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Gravitational binding energy

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1151: 20: 851: 72:. In newtonian gravity, the binding energy can be considered to be the linear sum of the interactions between all pairs of microscopic components of the system, while in General Relativity, this is only approximately true if the gravitational fields are all weak. When stronger fields are present within a system, the binding energy is a 605: 1488:
Neutron star relativistic equations of state include a graph of radius vs. mass for various models. The most likely radii for a given neutron star mass are bracketed by models AP4 (smallest radius) and MS2 (largest radius). BE is the ratio of gravitational binding energy mass equivalent to observed
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It can be easily demonstrated that this negative component can never exceed the positive component of a system. A negative binding energy greater than the mass of the system itself would indeed require that the radius of the system be smaller than:
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Planets and stars have radial density gradients from their lower density surfaces to their much denser compressed cores. Degenerate matter objects (white dwarfs; neutron star pulsars) have radial density gradients plus relativistic corrections.
1699: 846:{\displaystyle U=-G\int _{0}^{R}{\frac {\left(4\pi r^{2}\rho \right)\left({\tfrac {4}{3}}\pi r^{3}\rho \right)}{r}}dr=-G{\frac {16}{3}}\pi ^{2}\rho ^{2}\int _{0}^{R}{r^{4}}dr=-G{\frac {16}{15}}{\pi }^{2}{\rho }^{2}R^{5}} 598: 1775: 937: 498: 1295: 1552: 1166:, as there appears to be a serious conceptual inconsistency between the newtonian formula for binding energy and the relativistic concept of Schwarzschild radius. Perhaps the section would be best deleted.. 1831: 1960: 930: 419: 1470: 1888: 1604: 1394: 1135: 161: 80:
system, and it cannot be conceptually attributed among the elements of the system. In this case the binding energy can be considered to be the (negative) difference between the
284:, the gravitational binding energy required for hydrostatic equilibrium approaches zero and the star becomes unstable (highly sensitive to perturbations), which may lead to a 1421: 328:
is found by imagining that it is pulled apart by successively moving spherical shells to infinity, the outermost first, and finding the total energy needed for that.
873: 349: 505: 326: 424: 1614: 1207: 1500: 1897: 880: 2182: 1705: 354: 2065: 1430: 1975: 1781: 1843: 61: 54: 1556: 1346: 110: 1069:{\displaystyle U=-G{\frac {16}{15}}\pi ^{2}R^{5}\left({\frac {M}{{\frac {4}{3}}\pi R^{3}}}\right)^{2}=-{\frac {3GM^{2}}{5R}}} 1172: 242: 2157: 2100:
Katz, Joseph; Lynden-Bell, Donald; Bičák, Jiří (27 October 2006). "Gravitational energy in stationary spacetimes".
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of the system, as it is manifest in its gravitational interaction with other distant systems, and the sum of the
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from each other and reciprocally not moving, exert a gravitational force on a third body slightly smaller when
1084: 2102: 1328:), and if its atoms were sparse over an arbitrarily large volume the Earth would weigh its current mass plus 238: 49:
than the sum of the energies of its parts when these are completely separated—this is what keeps the system
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and therefore never visible to an external observer. However this is only a Newtonian approximation and in
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is simply equal to the mass of the whole divided by its volume for objects with uniform density, therefore
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of a system is the minimum energy which must be added to it in order for the system to cease being in a
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kilograms (and its gravitational pull over a third body would be accordingly stronger).
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For example, the fact that Earth is a gravitationally-bound sphere of its current size
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The required energy for a shell is the negative of the gravitational potential energy:
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The gravitational binding energy can be conceptually different within the theories of
2086: 245:(PREM). Using this, the real gravitational binding energy of Earth can be calculated 2208: 2141: 2129: 2082: 1980: 73: 1694:{\displaystyle G=6.6743\times 10^{-11}\,\mathrm {m^{3}\cdot kg^{-1}\cdot s^{-2}} } 2161: 2060: 2056: 234:, 60% of the absolute value of the potential energy per kilogram at the surface. 2174: 237:
The actual depth-dependence of density, inferred from seismic travel times (see
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is a sphere of uniform density (which it is not, but is close enough to get an
85: 23: 2202: 1317: 1201: 593:{\displaystyle dU=-G{\frac {m_{\mathrm {shell} }m_{\mathrm {interior} }}{r}}} 303: 297: 1150: 2154: 1770:{\displaystyle c^{2}=8.98755\times 10^{16}\,\mathrm {m^{2}\cdot s^{-2}} } 38: 1204:
component of the system, equal, for uniformly spherical solutions, to:
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are the largest known gravitationally bound structures in the universe.
