Astronomy:95 Arethusa

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Short description: Main-belt asteroid
95 Arethusa
95Arethusa (Lightcurve Inversion).png
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]
Minor planet categoryMain 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)
|{{{apsis}}}|helion}}3.53176 astronomical unit|AU (528.344 Gm)
|{{{apsis}}}|helion}}2.59737 AU (388.561 Gm)
3.06457 AU (458.453 Gm)
Eccentricity0.15245
Orbital period5.36 yr (1959.5 d)
Average Orbital speed16.91 km/s
Mean anomaly250.185°
Mean motion0° 11m 1.385s / day
Inclination12.9955°
Longitude of ascending node243.038°
154.196°
Physical characteristics
Dimensions136.04±10.1 km[4]
136.04 km
147 ± 32 km [5]
Mass2.6×1018 kg
Equatorial surface gravity
0.0380 m/s²
Equatorial escape velocity
0.0719 km/s
Rotation period8.705 h (0.3627 d)
Geometric albedo0.0698±0.012[4]
0.070 [6]
C
Absolute magnitude (H)8.0


Arethusa (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]

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

  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. 4.0 4.1 4.2 "95 Arethusa". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=95;cad=1. 
  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". Icarus 214 (2): 652–670. doi:10.1016/j.icarus.2011.03.016. Bibcode2011Icar..214..652D. http://astro.troja.mff.cuni.cz/projects/asteroids3D/download/durech_et_al_2011_occ_paper.pdf. Retrieved 26 January 2012. 
  6. "Asteroid Data Sets". http://www.psi.edu/pds/resource/albedo.html. 
  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, doi:10.1093/mnras/staa3077, Bibcode2020MNRAS.499.4570H 

External links