833:
1870:
1729:
Hanuš, J.; Ďurech, J.; Brož, M.; Marciniak, A.; Warner, B. D.; Pilcher, F.; et al. (March 2013). "Asteroids' physical models from combined dense and sparse photometry and scaling of the YORP effect by the observed obliquity distribution".
29:
772:– Reinmuth selected names from this calendar due to his many asteroid discoveries that he had trouble thinking of proper names. These names are not related to the discoverer's contemporaries.
610:
of 12.2 hours and measures approximately 26 kilometers (16 miles) in diameter. It was named "Rogeria", a name unrelated to the discoverer's contemporaries, that was taken from the almanac
1491:
Masiero, Joseph R.; Grav, T.; Mainzer, A. K.; Nugent, C. R.; Bauer, J. M.; Stevenson, R.; et al. (August 2014). "Main-belt
Asteroids with WISE/NEOWISE: Near-infrared Albedos".
2009:
1944:
2299:
2274:
2284:
1436:
Usui, Fumihiko; Kuroda, Daisuke; Müller, Thomas G.; Hasegawa, Sunao; Ishiguro, Masateru; Ootsubo, Takafumi; et al. (October 2011).
328:
599:
68:
1600:
2002:
1540:
1937:
1234:
1469:
2294:
571:
120:
1970:
999:
1891:
1995:
808:, though with an unusual spectrum (DTU). D-type asteroids are more common further out the asteroid belt and among the
2126:
1363:
1930:
1394:
51:
305:
2058:
640:
548:
234:
2279:
2217:
2289:
971:
781:
1655:
1145:
2043:
966:
864:
1953:
1185:
2207:
2197:
975:
403:
1677:
1255:
2202:
1306:
953:
63:
1852:
1828:
1820:
1805:
2038:
813:
509:
89:
1844:
1836:
1811:
1330:
914:
2222:
2106:
2018:
1864:
780:
learned about
Reinmuth's source of inspiration from private communications with Dutch astronomer
644:
482:
381:
336:
268:
223:
210:
202:
1899:
956:
survey, and individual observers (such as above), as well as sparse-in-time photometry from the
932:
2143:
855:
680:
529:
516:
2048:
888:
793:
718:
697:
612:
491:
317:
188:
110:
1883:
1875:
1753:
1616:
28:
2116:
1915:
1749:
1612:
1555:
1510:
1449:
1406:
660:
245:
1859:
8:
1031:
961:
928:
664:
636:
587:
294:
160:
1786:
1559:
1514:
1453:
1410:
1907:
1869:
1739:
1708:
1704:
1500:
1066:
742:
138:
1777:
1571:
1522:
1272:
2101:
2053:
1757:
1601:"SDSS-based taxonomic classification and orbital distribution of main belt asteroids"
1563:
1230:
991:
937:
919:
893:
859:
652:
216:
176:
832:
2227:
1620:
1518:
1457:
1222:
750:
714:
440:
168:
1625:
1226:
1069:
of 11.285. Further published mean-diameters and albedos by the WISE team include (
2148:
2091:
2076:
1599:
Carvano, J. M.; Hasselmann, P. H.; Lazzaro, D.; Mothé-Diniz, T. (February 2010).
1302:
869:
821:
805:
801:
746:
676:
656:
632:
607:
603:
504:
498:
495:
196:
1792:
1638:
2163:
2131:
2096:
1473:
809:
668:
628:
275:
256:
2268:
2187:
2086:
2081:
1800:
1761:
1567:
1462:
1437:
773:
595:
591:
56:
1987:
1153:
1133:
2253:
2026:
1964:
986:
According to the survey carried out by the
Infrared Astronomical Satellite
692:
648:
154:
1922:
2243:
2192:
2153:
1149:
924:
283:
1065:
derives an albedo of 0.0613 and a diameter of 29.71 km based on an
2212:
2158:
1976:
1136:
by Pravec and
Kusnirak at Ondřejov Observatory (2012). Rotation period
847:
836:
722:
695:
was named after the feminine form of the name "Roger", picked from the
180:
38:
1438:"Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey"
952:
hours using data from the
Uppsala Asteroid Photometric Catalogue, the
2248:
2138:
765:
726:
351:
144:
1393:
Tedesco, E. F.; Noah, P. V.; Noah, M.; Price, S. D. (October 2004).
