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Effective temperature

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67: 1151: 3116: 3127: 1116: 201:. Various colour-effective temperature relations exist in the literature. Their relations also have smaller dependencies on other stellar parameters, such as the stellar metallicity and surface gravity. The effective temperature of a star indicates the amount of heat that the star radiates per unit of surface area. From the hottest surfaces to the coolest is the sequence of 1382:
PrÅ”a, Andrej; Harmanec, Petr; Torres, Guillermo; Mamajek, Eric; Asplund, Martin; Capitaine, Nicole; Christensen-Dalsgaard, JĆørgen; Depagne, Ɖric; Haberreiter, Margit; Hekker, Saskia; Hilton, James; Kopp, Greg; Kostov, Veselin; Kurtz, Donald W.; Laskar, Jacques; Mason, Brian D.; Milone, Eugene F.;
985: 186:. Stars have a decreasing temperature gradient, going from their central core up to the atmosphere. The "core temperature" of the Sunā€”the temperature at the centre of the Sun where nuclear reactions take placeā€”is estimated to be 15,000,000 K. 1087:
and clouds) absorbing thermal radiation and reducing emissions to space, i.e., reducing the planet's emissivity of thermal radiation from its surface into space. Substituting the surface temperature into the equation and solving for Īµ gives an
750: 857: 546: 224:, either of which generates far greater energy but passes it through a surface so large that the star radiates little per unit of surface area. A star near the middle of the spectrum, such as the modest 384: 152:. The definition of the stellar radius is obviously not straightforward. More rigorously the effective temperature corresponds to the temperature at the radius that is defined by a certain value of the 465: 868: 2967: 1155: 1074:
at its mean orbital radius of 1.5Ɨ10 km. The calculation with Īµ=1 and remaining physical constants then gives an Earth effective temperature of 254 K (āˆ’19 Ā°C).
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Assuming the star radiates isotropically and that the planet is a long way from the star, the power absorbed by the planet is given by treating the planet as a disc of radius
54:), the actual temperature of the body will be higher than the effective temperature. The net emissivity may be low due to surface or atmospheric properties, such as the 569: 602:(Osiris) is 1,130 K, but the effective temperature is 1,359 K. The internal heating within Jupiter raises the effective temperature to about 152 K. 292:(the distance of the planet from the star). The calculation assumes the planet reflects some of the incoming radiation by incorporating a parameter called the 610:
The surface temperature of a planet can be estimated by modifying the effective-temperature calculation to account for emissivity and temperature variation.
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Also note here that this equation does not take into account any effects from internal heating of the planet, which can arise directly from sources such as
232:
radiates more energy per unit of surface area than the feeble red dwarf stars or the bloated supergiants, but much less than such a white or blue star as
296:(a). An albedo of 1 means that all the radiation is reflected, an albedo of 0 means all of it is absorbed. The expression for absorbed power is then: 651:. An albedo of 1 means that all the radiation is reflected, an albedo of 0 means all of it is absorbed. The expression for absorbed power is then: 1077:
The actual temperature of Earth's surface is an average 288 K (15 Ā°C) as of 2020. The difference between the two values is called the
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The next assumption we can make is that although the entire planet is not at the same temperature, it will radiate as if it had a temperature
657: 1518: 790: 1596: 582:(Bellerophon) is 1,258 K. A better estimate of effective temperature for some planets, such as Jupiter, would need to include the 1604: 1057: 160:. The effective temperature and the bolometric luminosity are the two fundamental physical parameters needed to place a star on the 476: 302: 1540: 2999: 1214: 1190: 263:, it can be calculated by equating the power received by the planet to the known power emitted by a blackbody of temperature 639:
is the radius of the planet. This area intercepts some of the power which is spread over the surface of a sphere of radius
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of a star indicates its temperature from the very coolā€”by stellar standardsā€”red M stars that radiate heavily in the
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of about 0.61 for a 288 K Earth. Furthermore, these values calculate an outgoing thermal radiation flux of
980:{\displaystyle T={\sqrt{{\frac {A_{\rm {abs}}}{A_{\rm {rad}}}}{\frac {L(1-a)}{4\pi \sigma \varepsilon D^{2}}}}}} 3177: 3152: 2979: 2616: 2600: 1635: 1030:, the point on the planet directly below the sun and gives the maximum temperature of the planet ā€” a factor of 1089: 3026: 2893: 3009: 2960: 2935: 2228: 1575: 571:
is the Stefanā€“Boltzmann constant. Note that the planet's radius has cancelled out of the final expression.
