Knowledge (XXG)

Standard asteroid physical characteristics

Source šŸ“

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gives calculations for the mean densities of C, S, and M class asteroids as 1.38, 2.71, and 5.32 g/cm. (Here "C" included Tholen classes C, D, P, T, B, G, and F, while "S" included Tholen classes S, K, Q, V, R, A, and E). Assuming these values (rather than the present ~2 g/cm) is a better guess.
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While these two albedos are correlated, the numerical factor between them depends in a very nontrivial way on the surface properties. Actual measurements of Bond albedo are not forthcoming for most asteroids because they require measurements from high phase angles that can only be acquired by
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is a constant. If the day of the relevant observations is known, the distance from the Sun on that day can be obtained from sources such as the NASA orbit calculator, and corresponding temperature estimates at perihelion, aphelion, etc. can be derived from the above. expression
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Some other information for large numbers of asteroids can be found at the Planetary Data System Small Bodies Node. Up-to-date information on pole orientation of several dozen asteroids is provided by Doc. Mikko Kaasalainen, and can be used to determine
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does this for 29 asteroids. These measurements are contingent for a particular day of observation. and the asteroid's surface temperature will change in a regular way depending on its distance from the Sun. From the Stefan-Boltzmann calculation above,
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Besides these estimations, masses can be obtained for the larger asteroids by solving for the perturbations they cause in each other's orbits, or when the asteroid has an orbiting companion of known orbital radius. The masses of the largest asteroids
2400:. Some complicated modelling of surface and thermal properties can lead to estimates of the Bond albedo given the geometric one, but this is beyond the scope of a quick estimate. It can be obtained for some asteroids from scientific publications. 1060: 2013: 837: 1813: 1468: 1332: 1728: 35:
are tabulated in the PDS, with the most reliable data being the syntheses labeled in the data tables. More recent determinations for several dozens of asteroids are collected at the web page of a Finnish research group in
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shows that for bodies in the asteroid albedo range, the typical difference between Bond and geometric albedo is 20% or less, with either quantity capable of being larger. Since the calculated temperature varies as
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For want of a better alternative for most asteroids, the best that can be done is to assume that the two albedos are equal, while keeping in mind the inherent inaccuracy present in the resulting temperature values.
23:, almost nothing is known apart from a few physical parameters and orbital elements. Some physical characteristics can only be estimated. The physical data is determined by making certain standard assumptions. 1581: 416: 2208: 742: 286: 1920: 891:
For irregularly shaped bodies, the surface gravity will differ appreciably with location. The above formula then is only an approximation, as the calculations become more involved. The value of
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The typical inaccuracy in calculated temperature from this source alone is found to be about 2%. This translates to an uncertainty of about Ā±5 K for maximum temperatures.
2369:(the proportion of total incoming power reflected, taking into account all directions), while the IRAS and MSX albedo data that is available for asteroids gives only the 1125: 950: 3673: 2480: 472: 2335: 2313: 2233: 1523: 1493: 1635: 451: 2574: 2554: 2390: 2367: 2130: 1837: 1605: 1177: 1103: 1083: 909: 881: 861: 659: 167: 542:. While these perturbations are tiny, they can be accurately measured from radar ranging data from the Earth to spacecraft on the surface of Mars, such as the 958: 1928: 750: 2047:
While this method gives a fairly good estimate of the average surface temperature, the local temperature varies greatly, as is typical for bodies without
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If the body in question is a member of a close binary with components of comparable mass, the effect of the second body may also be non-negligible.
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Apart from a few asteroids whose densities have been investigated, one has to resort to enlightened guesswork. See Carry for a summary.
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For many asteroids, lightcurve analysis provides estimates of pole direction and diameter ratios. Pre-1995 estimates collected by
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There is a snag when using these expressions to estimate the temperature of a particular asteroid. The calculation requires the
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Estimations of masses of the largest asteroids and the main asteroid belt from ranging to planets, Mars orbiters and landers
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Infra-red observations are commonly combined with albedo to measure the temperature more directly. For example, L.F. Lim
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A rough estimate of the maximum temperature can be obtained by assuming that when the Sun is overhead, the surface is in
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at surface points closer to the center of mass is usually somewhat greater than at surface points farther out.
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These data can be used to obtain a better estimate of dimensions. A body's dimensions are usually given as a
3475: 3364: 3355: 3157: 3035: 2512: 840: 2069: 3678: 3092: 2516: 82: 2415: 1159:. The negative sign indicates that it acts in the opposite direction to the gravitational acceleration 50: 116: 3714: 3274: 2849: 2833: 2798: 2236: 1130: 2524: 2060: 2021: 1846: 3777: 3756: 3028: 1108: 933: 44: 2459: 1367:
is obtained by equating the mean incident and radiated heat power. The total incident power is:
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which is running a systematic campaign to determine poles and shape models from lightcurves.
3650: 2857: 2837: 2786: 2529: 2370: 1637:, the asteroid is spherical, it is on a circular orbit, and that the Sun's energy output is 1584: 2318: 2296: 2216: 1506: 1476: 3645: 3612: 3607: 3602: 3597: 3592: 3571: 3566: 3542: 3537: 3532: 3527: 3522: 3517: 3512: 3493: 3488: 3483: 3463: 3458: 3453: 3448: 3443: 3438: 3433: 3419: 3414: 3409: 3404: 3399: 3392: 3387: 3382: 3377: 3372: 3338: 3266: 3229: 3124: 3107: 2757: 2504: 1526: 1360: 627: 2063:
with the instantaneous solar radiation. This gives an average "sub-solar" temperature of
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The simplest method which gives sensible results is to assume the asteroid behaves as a
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which characterises only the strength of light reflected back to the source (the Sun).
