29:
1779:
633:
222:
727:
and relationship to the parent body. Computer simulations of the collision are more consistent with
Eunomia being a re-accumulation of most of the fragments of a completely shattered parent body, yet Eunomia's quite high density would indicate that it is not a rubble pile after all. Whatever the case in this respect, it appears that any metallic core region, if present, has not been exposed.
726:
Altogether, these lines of evidence suggest that
Eunomia is the central remnant of the parent body of the Eunomia family, which was stripped of most of its crustal material by the disrupting impact, but was perhaps not disrupted itself. However, there is uncertainty over Eunomia's internal structure
730:
An older explanation of the compositional differences, that
Eunomia is a mantle fragment of a far larger parent body (with a bit of crust on one end, and a bit of core on the other), appears to be ruled out by studies of the mass distribution of the entire Eunomia family. These indicate that the
699:
studies suggest that
Eunomia has regions with differing compositions: A larger region dominated by olivine, which is pyroxene-poor and metal-rich, and another somewhat smaller region on one hemisphere (the less pointed end) that is noticeably richer in pyroxene, and has a generally
719:, formed by a collision of the common parent body, is large enough to encompass all the surface variations on Eunomia itself. The majority of smaller Eunomian asteroids are more pyroxene rich than Eunomia's surface, and contain very few metallic (
651:
Eunomia appears to be an elongated but fairly regularly shaped body, with what appear to be four sides of differing curvature and noticeably different average compositions. Its elongation led to the suggestion that
Eunomia may be a
738:
These indications are also in accord with recent mass determinations which indicate that
Eunomia's density is typical of mostly intact stony asteroids, and not the anomalously low "rubble pile" density of
1623:
Evolution and source regions of asteroids and comets : proceedings of the 173rd colloquium of the
International Astronomical Union, held in Tatranska Lomnica, Slovak Republic, August 24–28, 1998
168:
919:
1918:
1853:
2430:
2400:
2410:
1692:
359:
2195:
1911:
58:
1846:
2420:
1904:
1879:
2425:
2035:
1142:
1839:
41:
336:
799:
for this asteroid is 25,000 years, indicating that it occupies a chaotic orbit that will change randomly over time because of
1967:
657:
276:
731:
largest fragment (that is, Eunomia) has about 70% of the mass of the parent body, which is consistent with
Eunomia being a
2188:
2126:
596:
2415:
1800:
1203:
1952:
1621:Šidlichovský, M. (1999), Svoren, J.; Pittich, E. M.; Rickman, H. (eds.), "Resonances and chaos in the asteroid belt",
1371:
1107:
P. Vernazza et al. (2021) VLT/SPHERE imaging survey of the largest main-belt asteroids: Final results and synthesis.
2405:
2116:
2106:
800:
752:
661:
2111:
993:
53:
2181:
1947:
792:
79:
1696:
2131:
2015:
1927:
1773:
1646:
998:
519:
470:
379:
366:
305:
265:
251:
2052:
1710:
1506:
814:
1957:
1862:
885:
780:
348:
28:
2173:
1462:; Benz, Willy; Richardson, Derek C. (2004). "Catastrophic disruption of pre-shattered parent bodies".
2218:
2025:
1626:
1560:
1518:
1471:
1433:
1380:
1218:
1171:
1063:
607:
287:
46:
1761:
1737:
1729:
1600:
788:
325:
1547:
Tanga, P.; Hestroffer, D.; Cellino, A.; Lattanzi, M.; Martino, M. Di; Zappalà, V. (1 April 2003).
1271:
1753:
1745:
1720:
1714:
1487:
1421:
1398:
1362:
1234:
1081:
817:
545:
533:
1808:
1134:
1123:
632:
2010:
1962:
1578:
1417:
1204:"High-Precision Ephemerides of Planets – EPM and Determination of Some Astronomical Constants"
1160:"New mass determination of (15) Eunomia based on a very close encounter with (50278) 2000CZ12"
1138:
843:
611:
257:
237:
136:
1596:
1006:
648:
being a very close second), Eunomia has attracted a moderate amount of scientific attention.