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ranges from 1 to 0 with 1 meaning the planet is a perfect blackbody and emits all the incident power. The
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for a slowly rotating body, or a tidally locked body on the sunlit side. This ratio would be 1 for the
1452:"The GALAH survey: effective temperature calibration from the InfraRed Flux Method in the Gaia system" 35:. Effective temperature is often used as an estimate of a body's surface temperature when the body's 3021: 2898: 2875: 2457: 1906: 1901: 1896: 1891: 1886: 1881: 164:. Both effective temperature and bolometric luminosity depend on the chemical composition of a star. 32: 78:) is the temperature a black body of the same size must have to yield the same total emissive power. 2164: 2038: 1673: 1383:
Montgomery, Michele; Richards, Mercedes; Schmutz, Werner; Schou, Jesper; Stewart, Susan G. (2016).
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Meteorology For Scientists and Engineers. A technical companion book with Ahrens' Meteorology Today
781: 394: 104: 643:. We also allow the planet to reflect some of the incoming radiation by incorporating a parameter 470:
Equating these two expressions and rearranging gives an expression for the effective temperature:
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Equating these two expressions and rearranging gives an expression for the surface temperature:
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Temperature of a black body that would emit the same total amount of electromagnetic radiation
2955: 2925: 2920: 2910: 2838: 1792: 1327: 1316: 1144: 554: 2073: 1352: 1296: 288:, which intercepts some of the power which is spread over the surface of a sphere of radius 3096: 2994: 2984: 2833: 2801: 2595: 2390: 2375: 1688: 1601: 1473: 1406: 1292: 1265: 8: 2556: 2539: 2210: 2112: 1935: 2696: 1578:
of the Intergovernmental Panel on Climate Change. Cambridge University Press (In Press).
1477: 1410: 1269: 3091: 3052: 3004: 2989: 2903: 2843: 2766: 2676: 2646: 2636: 2580: 2502: 2193: 1829: 1628: 1565:(2021). Masson-Delmotte, V.; Zhai, P.; Pirani, A.; Connors, S. L.; et al. (eds.). 1463: 1432: 1396: 157: 123: 1100:(with Īµā‰ˆ1 at the surface). Both fluxes are near the confidence ranges reported by the 3042: 2467: 2440: 2420: 2220: 2004: 1992: 1819: 1799: 1753: 1735: 1703: 1500:
Swihart, Thomas. "Quantitative Astronomy". Prentice Hall, 1992, Chapter 5, Section 1.
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Baschek (June 1991). "The parameters R and Teff in stellar models and observations".
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which is again some fraction of the total area of the planet. There is also a factor
389:
The next assumption we can make is that the entire planet is at the same temperature
55: 2527: 1591: 1436: 1385:"Nominal Values for Selected Solar and Planetary Quantities: IAU 2015 Resolution B3" 212:, a star of feeble energy production and a small surface or a bloated giant or even 2870: 2823: 2773: 2761: 2739: 2734: 2661: 2621: 2568: 2350: 2273: 2248: 2142: 2063: 1787: 1748: 1481: 1424: 1414: 1063: 583: 3057: 2860: 2729: 2573: 2544: 2485: 2480: 2355: 2083: 2048: 1982: 1928: 1923: 1868: 1678: 1608: 66: 3119: 2885: 2724: 2551: 2522: 2497: 2430: 2119: 1987: 1873: 1775: 1665: 1655: 1258:
Introduction to Stellar Astrophysics, Volume 3, Stellar structure and evolution
