29:
1683:
35:
1039:
897:
1172:
902:
1034:{\displaystyle {\begin{aligned}2\cdot R_{*}&={\frac {(48\cdot 2.09\cdot 10^{-3})\ {\text{AU}}}{0.0046491\ {\text{AU}}/R_{\bigodot }}}\\&\approx 22\cdot R_{\bigodot }\end{aligned}}}
1061:
1108:
329:
1164:
1213:
719:
Evans, D. S. (June 20–24, 1966), "The
Revision of the General Catalogue of Radial Velocities", in Batten, Alan Henry; Heard, John Frederick (eds.),
1705:
1730:
1059:
Jones, K. L.; et al. (June 1992), "Spectroscopic investigation of cool giants and the authenticity of their reported microwave emission",
1128:
Richichi, A.; Percheron, I.; Khristoforova, M. (February 2005), "CHARM2: An updated
Catalog of High Angular Resolution Measurements",
882:
724:
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52:
1240:
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753:
459:
439:
807:
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1503:
530:
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114:
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1265:
497:
337:
1249:
1137:
1070:
836:
785:
728:
701:
692:
Eggen, O. J. (1962), "Space-velocity vectors for 3483 stars with proper motion and radial velocity",
671:
621:
226:
390:
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637:
611:
516:
caused by adaptation of the
European southern hemisphere constellations into the Chinese system,
493:
247:
97:
721:
Determination of Radial
Velocities and their Applications, Proceedings from IAU Symposium no. 30
500:
of about 4,900 K. This heat is causing it to glow with the characteristic orange hue of a
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878:
470:
431:
419:
48:
868:
1145:
1141:
1098:
1078:
844:
795:
790:
629:
625:
513:
488:. At the estimated distance of this star, this yields a physical size of about 11 times the
478:
466:
359:
210:
1666:
1562:
317:
158:
73:
469:
of this star matches the characteristics of a K0 III, which, according to models of
1074:
840:
732:
705:
675:
1312:
563:
547:
484:
398:
394:
378:
370:
218:
198:
186:
1715:
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1342:
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1226:
874:
849:
175:
60:
641:
1579:
1327:
1307:
1302:
1292:
559:
551:
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489:
304:
277:
34:
1199:
AEEA (Activities of
Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 7 月 29 日
1198:
800:
757:
1150:
633:
1332:
1317:
539:
535:
501:
352:
136:
125:
86:
662:
Johnson, H. L.; et al. (1966), "UBVRIJKL photometry of the bright stars",
1322:
1083:
602:
van
Leeuwen, F. (November 2007), "Validation of the new Hipparcos reduction",
555:
474:
447:
284:
233:
146:
827:
Liu, Y. J.; et al. (2007), "The abundances of nearby red clump giants",
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462:
of this star is +4.24, which is bright enough to be seen with the naked eye
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477:
stage, having exhausted the supply of hydrogen at its core. The measured
455:
1218:
1614:
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1632:
1103:
811:
451:
413:
344:
297:
238:
28:
780:
873:, Astronomy and astrophysics library, vol. 1 (3rd ed.),
616:
1275:
443:
435:
202:
190:
65:
1222:
762:
Data
Release 2: Summary of the contents and survey properties"
382:
1173:
Commonwealth
Scientific and Industrial Research Organisation
900:
664:
Communications of the Lunar and
Planetary Laboratory
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1631:
1607:
1589:
1578:
1555:
1502:
1394:
1351:
1283:
1274:
1033:
756:; et al. (Gaia collaboration) (August 2018).