2375: 2352: 2115: 1822: 1590: 1162: 1088: 1068: 1055:{\displaystyle g_{\rm {centrifugal}}=-\left({\frac {2\pi }{T}}\right)^{2}r\sin \theta } 894: 866: 846: 644: 427: 170: 152: 3771: 3256: 3224: 3219: 3182: 3129: 2794: 2397: 2008:{\displaystyle T={{(1-A)L_{\odot }} \over {16\pi a^{2}\epsilon \sigma }}^{1 \over 4}} 832:{\displaystyle G\approx 6.674\times 10^{-11}\,{\rm {m^{3}\cdot s^{-2}\cdot kg^{-1}}}} 543: 147: 32: 2840:; Vasilyev, M. V.; Yagudina, E. I. (July 2002). "Hidden Mass in the Asteroid Belt". 1808:{\displaystyle \sigma \approx 5.67\times 10^{-8}\,{\rm {W\cdot m^{-2}\cdot K^{-4}}}} 3744: 3709: 3261: 3167: 1463:{\displaystyle R_{\mathrm {in} }={\frac {(1-A)L_{\odot }\pi r^{2}}{4\pi a^{2}}},} 1327:{\displaystyle g_{\rm {effective}}=g_{\rm {gravitational}}+g_{\rm {centrifugal}}} 927:, when one is away from the poles. The centripetal acceleration experienced at a 3724: 3306: 3172: 2986: 2659: 2408: 2347: 2044:, estimated from detailed observations of a few of the large asteroids is used. 1500: 1364: 2736: 1723:{\displaystyle R_{\mathrm {out} }=4\pi r^{2}\epsilon \sigma T^{4}{\frac {}{}},} 2634: 2508: 1866: 1608: 2948: 1648:, the radiated power (from the entire spherical surface of the asteroid) is: 3197: 3162: 2920: 2691: 2527:
are usually given by either the IRAS or MSX minor planet surveys. These are
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is the latitude. Its magnitude is maximized when one is at the equator, and
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However, density depends on the asteroid's spectral type. Krasinsky
3739: 2892: 2816: 2917:"IRAS Minor Planet Survey Supplemental IRAS Minor Planet Survey" 2888: 2520: 2494: 1576:{\displaystyle L_{\odot }\approx 3.827\times 10^{26}\,{\rm {W}}} 539: 411:{\displaystyle c={\frac {d}{(\nu ^{2}\mu )^{\frac {1}{3}}}}\,\!} 3024: 3010: 2945:"Midcourse Space Experiment (MSX) Infrared Minor Planet Survey" 2501:(MSX) minor planet survey is the usual source of the diameter. 2654:
Magnusson, Per (1989). "Pole determinations of asteroids". In
2203:{\displaystyle T_{ss}^{\rm {max}}={\sqrt {\frac {2}{1-e}}}\ T} 453:
can be estimated from the diameter and assumed density values
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Temperature measurements and regular temperature variations
737:{\displaystyle g_{\rm {spherical}}={\frac {GM}{r^{2}}}\,\!} 923:
experienced by an object on the surface is reduced by the
2793:. 35th COSPAR Scientific Assembly. Held 18ā€“25 July 2004. 2576:
of a spherically symmetric body, the escape velocity is:
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is the distance from the Sun on any particular day, and
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at the PDS. Absolute magnitude is usually given by the
281:{\displaystyle a=d\,(\mu ^{2}\nu )^{\frac {1}{3}}\,\!} 47:, the axes of which are listed in decreasing order as 2585: 2562: 2542: 2462: 2456:, the dependence is fairly weak for typical asteroid 2418: 2378: 2355: 2321: 2299: 2261: 2219: 2144: 2118: 2072: 2024: 1931: 1875: 1849: 1825: 1739: 1657: 1617: 1607:
the asteroid's radius. It has been assumed that: the
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minor planet survey or the MSX minor planet survey.
1915:{\displaystyle R_{\mathrm {in} }=R_{\mathrm {out} }} 3702: 3664: 3631: 3474: 3363: 3354: 3324: 3315: 3148: 3058: 2621: 2568: 2548: 2474: 2448: 2384: 2361: 2329: 2307: 2282: 2227: 2202: 2124: 2101: 2036: 2007: 1914: 1857: 1831: 1807: 1722: 1629: 1599: 1575: 1517: 1487: 1462: 1326: 1171: 1151: 1119: 1097: 1077: 1054: 944: 903: 875: 855: 831: 736: 653: 602: 518: 466: 445: 410: 342: 280: 225:for consistency, and obtains the three diameters: 217: 161: 138: 105: 71: 3011:The Planetary Data System (PDS) Small Bodies Node 2326: 2304: 2224: 1854: 1514: 1484: 1116: 941: 733: 515: 407: 339: 277: 214: 2132:is the average temperature calculated as above. 2135:At perihelion, the radiation is maximised, and 603:{\displaystyle \rho =2\,{\rm {g\cdot cm^{-3}}}} 519:{\displaystyle M={\frac {\pi abc\rho }{6}}\,\!