2729:
2803:
1217:
2767:
2791:
31:
2779:
2740:
157:
is a misnomer, because G-type stars actually range in color from white, for more luminous types like the Sun, to only very slightly yellowish for less massive and luminous G-type main-sequence stars. The Sun is in fact white, but it can often appear yellow, orange or red through
193:
A G-type main-sequence star with the mass of the Sun will fuse hydrogen for approximately 10 billion years, until the hydrogen element is exhausted at the center of the star. When this happens, the star rapidly expands, cooling and darkening as it passes through the
573:
G-type main sequence stars can provide habitability for life to develop, such as the Sun with life on Earth. They also live long enough to give life enough time to develop, between 13 and 7.9 billion years. Our Sun lives about 10 billion years.
218:
branch. Expanding even further as helium starts running out as it pulses violently, the star's gravity is not sufficient to hold its outer envelope, resulting in significant mass loss and shedding. The ejected material remains as a
2580:
223:, radiating as it absorbs energetic photons from the photosphere. Eventually, the core begins to fade as nuclear reactions cease, and becomes a dense, compact
109:
to which the Earth is gravitationally bound, is an example of a G-type main-sequence star (G2V type). Each second, the Sun fuses approximately 600 million
902:
551:
B (G3V). The choices of G4 and G6 dwarf standards have changed slightly over the years among expert classifiers, but often-used examples include
2612:
712:
662:
1167:
860:
568:
689:
2823:
831:
2587:
1906:
985:
758:
735:
202:
phase, about 1 billion years after leaving the main sequence. After this, the star's degenerate helium core abruptly ignites in a
2299:
1118:
624:
1137:
1099:
166:, especially at sunrise and sunset. In addition, although the term "dwarf" is used to contrast G-type main-sequence stars with
2213:
805:
2592:
2229:
1248:
2639:
2506:
2757:
2622:
2573:
2548:
1841:
1926:
118:
2563:
2543:
2627:
2558:
2528:
524:
2634:
2511:
2488:
2070:
1519:
1509:
1504:
1499:
1494:
1097:
Fundamental stellar photometry for standards of spectral type on the revised system of the Yerkes spectral atlas
1777:
1651:
1286:
1221:
2304:
1973:
114:
2553:
2103:
2013:
1955:
1881:
1452:
1378:
1328:
1075:
2714:
2694:
2466:
2461:
2254:
2203:
2008:
1998:
1671:
1469:
1437:
1311:
532:
59:
2568:
2538:
2533:
2523:
2451:
2239:
1405:
674:
293:
67:
1686:
2709:
2607:
2597:
2446:
2414:
2208:
2003:
1988:
1301:
1032:
949:
1548:
2828:
2807:
2309:
2169:
2152:
1823:
1725:
1159:
856:
163:
709:
659:
2795:
2704:
2665:
2617:
2602:
2516:
2456:
2379:
2289:
2259:
2249:
2193:
2115:
1806:
1442:
1241:
1189:
1056:
1022:
1010:
967:
939:
852:
686:
2655:
2140:
2080:
2053:
2033:
1833:
1617:
1605:
1432:
1412:
1366:
1348:
1316:
1048:
640:
520:
spectral standard stars; however, not all of these still exactly conform to this designation.
