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511 Davida

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767: 741: 732: 29: 1379: 601: 586: 609: 1160: 756:: Double chord occultation of TYC 5597-01223 on 5 August 2016, observed by two amateur astronomers in eastern Australia. Both observers noted step events, thereby detecting the star has two components. 849: 1190: 655:. Conrad et al. (2007) show that craters of this size "can be expected from the impactor size distribution, without likelihood of catastrophic disruption of Davida." 770:
511 Davida occulted TYC 5597-01223 on 5 August 2016. Two observers recorded the event and both observed step events. Shown here is the step recording by Dave Herald.
173: 1518: 787:
Measurements of the short axis are less precise than the other two, but also involve a discrepancy between fitting the convolved and deconvolved images (
1453: 1304: 2035: 2000: 1161:"Determination of asteroid masses (6) Hebe, (10) Hygiea, (15) Eunomia, (52) Europa, (88) Thisbe, (444) Gyptis, (511) Davida and (704) Interamnia" 1315: 1795: 1003:
James Baer, Steven Chesley & Robert Matson (2011) "Astrometric masses of 26 asteroids and observations on asteroid porosity."
1511: 1271: 565:; approximately tied for 7th place, to within measurement uncertainties, and the 5th or 6th most massive. It was discovered by 2010: 1446: 1077: 131: 1479: 1400: 760:: Triple chord occultation of TYC 1964-00787, observed on 6 February 2009 by three astronomers in eastern United States. 2020: 1504: 1107: 2025: 1635: 1032:
P. Vernazza et al. (2021) VLT/SPHERE imaging survey of the largest main-belt asteroids: Final results and synthesis.
937: 1439: 41: 325: 1567: 531: 265: 1788: 1726: 562: 2015: 2005: 1552: 1462: 815: 1716: 1706: 1773: 1711: 1361: 1337: 1329: 766: 2030: 1781: 1547: 1353: 1345: 1320: 1731: 1615: 1527: 1373: 451: 364: 353: 303: 294: 254: 241: 1408: 1652: 625: 740: 731: 1557: 337: 1392: 1384: 1310: 1176: 1108:"High-Precision Ephemerides of Planets—EPM and Determination of Some Astronomical Constants" 1818: 1625: 1424: 1225: 1172: 1122: 749: 276: 1368: 8: 1050: 1046: 566: 314: 46: 1229: 1126: 1416: 1378: 590: 519: 143: 962: 1610: 1562: 720: 699:. This most recent estimate by Baer indicates that Davida is approximately tied with 247: 227: 28: 1279: 1736: 1233: 1180: 1130: 1103: 1081: 632: 220: 181: 81: 600: 1657: 1600: 1585: 1485: 1185: 967: 636: 621: 574: 570: 165: 123: 986: 620:
and comprises an estimated 1.5% of the total mass of the asteroid belt. It is a
1863: 1672: 1640: 1605: 700: 287: 1238: 1213: 1134: 1994: 1894: 1889: 1805: 1696: 1595: 1590: 651:. The facet is presumably a 150-km global-scale crater like the ones seen on 558: 1496: 1138: 1934: 1822: 1762: 1535: 652: 644: 640: 159: 1431: 1214:"Astrometric masses of 21 asteroids, and an integrated asteroid ephemeris" 1949: 1752: 1701: 1662: 1473: 716: 495: 1974: 1969: 1944: 1929: 1914: 1803: 1721: 1667: 381: 233: 585: 1964: 1959: 1954: 1924: 1919: 1909: 1899: 1868: 1858: 1757: 1647: 704: 648: 149: 1939: 1842: 1577: 617: 594: 554: 647:
and at least one flat facet with 15-km deviations from a best-fit
1837: 425: 719:
