Saturnus se natuurlike satelliete: Verskil tussen weergawes

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Wysiging soos op 00:02, 17 Januarie 2013

Saturnus het ses-en-vyftig bevestigde natuurlike satelliete, plus drie onbevestigde mane.

Tabel van bevestigde mane

Die Saturniese mane word hier volgens wentelperiode gelys, van die kortste tot die langste. Mane wat so groot is dat hulle oppervlak in 'n sferoïde ingestort het word uitgelig deur 'n ligpers kleur. Titan, wat die grootte van 'n planeet het, is met 'n donkerder kleur uitgewys. Die ongewone (gevange) mane is in grys aangewys: lig grys vir satelliete wat saam met die planeet wentel en donker grys vir planete wat teen die planeet se wenteling wentel.

Orde Naam (sferoïdeise mane vetgedruk)
 Beeld Diameter (km) Semi-belangrike
as (km) 		Wentel-
periode (d) 		Inklinasie (Graad °)
(tot Saturnus
se ewenaar) 		Posisie Ontdekking
1 XVIII Pan
30 (35 × 35 × 23) [1] 133,584 [2] +0.57505 [2] 0.000° In Encke-
divisie		 1990
2 XXXV Daphnis
6 - 8 136,505 [2] +0.59408 [2] 0.000° In Keeler-
gaping		 2005
3 XV Atlas
31 (46 × 38 × 19) [1] 137,670 [2] +0.60169 [2] Buitenste A-Ring skaapwagter 1980
4 XVI Prometheus
86 (119 × 87 × 61) [1] 139,380 [2] +0.61299 [2] 0.000° Binneste F-ring skaapwagter 1980
*   S/2004 S 6 [3]
~3-5 140,130 [2] +0.61801 [2] *Twyfelagtige voorwerpe
om die F-ring		 2004
*   S/2004 S 4 [4] ~3-5 ~140,100 [5] +0.619 [6] 2004
*   S/2004 S 3 [3]
~3-5 ~140,300 [7] ~ +0.62 2004
5 XVII Pandora
81 (103 × 80 × 64) [1] 141,720 [2] +0.62850 [2] Buitenste F-ring skaapwagter 1980
6 XI Epimetheus 113 (135 × 108 × 105) [1] 151,422 [2] +0.69433 [2] 0.335° Gedeelde wentelbane 1980
7 X Janus
179 (193 × 173 × 137) [1] 151,472 [2] +0.69466 [2] 0.165° 1966
8 I Mimas
397 (415 × 394 × 381) [8] 185,404 [9] +0.942422 [10] 1.566°   1789
9 XXXII Methone
3 194,440 [2] +1.00957 [2]   2004
10 XXXIII Pallene
4 212,280 [2] +1.15375 [2]   2004
11 II Enceladus
504 (513 × 503 × 497) [8] 237,950 [9] +1.370218 [10] 0.010° In die middel van die E-ring 1789
12 III Tethys
1066 (1081 × 1062 × 1055) [8] 294,619 [9] +1.887802 [10] 0.168°   1684
12a XIII Telesto
24 (29 × 22 × 20) [1] 1.158° Lei Tethys 1980
12b XIV Calypso
21 (30 × 23 × 14) [1] 1.473° Op Tethys se spoor 1980
15 IV Dione
1123 (1128 × 1122 × 1121) [8] 377,396 [9] +2.736915 [10] 0.002°   1684
15a XII Helene
33 (36 × 32 × 30) 0.212° Lei Dione 1980
15b XXXIV Polydeuces
3.5 [11] Op Dione se spoor 2004
18 V Rhea
1529 (1535 × 1525 × 1526) [8] 527,108 [12] +4.518212 [12] 0.327°   1672
19 VI Titan
5151 1,221,930 [9] +15.94542 1.634°   1655
20 VII Hyperion
292 (360 × 280 × 225) 1,481,010 [9] +21.27661 0.568°   1848
21 VIII Iapetus