1084: 1027: 995: 229: 149: 1096:(with Īµ=0.61 as viewed from space) versus a surface thermal radiation flux of 3146: 3071: 2865: 2828: 2796: 2671: 2380: 2203: 2174: 2152: 1770: 1743: 1720: 1621: 1486: 1451: 1037:(1.414) greater than the effective temperature of a rapidly rotating planet. 1003: 3131: 2806: 2756: 2751: 2651: 2534: 2517: 2475: 2445: 2435: 2370: 2253: 2198: 2179: 2159: 2137: 2129: 1972: 1965: 1804: 1725: 1708: 1045: 3047: 2719: 2711: 2701: 2681: 2656: 2585: 2507: 2263: 2238: 2233: 2147: 2107: 2068: 2033: 2016: 2011: 1683: 1121: 599: 579: 198: 190: 24: 1150: 1132: ā€“ temperature associated with the measured intensity and frequency 50:
in the relevant wavelength band is less than unity (less than that of a
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Note the ratio of the two areas. Common assumptions for this ratio are
773: 745:{\displaystyle P_{\rm {abs}}={\frac {LA_{\rm {abs}}(1-a)}{4\pi D^{2}}}} 591: 275: 221: 213: 87: 51: 47: 40: 36: 28: 2818: 2666: 2450: 2415: 2410: 2405: 2365: 2318: 2308: 2102: 2078: 2053: 1960: 1911: 1844: 1834: 1809: 1782: 1758: 1693: 1323: 1182: 209: 2811: 2512: 2186: 1945: 1918: 1468: 1401: 852:{\displaystyle P_{\rm {rad}}=A_{\rm {rad}}\varepsilon \sigma T^{4}} 194: 1083:. The greenhouse effect results from materials in the atmosphere ( 3086: 2561: 2323: 2090: 2043: 2026: 2021: 1940: 1141: ā€“ Property of light sources related to black-body radiation 575: 217: 3076: 3064: 2283: 2169: 648: 613:
The area of the planet that absorbs the power from the star is
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Stefanā€“Boltzmann law Ā§ Effective temperature of the Earth
541:{\displaystyle T={\sqrt{\frac {L(1-a)}{16\pi \sigma D^{2}}}}} 237: 2425: 1644: 1562: 1174: 1101: 379:{\displaystyle P_{\rm {abs}}={\frac {Lr^{2}(1-a)}{4D^{2}}}} 233: 83: 3126: 1115: 784:
gives an expression for the power radiated by the planet:
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gives an expression for the power radiated by the planet:
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to the very hot blue O stars that radiate largely in the
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as a power input. The actual temperature depends on
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Pages displaying wikidata descriptions as a fallback
1111: 460:{\displaystyle P_{\rm {rad}}=4\pi r^{2}\sigma T^{4}} 1044:and also be produced from frictions resulting from 393:, and that the planet radiates as a blackbody. The 259:To find the effective (blackbody) temperature of a 1315: 979: 851: 744: 605: 563: 540: 459: 378: 622:which is some fraction of the total surface area 3144: 1592:Effective temperature scale for solar type stars 1568:Climate Change 2021: The Physical Science Basis 178:for use as a unit of measure of temperature is 167:The effective temperature of the Sun is around 1051: 103:) as the star and is defined according to the 1629: 1561: 1255: 1636: 1622: 1449: 23:of a body such as a star or planet is the 1574:. Contribution of Working Group I to the 1485: 1467: 1418: 1400: 1168: 1062:Earth has an albedo of about 0.306 and a 31:that would emit the same total amount of 1344: 1229:The Stars: Their Structure and Evolution 270:Take the case of a planet at a distance 248: 65: 1282: 578:from this calculation is 88 K and 3145: 1226: 1617: 1350: 1318:CRC Handbook of Chemistry and Physics 594:effects. The actual temperature from 1541:"Climate Change: Global Temperature" 1521:from the original on 30 October 2010 1309: 1175:Archie E. Roy, David Clarke (2003). 