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then the relativistic fractional binding energy of a neutron star is
285: 493:{\displaystyle m_{\mathrm {interior} }={\frac {4}{3}}\pi r^{3}\rho } 16:
Minimum energy to remove a system from a gravitationally bound state
1312: 65: 19: 1290:{\displaystyle M_{\mathrm {binding} }=-{\frac {3GM^{2}}{5Rc^{2}}}} 100: 35: 1547:{\displaystyle BE={\frac {0.60\,\beta }{1-{\frac {\beta }{2}}}}} 1826:{\displaystyle M_{\odot }=1.98844\times 10^{30}\,\mathrm {kg} } 1955:{\displaystyle BE={\frac {885.975\,M_{x}}{R-738.313\,M_{x}}}} 1476:
conditions other factors must be taken into account as well.
1325: 183: 273: 269: 89: 925:{\displaystyle \rho ={\frac {M}{{\frac {4}{3}}\pi R^{3}}}} 308:
The gravitational binding energy of a sphere with radius
227: 414:{\displaystyle m_{\mathrm {shell} }=4\pi r^{2}\rho \,dr} 304:
Derivation within newtonian gravity for a uniform sphere
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The NIST Reference on Constants, Units, and Uncertainty
2175:"2022 CODATA Value: Newtonian constant of gravitation" 1402: 674: 351:, the masses of a shell and the sphere inside it are: 1900: 1846: 1784: 1708: 1617: 1559: 1503: 1465:{\displaystyle R\leq {\frac {3}{10}}r_{\mathrm {s} }} 1433: 1349: 1210: 1087: 940: 883: 861: 608: 508: 427: 357: 337: 314: 280:
to be maintained. As the gas in a star becomes more
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And finally, plugging this into our result leads to
2055: 1954: 1882: 1825: 1769: 1693: 1598: 1546: 1464: 1415: 1388: 1289: 1129: 1068: 924: 867: 845: 592: 492: 413: 343: 320: 155: 2031:An Introduction to the Study of Stellar Structure 2017: 2200: 1883:{\displaystyle M_{x}={\frac {M}{M_{\odot }}},} 288:in the case of a high-mass star due to strong 41:. A gravitationally bound system has a lower ( 2063:(1981). "Preliminary Reference Earth Model". 107:is given in newtonian gravity by the formula 2066:Physics of the Earth and Planetary Interiors 1599:{\displaystyle \beta ={\frac {GM}{Rc^{2}}}.} 1389:{\displaystyle R\leq {\frac {3GM}{5c^{2}}}} 226:. This is roughly equal to one week of the 2167: 1140: 2115: 1938: 1916: 1814: 1738: 1643: 1519: 404: 2036: 1316:of mass (roughly one fourth the mass of 1130:{\displaystyle U=-{\frac {3GM^{2}}{5R}}} 268:, the gravitational binding energy of a 156:{\displaystyle U=-{\frac {3GM^{2}}{5R}}} 55:minimum total potential energy principle 18: 2201: 1840:expressed relative to the solar mass, 1479: 1144: 602:Integrating over all shells yields: 2049: 1976:Stress–energy–momentum pseudotensor 1489:neutron star gravitational mass of 1192:Two bodies, placed at the distance 103:, the gravitational binding energy 13: 1819: 1816: 1754: 1741: 1678: 1662: 1658: 1646: 1456: 1235: 1232: 1229: 1226: 1223: 1220: 1217: 578: 575: 572: 569: 566: 563: 560: 557: 545: 542: 539: 536: 533: 455: 452: 449: 446: 443: 440: 437: 434: 376: 373: 370: 367: 364: 14: 2225: 2046:(Berlin: Springer Verlag), p. 272 243:Preliminary Reference Earth Model 1200:is small. This can be seen as a 1149: 272:is about two times its internal 99:For a spherical body of uniform 96:of the system if disassembled. 