2136:
1792:
1784:
1568:
1564:
1526:
1479:
1441:
1388:
1384:
1341:
1226:
1199:
1179:
1175:
1130:
1071:
560:
482:
230:
176:
95:
1824:
2057:
2000:
1985:
1768:
1650:
720:
653:
623:
588:
525:
1687:
shape model deduced from lightcurve, including composition variations across the surface
1662:
1630:
1522:
1475:
1437:
1222:
1067:
2263:
2072:
2040:
2005:
1816:
1778:
1459:
716:
600:
298:
215:
158:
1076:
1051:
221:
2394:
2294:
2289:
2205:
2096:
1995:
1990:
1505:
Tanga, P.; Cellino, A.; Michel, P.; Zappalà, V.; Paolicchi, P.; Dell'Oro, A. (1999).
1238:
1085:
796:
712:
584:
1491:
987:
715:
in the early period of the Solar System. The range of compositions of the remaining
2334:
2222:
2162:
1935:
1402:
825:
696:
314:
144:
1573:
1548:
1483:
1393:
1366:
1345:
1184:
1159:
1030:
626:. Its historical symbol is a heart with a star on top; it is in the pipeline for
2349:
2152:
2101:
2062:
807:
711:
processes, and became at least partially differentiated under the influence of
599:, in 6th to 8th place (to within measurement uncertainties). It is the largest
2374:
2369:
2344:
2329:
2284:
2121:
2067:
1686:
1230:
829:
768:
760:
756:
665:
400:
243:
1582:
2364:
2359:
2354:
2324:
2319:
2309:
2299:
2268:
2258:
2157:
2047:
1896:
1885:
1242:
847:
153:
1530:
1445:
1831:
1332:
Nathues, Andreas (2005). "Spectral study of the
Eunomia asteroid family".
1301:
1052:"Astrometric Masses of 26 Asteroids and Observations on Asteroid Porosity"
2339:
2242:
1977:
1873:
1258:
Eunomia 0.164E−11 solar masses; asteroid belt 15E−11 solar masses → 1.1%.
695:, along with nickel-iron metal, have been detected on Eunomia's surface.
688:
672:
580:
2237:
764:
692:
684:
627:
444:
707:
This composition indicates that the parent body was likely subject to
2379:
2304:
1507:"On the Size Distribution of Asteroid Families: The Role of Geometry"
863:
701:
676:
645:
592:
603:, and is estimated to contain 1% of the mass of the asteroid belt.
2088:
708:
671:
Like other true members of the family, its surface is composed of
615:
851:
821:
810:
784:
680:
410:
2177:
1900:
1835:
619:
1643:
735:
remnant, with the crust and part of the mantle stripped off.
182:
101:
1549:"Asteroid observations with the Hubble Space Telescope FGS"
1367:"Asteroid observations with the Hubble Space Telescope FGS"
1050:
Baer, James; Chesley, Steven R.; Matson, Robert D. (2011).
200:
197:
191:
119:
116:
110:
664:(β, λ) = (−65°, 2°) with a 10° uncertainty. This gives an
179:
98:
882:
Flattening derived from the maximum aspect ratio (c/a):
751:
15 Eunomia was in study of asteroids using the Hubble
1270:
Bala, Gavin Jared; Miller, Kirk (18 September 2023).
888:
203:
188:
107:
1422:"Shape and Albedo Variations of Asteroid 15 Eunomia"
2277:
2251:
2230:
2213:
2145:
2087:
2024:
1976:
1934:
558:
543:
531:
517:
480:
468:
441:
409:
399:
377:
365:
358:
346:
334:
324:
312:
296:
286:
274:
264:
250:
229:
214:
194:
185:
167:
142:
130:
113:
104:
89:
77:
72:
64:
52:
40:
35:
1122:
986:
913:
1272:"Unicode request for historical asteroid symbols"
1542:
1540:
1121:Donald H. Menzel & Jay M. Pasachoff (1983).
975:A Practical Dictionary of the English Language
2189:
1912:
1847:
8:
1663:"JPL Close-Approach Data: 50278 (2000 CZ12)"
1327:
1325:
1323:
779:The orbit of 15 Eunomia places it in a 7:16
21:
656:object, but this has been refuted. It is a
2196:
2182:
2174:
1940:
1919:
1905:
1897:
1854:
1840:
1832:
1777:
1357:
1355:
1158:Vitagliano, Aldo; Reiner M. Stoss (2006).
