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词条 Anthe (moon)
释义

  1. References

  2. External links

{{Infobox planet
| discoverer = Cassini Imaging Team {{sfn|Cassini Imaging Team}}
| period = 1.05089 d
| dimensions = 1.8 km [1]
| density = 0.5 g/cm³
| name = Anthe
| image = Anthe N1832831075 1.jpg
| caption = Anthe is the ellipsoid in the center
| discovered = May 30, 2007
| orbit_ref = {{sfn|IAUC 8857}}
| epoch =
| semimajor = 197,700 km
| eccentricity = 0.0011
| inclination = 0.1° to Saturn's equator
| satellite_of = Saturn
| avg_speed = 13.824 km/s
| mean_radius = 0.9 km
| circumference = ≈ 5.7 km
| mass = 1.5{{e|12}} kg[2]
| volume = 3 km³
| surface_area = 10.18 km²
| surface_grav = 0.00012 m/s² (0.12mm/s²)
| escape_velocity = ≈ 0.56 m/s (≈ 2km/h)
| rotation = assumed synchronous
| axial_tilt =
| albedo =
}}

Anthe ({{IPAc-en|ˈ|æ|n|θ|iː}} {{respell|AN|thee}}; Greek: Άνθη) is a very small natural satellite of Saturn 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.{{sfn|Agle|2007}}

It was discovered by the Cassini Imaging Team{{sfn|Cassini Imaging Team}} in images taken on 30 May 2007.{{sfn|IAUC 8857}} 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.{{sfn|IAUC 8857}}

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.{{sfn|Porco et al., 2008}}{{sfn|Hedman et al., 2009}}

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References

Notes

1. ^[https://solarsystem.nasa.gov/planets/anthe/facts]
2. ^[https://solarsystem.nasa.gov/planets/anthe/facts]
.


}}
Citations
{{reflist}}
Sources
  • {{cite web

| publisher = Cassini Imaging Central Laboratory for OPerationS
| title = Cassini Imaging Science Team
| url = http://ciclops.org/team/iss_team.php
| accessdate = 2012-01-01
| ref = {{sfnRef|Cassini Imaging Team}}
  • {{cite web

| last = Agle
| first = D. C.
| date = July 19, 2007
| title = Saturn Turns 60
| publisher = JPL/NASA
| work = Cassini Solstice Mission
| url = http://saturn.jpl.nasa.gov/news/cassinifeatures/feature20070719/
| accessdate = 2012-01-01
| ref = harv
  • {{cite journal

| last = Green
| first = Daniel W. E.
| title = S/ 2007 S 4
| date = July 18, 2007
| journal = IAU Circular
| volume = 8857
| url = http://www.cbat.eps.harvard.edu/iauc/08800/08857.html
| accessdate = 2012-01-01
| ref = {{sfnRef|IAUC 8857}}
  • {{cite journal|last1=Hedman |first1=M. M.

| last2=Murray |first2=C. D. |last3=Cooper|first3=N. J.
| last4=Tiscareno|first4=M. S. |last5=Beurle|first5=K.
| last6=Evans|first6=M. W. |last7=Burns|first7=J. A.
|title=Three tenuous rings/arcs for three tiny moons
|journal=Icarus |volume=199 |issue=2 |date=2008-11-25
|pages=378–386 |issn=0019-1035 |doi=10.1016/j.icarus.2008.11.001
| ref = {{sfnRef|Hedman et al., 2009}}
|bibcode = 2009Icar..199..378H }}
  • {{cite web | last = Porco C. C.

| first = et al.
| title = More Ring Arcs for Saturn
| work = Cassini Imaging Central Laboratory for Operations
| date = 2008-09-05
| url = http://ciclops.org/view_event/90/More_Ring_Arcs_for_Saturn
| accessdate = 2008-09-05
| ref = {{sfnRef|Porco et al., 2008}}

External links

{{Commons category-inline|Anthe}}{{Spoken Wikipedia|Anthe (moon).ogg|2010-01-16}}
  • From Dark Obscurity... A Tiny New Saturnian Moon Comes To Light
{{Moons of Saturn|state=uncollapsed}}{{Saturn}}{{DEFAULTSORT:Anthe (Moon)}}

2 : Moons of Saturn|Astronomical objects discovered in 2007

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