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95 Arethusa

From Wikipedia, the free encyclopedia
Main-belt asteroid

95 Arethusa
A three-dimensional model of 95 Arethusa based on its light curve.
Discovery
Discovered byKarl Theodor Robert Luther
Discovery date23 November 1867
Designations
(95) Arethusa
Pronunciation/ærəˈθjsə/[1]
Main belt
AdjectivesArethusian,[2] Arethusean[3]/ˌærəˈθjziən/
Orbital characteristics[4]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc143.53 yr (52424 d)
Aphelion3.53176 AU (528.344 Gm)
Perihelion2.59737 AU (388.561 Gm)
3.06457 AU (458.453 Gm)
Eccentricity0.15245
5.36yr (1959.5d)
16.91 km/s
250.185°
0° 11m 1.385s / day
Inclination12.9955°
243.038°
154.196°
Physical characteristics
Dimensions136.04±10.1 km[4]
136.04 km
147 ± 32 km[5]
Mass2.6×1018 kg
0.0380 m/s2 (0.00387 g0)
Equatorialescape velocity
0.0719 km/s
8.705 h (0.3627 d)
0.0698±0.012[4]
0.070[6]
C
8.0

95 Arethusa is a largemain-beltasteroid. It was discovered by German astronomerRobert Luther on 23 November 1867, and named after one of the variousArethusas inGreek mythology. Arethusa has been observedocculting astar three times:[7] first on 2 February 1998, and twice in January 2003.[citation needed]

This object is orbiting theSun with aperiod of 5.36 years and aneccentricity of 0.15. The cross-section diameter is around 136 km and it is spinning with arotation period of 8.7 hours. The spectrum matches aC-type asteroid, indicating a dark surface with a primitivecarbonaceous composition.

References

[edit]
  1. ^Benjamin Smith (1903)The Century Dictionary and Cyclopedia
  2. ^White & Riddle (1904)A Latin-English Dictionary for the Use of Junior Students
  3. ^Lucas Carpenter (1989)Selected Essays of Fletcher, p. 186
  4. ^abc"95 Arethusa".JPL Small-Body Database.NASA/Jet Propulsion Laboratory. Retrieved12 May 2016.
  5. ^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 fromthe original(PDF) on 3 March 2016. Retrieved26 January 2012.
  6. ^"Asteroid Data Sets". Archived fromthe original on 17 December 2009. Retrieved14 January 2007.
  7. ^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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