788:
1729:
1472:
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".
853:). Assuming an equatorial view, the observers also constrained the object's elongated shape to be at least 36% longer than wide. The result supersedes a tentative period determination by French amateur astronomer
1362:
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".
1868:
1803:
47:
2158:
2133:
1552:
Garceran, Alfonso
Carreno; Aznar, Amadeo; Mansego, Enrique Arce; Rodriguez, Pedro Brines; de Haro, Juan Lozano; Silva, Alvaro Fornas; et al. (January 2016).
1062:
gave a best-fit ellipse dimension of 19.0 × 19.0 kilometers. These timed observations are taken when the asteroid passes in front of a distant star.
350:
696:
611:
86:
1861:
1796:
1142:
579:
144:
1307:
Usui, Fumihiko; Kuroda, Daisuke; Müller, Thomas G.; Hasegawa, Sunao; Ishiguro, Masateru; Ootsubo, Takafumi; et al. (October 2011).
943:
1854:
1829:
1985:
2143:
1789:
1553:
1411:
69:
327:
1917:
656:
256:
1340:
2138:
2076:
2148:
1750:
915:
738:
1234:
1902:
2153:
2066:
2056:
1265:
919:
425:
46:
725:
was named. Rosalinde's maid in the operetta, "Adele", is likely the namesake chosen by Wolf for another asteroid,
2061:
1173:
910:
897:
820:
81:
1897:
107:
854:
2081:
1965:
1877:
1723:
660:
504:
403:
358:
245:
232:
224:
2002:
1612:
811:
761:
537:
524:
1907:
1812:
1087:
844:
787:
339:
210:
737:
learned about the discoverer's source of inspiration from private communications with Dutch astronomer
1975:
1568:
1492:
1426:
1381:
1320:
1277:
1059:
776:
676:
267:
1711:
1687:
1679:
1664:
975:
905:
680:
652:
595:
316:
182:
1703:
1695:
1670:
1197:
1531:
1482:
1371:
1007:
556:
1758:
900:
survey, and individual observers (such as above), as well as sparse-in-time photometry from the
1960:
1912:
1576:
1508:
1434:
1138:
1126:
935:
881:
859:
849:
815:
718:
668:
633:
606:
of approximately 19 kilometers (12 miles). It was discovered on 10 August 1918, by astronomer
238:
198:
134:
1554:"Nineteen Asteroids Lightcurves at Asteroids Observers (OBAS) - MPPD: 2015 April - September"
764:-classification by Xu (1995), which surveyed and classified a total of 221 objects. However,
2086:
1742:
1734:
1500:
1496:
1389:
1328:
1130:
1118:
462:
190:
1774:
2007:
1950:
1935:
1718:
825:
757:
753:
692:
672:
648:
623:
619:
615:
516:
513:
218:
31:
1645:
1572:
1430:
1385:
1324:
1281:
2022:
1990:
1955:
1766:
1728:
1527:
713:
711:
was probably named after the character "Rosalinde", Eisenstein's wife, in the operetta
684:
628:
297:
278:
127:
1636:
1584:
1442:
1393:
1006:
assumes an albedo of 0.0931 and calculates a diameter of 18.75 kilometers based on an
779:(II), where the bright S-types and the dark D-types do not have intermediate albedos.
2127:
2046:
1945:
1940:
1659:
1119:
1010:
of 11.83. Alternative mean-diameter measurements published by the WISE team include (
730:
603:
599:
2112:
1885:
722:
708:
664:
290:
176:
160:
1504:
1134:
626:
of 16.6 hours. It was likely named after "Rosalinde", a character in the operetta
1412:"Lightcurve Results for Asteroids 900 Rosalinde, 4666 Dietz, and 6302 Tengukogen"
1169:
2102:
2051:
2012:
1835:
1823:
1651:
305:
1344:
2071:
2017:
803:
796:
741:, who worked as a young astronomer at the discovering Heidelberg Observatory.