776:and represents atmospheric effects. 1354:Life in the Solar System and Beyond 1303: 1249: 174:. The nominal value defined by the 13: 913: 910: 907: 895: 892: 889: 827: 824: 821: 806: 803: 800: 700: 697: 694: 673: 670: 667: 419: 416: 413: 318: 315: 312: 14: 3189: 1585: 255:Planetary equilibrium temperature 70:The effective temperature of the 3125: 3115: 3114: 1312:"Properties of the Solar System" 1149: 1114: 1010:for a rapidly rotating body and 176:International Astronomical Union 46:When the star's or planet's net 1555: 1533: 1503: 1494: 606:Surface temperature of a planet 126:) luminosity of a star is then 82:The effective temperature of a 1597:Surface Temperature of Planets 1443: 1375: 1351:Jones, Barrie William (2004). 1276: 1220: 1199: 1154:Learning materials related to 939: 927: 718: 706: 574:The effective temperature for 505: 493: 355: 343: 205:known as O, B, A, F, G, K, M. 1: 3027:Timeline of stellar astronomy 1602:Planet temperature calculator 1162: 90:with the same luminosity per 1310:Lide, David R., ed. (2004). 1256:Bƶhm-Vitense, Erika (1992). 7: 2687:Hertzsprungā€“Russell diagram 1227:Tayler, Roger John (1994). 1209:, Brooks/Cole, Belmont CA, 1107: 1052:Earth effective temperature 208:A red star could be a tiny 162:Hertzsprungā€“Russell diagram 10: 3194: 2601:Kelvinā€“Helmholtz mechanism 1420:10.3847/0004-6256/152/2/41 1285:Astronomy and Astrophysics 1262:Cambridge University Press 1233:Cambridge University Press 1055: 252: 3173:Electromagnetic radiation 3110: 3035: 2884: 2782: 2710: 2609: 2466: 2341: 2219: 2128: 1864: 1855: 1734: 1664: 1651: 1643: 1450:Casagrande, Luca (2021). 243: 122:. Notice that the total ( 33:electromagnetic radiation 3168:Thermodynamic properties 2980:With multiple exoplanets 1389:The Astronomical Journal 86:is the temperature of a 39:curve (as a function of 1766:Asymptotic giant branch 1576:Sixth Assessment Report 1297:1991A&A...246..374B 564:{\displaystyle \sigma } 203:stellar classifications 156:(usually 1) within the 154:Rosseland optical depth 61: 3102:Tidal disruption event 2591:Circumstellar envelope 1825:Luminous blue variable 1487:10.1093/mnras/stab2304 1130:Brightness temperature 981: 853: 746: 596:spectroscopic analysis 565: 542: 461: 380: 79: 3178:Concepts in astronomy 3153:Astrophysics concepts 2627:Effective temperature 1156:Atmospheric retention 1145:List of hottest stars 982: 854: 747: 566: 543: 462: 381: 249:Blackbody temperature 69: 21:effective temperature 3097:Planet-hosting stars 2975:With resolved images 2946:Historical brightest 2876:Photometric-standard 2802:Solar radio emission 2596:Eddington luminosity 2376:Triple-alpha process 2314:Thorneā€“Å»ytkow object 1689:Young stellar object 1090:effective emissivity 869: 791: 782:Stefanā€“Boltzmann law 658: 555: 477: 404: 395:Stefanā€“Boltzmann law 303: 105:Stefanā€“Boltzmann law 2921:Highest temperature 2692:Colorā€“color diagram 2557:Protoplanetary disk 2361:Protonā€“proton chain 2039:Chemically peculiar 1515:nssdc.gsfc.nasa.gov 1478:2021MNRAS.507.2684C 1411:2016AJ....152...41P 1270:1992isa..book.....B 2926:Lowest temperature 2677:Photometric system 2647:Absolute magnitude 2581:Circumstellar dust 2194:Stellar black hole 1830:Stellar population 1716:Herbigā€“Haro object 1607:2012-11-27 at the 1511:"Earth Fact Sheet" 1205:Stull, R. (2000). 