211:
928:"Comprehensive analytic formulae for stellar evolution as a function of mass and metallicity"
2771:
2483:
2436:
2386:
2374:
2352:
2347:
2274:
2234:
2181:
1963:
1886:
1861:
1755:
1676:
1400:
1361:
1040:
957:
697:
599:
544:
282:
220:
215:
83:
779:
755:
2670:
2473:
2342:
2186:
2157:
2098:
2093:
1968:
1696:
1661:
1595:
1541:
1536:
1481:
1291:
1141:
1122:
1103:
809:
762:
739:
732:
716:
693:
666:
619:
187:
17:
1036:
953:
823:
2732:
2498:
2337:
2164:
2135:
2110:
2043:
1732:
1600:
1486:
1388:
1278:
1268:
1011:"Intrinsic Colors, Temperatures, and Bolometric Corrections of Pre-main-sequence Stars"
827:
263:
134:
94:
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2478:
2441:
2409:
2284:
1993:
1816:
1787:
1765:
1383:
1356:
1333:
1234:
1115:
1060:
962:
927:
883:
670:
528:
241:
55:
1134:
1096:
1044:
971:
531:
dwarf stars, i.e. those standard stars that have remained unchanged over years, are
198:
branch and ultimately expanding into many times its previous size at the tip of the
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2419:
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2264:
2147:
2130:
2088:
2048:
1983:
1866:
1811:
1792:
1772:
1750:
1742:
1585:
1578:
1417:
1338:
1321:
802:
629:
583:
267:
248:
203:
175:
106:
2660:
2359:
2332:
2324:
2314:
2294:
2269:
2198:
2120:
1876:
1851:
1846:
1760:
1720:
1681:
1646:
1629:
1624:
1296:
587:
552:
540:
302:
224:
183:
2244:
1941:
1914:
1891:
1871:
1856:
1708:
1612:
1590:
1568:
1563:
1427:
634:
556:
517:
278:
252:
167:
79:
63:
1052:
516:
The revised Yerkes Atlas system (Johnson & Morgan 1953) listed 11 G-type
2431:
2279:
2063:
2028:
2023:
2018:
1978:
1931:
1921:
1715:
1691:
1666:
1573:
1524:
1457:
1447:
1422:
1395:
1371:
1306:
595:
591:
227:, which cools slowly from its high initial temperature as the nebula fades.
199:
179:
171:
142:
82:). Like other main-sequence stars, a G-type main-sequence star converts the
170:
or bigger, stars similar to the Sun still outshine 90% of the stars in the
1216:
1144:, P.C. Keenan & R.C McNeil, "Astrophysical Journal Supplement Series"
559:(G6V). There are not yet any generally agreed upon G7V and G9V standards.
2424:
2125:
1799:
1558:
1531:
944:
607:
548:
195:
138:
86:
2699:
2174:
1936:
1703:
1656:
1639:
1634:
1553:
603:
75:
1076:"A Modern Mean Dwarf Stellar Color and Effective Temperature Sequence"
30:
2689:
2677:
1896:
1782:
1106:
H.L. Johnson & W.W. Morgan, 1953, Astrophysical
Journal, 117, 313
766:
743:
720:
207:
126:
122:
98:
90:
71:
2778:
2739:
547:(G8V). Other primary MK standard stars include HD 115043 (G1V) and
1027:
159:
133:, other well-known examples of G-type main-sequence stars include
29:
586:, some of the nearest G-type stars known to have planets include
2058:
2038:
1257:
1230:
2404:
1078:. University of Rochester, Department of Physics and Astronomy
881:
Dissanaike, George (19 October 1991). "Painting the sky red".
536:
130:
110:
102:
35:
1135:
The
Perkins Catalog of Revised MK Types for the Cooler Stars
986:"Evolution from the Main Sequence to Red Giants | Astronomy"
46:(spectral type: G-V), also often, and imprecisely, called a
812:, Mitchell N. Charity's webpage, accessed November 25, 2007
1226:
926:
Hurley, J. R.; Pols, O. R.; Tout, C. A. (1 July 2000).
1009:
Pecaut, Mark J.; Mamajek, Eric E. (1 September 2013).
2755:
2648:
2497:
2395:
2323:
2222:
2079:
1954:
1832:
1741:
1468:
1347:
1277:
113:of hydrogen into helium in a process known as the
38:, a typical example of a G-type main-sequence star
932:Monthly Notices of the Royal Astronomical Society
746:query result. Accessed on line December 4, 2007.
236:Properties of typical G-type main-sequence stars
723:query result. Accessed on line December 4, 2007.
1242:
186:which are much more common, the latter being
8:
1015:The Astrophysical Journal Supplement Series
1474:
1249:
1235:
1227:
234:
1026:
961:
943:
769:query result. Accessed December 4, 2007.
2762:
652:
7:
569:Habitability of yellow dwarf systems
62:G. Such a star has about 0.9 to 1.1
70:between about 5,300 and 6,000
1170:from the original on 7 August 2011
1148:(October 1989), pp. 245–266.
25:
677:, accessed on line June 19, 2007.