events observed since 1987, many of which produced two or three
675:. In 2007, Baer and Chesley estimated Davida to have a mass of 1979: 1904: 501: 462: 96: 1688: 883:"Baer Mass of 511 Davida" 0.220 / "Mass of Mbelt" 15 = 0.0146 1307:, IOTA – International Occultation Timing Association (2011) 612:
Keck telescope image sequence of Davida showing its rotation
938:"Asteroid 511 Davida – Nesvorny HCM Asteroid Families V3.0" 391: 205: 202: 187: 102: 87: 1224:(2008). Springer Science+Business Media B.V. 2007: 27–42. 1257: 1143: 608: 196: 812:
Flattening derived from the maximum aspect ratio (c/a):
1211: 818: 663:
In 2001, Michalak estimated Davida to have a mass of
208: 199: 193: 184: 99: 93: 84: 190: 90: 843: 624:, which means that it is dark in colouring with a 687:. As of 2010, Baer suggests Davida has a mass of 635:used the Keck II telescope, which is fitted with 1992: 923:John Daintith & William Gould, eds. (2006) 703:as the fifth-most-massive asteroid, though the 604:3D model of Davida based on lightcurve modeling 1016:Conrad (2007), as cited in Baer et al. (2011). 903:, per Michalak (2001), extended dynamic model. 639:, to photograph Davida. The asteroid is not a 1789: 1526: 1512: 1447: 1152: 1461: 1218:Celestial Mechanics and Dynamical Astronomy 616:Davida is approximately 270–310 km in 580: 1796: 1782: 1519: 1505: 1454: 1440: 1377: 1039: 1010: 999: 997: 995: 27: 1237: 1184: 1096: 925:The Facts On File Dictionary of Astronomy 1205: 1158: 765: 607: 599: 584: 2036:Astronomical objects discovered in 1903 2001:Minor planet object articles (numbered) 1212:Baer, James; Steven R. Chesley (2007). 1102: 1071: 1069: 1067: 992: 1993: 631:From 2002 to 2007, astronomers at the 1777: 1500: 1435: 1078:"Recent Asteroid Mass Determinations" 1028: 1026: 1024: 1022: 982: 980: 978: 930: 358:(357 ± 2) × (294 ± 2) × (231 ± 50) km 326:Longitude of ascending node 1075: 1064: 927:. 5th edition. Infobase Publishing. 589:Asteroid 511 Davida (lower left at 16:Large asteroid in the asteroid belt 13: 1080:. Personal Website. Archived from 1019: 975: 844:{\displaystyle f=1-{\frac {c}{a}}} 14: 2047: 1316:Al Conrad's research page at Keck 1298: 1325:AstDyS-2, Asteroids—Dynamic Site 1311:Time lapse photography of Davida 739: 730: 180: 80: 1264: 886: 877: 862: 710: 569:in 1903. Davida is named after 968:Merriam-Webster.com Dictionary 955: 917: 806: 781: 1: 910: 2011:Discoveries by Raymond Dugan 1165:Astronomy & Astrophysics 1034:Astronomy & Astrophysics 573:, an astronomy professor at 7: 1272:"PDS Asteroid/Dust Subnode" 1047:"Bright Minor Planets 2003" 723:. Two examples shown here. 338:Argument of perihelion 10: 2052: 1186:10.1051/0004-6361:20010731 795:), and fitting the edges ( 144:Minor planet category 2021:C-type asteroids (Tholen) 1877: 1851: 1830: 1814:Mean diameter 900–1000 km 1813: 1745: 1687: 1624: 1576: 1543: 1534: 1528:Small Solar System bodies 1469: 1239:10.1007/s10569-007-9103-8 1135:10.1007/s11208-005-0033-2 707:of Interamnia are large. 