1841:
1030:
1061:
895:
907:
1075:
207:
1134:
27:
1123:
Small frequent impacts tend to preferentially pulverize the weaker rocky debris, leading to an increased concentration of the larger metal fragments at the surface, such that they eventually comprise ~40% of the immediate surface at the present
812:), Hebe does not rank among the top twenty asteroids by volume. This high bulk density suggests an extremely solid body that has not been impacted by collisions, which is not typical of asteroids of its size – they tend to be loosely-bound
1015:
in 2017 indicate that the depressions caused by impacts on 6 Hebe are only 20% the volume of the nearby H-chondrite asteroid families, suggesting the Hebe is not the most likely or primary source of H-chondrite meteorites.
1116:
Large impacts caused local melting of the iron rich H chondrite surface. The metals, being heavier, would have settled to the bottom of the magma lake, forming a metallic layer buried by a relatively shallow layer of
1720:
953:
6 Hebe is extremely well placed to send impact debris to Earth-crossing orbits. Ejecta with even relatively small velocities (~280 m/s) can enter the chaotic regions of the 3:1
1256:
1176:). This was the first modern-day suggestion that asteroids have satellites. It was 17 years later when the first asteroid moon was formally discovered (Dactyl, the satellite of
1701:
988:
159:
1982:
636:
1917:
2282:
2277:
2247:
1169:
1007:
An analysis of likely contributors to Earth's meteorite flux places 6 Hebe at the top of the list, due to its position and relatively large size.
925:. This would imply that it is the source of about 40% of all meteorites striking Earth. Evidence for this connection includes the following:
2257:
1086:
Lightcurve analysis suggests that Hebe has a rather angular shape, which may be due to several large impact craters. Hebe rotates in a
932:
The IIE type are unusual among the iron meteorites, and probably formed from impact melt, rather than being fragments of the core of a
515:
1430:
1490:
James Baer, Steven
Chesley & Robert Matson (2011) "Astrometric masses of 26 asteroids and observations on asteroid porosity."
1975:
1101:
It has a bright surface and, if its identification as the parent body of the H chondrites is correct, a surface composition of
1910:
1399:
808:, containing around 0.5% of the mass of the belt. However, due to its apparently high bulk density (greater than that of the
134:
1943:
374:
1862:
2267:
1968:
2272:
2099:
1539:
1474:
P. Vernazza et al. (2021) VLT/SPHERE imaging survey of the largest main-belt asteroids: Final results and synthesis.
1903:
52:
497:
338:
1777:
2031:
1087:
741:
393:
265:
1605:
Hofrath Gauß gab auf Hencke's
Ansuchen diesem neuen Planetoiden den Namen Hebe mit dem Zeichen (ein Weinglas).
1506:
1191:
have consistently failed to detect any satellites around the asteroid, casting doubt on such a moon existing.
939:
The IIE irons and H chondrites likely come from the same parent body, due to similar trace mineral and oxygen
2252:
2190:
35:
1557:
2262:
2016:
1926:
1222:
2180:
2170:
1723:
Asteroid 6 Hebe: The probable parent body of the H-Type ordinary chondrites and the IIE iron meteorites
1091:
1575:
Wöchentliche
Unterhaltungen für Dilettanten und Freunde der Astronomie, Geographie und Witterungskunde
2175:
1352:
933:
1768:
1758:
2011:
78:
1823:
1799:
1791:
1618:
964:
839:. It has a mean opposition magnitude of +8.3, about equal to the mean brightness of Saturn's moon
2195:
2079:
1991:
1835:
715:
663:
546:
522:
508:
488:
462:
446:
384:
316:
294:
254:
236:
1870:
1815:
1807:
1782:
1531:
1524:
1373:
2116:
1427:
1200:
1188:
1594:
1573:
2021:
1109:
362:
1854:
1846:
1735:
950:
meteorites (accounting for 85% of all falls, including the H chondrites) are extremely rare.