162:'s atmosphere due to atmospheric
2801:
2789:
2777:
2765:
2738:
2728:
2727:
1215:
963:10.1046/j.1365-8711.2000.03426.x
903:"More G Stars | StarDate Online"
210:, and the star passes on to the
105:, the star in the center of the
863:from the original on 2017-10-30
834:from the original on 2012-03-20
174:(which are largely much dimmer
1158:Mullen, Leslie (18 May 2001).
1074:Mamajek, Eric (2 March 2021).
1:
2640:Timeline of stellar astronomy
1194:hyperphysics.phy-astr.gsu.edu
117:(4 hydrogens form 1 helium),
101:when hydrogen runs out. The
2300:HertzsprungâRussell diagram
625:HertzsprungâRussell diagram
523:The "anchor points" of the
2845:
2824:G-type main-sequence stars
2214:KelvinâHelmholtz mechanism
1160:"Galactic Habitable Zones"
566:
525:MK spectral classification
2723:
1477:
1264:
1045:10.1088/0067-0049/208/1/9
990:courses.lumenlearning.com
803:What Color Are the Stars?
700:, accessed June 19, 2007.
660:"Why Does The Sun Shine?"
44:G-type main-sequence star
18:G-type main sequence star
2593:With multiple exoplanets
853:"What Color is the Sun?"
824:"WHAT COLOR IS THE SUN?"
582:Besides the Sun and its
527:system among the G-type
121:about 4 million tons of
93:in its core by means of
78:; 9,100 and 10,000
58:(luminosity class V) of
1379:Asymptotic giant branch
231:Spectral standard stars
2715:Tidal disruption event
2204:Circumstellar envelope
1438:Luminous blue variable
74:(5,000 and 5,700
39:
27:Stellar classification
2240:Effective temperature
1224:at Wikimedia Commons
1164:Astrobiology Magazine
675:Ohio State University
68:effective temperature
33:
2710:Planet-hosting stars
2588:With resolved images
2559:Historical brightest
2489:Photometric-standard
2415:Solar radio emission
2209:Eddington luminosity
1989:Triple-alpha process
1927:ThorneâĆ»ytkow object
1302:Young stellar object
1125:, Robert F. Garrison
97:, but can also fuse
2534:Highest temperature
2305:Colorâcolor diagram
2170:Protoplanetary disk
1974:Protonâproton chain
1652:Chemically peculiar
1190:"Stellar Lifetimes"
1037:2013ApJS..208....9P
954:2000MNRAS.315..543H
857:Stanford University
237:
164:Rayleigh scattering
115:protonâproton chain
2539:Lowest temperature
2290:Photometric system
2260:Absolute magnitude
2194:Circumstellar dust
1807:Stellar black hole
1443:Stellar population
1329:HerbigâHaro object
1140:2017-10-11 at the
1121:2019-06-25 at the
1102:2019-04-02 at the
808:2017-08-06 at the
761:2019-04-28 at the
738:2019-04-28 at the
715:2019-04-28 at the
710:"Alpha Centauri A"
692:2007-06-16 at the
665:2006-09-09 at the
235:
214:, and then to the
56:main-sequence star
40:
2753:
2752:
2656:Substellar object
2635:Planetary nebulae
2054:Luminous red nova
1964:Deuterium burning
1950:
1949:
1433:Instability strip
1413:Wolf-Rayet nebula
1367:Horizontal branch
1312:Pre-main-sequence
1220:Media related to
784:www.whillyard.com
673:, Astronomy 162,
641:Yellow hypergiant
637:, survey of stars
514:
513:
212:horizontal branch
16:(Redirected from
2836:
2806:
2805:
2804:
2794:
2793:
2792:
2782:
2781:
2770:
2769:
2768:
2761:
2745:Stars portal
2743:
2742:
2731:
2730:
2387:Planetary system
2310:Strömgren sphere
2182:Asteroseismology
1903:Black hole star
1475:
1401:Planetary nebula
1362:Red-giant branch
1251:
1244:
1237:
1228:
1219:
1204:
1203:
1201:
1200:
1186:
1180:
1179:
1177:
1175:
1155:
1149:
1132:
1126:
1116:MK ANCHOR POINTS
1113:
1107:
1094:
1088:
1087:
1085:
1083:
1071:
1065:
1064:
1030:
1006:
1000:
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996:
982:
976:
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945:astro-ph/0001295
923:
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893:
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753:
747:
730:
724:
707:
701:
684:
678:
657:
545:61 Ursae Majoris
310:
238:
221:planetary nebula
216:asymptotic giant
188:stellar remnants
21:
2844:
2843:
2839:
2838:
2837:
2835:
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2833:
2814:
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2812:
2802:
2800:
2790:
2788:
2776:
2766:
2764:
2756:
2754:
2749:
2737:
2719:
2644:
2613:Milky Way novae
2549:Smallest volume
2493:
2474:Radial velocity
2397:
2391:
2343:Common envelope
2319:
2218:
2187:Helioseismology
2158:Bipolar outflow
2099:Microturbulence
2094:Convection zone
2075:
1969:Lithium burning
1956:Nucleosynthesis
1946:
1828:
1737:
1464:
1343:
1292:Molecular cloud
1273:
1260:
1255:
1213:
1208:
1207:
1198:
1196:
1188:
1187:
1183:
1173:
1171:
1157:
1156:
1152:
1142:Wayback Machine
1133:
1129:
1123:Wayback Machine
1114:
1110:
1104:Wayback Machine
1095:
1091:
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1079:
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810:Wayback Machine
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763:Wayback Machine
754:
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740:Wayback Machine
731:
727:
717:Wayback Machine
708:
704:
694:Wayback Machine
685:
681:
667:Wayback Machine
658:
654:
649:
620:G-dwarf problem
616:
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2544:Largest volume
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2255:Magnetic field
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2165:Accretion disk
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2145:
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2143:
2141:Alfvén surface
2138:
2136:Stellar corona
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2111:Radiation zone
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1491:Main sequence
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1470:Classification
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1406:Protoplanetary
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1211:External links
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1089:
1066:
1001:
977:
938:(3): 543â569.
918:
894:
891:(1791): 31â33.
873:
844:
828:Universe Today
822:Cain, Frazer.
814:
795:
780:"Type G Stars"
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567:Main article:
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276:
271:
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256:
253:
246:
232:
229:
150:
147:
135:Alpha Centauri
129:. Besides the
95:nuclear fusion
26:
24:
14:
13:
10:
9:
6:
4:
3:
2:
2841:
2830:
2827:
2825:
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2713:
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2708:
2706:
2705:Intergalactic
2703:
2701:
2698:
2696:
2693:
2691:
2688:
2686:
2685:Galactic year
2683:
2679:
2676:
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2591:
2589:
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2579:
2575:
2572:
2571:
2570:
2567:
2565:
2564:Most luminous
2562:
2560:
2557:
2555:
2552:
2550:
2547:
2545:
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2537:
2535:
2532:
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2518:
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2513:
2510:
2509:
2508:
2505:
2504:
2502:
2500:
2496:
2490:
2487:
2485:
2482:
2480:
2479:Proper motion
2477:
2475:
2472:
2468:
2465:
2463:
2460:
2458:
2455:
2454:
2453:
2450:
2448:
2445:
2443:
2442:Constellation
2440:
2438:
2435:
2433:
2430:
2426:
2423:
2421:
2418:
2416:
2413:
2411:
2410:Solar eclipse
2408:
2407:
2406:
2403:
2402:
2400:
2396:Earth-centric
2394:
2388:
2385:
2381:
2378:
2376:
2373:
2371:
2368:
2367:
2366:
2363:
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2322:
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2301:
2298:
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2281:
2278:
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2273:
2271:
2268:
2266:
2263:
2261:
2258:
2256:
2253:
2251:
2248:
2246:
2243:
2241:
2238:
2236:
2233:
2231:
2228:
2227:
2225:
2221:
2215:
2212:
2210:
2207:
2205:
2202:
2200:
2197:
2195:
2192:
2188:
2185:
2184:
2183:
2180:
2176:
2173:
2171:
2168:
2167:
2166:
2163:
2159:
2156:
2154:
2151:
2150:
2149:
2146:
2142:
2139:
2137:
2134:
2132:
2129:
2127:
2124:
2122:
2119:
2118:
2117:
2114:
2112:
2109:
2105:
2102:
2100:
2097:
2096:
2095:
2092:
2090:
2087:
2086:
2084:
2082:
2078:
2072:
2069:
2065:
2062:
2060:
2057:
2055:
2052:
2050:
2047:
2045:
2042:
2041:
2040:
2037:
2035:
2032:
2030:
2027:
2025:
2022:
2020:
2017:
2015:
2012:
2010:
2007:
2005:
2002:
2000:
1997:
1995:
1994:Alpha process
1992:
1990:
1987:
1985:
1982:
1980:
1977:
1975:
1972:
1970:
1967:
1965:
1962:
1961:
1959:
1957:
1953:
1943:
1940:
1938:
1935:
1933:
1930:
1928:
1925:
1923:
1920:
1916:
1913:
1910:
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1905:
1904:
1902:
1898:
1895:
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1865:
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1808:
1805:
1801:
1798:
1794:
1791:
1789:
1786:
1785:
1784:
1781:
1779:
1776:
1775:
1774:
1771:
1767:
1766:Helium planet
1764:
1763:
1762:
1759:
1757:
1756:Parker's star
1754:
1752:
1749:
1748:
1746:
1744:
1740:
1734:
1731:
1727:
1724:
1723:
1722:
1719:
1717:
1714:
1710:
1707:
1706:
1705:
1702:
1698:
1695:
1693:
1690:
1688:
1687:Lambda Boötis
1685:
1683:
1680:
1678:
1675:
1673:
1670:
1668:
1665:
1663:
1660:
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1501:
1498:
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1492:
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1488:
1485:
1483:
1480:
1479:
1476:
1473:
1471:
1467:
1459:
1456:
1454:
1453:Superluminous
1451:
1450:
1449:
1446:
1444:
1441:
1439:
1436:
1434:
1431:
1429:
1426:
1424:
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1414:
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1407:
1404:
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1402:
1399:
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1387:
1385:
1382:
1381:
1380:
1377:
1373:
1370:
1369:
1368:
1365:
1363:
1360:
1358:
1357:Main sequence
1355:
1354:
1352:
1350:
1346:
1340:
1337:
1335:
1334:Hayashi track
1332:
1330:
1327:
1323:
1320:
1318:
1315:
1313:
1310:
1308:
1305:
1304:
1303:
1300:
1298:
1295:
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1276:
1270:
1267:
1266:
1263:
1259:
1252:
1247:
1245:
1240:
1238:
1233:
1232:
1229:
1225:
1223:
1222:Yellow dwarfs
1218:
1210:
1195:
1191:
1185:
1182:
1169:
1165:
1161:
1154:
1151:
1147:
1143:
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1136:
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1128:
1124:
1120:
1117:
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1109:
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1038:
1034:
1029:
1024:
1020:
1016:
1012:
1005:
1002:
991:
987:
981:
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973:
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964:
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951:
946:
941:
937:
933:
929:
922:
919:
908:
904:
898:
895:
890:
886:
885:
884:New Scientist
877:
874:
862:
858:
854:
848:
845:
833:
829:
825:
818:
815:
811:
807:
804:
799:
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781:
775:
772:
768:
764:
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749:
745:
741:
737:
734:
729:
726:
722:
718:
714:
711:
706:
703:
699:
695:
691:
688:
683:
680:
676:
672:
671:Barbara Ryden
668:
664:
661:
656:
653:
646:
642:
639:
636:
633:
631:
628:
626:
623:
621:
618:
617:
613:
611:
609:
605:
601:
597:
593:
589:
585:
577:
575:
570:
562:
560:
558:
554:
550:
546:
542:
538:
534:
530:
529:main-sequence
526:
521:
519:
509:
506:
503:
500:
497:
494:
493:
489:
486:
483:
480:
477:
474:
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463:
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454:
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446:
443:
440:
437:
434:
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429:
426:
423:
420:
417:
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409:
406:
403:
400:
397:
394:
393:
389:
386:
383:
380:
377:
374:
373:
369:
366:
363:
360:
357:
354:
353:
349:
346:
343:
340:
337:
334:
333:
329:
326:
323:
320:
317:
314:
313:
306:
301:
297:
292:
289:
280:
277:
274:
265:
262:
259:
250:
247:
245:
240:
239:
230:
228:
226:
222:
217:
213:
209:
205:
201:
197:
191:
189:
185:
181:
177:
176:orange dwarfs
173:
169:
165:
161:
156:
148:
146:
144:
140:
136:
132:
128:
124:
120:
116:
112:
108:
104:
100:
96:
92:
88:
85:
81:
77:
73:
69:
65:
61:
60:spectral type
57:
53:
49:
45:
37:
32:
19:
2808:Solar System
2608:White dwarfs
2598:Brown dwarfs
2581:Most distant
2529:Most massive
2507:Proper names
2467:Photographic
2420:Solar System
2398:observations
2325:Star systems
2148:Stellar wind
2131:Chromosphere
2104:Oscillations
1984:Helium flash
1834:Hypothetical
1812:X-ray binary
1751:Compact star
1586:Bright giant
1514:
1339:Henyey track
1317:Herbig Ae/Be
1214:
1197:. Retrieved
1193:
1184:
1172:. Retrieved
1163:
1153:
1145:
1130:
1111:
1092:
1080:. Retrieved
1069:
1018:
1014:
1004:
993:. Retrieved
989:
980:
935:
931:
921:
910:. Retrieved
907:stardate.org
906:
897:
888:
882:
876:
865:. Retrieved
847:
836:. Retrieved
817:
798:
787:. Retrieved
783:
774:
751:
728:
705:
682:
655:
630:Solar analog
581:
572:
563:Habitability
522:
515:
204:helium flash
192:
184:white dwarfs
155:yellow dwarf
154:
152:
107:Solar System
64:solar masses
51:
48:yellow dwarf
47:
43:
41:
2796:Outer space
2661:Brown dwarf
2437:Circumpolar
2315:Kraft break
2295:Color index
2270:Metallicity
2230:Designation
2199:Cosmic dust
2121:Photosphere
1887:Dark-energy
1862:Electroweak
1847:Black dwarf
1778:Radio-quiet
1761:White dwarf
1647:White dwarf
1297:Bok globule
756:"51 Pegasi"
696:, entry at
669:, lecture,
588:61 Virginis
553:70 Virginis
541:Kappa1 Ceti
535:(G0V), the
296:temperature
225:white dwarf
168:giant stars
149:Description
2829:Star types
2818:Categories
2623:Candidates
2618:Supernovae
2603:Red dwarfs
2462:Extinction
2250:Kinematics
2245:Luminosity
2223:Properties
2116:Atmosphere
2014:Si burning
2004:Ne burning
1942:White hole
1915:Quasi-star
1842:Blue dwarf
1697:Technetium
1613:Hypergiant
1591:Supergiant
1199:2024-07-20
995:2022-04-22
912:2022-04-22
867:2017-11-06
838:2017-11-06
789:2022-04-22
733:"Tau Ceti"
647:References
635:Star count
557:82 Eridani
555:(G4V) and
279:Luminosity
180:red dwarfs
119:converting
2772:Astronomy
2554:Brightest
2452:Magnitude
2432:Pole star
2353:Symbiotic
2348:Eclipsing
2280:Starlight
2081:Structure
2071:Supernova
2064:Micronova
2059:Recurrent
2044:Symbiotic
2029:p-process
2024:r-process
2019:s-process
2009:O burning
1999:C burning
1979:CNO cycle
1922:Gravastar
1458:Hypernova
1448:Supernova
1423:Dredge-up
1396:Blue loop
1389:super-AGB
1372:Red clump
1349:Evolution
1307:Protostar
1287:Accretion
1279:Formation
1061:119308564
1053:0067-0049
1028:1307.2657
604:Cervantes
596:HD 147513
592:HD 102365
294:Effective
200:red giant
172:Milky Way
153:The term
143:51 Pegasi
2733:Category
2628:Remnants
2524:Extremes
2484:Parallax
2457:Apparent
2447:Asterism
2425:Sunlight
2375:Globular
2360:Multiple
2285:Variable
2275:Rotation
2235:Dynamics
2126:Starspot
1800:Magnetar
1743:Remnants
1559:Subgiant
1532:Subdwarf
1384:post-AGB
1168:Archived
1138:Archived
1119:Archived
1100:Archived
1021:(1): 9.