643:: there are at least two 544: 529: 517: 507: 494: 461: 449: 422: 390: 380: 362: 352: 347: 335: 323: 313: 301: 288:Orbital period (sidereal) 285: 275: 263: 253: 240: 226: 219: 172: 141: 129: 117: 75: 65: 60: 52: 40: 35: 26: 2026:C-type asteroids (SMASS) 1878:Mean diameter 200–300 km 1852:Mean diameter 300–500 km 1831:Mean diameter 500–600 km 1005:The Astronomical Journal 942:Small Bodies Data Ferret 774: 581:Physical characteristics 532:Absolute magnitude  348:Physical characteristics 236:2459396.5, heliocentric) 1463:Minor planets navigator 1374:JPL Small-Body Database 1177:2001A&A...374..703M 658: 452:Synodic rotation period 221:Orbital characteristics 1653:Trans-Neptunian object 1338:Observation prediction 1007:, Volume 141, Number 5 845: 771: 626:carbonaceous chondrite 613: 605: 597: 1305:Asteroid occultations 1159:Michalak, G. (2001). 1115:Solar System Research 846: 769: 611: 603: 588: 1808:greater than 200 km) 1626:Distant minor planet 1148:on October 31, 2008. 1076:Baer, James (2010). 989:Retrieved 2021-09-29 901:10 solar masses 868:(18.96 ± 0.99) × 10 816: 2016:Named minor planets 1425:Physical parameters 1230:2008CeMDA.100...27B 1193:on December 4, 2012 1127:2005SoSyR..39..176P 1051:Minor Planet Center 561:. It is one of the 53:Discovery date 23: 2006:Meliboea asteroids 1362:Observational info 971:. Merriam-Webster. 841: 772: 715:There have been 9 614: 606: 598: 593:12.5) near galaxy 553:is a large C-type 520:Apparent magnitude 457:0.2137 d (5.130 h) 42:Discovered by 21: 1988: 1987: 1804:Large asteroids ( 1771: 1770: 1683: 1682: 1568:Meanings of names 1494: 1493: 1282:on April 25, 2018 839: 563:largest asteroids 548: 547: 132:Alternative names 2043: 1798: 1791: 1784: 1775: 1774: 1541: 1540: 1521: 1514: 1507: 1498: 1497: 1456: 1449: 1442: 1433: 1432: 1417:Orbital elements 1381: 1292: 1291: 1289: 1287: 1278:. Archived from 1268: 1262: 1261: 1255: 1251: 1249: 1241: 1209: 1203: 1202: 1200: 1198: 1189:. Archived from 1188: 1156: 1150: 1149: 1147: 1137:. Archived from 1112: 1100: 1094: 1093: 1091: 1089: 1073: 1062: 1061: 1059: 1057: 1043: 1037: 1030: 1017: 1014: 1008: 1001: 990: 984: 973: 972: 959: 953: 952: 950: 948: 934: 928: 921: 904: 902: 900: 896: 890: 884: 881: 875: 866: 860: 858: 856: 851:, where (c/a) = 850: 848: 847: 842: 840: 832: 810: 804: 802: 800: 794: 792: 785: 743: 734: 698: 696: 692: 686: 684: 680: 674: 672: 668: 633:Keck Observatory 489: 487: 481: 479: 473: 471: 445: 443: 437: 435: 418: 416: 412: 406: 404: 400: 376: 374: 215: 214: 211: 210: 207: 204: 201: 198: 195: 192: 189: 186: 163: 109: 108: 105: 104: 101: 98: 95: 92: 89: 86: 31: 24: 20: 2051: 2050: 2046: 2045: 2044: 2042: 2041: 2040: 2031:1903 in science 1991: 1990: 1989: 1984: 1873: 1847: 1826: 1809: 1802: 1772: 1767: 1741: 1679: 1620: 1572: 1530: 1525: 1495: 1490: 1486:512 Taurinensis 1465: 1460: 1354:Proper elements 1301: 1296: 1295: 1285: 1283: 1270: 1269: 1265: 1253: 1247: 1245: 1210: 1206: 1196: 1194: 1157: 1153: 1141: 1110: 1101: 1097: 1087: 1085: 1084:on July 2, 2013 1074: 1065: 1055: 1053: 1045: 1044: 1040: 1031: 1020: 1015: 1011: 1002: 993: 985: 976: 961: 960: 956: 946: 944: 936: 935: 931: 922: 918: 913: 908: 907: 898: 894: 892: 891: 887: 882: 878: 874: 871: 867: 863: 854: 852: 831: 817: 814: 813: 811: 807: 798: 796: 790: 788: 786: 782: 777: 764: 763: 762: 