2089:
1886:
1348:
1184:
1012:
881:
828:
409:
276:
39:
1830:
1580:
Weekly entertainments for
Enthusiasts and Friends of Astronomy, Geography, and Meteorology
929:
The spectrum of Hebe matches a mix of 60% H chondrite and 40% IIE iron meteorite material.
8:
422:
327:
1173:
1043:
Please help update this article to reflect recent events or newly available information.
1878:
1840:
1149:
947:
922:
863:
820:
729:
146:
57:
2074:
2026:
1535:
1165:
990:
958:
400:
242:
222:
2200:
1403:
885:
876:
778:
756:
685:
215:
167:
126:
94:
2121:
2064:
2049:
1561:
721:
649:
2136:
2104:
2069:
1677:
1060:
906:
455:
442:
287:
200:
2241:
2160:
2059:
2054:
1753:
1510:
1450:
1434:
1074:
994:
802:
304:
1960:
894:
870:
discovered. It was the second and final asteroid discovery by Hencke, after
2226:
1999:
998:
954:
840:
1895:
1648:
1453:
Shapes and rotational properties of thirty asteroids from photometric data
1112:. A likely scenario for the formation of the surface metal is as follows:
2216:
2165:
2126:
1503:
1153:
1142:
915:
847:
813:
696:
435:
2185:
2131:
1145:
1137:
The orbit of 6 Hebe compared with the orbits of Earth, Mars and
Jupiter
1105:
1095:
1064:
565:
228:
2221:
2111:
1937:
918:
871:
851:
537:
533:
529:
504:
484:
246:
206:
152:
2041:
1102:
867:
836:
805:
1004:
Of the asteroids in this "well-placed" orbit, Hebe is the largest.
1177:
940:
889:
824:
609:
1521:
823:, Hebe is the fifth-brightest object in the asteroid belt after
1949:
1726:, Meteoritics & Planetary Science, Vol. 33, p. 1281 (1998).
832:
702:
1504:
Planetary Data System Small Bodies Node, lightcurve parameters
793:
787:
182:
173:
109:
103:
2152:
1554:
1078:
Size comparison: the first 10 asteroids profiled against the
477:
350:
1164:
As a result of the aforementioned 1977 occultation, a small
1133:
1094:(β, λ) = (45°, 339°) with a 10° uncertainty. This gives an
914:
Hebe was once thought to be the probable parent body of the
1079:
809:
575:
185:
1152:
star. Between 1977 and 2021, 6 Hebe has been observed to
467:
1711:, Astronomy & Astrophysics, Vol. 282, p. 955 (1994).
1219:
Flattening derived from the maximum aspect ratio (c/a):
26:
1530:(2nd ed.). Boston, MA: Houghton Mifflin. pp.
1183:
Detailed observations by many telescopes including the
1120:
Later sizeable impacts broke up and mixed these layers.
843:, and can reach +7.5 at an opposition near perihelion.
1376:. Department of Mathematics, University of Pisa, Italy
910:
Simulations (top) and direct images (bottom) of 6 Hebe
901:
1617:
Bala, Gavin Jared; Miller, Kirk (18 September 2023).
1225:
1180:). The discovery of Hebe's moon was never confirmed.
967:
188:
790:
179:
106:
784:
781:
176:
170:
100:
97:
1523:
1250:
993:which determines the high-inclination edge of the
982:
1619:"Unicode request for historical asteroid symbols"
1374:"AstDyS-2 Hebe Synthetic Proper Orbital Elements"
979:
2239:
1522:Donald H. Menzel & Jay M. Pasachoff (1983).
1090:direction, with the north pole pointing towards
850:meteorites, which account for about 40% of all
1695:
1322:A Practical Dictionary of the English Language
1990:
1976:
1911:
1714:
1603:] (in German). Vol. 3. p. 442.
