Astronomy:93 Minerva

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93 Minerva
A three-dimensional model of 93 Minerva based on its light curve on the top and an image of the asteroid on the bottom.
Discovery
Discovered byJames Craig Watson
Discovery siteAnn Arbor, Michigan
Discovery date24 August 1867
Designations
(93) Minerva
Pronunciation/mɪˈnɜːrvə/[1]
Named afterMinerva
1949 QN2, A902 DA
Minor planet categoryMain belt
AdjectivesMinervian, Minervean /mɪˈnɜːrviən/
Orbital characteristics[2]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc146.14 yr (53379 d)
|{{{apsis}}}|helion}}3.1429 astronomical unit|AU (470.17 Gm)
|{{{apsis}}}|helion}}2.3711 AU (354.71 Gm)
2.7570 AU (412.44 Gm)
Eccentricity0.13998
Orbital period4.58 yr (1672.0 d)
Average Orbital speed~17.86 km/s
Mean anomaly262.022°
Mean motion0° 12m 55.116s / day
Inclination8.56143°
Longitude of ascending node4.06265°
274.543°
Physical characteristics
Mean diameter154.155±1.298 km (IRAS)[2]
156 km[3]
Mass3.8×1018 kg (calculated)[lower-alpha 1]
Mean density1.9 g/cm3[3]
Equatorial surface gravity
4.139 cm/s2 (0.004221 g)[4]
Equatorial escape velocity
81 m/s[4]
Rotation period5.982 h (0.2493 d)[2]
Geometric albedo0.056±0.008[2]
C[2]
G?[3]
Absolute magnitude (H)7.91[2]


93 Minerva is a large triple main-belt asteroid. It is a C-type asteroid, meaning that it has a dark surface and possibly a primitive carbonaceous composition. It was discovered by J. C. Watson on 24 August 1867, and named after Minerva, the Roman equivalent of Athena, goddess of wisdom. An occultation of a star by Minerva was observed in France, Spain and the United States on 22 November 1982. An occultation diameter of ~170 km was measured from the observations. Since then two more occultations have been observed, which give an estimated mean diameter of ~150 km.[5][6]

Satellites

93 Minerva Lightcurve model.

On 16 August 2009, at 13:36 UT, the Keck Observatory's adaptive optics system revealed that the asteroid 93 Minerva possesses 2 small moons.[7] They are 4 and 3 km in diameter and the projected separations from Minerva correspond to 630 km (8.8 x Rprimary) and 380 km (5.2 x Rprimary) respectively.[7] They have been named Aegis[8] (/ˈɪs/)[9] and Gorgoneion[8] (/ˌɡɔːrɡəˈnən/).[10]

Notes

  1. Using a spherical radius of 78 km; volume of a sphere * density of 1.9 g/cm3 yields a mass (m=d*v) of 3.78E+18 kg

References

  1. Noah Webster (1884) A Practical Dictionary of the English Language
  2. 2.0 2.1 2.2 2.3 2.4 2.5 "JPL Small-Body Database Browser: 93 Minerva". Jet Propulsion Laboratory. https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=93. 
  3. 3.0 3.1 3.2 Franck Marchis (7 October 2011). "Is the triple Asteroid Minerva a baby-Ceres?". NASA blog (Cosmic Diary). http://cosmicdiary.org/fmarchis/2011/10/07/the-secrets-of-asteroid-minerva-and-its-two-moons/. 
  4. 4.0 4.1 "HEC:Exoplanets Calculator/Planet Density, Surface Gravity, and Escape Velocity". Planetary Habitability Laboratory. University of Puerto Rico at Arecibo. http://phl.upr.edu/projects/habitable-exoplanets-catalog/calculators. 
  5. Millis, R.L; Wasserman, L.H; Bowell, E; Franz, O.G; Nye, R; Osborn, W; Klemola, A (1985), "The occultation of AG+29°398 by 93 Minerva", Icarus 61 (1): 124–131, doi:10.1016/0019-1035(85)90159-9, Bibcode1985Icar...61..124M 
  6. "Observed minor planet occultation events". astro.cz. 26 July 2005. http://mpocc.astro.cz/world/mpocc1.txt. 
  7. 7.0 7.1 Franck Marchis (2009-08-21). "The discovery of a new triple asteroid, (93) Minerva". Cosmic Diary Blog. http://cosmicdiary.org/fmarchis/2009/08/21/the-discovery-of-a-new-triple-asteroid-93-minerva/. 
  8. 8.0 8.1 Franck Marchis (2013-12-26). "Asteroid Minerva finds its magical weapons in the sky". The Planetary Society. https://www.planetary.org/articles/20131224-asteroid-minerva-finds-its-magical-weapons-in-the-sky. 
  9. "aegis". aegis. Oxford University Press. http://www.lexico.com/definition/aegis. 
  10. "gorgoneion". gorgoneion. Oxford University Press. http://www.lexico.com/definition/gorgoneion.