1062:Monthly Notices of the Royal Astronomical Society
829:Monthly Notices of the Royal Astronomical Society
1054:
1052:
1050:
1048:
534:, refers to an asterism consisting of β Apodis,
597:
595:
1234:
1109:Centre de données astronomiques de Strasbourg
573:
567:
523:
517:
91:−77° 31′ 02.7629″
8:
566:. Consequently, β Apodis itself is known as
1169:Australia Telescope, Outreach and Education
1654:
1628:
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1280:
1241:
1227:
1219:
862:
860:
657:
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978:
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950:
928:
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901:
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848:
822:
820:
799:
789:
779:
615:
51:J2000
723:, vol. 30, University of Toronto:
687:
685:
591:
182:
18:
748:
746:
744:
742:
7:
1175:, December 21, 2004, archived from
194:
446:. It is located approximately 149
14:
1682:
1681:
850:10.1111/j.1365-2966.2007.11852.x
725:International Astronomical Union
217:21.8518 ± 0.2620
33:
27:
808:Gaia DR2 record for this source
454:) from Earth, as determined by
1706:Henry Draper Catalogue objects
959:
931:
473:, indicates that it is in the
40:Location of β Apodis (circled)
16:Star in the constellation Apus
1:
1731:Bright Star Catalogue objects
580:the Third Star of Exotic Bird
767:Astronomy & Astrophysics
197: −355.704 ± 0.576
185: −280.588 ± 0.440
801:10.1051/0004-6361/201833051
574:
524:
1752:
1151:10.1051/0004-6361:20042039
1130:Astronomy and Astrophysics
694:Royal Observatory Bulletin
634:10.1051/0004-6361:20078357
604:Astronomy and Astrophysics
1679:
1653:
1627:
1261:Apus in Chinese astronomy
1256:
867:Lang, Kenneth R. (2006),
579:
568:
518:
460:apparent visual magnitude
440:circumpolar constellation
430:(β Aps, β Apodis) is the
406:
376:
369:
365:
271:
266:
262:
152:
145:
108:
45:
24:
1142:2005A&A...431..773R
1084:10.1093/mnras/256.3.535
791:2018A&A...616A...1G
626:2007A&A...474..653V
248:Absolute magnitude
98:Apparent magnitude
1736:Durchmusterung objects
1035:
870:Astrophysical formulae
496:of Beta Apodis has an
1266:List of stars in Apus
1250:Constellation of Apus
1165:"The Colour of Stars"
1036:
498:effective temperature
169:−30.3 ± 0.7 km/s
898:
1075:1992MNRAS.256..535J
841:2007MNRAS.382..553L
733:1967IAUS...30...57E
706:1962RGOB...51...79E
676:1966CoLPL...4...99J
407:Database references
21:
1031:
1029:
458:measurements. The
371:Other designations
115:Spectral type
19:
1726:Hipparcos objects
1693:
1692:
1675:
1674:
1649:
1648:
1623:
1622:
1574:
1573:
1214:Image Beta Apodis
999:
981:
977:
968:
964:
490:radius of the Sun
471:stellar evolution
432:Bayer designation
425:
424:
237:(45.8 ± 0.5
1743:
1685:
1684:
1655:
1629:
1587:
1361:R (not variable)
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1125:
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646:
645:
619:
599:
581:
577:
571:
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527:
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494:outer atmosphere
487:
481:of this star is
479:angular diameter
438:in the southern
196:
184:
109:Characteristics
101:
81:
76:
46:Observation data
37:
31:
22:
1751:
1750:
1746:
1745:
1744:
1742:
1741:
1740:
1696:
1695:
1694:
1689:
1671:
1667:Sunburst galaxy
1645:
1619:
1603:
1581:
1570:
1551:
1537:137388 (Karaka)
1498:
1390:
1347:
1270:
1252:
1247:
1210:
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1190:
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1111:
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1028:
1027:
1017:
1002:
1001:
988:
971:
946:
930:
921:
911:
896:
895:
892:) is given by:
891:
888:. The radius (R
885:
866:
865:
858:
826:
825:
818:
754:Brown, A. G. A.
