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Satelit Saturnus

Dari Wikipedia bahasa Indonesia, ensiklopedia bebas
Saturnus dan satelit-satelitnya.
Diagram ini menunjukkan orbit satelit ireguler Saturnus. Di tengah, orbit Titan, sebuah satelit yang reguler, ditandai dengan warna merah sebagai perbandingan.

Satelit-satelit Saturnus adalah satelit alami yang mengelilingi planet Saturnus. Satelit ini ukurannya bervariasi antara kurang dari 1 km hingga lebih besar dari planet Merkurius. Saturnus memiliki 146 satelit, Tujuh satelit cukup besar sehingga bersifat elipsoidal. Beberapa satelit terpenting Saturnus adalah Titan, satelit terbesar kedua di Tata Surya dengan atmosfer mirip Bumi yang kaya akan nitrogen dan bentang alam yang berisi danau-danau hidrokarbon dan jaringan sungai kering,[1] dan Enseladus, yang mengeluarkan gas dan debu dan mungkin memiliki air di wilayah kutub selatannya.[2]

Ukuran

[sunting | sunting sumber]
Satelit utama Saturnus, dibandingkan dengan Bulan
Nama
 Diameter
(km)[3]		 Massa
(kg)[4]		 Radius orbit
(km)[5]		 Periode orbit
(hari)[5]
Mimas396
(12% Bulan)		4×1019
(0.05% Bulan)		185,539
(48% Bulan)		0.9
(3% Bulan)
Enseladus504
(14% Bulan)		1.1×1020
(0.2% Bulan)		237,948
(62% Bulan)		1.4
(5% Bulan)
Tetis1,062
(30% Bulan)		6.2×1020
(0.8% Bulan)		294,619
(77% Bulan)		1.9
(7% Bulan)
Dione1,123
(32% Bulan)		1.1×1021
(1.5% Bulan)		377,396
(98% Bulan)		2.7
(10% Bulan)
Rea1,527
(44% Bulan)		2.3×1021
(3% Bulan)		527,108
(137% Bulan)		4.5
(20% Bulan)
Titan5,149
(148% Bulan)
(75% Mars)		1.35×1023
(180% Bulan)		1,221,870
(318% Bulan)		16
(60% Bulan)
Iapetus1,470
(42% Bulan)		1.8×1021
(2.5% Bulan)		3,560,820
(926% Bulan)		79
(290% Bulan)

Daftar

[sunting | sunting sumber]
Diagram orbit bulan-bulan Saturnus

Bulan-bulan Saturnus di daftar ini diurutkan berdasarkan periode orbit (atau sumbu semi-mayor), dari yang terpendek hingga terpanjang. Bulan yang cukup masif dilambangkan dengan huruf tebal, sedangkan bulan yang tidak beraturan dilambangkan dengan warna merah, oranye, dan abu-abu.

