85:
627:
641:
20:
1674:
591:
among the core members (the group is separated by less than 900,000 km in semi major axis and only 0.5Β° in inclination) suggests that the Carme group may once have been a single body that was broken apart by an impact. The dispersion can be explained by a very small velocity impulse (5 < Ξ΄V
677:
of irregular satellites of
Jupiter change widely in short intervals due to heavy perturbation by the Sun. For example, changes of as much as 1 Gm in semi-major axis in 2 years, 0.5 in eccentricity in 12 years, and as much as 5Β° in 24 years have been reported. Mean orbital elements are the averages
23:
This diagram illustrates the largest irregular satellites of
Jupiter. The location of the Carme group is illustrated by Carme's presence in the lower middle. An object's position on the horizontal axis indicates its distance from Jupiter. The vertical axis indicates its
88:
This diagram compares the orbital elements and relative sizes of the core members of the Carme group. The horizontal axis illustrates their average distance from
Jupiter, the vertical axis their orbital inclination, and the circles their relative
32:
is indicated by yellow bars illustrating the object's maximum and minimum distances from
Jupiter. Circles illustrate an object's size in comparison to the others.
819:
1006:
632:
This diagram shows the Ananke group on the same scale as the other diagram, illustrating its wide dispersion in comparison with the compact Carme group.
592:< 50 m/s). The parent body was probably about the size of Carme, 46 km in diameter; 99% of the group's mass is still located in Carme.
724:
Edited by Fran
Bagenal, Timothy E. Dowling, William B. McKinnon. Cambridge planetary science, Vol. 1, Cambridge, UK: Cambridge University Press,
1715:
736:
729:
678:
calculated by the numerical integration of current elements over a long period of time, used to determine the dynamical families.
568:
999:
41:
1710:
1659:
626:
640:
816:
595:
Further support to the single body origin comes from the known colours: all the satellites appear light red, with
1705:
1678:
992:
952:
603:
615:
588:
772:
584:
1700:
1549:
851:
75:
29:
84:
71:
44:
25:
875:
733:
19:
1628:
1436:
943:
894:
867:
835:
725:
706:
266:
1654:
1328:
1303:
1278:
1015:
911:
859:
674:
1586:
1579:
1554:
1396:
1357:
1283:
1214:
1158:
1110:
1093:
1086:
1048:
1043:
839:
823:
740:
710:
607:
281:
236:
145:
63:
855:
760:
1623:
1603:
1540:
1471:
1352:
1323:
1268:
1243:
1233:
1146:
1063:
176:
130:
1694:
1608:
1574:
1476:
1451:
1426:
1421:
1345:
1333:
1293:
1153:
1120:
1079:
898:
842:(5 May 2003). "An abundant population of small irregular satellites around Jupiter".
714:
326:
191:
160:
1618:
1510:
1490:
1483:
1466:
1456:
1401:
1308:
1263:
1224:
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1163:
1053:
1038:
902:
879:
611:
296:
251:
206:
114:
56:
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1559:
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1134:
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596:
446:
431:
341:
221:
1569:
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1500:
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1406:
1391:
1386:
1381:
1338:
1313:
1298:
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1248:
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1189:
1173:
1168:
1139:
551:
536:
521:
506:
491:
476:
461:
416:
401:
386:
371:
356:
311:
1598:
1072:
67:
947:
906:
871:
1461:
1416:
600:
948:"Near-Infrared Photometry of Irregular Satellites of Jupiter and Saturn"
863:
807:
David
NesvornΓ½, Jose L. A. Alvarellos, Luke Dones, and Harold F. Levison
1441:
48:
790:
1593:
1515:
984:
969:
928:
83:
52:
988:
809:. Orbital and Collisional Evolution of the Irregular Satellites
687:
With the exception of Kalyke, which is substantially redder.
753:. Collisional Origin of Families of Irregular Satellites
610:. These data are consistent with a progenitor from the
1025:
Listed in increasing approximate distance from
Jupiter
797:. California Institute of Technology. 25 January 2024.
646:
This diagram shows the compactness of the Carme group.
66:(distances from Jupiter) range between 22.7 and 23.6
1647:
1539:
1371:
1223:
1207:
1182:
1119:
1103:
1062:
1031:
665:
Negative period is indicative of retrograde motion.
722:Jupiter. The planet, satellites and magnetosphere.
907:"Photometric Survey of the Irregular Satellites"
751:David NesvornΓ½, Cristian BeaugΓ©, and Luke Dones
1000:
8:
78:between 0.25 and 0.28 (with one exception).
1007:
993:
985:
92:
59:and are thought to have a common origin.
18:
699:
658:
779:. Minor Planet Center. 27 August 2019.
