:Semi-major axis
214:
142:
115:
107: 1.0
72:
55:
50:Right ascension
48:
23:
12:
11:
5:
2648:
2646:
2638:
2637:
2632:
2627:
2622:
2617:
2612:
2602:
2601:
2592:
2591:
2588:
2587:
2585:
2584:
2578:
2576:
2572:
2571:
2569:
2568:
2563:
2558:
2553:
2548:
2543:
2538:
2533:
2528:
2523:
2518:
2513:
2508:
2503:
2498:
2493:
2488:
2483:
2478:
2473:
2468:
2463:
2458:
2453:
2448:
2442:
2440:
2431:
2425:
2424:
2422:
2421:
2415:
2413:
2407:
2406:
2404:
2403:
2398:
2393:
2387:
2385:
2379:
2378:
2375:
2374:
2372:
2371:
2366:
2361:
2356:
2350:
2348:
2344:
2343:
2341:
2340:
2335:
2330:
2325:
2320:
2315:
2310:
2305:
2300:
2295:
2290:
2285:
2280:
2275:
2270:
2265:
2260:
2255:
2250:
2245:
2240:
2235:
2230:
2225:
2220:
2215:
2210:
2205:
2200:
2195:
2190:
2185:
2180:
2175:
2170:
2165:
2160:
2155:
2149:
2147:
2138:
2132:
2131:
2128:
2127:
2125:
2124:
2119:
2117:WISE 1828+2650
2114:
2109:
2104:
2102:LSR J1835+3259
2099:
2094:
2089:
2084:
2079:
2074:
2068:
2066:
2062:
2061:
2059:
2058:
2053:
2048:
2043:
2038:
2033:
2028:
2023:
2018:
2013:
2008:
2003:
1998:
1993:
1988:
1983:
1978:
1973:
1968:
1963:
1958:
1953:
1948:
1943:
1938:
1933:
1928:
1923:
1918:
1913:
1908:
1903:
1898:
1893:
1888:
1883:
1878:
1873:
1868:
1863:
1858:
1853:
1848:
1843:
1838:
1833:
1828:
1823:
1818:
1813:
1808:
1802:
1800:
1794:
1793:
1791:
1790:
1785:
1780:
1775:
1769:
1767:
1761:
1760:
1758:
1757:
1752:
1747:
1742:
1737:
1732:
1727:
1722:
1717:
1712:
1707:
1702:
1697:
1692:
1687:
1682:
1677:
1672:
1667:
1662:
1657:
1652:
1647:
1642:
1637:
1632:
1627:
1622:
1617:
1612:
1607:
1602:
1597:
1592:
1587:
1582:
1577:
1572:
1567:
1562:
1557:
1552:
1547:
1541:
1539:
1533:
1532:
1530:
1529:
1524:
1519:
1514:
1509:
1504:
1499:
1494:
1489:
1484:
1479:
1474:
1469:
1464:
1459:
1454:
1449:
1444:
1439:
1434:
1429:
1424:
1419:
1414:
1409:
1404:
1399:
1394:
1389:
1384:
1379:
1374:
1369:
1364:
1359:
1354:
1349:
1343:
1341:
1335:
1334:
1332:
1331:
1326:
1321:
1315:
1313:
1307:
1306:
1304:
1303:
1298:
1293:
1285:
1280:
1275:
1270:
1265:
1260:
1255:
1250:
1245:
1240:
1235:
1230:
1225:
1220:
1214:
1212:
1203:
1197:
1196:
1194:
1193:
1188:
1182:
1179:
1178:
1173:
1171:
1170:
1163:
1156:
1148:
1140:
1139:
1086:
1031:
994:
914:
874:
847:
816:
815:
813:
810:
807:
806:
802:
795:
789:
786:
777:
774:
770:
763:
755:
754:
749:
744:
739:
729:Orbital period
726:
716:Semimajor axis
713:
708:
673:Jupiter's mass
661:Main article:
658:
655:
603:orbital period
594:
591:
490:
487:
462:
461:
456:
448:
447:
442:
434:
433:
429:
428:
402:
399:
398:
392:
391:
388:
387:
378:
372:
364:
363:
360:
343:
342:
341:+0.12 (± 0.06)
339:
331:
330:
324:
316:
315:
311:
308:
301:
295:
287:
286:
282:
279:
272:
266:
258:
257:
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211:
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174:
168:
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136:
128:
127:
102:
93:
92:
89:
88:
82:
81:
78:
69:
68:
65:
59:
58:
53:
45:
44:
39:
33:
32:
13:
10:
9:
6:
4:
3:
2:
2647:
2636:
2635:2MASS objects
2633:
2631:
2628:
2626:
2623:
2621:
2618:
2616:
2613:
2611:
2608:
2607:
2605:
2598:
2583:
2580:
2579:
2577:
2573:
2567:
2564:
2562:
2559:
2557:
2554:
2552:
2549:
2547:
2544:
2542:
2539:
2537:
2534:
2532:
2529:
2527:
2524:
2522:
2519:
2517:
2514:
2512:
2509:
2507:
2504:
2502:
2499:
2497:
2494:
2492:
2489:
2487:
2484:
2482:
2479:
2477:
2474:
2472:
2469:
2467:
2464:
2462:
2459:
2457:
2454:
2452:
2449:
2447:
2444:
2443:
2441:
2439:
2435:
2432:
2430:
2426:
2420:
2417:
2416:
2414:
2412:
2408:
2402:
2399:
2397:
2394:
2392:
2389:
2388:
2386:
2384:
2383:Star clusters
2380:
2370:
2367:
2365:
2362:
2360:
2357:
2355:
2352:
2351:
2349:
2345:
2339:
2336:
2334:
2331:
2329:
2326:
2324:
2321:
2319:
2316:
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2311:
2309:
2306:
2304:
2301:
2299:
2296:
2294:
2291:
2289:
2286:
2284:
2281:
2279:
2276:
2274:
2271:
2269:
2266:
2264:
2261:
2259:
2256:
2254:
2251:
2249:
2246:
2244:
2241:
2239:
2236:
2234:
2231:
2229:
2226:
2224:
2221:
2219:
2216:
2214:
2211:
2209:
2206:
2204:
2201:
2199:
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2184:
2181:
2179:
2176:
2174:
2171:
2169:
2166:
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2161:
2159:
2156:
2154:
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2150:
2148:
2146:
2142:
2139:
2137:
2133:
2123:
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2118:
2115:
2113:
2110:
2108:
2105:
2103:
2100:
2098:
2095:
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2075:
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2057:
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2047:
2044:
2042:
2039:
2037:
2034:
2032:
2029:
2027:
2024:
2022:
2019:
2017:
2014:
2012:
2009:
2007:
2004:
2002:
1999:
1997:
1994:
1992:
1989:
1987:
1984:
1982:
1979:
1977:
1974:
1972:
1969:
1967:
1964:
1962:
1959:
1957:
1954:
1952:
1949:
1947:
1944:
1942:
1939:
1937:
1934:
1932:
1929:
1927:
1924:
1922:
1919:
1917:
1914:
1912:
1909:
1907:
1904:
1902:
1899:
1897:
1894:
1892:
1889:
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1879:
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1869:
1867:
1864:
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1368:
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1360:
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1327:
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1308:
1302:
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1297:
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1234:
1231:
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1226:
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1216:
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1211:
1207:
1204:
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1198:
1192:
1189:
1187:
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1176:
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1164:
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1157:
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1129:
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1119:
1114:
1109:
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1065:
1061:
1056:
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1043:
1035:
1032:
1019:
1018:
1013:
1007:
1005:
1003:
1001:
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989:
984:
979:
974:
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964:
960:
956:
952:
945:
943:
