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Pallene (moon)

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Moon of Saturn
Pallene
Cassini image of Pallene transiting Saturn on October 16, 2010
Discovery
Discovered byVoyager 2 (first discovery)
Cassini Imaging Team[1]
Discovery dateJune 1, 2004 (second discovery byCassini-Huygens)
Designations
Designation
Saturn XXXIII
Pronunciation/pəˈln/[2]
Named after
ΠαλλήνηPallēnē
S/1981 S 14 (first discovery)
S/2004 S 2 (second discovery)
AdjectivesPallenean/pæləˈnən/[3]
Orbital characteristics[4]
Epoch 20 June 2004 (JD 2453177.5)
212300 km[5]
Eccentricity0.004[5]
1.009549 d[5]
Inclination0.1810°±0.0014° (to Saturn's equator)
Satellite ofSaturn
GroupAlkyonides
Physical characteristics
Dimensions5.76 × 4.16 × 3.68 km
(± 0.14 × 0.14 × 0.14 km)[6]: 2 
4.46±0.14 km[6]: 2 
Volume46.5 km3[a]
Mass(1.15±0.40)×1013 kg[6]: 3 
0.251±0.075 g/cm3[6]: 3 
0.011–0.016 mm/s2[6]: 3 
0.0007 km/s at longest axis
to 0.0009 km/s at poles
synchronous
zero

Pallene/pəˈln/ is a very smallnatural satellite ofSaturn. It is one of three small moons known as theAlkyonides that lie between the orbits of the largerMimas andEnceladus. It is also designatedSaturn XXXIII.

Discovery

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Discovery image of Pallene in 2004 from theCassini probe

Pallene was discovered by the Cassini Imaging Team in 2004, during theCassini–Huygens mission.[7][8] It was given the temporary designationS/2004 S 2. In 2005, the name Pallene was provisionally approved by the IAU Division III Working Group for Planetary System Nomenclature,[9] and was ratified at the IAU General Assembly in 2006. The name refers toPallene, one of theAlkyonides, the seven beautiful daughters of thegiantAlkyoneus.

After the discovery in 2004, it was realized that Pallene had been first photographed on August 23, 1981, by the space probeVoyager 2. It had appeared in a single photograph and had been provisionally namedS/1981 S 14 and estimated to orbit 200,000 km from Saturn.[10] Because it had not been visible in other images, it had not been possible to compute its orbit at the time, but recent comparisons have shown it to match Pallene's orbit.[4]

Orbital characteristics

[edit]

Pallene is visibly affected by a perturbing mean-longitude resonance with the much larger Enceladus, although this effect is not as large as Mimas's perturbations onMethone. The perturbations cause Pallene'sosculating orbital elements to vary with an amplitude of about 4 km in semi-major axis, and 0.02° in longitude (corresponding to about 75 km). Eccentricity also changes on various timescales between 0.002 and 0.006, and inclination between about 0.178° and 0.184°.[4]

Ring

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Back-illuminated rings of Saturn as seen byCassini on 15 September 2006. The faint Pallene ring is visible at the bottom left as indicated.

In 2006, images taken in forward-scattered light by theCassini spacecraft enabled the Cassini Imaging Team to discover a faint dust ring around Saturn that shares Pallene's orbit, now named thePallene Ring.[11][12] The ring has a radial extent of about 2,500 km. Its source is particles blasted off Pallene's surface by meteoroid impacts, which then form a diffuse ring around its orbital path.[13][14]

Exploration

[edit]
Pallene's crescent illuminated bySaturnshine, imaged byCassini on 14 September 2011

TheCassini spacecraft, which studied Saturn and its moons until September, 2017, performed a fly-by of Pallene on 16 October 2010, and 14 September 2011 at a distance of 36,000 kilometers (22,000 miles) and 44,000 kilometers respectively.[15]

Notes

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  1. ^Calculated from Pallene's volume-equivalent sphere radius of2.23±0.07 km given by Thomas et al. (2020)[6]: 2 

References

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Citations

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  1. ^Cassini Imaging Team.
  2. ^Noah Webster (1884)A Practical Dictionary of the English Language
  3. ^"JPL (ca. 2008)Cassini Equinox Mission: Pallene". Archived fromthe original on 2016-04-12. Retrieved2020-03-05.
  4. ^abcSpitale Jacobson et al. 2006.
  5. ^abc"Planetary Satellite Mean Orbital Parameters".Jet Propulsion Laboratory. Retrieved5 June 2023.
  6. ^abcdefThomas & Helfenstein 2020.
  7. ^IAUC 8389.
  8. ^Porco Baker et al. 2005.
  9. ^IAUC 8471.
  10. ^IAUC 6162.
  11. ^IAUC 8759.
  12. ^CICLOPS 2006,Moonmade Rings.
  13. ^JPL/NASA: Creating New Rings.
  14. ^Hedman et al., 2009.
  15. ^"Cassini Tour Event Summary – Planned Observations of Small Satellites".Planetary Atmospheres Node. Planetary Data Services. Retrieved31 March 2022.