718:Jupiter's outer satellites and Trojans
171:substantially redder than the others
74:between 164.4Β° and 164.9Β°, and their
7:
16:Group of satellites orbiting Jupiter
791:"Planetary Satellite Mean Elements"
125:largest member and group prototype
14:
1673:
1672:
639:
625:
569:International Astronomical Union
571:(IAU) reserves names ending in
1:
1716:Moons with a retrograde orbit
675:Osculating orbital parameters
81:The Carme group members are:
755:, The Astronomical Journal,
599:B-V= 0.76 and V-R= 0.47 and
811:, The Astronomical Journal,
1732:
1660:Jupiter's moons in fiction
575:for all retrograde moons.
1668:
1022:
953:The Astrophysical Journal
795:Jet Propulsion Laboratory
815:(2003), pages 398β429.
759:(2004), pp. 1768β1783
739:June 14, 2007, at the
90:
76:orbital eccentricities
33:
822:15 April 2020 at the
732:, 2004, p. 263 β 280
589:mean orbital elements
87:
22:
1711:Irregular satellites
946:(22 December 2003).
72:orbital inclinations
51:that follow similar
45:irregular satellites
864:10.1038/nature01584
856:2003Natur.423..261S
944:Holman, Matthew J.
905:(2 January 2003).
895:Holman, Matthew J.
836:Sheppard, Scott S.
773:"Moons of Jupiter"
91:
34:
1688:
1687:
850:(6937): 261β263.
707:Scott S. Sheppard
565:
564:
1723:
1706:Moons of Jupiter
1676:
1675:
1655:Rings of Jupiter
1016:Moons of Jupiter
1009:
1002:
995:
986:
974:
973:
967:
965:
939:
933:
932:
926:
924:
890:
884:
883:
840:Jewitt, David C.
832:
826:
805:
799:
798:
787:
781:
780:
777:Carnegie Science
769:
763:
749:
743:
704:
688:
685:
679:
672:
666:
663:
643:
629:
608:D-type asteroids
93:
1731:
1730:
1726:
1725:
1724:
1722:
1721:
1720:
1691:
1690:
1689:
1684:
1664:
1643:
1535:
1367:
1219:
1203:
1183:Carpo group (2)
1178:
1115:
1099:
1058:
1027:
1018:
1013:
983:
978:
977:
963:
961:
941:
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936:
922:
920:
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891:
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834:
833:
829:
824:Wayback Machine
806:
802:
789:
788:
784:
771:
770:
766:
750:
746:
741:Wayback Machine
734:Full text(pdf).
711:David C. Jewitt
705:
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105:
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64:semi-major axes
17:
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5:
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1596:
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1562:
1557:
1552:
1546:
1544:
1541:Pasiphae group
1537:
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1369:
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1331:
1326:
1324:Jupiter LXVIII
1321:
1316:
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1296:
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1098:
1097:
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1064:Galilean moons
1060:
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1023:
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1011:
1004:
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989:
982:
981:External links
979:
976:
975:
934:
899:Gladman, Brett
885:
827:
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597:colour indices
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40:is a group of
15:
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1600:
1597:
1595:
1592:
1590:
1589:
1588:
1583:
1581:
1578:
1576:
1575:Jupiter LXVII
1573:
1571:
1568:
1566:
1563:
1561:
1558:
1556:
1553:
1551:
1550:Philophrosyne
1548:
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1478:
1477:Jupiter LXXII
1475:
1473:
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1463:
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1448:
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1423:
1422:Jupiter LXIII
1420:
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1128:
1127:
1125:
1122:
1121:Himalia group
1118:
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1003:
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980:
971:
959:
955:
954:
949:
945:
942:Grav, Tommy;
938:
935:
930:
918:
914:
913:
908:
904:
903:Aksnes, Kaare
900:
896:
893:Grav, Tommy;
889:
886:
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877:
873:
869:
865:
861:
857:
853:
849:
845:
841:
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748:
745:
742:
738:
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731:
730:0-521-81808-7
727:
723:
719:
716:
715:Carolyn Porco
712:
708:
703:
700:
693:
684:
681:
676:
671:
668:
662:
659:
653:
642:
628:
619:
617:
614:or a Jupiter
613:
609:
606:, similar to
605:
602:
598:
593:
590:
586:
583:The very low
578:
576:
574:
570:
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534:
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60:
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50:
46:
43:
39:
31:
27:
21:
1677:
1585:
1584:
1511:Jupiter LXVI
1482:
1481:
1402:Jupiter LXIX
1372:
1344:
1343:
1309:Jupiter LXIV
1225:Ananke group
1195:
1194:
1145:
1144:
1092:
1085:
1078:
1071:
1024:
968:– via
962:. Retrieved
957:
951:
937:
927:– via
921:. Retrieved
916:
910:
888:
847:
843:
830:
812:
808:
803:
794:
785:
776:
767:
756:
752:
747:
721:
717:
702:
683:
670:
661:
612:Hilda family
594:
582:
572:
566:
80:
61:
37:
35:
30:Eccentricity
1701:Carme group
1634:S/2003 J 23
1614:Jupiter LIX
1560:Jupiter LVI
1531:S/2003 J 10
1496:Jupiter LXI
1412:S/2003 J 24
1373:Carme group
1363:Jupiter LXX
1319:S/2003 J 12
1274:S/2003 J 16
1259:Jupiter LIV
1254:Jupiter LII
1032:Inner moons
960:: L141βL144
447:S/2003 J 24
432:S/2003 J 10
342:S/2003 J 19
38:Carme group
26:inclination
1695:Categories
1629:Callirrhoe
1570:S/2016 J 4
1565:S/2003 J 4
1526:S/2021 J 5
1521:S/2018 J 3
1506:S/2003 J 9
1501:Jupiter LI
1437:Kallichore
1432:S/2021 J 4
1407:S/2021 J 6
1392:S/2016 J 3
1387:S/2022 J 2
1382:S/2022 J 1
1339:S/2003 J 2
1314:S/2021 J 1
1299:S/2021 J 2
1289:S/2022 J 3
1249:S/2021 J 3
1239:Jupiter LV
1190:S/2018 J 4
1169:S/2011 J 3
1140:S/2018 J 2
761:Full text.