977: 849: 742: 561: 538: 457: 376: 274:from the star, of 158:stellar atmosphere 80: 3163:Planetary science 3158:Stellar astronomy 3140: 3139: 3043:Substellar object 3022:Planetary nebulae 2441:Luminous red nova 2351:Deuterium burning 2337: 2336: 1820:Instability strip 1800:Wolf-Rayet nebula 1754:Horizontal branch 1699:Pre-main-sequence 1322:(85th ed.). 1215:978-0-534-37214-9 1192:978-0-7503-0917-2 1139:Color temperature 1080:greenhouse effect 1042:radioactive decay 975: 967: 919: 740: 536: 530: 374: 56:greenhouse effect 3185: 3132:Stars portal 3130: 3129: 3118: 3117: 2774:Planetary system 2697:Strƶmgren sphere 2569:Asteroseismology 2290:Black hole star 1862: 1861: 1788:Planetary nebula 1749:Red-giant branch 1638: 1631: 1624: 1615: 1614: 1580: 1579: 1573: 1559: 1553: 1552: 1550: 1548: 1537: 1531: 1530: 1528: 1526: 1507: 1501: 1498: 1492: 1491: 1489: 1471: 1462:(2): 2684ā€“2696. 1447: 1441: 1440: 1422: 1404: 1379: 1373: 1372: 1348: 1342: 1341: 1321: 1307: 1301: 1300: 1280: 1274: 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2051: 2046: 2036: 2031: 2030: 2029: 2024: 2019: 2009: 2008: 2007: 1997: 1996: 1995: 1990: 1985: 1975: 1970: 1969: 1968: 1963: 1958: 1948: 1943: 1938: 1933: 1932: 1931: 1926: 1916: 1915: 1914: 1909: 1904: 1899: 1894: 1889: 1884: 1878:Main sequence 1876: 1871: 1865: 1859: 1857:Classification 1853: 1852: 1850: 1849: 1848: 1847: 1842: 1832: 1827: 1822: 1817: 1812: 1807: 1802: 1797: 1796: 1795: 1793:Protoplanetary 1785: 1780: 1779: 1778: 1773: 1763: 1762: 1761: 1751: 1746: 1740: 1738: 1732: 1731: 1729: 1728: 1723: 1718: 1713: 1712: 1711: 1706: 1701: 1696: 1686: 1681: 1676: 1670: 1668: 1662: 1661: 1659: 1658: 1652: 1649: 1648: 1641: 1640: 1633: 1626: 1618: 1612: 1611: 1599: 1594: 1587: 1586:External links 1584: 1582: 1581: 1554: 1532: 1502: 1493: 1442: 1374: 1367: 1343: 1336: 1302: 1291:(2): 374ā€“382. 1275: 1264:. p. 14. 1248: 1241: 1235:. p. 16. 1219: 1198: 1191: 1166: 1164: 1161: 1160: 1159: 1158:at Wikiversity 1147: 1142: 1136: 1126: 1125: 1109: 1106: 1053: 1050: 1028:subsolar point 988: 987: 973: 963: 959: 955: 952: 949: 946: 941: 938: 935: 932: 929: 926: 915: 912: 909: 904: 897: 894: 891: 886: 877: 874: 860: 859: 846: 842: 838: 835: 829: 826: 823: 818: 814: 808: 805: 802: 797: 764: 753: 752: 736: 732: 728: 725: 720: 717: 714: 711: 708: 702: 699: 696: 691: 687: 681: 675: 672: 669: 664: 627: 618: 607: 604: 560: 549: 548: 534: 526: 522: 518: 515: 512: 507: 504: 501: 498: 495: 492: 485: 482: 468: 467: 454: 450: 446: 441: 437: 433: 430: 427: 421: 418: 415: 410: 387: 386: 370: 366: 362: 357: 354: 351: 348: 345: 340: 336: 332: 326: 320: 317: 314: 309: 253:Main article: 250: 247: 245: 242: 150:stellar radius 138: 118: 111: 99: 63: 60: 15: 9: 6: 4: 3: 2: 3190: 3179: 3176: 3174: 3171: 3169: 3166: 3164: 3161: 3159: 3156: 3154: 3151: 3150: 3148: 3133: 3128: 3123: 3121: 3113: 3112: 3109: 3103: 3100: 3098: 3095: 3093: 3092:Intergalactic 3090: 3088: 3085: 3083: 3080: 3078: 3075: 3073: 3072:Galactic year 3070: 3066: 3063: 3059: 3056: 3054: 3051: 3050: 3049: 3046: 3045: 3044: 3041: 3040: 3038: 3034: 3028: 3025: 3023: 3020: 3016: 3013: 3011: 3008: 3007: 3006: 3003: 3001: 2998: 2996: 2993: 2991: 2988: 2986: 2983: 2981: 2978: 2976: 2973: 2969: 2966: 2962: 2959: 2958: 2957: 2954: 2952: 2951:Most luminous 2949: 2947: 2944: 2942: 2939: 2937: 2934: 2932: 2929: 2927: 2924: 2922: 2919: 2917: 2914: 2913: 2912: 2909: 2905: 2902: 2900: 2897: 2896: 2895: 2892: 2891: 2889: 2887: 2883: 2877: 2874: 2872: 2869: 2867: 2866:Proper motion 2864: 2862: 2859: 2855: 2852: 2850: 2847: 2845: 2842: 2841: 2840: 2837: 2835: 