1515:
1566:
1446:
1444:
1442:
1925:
1486:
1484:
1019:
1983:
1969:
1918:
1904:
1839:
1616:
1610:
25:
1704:Delivery of meteorites through the ν
1672:
1670:
1439:
1343:
1341:
978:
888:as its symbol. It is in the pipeline for
1738:Other reports of Asteroid/TNO Companions
1640:
1481:
1397:
1300:Calculated based on the known parameters
1132:
1073:
1059:
905:
2283:Objects observed by stellar occultation
2278:Astronomical objects discovered in 1847
2248:Minor planet object articles (numbered)
1649:"Proposed New Characters: The Pipeline"
1366:
379:0.97 AU (145 million km)
271:2.43 AU (364 million km)
259:1.93 AU (289 million km)
2240:
1667:
1592:
1586:
1526:A Field Guide to the Stars and Planets
1423:
1421:
1393:
1391:
1338:
946:Asteroids with spectra similar to the
862:Hebe was discovered on 1 July 1847 by
1964:
1899:
1470:
1468:
1466:
1464:
1462:
1428:Supplemental IRAS Minor Planet Survey
1400:"Recent Asteroid Mass Determinations"
1294:
339:Longitude of ascending node
1601:Supplementary Conversational Lexicon
1023:
880:, goddess of youth, was proposed by
1754:shape model deduced from lightcurve
1646:
1418:
1388:
902:Potential as major meteorite source
884:at Hencke's request. Gauss chose a
846:Hebe may be the parent body of the
13:
1459:
1456:, Icarus, Vol. 164, p. 346 (2003).
1402:. Personal Website. Archived from
1251:{\displaystyle f=1-{\frac {c}{a}}}
14:
2294:
2258:Discoveries by Karl Ludwig Hencke
1747:
1721:M. J. Gaffey & S. L. Gilbert
1349:"JPL Small-Body Database: 6 Hebe"
675:Equatorial rotation velocity
1787:AstDyS-2, Asteroids—Dynamic Site
1159:
1028:
893:
777:
205:
166:
93:
1729:
1596:Ergänzungs-conversationslexikon
1548:
1497:
1269:
1172:. It was nicknamed "Jebe" (see
1678:"Not the mother of meteorites"
1326:
1314:
1213:
1082:. Hebe is sixth from the left.
1:
1307:
1011:However, observations by the
36:European Southern Observatory
1476:Astronomy & Astrophysics
1168:around Hebe was reported by
983:{\displaystyle \nu _{6}\,\!}
7:
1194:
1108:rocks mixed with pieces of
363:Argument of perihelion
10:
2299:
1148:, a moderately bright 3rd-
857:
147:Minor planet category
2268:S-type asteroids (Tholen)
2209:
2151:
2088:
2040:
2007:
1998:
1992:Small Solar System bodies
1933:
1582:]. 1847. p. 315.
1353:Jet Propulsion Laboratory
1037:This article needs to be
766:
754:
739:
727:
713:
695:
683:
673:
661:
646:
633:
606:
574:
564:
544:
521:
514:
494:
474:
452:
432:
419:
406:
390:
383:
372:
360:
348:
336:
326:
314:
301:
288:Orbital period (sidereal)
285:
275:
263:
253:
235:
221:
214:
199:
158:
144:
132:
120:
88:
76:
71:
63:
51:
46:
24:
2273:S-type asteroids (SMASS)
1765:(discovery announcement)
1655:. The Unicode Consortium
1492:The Astronomical Journal
1206:
1128:
1020:Physical characteristics
742:Absolute magnitude
516:Physical characteristics
135:Alternative designations
16:Large main-belt asteroid
1927:Minor planets navigator
1836:JPL Small-Body Database
1555:The Brightest Asteroids
664:Synodic rotation period
496:Precession of the
385:Proper orbital elements
351:Time of perihelion
245:(437 million
216:Orbital characteristics
2117:Trans-Neptunian object
1800:Observation prediction
1593:Steger, Franz (1847).
1494:, Volume 141, Number 5
1332:Gabriel Nisbet (1733)
1252:
1201:List of former planets
1189:Hubble Space Telescope
1138:
1083:
1071:
984:
911:
225:13 September 2023
1702:A. Morbidelli et al.