1045:
1043:
1041:
1039:
27:
1693:"Elements and Ephemeris for (15) Eunomia"
1572:
1392:
1183:
1075:
901:
887:
618:(Hours), a personification of order and
2431:Astronomical objects discovered in 1851
2401:Minor planet object articles (numbered)
1302:"Proposed New Characters: The Pipeline"
966:
875:
660:rotator with its pole pointing towards
1125:A Field Guide to the Stars and Planets
20:
1695:. Minor Planet Center. Archived from
1103:
1101:
1099:
1097:
1095:
1026:
1024:
1022:
1020:
1018:
1016:
644:As the largest S-type asteroid (with
337:Longitude of ascending node
7:
1007:participating institution membership
2411:Discoveries by Annibale de Gasparis
1782:
914:{\displaystyle f=1-{\frac {c}{a}}}
610:on July 29, 1851, and named after
587:. It is the largest of the stony (
14:
854:) from Eunomia on March 4, 2002.
595:as a close second. It is quite a
1725:AstDyS-2, Asteroids—Dynamic Site
864:Former classification of planets
743:that had been reported earlier.
631:
220:
175:
94:
828:, and can reach +7.9 at a near
372:(357 × 255 × 212) ± 15 km
1:
1420:; Lebofsky, Larry A. (1997).
1553:Astronomy & Astrophysics
1484:10.1016/J.ICARUS.2003.12.011
1372:Astronomy & Astrophysics
1346:10.1016/j.icarus.2004.12.013
1129:(2nd ed.). Boston, MA:
1109:Astronomy & Astrophysics
820:of +8.5, about equal to the
813:three times. It has a mean
755:. Asteroids studied include
476:6.083 h (0.2535 d)
1077:10.1088/0004-6256/141/5/143
801:gravitational perturbations
349:Argument of perihelion
282:2.644 AU (395 Gm)
2447:
1574:10.1051/0004-6361:20030032
1394:10.1051/0004-6361:20030032
1185:10.1051/0004-6361:20065760
1164:Astronomy and Astrophysics
842:passed about 0.00037
806:Eunomia has been observed
606:Eunomia was discovered by
270:2.15 AU (321 Gm)
145:Minor planet category
2421:S-type asteroids (Tholen)
2214:Mean diameter 900–1000 km
1943:
1928:Small Solar System bodies
1869:
1231:10.1007/s11208-005-0033-2
994:Oxford English Dictionary
787:. Eunomia is used by the
570:
299:Orbital period (sidereal)
236:
26:
2426:S-type asteroids (SMASS)
2278:Mean diameter 200–300 km
2252:Mean diameter 300–500 km
2231:Mean diameter 500–600 km
1308:. The Unicode Consortium
1056:The Astronomical Journal
546:Absolute magnitude
360:Physical characteristics
246:2459396.5, heliocentric)
1863:Minor planets navigator
1774:JPL Small-Body Database
1644:The Brightest Asteroids
1565:2003A&A...401..733T
1385:2003A&A...401..733T
1176:2006A&A...455L..29V
999:Oxford University Press
683:, and is quite bright.
471:Synodic rotation period
231:Orbital characteristics
2053:Trans-Neptunian object
1738:Observation prediction
1531:10.1006/icar.1999.6148
1446:10.1006/icar.1996.5627
915:
1211:Solar System Research
916:
781:mean-motion resonance
2208:greater than 200 km)
2026:Distant minor planet
1625:, pp. 297–308,
1033:Retrieved 2021-09-29
973:Noah Webster (1884)
886:
662:ecliptic coordinates
630:17.0 as U+1CEC8 (
608:Annibale de Gasparis
80:MPC designation
47:Annibale de Gasparis
2416:Named minor planets
1825:Physical parameters
1631:1999esra.conf..297S
1601:Minor Planet Center
1597:"Perturbing Bodies"
1523:1999Icar..141...65T
1476:2004Icar..168..420M
1438:1997Icar..125..446R
1223:2005SoSyR..39..176P
1068:2011AJ....141..143B
997:(Online ed.).