} 432:Barring detailed mass determinations, the mass 2622:{\displaystyle v_{e}={\sqrt {\frac {2GM}{r}}}} 3036: 8: 2985:. PDS Asteroid/Dust Archive. Archived from 2947:. PDS Asteroid/Dust Archive. Archived from 2919:. PDS Asteroid/Dust Archive. Archived from 2735:. PDS Asteroid/Dust Archive. Archived from 538:can also be obtained from perturbations of 3360: 3321: 3043: 3029: 3021: 218:{\displaystyle d=(abc)^{\frac {1}{3}}\,\!} 2726: 2724: 2599: 2590: 2584: 2561: 2541: 2461: 2435: 2417: 2377: 2354: 2325: 2320: 2303: 2298: 2268: 2260: 2223: 2218: 2174: 2158: 2157: 2149: 2143: 2117: 2089: 2077: 2071: 2023: 1994: 1979: 1968: 1961: 1941: 1939: 1930: 1899: 1898: 1881: 1880: 1874: 1853: 1848: 1824: 1794: 1778: 1767: 1766: 1765: 1756: 1738: 1711: 1705: 1689: 1663: 1662: 1656: 1616: 1592: 1567: 1566: 1565: 1559: 1540: 1534: 1513: 1508: 1483: 1478: 1448: 1430: 1417: 1395: 1382: 1381: 1375: 1287: 1286: 1236: 1235: 1197: 1196: 1190: 1164: 1132: 1115: 1110: 1090: 1070: 1034: 1015: 967: 966: 960: 940: 935: 896: 868: 848: 818: 799: 786: 781: 780: 779: 770: 752: 732: 724: 710: 676: 675: 669: 646: 589: 575: 574: 573: 562: 514: 490: 482: 463: 458: 442: 437: 406: 392: 379: 366: 358: 338: 327: 313: 307: 296: 276: 265: 252: 244: 233: 213: 202: 178: 154: 126: 118: 102: 92: 84: 52: 2939: 2937: 2911: 2909: 2710: 2708: 2396:spacecraft that pass near or beyond the 2283:{\displaystyle T={\frac {c}{\sqrt {d}}}} 2823:to be published, accessed Dec. 20, 2013 2646: 3273:Outer Solar System, does not include 7: 2102:{\displaystyle T_{ss}={\sqrt {2}}T} 1085:is the rotation period in seconds, 2874:Icarus, Volume no. 173, 385 (2005) 2165: 2162: 2159: 1906: 1903: 1900: 1885: 1882: 1791: 1775: 1768: 1670: 1667: 1664: 1568: 1386: 1383: 1318: 1315: 1312: 1309: 1306: 1303: 1300: 1297: 1294: 1291: 1288: 1273: 1270: 1267: 1264: 1261: 1258: 1255: 1252: 1249: 1246: 1243: 1240: 1237: 1222: 1219: 1216: 1213: 1210: 1207: 1204: 1201: 1198: 998: 995: 992: 989: 986: 983: 980: 977: 974: 971: 968: 815: 811: 796: 783: 701: 698: 695: 692: 689: 686: 683: 680: 677: 586: 582: 576: 106:{\displaystyle \mu ={a \over b}\,} 14: 2762:"Masses of the Largest Asteroids" 2449:{\displaystyle (1-A)^{1 \over 4}} 1359:in equilibrium with the incident 919:On a rotating body, the apparent 79:. If we have the diameter ratios 72:{\displaystyle a\times b\times c} 3752: 3751: 3246:Between Earth and the main belt 2733:"Asteroid Densities Compilation" 1644:Using a greybody version of the 139:{\displaystyle \nu ={b \over c}} 3641:Asteroids visited by spacecraft 557:For many asteroids, a value of 2432: 2419: 1954: 1942: 1410: 1398: 1182:The effective acceleration is 1152:{\displaystyle \sin \theta =1} 1105:is the equatorial radius, and 389: 372: 262: 245: 199: 186: 146:from lightcurves, and an IRAS 1: 2821:Planetary & Space Science 2037:{\displaystyle \epsilon =0.9} 1858:{\displaystyle \epsilon \,\!} 863:is the mass of the body, and 1865:is the asteroid's infra-red 2674:University of Arizona Press 2497:minor planet survey or the 2489:Data and derived parameters 1120:{\displaystyle \theta \,\!} 945:{\displaystyle \theta \,\!} 3794: 2515:is usually taken from the 2499:Midcourse Space Experiment 2475:{\displaystyle A\approx p} 639:gravitational acceleration 637:For a spherical body, the 625: 425: 3735: 3689:Discovering observatories 2970:PDS Asteroid/Dust Archive 2342:Albedo inaccuracy problem 1817:Stefanā€“Boltzmann constant 3071:Physical characteristics 2688:"Asteroid Spin Vectors" 2511:parameters at the PDS. 467:{\displaystyle \rho \,} 16:Astronomical parameters 3720:Asteroids in astrology 2862:10.1006/icar.2002.6837 2623: 2570: 2550: 2507:is usually taken from 2476: 2450: 2386: 2363: 2331: 2309: 2284: 2229: 2204: 2126: 2103: 2038: 2018:The standard value of 2009: 1916: 1859: 1839:is the temperature in 1833: 1809: 1724: 1631: 1601: 1577: 1519: 1489: 1464: 1328: 1173: 1153: 1121: 1099: 1079: 1056: 946: 905: 877: 857: 841:gravitational constant 833: 738: 655: 604: 520: 468: 447: 412: 344: 282: 219: 163: 140: 107: 73: 3275:distant minor planets 3135:Palomarā€“Leiden survey 3093:Gravitational keyhole 3016:NASA orbit calculator 2760:(November 30, 1999). 2676:. pp. 1180ā€“1190. 