2068:
1598:
944:
In 2016, a modeled lightcurve gave a concurring sidereal period of
769:
730:
672:
1744:
1505:
995:
717:
region from the late 17th throughout the early 20th century. The
710:
2179:
987:
957:
702:
393:
1806:
729:. For 5 January, the calendar gives "Roger" as the German
1728:
1490:
1435:
1303:"JPL Small-Body Database Browser: 920 Rogeria (A919 RC)"
913:
magnitude was made by French amateur French astronomer
1705:"Asteroids and comets rotation curves – (920) Rogeria"
1392:
1541:"Lightcurve Analysis for Seven Main-belt Asteroids"
1030:) kilometers in diameter and its surface has a low
784:, who worked as a young astronomer at Heidelberg.
1442:Publications of the Astronomical Society of Japan
2266:
1594:
1592:
1534:
1532:
1144:mag. Quality Code is 2−. Summary figures at the
1325:
1323:
1486:
1484:
1482:
709:(lit. "limping messenger") was a very popular
2017:
2003:
1938:
1589:
1529:
741:, the protestant and catholic entries in the
655:once every 4 years and 3 months (1,552 days;
1320:
1180:
1178:
1176:
1174:
1172:
827:
756:
651:asteroid belt at a distance of 2.3–2.9
1952:
1722:
1670:
1479:
1217:Schmadel, Lutz D. (2007). "(920) Rogeria".
1127:
974:of (238.0°, −15.0°) and (47.0°, −35.0°) in
787:
764:As with 22 other asteroids – starting with
619:
2010:
1996:
1945:
1931:
1868:
1696:
1221:. Springer Berlin Heidelberg. p. 82.
1212:
1210:
1208:
1206:
1150:Pravec, P.; Wolf, M.; Sarounova, L. (2007)
935:in June 2007 gave a period of 8.09 hours (
27:
1793:Asteroids and comets rotation curves, CdR
1743:
1624:
1504:
1461:
1297:
1295:
1293:
1291:
1289:
1287:
1285:
1283:
1169:
868:) in Arizona. Lightcurve analysis gave a
683:with its official discovery observation.
1358:
1356:
1354:
1352:
1350:
1348:
1331:"Asteroid 920 Rogeria – Proper Elements"
1216:
831:
2300:Astronomical objects discovered in 1919
2275:Minor planet object articles (numbered)
1678:"Lahrer hinkender Bote – Kalender 1925"
1650:
1648:
1646:
1538:
1431:
1429:
1427:
1388:
1386:
1384:
1256:"Lahrer hinkender Bote – Kalender 1925"
1250:
1248:
1246:
1203:
897:). A tentative period determination of
627:, located in the orbital region of the
600:Heidelberg-Königstuhl State Observatory
2267:
1280:
1063:Collaborative Asteroid Lightcurve Link
981:
1991:
1926:
1658:. Asteroid Lightcurve Database (LCDB)
1345:
1140:hours with a brightness amplitude of
880:hours with a brightness variation of
306:Longitude of ascending node
2285:Discoveries by Karl Wilhelm Reinmuth
1643:
1424:
1381:
1333:. AstDyS-2, Asteroids – Dynamic Site
1243:
804:and somewhat similar to an uncommon
1702:
1000:Wide-field Infrared Survey Explorer
862:at the Command Module Observatory (
725:, the dates of important fairs and
659:of 2.62 AU). Its orbit has an
13:
594:, discovered by German astronomer
14:
2311:
1771:
1093:) with corresponding albedos of (
970:). The study also determined two
1816:AstDyS-2, Asteroids—Dynamic Site
1787:Dictionary of Minor Planet Names
1219:Dictionary of Minor Planet Names
1134:lightcurve plot of (920) Rogeria
778:Dictionary of Minor Planet Names
1395:"IRAS Minor Planet Survey V6.0"
590:from the central region of the
1405:: IRAS-A-FPA-3-RDR-IMPS-V6.0.