789:Minor Planet Center
65:Discovery date
54:Discovery site
23:
1762:Observational info
1649:2008-05-11 at the
1418:Gaffey, Michael J.
1248:on 31 October 2008
911:
717:Eunomian asteroids
591:) asteroids, with
534:Apparent magnitude
395:231.689 ± 2.234 km
42:Discovered by
16:Main-belt asteroid
2406:Eunomia asteroids
2388:
2387:
2204:Large asteroids (
2171:
2170:
2083:
2082:
1968:Meanings of names
1894:
1893:
1005:(Subscription or
909:
759:, (15) Eunomia,
601:Eunomian asteroid
574:
573:
2438:
2198:
2191:
2184:
2175:
1941:
1921:
1914:
1907:
1898:
1856:
1849:
1842:
1833:
1817:Orbital elements
1781:
1708:
1706:
1704:
1675:
1674:
1672:
1670:
1659:
1653:
1641:
1635:
1634:
1618:
1612:
1611:
1609:
1607:
1593:
1587:
1586:
1576:
1544:
1535:
1534:
1502:
1496:
1495:
1456:
1450:
1449:
1416:Reed, Kevin L.;
1413:
1407:
1406:
1396:
1359:
1350:
1349:
1329:
1318:
1317:
1315:
1313:
1297:
1291:
1290:
1288:
1286:
1276:
1267:
1261:
1260:
1255:
1253:
1247:
1241:. Archived from
1208:
1196:
1190:
1189:
1187:
1155:
1149:
1148:
1131:Houghton Mifflin
1128:
1118:
1112:
1105:
1090:
1089:
1079:
1047:
1034:
1028:
1011:
1010:
1002:
990:
983:
977:
971:
955:
954:
946:
942:
936:
930:
928:
926:
921:, where (c/a) =
920:
918:
917:
912:
910:
902:
880:
841:
803:of the planets.
783:with the planet
742:
713:internal heating
635:
597:massive asteroid
579:is a very large
561:Angular diameter
512:
510:
504:
502:
496:
494:
483:Geometric albedo
464:
462:
456:
454:
437:
435:
431:
425:
423:
419:
391:
389:
373:
224:
210:
209:
206:
205:
202:
199:
196:
193:
190:
187:
184:
181:
126:
125:
122:
121:
118:
115:
112:
109:
106:
103:
100:
31:
24:
2446:
2445:
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2440:
2439:
2437:
2436:
2435:
2391:
2390:
2389:
2384:
2273:
2247:
2226:
2209:
2202:
2172:
2167:
2141:
2079:
2020:
1972:
1930:
1925:
1895:
1890:
1865:
1860:
1754:Proper elements
1702:
1700:
1699:on 3 March 2016
1691:
1683:
1678:
1668:
1666:
1661:
1660:
1656:
1651:Wayback Machine
1642:
1638:
1620:
1619:
1615:
1605:
1603:
1595:
1594:
1590:
1546:
1545:
1538:
1504:
1503:
1499:
1460:Michel, Patrick
1458:
1457:
1453:
1415:
1414:
1410:
1361:
1360:
1353:
1331:
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1321:
1311:
1309:
1299:
1298:
1294:
1284:
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1274:
1269:
1268:
1264:
1251:
1249:
1245:
1206:
1198:
1197:
1193:
1157:
1156:
1152:
1145:
1120:
1119:
1115:
1106:
1093:
1049:
1048:
1037:
1029:
1014:
1004:
985:
984:
980:
972:
968:
964:
959:
958:
953:
950:
944:
940:
938:
937:
933:
924:
922:
884:
883:
881:
877:
872:
860:
840:
837:(50278) 2000 CZ
836:
795:. The computed
777:
749:
740:
668:of about 165°.
