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Amphitrite (minor planet designation: 29 Amphitrite) is one of the largest S-type asteroids, approximately 200 kilometers (120 miles) in diameter, and probably fifth largest after Eunomia, Juno, Iris and Herculina.

29 Amphitrite
VLT image of Amphitrite
Discovery [1]
Discovered byA. Marth
Discovery siteLondon
Discovery date1 March 1854
Designations
MPC designation
(29) Amphitrite
Pronunciation/æmfɪˈtraɪtiː/[2]
Named after
Amphitrite [3]
(Greek mythology)
Alternative designations
A899 NG
Minor planet category
main-belt [1][4] · (middle)
background [5][6]
AdjectivesAmphitritean /ˌæmfɪtrɪˈtiːən/, /ˌæmfɪˈtraɪtiən/
Orbital characteristics [4]
Epoch 23 March 2018 (JD 2458200.5)
Uncertainty parameter 0
Observation arc162.83 yr (59,472 d)
Aphelion2.7400 AU
Perihelion2.3712 AU
Semi-major axis
2.5556 AU
Eccentricity0.0722
Orbital period (sidereal)
4.09 yr (1,492 d)
Mean anomaly
187.97°
Mean motion
0° 14m 28.68s / day
Inclination6.0823°
Longitude of ascending node
356.37°
Argument of perihelion
63.036°
Physical characteristics
Dimensionsc/a = 0.82±0.03[7]
233 km × 212 km × 193 km[8]
Mean diameter
204±2 km[7]
189.6±1.1 km[9]
196±22 km[10]
206.86 km[11]
212.22±6.8 km[12]
227.1±4.0 km[13]
Mass(12.7±2.0)×1018 kg[7]
(11.8±?)×1018 kg[8]
Mean density
2.86±0.45 g/cm3[7]
2.36±0.26 g/cm3[8]
Synodic rotation period
5.3921 h[14][6]
Geometric albedo
0.194[7]
0.157±0.035[13]
0.1793±0.012[12]
0.195[11]
0.216±0.043[9]
Spectral type
S [6]
Absolute magnitude (H)
5.85[1][4]
6.0[5]

    Discovery


    Amphitrite was discovered by Albert Marth on 1 March 1854, at the private South Villa Observatory, in Regent's Park, London. It was Marth's only asteroid discovery. Its name was chosen by George Bishop, the owner of the observatory, who named it after Amphitrite, a sea goddess in Greek mythology.[3]


    Characteristics


    Lightcurve-based 3D-model of Amphitrite
    Lightcurve-based 3D-model of Amphitrite

    Amphitrite's orbit is less eccentric and inclined than those of its larger cousins; indeed, it is the most circular of any asteroid discovered up to that point. As a consequence, it never becomes as bright as Iris or Hebe, especially as it is much further from the Sun than those asteroids. It can reach magnitudes of around +8.6 at a favorable opposition, but usually is around the binocular limit of +9.5.

    In 2007, James Baer and Steven R. Chesley estimated Amphitrite to have a mass of 1.9×1019 kg.[15] A more recent estimate by Baer suggests it has a mass of 1.18×1019 kg.[8]

    A satellite of the asteroid is suspected to exist, based on lightcurve data collected by Edward F. Tedesco.[16][17] In 1988 a search for satellites or dust orbiting this asteroid was performed using the UH88 telescope at the Mauna Kea Observatories, but neither were found.[18]