175:is the mass of the sphere, and 2148: 2093: 1992: 230:'s total energy output. It is 47:gravitational potential energy 1: 2155:Neutron Star Masses and Radii 2103:Classical and Quantum Gravity 1986: 2087:10.1016/0031-9201(81)90046-7 1416:{\textstyle {\frac {3}{10}}} 1079:Gravitational binding energy 331:Assuming a constant density 68:'s theory of gravity called 32:gravitational binding energy 7: 2134:10.1088/0264-9381/23/23/030 1964: 1162:to comply with Knowledge's 10: 2230: 239:Adams–Williamson equation 1175:may contain suggestions. 1160:may need to be rewritten 1141:Negative mass component 278:hydrostatic equilibrium 53:in accordance with the 2044:Astrophysical Formulae 1956: 1884: 1827: 1771: 1695: 1600: 1548: 1466: 1417: 1396:which is smaller than 1390: 1291: 1131: 1070: 926: 869: 847: 594: 494: 415: 345: 322: 169:gravitational constant 157: 27: 1957: 1885: 1828: 1772: 1696: 1608:Given current values 1601: 1549: 1467: 1418: 1391: 1292: 1132: 1071: 927: 870: 868:{\displaystyle \rho } 848: 595: 495: 416: 346: 344:{\displaystyle \rho } 323: 158: 22: 1971:Stress–energy tensor 1898: 1844: 1782: 1706: 1615: 1557: 1501: 1431: 1425:Schwarzschild radius 1400: 1347: 1208: 1085: 938: 881: 859: 606: 506: 425: 355: 335: 312: 111: 94:elementary particles 2126:2006CQGra..23.7111K 2079:1981PEPI...25..297D 1480:Non-uniform spheres 771: 635: 241:), is given in the 2160:2011-12-17 at the 2042:Lang, K. R. 1980, 2000:"Spot the cluster" 1952: 1880: 1836:and the star mass 1823: 1767: 1691: 1596: 1544: 1462: 1413: 1386: 1287: 1127: 1066: 922: 865: 843: 757: 683: 621: 590: 490: 411: 341: 318: 290:radiation pressure 188:order-of-magnitude 182:Assuming that the 153: 70:General Relativity 28: 2164:, p. 9/20, bottom 2110:(23): 7111–7128. 2057:Dziewonski, A. M. 2027:Chandrasekhar, S. 1950: 1875: 1591: 1542: 1539: 1448: 1411: 1384: 1285: 1190: 1189: 1164:quality standards 1125: 1064: 1018: 1002: 961: 920: 904: 807: 735: 710: 682: 588: 472: 321:{\displaystyle R} 296:in the case of a 264:According to the 151: 62:newtonian gravity 45:, more negative) 2221: 2194: 2193: 2191: 2190: 2171: 2165: 2152: 2146: 2145: 2119: 2097: 2091: 2090: 2053: 2047: 2040: 2034: 2024: 2015: 2014: 2012: 2010: 1996: 1981:Nordtvedt effect 1961: 1959: 1958: 1953: 1951: 1949: 1948: 1947: 1927: 1926: 1925: 1911: 1889: 1887: 1886: 1881: 1876: 1874: 1873: 1861: 1856: 1855: 1832: 1830: 1829: 1824: 1822: 1813: 1812: 1794: 1793: 1776: 1774: 1773: 1768: 1766: 1765: 1764: 1749: 1748: 1737: 1736: 1718: 1717: 