846:In October 2010, a rotational
641:hierarchical clustering method
1:
1656:"LCDB Data for (920) Rogeria"
1227:10.1007/978-3-540-29925-7_921
1163:
964:, and the La Palma surveys (
782:Ingrid van Houten-Groeneveld
635:asteroid of the main belt's
106:Name picked from the almanac
7:
2295:DTU-type asteroids (Tholen)
1626:10.1051/0004-6361/200913322
1539:Polakis, Tom (April 2018).
1523:10.1088/0004-637X/791/2/121
905:hours with an amplitude of
647:. It orbits the Sun in the
318:Argument of perihelion
10:
2316:
1732:Astronomy and Astrophysics
1682:Badischen Landesbibliothek
1605:Astronomy and Astrophysics
1399:NASA Planetary Data System
1260:Badischen Landesbibliothek
923:). Another observation by
139:Minor planet category
2236:
2178:
2115:
2067:
2034:
2025:
2019:Small Solar System bodies
1960:
1778:Lightcurve Database Query
1493:The Astrophysical Journal
1307:Jet Propulsion Laboratory
954:Palomar Transient Factory
828:Rotation period and poles
701:, which was published in
686:
602:on 1 September 1919. The
561:
546:
480:
438:
400:
379:
334:
327:
315:
303:
293:
281:
266:
257:Orbital period (sidereal)
254:
244:
232:
222:
209:
195:
187:
175:
167:
136:
118:
99:
87:
82:
74:
62:
50:
45:
26:
1368:Small Bodies Data Ferret
1305:(2019-05-11 last obs.).
1120:
788:Physical characteristics
727:astronomical ephemerides
620:Orbit and classification
549:Absolute magnitude
329:Physical characteristics
121:Alternative designations
16:Dark background asteroid
1954:Minor planets navigator
1865:JPL Small-Body Database
1754:2013A&A...551A..67H
1617:2010A&A...510A..43C
1186:"920 Rogeria (A919 RC)"
645:proper orbital elements
382:Synodic rotation period
169:Orbital characteristics
2144:Trans-Neptunian object
1829:Observation prediction
1463:10.1093/pasj/63.5.1117
1364:"Asteroid 920 Rogeria"
843:
745:, likely referring to
705:, southern Germany. A
681:Heidelberg Observatory
1808:– Minor Planet Center
1548:Minor Planet Bulletin
835:
800:is closest to a dark
794:Tholen classification
698:Lahrer Hinkender Bote
637:background population
613:Lahrer Hinkender Bote
189:Uncertainty parameter
111:Lahrer Hinkender Bote
2280:Background asteroids
2117:Distant minor planet
1782:www.minorplanet.info
976:ecliptic coordinates
933:Ondřejov Observatory
776:, the author of the
713:, especially in the
671:with respect to the
90:MPC designation
2290:Named minor planets
1916:Physical parameters
1577:on 12 February 2020
1560:2018MPBu...45..112P
1515:2014ApJ...791..121M
1474:AcuA catalog p. 153
1454:2011PASJ...63.1117U
1411:2004PDSS...12.....T
1190:Minor Planet Center
982:Diameter and albedo
962:Catalina Sky Survey
839:-based 3D-model of
812:population. In the
588:background asteroid
412:(238.0°, −15.0°) (λ
75:Discovery date
64:Discovery site
23:
1853:Observational info
1797:Geneva Observatory
1709:Geneva Observatory
1067:absolute magnitude
998:mission of NASA's
854:was obtained from
844:
768:, and ending with
743:calendar of saints
715:alemannic-speaking
639:when applying the
423:(47.0°, −35.0°) (λ
52:Discovered by
33:Modelled shape of
21:
2262:
2261:
2174:
2173:
2059:Meanings of names
1985:
1984:
1684:. 1925. p. 2
1262:. 1925. p. 1
1236:978-3-540-00238-3
1058:), respectively.