694:References
585:dispersion
552:S/2022 J 2
537:S/2022 J 1
522:S/2021 J 6
507:S/2021 J 5
492:S/2021 J 4
477:S/2018 J 3
462:S/2016 J 3
417:S/2003 J 9
402:S/2011 J 1
387:S/2017 J 8
372:S/2017 J 5
357:S/2017 J 2
312:S/2010 J 1
267:Kallichore
42:retrograde
1599:Megaclite
1329:Thelxinoe
1304:Praxidike
1279:Harpalyke
964:2 January
923:2 January
1679:Category
1648:See also
1587:Pasiphae
1580:Hegemone
1555:Eurydome
1462:Eukelade
1417:Chaldene
1397:Pasithee
1358:Hermippe
1284:Orthosie
1215:Valetudo
1208:Valetudo
1159:Lysithea
1111:Themisto
1104:Themisto
1094:Callisto
1087:Ganymede
1049:Amalthea
1044:Adrastea
872:12748634
820:Archived
737:Archived
601:infrared
282:Eukelade
237:Pasithee
146:Chaldene
99:Diameter
70:, their
1624:Autonoe
1604:Cyllene
1472:Taygete
1442:Erinome
1353:Iocaste
1269:Euanthe
1244:Eupheme
1234:Euporie
1147:Himalia
919:: 33β45
880:4424447
852:Bibcode
604:spectra
587:of the
559:β781.56
544:β738.33
529:β720.97
514:β747.74
499:β728.28
484:β747.02
469:β713.64
454:β721.60
439:β755.43
424:β736.86
409:β733.21
394:β719.76
379:β737.28
364:β724.71
349:β734.78
334:β729.84
319:β736.51
304:β734.52
289:β730.30
274:β728.26
259:β731.88
244:β719.47
229:β729.64
214:β730.10
199:β726.27
184:β728.48
177:Erinome
168:β742.02
153:β723.71
138:β732.45
131:Taygete
122:β734.19
49:Jupiter
1609:Sinope
1594:Sponde
1516:Kalyke
1452:Eirene
1427:Isonoe
1346:Ananke
1334:Thyone
1294:Helike
1154:Pandia
1080:Europa
912:Icarus
878:
870:
844:Nature
728:
720:, In:
616:trojan
579:Origin
327:Eirene
192:Isonoe
161:Kalyke
109:Notes
106:(days)
104:Period
89:sizes.
62:Their
53:orbits
1619:Aoede
1491:Herse
1484:Carme
1467:Arche
1457:Aitne
1264:Mneme
1197:Carpo
1164:Elara
1054:Thebe
1039:Metis
970:ArXiv
929:ArXiv
876:S2CID
817:(pdf)
654:Notes
297:Herse
252:Arche
207:Aitne
115:Carme
57:Carme
1639:Kore
1543:(18)
1447:Kale
1375:(30)
1227:(26)
1135:Ersa
1130:Leda
966:2024
925:2024
868:PMID
726:ISBN
567:The
222:Kale
101:(km)
96:Name
36:The
1174:Dia
1123:(9)
958:605
917:166
860:doi
848:423
813:126
757:127
55:to
47:of
1697::
1073:Io
956:.
950:.
915:.
909:.
901:;
897:;
874:.
866:.
858:.
846:.
838:;
793:.
775:.
713:,
709:,
618:.
573:-e
119:46
68:Gm
28:.
1008:e
1001:t
994:v
972:.
931:.
882:.
862::
854::
556:1
541:2
526:1
511:2
496:1
481:1
466:2
451:2
436:2
421:1
406:2
391:1
376:2
361:2
346:2
331:4
316:2
301:2
286:4
271:2
256:3
241:2
226:2
211:3
196:4
181:3
165:5
150:4
135:5
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