972:18523597
861:Archived
832:Archived
806:Archived
759:Archived
736:Archived
713:Archived
690:Archived
663:Archived
614:See also
608:Tau Ceti
600:Chalawan
549:16 Cygni
287:☉
272:☉
257:☉
242:Spectral
196:subgiant
139:Tau Ceti
87:hydrogen
2758:Portals
2700:Gravity
2649:Related
2569:Nearest
2517:Chinese
2365:Cluster
2338:Contact
2175:Proplyd
2049:Remnant
1937:Blitzar
1911:Hawking
1867:Strange
1817:Burster
1773:Neutron
1726:Extreme
1677:He-weak
1322:T Tauri
1033:Bibcode
950:Bibcode
584:planets
578:Planets
543:(G5V),
539:(G2V),
309:(B â V)
206:fusing
84:element
66:and an
54:, is a
2690:Galaxy
2678:Planet
2666:Desert
2574:bright
2512:Arabic
2333:Binary
2153:Bubble
1877:Planck
1852:Exotic
1788:Binary
1783:Pulsar
1721:Helium
1682:Barium
1625:Carbon
1618:Yellow
1606:Yellow
1579:Yellow
1418:PG1159
1174:1 June
1082:5 July
1059:
1051:
970:
767:SIMBAD
744:SIMBAD
721:SIMBAD
698:ARICNS
264:Radius
208:helium
182:, and
141:, and
127:energy
123:matter
99:helium
91:helium
52:G star
2784:Stars
2695:Guest
2499:Lists
2380:Super
2034:Fusor
1907:Black
1892:Quark
1872:Preon
1857:Boson
1793:X-ray
1709:Shell
1662:Ap/Bp
1564:Giant
1482:Early
1428:OH/IR
1258:Stars
1057:S2CID
1023:arXiv
968:S2CID
940:arXiv
687:"Sun"
533:Chara
518:dwarf
510:0.78
507:5,380
501:0.853
490:0.73
487:5,480
481:0.914
470:0.71
467:5,550
461:0.927
450:0.70
447:5,600
441:0.949
430:0.68
427:5,660
421:0.977
410:0.67
407:5,680
401:0.991
398:0.985
390:0.66
387:5,720
381:1.002
370:0.65
367:5,770
361:1.012
350:0.62
347:5,860
341:1.060
330:0.60
327:5,930
321:1.100
305:index
303:Color
160:Earth
50:, or
2370:Open
2265:Mass
2089:Core
2039:Nova
1932:Iron
1882:Dark
1692:Lead
1672:HgMn
1667:CEMP
1596:Blue
1569:Blue
1487:Late
1269:List
1176:2020
1084:2021
1049:ISSN
606:and
504:0.55
498:0.90
484:0.68
478:0.94
464:0.74
458:0.95
444:0.79
438:0.97
424:0.89
418:0.98
404:0.91
384:0.98
378:0.99
364:1.02
358:1.00
344:1.20
338:1.03
324:1.35
318:1.06
299:(K)
249:Mass
244:type
111:tons
34:The
2671:Sub
2405:Sun
1824:SGR
1601:Red
1574:Red
1041:doi
1019:208
958:doi
936:315
889:132
537:Sun
495:G9V
475:G8V
455:G7V
435:G6V
415:G5V
395:G4V
375:G3V
355:G2V
335:G1V
315:G0V
190:).
131:Sun
125:to
103:Sun
89:to
36:Sun
2820::
1704:Be
1657:Am
1640:CH
1635:CN
1554:OB
1549:WR
1192:.
1166:.
1162:.
1146:71
1055:.
1047:.
1039:.
1031:.
1017:.
1013:.
988:.
966:.
956:.
948:.
934:.
930:.
905:.
887:.
859:.
855:.
830:.
826:.
782:.
765:,
742:,
719:,
610:.
602:,
598:,
594:,
590:,
290:)
275:)
260:)
178:,
145:.
137:,
80:°F
76:°C
42:A
2760::
1897:Q
1716:B
1630:S
1542:B
1537:O
1525:M
1520:K
1515:G
1510:F
1505:A
1500:B
1495:O
1250:e
1243:t
1236:v
1202:.
1178:.
1086:.
1063:.
1043::
1035::
1025::
998:.
974:.
960::
952::
942::
915:.
870:.
841:.
792:.
284:L
281:(
269:R
266:(
254:M
251:(
72:K
20:)
Text is available under the Creative Commons Attribution-ShareAlike License. Additional terms may apply.
