431:
440:
20:
1358:
419:, the theory of a single impact origin for the Pasiphae group is not accepted by all studies. This is because the Pasiphae group, while similar in semi-major axis, is more widely dispersed in inclination. Alternatively, Sinope might be not a part of the remnants of the same collision and captured independently instead. The differences of colour between the objects (grey for Pasiphae, light red for
434:
This diagram compares the orbital elements and relative sizes of the core members of the
Pasiphae group. The horizontal axis illustrates their average distance from Jupiter, the vertical axis their orbital inclination, and the circles their relative
23:
This diagram illustrates the largest irregular satellites of
Jupiter. Among the Pasiphae group, Sinope and Pasiphae itself are labelled. An object's position on the horizontal axis indicates its distance from Jupiter. The vertical axis indicates its
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.
400:
which subsequently broke up after a collision. The original asteroid was not disturbed heavily: the original body is calculated to have been 60 km in
690:
473:, known for both Pasiphae and Sinope, could shape the orbits and provide the explanation for the post-collision dispersal of the orbital elements.
510:
Edited by Fran
Bagenal, Timothy E. Dowling, William B. McKinnon. Cambridge planetary science, Vol. 1, Cambridge, UK: Cambridge University Press,
1399:
522:
515:
443:
This diagram compares the wide dispersion of the
Pasiphae group (red) with the more compact Ananke (blue) and Carme (green) groups.
381:
683:
1394:
1343:
1389:
1362:
676:
1384:
542:
430:
469:
Nesvorný 2003, concurring on the Ananke and Carme groups, lists only
Megaclite for Pasiphae. However,
1233:
585:
289:
75:
29:
439:
44:
25:
609:
404:, about the same size as Pasiphae; Pasiphae retains 99% of the original body's mass. However, if
519:
19:
1312:
1120:
601:
569:
511:
492:
470:
420:
137:
41:
1338:
1012:
987:
962:
699:
593:
424:
153:
1270:
1263:
1238:
1080:
1041:
967:
898:
842:
794:
777:
770:
732:
727:
573:
526:
496:
214:
184:
105:
63:
56:
635:
589:
427:) also suggest that the group could have a more complex origin than a single collision.
1307:
1287:
1155:
1036:
1007:
952:
927:
917:
830:
747:
244:
169:
576:(May 5, 2003). "An abundant population of small irregular satellites around Jupiter".
66:(distances from Jupiter) range between 22.6 and 24.3 million km (similar range as the
1378:
1292:
1258:
1160:
1135:
1110:
1105:
1029:
1017:
977:
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229:
1322:
1317:
1297:
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1214:
1179:
1130:
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1056:
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1002:
957:
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937:
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412:
349:
259:
71:
67:
1253:
1248:
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1204:
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1184:
1115:
1090:
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1070:
1065:
1022:
997:
982:
972:
932:
922:
873:
857:
852:
823:
364:
334:
319:
304:
274:
1282:
756:
396:
The
Pasiphae group is believed to have been formed when Jupiter captured an
605:
1145:
1100:
661:
401:
397:
597:
1125:
48:
557:
1277:
1199:
668:
438:
429:
52:
672:
709:
Listed in increasing approximate distance from
Jupiter
628:
Collisional Origin of
Families of Irregular Satellites
408:
belongs to the group, the ratio is much smaller, 87%.
460:
Negative periods are indicative of retrograde motion.
649:
Grav, Tommy; Holman, Matthew J.; Gladman, Brett J.;
1331:
1223:
1055:
907:
891:
866:
803:
787:
746:
715:
508:Jupiter. The planet, satellites and magnetosphere.
626:David Nesvorný, Cristian Beaugé, and Luke Dones
654:Photometric survey of the irregular satellites
684:
8:
691:
677:
669:
645:
643:
83:
59:and are thought to have a common origin.
18:
541:, Scott S. Sheppard Carnegie Science,
485:
453:
81:The members of the Pasiphae group are:
504:Jupiter's outer satellites and Trojans
74:between 141.5° and 157.3°, and their
7:
116:largest member and group prototype
14:
554:Planetary Satellite Mean Elements
1357:
1356:
382:International Astronomical Union
384:(IAU) reserves names ending in
556:, Jet Propulsion Laboratory,
1:
1400:Moons with a retrograde orbit
630:, The Astronomical Journal,
559:, Retrieved 25 January 2024
544:, Retrieved 25 January 2024
1416:
1344:Jupiter's moons in fiction
388:for all retrograde moons.
1352:
706:
16:Group of Jupiter's moons
78:between 0.22 and 0.44.
634:(2004), pp. 1768–1783
444:
436:
33:
518:, 2004, p. 263 - 280
442:
433:
22:
1395:Irregular satellites
660:,(2003), pp. 33-45.
51:that follow similar
45:irregular satellites
598:10.1038/nature01584
590:2003Natur.423..261S
537:Scott S. Sheppard
570:Sheppard, Scott S.
525:2007-06-14 at the
471:secular resonances
445:
437:
34:
1372:
1371:
584:(6937): 261–263.
493:Scott S. Sheppard
378:
377:
1407:
1390:Moons of Jupiter
1360:
1359:
1339:Rings of Jupiter
700:Moons of Jupiter
693:
686:
679:
670:
664:
647:
638:
624:
618:
617:
574:Jewitt, David C.
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560:
551:
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539:Moons of Jupiter
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1327:
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903:
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867:Carpo group (2)
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625:
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527:Wayback Machine
520:Full text(pdf).