2624: 2571: 2551: 2517:Tholen classification 2477: 2451: 2387: 2364: 2332: 2330:{\displaystyle c\,\!} 2310: 2308:{\displaystyle d\,\!} 2285: 2230: 2228:{\displaystyle e\,\!} 2205: 2127: 2104: 2039: 2010: 1917: 1860: 1834: 1810: 1725: 1632: 1602: 1578: 1520: 1518:{\displaystyle a\,\!} 1490: 1488:{\displaystyle A\,\!} 1465: 1329: 1174: 1154: 1122: 1100: 1080: 1057: 947: 906: 878: 858: 834: 739: 656: 605: 521: 474:worked out as below. 469: 448: 413: 345: 283: 220: 164: 141: 108: 74: 3715:Asteroids in fiction 2983:"Asteroid Data Sets" 2968:Asteroid Taxonomies 2817:Density of asteroids 2768:on February 12, 2009 2583: 2560: 2540: 2536:For surface gravity 2525:Astronomical albedos 2482:values of 0.05āˆ’0.3. 2460: 2416: 2376: 2353: 2319: 2297: 2259: 2217: 2142: 2116: 2070: 2022: 1929: 1873: 1847: 1823: 1737: 1655: 1646:Stefanā€“Boltzmann law 1615: 1591: 1533: 1507: 1477: 1374: 1189: 1163: 1131: 1109: 1089: 1069: 959: 934: 895: 867: 847: 751: 668: 645: 561: 481: 457: 436: 357: 295: 232: 177: 153: 117: 83: 51: 2854:2002Icar..158...98K 2803:2004cosp...35.2014P 2714:Modeled asteroids. 2664:Mildred S. Matthews 2170: 2061:thermal equilibrium 1630:{\displaystyle 1-A} 1346:Surface temperature 446:{\displaystyle M\,} 3194:Interior to Earth 2619: 2566: 2546: 2472: 2446: 2382: 2359: 2327: 2305: 2280: 2225: 2200: 2145: 2122: 2099: 2034: 2005: 1912: 1855: 1829: 1805: 1720: 1627: 1597: 1573: 1515: 1485: 1460: 1324: 1169: 1149: 1117: 1095: 1075: 1052: 942: 901: 873: 853: 829: 734: 651: 610:has been assumed. 600: 516: 464: 443: 408: 340: 278: 215: 159: 136: 103: 69: 45:triaxial ellipsoid 19:For most numbered 3765: 3764: 3627: 3626: 3623: 3622: 3066:Notable asteroids 2656:Richard P. Binzel 2617: 2616: 2569:{\displaystyle r} 2549:{\displaystyle g} 2530:geometric albedos 2443: 2385:{\displaystyle p} 2362:{\displaystyle A} 2278: 2277: 2196: 2192: 2191: 2125:{\displaystyle T} 2094: 2002: 1992: 1832:{\displaystyle T} 1715: 1714: 1713: 1600:{\displaystyle r} 1455: 1363:. Then, its mean 1172:{\displaystyle g} 1098:{\displaystyle r} 1078:{\displaystyle T} 1028: 925:centripetal force 915:Centripetal force 904:{\displaystyle g} 876:{\displaystyle r} 856:{\displaystyle M} 730: 654:{\displaystyle g} 512: 404: 400: 335: 321: 273: 210: 173:of the diameters 162:{\displaystyle d} 134: 100: 3785: 3755: 3754: 3361: 3322: 3295:Neptune-crossers 3280:Jupiter-crossers 3267:Active asteroids 3203:Mercury-crossers 3103:Close approaches 3083:Impact avoidance 3045: 3038: 3031: 3022: 2998: 2997: 2995: 2994: 2979: 2973: 2966: 2960: 2959: 2957: 2956: 2941: 2932: 2931: 2929: 2928: 2913: 2904: 2903: 2901: 2900: 2891:. Archived from 2885:"Orbit Diagrams" 2881: 2875: 2872: 2866: 2865: 2834:Krasinsky, G. A. 2830: 2824: 2813: 2807: 2806: 2797:. p. 2014. 2783: 2777: 2776: 2774: 2773: 2764:. Archived from 2758:Hilton, James L. 2754: 2748: 2747: 2745: 2744: 2728: 2719: 2712: 2703: 2702: 2700: 2699: 2690:. Archived from 2684: 2678: 2677: 2651: 2628: 2626: 2625: 2620: 2618: 2612: 2601: 2600: 2595: 2594: 2575: 2573: 2572: 2567: 2555: 2553: 2552: 2547: 2481: 2479: 2478: 2473: 2455: 2453: 2452: 2447: 2445: 2444: 2436: 2391: 2389: 2388: 2383: 2371:geometric albedo 2368: 2366: 2365: 2360: 2336: 2334: 2333: 2328: 2314: 2312: 2311: 2306: 2289: 2287: 2286: 2281: 2279: 2273: 2269: 2234: 2232: 2231: 2226: 2209: 2207: 2206: 2201: 2194: 2193: 2190: 2176: 2175: 2169: 2168: 2156: 2131: 2129: 2128: 2123: 2108: 2106: 2105: 2100: 2095: 2090: 2085: 2084: 2043: 2041: 2040: 2035: 2014: 2012: 2011: 2006: 2004: 2003: 1995: 1993: 1991: 1984: 1983: 1967: 1966: 1965: 1940: 1921: 1919: 1918: 1913: 1911: 1910: 1909: 1890: 1889: 1888: 1864: 1862: 1861: 1856: 1838: 1836: 1835: 1830: 1814: 1812: 1811: 1806: 1804: 1803: 1802: 1801: 1786: 1785: 1764: 1763: 1729: 1727: 1726: 1721: 1716: 1712: 1710: 1709: 1694: 1693: 1675: 1674: 1673: 1636: 1634: 1633: 1628: 1606: 1604: 1603: 1598: 1585:solar luminosity 1582: 1580: 1579: 1574: 1572: 1571: 1564: 1563: 1545: 1544: 1524: 1522: 1521: 1516: 1499:(precisely, the 1495:is the asteroid 1494: 1492: 1491: 1486: 1469: 1467: 1466: 1461: 1456: 1454: 1453: 1452: 1436: 1435: 1434: 1422: 1421: 1396: 1391: 1390: 1389: 1333: 1331: 1330: 1325: 