761: 752:by 511 Davida: 746: 745: 744: 736: 735: 713: 694: 690: 688: 682: 678: 676: 670: 666: 664: 661: 637:adaptive optics 622:C-type asteroid 583: 575:Amherst College 571:David Peck Todd 537: 522: 510: 485: 483: 477: 475: 469: 467: 454: 441: 439: 438: 433: 431: 428: 414: 410: 408: 407: 402: 398: 396: 372: 370: 367: 340: 328: 306: 290: 268: 266:Semi-major axis 231: 183: 179: 164: 157: 146: 134: 124:David Peck Todd 120: 83: 79: 68: 17: 12: 11: 5: 2049: 2039: 2038: 2033: 2028: 2023: 2018: 2013: 2008: 2003: 1986: 1985: 1983: 1982: 1977: 1972: 1967: 1962: 1957: 1952: 1947: 1942: 1937: 1932: 1927: 1922: 1917: 1912: 1907: 1902: 1897: 1892: 1887: 1881: 1879: 1875: 1874: 1872: 1871: 1866: 1861: 1855: 1853: 1849: 1848: 1846: 1845: 1840: 1834: 1832: 1828: 1827: 1817: 1815: 1811: 1810: 1801: 1800: 1793: 1786: 1778: 1769: 1768: 1766: 1765: 1760: 1755: 1749: 1747: 1743: 1742: 1740: 1739: 1734: 1729: 1727:Near-parabolic 1724: 1719: 1714: 1709: 1704: 1699: 1693: 1691: 1685: 1684: 1681: 1680: 1678: 1677: 1676: 1675: 1673:Scattered disc 1670: 1665: 1660: 1650: 1645: 1644: 1643: 1641:Neptune trojan 1638: 1630: 1628: 1622: 1621: 1619: 1618: 1616:Spectral types 1613: 1608: 1606:Jupiter trojan 1603: 1598: 1593: 1588: 1582: 1580: 1574: 1573: 1571: 1570: 1565: 1560: 1555: 1550: 1544: 1538: 1532: 1531: 1524: 1523: 1516: 1509: 1501: 1492: 1491: 1489: 1488: 1483: 1476: 1470: 1467: 1466: 1459: 1458: 1451: 1444: 1436: 1430: 1429: 1428: 1427: 1385:Close approach 1366: 1365: 1364: 1318: 1313: 1308: 1300: 1299:External links 1297: 1294: 1293: 1263: 1204: 1151: 1104:Pitjeva, E. V. 1095: 1063: 1038: 1018: 1009: 991: 974: 954: 929: 915: 914: 912: 909: 906: 905: 885: 876: 872: 869: 861: 838: 835: 830: 827: 824: 821: 805: 779: 778: 776: 773: 748: 747: 738: 737: 729: 728: 727: 726: 725: 712: 709: 701:704 Interamnia 660: 657: 582: 579: 546: 545: 542: 541: 538: 530: 527: 526: 523: 518: 515: 514: 511: 508: 505: 504: 498: 492: 491: 465: 459: 458: 455: 450: 447: 446: 444:1.30 g/cm 436:0.53 g/cm 429: 423: 420: 419: 394: 388: 387: 384: 378: 377: 368: 363: 360: 359: 356: 350: 349: 345: 344: 341: 336: 333: 332: 329: 324: 321: 320: 317: 311: 310: 307: 302: 299: 298: 291: 286: 283: 282: 279: 273: 272: 269: 264: 261: 260: 257: 251: 250: 244: 238: 237: 230:July 01, 2021 224: 223: 217: 216: 176: 170: 169: 147: 142: 139: 138: 135: 130: 127: 126: 121: 118: 115: 114: 77: 73: 72: 69: 66: 63: 62: 58: 57: 54: 50: 49: 44: 38: 37: 33: 32: 15: 9: 6: 4: 3: 2: 2048: 2037: 2034: 2032: 2029: 2027: 2024: 2022: 2019: 2017: 2014: 2012: 2009: 2007: 2004: 2002: 1999: 1998: 1996: 1981: 1978: 1976: 1973: 1971: 1968: 1966: 1963: 1961: 1958: 1956: 1953: 1951: 1948: 1946: 1943: 1941: 1938: 1936: 1933: 1931: 1928: 1926: 1923: 1921: 1918: 1916: 1913: 1911: 1908: 1906: 1903: 1901: 1898: 1896: 1893: 1891: 1888: 1886: 1883: 1882: 1880: 1876: 1870: 1867: 1865: 1862: 1860: 1857: 1856: 1854: 1850: 1844: 1841: 1839: 1836: 1835: 1833: 1829: 1824: 1820: 1816: 1812: 1807: 1806:mean diameter 1799: 1794: 1792: 1787: 1785: 1780: 1779: 1776: 1764: 1761: 1759: 1756: 1754: 1751: 1750: 1748: 1744: 1738: 1735: 1733: 1730: 1728: 1725: 1723: 1720: 1718: 1715: 1713: 1710: 1708: 