    References


    1. "29 Amphitrite". Minor Planet Center. Retrieved 1 June 2018.
    2. Noah Webster (1884) A Practical Dictionary of the English Language
    3. Schmadel, Lutz D. (2007). "(29) Amphitrite". Dictionary of Minor Planet Names – (29) Amphitrite. Springer Berlin Heidelberg. p. 18. doi:10.1007/978-3-540-29925-7_30. ISBN 978-3-540-00238-3.
    4. "JPL Small-Body Database Browser: 29 Amphitrite" (2018-05-23 last obs.). Jet Propulsion Laboratory. Retrieved 1 June 2018.
    5. "Asteroid (29) Amphitrite". AstDyS-2, Asteroids – Dynamic Site. Retrieved 25 May 2018.
    6. "Asteroid 29 Amphitrite". Small Bodies Data Ferret. Retrieved 1 June 2018.
    7. P. Vernazza et al. (2021) VLT/SPHERE imaging survey of the largest main-belt asteroids: Final results and synthesis. Astronomy & Astrophysics 54, A56
    8. Jim Baer (2008). "Recent Asteroid Mass Determinations". Personal Website. Archived from the original on 2 July 2013. Retrieved 27 November 2008.
    9. Masiero, Joseph R.; Grav, T.; Mainzer, A. K.; Nugent, C. R.; Bauer, J. M.; Stevenson, R.; et al. (August 2014). "Main-belt Asteroids with WISE/NEOWISE: Near-infrared Albedos". The Astrophysical Journal. 791 (2): 11. arXiv:1406.6645. Bibcode:2014ApJ...791..121M. doi:10.1088/0004-637X/791/2/121. S2CID 119293330.
    10. Hanus, J.; Marchis, F.; Durech, J. (September 2013). "Sizes of main-belt asteroids by combining shape models and Keck adaptive optics observations". Icarus. 226 (1): 1045–1057. arXiv:1308.0446. Bibcode:2013Icar..226.1045H. doi:10.1016/j.icarus.2013.07.023. S2CID 118710558.
    11. Usui, Fumihiko; Kuroda, Daisuke; Müller, Thomas G.; Hasegawa, Sunao; Ishiguro, Masateru; Ootsubo, Takafumi; et al. (October 2011). "Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey". Publications of the Astronomical Society of Japan. 63 (5): 1117–1138. Bibcode:2011PASJ...63.1117U. doi:10.1093/pasj/63.5.1117. (online, AcuA catalog p. 153)
    12. Tedesco, E. F.; Noah, P. V.; Noah, M.; Price, S. D. (October 2004). "IRAS Minor Planet Survey V6.0". NASA Planetary Data System. 12: IRAS-A-FPA-3-RDR-IMPS-V6.0. Bibcode:2004PDSS...12.....T. Retrieved 22 October 2019.
    13. Mainzer, A.; Grav, T.; Masiero, J.; Hand, E.; Bauer, J.; Tholen, D.; et al. (November 2011). "NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results". The Astrophysical Journal. 741 (2): 25. arXiv:1109.6407. Bibcode:2011ApJ...741...90M. doi:10.1088/0004-637X/741/2/90. S2CID 118700974. (catalog)
    14. "LCDB Data for (29) Amphitrite". Asteroid Lightcurve Database (LCDB). Retrieved 1 June 2018.
    15. Baer, James; Steven R. Chesley (2008). "Astrometric masses of 21 asteroids, and an integrated asteroid ephemeris". Celestial Mechanics and Dynamical Astronomy. 100 (2008): 27–42. Bibcode:2008CeMDA.100...27B. doi:10.1007/s10569-007-9103-8.
    16. Tedesco, E. F. (March 1979). "Binary Asteroids: Evidence for Their Existence from Lightcurves". Science. New Series. 203 (4383): 905–907. Bibcode:1979Sci...203..905T. doi:10.1126/science.203.4383.905. PMID 17771729. S2CID 19431574.
    17. van Flandern, T. C.; Tedesco, E. F.; Binzel, R. P. (1979). "Satellites of asteroids". Asteroids. Tucson, AZ: University of Arizona Press. pp. 443–465. Bibcode:1979aste.book..443V.
    18. Gradie, J.; Flynn, L. (March 1988), "A Search for Satellites and Dust Belts Around Asteroids: Negative Results", Abstracts of the Lunar and Planetary Science Conference, vol. 19, pp. 405–406, Bibcode:1988LPI....19..405G



    На других языках

    [de] (29) Amphitrite

    (29) Amphitrite ist ein Asteroid des Asteroiden-Hauptgürtels, der am 1. März 1854 von Albert Marth am George-Bishop-Observatorium entdeckt wurde. Benannt wurde sie nach der griechisch-römischen Meeresgöttin Amphitrite, Tochter des Nereus und der Doris, Gattin des Poseidon.
    - [en] 29 Amphitrite

    [es] (29) Amphitrite

    (29) Amphitrite es un asteroide descubierto desde Londres en 1854 por Albert Marth. Es uno de los mayores asteroides de tipo S, probablemente de más de 200 kilómetros, el tercero en diámetro tras Eunomia y Juno, de superficie similar a Iris y Herculina.

    [ru] (29) Амфитрита

    (29) Амфитри́та (лат. Amphitrite) — астероид главного пояса, который входит в число 25 самых крупных астероидов главного пояса и принадлежит к светлому спектральному классу S[7]. Он был открыт 1 марта 1854 года немецким астрономом Альбертом Мартом в обсерватории Бишопа, Великобритания и назван в честь древнегреческой нереиды Амфитриты, жены Посейдона, матери Тритона и Роды[8].


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