1323: 1322: 1321: 1278: 1277: 1276: 1227: 1226: 1225: 1178: 1176: 1175: 1170: 1158: 1156: 1155: 1150: 1126: 1124: 1123: 1118: 1104: 1102: 1101: 1096: 1084: 1082: 1081: 1076: 1061: 1059: 1058: 1053: 1039: 1038: 1033: 1029: 1024: 1016: 1003: 1002: 1001: 951: 949: 948: 943: 910: 908: 907: 902: 882: 880: 879: 874: 862: 860: 859: 854: 838: 836: 835: 830: 828: 827: 826: 825: 807: 806: 791: 790: 778: 777: 743: 741: 740: 735: 731: 729: 728: 719: 711: 706: 705: 704: 660: 658: 657: 652: 609: 607: 606: 601: 599: 598: 597: 596: 525: 523: 522: 517: 513: 508: 491: 473: 471: 470: 465: 452: 450: 449: 444: 417: 415: 414: 409: 405: 403: 402: 401: 393: 384: 383: 367: 349: 347: 346: 341: 337: 336: 328: 326: 322: 314: 287: 285: 284: 279: 275: 274: 266: 257: 256: 224: 222: 221: 216: 212: 211: 203: 168: 166: 165: 160: 145: 143: 142: 137: 135: 127: 112: 110: 109: 104: 101: 93: 78: 76: 75: 70: 3793: 3792: 3788: 3787: 3786: 3784: 3783: 3782: 3768: 3767: 3766: 3761: 3731: 3698: 3660: 3619: 3470: 3350: 3311: 3290:Uranus-crossers 3285:Saturn-crossers 3188:Neptune trojans 3178:Jupiter trojans 3144: 3054: 3049: 3007: 3002: 3001: 2992: 2990: 2981: 2980: 2976: 2967: 2963: 2954: 2952: 2943: 2942: 2935: 2926: 2924: 2915: 2914: 2907: 2898: 2896: 2883: 2882: 2878: 2873: 2869: 2832: 2831: 2827: 2814: 2810: 2785: 2784: 2780: 2771: 2769: 2756: 2755: 2751: 2742: 2740: 2731: 2729: 2722: 2716:rni.helsinki.fi 2713: 2706: 2697: 2695: 2686: 2685: 2681: 2653: 2652: 2648: 2643: 2602: 2586: 2581: 2580: 2558: 2557: 2538: 2537: 2505:Rotation period 2491: 2458: 2457: 2431: 2414: 2413: 2374: 2373: 2351: 2350: 2344: 2317: 2316: 2295: 2294: 2257: 2256: 2245: 2215: 2214: 2180: 2140: 2139: 2114: 2113: 2073: 2068: 2067: 2057: 2020: 2019: 1975: 1957: 1938: 1927: 1926: 1894: 1876: 1871: 1870: 1845: 1844: 1821: 1820: 1790: 1774: 1752: 1735: 1734: 1701: 1685: 1658: 1653: 1652: 1613: 1612: 1589: 1588: 1555: 1536: 1531: 1530: 1527:semi-major axis 1505: 1504: 1475: 1474: 1444: 1437: 1426: 1413: 1397: 1377: 1372: 1371: 1361:solar radiation 1353: 1348: 1340: 1282: 1231: 1192: 1187: 1186: 1161: 1160: 1129: 1128: 1107: 1106: 1087: 1086: 1067: 1066: 1017: 1011: 1010: 962: 957: 956: 932: 931: 917: 893: 892: 889: 883:is its radius. 865: 864: 845: 844: 814: 795: 782: 766: 749: 748: 720: 712: 671: 666: 665: 643: 642: 641:at the surface 635: 630: 628:Surface gravity 624: 622:Surface gravity 585: 559: 558: 552: 492: 479: 478: 455: 454: 434: 433: 430: 424: 388: 375: 371: 355: 354: 309: 308: 293: 292: 261: 248: 230: 229: 198: 175: 174: 169:, one sets the 151: 150: 115: 114: 81: 80: 49: 48: 29: 17: 12: 11: 5: 3791: 3789: 3781: 3780: 3770: 3769: 3763: 3762: 3760: 3759: 3748: 3747: 3742: 3736: 3733: 3732: 3730: 3729: 3728: 3727: 3717: 3712: 3706: 3704: 3700: 3699: 3697: 3696: 3694:Space missions 3691: 3686: 3681: 3676: 3670: 3668: 3662: 3661: 3659: 3658: 3653: 3648: 3643: 3637: 3635: 3629: 3628: 3625: 3624: 3621: 3620: 3618: 3617: 3616: 3615: 3610: 3605: 3600: 3595: 3585: 3584: 3583: 3580: 3577: 3574: 3563: 3562: 3561: 3560: 3557: 3554: 3551: 3548: 3545: 3540: 3535: 3530: 3525: 3520: 3510: 3509: 3508: 3505: 3502: 3499: 3496: 3491: 3480: 3478: 3472: 3471: 3469: 3468: 3467: 3466: 3461: 3456: 3451: 3446: 3441: 3436: 3425: 3424: 3423: 3422: 3417: 3412: 3402: 3397: 3396: 3395: 3390: 3385: 3380: 3369: 3367: 3358: 3352: 3351: 3349: 3348: 3341: 3336: 3330: 3328: 3319: 3317:Classification 3313: 3312: 3310: 3309: 3304: 3299: 3298: 3297: 3292: 3287: 3282: 3271: 3270: 3269: 3264: 3254: 3253: 3252: 3244: 3243: 3242: 3240:Earth-crossers 3237: 3232: 3227: 3222: 3212: 3211: 3210: 3208:Venus-crossers 3205: 3200: 3192: 3191: 3190: 3185: 3183:Uranus trojans 3180: 3175: 3170: 3165: 3154: 3152: 3146: 3145: 3143: 3142: 3140:Contact binary 3137: 3132: 3127: 3122: 3121: 3120: 3115: 3105: 3100: 3095: 3090: 3085: 3080: 3079: 3078: 3076:dynamic method 3068: 3062: 3060: 3056: 3055: 3050: 3048: 3047: 3040: 3033: 3025: 3019: 3018: 3013: 3006: 3005:External links 3003: 3000: 2999: 2974: 2961: 2933: 2905: 2876: 2867: 2838:Pitjeva, E. V. 2825: 2815:Benoit Carry, 2808: 2787:Pitjeva, E. V. 2778: 2749: 2720: 2704: 2679: 2645: 2644: 2642: 2639: 2630: 2629: 2615: 2611: 2608: 2605: 2598: 2593: 2589: 2565: 2545: 2513:Spectral class 2493:Data from the 2490: 2487: 2471: 2468: 2465: 2442: 2439: 2434: 2430: 2427: 2424: 2421: 2381: 2358: 2343: 2340: 2324: 2302: 2291: 2290: 2276: 2272: 2267: 2264: 2244: 2241: 2239:of the orbit. 