642:
640:Characteristics
624:Greek mythology
566:0.29″ to 0.085″
563:
551:
536:
526:S-type asteroid
522:
508:
506:
500:
498:
492:
490:
489:
485:
473:
460:
458:
457:
452:
450:
447:
433:
429:
427:
426:
421:
417:
415:
394:
392:
387:
385:
382:
371:
351:
339:
317:
301:
279:
277:Semi-major axis
241:
178:
174:
163:
147:
133:
97:
93:
82:
17:
12:
11:
5:
2444:
2442:
2434:
2433:
2428:
2423:
2418:
2413:
2408:
2403:
2393:
2392:
2386:
2385:
2383:
2382:
2377:
2372:
2367:
2362:
2357:
2352:
2347:
2342:
2337:
2332:
2327:
2322:
2317:
2312:
2307:
2302:
2297:
2292:
2287:
2281:
2279:
2275:
2274:
2272:
2271:
2266:
2261:
2255:
2253:
2249:
2248:
2246:
2245:
2240:
2234:
2232:
2228:
2227:
2217:
2215:
2211:
2210:
2203:
2201:
2200:
2193:
2186:
2178:
2169:
2168:
2166:
2165:
2160:
2155:
2149:
2147:
2143:
2142:
2140:
2139:
2134:
2129:
2127:Near-parabolic
2124:
2119:
2114:
2109:
2104:
2099:
2093:
2091:
2085:
2084:
2081:
2080:
2078:
2077:
2076:
2075:
2073:Scattered disc
2070:
2065:
2060:
2050:
2045:
2044:
2043:
2041:Neptune trojan
2038:
2030:
2028:
2022:
2021:
2019:
2018:
2016:Spectral types
2013:
2008:
2006:Jupiter trojan
2003:
1998:
1993:
1988:
1982:
1980:
1974:
1973:
1971:
1970:
1965:
1960:
1955:
1950:
1944:
1938:
1932:
1931:
1926:
1924:
1923:
1916:
1909:
1901:
1892:
1891:
1889:
1888:
1883:
1876:
1870:
1867:
1866:
1861:
1859:
1858:
1851:
1844:
1836:
1830:
1829:
1828:
1827:
1785:Close approach
1766:
1765:
1764:
1718:
1689:
1682:
1681:External links
1679:
1677:
1676:
1654:
1636:
1613:
1588:
1559:(2): 733–741.
1536:
1497:
1470:(2): 420–432.
1451:
1408:
1379:(2): 733–741.
1351:
1340:(2): 452–463.
1319:
1292:
1262:
1217:(3): 176–186.
1200:Pitjeva, E. V.
1191:
1170:(3): L29–L31.
1150:
1143:
1113:
1091:
1035:
1012:
978:
965:
963:
960:
957:
956:
951:
948:
931:
908:
905:
900:
897:
894:
891:
874:
873:
871:
868:
867:
866:
859:
856:
850:; 34,000
838:
824:brightness of
776:
773:
748:
745:
641:
638:
583:in the middle
572:
571:
568:
567:
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559:
556:
555:
552:
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541:
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532:
529:
528:
523:
518:
515:
514:
486:
481:
478:
477:
474:
469:
466:
465:
463:0.53 g/cm
455:0.21 g/cm
448:
442:
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413:
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403:
397:
396:
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240:July 01, 2021
234:
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211:
171:
165:
164:
162:
161:
159:Eunomia family
156:
150:
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143:
140:
139:
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131:
128:
127:
91:
87:
86:
83:
78:
75:
74:
70:
69:
66:
62:
61:
56:
50:
49:
44:
38:
37:
33:
32:
15:
13:
10:
9:
6:
4:
3:
2:
2443:
2432:
2429:
2427:
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2419:
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2414:
2412:
2409:
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2399:
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2381:
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2328:
2326:
2323:
2321:
2318:
2316:
2313:
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2308:
2306:
2303:
2301:
2298:
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2291:
2288:
2286:
2283:
2282:
2280:
2276:
2270:
2267:
2265:
2262:
2260:
2257:
2256:
2254:
2250:
2244:
2241:
2239:
2236:
2235:
2233:
2229:
2224:
2220:
2216:
2212:
2207:
2206:mean diameter
2199:
2194:
2192:
2187:
2185:
2180:
2179:
2176:
2164:
2161:
2159:
2156:
2154:
2151:
2150:
2148:
2144:
2138:
2135:
2133:
2130:
2128:
2125:
2123:
2120:
2118:
2115:
2113:
2110:
2108:
2105:
2103:
2100:
2098:
2095:
2094:
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2090:
2086:
2074:
2071:
2069:
2066:
2064:
2061:
2059:
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2055:
2054:
2051:
2049:
2046:
2042:
2039:
2037:
2034:
2033:
2032:
2031:
2029:
2027:
2023:
2017:
2014:
2012:
2009:
2007:
2004:
2002:
1999:
1997:
1996:Asteroid belt
1994:
1992:
1991:Aten asteroid
1989:
1987:
1984:
1983:
1981:
1979:
1975:
1969:
1966:
1964:
1961:
1959:
1956:
1954:
1951:
1949:
1946:
1945:
1942:
1939:
1937:
1936:Minor planets
1933:
1929:
1922:
1917:
1915:
1910:
1908:
1903:
1902:
1899:
1887:
1884:
1882:
1881:
1877:
1875:
1872:
1871:
1868:
1864:
1857:
1852:
1850:
1845:
1843:
1838:
1837:
1834:
1826:
1822:
1818:
1814:
1810:
1809:Orbit diagram
1806:
1802:
1798:
1794:
1790:
1786:
1783:
1780:
1776:
1775:
1770:
1767:
1763:
1759:
1755:
1751:
1747:
1743:
1739:
1735:
1731:
1728:
1727:
1726:
1722:
1719:
1716:
1713:from Sun and
1712:
1698:
1694:
1690:
1688:
1685:
1684:
1680:
1665:. 31 May 2013
1664:
1658:
1655:
1652:
1648:
1645:
1640:
1637:
1632:
1628:
1624:
1617:
1614:
1602:
1598:
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1584:
1580:
1575:
1570:
1566:
1562:
1558:
1554:
1550:
1543:
1541:
1537:
1532:
1528:
1524:
1520:
1516:
1512:
1508:
1501:
1498:
1493:
1489:
1485:
1481:
1477:
1473:
1469:
1465:
1461:
1455:
1452:
1447:
1443:
1439:
1435:
1431:
1427:
1423:
1419:
1412:
1409:
1404:
1400:
1395:
1390:
1386:
1382:
1378:
1374:
1373:
1368:
1364:
1358:
1356:
1352:
1347:
1343:
1339:
1335:
1328:
1326:
1324:
1320:
1307:
1303:
1296:
1293:
1280:
1273:
1266:
1263:
1259:
1244:
1240:
1236:
1232:
1228:
1224:
1220:
1216:
1212:
1205:
1201:
1195:
1192:
1186:
1181:
1177:
1173:
1169:
1165:
1161:
1154:
1151:
1146:
1144:0-395-34835-8
1140:
1136:
1132:
1127:
1126:
1117:
1114:
1110:
1104:
1102:
1100:
1098:
1096:
1092:
1087:
1083:
1078:
1073:
1069:
1065:
1061:
1057:
1053:
1046:
1044:
1042:
1040:
1036:
1032:
1027:
1025:
1023:
1021:
1019:
1017:
1013:
1008:
1000:
996:
995:
989:
982:
979:
976:
970:
967:
961:
935:
932:
906:
903:
898:
895:
892:
889:
879:
876:
869:
865:
862:
861:
857:
855:
853:
849:
846:(55,000
845:
833:
831:
827:
823:
819:
816:
812:
809:
804:
802:
798:
797:Lyapunov time
794:
793:perturbations
791:to calculate
790:
786:
782:
774:
772:
770:
766:
762:
758:
754:
746:
744:
736:
734:
728:
724:
722:
718:
714:
710:
705:
704:composition.
