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Telesto (moon)





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Telesto /təˈlɛst/ is a moonofSaturn. It was discovered by Smith, Reitsema, Larson and Fountain in 1980 from ground-based observations, and was provisionally designated S/1980 S 13.[4] In the following months, several other apparitions were observed: S/1980 S 24,[5] S/1980 S 33,[6] and S/1981 S 1.[7]

Telesto
Telesto as seen by the Cassini probe on 11 October 2005
Discovery
Discovered by
  • Harold Reitsema
  • Stephen M. Larson
  • John W. Fountain
  • Discovery dateApril 8, 1980
    Designations

    Designation

    Saturn XIII
    Pronunciation/təˈlɛst/

    Named after

    Τελεστώ Telestō

    Alternative names

    Tethys B
    S/1980 S 13
    AdjectivesTelestoan /tɛləˈst.ən/orTelestoian /tɛləˈst.iən/
    Orbital characteristics

    Semi-major axis

    295000 km[1]
    Eccentricity0.001[1]

    Orbital period (sidereal)

    1.887802 d[1]
    Inclination1.19° (to Saturn's equator)
    Satellite ofSaturn
    GroupL4 Tethys trojan
    Physical characteristics
    Dimensions33.2 × 23.4 × 19.2 km
    (± 0.6 × 0.6 × 0.4 km)[2]: 2 

    Mean diameter

    24.6±0.6 km[2]: 2 
    Volume7795 km3[a]
    Mass≈ 4×1015 kg (assumed; unmeasured)[b]

    Mean density

    ≈ 0.5 g/cm3 (assumed; unmeasured)[2]: 3 

    Surface gravity

    ≈ 0.0011–0.0014 m/s2[2]: 3 

    Escape velocity

    ≈ 0.006 km/s at longest axis
    to ≈ 0.007 km/s at poles

    Axial tilt

    zero

    Apparent magnitude

    18.7[3]

    In 1983 it was officially named after TelestoofGreek mythology.[c] It is also designated as Saturn XIIIorTethys B.

    Telesto is co-orbital with Tethys, residing in Tethys' leading Lagrangian point (L4). This relationship was first identified by Seidelmann et al. in 1981.[8] Another moon, Calypso, resides in the other (trailing) Lagrangian point of Tethys, 60 degrees in the other direction from Tethys. The Saturnian system has two additional trojan moons.

    Exploration

    edit

    The Cassini probe performed a distant flyby of Telesto on October 11, 2005. The resulting images show that its surface is surprisingly smooth, devoid of small impact craters.

    Notes

    edit
    1. ^ Calculated from Telesto's volume-equivalent sphere radius of 12.3±0.3 km given by Thomas et al. (2020)[2]: 2 
  • ^ Calculated by multiplying Telesto's volume with its assumed density of 500 kg/m3.
  • ^ Transactions of the International Astronomical Union, Vol. XVIIIA, 1982 (confirms Janus, names Epimetheus, Telesto, Calypso) (mentioned in IAUC 3872)
  • References

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    Citations

    edit
    1. ^ a b c "Planetary Satellite Mean Orbital Parameters". Jet Propulsion Laboratory. Retrieved 5 June 2023.
  • ^ a b c d e Thomas & Helfenstein 2020.
  • ^ Hamilton.
  • ^ IAUC 3466.
  • ^ IAUC 3484.
  • ^ IAUC 3605.
  • ^ IAUC 3593.
  • ^ Seidelmann Harrington et al. 1981.
  • Sources

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    Retrieved from "https://en.wikipedia.org/w/index.php?title=Telesto_(moon)&oldid=1227528278"
     



    Last edited on 6 June 2024, at 08:17  





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    This page was last edited on 6 June 2024, at 08:17 (UTC).

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