2222: 2211: 2210: 2199: 2189: 2186: 2183: 2179: 2173: 2167: 2164: 2161: 2155: 2152: 2148: 2121: 2110: 2109: 2098: 2093: 2088: 2083: 2080: 2076: 2056: 2053: 2033: 2030: 2027: 2016: 2015: 2001: 1998: 1990: 1987: 1982: 1978: 1974: 1971: 1964: 1960: 1956: 1953: 1950: 1947: 1944: 1937: 1934: 1922:, one obtains 1908: 1905: 1902: 1897: 1893: 1887: 1884: 1879: 1852: 1828: 1800: 1797: 1793: 1789: 1784: 1781: 1777: 1773: 1770: 1762: 1759: 1755: 1751: 1748: 1745: 1742: 1731: 1730: 1719: 1708: 1704: 1700: 1697: 1692: 1688: 1684: 1681: 1678: 1672: 1669: 1666: 1661: 1626: 1623: 1620: 1596: 1570: 1562: 1558: 1554: 1551: 1548: 1543: 1539: 1512: 1482: 1471: 1470: 1459: 1451: 1447: 1443: 1440: 1433: 1429: 1425: 1420: 1416: 1412: 1409: 1406: 1403: 1400: 1394: 1388: 1385: 1380: 1352: 1349: 1347: 1344: 1339: 1338:Close binaries 1336: 1335: 1334: 1320: 1317: 1314: 1311: 1308: 1305: 1302: 1299: 1296: 1293: 1290: 1285: 1281: 1275: 1272: 1269: 1266: 1263: 1260: 1257: 1254: 1251: 1248: 1245: 1242: 1239: 1234: 1230: 1224: 1221: 1218: 1215: 1212: 1209: 1206: 1203: 1200: 1195: 1168: 1148: 1145: 1142: 1139: 1136: 1114: 1094: 1074: 1063: 1062: 1051: 1048: 1045: 1042: 1037: 1032: 1027: 1023: 1020: 1014: 1009: 1006: 1000: 997: 994: 991: 988: 985: 982: 979: 976: 973: 970: 965: 939: 916: 913: 900: 888: 887:Irregular body 885: 872: 852: 824: 821: 817: 813: 810: 805: 802: 798: 794: 789: 785: 776: 773: 769: 765: 762: 759: 756: 745: 744: 727: 723: 718: 715: 709: 703: 700: 697: 694: 691: 688: 685: 682: 679: 674: 650: 634: 633:Spherical body 631: 626:Main article: 623: 620: 595: 592: 588: 584: 581: 578: 572: 569: 566: 551: 548: 544:Viking landers 527: 526: 511: 507: 504: 501: 498: 495: 489: 486: 462: 441: 428:Dynamic method 423: 420: 419: 418: 399: 396: 391: 387: 382: 378: 374: 370: 365: 362: 351: 350: 334: 331: 325: 320: 317: 312: 306: 303: 300: 289: 288: 272: 269: 264: 260: 255: 251: 247: 243: 240: 237: 209: 206: 201: 197: 194: 191: 188: 185: 182: 171:geometric mean 158: 133: 130: 125: 122: 99: 96: 91: 88: 68: 65: 62: 59: 56: 28: 25: 15: 13: 10: 9: 6: 4: 3: 2: 3790: 3779: 3776: 3775: 3773: 3758: 3750: 3749: 3746: 3743: 3741: 3738: 3737: 3734: 3726: 3723: 3722: 3721: 3718: 3716: 3713: 3711: 3708: 3707: 3705: 3701: 3695: 3692: 3690: 3687: 3685: 3682: 3680: 3679:Minor planets 3677: 3675: 3672: 3671: 3669: 3667: 3663: 3657: 3654: 3652: 3649: 3647: 3644: 3642: 3639: 3638: 3636: 3634: 3630: 3614: 3611: 3609: 3606: 3604: 3601: 3599: 3596: 3594: 3591: 3590: 3589: 3586: 3581: 3578: 3575: 3573: 3570: 3569: 3568: 3565: 3564: 3558: 3555: 3552: 3549: 3546: 3544: 3541: 3539: 3536: 3534: 3531: 3529: 3526: 3524: 3521: 3519: 3516: 3515: 3514: 3511: 3506: 3503: 3500: 3497: 3495: 3492: 3490: 3487: 3486: 3485: 3482: 3481: 3479: 3477: 3473: 3465: 3462: 3460: 3457: 3455: 3452: 3450: 3447: 3445: 3442: 3440: 3437: 3435: 3432: 3431: 3430: 3429:small classes 3427: 3426: 3421: 3418: 3416: 3413: 3411: 3408: 3407: 3406: 3403: 3401: 3398: 3394: 3391: 3389: 3386: 3384: 3381: 3379: 3376: 3375: 3374: 3371: 3370: 3368: 3366: 3362: 3359: 3357: 3353: 3347: 3346: 3342: 3340: 3337: 3335: 3332: 3331: 3329: 3327: 3323: 3320: 3318: 3314: 3308: 3305: 3303: 3300: 3296: 3293: 3291: 3288: 3286: 3283: 3281: 3278: 3277: 3276: 3272: 3268: 3265: 3263: 3260: 3259: 3258: 3257:Asteroid belt 3255: 3251: 3250:Mars crossers 3248: 3247: 3245: 3241: 3238: 3236: 3233: 3231: 3228: 3226: 3223: 3221: 3218: 3217: 3216: 3213: 3209: 3206: 3204: 3201: 3199: 3196: 3195: 3193: 3189: 3186: 3184: 3181: 3179: 3176: 3174: 3171: 3169: 3168:Earth trojans 3166: 3164: 3161: 3160: 3159: 3156: 3155: 3153: 3151: 3147: 3141: 3138: 3136: 3133: 3131: 3130:Asteroid pair 3128: 3126: 3123: 3119: 3116: 3114: 3111: 3110: 3109: 3106: 3104: 3101: 3099: 3098:Earth-crosser 3096: 3094: 3091: 3089: 3086: 3084: 3081: 3077: 3074: 3073: 3072: 3069: 3067: 3064: 3063: 3061: 3057: 3053: 3046: 3041: 3039: 3034: 3032: 3027: 3026: 3023: 3017: 3014: 3012: 3009: 3008: 3004: 2989:on 2006-09-28 2988: 2984: 2978: 2975: 2972:. 