860:Thomas A. Polakis
816:-based taxonomy,
733:analogue next to
721:section contains
573:prov. designation
565:
564:
404:ecliptic latitude
262:4.25 yr (1,552 d)
2307:
2032:
2031:
2012:
2005:
1998:
1989:
1988:
1947:
1940:
1933:
1924:
1923:
1908:Orbital elements
1872:
1766:
1765:
1747:
1726:
1720:
1719:
1717:
1715:
1703:Behrend, Raoul.
1700:
1694:
1693:
1691:
1689:
1674:
1668:
1667:
1665:
1663:
1652:
1641:
1637:
1635:
1633:
1628:
1596:
1587:
1586:
1584:
1582:
1576:
1570:. Archived from
1545:
1536:
1527:
1526:
1508:
1488:
1477:
1467:
1465:
1448:(5): 1117–1138.
1433:
1422:
1421:
1419:
1417:
1390:
1379:
1378:
1376:
1374:
1360:
1343:
1342:
1340:
1338:
1327:
1318:
1317:
1315:
1313:
1299:
1278:
1271:
1269:
1267:
1252:
1241:
1240:
1214:
1201:
1200:
1198:
1196:
1182:
1157:
1143:
1139:
1131:
1116:
1114:
1108:
1106:
1100:
1098:
1092:
1090:
1084:
1082:
1076:
1074:
1057:
1055:
1049:
1047:
1041:
1039:
1029:
1027:
1021:
1019:
1013:
1011:
969:
951:
949:
940:
922:
912:
910:
904:
902:
896:
887:
885:
879:
877:
867:
858:observations by
751:Pope Telesphorus
585:
579:
539:
537:
526:
524:
513:
473:
471:
464:
462:
455:
453:
441:Geometric albedo
396:
391:
372:
370:
363:
361:
354:
349:
289:0° 13 55.2 / day
158:
107:
78:1 September 1919
46:Discovery
31:
24:
20:
2315:
2314:
2310:
2309:
2308:
2306:
2305:
2304:
2265:
2264:
2263:
2258:
2232:
2170:
2111:
2063:
2021:
2016:
1986:
1981:
1956:
1951:
1845:Proper elements
1774:
1769:
1727:
1723:
1713:
1711:
1701:
1697:
1687:
1685:
1676:
1675:
1671:
1661:
1659:
1654:
1653:
1644:
1631:
1629:
1597:
1590:
1580:
1578:
1574:
1543:
1537:
1530:
1489:
1480:
1434:
1425:
1415:
1413:
1391:
1382:
1372:
1370:
1362:
1361:
1346:
1336:
1334:
1329:
1328:
1321:
1311:
1309:
1301:
1300:
1281:
1265:
1263:
1254:
1253:
1244:
1237:
1215:
1204:
1194:
1192:
1184:
1183:
1170:
1166:
1161:
1160:
1141:
1137:
1132:
1128:
1123:
1112:
1110:
1104:
1102:
1096:
1094:
1088:
1086:
1080:
1078:
1072:
1070:
1053:
1051:
1045:
1043:
1037:
1035:
1025:
1023:
1017:
1015:
1009:
1007:
992:Akari satellite
990:, the Japanese
984:
965:
947:
945:
936:
918:
908:
906:
900:
898:
892:
883:
881:
875:
873:
870:rotation period
863:
830:
822:X-type asteroid
806:T-type asteroid
790:
762:
747:Simeon Stylites
689:
677:observation arc
663:of 0.11 and an
657:semi-major axis
622:
608:rotation period
604:D-type asteroid
583:
577:
554:
542:
535:
533:
522:
520:
507:
485:
476:
469:
467:
460:
458:
451:
449:
443:
434:
430:
426:
419:
415:
406:
389:
387:
384:
375:
368:
366:
359:
357:
347:
345:
339:
320:
308:
286:
271:
259:
237:
235:Semi-major axis
197:Observation arc
159:
152:
141:
131:
123:
108:
105:
102:
92:
69:Heidelberg Obs.
