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706:. This appears to consist primarily of material that is ejected from the surfaces of Jupiter's four small inner satellites by meteorite impacts. It is easy for the impact ejecta to be lost from these satellites into space. This is due to the satellites' low density and their surfaces lying close to the edge of their
527:
620:
Adrastea has an irregular shape and measures 20×16×14 km across. A surface area estimate would be between 840 and 1,600 (~1,200) km. This makes it the smallest of the four inner moons. The bulk, composition, and mass of
Adrastea are not known, but assuming that its mean density is like that of
713:
It seems that
Adrastea is the most copious source of this ring material, as evidenced by the densest ring (the main ring) being located at and within Adrastea's orbit. More precisely, the orbit of Adrastea lies near the outer edge of Jupiter's main ring. The exact extent of visible ring material
965:
Anderson, J. D.; Johnson, T. V.; Schubert, G.; Asmar, S.; Jacobson, R. A.; Johnston, D.; Lau, E. L.; Lewis, G.; Moore, W. B.; Taylor, A.; Thomas, P. C.; Weinwurm, G. (27 May 2005). "Amalthea's
Density is Less Than That of Water".
1305:
1011:
Burns, Joseph A.; Showalter, Mark R.; Hamilton, Douglas P.; Nicholson, Philip D.; de Pater, Imke; Ockert-Bell, Maureen E.; Thomas, Peter C. (14 May 1999). "The
Formation of Jupiter's Faint Rings".
671:, Adrastea rotates synchronously with its orbital period, keeping one face always looking toward the planet. Its long axis is aligned towards Jupiter, this being the lowest energy configuration.
1303:
1236:
Thomas, P. C.; Burns, J. A.; Rossier, L.; Simonelli, D.; Veverka, J.; Chapman, C. R.; Klaasen, K.; Johnson, T. V.; Belton, M. J. S.; Galileo Solid State
Imaging Team (September 1998).
1304:
43:
690:
are slowly causing its orbit to decay so that it will one day impact
Jupiter. If its density is similar to Amalthea's then its orbit would actually lie within the fluid
158:
558:. Although it appeared only as a dot, it was the first moon to be discovered by an interplanetary spacecraft. Soon after its discovery, two other of the inner
543:
608:, it is almost entirely focused on observations of Jupiter itself. However, if all goes well, it should be able to capture some limited images of the moons
1082:
Evans, M. W.; Porco, C. C.; Hamilton, D. P. (September 2002). "The Orbits of Metis and
Adrastea: The Origin and Significance of their Inclinations".
2066:
1277:
1048:
Burns, Joseph A.; Simonelli, Damon P.; Showalter, Mark R.; Hamilton, Douglas P.; Porco, Carolyn C.; Throop, Henry; Esposito, Larry W. (2004).
625:, around 0.86 g/cm, its mass can be estimated at 2 × 10 kg. Amalthea's density implies that the moon is composed of water
2076:
652:
at 70,200 mph at a radius of about 129,000 km (80,000 mi) (1.806 Jupiter radii) at the exterior edge of the planet's
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was able to determine the moon's shape in 1998, but the images remain poor. In 1983, Adrastea was officially named after the Greek nymph
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Ockert-Bell, M. E.; Burns, J. A.; Daubar, I. J.; Thomas, P. C.; Veverka, J.; Belton, M. J. S.; Klaasen, K. P. (1 April 1999).
1072:
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1103:
Jewitt, David C.; Danielson, G. Edward; Synnott, Stephen P. (November 23, 1979). "Discovery of a New
Jupiter Satellite".
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510:, very little is known about the moon's physical characteristics other than its size and the fact that it is
722:(which reveals much bigger particles) there appears to also be a narrow ringlet outside Adrastea's orbit.
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known to orbit its planet in less than the length of that planet's day. It orbits at the edge of
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534:. Adrastea is the fainter dot, in the very middle, straddling the line of the Jovian rings.
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No surface details of
Adrastea are known, due to the low resolution of available images.
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1203:"The Structure of Jupiter's Ring System as Revealed by the Galileo Imaging Experiment"
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was created from a revision of this article dated 1 March 2021
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1055:. In Bagenal, Fran; Dowling, Timothy E.; McKinnon, William B. (eds.).