752:
751:
740:
718:
717:
713:
691:
690:
683:
661:
660:
649:
601:
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593:
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510:
492:. The expanded
482:
402:
381:-77 1221,
318:Surface gravity
310:
307:
290:
287:
253:
236:
193:
164:
159:Radial velocity
96:
79:
74:Right ascension
72:
47:
41:
39:
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17:
12:
11:
5:
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1254:
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1238:
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1223:
1217:
1216:
1209:
1208:External links
1206:
1203:
1202:
1188:
1156:
1136:(2): 773–777,
1120:
1090:
1069:(3): 535–544,
1044:
1042:
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1016:
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856:
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738:
727:, p. 57,
711:
681:
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610:(2): 653–664,
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32:
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15:
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6:
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3:
2:
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1737:
1734:
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1727:
1724:
1722:
1721:K-type giants
1719:
1717:
1714:
1712:
1711:Bayer objects
1709:
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1704:
1703:
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1189:
1179:on 2012-03-18
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884:3-540-29692-1
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835:(2): 553–66,
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176:Proper motion
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67:
64:
62:
61:Constellation
59:
58:
54:
50:
44:
36:
30:
23:
1563:
1297:
1196:(in Chinese)
1191:
1181:, retrieved
1177:the original
1168:
1159:
1133:
1129:
1123:
1112:. Retrieved
1102:
1093:
1066:
1060:
869:
832:
828:
771:
765:
759:
720:
714:
697:
693:
667:
663:
607:
603:
529:
511:
483:2.09 ± 0.11
464:
427:
426:
412:
397: 6163,
385: 3319,
351:
336:
321:
316:
296:
276:
246:
225:
209:
174:
157:
119:K0 III
20:Beta Apodis
578:, English:
531:Exotic Bird
528:), meaning
502:K-type star
448:light-years
428:Beta Apodis
358:–0.02
353:Metallicity
343:4,900
338:Temperature
137:color index
126:color index
87:Declination
1700:Categories
1183:2012-01-16
1114:2012-06-28
875:Birkhäuser
781:1804.09365
670:(99): 99,
586:References
575:Yì Què sān
548:δ Octantis
475:giant star
320:(log
283:1.84
147:Astrometry
1641:Hen 2-131
1099:"bet Aps"
1023:⨀
1015:⋅
1009:≈
994:⨀
973:0.0046491
952:−
944:⋅
938:⋅
917:∗
909:⋅
617:0708.1752
328:3.0
100: (V)
1687:Category
1659:Galaxies
1582:clusters
1564:Godzilla
1353:Variable
642:18759600
564:ε Apodis
560:α Apodis
556:η Apodis
552:δ Apodis
544:γ Apodis
540:ι Apodis
536:ζ Apodis
467:spectrum
456:parallax
309:☉
303:11
289:☉
250: (M
227:Distance
211:Parallax
1633:Nebulae
1615:IC 4499
1138:Bibcode
1071:Bibcode
837:Bibcode
786:Bibcode
729:Bibcode
702:Bibcode
672:Bibcode
622:Bibcode
514:Chinese
452:parsecs
267:Details
53:Equinox
1547:152010
1542:141846
1532:137366
1527:134606
1522:131664
1517:129899
1512:128294
1104:SIMBAD
976:
963:
881:
812:VizieR
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700:: 79,
640:
525:Yì Què
508:Naming
434:for a
414:SIMBAD
298:Radius
141:+1.06
130:+0.95
104:+4.24
55:J2000
1608:Other
1556:Other
1285:Bayer
1276:Stars
806:
776:arXiv
638:S2CID
612:arXiv
258:0.819
195:Dec.:
49:Epoch
1716:Apus
1599:6101
1580:Star
1566:star
1494:6751
1489:6731
1484:6646
1479:6635
1474:6373
1469:6357
1464:6135
1459:5955
1454:5786
1449:5757
1444:5628
1439:5555
1434:5547
1429:5520
1424:5389
1419:5327
1414:5306
1409:5279
1404:5240
941:2.09
879:ISBN
760:Gaia
562:and
465:The
450:(46
444:Apus
436:star
420:data
278:Mass
135:B−V
124:U−B
66:Apus
1591:NGC
1146:doi
1134:431
1079:doi
1067:256
845:doi
833:382
810:at
796:doi
772:616
630:doi
608:474
582:.)
569:異雀三
512:In
485:mas
442:of
399:SAO
391:HIP
383:FK5
360:dex
330:cgs
219:mas
213:(π)
199:mas
187:mas
183:RA:
178:(μ)
1702::
1504:HD
1396:HR
1386:NO
1381:NN
1376:MY
1171:,
1167:,
1144:,
1132:,
1107:.
1101:.
1077:,
1065:,
1047:^
1012:22
980:AU
967:AU
948:10
935:48
877:,
859:^
843:,
831:,
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770:.
764:.
741:^
698:51
696:,
684:^
666:,
650:^
636:,
628:,
620:,
606:,
594:^
558:,
554:,
550:,
546:,
542:,
538:,
519:異雀
504:.
395:HR
387:HD
379:CP
239:pc
234:ly
203:yr
191:yr
161:(R
1371:Z
1366:S
1343:κ
1338:κ
1333:ι
1328:θ
1323:η
1318:ζ
1313:ε
1308:δ
1303:γ
1298:β
1293:α
1242:e
1235:t
1228:v
1148::
1140::
1117:.
1087:.
1081::
1073::
1019:R
990:R
985:/
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955:3
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668:4
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345:K
324:)
322:g
306:R
286:M
254:)
252:V
241:)
201:/
189:/
165:)
163:v
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