41:
17:
12:
11:
5:
2313:
2303:
2302:
2297:
2292:
2287:
2282:
2277:
2260:
2259:
2257:
2256:
2251:
2246:
2240:
2238:
2234:
2233:
2231:
2230:
2225:
2220:
2218:Near-parabolic
2215:
2210:
2205:
2200:
2195:
2190:
2184:
2182:
2176:
2175:
2172:
2171:
2169:
2168:
2167:
2166:
2164:Scattered disc
2161:
2156:
2151:
2141:
2136:
2135:
2134:
2132:Neptune trojan
2129:
2121:
2119:
2113:
2112:
2110:
2109:
2107:Spectral types
2104:
2099:
2097:Jupiter trojan
2094:
2089:
2084:
2079:
2073:
2071:
2065:
2064:
2062:
2061:
2056:
2051:
2046:
2041:
2035:
2029:
2023:
2022:
2015:
2014:
2007:
2000:
1992:
1983:
1982:
1980:
1979:
1974:
1967:
1961:
1958:
1957:
1950:
1949:
1942:
1935:
1927:
1921:
1920:
1919:
1918:
1876:Close approach
1857:
1856:
1855:
1809:
1803:
1790:
1789:, Google books
1784:
1773:
1772:External links
1770:
1768:
1767:
1721:
1695:
1669:
1642:
1639:(PDS data set)
1588:
1554:(2): 112–115.
1528:
1478:
1423:
1380:
1344:
1319:
1279:
1242:
1235:
1202:
1167:
1165:
1162:
1159:
1158:
1125:
1124:
1122:
1119:
983:
980:
978:(λ, β).
929:Peter Kušnirák
917:in July 2012 (
829:
826:
810:Jupiter trojan
789:
786:
766:913 Otila
761:
759:calendar names
755:
707:Hinkender Bote
688:
685:
629:Eunomia family
621:
618:
563:
562:
559:
558:
555:
547:
544:
543:
541:
540:
527:
514:
502:
488:
486:
481:
478:
477:
475:
474:
465:
456:
446:
444:
439:
436:
435:
433:
432:
428:
424:
421:
417:
413:
409:
407:
401:
398:
397:
385:
380:
377:
376:
374:
373:
364:
355:
342:
340:
335:
332:
331:
325:
324:
321:
316:
313:
312:
309:
304:
301:
300:
297:
291:
290:
287:
282:
279:
278:
272:
267:
264:
263:
260:
255:
252:
251:
248:
242:
241:
238:
233:
230:
229:
226:
220:
219:
213:
207:
206:
199:
193:
192:
185:
184:
173:
172:
165:
164:
142:
137:
134:
133:
124:
119:
116:
115:
103:
100:
97:
96:
93:
88:
85:
84:
80:
79:
76:
72:
71:
66:
60:
59:
54:
48:
47:
43:
42:
32:
15:
9:
6:
4:
3:
2:
2312:
2301:
2298:
2296:
2293:
2291:
2288:
2286:
2283:
2281:
2278:
2276:
2273:
2272:
2270:
2255:
2252:
2250:
2247:
2245:
2242:
2241:
2239:
2235:
2229:
2226:
2224:
2221:
2219:
2216:
2214:
2211:
2209:
2206:
2204:
2201:
2199:
2196:
2194:
2191:
2189:
2186:
2185:
2183:
2181:
2177:
2165:
2162:
2160:
2157:
2155:
2152:
2150:
2147:
2146:
2145:
2142:
2140:
2137:
2133:
2130:
2128:
2125:
2124:
2123:
2122:
2120:
2118:
2114:
2108:
2105:
2103:
2100:
2098:
2095:
2093:
2090:
2088:
2087:Asteroid belt
2085:
2083:
2082:Aten asteroid