202:
56:
1580:
1512:
1438:
1333:
1308:
2107:
1997:
1846:
726:
373:
166:
930:
According to the survey carried out by the
Infrared Astronomical Satellite
1781:
1927:
688:
607:
74:
17:
939:
1309:"Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey"
896:
hours using data from the
Uppsala Asteroid Photometric Catalogue, the
863:). Additional observation by the Spanish OBAS group gave a period of
775:
does not correspond to more modern taxonomies such as the Bus–Binzel
1264:
Tedesco, E. F.; Noah, P. V.; Noah, M.; Price, S. D. (October 2004).
888:
In 2016, a modeled lightcurve gave a concurring sidereal period of
824:) of the Alfred University in New York. Lightcurve analysis gave a
2038:
1487:
1376:
786:
931:
901:
415:
1850:
1785:
814:
observations by
Meaghann Stoelting and David DeGraffat at the
699:
with its official discovery observation on 10 August 1918.
1665:
1170:"JPL Small-Body Database Browser: 900 Rosalinde (A918 PJ)"
1528:"Asteroids and comets rotation curves – (900) Rosalinde"
1410:
Stoelting, Meaghann; DeGraff, David R. (January 2016).
2095:
2037:
1974:
1926:
1884:
554:
502:
460:
422:
401:
356:
349:
337:
325:
315:
303:
288:
276:
266:
254:
244:
231:
217:
189:
158:
142:
117:
105:
100:
92:
80:
68:
63:
771:s classification, with its moderate albedo of 0.1
1313:Publications of the Astronomical Society of Japan
1405:
1403:
974:) kilometers in diameter and its surface has an
1192:
1190:
1467:
1465:
1463:
1357:
1355:
1353:
671:once every 3 years and 11 months (1,421 days;
1862:
1797:
1117:Schmadel, Lutz D. (2007). "(900) Rosalinde".
8:
1082:
1080:
1078:
1076:
1074:
667:asteroid belt at a distance of 2.1–2.9
39:
1890:
1869:
1855:
1847:
1804:
1790:
1782:
1727:
1198:"Asteroid 900 Rosalinde – Proper Elements"
1112:
1110:
1108:
45:
1652:Asteroids and comets rotation curves, CdR
1486:
1375:
1332:
1164:
1162:
1160:
1158:
1156:
1154:
918:of (276.0°, 70.0°) and (90.0°, 39.0°) in
1229:
1227:
1225:
1223:
1221:
1219:
1217:
1215:
2159:Astronomical objects discovered in 1918
2134:Minor planet object articles (numbered)
1607:
1605:
1302:
1300:
1298:
1259:
1257:
1255:
1070:
697:Heidelberg-Königstuhl State Observatory
612:Heidelberg-Königstuhl State Observatory
1125:. Springer Berlin Heidelberg. p.
1004:Collaborative Asteroid Lightcurve Link
38:
1615:. Asteroid Lightcurve Database (LCDB)
836:hours with a brightness variation of
328:Longitude of ascending node
7:
1200:. AstDyS-2, Asteroids – Dynamic Site
1732:
944:Wide-field Infrared Survey Explorer
675:of 2.47 AU). Its orbit has an
614:in southwest Germany. The lengthy
25:
1034:) with corresponding albedos of (
914:). The study also determined two
30:For the satellite of Uranus, see
1675:AstDyS-2, Asteroids—Dynamic Site
1646:Dictionary of Minor Planet Names
1121:Dictionary of Minor Planet Names
735:Dictionary of Minor Planet Names
1613:"LCDB Data for (900) Rosalinde"
1266:"IRAS Minor Planet Survey V6.0"
1276:: IRAS-A-FPA-3-RDR-IMPS-V6.0.
657:hierarchical clustering method
598:from the inner regions of the
1:
1135:10.1007/978-3-540-29925-7_901
27:Elongated background asteroid
908:, and the La Palma surveys (
739:Ingrid van Houten-Groeneveld
651:asteroid of the main belt's
1505:10.1051/0004-6361/201220701
1394:10.1088/0004-637X/791/2/121
871:hours with an amplitude of
802:In June 2011, a rotational
663:. It orbits the Sun in the
340:Argument of perihelion
2175:
1475:Astronomy and Astrophysics
1270:NASA Planetary Data System
161:Minor planet category
29:
1893:
1878:Small Solar System bodies
1819:
1637:Lightcurve Database Query
1364:The Astrophysical Journal
1174:Jet Propulsion Laboratory
1088:"900 Rosalinde (A918 PJ)"
898:Palomar Transient Factory
569:
279:Orbital period (sidereal)
209:
197:
123:Character "Rosalinde" in
44:
1239:Small Bodies Data Ferret
1235:"Asteroid 900 Rosalinde"
1172:(2020-01-24 last obs.).