Lambang
†

Bulan es yang besar

 ♠

Titan

 ‡

Kelompok inuit

 ♦

Kelompok Gallic

 ♣

Kelompok norse

Bulan yang telah dikonfirmasi

[sunting | sunting sumber]
Urutan Label Nama Pengucapan Gambar Magnitudo absolut Diameter (km)[a] Massa
(×1015 kg) [b]		 Sumbu semi-mayor (km)[c] Periode orbit (h)[c][d] Inklinasi [c][e] Eksentrisitas Tahun penemuan[9] Penemu
[9]
1 S/2009 S 1—≈20?≈ 0,3< 0,0001≈ 117.000≈ 0,47≈ 0°≈ 02009Cassini[10]
(bulan kecil)—A noisy image showing a few bright dots marked by circles?0.04 hingga 0.4< 0,0001≈ 130.000≈ 0,55≈ 0°≈ 02006Cassini
2XVIII Pan/ˈpæn/A bright fuzzy band (rings of Saturn) is running from the left to right. In the center a bright irregularity shaped body is superimposed on its upper edge. A narrow grayish band, which is a part of the main band, partially covers the body.9.128,2±2,6
(34 × 31 × 20)		4,95±0,75133.584+0,575050.001°0,0000351990M. Showalter
3XXXV Daphnis/ˈdæfnɪs/Two bright bands run from the left to right. In the narrow gap between them (Keeler gap), which has wavy edges, a small oblong object can be seen.12.07,6±1,6
(9 × 8 × 6)		0,084±0,012136.505+0,59408≈ 0°≈ 02005Cassini
4XV Atlas/ˈætləs/An irregularly shaped body is fully illuminated. The body, which looks like a cone viewed from the south pole, is elongated downward.10.730,2±1,8
(41 × 35 × 19)		6,6±0,045137.670+0,601690.003°0,00121980Voyager 1
5XVI Prometheus/proʊˈmiːθiəs/An irregularly shaped oblong body is fully illuminated. It is elongated in the direction from the right to left. Its surface is covered by craters. There is valley at the top.6.586,2±5,4
(136 × 79 × 59)		159,5±1,5139.380+0,612990.008°0,00221980Voyager 1
6XVII Pandora/pænˈdɔːrə/An irregularly shaped body is half illuminated from the bottom. The terminator runs from the left to right. The surface is covered by numerous craters.6.681,4±3,0
(104 × 81 × 64)		137,1±1,9141.720+0,628500.050°0,00421980Voyager 1
7aXI Epimetheus/ɛpɪˈmiːθiəs/A partially-illuminated irregular body, which has a shape remotely resembling a cube. The body's surface consists of ridges and valleys and is covered by craters.5.6116,2±3,6
(130 × 114 × 106)		526,6±0,6151.422+0,694330.335°0,00981977J. Fountain, and S. Larson
7bX Janus/ˈdʒeɪnəs/An irregular body, whose outline looks like an approximate circle in this image. It is illuminated from the bottom-left. The terminator runs from the top-left to bottom-right. The surface is covered by craters.4.7179,0±2,8
(203 × 185 × 153)		1.897,5±0,6151.472+0,694660.165°0,00681966A. Dollfus
9LIII Aegaeon/iːˈdʒiːən/Image of Aegaeon.≈20.3?≈ 0,5≈ 0,0001167.500+0,808120.001°0,00022008Cassini
10I †Mimas/ˈmaɪməs/A spherical body is half illuminated from the left. The terminator runs from the top to bottom in the vicinity of the right limb. A large crater with a central peak sits on the terminator slightly to the right and above the center of the body. It makes the body look like the Death Star. There are numerous smaller craters.4.2396,4±0,8
(416 × 393 × 381)		37.493±31185.404+0,9424221.566°0,02021789W. Herschel
11XXXII Methone/mɪˈθoʊniː/From May 2012 flyby13.83,2±1,2≈ 0,02194.440+1,009570.007°0,00012004Cassini
12XLIX Anthe/ˈænθiː/14.81,8≈ 0,0015197.700+1,050890.1°0,00112007Cassini
13XXXIII Pallene/pəˈliːniː/In the center is Pallene, a moon of Saturn12.95,0±1,2
(6 × 6 × 4)		≈ 0,05212.280+1,153750.181°0,00402004Cassini