2080:
2078:
2075:
2074:
2072:
2070:
2066:
2060:
2057:
2055:
2052:
2050:
2047:
2045:
2042:
2040:
2037:
2036:
2033:
2030:
2028:
2027:Minor planets
2024:
2020:
2013:
2008:
2006:
2001:
1999:
1994:
1993:
1990:
1978:
1975:
1973:
1972:
1968:
1966:
1965:919 Ilsebill
1963:
1962:
1959:
1955:
1948:
1943:
1941:
1936:
1934:
1929:
1928:
1925:
1917:
1913:
1909:
1905:
1901:
1900:Orbit diagram
1897:
1893:
1889:
1885:
1881:
1877:
1874:
1873:
1871:
1867:
1866:
1861:
1858:
1854:
1850:
1846:
1842:
1838:
1834:
1830:
1826:
1822:
1819:
1818:
1817:
1813:
1810:
1807:
1804:
1802:
1801:Raoul Behrend
1798:
1794:
1791:
1788:
1785:
1783:
1779:
1776:
1775:
1763:
1759:
1755:
1751:
1746:
1741:
1737:
1733:
1725:
1710:
1706:
1699:
1683:
1679:
1673:
1657:
1651:
1649:
1647:
1640:
1627:
1622:
1618:
1614:
1610:
1606:
1602:
1595:
1593:
1573:
1569:
1565:
1561:
1557:
1553:
1549:
1542:
1535:
1533:
1524:
1520:
1516:
1512:
1507:
1502:
1498:
1494:
1487:
1485:
1483:
1475:
1471:
1464:
1459:
1455:
1451:
1447:
1443:
1439:
1432:
1430:
1428:
1412:
1408:
1404:
1400:
1396:
1389:
1387:
1385:
1369:
1365:
1359:
1357:
1355:
1353:
1351:
1349:
1332:
1326:
1324:
1308:
1304:
1298:
1296:
1294:
1292:
1290:
1288:
1286:
1284:
1277:
1275:
1261:
1257:
1251:
1249:
1247:
1238:
1232:
1228:
1224:
1220:
1213:
1211:
1209:
1207:
1191:
1187:
1181:
1179:
1177:
1175:
1173:
1168:
1155:
1154:Ondrejov data
1151:
1147:
1135:
1130:
1126:
1118:
1091:0.260 km
1068:
1064:
1059:
1033:
1005:
1001:
997:
993:
989:
979:
977:
973:
968:
963:
959:
955:
942:
939:
934:
930:
926:
921:
916:
895:
890:
871:
866:
861:
857:
853:
849:
842:
838:
834:
825:
823:
819:
815:
811:
807:
803:
799:
795:
785:
783:
779:
775:
774:Lutz Schmadel
771:
770:1144 Oda
767:
760:
754:
752:
748:
744:
740:
736:
732:
728:
724:
720:
716:
712:
708:
704:
700:
699:
694:
684:
682:
678:
675:. The body's
674:
670:
666:
662:
658:
654:
650:
646:
642:
638:
634:
630:
626:
617:
615:
614:
609:
605:
601:
597:
596:Karl Reinmuth
593:
592:asteroid belt
589:
582:
575:
574:
569:
560:
556:
553:
552:
545:
531:
528:
518:
515:
511:
506:
503:
500:
497:
493:
490:
489:
487:
484:
483:Spectral type
479:
466:
457:
448:
447:
445:
442:
437:
422:
411:
410:
408:
405:
399:
395:
386:
383:
378:
371:0.168 km
365:
356:
353:
344:
343:
341:
338:
337:Mean diameter
333:
330:
326:
322:
319:
314:
310:
307:
302:
298:
296:
292:
288:
285:
280:
277:
273:
270:
265:
261:
258:
253:
249:
247:
243:
239:
236:
231:
227:
225:
221:
218:
214:
212:
208:
204:
200:
198:
194:
190:
186:
182:
179:31 May 2020 (
178:
174:
170:
166:
162:
156:
150:
147:
146:
143:
140:
135:
129:
126:A919 RC
125:
122:
117:
113:
112:
104:
98:
95:(920) Rogeria
94:
91:
86:
81:
77:
73:
70:
67:
65:
61:
58:
55:
53:
49:
44:
40:
36:
30:
25:
19:
2254:Space debris
1969:
1911:
1903:
1895:
1887:
1879:
1863:
1848:
1840:
1837:Orbital info
1832:
1824:
1815:
1796:
1781:
1735:
1731:
1724:
1712:. Retrieved
1698:
1686:. Retrieved
1681:
1672:
1660:. Retrieved
1630:. Retrieved
1608:
1604:
1579:. Retrieved
1572:the original
1551:
1547:
1496:
1492:
1445:
1441:
1414:. Retrieved
1402:
1398:
1371:. Retrieved
1367:
1335:. Retrieved
1310:. Retrieved
1273:
1264:. Retrieved
1259:
1218:
1193:. Retrieved
1189:
1129:
1083:7.40 km
1075:4.45 km
1062:
1060:
1003:
985:
943:
851:
845:
840:
817:
797:
791:
777:
763:
758:
738:
734:
706:
696:
693:minor planet
690:
661:eccentricity
624:
623:
611:
586:) is a dark
580:
572:
567:
566:
550:
362:0.36 km
269:Mean anomaly
246:Eccentricity
148:
130: 1919 FT
127:
109:
83:Designations
34:
18:
2244:Cosmic dust
2208:Long-period
2198:Halley-type
2154:Kuiper belt
2039:Designation
1971:920 Rogeria
1860:920 Rogeria
1812:920 Rogeria
1780:(LCDB), at
1714:21 February
1688:20 February
1662:21 February
1632:21 February
1581:22 February
1416:21 February
1373:21 February
1337:21 February
1312:21 February
1274:Lahrer Bote
1266:21 February
1195:21 February
925:Petr Pravec
856:photometric
757:Reinmuth's
665:inclination
631:, is a non-
606:(DT) has a
568:920 Rogeria
392:0.003
295:Inclination
284:Mean motion
101:Named after
57:K. Reinmuth
22:920 Rogeria
2269:Categories
2249:Meteoroids
2228:Sungrazing
2203:Hyperbolic
2159:Oort cloud
2102:Near-Earth
1977:921 Jovita
1164:References
1006:measures (
994:, and the
848:lightcurve
837:Lightcurve
723:feast days
679:begins at
224:Perihelion
205:(36,412 d)
183:2459000.5)
161:background
39:lightcurve
2139:Damocloid
1892:Ephemeris
1884:Discovery
1821:Ephemeris
1762:0004-6361
1745:1301.6943
1568:1052-8091
1506:1406.6645
1499:(2): 11.
972:spin axes
889:magnitude
350:0.9
240:2.6234 AU
228:2.3476 AU
145:main-belt
37:from its
2223:Periodic
2149:Detached
2069:Asteroid
1002:(WISE),
915:René Roy
739:Telesph.
731:name day
719:calendar
673:ecliptic
501:U
211:Aphelion
2188:Extinct
2127:Centaur
1862:at the
1750:Bibcode
1738:: A67.