2832: 2830: 2829:Constellation 2827: 2825: 2822: 2820: 2817: 2813: 2810: 2808: 2805: 2803: 2800: 2798: 2797:Solar eclipse 2795: 2794: 2793: 2790: 2789: 2787: 2783:Earth-centric 2781: 2775: 2772: 2768: 2765: 2763: 2760: 2758: 2755: 2754: 2753: 2750: 2748: 2745: 2741: 2738: 2736: 2733: 2731: 2728: 2726: 2723: 2722: 2721: 2718: 2717: 2715: 2713: 2709: 2703: 2700: 2698: 2695: 2693: 2690: 2688: 2685: 2683: 2680: 2678: 2675: 2673: 2670: 2668: 2665: 2663: 2660: 2658: 2655: 2653: 2650: 2648: 2645: 2643: 2640: 2638: 2635: 2633: 2630: 2628: 2625: 2623: 2620: 2618: 2615: 2614: 2612: 2608: 2602: 2599: 2597: 2594: 2592: 2589: 2587: 2584: 2582: 2579: 2575: 2572: 2571: 2570: 2567: 2563: 2560: 2558: 2555: 2554: 2553: 2550: 2546: 2543: 2541: 2538: 2537: 2536: 2533: 2529: 2526: 2524: 2521: 2519: 2516: 2514: 2511: 2509: 2506: 2505: 2504: 2501: 2499: 2496: 2492: 2489: 2487: 2484: 2483: 2482: 2479: 2477: 2474: 2473: 2471: 2469: 2465: 2459: 2456: 2452: 2449: 2447: 2444: 2442: 2439: 2437: 2434: 2432: 2429: 2428: 2427: 2424: 2422: 2419: 2417: 2414: 2412: 2409: 2407: 2404: 2402: 2399: 2397: 2394: 2392: 2389: 2387: 2384: 2382: 2381:Alpha process 2379: 2377: 2374: 2372: 2369: 2367: 2364: 2362: 2359: 2357: 2354: 2352: 2349: 2348: 2346: 2344: 2340: 2330: 2327: 2325: 2322: 2320: 2317: 2315: 2312: 2310: 2307: 2303: 2300: 2297: 2295: 2292: 2291: 2289: 2285: 2282: 2280: 2277: 2275: 2272: 2270: 2267: 2265: 2262: 2260: 2257: 2255: 2252: 2250: 2247: 2245: 2242: 2241: 2240: 2237: 2235: 2232: 2230: 2227: 2226: 2224: 2222: 2218: 2212: 2209: 2205: 2202: 2201: 2200: 2197: 2195: 2192: 2188: 2185: 2181: 2178: 2176: 2173: 2172: 2171: 2168: 2166: 2163: 2162: 2161: 2158: 2154: 2153:Helium planet 2151: 2150: 2149: 2146: 2144: 2143:Parker's star 2141: 2139: 2136: 2135: 2133: 2131: 2127: 2121: 2118: 2114: 2111: 2110: 2109: 2106: 2104: 2101: 2097: 2094: 2093: 2092: 2089: 2085: 2082: 2080: 2077: 2075: 2074:Lambda Boƶtis 2072: 2070: 2067: 2065: 2062: 2060: 2057: 2055: 2052: 2050: 2047: 2045: 2042: 2041: 2040: 2037: 2035: 2032: 2028: 2025: 2023: 2020: 2018: 2015: 2014: 2013: 2010: 2006: 2003: 2002: 2001: 1998: 1994: 1991: 1989: 1986: 1984: 1981: 1980: 1979: 1976: 1974: 1971: 1967: 1964: 1962: 1959: 1957: 1954: 1953: 1952: 1949: 1947: 1944: 1942: 1939: 1937: 1934: 1930: 1927: 1925: 1922: 1921: 1920: 1917: 1913: 1910: 1908: 1905: 1903: 1900: 1898: 1895: 1893: 1890: 1888: 1885: 1883: 1880: 1879: 1877: 1875: 1872: 1870: 1867: 1866: 1863: 1860: 1858: 1854: 1846: 1843: 1841: 1840:Superluminous 1838: 1837: 1836: 1833: 1831: 1828: 1826: 1823: 1821: 1818: 1816: 1813: 1811: 1808: 1806: 1803: 1801: 1798: 1794: 1791: 1790: 1789: 1786: 1784: 1781: 1777: 1774: 1772: 1769: 1768: 1767: 1764: 1760: 1757: 1756: 1755: 1752: 1750: 1747: 1745: 1744:Main sequence 1742: 1741: 1739: 1737: 1733: 1727: 1724: 1722: 1721:Hayashi track 1719: 1717: 1714: 1710: 1707: 1705: 1702: 1700: 1697: 1695: 1692: 1691: 1690: 1687: 1685: 1682: 1680: 1677: 1675: 1672: 1671: 1669: 1667: 1663: 1657: 1654: 1653: 1650: 1646: 1639: 1634: 1632: 1627: 1625: 1620: 1619: 1616: 1610: 1606: 1603: 1600: 1598: 1595: 1593: 1590: 1589: 1577: 1570: 1569: 1564: 1558: 1542: 1536: 1520: 1516: 1512: 1506: 1497: 1488: 1483: 1479: 1475: 1470: 1465: 1461: 1457: 1453: 1446: 1438: 1434: 1430: 1426: 1421: 1416: 1412: 1408: 1403: 1398: 1394: 1390: 1386: 1378: 1370: 1368:1-85233-101-1 1364: 1361:. p. 7. 