1700: 1698: 1697: 1692: 1690: 1689: 1688: 1673: 1672: 1654: 1653: 1642: 1641: 1605: 1603: 1602: 1597: 1592: 1590: 1589: 1588: 1575: 1567: 1553: 1551: 1550: 1545: 1543: 1541: 1540: 1532: 1523: 1514: 1471: 1469: 1468: 1463: 1461: 1460: 1459: 1449: 1441: 1422: 1420: 1419: 1414: 1412: 1404: 1395: 1393: 1392: 1387: 1385: 1383: 1382: 1381: 1368: 1357: 1338: 1336: 1333: 1320:– see above for 1315: 1310: 1307: 1296: 1294: 1293: 1288: 1286: 1284: 1283: 1282: 1266: 1265: 1264: 1248: 1240: 1239: 1238: 1185: 1182: 1176: 1153: 1145: 1136: 1134: 1133: 1128: 1126: 1124: 1116: 1115: 1114: 1098: 1075: 1073: 1072: 1067: 1065: 1063: 1055: 1054: 1053: 1037: 1029: 1028: 1023: 1019: 1017: 1016: 1015: 1003: 995: 989: 982: 981: 972: 971: 962: 954: 931: 929: 928: 923: 921: 919: 918: 917: 905: 897: 891: 874: 872: 871: 866: 852: 850: 849: 844: 842: 841: 832: 831: 826: 820: 819: 814: 808: 800: 783: 782: 781: 770: 765: 756: 755: 746: 745: 736: 728: 711: 706: 705: 701: 697: 696: 684: 675: 667: 663: 659: 658: 637: 634: 629: 599: 597: 596: 591: 589: 584: 583: 582: 581: 550: 549: 548: 525: 499: 497: 496: 491: 486: 485: 473: 465: 460: 459: 458: 420: 418: 417: 412: 400: 399: 381: 380: 379: 350: 348: 347: 342: 327: 325: 324: 319: 260: 258: 233: 225: 223: 213: 211: 201: 199: 162: 160: 159: 154: 152: 150: 142: 141: 140: 124: 76:property of the 2229: 2228: 2224: 2223: 2222: 2220: 2219: 2218: 2199: 2198: 2197: 2188: 2186: 2173: 2172: 2168: 2162:Wayback Machine 2153: 2149: 2098: 2094: 2061:Anderson, D. L. 2054: 2050: 2041: 2037: 2025: 2018: 2008: 2006: 1998: 1997: 1993: 1989: 1967: 1943: 1939: 1928: 1921: 1917: 1912: 1910: 1899: 1896: 1895: 1869: 1865: 1860: 1851: 1847: 1845: 1842: 1841: 1815: 1808: 1804: 1789: 1785: 1783: 1780: 1779: 1757: 1753: 1744: 1740: 1739: 1732: 1728: 1713: 1709: 1707: 1704: 1703: 1681: 1677: 1665: 1661: 1649: 1645: 1644: 1634: 1630: 1616: 1613: 1612: 1584: 1580: 1576: 1568: 1566: 1558: 1555: 1554: 1531: 1524: 1515: 1513: 1502: 1499: 1498: 1482: 1455: 1454: 1450: 1440: 1432: 1429: 1428: 1403: 1401: 1398: 1397: 1377: 1373: 1369: 1358: 1356: 1348: 1345: 1344: 1334: 1331: 1329: 1308: 1305: 1303: 1278: 1274: 1267: 1260: 1256: 1249: 1247: 1216: 1215: 1211: 1209: 1206: 1205: 1186: 1180: 1177: 1167: 1154: 1143: 1138: 1117: 1110: 1106: 1099: 1097: 1086: 1083: 1082: 1056: 1049: 1045: 1038: 1036: 1024: 1011: 1007: 994: 993: 988: 984: 983: 977: 973: 967: 963: 953: 939: 936: 935: 913: 909: 896: 895: 890: 882: 879: 878: 860: 857: 856: 837: 833: 827: 822: 821: 815: 810: 809: 799: 777: 773: 772: 766: 761: 751: 747: 741: 737: 727: 692: 688: 673: 672: 668: 654: 650: 643: 639: 638: 636: 630: 625: 607: 604: 603: 556: 555: 551: 532: 531: 527: 526: 524: 507: 504: 503: 481: 477: 464: 433: 432: 428: 426: 423: 422: 395: 391: 363: 362: 358: 356: 353: 352: 336: 333: 332: 313: 310: 309: 306: 256: 254: 232:37.5 MJ/kg 231: 221: 219: 209: 207: 197: 195: 190:estimate) with 179:is its radius. 