14II †Enseladus/ɛnˈsɛlədəs/A spherical body is half illuminated from the right. The terminator runs from the top to bottom in the vicinity of the left limb. In the center and at the top there are heavily cratered areas.1.7504,2±0,4
(513 × 503 × 497)		108.022±101237.950+1,3702180.010°0,00471789W. Herschel
15III †Tetis/ˈtiːθɪs/A spherical heavily cratered body is illuminated from the bottom. The terminator runs from the left to right in the vicinity of the top limb. There is a wide curved graben running from the center of the body to the bottom. It is Ithaca Chasma.0.31062±1,2
(1077 × 1057 × 1053)		617.449±132294.619+1,8878020.168°0,00011684G. Cassini
15aXIII Telesto/tɪˈlɛstoʊ/8.724,8±0,8
(33 × 24 × 20)		≈ 9,41294.619+1,8878021.158°0,00001980B. Smith, H. Reitsema, S. Larson, and J. Fountain
15bXIV Calypso/kəˈlɪpsoʊ/An oblong reddish body is seen in this low resolution image.8.721,4±1,4
(30 × 23 × 14)		≈ 6,3294.619+1,8878021.473°0,00001980D. Pascu, P. Seidelmann, W. Baum, and D. Currie
18IV †Dione/daɪˈoʊniː/A spherical body is half illuminated from the right. The terminator is running from the top to bottom slightly to the left off the center. The central part of the body is smooth and has only a few craters. A heavily cratered terrain is near the right limb. A part of a large crater is intersected by the terminator in the lower-left corner. To the left of it there is a long crack running parallel to the terminator.0.41.122,8±0,8
(1128 × 1123 × 1119)		1.095.452±168377.396+2,7369150.002°0,00221684G. Cassini
18aXII Helene/ˈhɛlɪniː/An irregularly shaped body illuminated from the left. Its surface is covered by numerous impact craters.7.335,2±0,8
(43 × 38 × 26)		≈ 24,46377.396+2,7369150.212°0,00221980P. Laques and J. Lecacheux
18bXXXIVPolydeuces/pɒliˈdjuːsiːz/A small oblong body is barely resolved in this image.13.52,6±0,8
(3 × 2 × 1)		≈ 0,03377.396+2,7369150.177°0,01922004Cassini
21V †Rea/ˈriːə/A spherical body is almost fully illuminated. The terminator is running near the top edge. The surface is covered by numerous craters. Two partially overlapping large craters can be seen above the center. One that is younger is above and to the right from the older one.-0.21.527,0±1,2
(1530 × 1526 × 1525)		2.306.518±353527.108+4,5182120.327°0,0012581672G. Cassini
22VI ♠Titan/ˈtaɪtən/-1.35.149,46±0,18
(5149 × 5149 × 5150)		134.520.000±20.0001.221.930+15,945420.3485°0,02881655C. Huygens
23VII †Hyperion/haɪˈpɪəriən/An irregularly shaped oblong body is illuminated from the left. The terminator is near the right limb. The body is elongated in the top-bottom direction. The surface is punctured by numerous impact craters, which make it look like a sponge or cheese.4.8270±8
(360 × 266 × 205)		5620±501.481.010+21,276610.568°0,1230061848W. Bond
G. Bond
W. Lassell
24VIII †Iapetus/aɪˈæpɪtəs/A walnut shaped body illuminated from the bottom-left. The terminator runs from the top to right along the top-right limb. An equatorial ridge runs from the left to right and is convex in the direction of the bottom-left. Above and below it there are dark areas. Above the upper dark area and below the lower one there are bright poles. There numerous craters. Three among them are very large: one sits on the limb at the right another is in the center above the ridge. The third is below the ridge near the left limb.0.61.468,6±5,6