703:
698:
697:Spectroscopic
694:
690:
686:
682:
678:
674:
669:
667:
663:
659:
655:
649:
647:
639:
637:
634:
629:
625:
621:
617:
614:, one of the
613:
609:
604:
602:
598:
594:
590:
586:
585:asteroid belt
582:
578:
569:
565:
562:
557:
553:
550:
549:
542:
538:
535:
530:
527:
524:
521:
520:Spectral type
516:
487:
484:
479:
475:
472:
467:
449:
446:
440:
414:
412:
408:
404:
402:
398:
384:
381:
380:Mean diameter
376:
370:
368:
364:
361:
357:
353:
350:
345:
341:
338:
333:
329:
327:
323:
319:
316:
311:
308:(1571 d)
307:
303:
300:
295:
291:
289:
285:
281:
278:
273:
269:
267:
263:
260:(469 Gm)
259:
255:
253:
249:
245:
239:
235:
232:
228:
223:
219:
217:
213:
208:
172:
170:
166:
160:
157:
155:
152:
151:
149:
146:
141:
138:
135:
129:
124:
92:
90:Pronunciation
88:
84:
81:
76:
71:
67:
63:
60:
57:
55:
51:
48:
45:
43:
39:
34:
30:
25:
19:
2314:
2223:dwarf planet
2163:Space debris
1878:
1820:
1812:
1804:
1796:
1788:
1772:
1757:
1749:
1746:Orbital info
1741:
1733:
1724:
1701:. Retrieved
1697:the original
1667:. Retrieved
1657:
1639:
1622:
1616:
1604:. Retrieved
1591:
1556:
1552:
1517:(1): 65–78.
1514:
1510:
1500:
1467:
1463:
1454:
1429:
1425:
1411:
1376:
1370:
1363:Tanga, Paolo
1337:
1333:
1310:. Retrieved
1305:
1295:
1285:26 September
1283:. Retrieved
1278:
1265:
1257:
1250:. Retrieved
1243:the original
1214:
1210:
1194:
1167:
1163:
1153:
1124:
1116:
1108:
1059:
1055:
992:
981:
974:
969:
934:
878:
834:
832:opposition.
805:
778:
769:(624) Hektor
761:(43) Ariadne
757:(63) Ausonia
750:
737:
732:
729:
725:
706:
670:
650:
643:
605:
576:
575:
547:
539:7.9 to 11.24
315:Mean anomaly
288:Eccentricity
225:(historical)
85:(15) Eunomia
73:Designations
68:29 July 1851
18:
2153:Cosmic dust
2117:Long-period
2107:Halley-type
2063:Kuiper belt
1948:Designation
1669:8 September
1306:unicode.org
1279:unicode.org
1252:18 November
1133:. pp.
741:1 g/cm
497:geometric (
393:268 km
326:Inclination
132:Named after
59:Naples Obs.
2395:Categories
2290:Euphrosyne
2264:Interamnia
2158:Meteoroids
2137:Sungrazing
2112:Hyperbolic
2068:Oort cloud
2011:Near-Earth
1880:15 Eunomia
1769:15 Eunomia
1721:15 Eunomia
1709:(displays
1432:(2): 446.
1312:6 November
1062:(5): 143.
1009:required.)
988:"Eunomian"
962:References
830:perihelion
815:opposition
723:) bodies.
666:axial tilt
658:retrograde
577:15 Eunomia
436:10 kg
424:10 kg
401:Flattening
367:Dimensions
304:4.30
266:Perihelion
256:3.14
169:Adjectives
22:15 Eunomia
2295:Patientia
2048:Damocloid
1886:16 Psyche
1874:14 Irene
1801:Ephemeris
1793:Discovery
1730:Ephemeris
1717:for 2011)
1583:0004-6361
1300:Unicode.
1281:. Unicode
1239:120467483
1086:121625885
899:−
835:Asteroid
818:magnitude
808:occulting
765:(44) Nysa
689:pyroxenes
675:and some
673:silicates
390:3 km
173:Eunomian
154:Main belt
36:Discovery
2335:Bamberga
2132:Periodic
2058:Detached
1978:Asteroid
1647:Archived
1606:18 April
1492:18834098
1365:(2003).
1202:(2005).