1360: 1356: 1355: 1347: 1339: 1337:9780849304859 1333: 1329: 1325: 1320: 1319: 1313: 1306: 1298: 1294: 1290: 1286: 1279: 1271: 1267: 1263: 1259: 1252: 1244: 1242:0-521-45885-4 1238: 1234: 1230: 1223: 1216: 1212: 1208: 1202: 1194: 1188: 1184: 1180: 1179: 1171: 1167: 1157: 1152: 1148: 1146: 1143: 1140: 1137: 1131: 1128: 1127: 1123: 1117: 1112: 1105: 1103: 1091: 1086: 1082: 1081: 1075: 1065: 1059: 1049: 1047: 1043: 1038: 1029: 1005: 997: 971: 961: 957: 953: 950: 947: 944: 936: 933: 930: 924: 902: 884: 875: 872: 865: 864: 863: 844: 840: 836: 833: 816: 812: 795: 787: 786: 785: 783: 775: 763: 759:over an area 734: 730: 726: 723: 715: 712: 709: 689: 685: 679: 662: 654: 653: 652: 650: 633: 626: 617: 611: 603: 601: 597: 593: 589: 585: 581: 577: 572: 558: 532: 524: 520: 516: 513: 510: 502: 499: 496: 490: 483: 480: 473: 472: 471: 452: 448: 444: 439: 435: 431: 428: 425: 408: 400: 399: 398: 396: 368: 364: 360: 352: 349: 346: 338: 334: 330: 324: 307: 299: 298: 297: 295: 282: 277: 268: 262: 256: 241: 239: 235: 231: 228:or the giant 227: 223: 219: 216:star such as 215: 211: 206: 204: 200: 196: 192: 187: 177: 172: 165: 163: 159: 155: 151: 146: 137: 134: 130: 125: 117: 106: 93: 89: 85: 77: 73: 68: 59: 57: 53: 49: 44: 42: 38: 34: 30: 26: 22: 2995:White dwarfs 2985:Brown dwarfs 2968:Most distant 2916:Most massive 2894:Proper names 2854:Photographic 2807:Solar System 2785:observations 2712:Star systems 2626: 2535:Stellar wind 2518:Chromosphere 2491:Oscillations 2371:Helium flash 2221:Hypothetical 2199:X-ray binary 2138:Compact star 1973:Bright giant 1726:Henyey track 1704:Herbig Ae/Be 1567: 1557: 1545:. Retrieved 1535: 1523:. Retrieved 1514: 1505: 1496: 1459: 1455: 1445: 1392: 1388: 1377: 1353: 1346: 1317: 1305: 1288: 1284: 1278: 1257: 1251: 1228: 1222: 1206: 1201: 1177: 1170: 1078: 1076: 1061: 1046:tidal forces 1039: 989: 861: 761: 754: 631: 624: 615: 612: 609: 573: 550: 469: 388: 283: 269: 258: 207: 188: 166: 144: 135: 132: 128: 115: 92:surface area 91: 81: 45: 20: 18: 3048:Brown dwarf 2824:Circumpolar 2702:Kraft break 2682:Color index 2657:Metallicity 2617:Designation 2586:Cosmic dust 2508:Photosphere 2274:Dark-energy 2249:Electroweak 2234:Black dwarf 2165:Radio-quiet 2148:White dwarf 2034:White dwarf 1684:Bok globule 1429:1885/108637 1122:Star portal 647:called the 600:HD 209458 b 580:51 Pegasi b 199:ultraviolet 191:color index 169:5,778  25:temperature 3147:Categories 3010:Candidates 3005:Supernovae 2990:Red dwarfs 2849:Extinction 2637:Kinematics 2632:Luminosity 2610:Properties 2503:Atmosphere 2401:Si burning 2391:Ne burning 2329:White hole 2302:Quasi-star 2229:Blue dwarf 2084:Technetium 2000:Hypergiant 1978:Supergiant 1469:2011.02517 1402:1605.09788 1326:. p.  1163:References 1056:See also: 774:emissivity 592:atmosphere 276:luminosity 222:Betelgeuse 214:supergiant 184:0.8 K 124:bolometric 88:black body 52:black body 48:emissivity 41:wavelength 37:emissivity 29:black body 2941:Brightest 2839:Magnitude 2819:Pole star 2740:Symbiotic 2735:Eclipsing 2667:Starlight 2468:Structure 2458:Supernova 2451:Micronova 2446:Recurrent 2431:Symbiotic 2416:p-process 2411:r-process 2406:s-process 2396:O burning 2386:C burning 2366:CNO cycle 2309:Gravastar 1845:Hypernova 1835:Supernova 1810:Dredge-up 1783:Blue loop 1776:super-AGB 1759:Red clump 1736:Evolution 1694:Protostar 1674:Accretion 1666:Formation 1395:(2): 41. 1324:CRC Press 1217:, p. 400. 