1705: 1703: 1700: 1698: 1695: 1694: 1692: 1690: 1686: 1674: 1671: 1669: 1666: 1664: 1661: 1659: 1656: 1655: 1654: 1651: 1649: 1646: 1642: 1639: 1637: 1634: 1633: 1632: 1631: 1629: 1627: 1623: 1617: 1614: 1612: 1609: 1607: 1604: 1602: 1599: 1597: 1596:Asteroid belt 1594: 1592: 1591:Aten asteroid 1589: 1587: 1584: 1583: 1581: 1579: 1575: 1569: 1566: 1564: 1561: 1559: 1556: 1554: 1551: 1549: 1546: 1545: 1542: 1539: 1537: 1536:Minor planets 1533: 1529: 1522: 1517: 1515: 1510: 1508: 1503: 1502: 1499: 1487: 1484: 1482: 1481: 1477: 1475: 1472: 1471: 1468: 1464: 1457: 1452: 1450: 1445: 1443: 1438: 1437: 1434: 1426: 1422: 1418: 1414: 1410: 1409:Orbit diagram 1406: 1402: 1398: 1394: 1390: 1386: 1383: 1382: 1380: 1376: 1375: 1370: 1367: 1363: 1359: 1355: 1351: 1347: 1343: 1339: 1335: 1331: 1328: 1327: 1326: 1322: 1319: 1317: 1314: 1312: 1309: 1306: 1303: 1302: 1281: 1277: 1273: 1267: 1260: 1259: 1240: 1235: 1231: 1227: 1223: 1219: 1215: 1208: 1192: 1187: 1182: 1178: 1174: 1170: 1166: 1162: 1155: 1145: 1140: 1136: 1132: 1128: 1124: 1120: 1116: 1109: 1105: 1099: 1083: 1079: 1072: 1070: 1068: 1052: 1048: 1042: 1035: 1029: 1027: 1025: 1023: 1013: 1006: 1000: 998: 996: 988: 983: 981: 979: 970: 969: 964: 958: 943: 939: 933: 926: 920: 916: 889: 880: 865: 836: 833: 828: 825: 822: 819: 809: 784: 780: 768: 759: 755: 751: 742: 733: 724: 722: 718: 708: 706: 702: 656: 654: 650: 646: 642: 638: 634: 629: 628:composition. 627: 623: 619: 610: 602: 596: 592: 587: 578: 576: 572: 568: 564: 560: 559:asteroid belt 556: 552: 543: 539: 536: 535: 528: 525:9.50 to 12.98 524: 521: 516: 512: 509:Spectral type 506: 503: 499: 497: 493: 466: 464: 460: 456: 453: 448: 430: 427: 421: 395: 393: 389: 385: 383: 379: 369: 366: 365:Mean diameter 361: 357: 355: 351: 346: 342: 339: 334: 330: 327: 322: 318: 316: 312: 308: 305: 300: 296: 292: 289: 284: 280: 278: 274: 270: 267: 262: 258: 256: 252: 249: 245: 243: 239: 235: 229: 225: 222: 218: 213: 177: 175: 171: 167: 161: 155: 151: 148: 145: 140: 136: 133: 128: 125: 122: 116: 113: 107: 78: 76:Pronunciation 74: 70: 64: 59: 55: 51: 48: 45: 43: 39: 34: 30: 25: 19: 1884: 1823:dwarf planet 1763:Space debris 1478: 1420: 1412: 1404: 1396: 1388: 1372: 1357: 1349: 1346:Orbital info 1341: 1333: 1324: 1284:. Retrieved 1280:the original 1275: 1266: 1258:solar masses 1243: 1221: 1217: 1207: 1195:. Retrieved 1191:the original 1168: 1164: 1154: 1139:the original 1118: 1114: 1098: 1088:February 13, 1086:. Retrieved 1082:the original 1054:. Retrieved 1041: 1033: 1012: 1004: 966: 957: 945:. Retrieved 941: 932: 924: 919: 888: 879: 864: 808: 783: 757: 753: 750:Occultations 714: 711:Occultations 662: 653:253 Mathilde 645:promontories 641:dwarf planet 630: 615: 550: 549: 533: 304:Mean anomaly 277:Eccentricity 153: 111: 71:(511) Davida 61:Designations 56:May 30, 1903 18: 1753:Cosmic dust 1717:Long-period 1707:Halley-type 1663:Kuiper belt 1548:Designation 1474:510 Mabella 1276:sbn.psi.edu 1197:November 4, 1171:: 703–711. 947:October 24, 801:114 km 717:occultation 567:R. S. Dugan 496:Temperature 474:geometric ( 315:Inclination 119:Named after 67:Designation 47:R. S. Dugan 1995:Categories 1890:Euphrosyne 1864:Interamnia 1758:Meteoroids 1737:Sungrazing 1712:Hyperbolic 1668:Oort cloud 1611:Near-Earth 1480:511 Davida 1369:511 Davida 1321:511 Davida 1121:(3): 176. 