143: 136: 132: 125: 123: 112: 109: 108: 66:Albert Einstein 36:gravitationally 24:Galaxy clusters 17: 12: 11: 5: 2227: 2217: 2216: 2214:Binding energy 2211: 2196: 2195: 2166: 2147: 2092: 2073:(4): 297–356. 2048: 2035: 2016: 1990: 1988: 1985: 1984: 1983: 1978: 1973: 1966: 1963: 1946: 1942: 1937: 1934: 1931: 1924: 1920: 1915: 1909: 1906: 1903: 1879: 1872: 1868: 1864: 1859: 1854: 1850: 1834: 1833: 1821: 1818: 1811: 1807: 1803: 1800: 1797: 1792: 1788: 1777: 1763: 1760: 1756: 1752: 1747: 1743: 1735: 1731: 1727: 1724: 1721: 1716: 1712: 1701: 1687: 1684: 1680: 1676: 1671: 1668: 1664: 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559: 554: 547: 544: 541: 538: 535: 530: 523: 520: 517: 514: 511: 489: 484: 480: 476: 471: 468: 463: 457: 454: 451: 448: 445: 442: 439: 436: 431: 410: 407: 403: 398: 394: 390: 387: 384: 378: 375: 372: 369: 366: 361: 340: 317: 305: 302: 274:thermal energy 266:virial theorem 149: 146: 139: 135: 131: 128: 122: 119: 116: 79: 15: 9: 6: 4: 3: 2: 2226: 2215: 2212: 2210: 2207: 2206: 2204: 2184: 2180: 2176: 2170: 2163: 2159: 2156: 2151: 2143: 2139: 2135: 2131: 2127: 2123: 2118: 2117:gr-qc/0610052 2113: 2109: 2105: 2104: 2096: 2088: 2084: 2080: 2076: 2072: 2068: 2067: 2062: 2058: 2052: 2045: 2039: 2032: 2028: 2023: 2021: 2005: 2001: 1995: 1991: 1982: 1979: 1977: 1974: 1972: 1969: 1968: 1962: 1944: 1940: 1935: 1932: 1929: 1922: 1918: 1913: 1907: 1904: 1901: 1893: 1890: 1877: 1870: 1866: 1862: 1857: 1852: 1848: 1839: 1809: 1805: 1801: 1798: 1795: 1790: 1786: 1778: 1761: 1758: 1750: 1745: 1733: 1729: 1725: 1722: 1719: 1714: 1710: 1702: 1685: 1682: 1674: 1669: 1666: 1655: 1650: 1638: 1635: 1631: 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Retrieved 2178: 2169: 2150: 2107: 2101: 2095: 2070: 2064: 2051: 2043: 2038: 2030: 2007:. Retrieved 2003: 1994: 1894: 1891: 1837: 1835: 1607: 1494: 1493:with radius 1490: 1487: 1483: 1474:relativistic 1341: 1300: 1298: 1197: 1193: 1191: 1178: 1169:You can help 1159: 1081: 1078: 933: 877: 854: 601: 501: 330: 307: 298:neutron star 282:relativistic 263: 250: 236: 215: 203: 191: 181: 176: 172: 164: 104: 98: 59: 42: 31: 29: 2004:www.eso.org 1181:August 2024 247:numerically 88:of all the 39:bound state 2203:Categories 2189:2024-05-18 2185:. May 2024 1987:References 1337:10 kg 294:black hole 200:10 kg 92:and other 51:aggregated 1933:− 1871:⊙ 1802:× 1791:⊙ 1759:− 1751:⋅ 1726:× 1683:− 1675:⋅ 1667:− 1656:⋅ 1636:− 1628:× 1561:β 1534:β 1529:− 1521:β 1438:≤ 1354:≤ 1245:− 1173:talk page 1095:− 1034:− 1005:π 965:π 948:− 907:π 885:ρ 863:ρ 824:ρ 812:π 794:− 759:∫ 749:ρ 739:π 722:− 699:ρ 686:π 661:ρ 648:π 623:∫ 616:− 519:− 488:ρ 475:π 402:ρ 389:π 339:ρ 286:supernova 259:10 J 224:10 J 212:10 m 121:− 74:nonlinear 2158:Archived 1965:See also 1311:10  292:or to a 