1253:
1146:Kaffaljidhma (γ Ceti)
1141:On 5 March 1977 Hebe
1136:
1077:
1063:
985:
909:
2253:Background asteroids
2090:Distant minor planet
1320:Noah Webster (1884)
1223:
1185:Very Large Telescope
1092:ecliptic coordinates
965:
892:17.0 as U+1CEC0 (
882:Carl Friedrich Gauss
637:surface gravity
79:MPC designation
40:Very Large Telescope
2263:Named minor planets
1887:Physical parameters
1067:-based 3D-model of
923:IIE iron meteorites
498:ascending node
64:Discovery date
21:
1824:Observational info
1560:2008-05-11 at the
1248:
1139:
1084:
1072:
980:
948:ordinary chondrite
912:
864:Karl Ludwig Hencke
730:Apparent magnitude
58:Karl Ludwig Hencke
53:Discovered by
19:
2235:
2234:
2147:
2146:
2032:Meanings of names
1958:
1957:
1708:secular resonance
1451:J. Torppa et al.
1398:Jim Baer (2008).
1246:
1058:
1057:
991:secular resonance
770:
769:
655:~0.127–0.135 km/s
2290:
2005:
2004:
1985:
1978:
1971:
1962:
1961:
1920:
1913:
1906:
1897:
1896:
1879:Orbital elements
1843:
1741:
1733:
1727:
1718:
1712:
1699:
1693:
1692:
1690:
1688:
1674:
1665:
1664:
1662:
1660:
1644:
1638:
1637:
1635:
1633:
1623:
1614:
1608:
1607:
1590:
1584:
1583:
1570:
1564:
1552:
1546:
1545:
1529:
1519:
1513:
1509:14 June 2006 at
1501:
1495:
1488:
1479:
1472:
1457:
1448:
1437:
1433:23 June 2006 at
1425:
1416:
1415:
1413:
1411:
1395:
1386:
1385:
1383:
1381:
1370:
1364:
1363:
1361:
1359:
1345:
1336:
1330:
1324:
1318:
1301:
1298:
1292:
1291:
1283:
1279:
1273:
1267:
1265:
1263:
1258:, where (c/a) =
1257:
1255:
1254:
1249:
1247:
1239:
1217:
1053:
1050:
1044:
1032:
1031:
1024:
989:
987:
986:
981:
977:
976:
897:
854:striking Earth.
800:
799:
796:
795:
792:
789:
786:
783:
762:0.26" to 0.065"
757:Angular diameter
686:Geometric albedo
642:~0.079–0.099 m/s
629:
627:
621:
619:
602:
600:
596:
590:
588:
584:
558:
556:
540:
503:−41.829042
231: 2453300.5)
209:
195:
194:
191:
190:
187:
184:
181:
178:
175:
172:
140:A847 NA; 1847 JB
116:
115:
112:
111:
108:
105:
102:
99:
29:
22:
18:
2298:
2297:
2293:
2292:
2291:
2289:
2288:
2287:
2238:
2237:
2236:
2231:
2205:
2143:
2084:
2036:
1994:
1989:
1959:
1954:
1929:
1924:
1816:Proper elements
1750:
1745:
1744:
1736:W. R. Johnston
1734:
1730:
1719:
1715:
1707:
1700:
1696:
1686:
1684:
1676:
1675:
1668:
1658:
1656:
1645:
1641:
1631:
1629:
1621:
1615:
1611:
1591:
1587:
1572:
1571:
1567:
1562:Wayback Machine
1553:
1549:
1542:
1520:
1516:
1502:
1498:
1489:
1482:
1473:
1460:
1449:
1440:
1426:
1419:
1409:
1407:
1396:
1389:
1379:
1377:
1372:
1371:
1367:
1357:
1355:
1347:
1346:
1339:
1334:Caledon's Tears
1331:
1327:
1319:
1315:
1310:
1305:
1304:
1299:
1295:
1290:
1287:
1281:
1277:
1275:
1274:
1270:
1261:
1259:
1238:
1224:
1221:
1220:
1218:
1214:
1209:
1197:
1162:
1156:fourteen stars.