745:Physical characteristics
721:(1825–1899), after whom
640:Orbit and classification
557:Absolute magnitude
351:Physical characteristics
145:Alternative designations
2144:Discoveries by Max Wolf
1813:Minor planets navigator
1724:JPL Small-Body Database
1497:2013A&A...551A..67H
661:proper orbital elements
404:Synodic rotation period
191:Orbital characteristics
2003:Trans-Neptunian object
1688:Observation prediction
1334:10.1093/pasj/63.5.1117
1058:). On 7 June 2015, an
799:
1667:– Minor Planet Center
1561:Minor Planet Bulletin
1419:Minor Planet Bulletin
1002:), respectively. The
790:
653:background population
211:Uncertainty parameter
2139:Background asteroids
1976:Distant minor planet
1641:www.minorplanet.info
1060:asteroid occultation
920:ecliptic coordinates
777:SMASS classification
733:, the author of the
687:with respect to the
108:MPC designation
2149:Named minor planets
1775:Physical parameters
1573:2016MPBu...43...92G
1431:2016MPBu...43...44S
1386:2014ApJ...791..121M
1345:AcuA catalog p. 153
1325:2011PASJ...63.1117U
1282:2004PDSS...12.....T
1092:Minor Planet Center
926:Diameter and albedo
906:Catalina Sky Survey
596:background asteroid
93:Discovery date
82:Discovery site
41:
1712:Observational info
1656:Geneva Observatory
1532:Geneva Observatory
1008:absolute magnitude
942:mission of NASA's
810:was obtained from
800:
655:when applying the
594:) is an elongated
434:(276.0°, 70.0°) (λ
70:Discovered by
51:Modelled shape of
2154:Johann Strauss II
2121:
2120:
2033:
2032:
1918:Meanings of names
1844:
1843:
1590:on 3 October 2020
1448:on 3 October 2020
1144:978-3-540-00238-3
816:Stull Observatory
723:4559 Strauss
719:Johann Strauss II
634:Johann Strauss II
581:prov. designation
573:
572:
445:(90.0°, 39.0°) (λ
426:ecliptic latitude
311:0° 15 12.24 / day
284:3.89 yr (1,421 d)
135:Johann Strauss II
16:(Redirected from
2166:
1891:
1871:
1864:
1857:
1848:
1806:
1799:
1792:
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1767:Orbital elements
1731:
1625:
1624:
1622:
1620:
1609:
1600:
1599:
1597:
1595:
1589:
1583:. Archived from
1558:
1549:
1543:
1542:
1540:
1538:
1526:Behrend, Raoul.
1523:
1517:
1516:
1490:
1469:
1458:
1457:
1455:
1453:
1447:
1441:. Archived from
1416:
1407:
1398:
1397:
1379:
1359:
1348:
1338:
1336:
1319:(5): 1117–1138.
1304:
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593:
587:
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463:Geometric albedo
418:
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371:
180:
138:
131:
64:Discovery
49:
42:
21:
2174:
2173:
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2123:
2122:
2117:
2091:
2029:
1970:
1922:
1880:
1875:
1845:
1840:
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1810:
1704:Proper elements
1633:
1628:
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997:
995:
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987:
981:
979:
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967:
961:
959:
953:
951:
936:Akari satellite
934:, the Japanese
928:
909:
891:
889:
880:
874:
872:
866:
864:
858:
857:from May 2007 (
848:
839:
837:
831:
829:
826:rotation period
819:
785:
783:Rotation period
768:
760:in the SMASS-I
747:
705:
693:observation arc
679:of 0.16 and an
673:semi-major axis
642:
624:rotation period
620:D-type asteroid
591:
585:
562:
550:
543:
541:
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259:
257:Semi-major axis
219:Observation arc
181:
174:
163:
147:
132:
124:
120:
113:(900) Rosalinde
110:
87:Heidelberg Obs.