1472 (1494 × 1498 × 1425) [8] 3,560,820 +79.3215 [6] 7.570°   1671
22 XXIV Kiviuq ~16 11 294 800 [12] +448.16 [12] 49.087° Inuit groep 2000
23 XXII Ijiraq ~12 11 355 316 [12] +451.77 [12] 50.212° 2000
24 IX Phoebe
220 (230 × 220 × 210) 12 869 700 -545.09[6][13] 173.047° Noorse groep 1899
25 XX Paaliaq ~22 15 103 400 [12] +692.98 [12] 46.151° Inuit groep 2000
26 XXVII Skathi ~8 15 672 500 [12] -732.52 [10][13] 149.084° Noorse (Skathi) groep 2000
27 XXVI Albiorix ~32 16 266 700 [12] +774.58 [12] 38.042° Galliese groep 2000
28 XXXVII S/2004 S 11 ~6 17 153 520 [12] +838.77 [12] 40.484° Inuit groep 2004
29 XXVIII Erriapo ~10 17 236 900 [12] +844.89 [12] 38.109° Galliese groep 2000
30 XLVII S/2006 S 8 ~6 17 473 800 [9] -862.37 [12] 155.624° Noorse groep 2006
31 XXIX Siarnaq ~40 17 776 600 [12] +884.88 [12] 45.798° Inuit groep 2000
32   S/2004 S 13 ~6 18 056 300 [12] -905.85 [10][13] 167.379° Noorse groep 2004
33   S/2006 S 4 ~6 18 065 700 [9] -906.56 [12] 172.666° 2006
34 XLIV S/2004 S 19 ~8 18 168 300 [9] -914.29 [12] 153.272° 2006
35   S/2006 S 6 ~6 18 556 900 [9] -943.78 [12] 162.861° 2006
36 XXI Tarvos ~15 18 562 800 [12] +944.23 [12] 34.679° Galliese groep 2000
37 XXV Mundilfari ~7 18 725 800 [12] -956.70 [10][13] 169.378° Noorse groep 2000
38   S/2006 S 1 ~6 18 930 200 [9] -972.41 [12] 154.232° 2006
39   S/2004 S 17 ~4 19 099 200 [12] -985.45 [10][13] 166.881° 2004
40 XXXVIII S/2004 S 15 ~6 19 104 000 [12] -985.83 [10][13] 157.384° Noorse (Skathi) groep 2004
41 XXXI Narvi ~7 19 395 200 [12] -1008.45 [10][13] 137.292° Noorse groep 2003
42 XXIII Suttungr ~7 19 579 000 [12] -1022.82 [10][13] 174.321° 2000
43 XLIII S/2004 S 14 ~6 19 709 300 [12] -1033.05 [10][13] 163.131° 2004
44   S/2004 S 12 ~5 19 905 900 [12] -1048.54 [10][13] 164.042° 2004
45 XL S/2004 S 9 ~5 19 984 800 [12] -1054.78 [10][13] 158.361° Noorse (Skathi) groep 2004
46 XXX Thrymr ~7 20 278 100 [12] -1078.09 [10][13] 174.524° Noorse groep 2000
47 XXXVI S/2004 S 10 ~6 20 482 900 [12] -1094.46 [10][13] 167.425° 2004
48 XXXIX S/2004 S 18 ~7 20 570 000 [12] -1101.45 [10][13] 147.395° Noorse (Skathi) groep 2004
49   S/2004 S 7 ~6 20 576 700 [12] -1101.99 [10][13] 165.596° Noorse groep 2004
50   S/2006 S 3 ~6 21 076 300 [9] -1142.37 [12] 150.817° 2006
51 XLI S/2004 S 16 ~4 21 930 644 [12] -1212.53 [10][13] 162.832° 2004
52 XLVIII S/2006 S 7 ~6 22 288 916 [9] -1242.36 [12] 166.918° 2006
53 XLV S/2006 S 2 ~7 22 321 200 [9] -1245.06 [12] 148.384° 2006
54 XIX Ymir ~18 22 429 673 [12] -1254.15 [10][13] 172.143° 2000
55 XLVI S/2006 S 5 ~6 22 984 322 [9] -1300.95 [12] 166.539° 2006
56 XLII S/2004 S 8 ~6 24 504 879 [12] -1432.16 [10][13] 167.886° 2004