963:"Davidian" 911:References 793:40 km 705:error bars 697:10 kg 685:10 kg 673:10 kg 551:511 Davida 417:10 kg 405:10 kg 382:Flattening 354:Dimensions 255:Perihelion 174:Adjectives 22:511 Davida 1895:Patientia 1648:Damocloid 1401:Ephemeris 1393:Discovery 1330:Ephemeris 1286:April 27, 829:− 649:ellipsoid 375:4 km 178:Davidian 150:main-belt 36:Discovery 1935:Bamberga 1732:Periodic 1658:Detached 1578:Asteroid 1106:(2005). 987:JPL data 873:☉ 618:diameter 595:NGC 5792 555:asteroid 297:(2055 d) 271:3.163 AU 259:2.569 AU 242:Aphelion 166:Meliboea 110:, Latin 1975:Fortuna 1970:Eugenia 1950:Camilla 1915:Eunomia 1697:Extinct 1636:Centaur 1371:at the 1226:Bibcode 1173:Bibcode 1123:Bibcode 1056:May 21, 1036:54, A56 557:in the 426:density 168:  137:1903 LU 1965:Egeria 1960:Daphne 1955:Aurora 1945:Ursula 1930:Hektor 1925:Psyche 1920:Thisbe 1910:Cybele 1900:Sylvia 1885:Davida 1869:Europa 1859:Hygiea 1843:Pallas 1689:Comets 1601:Family 1586:Active 1553:Groups 1421:· 1419:  1413:· 1411:  1405:· 1403:  1397:· 1395:  1389:· 1387:  1358:· 1356:  1350:· 1348:  1342:· 1340:  1334:· 1332:  721:chords 463:Albedo 343:337.2° 331:107.6° 319:15.94° 293:5.626 246:3.759 154:· 152:  112:Dāvīda 1940:Doris 1838:Vesta 1819:Ceres 1746:Other 1702:Great 1423: 1415: 1407: 1399: 1391: 1360: 1352: 1344: 1336: 1111:(PDF) 897:0.28) 893:(3.34 775:Notes 758:Right 693:0.20) 689:(3.84 669:0.56) 665:(6.64 500:~160 488:0.020 484:0.363 480:0.013 476:0.717 472:0.007 468:0.076 424:Mean 397:(26.6 281:0.188 228:Epoch 160:outer 156: 1980:Iris 1905:Juno 1722:Lost 1563:Moon 1558:List 1288:2018 1250:0.30 1246:2.98 1199:2008 1090:2011 1058:2008 949:2019 857:0.06 853:0.70 754:Left 681:0.6) 677:(5.9 659:Mass 540:6.43 482:BV, 440:2.97 432:1.92 401:7.3) 392:Mass 386:0.30 309:113° 1821:(a 1323:at 1256:10 1234:doi 1222:100 1181:doi 1169:374 1144:PDF 1131:doi 797:191 789:241 591:mag 534:(H) 409:(38 371:298 1997:: 1274:. 1242:. 1232:. 1220:. 1216:. 1179:. 1167:. 1163:. 1129:. 1119:39 1117:. 1113:. 1066:^ 1049:. 1021:^ 994:^ 977:^ 965:. 940:. 803:). 577:. 413:2) 295:yr 248:AU 234:JD 97:iː 1825:) 1797:e 1790:t 1783:v 1520:e 1513:t 1506:v 1455:e 1448:t 1441:v 1290:. 1254:× 1252:) 1248:± 1244:( 1236:: 1228:: 1201:. 1183:: 1175:: 1146:) 1142:( 1133:: 1125:: 1092:. 1060:. 951:. 899:× 895:± 870:M 859:. 855:± 837:a 834:c 826:1 823:= 820:f 799:± 791:± 695:× 691:± 683:× 679:± 671:× 667:± 513:C 502:K 490:) 486:± 478:± 470:± 442:± 434:± 415:× 411:± 403:× 399:± 373:± 232:( 212:/ 209:n 206:ə 203:i 200:d 197:ɪ 194:v 191:ˈ 188:ə 185:d 182:/ 162:) 158:( 106:/ 103:ə 100:d 94:v 91:ˈ 88:ə 85:d 82:/

Index


Discovered by
R. S. Dugan
/dəˈvdə/
David Peck Todd
Alternative names
Minor planet category
main-belt
outer
Meliboea
Adjectives
/dəˈvɪdiən/
Orbital characteristics
Epoch
JD
Aphelion
AU
Perihelion
Semi-major axis
Eccentricity
Orbital period (sidereal)
yr
Mean anomaly
Inclination
Longitude of ascending node
Argument of perihelion
Dimensions
Mean diameter
Flattening
Mass

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