(1491 × 1491 × 1424)		1.805.635±3753.560.820+79,321515.47°0,0286131671G. Cassini
25XXIV ‡Kiviuq/ˈkɪviək/12.7≈ 16≈ 2,7911.294.800+448,1649.087°0,32882000B. Gladman, J. Kavelaars, et al.
26XXII ‡Ijiraq/ˈiːɪrɒk/13.2≈ 12≈ 1,1811.355.316+451,7750.212°0,31612000B. Gladman, J. Kavelaars, et al.
27IX ♣†Phoebe/ˈfiːbiː/An approximately spherical heavily cratered body is illuminated from the bottom-right. The terminator runs near the left and top limbs. There is huge crater at the top, which affects the shape, and another slightly smaller at the bottom.2.0213,0±1,4
(219 × 217 × 204)		8292±1012.869.700−545,09173.047°0,1562421899W. Pickering
28XX ‡Paaliaq/ˈpɑːliɒk/11.9≈ 22≈ 7,2515.103.400+692,9846.151°0,36312000B. Gladman, J. Kavelaars, et al.
29XXVII ♣Skathi/ˈskɑːði/14.2≈ 8≈ 0,3515.672.500−732,52149.084°0,2462000B. Gladman, J. Kavelaars, et al.
30  ♣S/2004 S 37—15.9≈ 4≈ 0,0515.892.000−748,18162.937°0.49652019S. Sheppard, D. Jewitt, J. Kleyna
31  ♣S/2007 S 2—15.7≈ 4≈ 0,0516.055.000−759,71176.65°0,23702007S. Sheppard, D. Jewitt, J. Kleyna, B. Marsden
32XXVI ♦Albiorix/ˌælbiˈɒrɪks/11.4≈ 32≈ 22,316.266.700+774,5838.042°0,4772000M. Holman
33  ‡S/2004 S 29—15.8≈ 4≈ 0,0516.981.000+826,4445.102°0,44012019S. Sheppard, D. Jewitt, J. Kleyna, B. Marsden
34XXXVII ♦Bebhionn/bɛˈviːn/14.9≈ 6≈ 0,1517.153.520+838,7740.484°0,3332004S. Sheppard, D. Jewitt, J. Kleyna
35XXVIII ♦Erriapus/ɛriˈæpəs/13.7≈ 10≈ 0,6817.236.900+844,8938.109°0,47242000B. Gladman, J. Kavelaars, et al.
36XLVII ♣Skoll/ˈskɒl/15.4≈ 6≈ 0,1517.473.800−862,37155.624°0,4182006S. Sheppard, D. Jewitt, J. Kleyna
37  ‡S/2004 S 31—15.6≈ 4≈ 0,0517.568.000+869,6548.815°0,24032019S. Sheppard, D. Jewitt, J. Kleyna, B. Marsden
38XXIX ‡Siarnaq/ˈsiːɑːrnək/10.6≈ 40≈ 43,517.776.600+884,8845.798°0,249612000B. Gladman, J. Kavelaars, et al.
39LII ‡Tarqeq/ˈtɑːrkeɪk/14.8≈ 7≈ 0,2317.910.600+894,8649.904°0,10812007S. Sheppard, D. Jewitt, J. Kleyna
40 (hilang) ♣S/2004 S 13—15.6≈ 6≈ 0,1518.056.300
(18.183.000±2.020.000[11])		−905,85
(-915.47[11])		167.379°0,261
(0,2653±0,0809[11])		2004S. Sheppard, D. Jewitt, J. Kleyna
41LI ♣Greip/ˈɡreɪp/15.3≈ 6≈ 0,1518.065.700−906,56172.666°0,37352006S. Sheppard, D. Jewitt, J. Kleyna
42XLIV ♣Hyrrokkin/hɪˈrɒkɪn/14.3≈ 8≈ 0,3518.168.300−914,29153.272°0,36042006S. Sheppard, D. Jewitt, J. Kleyna
43L ♣Jarnsaxa/jɑːrnˈsæksə/15.7≈ 6≈ 0,1518.556.900−943,78162.861°0,19182006S. Sheppard, D. Jewitt, J. Kleyna
44XXI ♦Tarvos/ˈtɑːrvəs/12.8≈ 15≈ 2,318.562.800+944,2334.679°0,53052000B. Gladman, J. Kavelaars, et al.
45XXV ♣Mundilfari/mʊndəlˈværi/14.5≈ 7≈ 0,2318.725.800−956,70169.378°0,1982000B. Gladman, J. Kavelaars, et al.
46  ♣S/2006 S 1—15.5≈ 6≈ 0,1518.930.200−972,41154.232°0,13032006S. Sheppard, D.C. Jewitt, J. Kleyna
47 (hilang) ♣S/2004 S 17—16.0≈ 4≈ 0,0519.099.200
(19.080.000±685.000[11])		−985,45
(-984.11[11])		166.881°0,226
(0,2268±0,0440[11])		2004S. Sheppard, D. Jewitt, J. Kleyna
48XXXVIII ♣Bergelmir/bɛərˈjɛlmɪər/15.1≈ 6≈ 0,1519.104.000−985,83157.384°0,1522004S. Sheppard, D. Jewitt, J. Kleyna
49XXXI ♣Narvi/ˈnɑːrvi/14.6≈ 7≈ 0,2319.395.200−1.008,45137.292°0,3202003S. Sheppard, D. Jewitt, J. Kleyna
50  ♣S/2004 S 20—15.8≈ 3≈ 0,0319.418.000−1.010,55162.570°0,1972019S. Sheppard, D. Jewitt, J. Kleyna
51XXIII ♣Suttungr/ˈsʊtʊŋɡər/14.3≈ 7≈ 0,2319.579.000−1.022,82174.321°0,1312000B. Gladman, J. Kavelaars, et al.
52XLIII ♣Hati/ˈhɑːti/13.5≈ 6≈ 0,1519.709.300−1.033,05163.131°0,2912004S. Sheppard, D. Jewitt, J. Kleyna