59:
35:
32:Rosalind (moon)
28:
23:
22:
15:
12:
11:
5:
2172:
2170:
2162:
2161:
2156:
2151:
2146:
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2136:
2126:
2125:
2119:
2118:
2116:
2115:
2110:
2105:
2099:
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2093:
2092:
2090:
2089:
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2079:
2077:Near-parabolic
2074:
2069:
2064:
2059:
2054:
2049:
2043:
2041:
2035:
2034:
2031:
2030:
2028:
2027:
2026:
2025:
2023:Scattered disc
2020:
2015:
2010:
2000:
1995:
1994:
1993:
1991:Neptune trojan
1988:
1980:
1978:
1972:
1971:
1969:
1968:
1966:Spectral types
1963:
1958:
1956:Jupiter trojan
1953:
1948:
1943:
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1924:
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1735:Close approach
1716:
1715:
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1668:
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1649:
1648:, Google books
1643:
1632:
1631:External links
1629:
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1067:
1064:
927:
924:
922:(λ, β).
784:
781:
746:
743:
727:812 Adele
714:Die Fledermaus
704:
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629:Die Fledermaus
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96:10 August 1918
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1946:Asteroid belt
1944:
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1941:Aten asteroid
1939:
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1886:Minor planets
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1830:900 Rosalinde
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1759:Orbit diagram
1756:
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1719:900 Rosalinde
1717:
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1671:900 Rosalinde
1669:
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1663:
1661:
1660:Raoul Behrend
1657:
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1061:
1032:0.160 km
1016:5.124 km
1009:
1005:
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917:
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813:
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795:based on its
794:
789:
782:
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774:
767:
763:
762:spectral type
759:
755:
751:
744:
742:
740:
736:
732:
731:Lutz Schmadel
728:
724:
720:
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702:
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698:
694:
691:. The body's
690:
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631:
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621:
617:
613:
609:
605:
604:mean diameter
602:, that has a
601:
600:asteroid belt
597:
590:
583:
582:
577:
576:900 Rosalinde
568:
564:
561:
560:
553:
539:
536:
526:
523:
520:(SMASS-I; Xu)
518:
515:
512:
511:
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505:Spectral type
501:
488:
479:
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469:
467:
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444:
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427:
421:
417:
408:
405:
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393:0.057 km
387:
378:
375:
366:
365:
363:
360:
359:Mean diameter
355:
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201:31 May 2020 (
200:
196:
192:
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178:
172:
169:
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162:
157:
153:
150:A918 PJ
149:
146:
141:
136:
130:
129:
125:the operetta
122:
116:
112:
109:
104:
99:
95:
91:
88:
85:
83:
79:
76:
73:
71:
67:
62:
58:
54:
48:
43:
40:900 Rosalinde
37:
33:
19:
2113:Space debris
1828:
1824:899 Jokaste
1770:
1762:
1754:
1746:
1738:
1722:
1707:
1699:
1696:Orbital info
1691:
1683:
1674:
1655:
1640:
1617:. Retrieved
1592:. Retrieved
1585:the original
1567:(1): 92–97.
1564:
1560:
1547:
1535:. Retrieved
1521:
1478:
1474:
1450:. Retrieved
1443:the original
1425:(1): 44–45.