1131:
1054:
1048:
1045:
1042:
1033:
1029:
1022:
972:
968:
966:
963:
962:
961:and the nearby
904:
860:
780:
776:
759:
747:
732:
718:
705:
688:
676:
666:
656:
652:
650:escape velocity
639:
625:
623:
622:
617:
615:
612:
598:
594:
592:
591:
586:
582:
580:
559:
554:
552:
549:
527:
500:
483:31.568209
480:
465:
458:
441:95.303184
438:
425:
412:
399:2.4252710
396:
394:semi-major axis
365:
353:
341:
319:
307:
290:
268:
266:Semi-major axis
226:
169:
165:
149:
137:
123:
96:
92:
81:
42:
17:
12:
11:
5:
2296:
2286:
2285:
2280:
2275:
2270:
2265:
2260:
2255:
2250:
2233:
2232:
2230:
2229:
2224:
2219:
2213:
2211:
2207:
2206:
2204:
2203:
2198:
2193:
2191:Near-parabolic
2188:
2183:
2178:
2173:
2168:
2163:
2157:
2155:
2149:
2148:
2145:
2144:
2142:
2141:
2140:
2139:
2137:Scattered disc
2134:
2129:
2124:
2114:
2109:
2108:
2107:
2105:Neptune trojan
2102:
2094:
2092:
2086:
2085:
2083:
2082:
2080:Spectral types
2077:
2072:
2070:Jupiter trojan
2067:
2062:
2057:
2052:
2046:
2044:
2038:
2037:
2035:
2034:
2029:
2024:
2019:
2014:
2008:
2002:
1996:
1995:
1988:
1987:
1980:
1973:
1965:
1956:
1955:
1953:
1952:
1947:
1940:
1934:
1931:
1930:
1923:
1922:
1915:
1908:
1900:
1892:
1891:
1890:
1889:
1847:Close approach
1828:
1827:
1826:
1780:
1775:
1766:
1756:
1749:
1748:External links
1746:
1743:
1742:
1728:
1713:
1705:
1694:
1666:
1639:
1609:
1585:
1565:
1547:
1540:
1514:
1496:
1480:
1458:
1438:
1417:
1406:on 2 July 2013
1387:
1365:
1337:
1325:
1312:
1311:
1309:
1306:
1303:
1302:
1293:
1288:
1285:
1268:
1245:
1242:
1237:
1234:
1231:
1228:
1211:
1210:
1208:
1205:
1204:
1203:
1196:
1193:
1174:heebie-jeebies
1161:
1158:
1130:
1127:
1126:
1125:
1121:
1118:
1056:
1055:
1036:
1034:
1027:
1021:
1018:
1009:
1008:
1005:
1002:
997:at about 16°
975:
971:
951:
944:
937:
934:differentiated
930:
903:
900:
859:
856:
768:
767:
764:
763:
760:
755:
752:
751:
748:
740:
737:
736:
733:
728:
725:
724:
719:
714:
711:
710:
699:
693:
692:
689:
684:
681:
680:
677:
674:
671:
670:
667:
662:
659:
658:
657:(457–486 km/h)
653:
647:
644:
643:
640:
634:
631:
630:
628:0.43 g/cm
620:0.64 g/cm
613:
607:
604:
603:
578:
572:
571:
568:
562:
561:
550:
545:
542:
541:
525:
519:
518:
512:
511:
501:
495:
492:
491:
481:
476:Precession of
475:
472:
471:
459:
456:orbital period
453:
450:
449:
439:
433:
430:
429:
426:
420:
417:
416:
413:
407:
404:
403:
397:
391:
388:
387:
381:
380:
377:
370:
369:
366:
361:
358:
357:
354:
349:
346:
345:
342:
337:
334:
333:
330:
324:
323:
320:
315:
312:
311:
308:
302:
299:
298:
291:
286:
283:
282:
279:
273:
272:
269:
264:
261:
260:
257:
251:
250:
239:
233:
232:
219:
218:
212:
211:
203:
197:
196:
162:
156:
155:
150:
145:
142:
141:
138:
133:
130:
129:
124:
121:
118:
117:
90:
86:
85:
82:
77:
74:
73:
69:
68:
65:
61:
60:
55:
49:
48:
44:
43:
34:imaged by the
30:
15:
9:
6:
4:
3:
2:
2295:
2284:
2281:
2279:
2276:
2274:
2271:
2269:
2266:
2264:
2261:
2259:
2256:
2254:
2251:
2249:
2246:
2245:
2243:
2228:
2225:
2223:
2220:
2218:
2215:
2214:
2212:
2208:
2202:
2199:
2197:
2194:
2192:
2189:
2187:
2184:
2182:
2179:
2177:
2174:
2172:
2169:
2167:
2164:
2162:
2159:
2158:
2156:
2154:
2150:
2138:
2135:
2133:
2130:
2128:
2125:
2123:
2120:
2119:
2118:
2115:
2113:
2110:
2106:
2103:
2101:
2098:
2097:
2096:
2095:
2093:
2091:
2087:
2081:
2078:
2076:
2073:
2071:
2068:
2066:
2063:
2061:
2060:Asteroid belt
2058:
2056:
2055:Aten asteroid
2053:
2051:
2048:
2047:
2045:
2043:
2039:
2033:
2030:
2028:
2025:
2023:
2020:
2018:
2015:
2013:
2010:
2009:
2006:
2003:
2001:
2000:Minor planets
1997:
1993:
1986:
1981:
1979:
1974:
1972:
1967:
1966:
1963:
1951:
1948:
1946:
1945:
1941:
1939:
1936:
1935:
1932:
1928:
1921:
1916:
1914:
1909:
1907:
1902:
1901:
1898:
1894:
1888:
1884:
1880:
1876:
1872:
1871:Orbit diagram
1868:
1864:
1860:
1856:
1852:
1848:
1845:
1844:
1842:
1838:
1837:
1832:
1829:
1825:
1821:
1817:
1813:
1809:
1805:
1801:
1797:
1793:
1790:
1789:
1788:
1784:
1781:
1779:
1778:JPL Ephemeris
1776:
1774:
1772:
1767:
1764:
1762:
1757:
1755:
1752:
1751:
1740:
1739:
1732:
1725:
1724:
1717:
1710:
1709:
1698:
1683:
1679:
1673:
1671:
1654:
1650:
1643:
1627:
1620:
1613:
1606:
1602:
1598:
1597:
1589:
1581:
1577:
1576:
1569:
1563:
1559:
1556:
1551:
1543:
1541:0-395-34835-8
1537:
1533:
1528:
1527:
1518:
1512:
1511:archive.today
1508:
1505:
1500:
1493:
1487:
1485:
1477:
1471:
1469:
1467:
1465:
1463:
1455:
1454:
1447:
1445:
1443:
1436:
1435:archive.today
1432:
1429:
1424:
1422:
1405:
1401:
1394:
1392:
1375:
1369:
1354:
1350:
1344:
1342:
1335:
1329:
1323:
1317:
1313:
1297:
1272:
1243:
1240:
1235:
1232:
1229:
1226:
1216:
1212:
1202:
1199:
1198:
1192:
1190:
1186:
1181:
1179:
1175:
1171:
1170:Paul D. Maley
1167:
1160:Possible moon
1157:
1155:
1151:
1147:
1144:
1135:
1122:
1119:
1115:
1114:
1113:
1111:
1107:
1104:
1099:
1097:
1093:
1089:
1081:
1076:
1070:
1066:
1062:
1052:
1040:
1035:
1026:
1025:
1017:
1014:
1006:
1003:
1000:
996:
995:asteroid belt
992:
973:
969:
960:
956:
952:
949:
945:
942:
938:
935:
931:
928:
927:
926:
924:
920:
917:
908:
899:
896:
891:
887:
883:
879:
878:
873:
869:
865:
855:
853:
849:
844:
842:
838:
834:
830:
826:
822:
817:
815:
811:
807:
804:
801:) is a large
798:
774:
765:
761:
758:
753:
749:
746:
745:
738:
734:
731:
726:
723:
720:
717:
716:Spectral type
712:
709:~269 K (−4°C)
708:
704:
700:
698:
694:
690:
687:
682:
679:22.2–24.6 m/s
678:
672:
668:
665:
660:
654:
651:
645:
641:
638:
632:
614:
611:
605:
579:
577:
573:
569:
567:
563:
551:
548:
547:Mean diameter
543:
539:
535:
531:
526:
524:
520:
517:
513:
510:
506:
502:
499:
493:
490:
486:
482:
479:
473:
469:
464:
460:
457:
451:
448:
444:
440:
437:
431:
427:
424:
418:
414:
411:
405:
402:
398:
395:
389:
386:
382:
378:
376:
371:
367:
364:
359:
356:10 March 2022
355:
352:
347:
343:
340:
335:
331:
329:
325:
321:
318:
313:
309:
306:
305:orbital speed
300:
296:
292:
289:
284:
280:
278:
274:
270:
267:
262:
258:
256:
252:
248:
244:
240:
238:
234:
230:
224:
220:
217:
213:
208:
204:
202:
198:
193:
163:
161:
157:
154:
151:
148:
143:
139:
136:
131:
128:
125:
119:
114:
91:
89:Pronunciation
87:
83:
80:
75:
70:
66:
62:
59:
56:
54:
50:
45:
41:
37:
33:
28:
23:
2227:Space debris
1942:
1893:
1882:
1874:
1866:
1858:
1850:
1834:
1819:
1811:
1808:Orbital info
1803:
1795:
1786:
1770:
1760:
1737:
1731:
1722:
1716:
1703:
1697:
1685:. Retrieved
1681:
1657:. Retrieved
1652:
1642:
1632:26 September
1630:. Retrieved
1625:
1612:
1604:
1600:
1595:
1588:
1579:
1574:
1568:
1550:
1525:
1517:
1499:
1491:
1475:
1452:
1408:. Retrieved
1404:the original
1378:. Retrieved
1368:
1358:20 September
1356:. Retrieved
1333:
1328:
1321:
1316:
1296:
1271:
1215:
1182:
1163:
1140:
1100:
1085:
1068:
1049:October 2019
1046:
1038:
1010:
999:inclinations
955:Kirkwood gap
913:
875:
866:, the sixth
861:
845:
818:
814:rubble piles
772:
771:
743:
735:7.5 to 11.50
706:
507: /
487: /
445: /
410:eccentricity
317:Mean anomaly
277:Eccentricity
210:(historical)
72:Designations
31:
2217:Cosmic dust
2181:Long-period
2171:Halley-type
2127:Kuiper belt
2012:Designation
1653:unicode.org
1626:unicode.org
1410:28 November
1110:iron–nickel
1001:hereabouts.
916:H chondrite
874:. The name
848:H chondrite
697:Temperature
648:Equatorial
635:Equatorial
536:× 170
532:× 185
436:mean motion
428:14.3511092°
423:inclination
373:Earth
328:Inclination
297:(1379.85 d)
122:Named after
67:1 July 1847
2242:Categories
2222:Meteoroids
2201:Sungrazing
2176:Hyperbolic
2132:Oort cloud
2075:Near-Earth
1773:(1848) 103
1763:(1847) 283
1659:6 November
1308:References
1117:silicates.
1106:chondritic
1096:axial tilt
1065:Lightcurve
919:meteorites
852:meteorites
821:brightness
601:10 kg
589:10 kg
566:Flattening
523:Dimensions
478:perihelion
466:(1379.702
310:18.93 km/s
255:Perihelion
241:2.92
160:Adjectives
2112:Damocloid
1938:5 Astraea
1863:Ephemeris
1855:Discovery
1792:Ephemeris
1647:Unicode.