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probe photographs taken on July 8, 1979, and received the designation
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For the moon of
Jupiter known by this name between 1955 and 1975, see
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orbiter, which arrived at Jupiter in 2016, has a camera called
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Hansen, C. J.; Orton, G. S. American Geophysical Union 12/2015
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and is thought to be the main contributor of material to the
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Adrastea is the smallest and second-closest member of the
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to be discovered from images taken by an interplanetary
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Discovery image of Adrastea, taken on July 8, 1979, by
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Listed in increasing approximate distance from Jupiter
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relative to Jupiter's equator of 0.03°, respectively.
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JunoCam: Science and Outreach Opportunities with Juno
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1057:Jupiter: The Planet, Satellites and Magnetosphere
774:Plutarch's lives: the translation called Dryden's
718:Adrastea is firmly outside the main ring, but in
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1059:. Cambridge University Press. pp. 241–262.
871:
856:
503:. Despite observations made in the 1990s by the
762:A Practical Dictionary of the English Language
1361:
1084:Bulletin of the American Astronomical Society
714:depends on the phase angle of the images: in
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741:Calculated on the basis of other parameters.
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456:. It was discovered in photographs taken by
615:
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1331:, and does not reflect subsequent edits.
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1177:Marsden, Brian G. (September 30, 1983).
633:of 10–15%, and Adrastea may be similar.
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491:Adrastea is one of the few moons in the
2067:Astronomical objects discovered in 1979
1238:"The Small Inner Satellites of Jupiter"
1148:Marsden, Brian G. (February 25, 1980).
313:20 × 16 × 14 km
2054:
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760:as "Adrastia" in Noah Webster (1884)
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54:between November 1996 and June 1997
13:
2077:Discoveries by G. Edward Danielson
1301:
1179:"Satellites of Jupiter and Saturn"
674:The orbit of Adrastea lies inside
14:
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698:Relationship with Jupiter's rings
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26:For the main-belt asteroid, see
1282:NASA's Solar System Exploration
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2072:Discoveries by David C. Jewitt
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1:
1033:10.1126/science.284.5417.1146
950:Ockert-Bell Burns et al. 1999
748:
656:. Its orbit has a very small
646:inner Jovian satellite family
462:in 1979, making it the first
1125:10.1126/science.206.4421.951
1050:"Jupiter's Ring-Moon System"
923:Anderson Johnson et al. 2005
896:Jewitt Danielson et al. 1979
7:
2082:Moons with a prograde orbit
935:Burns Showalter et al. 1999
824:Burns Simonelli et al. 2004
538:Adrastea was discovered by
47:Image of Adrastea taken by
10:
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2021:Jupiter's moons in fiction
522:Discovery and observations
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303:Physical characteristics
988:10.1126/science.1110422
793:Evans Porco et al. 2002
716:forward-scattered light
481:—the equivalent of the
474:, foster mother of the
350:Synodic rotation period
209:Orbital characteristics
1309:
1289:Listen to this article
1263:10.1006/icar.1998.5976
1228:10.1006/icar.1998.6072
686:'s), and as a result,
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454:inner moons of Jupiter
286:(to Jupiter's equator)
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1340:More spoken articles
720:back-scattered light
555:S/1979 J 1
342:≈ 2345 km
1254:1998Icar..135..360T
1219:1999Icar..138..188O
1117:1979Sci...206..951J
1096:2002DPS....34.2403E
1065:2004jpsm.book..241B
1025:1999Sci...284.1146B
1019:(5417): 1146–1150.
980:2005Sci...308.1291A
974:(5726): 1291–1293.
772:A.H. Clough (1905)
544:G. Edward Danielson
497:Jupiter's main ring
86:Discovery date
78:G. Edward Danielson
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1150:"Editorial Notice"
587:, the daughter of
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66:Discovered by
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1197:(naming the moon)
1074:978-0-521-81808-7
776:, vol. 3, p. 238.