1422:
1418:
1367:
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1312:
1285:. Retrieved
1273:
1269:
1242:. Retrieved
1238:
1202:. Retrieved
1177:. Retrieved
1120:
1095:. Retrieved
1091:
1024:6.22 km
1003:
947:
929:
887:
807:
801:
792:
791:3D-model of
772:
765:
749:
748:
734:
712:
709:minor planet
706:
677:eccentricity
644:
643:
627:
588:
580:
575:
574:
558:
384:0.31 km
291:Mean anomaly
268:Eccentricity
170:
154: 1918 EC
151:
126:
101:Designations
52:
36:
2103:Cosmic dust
2067:Long-period
2057:Halley-type
2013:Kuiper belt
1898:Designation
1836:901 Brunsia
1639:(LCDB), at
1619:24 February
1594:24 February
1537:24 February
1452:24 February
1287:24 February
1244:24 February
1204:24 February
1179:24 February
1097:24 February
879:magnitude (
812:photometric
773:(see below)
681:inclination
414:0.009
317:Inclination
306:Mean motion
119:Named after
2128:Categories
2108:Meteoroids
2087:Sungrazing
2062:Hyperbolic
2018:Oort cloud
1961:Near-Earth
1066:References
950:measures (
938:, and the
804:lightcurve
797:lightcurve
695:begins at
246:Perihelion
227:(37,057 d)
205:2459000.5)
183:background
75:M. F. Wolf
57:lightcurve
1998:Damocloid
1751:Ephemeris
1743:Discovery
1680:Ephemeris
1581:1052-8091
1513:0004-6361
1488:1301.6943
1439:1052-8091
1377:1406.6645
1370:(2): 11.
948:Rosalinde
916:spin axes
845:magnitude
808:Rosalinde
793:Rosalinde
766:Rosalinde
750:Rosalinde
647:is a non-
645:Rosalinde
372:1.4
262:2.4732 AU
250:2.0705 AU
167:main-belt
55:from its
53:Rosalinde
18:Rosalinde
2082:Periodic
2008:Detached
1928:Asteroid
946:(WISE),
855:René Roy
689:ecliptic
608:Max Wolf
233:Aphelion
2047:Extinct
1986:Centaur
1721:at the
1569:Bibcode
1493:Bibcode
1481:: A67.
1427:Bibcode
1382:Bibcode
1321:Bibcode
1278:Bibcode
1050:) and (
1026:) and (
994:) and (
966:) and (
940:NEOWISE
890:16.6868
659:to its
610:at the
592:1918 EC
586:A918 PJ
345:121.78°
333:182.26°
321:11.559°
237:2.8758
223:101.46
193:
185:
2039:Comets
1951:Family
1936:Active
1903:Groups
1771:·
1769:
1763:·
1761:
1755:·
1753:
1747:·
1745:
1739:·
1737:
1708:·
1706:
1700:·
1698:
1692:·
1690:
1684:·
1682:
1579:
1511:
1437:
1341:online
1141:
1056:0.0106
1052:0.0750
1028:20.908
1012:18.191
980:0.1008
976:albedo
968:19.618
904:, the
894:0.0002
830:16.648
758:D-type
754:S-type
752:is an
703:Naming
649:family
622:has a
490:0.1008
410:16.648
389:19.618
296:73.490
272:0.1628
171:·
152:·
2096:Other
2052:Great
1773:
1765:
1757:
1749:
1741:
1710:
1702:
1694:
1686:
1588:(PDF)
1557:(PDF)
1483:arXiv
1446:(PDF)
1415:(PDF)
1372:arXiv
1040:0.105
1036:0.131
1020:19.69
1000:0.021
996:0.085
992:0.004
988:0.096
984:0.017
972:0.057
960:19.56
952:18.78
882:U=2/2
865:16.70
834:0.009
769:'
707:This
683:of 12
665:inner
546:0.030
542:0.390
533:0.020
529:0.860
494:0.017
485:0.004
481:0.096
476:0.021
472:0.085
424:Pole
380:19.56
368:18.78
199:Epoch
177:inner
173:
2072:Lost
1913:Moon
1908:List
1621:2020
1596:2020
1577:ISSN
1539:2020
1509:ISSN
1454:2020
1435:ISSN
1289:2020
1246:2020
1206:2020
1181:2020
1139:ISBN
1099:2020
1048:0.08
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902:NOFS
877:0.02
873:0.28
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850:U=2+
842:0.02
838:0.33
565:11.6
133:(by
1673:at
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1390:doi
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1329:doi
1131:doi
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911:950
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860:U=2
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821:784
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717:by
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669:AU
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239:AU
225:yr
203:JD
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