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939:
937:
935:
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929:
927:
925:
923:
921:
919:
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902:
898:
897:
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811:
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790:
787:
778:
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764:
762:
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756:
753:
748:
743:
736:
730:
723:
717:
712:
701:
695:
692:
690:
686:
681:7.1 g/cm
678:
677:Jupiter radii
674:
670:
664:
656:
654:
652:
648:
644:
640:
636:
632:
626:
624:
620:
616:
612:
608:
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592:
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584:
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568:
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508:
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468:
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457:
455:
454:
450:
449:
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443:
441:
440:
436:
435:
430:
425:
421:
418:03546-00413,
417:
413:
409:
405:
400:
397:
393:
389:
386:
373:
371:
370:
366:
365:
361:
359:
357:
353:
349:
345:
344:
340:
338:
337:
333:
332:
329:
325:
323:
322:
318:
317:
314:
296:
294:
293:
289:
288:
285:
267:
265:
264:
260:
259:
256:
247:
245:
244:
240:
239:
235:
230:
227:
223:
220:
218:
213:
212:
209:
205:
203:
201:
197:
196:
192:
190:
187:
186:
182:
180:
177:
176:
173:
169:
165:
163:
160:
159:
154:
150:
146:
141:
137:
135:
134:
130:
129:
126:
122:
114:
110:
103:
101:
99:
98:Proper motion
95:
94:
90:
87:
83:
79:
75:
71:
70:
66:
64:
61:
60:
54:
51:
47:
46:
43:
40:
38:
37:Constellation
35:
34:
30:
26:
20:
2615:Binary stars
2596:
2364:HD 178911 Bb
1825:
1289:
1103:
1099:
1089:
1045:
1041:
1034:
1022:. Retrieved
1015:
958:
954:
905:. Retrieved
894:
860:
856:
850:
833:
784:0.0000003985
780:6.7901236131
758:
742:Eccentricity
693:
666:
647:iron content
635:Sun's radius
627:
596:
587:
516:
500:
466:
465:
451:
437:
414:3546-413-1,
367:
355:
351:
346:
334:
319:
290:
273:−0.084
261:
241:
215:
198:
188:
178:
131:
96:
56:19 10 50.110
2419:Ring Nebula
1610:7043 (Xihe)
1263:η (Aladfar)
1228:γ (Sulafat)
1223:β (Sheliak)
907:5 September
863:: L27–L30.
747:Inclination
619:light years
579:photometric
551:binary star
471:binary star
336:Metallicity
321:Temperature
302:−0.58
63:Declination
2604:Categories
2396:Messier 56
2136:Exoplanets
2072:Gliese 758
1290:(Alathfar)
1113:2103.03259
1055:1807.00549
812:References
797:1.14
691:of 0.035.
685:Kepler-10b
663:Kepler-14b
583:Kepler-14b
533:data from
479:Kepler-14b
410:10264660,
379:−0.1
292:Luminosity
193:Kepler-14B
183:Kepler-14A
143:(980
138:3200
86:Astrometry
17:Kepler-14
1311:Flamsteed
1082:119082221
1048:(2): 61,
968:1106.5510
765:8.4
703:Companion
467:Kepler-14
189:Companion
76: (V)
2429:Galaxies
2401:NGC 6791
2097:LHS 6343
1339:Variable
1218:α (Vega)
1024:18 April
901:Archived
571:Kepler-8
567:Kepler-7
563:Kepler-6
559:Kepler-5
555:Kepler-4
545:and the
514:(KFOP).
312:☉
283:☉
254:☉
133:Distance
2582:IC 1296
2411:Nebulae
2369:TrES-1b
2112:WASP-58
2077:GJ 4063
1118:Bibcode
1060:Bibcode
973:Bibcode
961:(1) 3.