86:energies 82:ADM mass 2209:Gravity 2142:1375765 2122:Bibcode 2075:Bibcode 2009:31 July 1936:738.313 1914:885.975 1799:1.98844 1723:8.98755 214:, then 167:is the 101:density 2140:  2029:1939, 1625:6.6743 1326:Joules 1318:Phobos 1171:. The 855:Since 163:where 78:entire 2138:S2CID 2112:arXiv 1330:2.494 1304:2.494 1301:costs 184:Earth 90:atoms 2183:NIST 2011:2017 1517:0.60 1423:its 421:and 270:star 255:2.49 220:2.24 208:6.37 202:and 196:5.97 64:and 57:. 43:i.e. 30:The 2130:doi 2083:doi 1497:, 1324:in 249:as 228:Sun 2205:: 2181:. 2177:. 2136:. 2128:. 2120:. 2108:23 2106:. 2081:. 2071:25 2069:. 2059:; 2019:^ 2002:. 1810:30 1806:10 1734:16 1730:10 1639:11 1632:10 1446:10 1427:: 1409:10 1332:21 1313:kg 1306:21 959:15 956:16 805:15 802:16 730:16 300:. 261:. 253:= 218:= 206:= 194:= 171:, 2192:. 2144:. 2132:: 2124:: 2114:: 2089:. 2085:: 2077:: 2013:. 1945:x 1941:M 1930:R 1923:x 1919:M 1908:= 1905:E 1902:B 1878:, 1867:M 1863:M 1858:= 1853:x 1849:M 1838:M 1820:g 1817:k 1796:= 1787:M 1762:2 1755:s 1746:2 1742:m 1720:= 1715:2 1711:c 1686:2 1679:s 1670:1 1663:g 1659:k 1651:3 1647:m 1622:= 1619:G 1594:. 1586:2 1582:c 1578:R 1573:M 1570:G 1564:= 1537:2 1526:1 1511:= 1508:E 1505:B 1495:R 1491:M 1457:s 1452:r 1443:3 1435:R 1406:3 1379:2 1375:c 1371:5 1366:M 1363:G 1360:3 1351:R 1335:Ă— 1309:Ă— 1280:2 1276:c 1272:R 1269:5 1262:2 1258:M 1254:G 1251:3 1242:= 1236:g 1233:n 1230:i 1227:d 1224:n 1221:i 1218:b 1213:M 1198:R 1194:R 1183:) 1179:( 1122:R 1119:5 1112:2 1108:M 1104:G 1101:3 1092:= 1089:U 1061:R 1058:5 1051:2 1047:M 1043:G 1040:3 1031:= 1026:2 1021:) 1013:3 1009:R 1000:3 997:4 991:M 986:( 979:5 975:R 969:2 951:G 945:= 942:U 915:3 911:R 902:3 899:4 893:M 888:= 839:5 835:R 829:2 817:2 797:G 791:= 788:r 785:d 779:4 775:r 768:R 763:0 753:2 743:2 733:3 725:G 719:= 716:r 713:d 708:r 703:) 694:3 690:r 680:3 677:4 670:( 665:) 656:2 652:r 645:4 641:( 632:R 627:0 619:G 613:= 610:U 586:r 579:r 576:o 573:i 570:r 567:e 564:t 561:n 558:i 553:m 546:l 543:l 540:e 537:h 534:s 529:m 522:G 516:= 513:U 510:d 483:3 479:r 470:3 467:4 462:= 456:r 453:o 450:i 447:r 444:e 441:t 438:n 435:i 430:m 409:r 406:d 397:2 393:r 386:4 383:= 377:l 374:l 371:e 368:h 365:s 360:m 316:R 257:Ă— 251:U 222:Ă— 216:U 210:Ă— 204:r 198:Ă— 192:M 177:R 173:M 165:G 148:R 145:5 138:2 134:M 130:G 127:3 118:= 115:U 105:U

Index


Galaxy clusters
gravitationally
bound state
gravitational potential energy
aggregated
minimum total potential energy principle
newtonian gravity
Albert Einstein
General Relativity
nonlinear
ADM mass
energies
atoms
elementary particles
density
gravitational constant
Earth
order-of-magnitude
Sun
Adams–Williamson equation
Preliminary Reference Earth Model
numerically
virial theorem
star
thermal energy
hydrostatic equilibrium
relativistic
supernova
radiation pressure

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