1031:JPL data
952:☉
947:10
858:See also
709:magmatic
702:basaltic
581:asteroid
252:Aphelion
2375:Fortuna
2370:Eugenia
2350:Camilla
2315:Eunomia
2097:Extinct
2036:Centaur
1771:at the
1627:Bibcode
1561:Bibcode
1519:Bibcode
1472:Bibcode
1434:Bibcode
1403:8977642
1381:Bibcode
1219:Bibcode
1172:Bibcode
1111:54, A56
1064:Bibcode
747:Studies
733:central
693:olivine
685:Calcium
628:Unicode
612:Eunomia
445:density
137:Eunomia
2365:Egeria
2360:Daphne
2355:Aurora
2345:Ursula
2330:Hektor
2325:Psyche
2320:Thisbe
2310:Cybele
2300:Sylvia
2285:Davida
2269:Europa
2259:Hygiea
2243:Pallas
2089:Comets
2001:Family
1986:Active
1953:Groups
1821:·
1819:
1813:·
1811:
1805:·
1803:
1797:·
1795:
1789:·
1787:
1758:·
1756:
1750:·
1748:
1742:·
1740:
1734:·
1732:
1703:26 May
1581:
1511:Icarus
1490:
1464:Icarus
1426:Icarus
1401:
1334:Icarus
1237:
1141:
1084:
939:(15.97
767:, and
721:M-type
687:-rich
677:nickel
654:binary
646:3 Juno
593:3 Juno
589:S-type
330:11.75°
216:Symbol
2340:Doris
2238:Vesta
2219:Ceres
2146:Other
2102:Great
1823:
1815:
1807:
1799:
1791:
1760:
1752:
1744:
1736:
1715:V mag
1711:Elong
1488:S2CID
1399:S2CID
1275:(PDF)
1246:(PDF)
1235:S2CID
1207:(PDF)
1082:S2CID
1003:
943:0.15)
870:Notes
826:Titan
811:stars
775:Orbit
616:Horae
488:0.187
443:Mean
428:(31.8
416:(30.5
292:0.186
238:Epoch
2380:Iris
2305:Juno
2122:Lost
1963:Moon
1958:List
1705:2011
1671:2013
1608:2013
1579:ISSN
1314:2023
1287:2023
1254:2008
1139:ISBN
927:0.02
923:0.53
822:mean
785:Mars
691:and
681:iron
554:5.41
511:0.02
507:0.45
505:BV,
503:0.02
499:0.84
491:0.25
459:3.14
451:2.96
432:0.3)
420:1.9)
411:Mass
405:0.47
342:293°
320:206°
2221:(a
1723:at
1569:doi
1557:401
1527:doi
1515:141
1480:doi
1468:168
1442:doi
1430:125
1389:doi
1377:401
1342:doi
1338:175
1227:doi
1180:doi
1168:455
1135:391
1072:doi
1060:141
753:FGS
636:).
622:in
620:law
548:(H)
513:UB)
386:270
354:99°
2397::
1599:.
1577:.
1567:.
1555:.
1551:.
1539:^
1525:.
1513:.
1509:.
1486:.
1478:.
1466:.
1440:.
1428:.
1424:.
1397:.
1387:.
1375:.
1369:.
1354:^
1336:.
1322:^
1304:.
1277:.
1256:.
1233:.
1225:.
1215:39
1213:.
1209:.
1178:.
1166:.
1162:.
1137:.
1094:^
1080:.
1070:.
1058:.
1054:.
1038:^
1015:^
991:.
852:mi
848:km
844:AU
839:12
771:.
763:,
306:yr
258:AU
244:JD
192:oʊ
183:uː
111:oʊ
102:uː
2225:)
2197:e
2190:t
2183:v
1920:e
1913:t
1906:v
1855:e
1848:t
1841:v
1707:.
1673:.
1633:.
1629::
1610:.
1585:.
1571::
1563::
1533:.
1529::
1521::
1494:.
1482::
1474::
1448:.
1444::
1436::
1405:.
1391::
1383::
1348:.
1344::
1316:.
1289:.
1229::
1221::
1188:.
1182::
1174::
1147:.
1088:.
1074::
1066::
1001:.
949:M
945:×
941:±
929:.
925:±
907:a
904:c
896:1
893:=
890:f
739:~
679:-
509:±
501:±
495:4
493:±
461:±
453:±
434:×
430:±
422:×
418:±
388:±
242:(
207:/
204:n
201:ə
198:i
195:m
189:n
186:ˈ
180:j
177:/
123:/
120:ə
117:i
114:m
108:n
105:ˈ
99:j
96:/
Text is available under the Creative Commons Attribution-ShareAlike License. Additional terms may apply.