53 (hilang) ♣S/2004 S 12—15.7≈ 5≈ 0,0919.905.900
(19.999.000±119.000[11])		−1.048,54
(-1056.23[11])		164.042°0,396
(0,3933±0,0223[11])		2004S. Sheppard, D. Jewitt, J. Kleyna
54  ♣S/2004 S 27—15.3≈ 6≈ 0,1519.976.000−1.054,45167.804°0,12202019S. Sheppard, D. Jewitt, J. Kleyna, B. Marsden, R. Jacobson
55XL ♣Farbauti/fɑːrˈbaʊti/15.6≈ 5≈ 0,0919.984.800−1.054,78158.361°0,2092004S. Sheppard, D. Jewitt, J. Kleyna
56XXX ♣Thrymr/ˈθrɪmər/14.3≈ 7≈ 0,2320.278.100−1.078,09174.524°0,4532000B. Gladman, J. Kavelaars, et al.
57  ♣S/2004 S 30—16.2≈ 3≈ 0,0320.396.000−1.087,84156.3°[12]0.11292019S. Sheppard, D. Jewitt, J. Kleyna
58XXXVI ♣Aegir/ˈaɪ.ɪər/15.4≈ 6≈ 0,1520.482.900−1.094,46167.425°0,2372004S. Sheppard, D. Jewitt, J. Kleyna
59 (hilang) ♣S/2007 S 3—15.7≈ 5≈ 0,0920.518.500
(19.202.000±519.000[11]		≈ −1100
(-993.50[11])		177.22°0,130
(0,1499±0,0336[11])		2007S. Sheppard, D. Jewitt, J. Kleyna
60XXXIX ♣Bestla/ˈbɛstlə/14.7≈ 7≈ 0,2320.570.000−1.101,45147.395°0,51452004S. Sheppard, D. Jewitt, J. Kleyna
61 (hilang) ♣S/2004 S 7—15.2≈ 6≈ 0,1520.576.700
(20.685.000±396.000[11])		−1.101,99
(−1.111,09[11])		165.596°0,5299
(0,5549±0,0212[11])		2004S. Sheppard, D. Jewitt, J. Kleyna
62  ♣S/2004 S 22—16.1≈ 3≈ 0,0320.636.000−1.107,132177.321°0,25132019S. Sheppard, D. Jewitt, J. Kleyna
63  ♣S/2004 S 23—15.6≈ 4≈ 0,0521.163.000−1.149,82176.988°0,37292019S. Sheppard, D. Jewitt, J. Kleyna
64  ♣S/2004 S 25—15.9≈ 4≈ 0,0521.174.000−1.150,69172.996°0,44242019S. Sheppard, D. Jewitt, J. Kleyna
65  ♣S/2004 S 32—15.6≈ 4≈ 0,0521.214.000−1.153,96159.091°0,25052019S. Sheppard, D. Jewitt, J. Kleyna
66  ♣S/2006 S 3—15.6≈ 6≈ 0,1521.308.000−1.161,65152.878°0,47072006S. Sheppard, D. Jewitt, J. Kleyna
67  ♣S/2004 S 38—15.9≈ 4≈ 0,0521.908.000−1.211,024154.090°0,43662019S. Sheppard, D. Jewitt, J. Kleyna
68XLI ♣Fenrir/ˈfɛnrɪər/15.9≈ 4≈ 0,0521.930.644−1.212,53162.832°0,1312004S. Sheppard, D. Jewitt, J. Kleyna
69  ♣S/2004 S 28—15.8≈ 4≈ 0,0522.020.000−1.220,31170.322°0,14282019S. Sheppard, D. Jewitt, J. Kleyna, B. Marsden
70XLVIII ♣Surtur/ˈsɜːrtər/15.7≈ 6≈ 0,1522.288.916−1.242,36166.918°0,36802006S. Sheppard, D. Jewitt, J. Kleyna
71XLV ♣Kari/ˈkɑːri/14.9≈ 7≈ 0,2322.321.200−1.245,06148.384°0,34052006S. Sheppard, D. Jewitt, J. Kleyna
72  ♣S/2004 S 3515.5≈ 6≈ 0,1522.412.000−1.253,08176.717°0,18372019S. Sheppard, D. Jewitt, J. Kleyna, B. Marsden
73XIX ♣Ymir/ˈɪmɪər/12.3≈ 18≈ 3,9722.429.673−1.254,15172.143°0,33492000B. Gladman, J. Kavelaars, et al.
74  ♣S/2004 S 21—16.3≈ 3≈ 0,0322.645.000−1.272,61159.950°0,31832019S. Sheppard, D. Jewitt, J. Kleyna
75  S/2004 S 24—16.0≈ 3≈ 0,0322.901.000+1.294,2535.538°0.08462019S. Sheppard, D. Jewitt, J. Kleyna, B. Marsden
76XLVI ♣Loge/ˈlɔɪ.eɪ/15.4≈ 6≈ 0,1522.984.322−1.300,95166.539°0,13902006S. Sheppard, D. Jewitt, J. Kleyna
77  ♣S/2004 S 36—16.1≈ 3≈ 0,0323.192.000−1.319,07154.992°0,74842019S. Sheppard, D. Jewitt, J. Kleyna
78  ♣S/2004 S 39—16.3≈ 3≈ 0,0323.575.000−1.351,83166.579°0.08042019S. Sheppard, D. Jewitt, J. Kleyna
79  ♣S/2004 S 33—15.9≈ 4≈ 0,0524.168.000−1.403,18160.471°0,39942019S. Sheppard, D. Jewitt, J. Kleyna
80  ♣S/2004 S 34—16.1≈ 3≈ 0,0324.299.000−1.414,59166.039°0,23522019S. Sheppard, D. Jewitt, J. Kleyna
81XLII ♣Fornjot/ˈfɔːrnjɒt/15.3≈ 6≈ 0,1524.504.879−1.432,16167.886°0,1862004S. Sheppard, D. Jewitt, J. Kleyna
82  ♣S/2004 S 26—15.8≈ 4≈ 0,0526.676.000−1.627,18171.369°0,16452019S. Sheppard, D. Jewitt, J. Kleyna, B. Marsden

