astro.wikisort.org - AsteroidArethusa (minor planet designation: 95 Arethusa) is a large main-belt asteroid. It was discovered by German astronomer Robert Luther on 23 November 1867, and named after one of the various Arethusas in Greek mythology. Arethusa has been observed occulting a star three times:[7] first on 2 February 1998, and twice in January 2003.[citation needed]
Main-belt asteroid
95 Arethusa A three-dimensional model of 95 Arethusa based on its light curve. |
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Discovered by | Karl Theodor Robert Luther |
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Discovery date | 23 November 1867 |
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MPC designation | (95) Arethusa |
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Pronunciation | [1] |
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Minor planet category | Main belt |
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Adjectives | Arethusian,[2] Arethusean[3] |
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Epoch 31 July 2016 (JD 2457600.5) |
Uncertainty parameter 0 |
Observation arc | 143.53 yr (52424 d) |
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Aphelion | 3.53176 AU (528.344 Gm) |
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Perihelion | 2.59737 AU (388.561 Gm) |
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Semi-major axis | 3.06457 AU (458.453 Gm) |
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Eccentricity | 0.15245 |
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Orbital period (sidereal) | 5.36 yr (1959.5 d) |
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Average orbital speed | 16.91 km/s |
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Mean anomaly | 250.185° |
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Mean motion | 0° 11m 1.385s / day |
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Inclination | 12.9955° |
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Longitude of ascending node | 243.038° |
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Argument of perihelion | 154.196° |
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Dimensions | 136.04±10.1 km [4] 136.04 km† 147 ± 32 km [5] |
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Mass | 2.6×1018 kg |
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Equatorial surface gravity | 0.0380 m/s² |
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Equatorial escape velocity | 0.0719 km/s |
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Synodic rotation period | 8.705 h (0.3627 d) |
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Geometric albedo | 0.0698±0.012 [4] 0.070 [6] |
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Spectral type | C |
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Absolute magnitude (H) | 8.0 |
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This object is orbiting the Sun with a period of 5.36 years and an eccentricity of 0.15. The cross-section diameter is around 136 km and it is spinning with a rotation period of 8.7 hours. The spectrum matches a C-type asteroid, indicating a dark surface with a primitive carbonaceous composition.
References
- Benjamin Smith (1903) The Century Dictionary and Cyclopedia
- White & Riddle (1904) A Latin-English Dictionary for the Use of Junior Students
- Lucas Carpenter (1989) Selected Essays of Fletcher, p. 186
- "95 Arethusa". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. Retrieved 12 May 2016.
- Ďurech, Josef; Kaasalainen, Mikko; Herald, David; Dunham, David; Timerson, Brad; Hanuš, Josef; et al. (2011). "Combining asteroid models derived by lightcurve inversion with asteroidal occultation silhouettes" (PDF). Icarus. 214 (2): 652–670. arXiv:1104.4227. Bibcode:2011Icar..214..652D. doi:10.1016/j.icarus.2011.03.016. Archived from the original (PDF) on 3 March 2016. Retrieved 26 January 2012.
- "Asteroid Data Sets". Archived from the original on 17 December 2009. Retrieved 14 January 2007.
- Herald, David; et al. (October 2020), "Precise astrometry and diameters of asteroids from occultations - a data set of observations and their interpretation", Monthly Notices of the Royal Astronomical Society, 499 (3): 4570–4590, arXiv:2010.06086, Bibcode:2020MNRAS.499.4570H, doi:10.1093/mnras/staa3077
External links
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На других языках
[de] (95) Arethusa
(95) Arethusa ist ein Asteroid des Hauptgürtels, der am 23. November 1867 von dem deutschen Astronomen Karl Theodor Robert Luther entdeckt wurde[1].
- [en] 95 Arethusa
[es] (95) Arethusa
(95) Arethusa es un asteroide que forma parte del cinturón de asteroides y fue descubierto el 23 de noviembre de 1867 por Karl Theodor Robert Luther desde el observatorio de Düsseldorf-Bilk, Alemania.
Está nombrado por Aretusa, una diosecilla de la mitología griega.[2]
[fr] (95) Aréthuse
(95) Aréthuse, désignation internationale (95) Arethusa, est un astéroïde de la ceinture principale d'astéroïdes découvert par Robert Luther le 23 novembre 1867 à Düsseldorf.
[it] 95 Arethusa
95 Arethusa (in italiano 95 Aretusa) è un grande asteroide della Fascia principale. Ha una superficie scura e una composizione carboniosa e primitiva.
[ru] (95) Аретуса
(95) Арету́са (лат. Arethusa) — астероид главного пояса, принадлежащий к тёмному спектральному классу C. Он был открыт 23 ноября 1867 года немецким астрономом Робертом Лютером в Дюссельдорфской обсерватории, Германия и назван в честь Аретусы, одной из нимф из древнегреческой мифологии[2].
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