Verwysings

  1. ↑ 1,0 1,1 1,2 1,3 1,4 1,5 1,6 1,7 Physical characteristics and possible accretionary origins for Saturn's small satellites deur C.C. Porco. Soos verskyn in die Bulletin of the American Astronomical Society, 2006: 37, bl768.
  2. ↑ 2,00 2,01 2,02 2,03 2,04 2,05 2,06 2,07 2,08 2,09 2,10 2,11 2,12 2,13 2,14 2,15 2,16 2,17 2,18 2,19 The orbits of Saturn's small satellites derived from combined historic and Cassini imaging observations deur J.N. Spitale et al. Soos verskyn in The Astronomical Journal, 2006:132, bl. 692.
  3. ↑ 3,0 3,1 Dit is nog nie bekend of hierdie regte satelliete of net blywende klonte binne-in die F-ring is nie.
  4. ↑ S/2004 S4 was heel moontlik slegs 'n verbygaande klont - dit is sedert die eerste waarneming nog nie weer gesien nie.
  5. ↑ PGJ Astronomie webpage (Gilbert Javaux). Die F-ring is in die middel by ~140,180 km
  6. ↑ 6,0 6,1 6,2 Bereken vanaf die semi-belangrike as deur middel van die IAU-MPC Natural Satellites Ephemeris Service se µ-waarde
  7. ↑ Sien verwysings van S/2004 S 3
  8. ↑ 8,0 8,1 8,2 8,3 8,4 8,5 Source: Shapes of the Saturnian Icy Satellites. deur P.C. Thomas et al. 2006. Soos verskyn in Lunar and Planetary Science XXXVII (2006).]
  9. ↑ 9,00 9,01 9,02 9,03 9,04 9,05 9,06 9,07 9,08 9,09 9,10 9,11 9,12 9,13 9,14 Bereken vanaf die periode deur middel van die IAU-MPC Natural Satellites Ephemeris Servicese µ-waarde
  10. ↑ 10,00 10,01 10,02 10,03 10,04 10,05 10,06 10,07 10,08 10,09 10,10 10,11 10,12 10,13 10,14 10,15 10,16 10,17 10,18 10,19 10,20 Bron: NASA
  11. ↑ Source: Cassini Imaging Science: Initial Results on Saturn's Rings and Small Satellites deur C.C. Porco et al. Soos verskyn in Science, 25 February 2005: Vol. 307. no. 5713, bl. 1226-1236.
  12. ↑ 12,00 12,01 12,02 12,03 12,04 12,05 12,06 12,07 12,08 12,09 12,10 12,11 12,12 12,13 12,14 12,15 12,16 12,17 12,18 12,19 12,20 12,21 12,22 12,23 12,24 12,25 12,26 12,27 12,28 12,29 12,30 12,31 12,32 12,33 12,34 12,35 12,36 12,37 12,38 12,39 12,40 12,41 12,42 12,43 Bron: IAU-MPC Natural Satellites Ephemeris Service by die Harvard-Smithsonian Center for Astrophysics se webwerf.
  13. ↑ 13,00 13,01 13,02 13,03 13,04 13,05 13,06 13,07 13,08 13,09 13,10 13,11 13,12 13,13 13,14 13,15 13,16 13,17 Negatiewe wentelperiode dui op 'n omwentelingsrigting in teenstelling met die planeet se omwenteling.

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