680:synchronous orbit
464:natural satellite
446:), also known as
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2016:Rings of Jupiter
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1492:
1489:
1488:
1486:
1483:
1482:Himalia group
1479:
1473:
1470:
1469:
1467:
1463:
1457:
1456:
1452:
1450:
1449:
1445:
1443:
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1438:
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1422:
1416:
1413:
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1408:
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1403:
1401:
1398:
1397:
1395:
1391:
1387:
1382:
1378:
1371:
1366:
1364:
1359:
1357:
1352:
1351:
1348:
1341:
1337:
1322:
1283:
1279:
1276:
1275:
1264:
1259:
1255:
1251:
1247:
1243:
1239:
1234:
1229:
1224:
1220:
1216:
1212:
1208:
1204:
1199:
1188:
1184:
1180:
1175:
1164:on 2011-07-25
1163:
1159:
1155:
1151:
1146:
1142:
1138:
1134:
1130:
1126:
1122:
1118:
1114:
1111:(4421): 951.
1110:
1106:
1101:
1097:
1093:
1089:
1085:
1080:
1076:
1070:
1066:
1062:
1058:
1051:
1046:
1042:
1038:
1034:
1030:
1026:
1022:
1018:
1014:
1009:
1005:
1001:
997:
993:
989:
985:
981:
977:
973:
969:
963:
962:
961:
960:
959:Cited sources
951:
946:
944:
936:
931:
924:
919:
917:
909:
904:
897:
892:
890:
882:
877:
875:
867:
862:
860:
852:
847:
845:
843:
841:
839:
837:
835:
833:
825:
820:
818:
816:
814:
812:
810:
808:
806:
804:
802:
794:
789:
787:
785:
783:
775:
769:
763:
757:
753:
738:
736:
731:
723:
721:
717:
711:
709:
705:
695:
693:
689:
685:
681:
677:
672:
670:
669:tidal locking
665:
663:
659:
655:
651:
647:
637:
634:
632:
628:
624:
613:
611:
607:
603:
602:
598:Although the
596:
594:
590:
586:
582:
580:
575:
574:
569:
565:
561:
557:
551:
550:
545:
541:
533:
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519:
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509:
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498:
494:
489:
487:
484:
480:
477:
473:
469:
465:
461:
460:
455:
451:
443:
407:
398:
395:≈ 122 K
394:
392:
388:
378:
376:
372:
368:
365:
360:
357:
354:
351:
346:
340:
338:
334:
324:
321:
316:
312:
310:
306:
301:
298:
295:
293:
289:
283:
281:
277:
273:
270:
269:orbital speed
264:
252:
249:
244:
238:
236:
232:
222:
219:
213:
210:
206:
201:
162:
160:
156:
153:
150:
147:
141:
136:
101:
99:Pronunciation
97:
92:
88:
84:
77:
75:
72:
71:
69:
67:
63:
58:
53:
51:
44:
39:
33:
29:
22:
21:Ananke (moon)
2038:
1946:
1945:
1872:Jupiter LXVI
1843:
1842:
1763:Jupiter LXIX
1705:
1704:
1670:Jupiter LXIV
1586:Ananke group
1556:
1555:
1506:
1505:
1453:
1446:
1439:
1432:
1404:
1385:
1245:
1241:
1210:
1206:
1190:. Retrieved
1186:
1183:IAU Circular
1182:
1166:. Retrieved
1162:the original
1157:
1154:IAU Circular
1153:
1108:
1104:
1087:
1083:
1056:
1016:
1012:
971:
967:
958:
957:
930:
903:
773:
768:
761:
756:
712:
708:Hill spheres
701:
688:tidal forces
673:
666:
658:eccentricity
648:. It orbits
643:
635:
619:
599:
597:
578:
571:
553:
547:
537:
531:
505:
493:Solar System
490:
457:
447:
405:
404:
235:Eccentricity
151:
94:Designations
49:
32:
28:239 Adrastea