Sources

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External links

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Listed in approximate increasing distance from Saturn
Ring moonlets
Ring shepherds
Alkyonides
Large moons
(withtrojans)
Inuit group (36)
Kiviuq subgroup (20)
Paaliaq
Siarnaq subgroup (15)
Gallic group (17)
Norse group (197)
Low-inclination (12)
Kari subgroup (15)
Mundilfari subgroup (143)
  • S/2023 S 50
  • S/2023 S 9
  • S/2004 S 56
  • S/2023 S 8
  • S/2023 S 11
  • S/2006 S 21
  • S/2006 S 22
  • S/2023 S 13
  • S/2023 S 10
  • S/2023 S 12
  • S/2007 S 5
  • S/2007 S 7
  • S/2004 S 37
  • S/2004 S 47
  • S/2004 S 40
  • S/2020 S 14
  • S/2019 S 27
  • S/2023 S 14
  • S/2020 S 16
  • S/2023 S 16
  • S/2019 S 3
  • S/2020 S 7
  • S/2019 S 28
  • Skoll
  • S/2019 S 30
  • S/2023 S 21
  • S/2023 S 4
  • S/2020 S 18
  • S/2020 S 2
  • S/2019 S 4
  • S/2020 S 20
  • S/2004 S 41
  • S/2004 S 57
  • S/2006 S 24
  • S/2004 S 42
  • S/2023 S 15
  • S/2023 S 24
  • S/2004 S 13
  • S/2007 S 6
  • S/2019 S 35
  • S/2006 S 25
  • Mundilfari
  • S/2006 S 26
  • S/2019 S 33
  • S/2023 S 23
  • S/2020 S 21
  • S/2004 S 43
  • S/2006 S 10
  • S/2019 S 5
  • S/2023 S 25
  • S/2004 S 59
  • S/2006 S 27
  • Gridr
  • Bergelmir
  • Jarnsaxa
  • S/2023 S 44
  • S/2020 S 22
  • S/2004 S 44
  • Hati
  • S/2004 S 17
  • S/2004 S 12
  • S/2020 S 23
  • Eggther
  • S/2023 S 28
  • S/2023 S 37
  • S/2023 S 26
  • S/2019 S 36
  • S/2006 S 13
  • S/2023 S 48
  • S/2023 S 29
  • S/2007 S 9
  • Farbauti
  • S/2019 S 9
  • S/2023 S 32
  • S/2020 S 24
  • Aegir
  • S/2019 S 10
  • Beli
  • S/2023 S 31
  • S/2020 S 25
  • S/2023 S 34
  • S/2023 S 39
  • S/2019 S 12
  • S/2004 S 61
  • S/2006 S 14
  • S/2023 S 40
  • Gunnlod
  • S/2019 S 15
  • S/2020 S 6
  • S/2020 S 26
  • S/2023 S 41
  • S/2004 S 7
  • S/2005 S 5
  • S/2006 S 16
  • S/2023 S 49
  • S/2006 S 15
  • S/2023 S 42
  • S/2004 S 28
  • S/2020 S 32
  • S/2020 S 8
  • S/2020 S 28
  • S/2019 S 38
  • S/2004 S 48
  • S/2023 S 36
  • S/2023 S 35
  • S/2020 S 29
  • Fenrir
  • S/2004 S 50
  • S/2006 S 17
  • S/2004 S 49
  • S/2020 S 34
  • S/2020 S 31
  • S/2023 S 43
  • Surtur
  • S/2006 S 18
  • S/2020 S 36
  • Loge
  • S/2020 S 33
  • S/2004 S 39
  • S/2019 S 16
  • S/2004 S 53
  • S/2023 S 45
  • Thiazzi
  • S/2020 S 38
  • S/2020 S 40
  • S/2019 S 40
  • S/2019 S 42
  • Saturn LXIV
  • S/2020 S 39
  • S/2019 S 41
  • Fornjot
  • S/2023 S 47
  • S/2004 S 51
  • S/2020 S 10
  • S/2020 S 42
  • S/2020 S 9
  • S/2023 S 5
  • S/2020 S 41
  • S/2019 S 21
  • S/2004 S 52
  • S/2020 S 43
  • S/2019 S 43
  • S/2020 S 44
Phoebe subgroup (27)
Geography
Moons
Astronomy
Exploration
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