Bulan yang belum dikonfirmasi

[sunting | sunting sumber]

Benda-benda berikut (diamati oleh Cassini) belum dikonfirmasi sebagai satelit Saturnus. Belum jelas apakah ini benar-benar satelit atau gumpalan dalam Cincin F.[13]

Nama Gambar Diameter (km) Sumbu semi-mayor (km)[7] Periode orbit (h)[7] Posisi Tahun Penemuan
S/2004 S 6 A bright narrow band runs from the top to bottom. To the right of it in the diffuse halo the is a bright small object. ≈ 3–5 ≈ 140.130 +0,61801 benda tidak jelas di sekitar Cincin F. 2004
S/2004 S 3/S 4 ≈ 3–5 ≈ 140.300 ≈ +0,619 2004
S/2001 S 7 ??? ??? ??? Cincin F 2001
S/2001 S 4 ??? 122 124 0.633 19 Cincin F 2001

Catatan kaki

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  1. ↑ Diameter dan dimensi dari satelit bagian dalam: Pan, Janus, Methone, Pallene, Telepso, Calypso, Helene, Hyperion dan Phoebe diambil dari Thomas 2010, Tabel 3.[3] Diameter dan dimensi Mimas, Enseladus, Tetis, Dione, Rea, dan Iapetus diambil dari Thomas 2010, Tabel 1.[3] Perkiraan ukuran satelit Saturnus lainnya berasal dari situs web Scott Sheppard.[6]
  2. ↑ Massa dari bulan-bulan besar diambil dari Jacobson, 2006.[4] Massa Pan, Daphnis, Atlas, Prometheus, Pandora, Epimetheus, Janus, Hyperion dan Phoebe diambil dari Thomas, 2010, Tabel 3.[3] Massa bulan-bulan kecil lainnya dihitung dengan asumsi massa jenis 1.3 g/cm3.
  3. 1 2 3 Parameter orbit diambil dari Spitale, et al. 2006,[7] IAU-MPC Natural Satellites Ephemeris Service,[8] dan NASA/NSSDC.[5]
  4. ↑ Periode orbit negatif menunjukkan orbit retrograde di sekitar Saturnus (berlawanan dengan rotasi planet).
  5. ↑ Ke ekuator Saturnus untuk satelit reguler, dan ke ekliptika untuk satelit ireguler.