865:Bibcode
838:Bibcode
669:Jupiter
617:(3,196
615:parsecs
232:Details
179:Primary
29:Equinox
2145:Kepler
2107:WASP-3
2092:KSw 71
1798:Kepler
1788:181068
1783:180314
1778:179070
1773:177830
1347:R (13)
1080:
1020:. NASA
788:0.035
752:Radius
631:F-type
569:, and
503:Kepler
475:Kepler
439:SIMBAD
383:
306:
277:
268:2.048
263:Radius
206:~2800
200:Period
80:12.00
31:J2000
2575:Other
2347:Other
2065:Other
1210:Bayer
1201:Stars
1108:arXiv
1078:S2CID
1050:arXiv
963:arXiv
469:is a
424:2MASS
406:-98,
297:6.29
172:Orbit
117:Dec.:
25:Epoch
2610:Lyra
2566:6792
2561:6765
2556:6745
2551:6740
2546:6713
2541:6710
2536:6703
2531:6702
2526:6700
2521:6695
2516:6692
2511:6688
2506:6686
2501:6685
2496:6675
2491:6672
2486:6671
2481:6665
2476:6663
2471:6662
2466:6657
2461:6646
2456:6640
2451:6612
2446:6606
2338:705b
2333:453b
2328:422b
2323:440b
2318:438b
2308:277b
2056:1513
1755:7382
1750:7376
1745:7359
1740:7346
1735:7345
1730:7338
1725:7302
1720:7284
1715:7280
1710:7272
1705:7253
1700:7244
1695:7238
1690:7237
1685:7212
1680:7204
1675:7202
1670:7181
1665:7162
1660:7146
1655:7140
1650:7132
1645:7118
1640:7115
1635:7112
1630:7081
1625:7073
1620:7064
1615:7044
1605:7041
1600:7033
1595:7030
1590:7019
1585:7017
1580:7016
1575:6997
1570:6984
1565:6968
1560:6901
1555:6853
1550:6847
1545:6845
1527:V558
1522:V550
1517:V545
1512:V543
1507:V542
1502:V533
1497:V478
1492:V477
1487:V473
1482:V404
1477:V361
1472:V344
1026:2019
909:2011
735:days
711:Mass
507:NASA
459:data
445:data
374:2.2
243:Mass
224:280
42:Lyra
2438:NGC
2303:93b
2298:91b
2273:62b
2268:60d
2263:59b
2248:37b
2243:26e
2233:25b
2213:24b
2183:20b
2178:14b
2051:705
2046:635
2041:444
2036:429
2031:421
2026:410
2021:350
2016:282
2011:279
2006:277
2001:238
1996:177
1991:174
1986:160
1981:138
1976:131
1971:130
1966:128
1961:109
1956:105
1951:104
1946:103
1941:102
1936:100
1128:doi
1104:503
1068:doi
1046:157
983:doi
959:197
861:355
791:~90
453:KIC
420:WDS
416:GSC
412:TYC
408:KIC
404:KOI
385:Gyr
369:Age
219:(a)
202:(P)
121:mas
109:mas
105:RA:
100:(μ)
2606::
2163:9b
2158:8b
2153:7b
1931:98
1926:95
1921:94
1916:93
1911:92
1906:91
1901:88
1896:75
1891:65
1886:62
1881:60
1876:59
1871:46
1866:38
1861:37
1856:30
1851:26
1846:25
1841:24
1836:20
1831:19
1826:14
1821:13
1765:HD
1537:HR
1467:MV
1462:KX
1457:HR
1452:HP
1447:HK
1442:FL
1437:EZ
1432:EP
1427:DM
1422:CY
1417:CN
1412:CC
1407:AY
1402:XY
1397:UZ
1392:TZ
1387:TT
1382:RZ
1377:RV
1372:RR
1329:19
1324:17
1319:16
1288:μ
1126:.
1116:.
1102:.
1098:.
1076:,
1066:,
1058:,
1044:,
1014:.
997:^
981:.
971:.
957:.
953:.
917:^
899:.
893:.
877:^
859:.
836:.
820:^
776:—
722:AU
565:,
561:,
557:,
226:AU
208:yr
166:F
145:pc
140:ly
125:yr
113:yr
2313:c
2293:f
2288:e
2283:d
2278:c
2258:d
2253:c
2238:c
2228:e
2223:d
2218:c
2208:g
2203:f
2198:e
2193:d
2188:c
2173:d
2168:c
1816:9
1811:8
1806:7
1367:W
1362:V
1357:T
1352:S
1301:ν
1296:ν
1283:λ
1278:κ
1273:ι
1268:θ
1258:ζ
1253:ζ
1248:ε
1243:ε
1238:δ
1233:δ
1167:e
1160:t
1153:v
1136:.
1130::
1120::
1110::
1070::
1062::
1052::
1028:.
991:.
985::
975::
965::
911:.
871:.
867::
844:.
840::
803:J
800:R
793:°
782:±
771:J
768:M
760:b
737:)
733:(
724:)
720:(
643:K
358:)
356:i
352:v
350:(
328:K
309:L
280:R
251:M
147:)
123:/
111:/
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