1995:S/2003 J 23
1975:Jupiter LIX
1921:Jupiter LVI
1892:S/2003 J 10
1857:Jupiter LXI
1773:S/2003 J 24
1734:Carme group
1724:Jupiter LXX
1680:S/2003 J 12
1635:S/2003 J 16
1620:Jupiter LIV
1615:Jupiter LII
1393:Inner moons
1173:(discovery)
692:Roche limit
662:inclination
391:Temperature
356:synchronous
330:2.0 km
320:Mean radius
280:Inclination
274:31.378 km/s
216:Mean orbit
144:Named after
89:8 July 1979
2056:Categories
1990:Callirrhoe
1931:S/2016 J 4
1926:S/2003 J 4
1887:S/2021 J 5
1882:S/2018 J 3
1867:S/2003 J 9
1862:Jupiter LI
1798:Kallichore
1793:S/2021 J 4
1768:S/2021 J 6
1753:S/2016 J 3
1748:S/2022 J 2
1743:S/2022 J 1
1700:S/2003 J 2
1675:S/2021 J 1
1660:S/2021 J 2
1650:S/2022 J 3
1610:S/2021 J 3
1600:Jupiter LV
1551:S/2018 J 4
1530:S/2011 J 3
1501:S/2018 J 2
1336:Audio help
1327:2021-03-01
1192:2012-03-28
1168:2012-03-28
749:References
581:spacecraft
508:spacecraft
468:spacecraft
449:Jupiter XV
364:Axial tilt
309:Dimensions
163:Adrastean
159:Adjectives
52:spacecraft
1960:Megaclite
1690:Thelxinoe
1665:Praxidike
1640:Harpalyke
881:IAUC 3872
866:IAUC 3454
654:main ring
483:Roman god
476:Greek god
472:Adrasteia
152:Adrasteia
149:Ἀδράστεια
60:Discovery
2040:Category
2009:See also
1948:Pasiphae
1941:Hegemone
1916:Eurydome
1823:Eukelade
1778:Chaldene
1758:Pasithee
1719:Hermippe
1645:Orthosie
1576:Valetudo
1569:Valetudo
1520:Lysithea
1472:Themisto
1465:Themisto
1455:Callisto
1448:Ganymede
1410:Amalthea
1405:Adrastea
1338: ·
1133:17733911
1041:10325220
996:15919987
631:porosity
623:Amalthea
585:Adrastea
406:Adrastea
267:Average
228: km
36:Adrastea
1985:Autonoe
1965:Cyllene
1833:Taygete
1803:Erinome
1714:Iocaste
1630:Euanthe
1605:Eupheme
1595:Euporie
1508:Himalia
1325: (
1296:minutes
1250:Bibcode
1215:Bibcode
1141:6391249
1113:Bibcode
1105:Science
1092:Bibcode
1090:: 883.
1061:Bibcode
1021:Bibcode
1013:Science
976:Bibcode
968:Science
676:Jupiter
667:Due to
650:Jupiter
629:with a
606:JunoCam
579:Galileo
516:Jupiter
506:Galileo
486:Jupiter
297:Jupiter
258: d
50:Galileo
1970:Sinope
1955:Sponde
1877:Kalyke
1813:Eirene
1788:Isonoe
1707:Ananke
1695:Thyone
1655:Helike
1515:Pandia
1441:Europa
1242:Icarus
1207:Icarus
1139:
1131:
1071:
1039:
1004:924257
1002:
994:
593:Ananke
576:. The
375:Albedo
337:Volume
284:0.03°
240:0.0015
218:radius
1980:Aoede
1852:Herse
1845:Carme
1828:Arche
1818:Aitne
1625:Mneme
1558:Carpo
1525:Elara
1415:Thebe
1400:Metis
1137:S2CID
1053:(PDF)
1000:S2CID
726:Notes
684:Metis
640:Orbit
610:Metis
568:Metis
564:Thebe
384:0.045
254:0.298
2000:Kore
1904:(18)
1808:Kale
1736:(30)
1588:(26)
1496:Ersa
1491:Leda
1187:3872
1158:3454
1129:PMID
1069:ISBN
1037:PMID
992:PMID
601:Juno
589:Zeus
566:and
542:and
479:Zeus
380:0.10
369:zero
1535:Dia
1484:(9)
1280:by
1258:doi
1246:135
1223:doi
1211:138
1121:doi
1109:206
1029:doi
1017:284
984:doi
972:308
678:'s
627:ice
546:in
514:to
326:8.2
226:000
224:129
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1225::
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23:.
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