Referensi

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  1. ↑ Science, Nola Taylor Redd 2018-03-27T01:32:00Z; Astronomy. "Titan: Facts About Saturn's Largest Moon". Space.com (dalam bahasa Inggris). Diakses tanggal 2019-11-09. Pemeliharaan CS1: Nama numerik: authors list (link)
  2. ↑ "Enceladus". NASA Solar System Exploration. Diakses tanggal 2019-11-09.
  3. 1 2 3 4 Thomas, P. C. (July 2010). "Sizes, shapes, and derived properties of the saturnian satellites after the Cassini nominal mission" (PDF). Icarus. 208 (1): 395–401. Bibcode:2010Icar..208..395T. doi:10.1016/j.icarus.2010.01.025. Diarsipkan dari asli (PDF) tanggal 2018-12-23. Diakses tanggal 2019-11-09. ;
  4. 1 2 Jacobson, R. A.; Antreasian, P. G.; Bordi, J. J.; Criddle, K. E.; Ionasescu, R.; Jones, J. B.; Mackenzie, R. A.; Meek, M. C.; Parcher, D.; Pelletier, F. J.; Owen, Jr., W. M.; Roth, D. C.; Roundhill, I. M.; Stauch, J. R. (December 2006). "The Gravity Field of the Saturnian System from Satellite Observations and Spacecraft Tracking Data". The Astronomical Journal. 132 (6): 2520–2526. Bibcode:2006AJ....132.2520J. doi:10.1086/508812.
  5. 1 2 3 Williams, David R. (August 21, 2008). "Saturnian Satellite Fact Sheet". NASA (National Space Science Data Center). Diakses tanggal April 27, 2010.
  6. ↑ Sheppard, Scott S. "Saturn's Known Satellites". Diarsipkan dari asli tanggal Mei 15, 2011. Diakses tanggal Januari 7, 2010.
  7. 1 2 3 Spitale, J. N.; Jacobson, R. A.; Porco, C. C.; Owen, W. M., Jr. (2006). "The orbits of Saturn's small satellites derived from combined historic and Cassini imaging observations" (PDF). The Astronomical Journal. 132 (2): 692–710. Bibcode:2006AJ....132..692S. doi:10.1086/505206. Pemeliharaan CS1: Banyak nama: authors list (link)
  8. ↑ "Natural Satellites Ephemeris Service". IAU: Minor Planet Center. Diakses tanggal 2011-01-08.
  9. 1 2 "Planet and Satellite Names and Discoverers". Gazetteer of Planetary Nomenclature. USGS Astrogeology. July 21, 2006. Diakses tanggal August 6, 2006.
  10. ↑ Porco, C. and the Cassini Imaging Team (November 2, 2009). "S/2009 S1". IAU Circular. 9091. Diarsipkan dari asli tanggal 2011-06-11. Diakses tanggal 2013-08-17.
  11. 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 Gray, Bill. "Find_Orb Orbit determination software". projectpluto.com. Diakses tanggal 7 October 2019.
  12. ↑ Sheppard, Scott. "Scott S. Sheppard - SaturnMoons". sites.google.com. Diakses tanggal 7 October 2019.
  13. ↑ Porco, C. C.; Baker, E.; Barbara, J.; et al. (2005). "Cassini Imaging Science: Initial Results on Saturn's Rings and Small Satellites" (PDF). Science. 307 (5713): 1226–36. Bibcode:2005Sci...307.1226P. doi:10.1126/science.1108056. PMID 15731439.

Pranala luar

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