2006-10-21. 2971: 2965: 2962: 2951:on 2006-09-02 2950: 2946: 2940: 2938: 2934: 2923:on 2006-09-02 2922: 2918: 2912: 2910: 2906: 2895:on 2000-08-17 2894: 2890: 2886: 2880: 2877: 2871: 2868: 2863: 2859: 2855: 2851: 2848:(1): 98ā€“105. 2847: 2843: 2839: 2835: 2829: 2826: 2822: 2818: 2812: 2809: 2804: 2800: 2796: 2795:Paris, France 2792: 2788: 2782: 2779: 2767: 2763: 2759: 2753: 2750: 2739:on 2006-09-02 2738: 2734: 2727: 2725: 2721: 2718:. 2006-06-18. 2717: 2711: 2709: 2705: 2694:on 2006-09-02 2693: 2689: 2683: 2680: 2675: 2671: 2670: 2665: 2661: 2657: 2650: 2647: 2640: 2638: 2636: 2613: 2609: 2606: 2603: 2596: 2591: 2587: 2579: 2578: 2577: 2563: 2543: 2534: 2532: 2531: 2526: 2522: 2518: 2514: 2510: 2506: 2502: 2500: 2496: 2488: 2486: 2483: 2469: 2466: 2463: 2440: 2437: 2428: 2425: 2422: 2410: 2405: 2401: 2399: 2398:asteroid belt 2393: 2379: 2372: 2356: 2349: 2341: 2339: 2322: 2300: 2274: 2270: 2265: 2262: 2255: 2254: 2253: 2250: 2242: 2240: 2238: 2220: 2197: 2187: 2184: 2181: 2177: 2171: 2153: 2150: 2146: 2138: 2137: 2136: 2133: 2119: 2096: 2091: 2086: 2081: 2078: 2074: 2066: 2065: 2064: 2062: 2054: 2052: 2050: 2045: 2031: 2028: 2025: 1999: 1996: 1988: 1985: 1980: 1976: 1972: 1969: 1962: 1958: 1951: 1948: 1945: 1935: 1932: 1925: 1924: 1923: 1895: 1891: 1877: 1868: 1850: 1842: 1826: 1818: 1798: 1795: 1787: 1782: 1779: 1771: 1760: 1757: 1753: 1749: 1746: 1743: 1740: 1717: 1706: 1702: 1698: 1695: 1690: 1686: 1682: 1679: 1676: 1659: 1651: 1650: 1649: 1647: 1642: 1640: 1624: 1621: 1618: 1610: 1594: 1586: 1560: 1556: 1552: 1549: 1546: 1541: 1537: 1528: 1510: 1502: 1498: 1480: 1457: 1449: 1445: 1441: 1438: 1431: 1427: 1423: 1418: 1414: 1407: 1404: 1401: 1392: 1378: 1370: 1369: 1368: 1366: 1362: 1358: 1350: 1345: 1343: 1337: 1283: 1279: 1232: 1228: 1193: 1185: 1184: 1183: 1180: 1166: 1146: 1143: 1140: 1137: 1134: 1112: 1092: 1072: 1049: 1046: 1043: 1040: 1035: 1030: 1025: 1021: 1018: 1012: 1007: 1004: 963: 955: 954: 953: 937: 930: 926: 922: 914: 912: 898: 886: 884: 870: 850: 842: 822: 819: 808: 803: 800: 792: 787: 774: 771: 767: 763: 760: 757: 754: 725: 721: 716: 713: 707: 672: 664: 663: 662: 648: 640: 632: 629: 621: 619: 616: 611: 593: 590: 579: 570: 567: 564: 555: 549: 547: 545: 541: 537: 533: 509: 505: 502: 499: 496: 493: 487: 484: 477: 476: 475: 460: 439: 429: 421: 397: 394: 385: 380: 376: 368: 363: 360: 353: 352: 332: 329: 323: 318: 315: 310: 304: 301: 298: 291: 290: 270: 267: 258: 253: 249: 241: 238: 235: 228: 227: 226: 207: 204: 195: 192: 189: 183: 180: 172: 156: 149: 148:mean diameter 131: 128: 123: 120: 97: 94: 89: 86: 66: 63: 60: 57: 54: 46: 41: 39: 34: 33:Per Magnusson 26: 24: 22: 3745:Minor planet 3710:Asteroid Day 3656:Colonization 3587: 3428: 3343: 3307:Exoasteroids 3262:Kirkwood gap 3173:Mars trojans 3163:Venus trojan 3150:Distribution 3070: 2991:. Retrieved 2987:the original 2977: 2969: 2964: 2953:. Retrieved 2949:the original 2925:. Retrieved 2921:the original 2897:. Retrieved 2893:the original 2879: 2870: 2845: 2841: 2828: 2820: 2811: 2790: 2781: 2770:. Retrieved 2766:the original 2752: 2741:. Retrieved 2737:the original 2730:For example 2715: 2696:. Retrieved 2692:the original 2682: 2669:Asteroids II 2668: 2649: 2631: 2535: 2528: 2503: 2492: 2484: 2406: 2402: 2394: 2345: 2292: 2248: 2246: 2237:eccentricity 2212: 2134: 2111: 2058: 2046: 2017: 1732: 1643: 1609:absorptivity 1472: 1354: 1341: 1181: 1064: 918: 890: 746: 661:is given by 636: 614: 612: 556: 553: 528: 431: 42: 30: 18: 3725:occultation 3633:Exploration 3588:small types 2660:Tom Gehrels 2556:and radius 2348:Bond albedo 2049:atmospheres 1869:. Equating 1501:Bond albedo 1365:temperature 3674:Near-Earth 3215:Near-Earth 3198:Vulcanoids 2993:2006-10-21 2955:2006-10-21 2927:2006-10-21 2899:2006-06-18 2772:2009-09-05 2743:2006-10-21 2698:2006-10-21 2672:. Tucson: 2641:References 2635:axial tilt 2509:lightcurve 1867:emissivity 426:See also: 27:Dimensions 3778:Asteroids 3052:Asteroids 2467:≈ 2426:− 2185:− 2026:ϵ 1989:σ 1986:ϵ 1973:π 1963:⊙ 1949:− 1851:ϵ 1796:− 1788:⋅ 1780:− 1772:⋅ 1758:− 1750:× 1744:≈ 1741:σ 1699:σ 1696:ϵ 1683:π 1639:isotropic 1622:− 1553:× 1547:≈ 1542:⊙ 1442:π 1424:π 1419:⊙ 1405:− 1141:θ 1138:⁡ 1113:θ 1050:θ 1047:⁡ 1022:π 1008:− 938:θ 820:− 809:⋅ 801:− 793:⋅ 772:− 764:× 758:≈ 591:− 580:⋅ 565:ρ 506:ρ 494:π 461:ρ 386:μ 377:ν 319:μ 316:ν 259:ν 250:μ 121:ν 87:μ 64:× 58:× 21:asteroids 3772:Category 3757:Category 3356:Spectral 3302:Centaurs 3088:Tracking 2789:(2004). 