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Anthe (moon)





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Anthe /ˈænθ/ is a very small natural satelliteofSaturn lying between the orbits of Mimas and Enceladus. It is also known as Saturn XLIX; its provisional designation was S/2007 S 4. It is named after one of the Alkyonides; the name means flowery. It is the sixtieth confirmed moon of Saturn.[5]

Anthe
Anthe is the ellipsoid in the center
Discovery
Discovered byCassini Imaging Team [1]
Discovery dateMay 30, 2007
Designations

Designation

Saturn XLIX
Pronunciation/ˈænθ/[a]

Named after

Άνθη Anthē
AdjectivesAnthean /ænˈθən/
Orbital characteristics[2]

Semi-major axis

197,700 km
Eccentricity0.0011

Orbital period (sidereal)

1.05089 d

Average orbital speed

13.824 km/s
Inclination0.1° to Saturn's equator
Satellite ofSaturn
GroupAlkyonides
Physical characteristics
Dimensions1.8 km [3]

Mean radius

0.9 km
Circumference≈ 5.7 km

Surface area

10.18 km2
Volume3 km3
Mass1.5×1012kg[4]

Mean density

0.5 g/cm3

Surface gravity

0.00012 m/s2 (0.12 mm/s2)

Escape velocity

≈ 0.56 m/s (≈ 2 km/h)

Synodic rotation period

assumed synchronous

The designation S/2007 S 4 was also accidentally and incorrectly used for a different Saturnian satellite discovered later. The published discovery was retracted a few hours later and republished the next day under the correct name of S/2007 S 5.

It was discovered by the Cassini Imaging Team[1] in images taken on 30 May 2007.[2] Once the discovery was made, a search of older Cassini images revealed it in observations from as far back as June 2004. It was first announced on 18 July 2007.[2]

Discovery images of Anthe

Anthe is visibly affected by a perturbing 10:11 mean-longitude resonance with the much larger Mimas. This causes its osculating orbital elements to vary with an amplitude of about 20 km in semi-major axis on a timescale of about 2 Earth years. The close proximity to the orbits of Pallene and Methone suggests that these moons may form a dynamical family.

Material blasted off Anthe by micrometeoroid impacts is thought to be the source of the Anthe Ring Arc, a faint partial ring about Saturn co-orbital with the moon first detected in June 2007.[6][7]

References

edit
Notes
  1. ^ This name is too new to appear in dictionaries, but the OED has the analogous rhodanthe /roʊˈdænθiː/ from the same root.
Citations
  • ^ a b c IAUC 8857.
  • ^ [1][dead link]
  • ^ [2][dead link]
  • ^ Agle 2007.
  • ^ Porco et al., 2008.
  • ^ Hedman et al., 2009.
  • Sources
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    Last edited on 25 June 2023, at 06:06  





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    This page was last edited on 25 June 2023, at 06:06 (UTC).

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