1613:Bibcode
1556:Bibcode
1511:Bibcode
1450:Bibcode
1407:Bibcode
1276:archive
1109:) and (
1085:) and (
1050:) and (
1022:) and (
1004:Rogeria
996:NEOWISE
946:12.5749
852:Rogeria
841:Rogeria
818:Rogeria
798:Rogeria
792:In the
711:almanac
649:central
643:to its
625:Rogeria
598:at the
584:1919 FT
578:A919 RC
323:268.97°
311:192.79°
299:11.577°
215:2.8993
171:
163:
132:1973 QC
114:
35:Rogeria
2180:Comets
2092:Family
2077:Active
2044:Groups
1912:·
1910:
1904:·
1902:
1896:·
1894:
1888:·
1886:
1880:·
1878:
1849:·
1847:
1841:·
1839:
1833:·
1831:
1825:·
1823:
1760:
1611:: 12.
1566:
1470:online
1233:
1115:0.0030
1111:0.0670
1087:29.683
1036:0.1035
1032:albedo
1024:26.656
960:, the
950:0.0002
874:12.244
820:is an
802:D-type
735:Simeon
687:Naming
633:family
492:Tholen
468:0.1035
388:12.244
367:26.656
274:162.25
250:0.1051
201:99.69
155:middle
149:·
128:·
2237:Other
2193:Great
1914:
1906:
1898:
1890:
1882:
1851:
1843:
1835:
1827:
1740:arXiv
1575:(PDF)
1544:(PDF)
1501:arXiv
1121:Notes
1079:23.69
1071:22.03
1056:0.012
1052:0.076
1048:0.003
1044:0.090
1040:0.008
1028:0.168
1016:25.80
1008:23.89
878:0.003
691:This
667:of 12
538:0.032
534:0.300
525:0.020
521:0.800
512:-MOC)
472:0.008
463:0.003
459:0.090
454:0.012
450:0.076
402:Pole
358:25.80
346:23.89
177:Epoch
151:
2213:Lost
2054:Moon
2049:List
1758:ISSN
1716:2020
1690:2020
1664:2020
1634:2020
1583:2020
1564:ISSN
1418:2020
1375:2020
1339:2020
1314:2020
1268:2020
1231:ISBN
1197:2020
1148:and
1146:LCDB
1142:0.16
1138:8.09
1107:0.05
1103:0.09
1101:), (
1099:0.06
1095:0.09
1077:), (
1061:The
1042:), (
1034:of (
1020:0.36
1014:), (
988:IRAS
958:NOFS
938:U=2−
927:and
920:U=2−
911:0.01
907:0.21
903:0.05
899:9.05
894:U=3−
886:0.03
882:0.31
814:SDSS
749:and
737:and
703:Lahr
557:11.3
510:SDSS
1814:at
1736:551
1621:doi
1609:510
1519:doi
1497:791
1458:doi
1223:doi
1117:).
1012:0.9
967:950
941:).
931:at
872:of
865:V02
850:of
551:(H)
530:U–B
517:B–V
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1799:,
1795:–
1756:.
1748:.
1734:.
1707:.
1680:.
1645:^
1619:.
1607:.
1603:.
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1562:.
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1550:.
1546:.
1531:^
1517:.
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1481:^
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1456:.
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1440:.
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1282:^
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1229:.
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1171:^
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796:,
753:.
653:AU
616:.
581:or
576::
532:=
519:=
494:=
427:/β
416:/β
352:km
217:AU
203:yr
181:JD
2011:e
2004:t
1997:v
1946:e
1939:t
1932:v
1764:.
1752::
1742::
1718:.
1692:.
1666:.
1636:.
1623::
1615::
1585:.
1558::
1525:.
1521::
1513::
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1476:)
1468:(
1466:.
1460::
1452::
1420:.
1409::
1377:.
1341:.
1316:.
1270:.
1239:.
1225::
1199:.
1152:(
1113:±
1105:±
1097:±
1089:±
1081:±
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1046:±
1038:±
1026:±
1018:±
1010:±
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909:±
901:±
891:(
884:±
876:±
669:°
570:(
536:±
523:±
508:(
505:X
499:T
496:D
470:±
461:±
452:±
431:)
429:2
425:2
420:)
418:1
414:1
394:h
390:±
369:±
360:±
348:±
276:°
191:0
157:)
153:(
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