2666:(eds.). 1357:greybody 929:latitude 532:2 Pallas 38:Helsinki 3703:Related 3651:Capture 3603:Ld-type 3567:X-group 3513:S-group 3484:C-group 3405:X-group 3373:C-group 3326:Orbital 3158:Trojans 3118:contact 2850:Bibcode 2799:Bibcode 2235:is the 2055:Maximum 1841:kelvins 1815:is the 1583:is the 839:is the 550:Density 536:4 Vesta 3646:Mining 3613:V-type 3608:O-type 3598:D-type 3593:T-type 3572:X-type 3543:S-type 3538:L-type 3533:K-type 3528:R-type 3523:Q-type 3518:A-type 3494:C-type 3489:B-type 3464:V-type 3459:R-type 3454:Q-type 3449:T-type 3444:J-type 3439:D-type 3434:A-type 3420:P-type 3415:E-type 3410:M-type 3400:S-type 3393:C-type 3388:G-type 3383:F-type 3378:B-type 3365:Tholen 3345:(list) 3339:Family 3230:Apollo 3125:Active 3108:Binary 2842:Icarus 2293:where 2249:et al. 2213:where 2195:  2112:where 1843:, and 1733:where 1587:, and 1497:albedo 1473:where 1065:where 921:weight 747:where 615:et al. 534:, and 3740:Comet 3666:Lists 3476:SMASS 3334:Group 3235:Atira 2409:table 1550:3.827 761:6.674 3684:Lost 3225:Amor 3220:Aten 3113:moon 3059:Main 2889:NASA 2521:IRAS 2495:IRAS 2407:The 1747:5.67 1525:its 1351:Mean 540:Mars 422:Mass 3504:Cgh 2858:doi 2846:158 2819:, 2032:0.9 1611:is 1503:), 1179:'. 1135:sin 1044:sin 952:is 3774:: 3582:Xk 3579:Xc 3576:Xe 3559:Sl 3556:Sk 3553:Sr 3550:Sq 3547:Sa 3507:Cb 3501:Ch 3498:Cg 2936:^ 2908:^ 2887:. 2856:. 2844:. 2836:; 2723:^ 2707:^ 2662:; 2658:; 2637:. 2051:. 1970:16 1819:, 1754:10 1641:. 1561:26 1557:10 1529:, 843:, 775:11 768:10 546:. 113:, 3044:e 3037:t 3030:v 2996:. 2958:. 2930:. 2902:. 2864:. 2860:: 2852:: 2805:. 2801:: 2775:. 2746:. 2701:. 2614:r 2610:M 2607:G 2604:2 2597:= 2592:e 2588:v 2564:r 2544:g 2470:p 2464:A 2441:4 2438:1 2433:) 2429:A 2423:1 2420:( 2380:p 2357:A 2323:c 2301:d 2275:d 2271:c 2266:= 2263:T 2221:e 2198:T 2188:e 2182:1 2178:2 2172:= 2166:x 2163:a 2160:m 2154:s 2151:s 2147:T 2120:T 2097:T 2092:2 2087:= 2082:s 2079:s 2075:T 2029:= 2000:4 1997:1 1981:2 1977:a 1959:L 1955:) 1952:A 1946:1 1943:( 1936:= 1933:T 1907:t 1904:u 1901:o 1896:R 1892:= 1886:n 1883:i 1878:R 1827:T 1799:4 1792:K 1783:2 1776:m 1769:W 1761:8 1718:, 1707:4 1703:T 1691:2 1687:r 1680:4 1677:= 1671:t 1668:u 1665:o 1660:R 1625:A 1619:1 1595:r 1569:W 1538:L 1511:a 1481:A 1458:, 1450:2 1446:a 1439:4 1432:2 1428:r 1415:L 1411:) 1408:A 1402:1 1399:( 1393:= 1387:n 1384:i 1379:R 1319:l 1316:a 1313:g 1310:u 1307:f 1304:i 1301:r 1298:t 1295:n 1292:e 1289:c 1284:g 1280:+ 1274:l 1271:a 1268:n 1265:o 1262:i 1259:t 1256:a 1253:t 1250:i 1247:v 1244:a 1241:r 1238:g 1233:g 1229:= 1223:e 1220:v 1217:i 1214:t 1211:c 1208:e 1205:f 1202:f 1199:e 1194:g 1167:g 1147:1 1144:= 1093:r 1073:T 1041:r 1036:2 1031:) 1026:T 1019:2 1013:( 1005:= 999:l 996:a 993:g 990:u 987:f 984:i 981:r 978:t 975:n 972:e 969:c 964:g 899:g 871:r 851:M 823:1 816:g 812:k 804:2 797:s 788:3 784:m 755:G 726:2 722:r 717:M 714:G 708:= 702:l 699:a 696:c 693:i 690:r 687:e 684:h 681:p 678:s 673:g 649:g 594:3 587:m 583:c 577:g 571:2 568:= 510:6 503:c 500:b 497:a 488:= 485:M 440:M 398:3 395:1 390:) 381:2 373:( 369:d 364:= 361:c 333:3 330:1 324:) 311:( 305:d 302:= 299:b 271:3 268:1 263:) 254:2 246:( 242:d 239:= 236:a 208:3 205:1 200:) 196:c 193:b 190:a 187:( 184:= 181:d 157:d 132:c 129:b 124:= 98:b 95:a 90:= 67:c 61:b 55:a

Index

asteroids
Per Magnusson
Helsinki
triaxial ellipsoid
mean diameter
geometric mean
Dynamic method
2 Pallas
4 Vesta
Mars
Viking landers
Surface gravity
gravitational acceleration
gravitational constant
weight
centripetal force
latitude
greybody
solar radiation
temperature
albedo
Bond albedo
semi-major axis
solar luminosity
absorptivity
isotropic
Stefanā€“Boltzmann law
Stefanā€“Boltzmann constant
kelvins
emissivity

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