497:David C. Jewitt
491:
487:
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477:
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164:reddish colour
148:reddish colour
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64:semi-major axes
17:
12:
11:
5:
1413:
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1385:Pasiphae group
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1008:Jupiter LXVIII
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748:Galilean moons
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76:eccentricities
40:is a group of
38:Pasiphae group
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1259:Jupiter LXVII
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1234:Philophrosyne
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1161:Jupiter LXXII
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1106:Jupiter LXIII
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811:
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805:Himalia group
802:
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792:
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786:
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651:Aksnes, Kaare
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516:0-521-81808-7
513:
509:
505:
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501:Carolyn Porco
498:
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486:
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472:
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457:
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447:
441:
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428:
426:
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418:
417:Ananke groups
414:
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290:Philophrosyne
288:
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31:
27:
21:
1361:
1269:
1268:
1224:
1195:Jupiter LXVI
1166:
1165:
1086:Jupiter LXIX
1028:
1027:
993:Jupiter LXIV
909:Ananke group
879:
878:
829:
828:
776:
769:
762:
755:
708:
657:
653:
631:
627:
622:
581:
577:
564:
553:
549:
538:
533:
507:
503:
488:
465:
456:
410:
395:
385:
379:
80:
72:inclinations
61:
37:
35:
30:Eccentricity
1318:S/2003 J 23
1298:Jupiter LIX
1244:Jupiter LVI
1215:S/2003 J 10
1180:Jupiter LXI
1096:S/2003 J 24
1057:Carme group
1047:Jupiter LXX
1003:S/2003 J 12
958:S/2003 J 16
943:Jupiter LIV
938:Jupiter LII
716:Inner moons
411:Unlike the
350:S/2003 J 23
132:red colour
68:Carme group
26:inclination
1379:Categories
1313:Callirrhoe
1254:S/2016 J 4
1249:S/2003 J 4
1210:S/2021 J 5
1205:S/2018 J 3
1190:S/2003 J 9
1185:Jupiter LI
1121:Kallichore
1116:S/2021 J 4
1091:S/2021 J 6
1076:S/2016 J 3
1071:S/2022 J 2
1066:S/2022 J 1
1023:S/2003 J 2
998:S/2021 J 1
983:S/2021 J 2
973:S/2022 J 3
933:S/2021 J 3
923:Jupiter LV
874:S/2018 J 4
853:S/2011 J 3
824:S/2018 J 2
656:, Icarus,
636:Full text.
481:References
421:Callirrhoe
365:S/2016 J 4
335:S/2003 J 4
320:S/2017 J 6
305:S/2017 J 1
275:S/2011 J 2
138:Callirrhoe
42:retrograde
1283:Megaclite
1013:Thelxinoe
988:Praxidike
963:Harpalyke
425:Megaclite
154:Megaclite
70:), their
1363:Category
1332:See also
1271:Pasiphae
1264:Hegemone
1239:Eurydome
1146:Eukelade
1101:Chaldene
1081:Pasithee
1042:Hermippe
968:Orthosie
899:Valetudo
892:Valetudo
843:Lysithea
795:Themisto
788:Themisto
778:Callisto
771:Ganymede
733:Amalthea
728:Adrastea
662:Preprint
606:12748634
523:Archived
402:diameter
398:asteroid
215:Hegemone
185:Eurydome
106:Pasiphae
90:Diameter
57:Pasiphae
1308:Autonoe
1288:Cyllene
1156:Taygete
1126:Erinome
1037:Iocaste
953:Euanthe
928:Eupheme
918:Euporie
831:Himalia
614:4424447
586:Bibcode
372:–727.01
357:–760.00
342:–718.10
327:–733.99
312:–756.41
297:–702.54
282:–718.32
267:–776.76
252:–751.97
245:Cyllene
237:–761.42
222:–739.81
207:–748.29
192:–717.31
177:–761.00
170:Autonoe
161:–752.86
145:–758.87
129:–758.85
113:–743.61
49:Jupiter
1293:Sinope
1278:Sponde
1200:Kalyke
1136:Eirene
1111:Isonoe
1030:Ananke
1018:Thyone
978:Helike
838:Pandia
764:Europa
612:
604:
578:Nature
514:
506:, In:
435:sizes.
406:Sinope
392:Origin
200:Sponde
122:Sinope
100:Notes
97:(days)
95:Period
62:Their
53:orbits
1303:Aoede
1175:Herse
1168:Carme
1151:Arche
1141:Aitne
948:Mneme
881:Carpo
848:Elara
738:Thebe
723:Metis
610:S2CID
448:Notes
413:Carme
230:Aoede
1323:Kore
1227:(18)
1131:Kale
1059:(30)
911:(26)
819:Ersa
814:Leda
602:PMID
512:ISBN
423:and
415:and
380:The
260:Kore
92:(km)
87:Name
36:The
858:Dia
807:(9)
658:166
632:127
594:doi
582:423
55:to
47:of
1381::
757:Io
642:^
608:.
600:.
592:.
580:.
572:;
499:,
495:,
386:-e
126:38
110:58
28:.
692:e
685:t
678:v
616:.
596::
588::
369:1
354:2
339:2
324:2
309:2
294:2
279:1
264:2
249:2
234:4
219:3
204:2
189:3
174:4
158:6
142:7
Text is available under the Creative Commons Attribution-ShareAlike License. Additional terms may apply.