1183:CRC Press 1178:Astronomy 1068:L / 4 Ļ€ D 954:ε 951:σ 948:π 934:− 837:σ 834:ε 727:π 713:− 559:σ 517:σ 514:π 500:− 445:σ 432:π 350:− 210:red dwarf 3120:Category 3015:Remnants 2911:Extremes 2871:Parallax 2844:Apparent 2834:Asterism 2812:Sunlight 2762:Globular 2747:Multiple 2672:Variable 2662:Rotation 2622:Dynamics 2513:Starspot 2187:Magnetar 2130:Remnants 1946:Subgiant 1919:Subdwarf 1771:post-AGB 1605:Archived 1519:Archived 1437:55319250 1359:Springer 1108:See also 1072:1361 W m 635:, where 195:infrared 142:, where 3087:Gravity 3036:Related 2956:Nearest 2904:Chinese 2752:Cluster 2725:Contact 2562:Proplyd 2436:Remnant 2324:Blitzar 2298:Hawking 2254:Strange 2204:Burster 2160:Neutron 2113:Extreme 2064:He-weak 1709:T Tauri 1474:Bibcode 1407:Bibcode 1293:Bibcode 1266:Bibcode 1098:390 W m 1094:238 W m 1032:√ 1024:⁠ 1012:⁠ 1008:⁠ 992:⁠ 576:Jupiter 230:Capella 218:Antares 148:is the 76:kelvins 3077:Galaxy 3065:Planet 3053:Desert 2961:bright 2899:Arabic 2720:Binary 2540:Bubble 2264:Planck 2239:Exotic 2175:Binary 2170:Pulsar 2108:Helium 2069:Barium 2012:Carbon 2005:Yellow 1993:Yellow 1966:Yellow 1805:PG1159 1547:6 July 1543:. NOAA 1435:  1365:  1334:  1239:  1213:  1189:  649:albedo 588:albedo 551:Where 294:albedo 261:planet 244:Planet 74:(5778 3082:Guest 2886:Lists 2767:Super 2421:Fusor 2294:Black 2279:Quark 2259:Preon 2244:Boson 2180:X-ray 2096:Shell 2049:Ap/Bp 1951:Giant 1869:Early 1815:OH/IR 1645:Stars 1572:(PDF) 1525:8 May 1464:arXiv 1456:MNRAS 1433:S2CID 1397:arXiv 1070:) of 628:total 238:Rigel 180:5,772 27:of a 2757:Open 2652:Mass 2476:Core 2426:Nova 2319:Iron 2269:Dark 2079:Lead 2059:HgMn 2054:CEMP 1983:Blue 1956:Blue 1874:Late 1656:List 1563:IPCC 1549:2023 1527:2018 1363:ISBN 1332:ISBN 1328:14-2 1237:ISBN 1211:ISBN 1187:ISBN 1102:IPCC 630:= 4Ļ€ 598:for 590:and 234:Vega 189:The 131:= 4Ļ€ 84:star 62:Star 19:The 3058:Sub 2792:Sun 2211:SGR 1988:Red 1961:Red 1482:doi 1460:507 1425:hdl 1415:doi 1393:152 1289:246 765:rad 619:abs 236:or 226:Sun 220:or 139:eff 119:eff 112:Bol 100:Bol 72:Sun 3149:: 2091:Be 2044:Am 2027:CH 2022:CN 1941:OB 1936:WR 1517:. 1513:. 1480:. 1472:. 1458:. 1454:. 1431:. 1423:. 1413:. 1405:. 1391:. 1387:. 1357:. 1330:. 1314:. 1287:. 1260:. 1231:. 1185:. 1181:. 1104:. 1048:. 511:16 281:. 267:. 240:. 136:ĻƒT 116:ĻƒT 114:= 58:. 2284:Q 2103:B 2017:S 1929:B 1924:O 1912:M 1907:K 1902:G 1897:F 1892:A 1887:B 1882:O 1637:e 1630:t 1623:v 1551:. 1529:. 1490:. 1484:: 1476:: 1466:: 1439:. 1427:: 1417:: 1409:: 1399:: 1371:. 1340:. 1299:. 1295:: 1272:. 1268:: 1245:. 1195:. 1066:( 1034:2 1021:2 1018:/ 1015:1 1004:4 1000:/ 996:1 972:4 962:2 958:D 945:4 940:) 937:a 931:1 928:( 925:L 914:d 911:a 908:r 903:A 896:s 893:b 890:a 885:A 876:= 873:T 845:4 841:T 828:d 825:a 822:r 817:A 813:= 807:d 804:a 801:r 796:P 778:Īµ 770:Īµ 762:A 757:T 735:2 731:D 724:4 719:) 716:a 710:1 707:( 701:s 698:b 695:a 690:A 686:L 680:= 674:s 671:b 668:a 663:P 645:a 641:D 637:r 632:r 625:A 616:A 533:4 525:2 521:D 506:) 503:a 497:1 494:( 491:L 484:= 481:T 453:4 449:T 440:2 436:r 429:4 426:= 420:d 417:a 414:r 409:P 391:T 369:2 365:D 361:4 356:) 353:a 347:1 344:( 339:2 335:r 331:L 325:= 319:s 316:b 313:a 308:P 290:D 286:r 279:L 272:D 265:T 182:Ā± 171:K 145:R 133:R 129:L 109:F 97:F 94:(

Index

temperature
black body
electromagnetic radiation
emissivity
wavelength
emissivity
black body
greenhouse effect

Sun
kelvins
star
black body
Stefanā€“Boltzmann law
bolometric
stellar radius
Rosseland optical depth
stellar atmosphere
Hertzsprungā€“Russell diagram
K
International Astronomical Union
color index
infrared
ultraviolet
stellar classifications
red dwarf
supergiant
Antares
Betelgeuse
Sun

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