1628:. Unicode
1380:1 October
1236:−
1150:magnitude
970:ν
936:asteroid.
886:wineglass
872:5 Astraea
803:main-belt
557:3 km
528:205
415:0.1584864
153:Main belt
47:Discovery
2196:Periodic
2122:Detached
2042:Asteroid
1558:Archived
1507:Archived
1478:54, A56
1431:Archived
1289:☉
1284:10
1195:See also
1187:and the
1143:occulted
1103:silicate
1098:of 42°.
1088:prograde
957:at 2.50
921:and the
868:asteroid
806:asteroid
669:0.3031 d
461:3.77742
303:Average
237:Aphelion
84:(6) Hebe
2161:Extinct
2100:Centaur
1833:at the
1687:19 June
1682:eso.org
1178:243 Ida
1039:updated
943:ratios.
941:isotope
890:Unicode
858:History
610:density
454:Proper
434:Proper
421:Proper
408:Proper
392:Proper
368:239.59°
344:138.63°
332:14.736°
164:Hebean
2153:Comets
2065:Family
2050:Active
2017:Groups
1950:7 Iris
1944:6 Hebe
1883:·
1881:
1875:·
1873:
1867:·
1865:
1859:·
1857:
1851:·
1849:
1831:6 Hebe
1820:·
1818:
1812:·
1810:
1804:·
1802:
1796:·
1794:
1783:6 Hebe
1769:MNRAS
1759:MNRAS
1538:
1154:occult
837:Pallas
835:, and
773:6 Hebe
560:186 km
505:arcsec
485:arcsec
322:144.0°
281:0.2027
201:Symbol
20:6 Hebe
2210:Other
2166:Great
1885:
1877:
1869:
1861:
1853:
1822:
1814:
1806:
1798:
1622:(PDF)
1599:[
1578:[
1280:0.67)
1276:(6.40
1207:Notes
1129:Orbit
1124:time.
841:Titan
829:Ceres
825:Vesta
701:~170
691:0.268
608:Mean
597:0.13)
593:(1.27
585:0.24)
581:(1.24
293:3.78
223:Epoch
2186:Lost
2027:Moon
2022:List
1689:2017
1661:2023
1634:2023
1536:ISBN
1412:2008
1382:2011
1360:2023
1264:0.04
1260:0.75
1166:moon
1080:Moon
1069:Hebe
877:Hebe
833:Iris
810:Moon
750:5.61
707:max:
624:3.77
616:3.18
576:Mass
570:0.25
375:MOID
127:Hēbē
32:Hebe
1785:at
1532:391
1013:VLT
898:).
819:In
744:(H)
553:195
443:deg
38:'s
2244::
1680:.
1669:^
1651:.
1624:.
1534:.
1483:^
1461:^
1441:^
1420:^
1390:^
1351:.
1340:^
959:AU
831:,
827:,
816:.
794:iː
788:iː
538:km
534:km
530:km
509:yr
489:yr
463:yr
447:yr
401:AU
295:yr
247:km
243:AU
229:JD
183:iː
174:iː
110:iː
104:iː
1984:e
1977:t
1970:v
1919:e
1912:t
1905:v
1771:8
1761:7
1706:6
1691:.
1663:.
1636:.
1544:.
1414:.
1384:.
1362:.
1286:M
1282:×
1278:±
1266:.
1262:±
1244:a
1241:c
1233:1
1230:=
1227:f
1051:)
1047:(
1041:.
974:6
797:/
791:b
785:h
782:ˈ
779:/
775:(
722:S
703:K
626:±
618:±
599:×
595:±
587:×
583:±
555:±
470:)
468:d
249:)
227:(
192:/
189:n
186:ə
180:b
177:ˈ
171:h
168:/
113:/
107:b
101:h
98:ˈ
95:/
Text is available under the Creative Commons Attribution-ShareAlike License. Additional terms may apply.
.svg){kind=small}