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93 Minerva

From Wikipedia, the free encyclopedia
Main-belt asteroid

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 after
Minerva
1949 QN2, A902 DA
Main belt
AdjectivesMinervian, Minervean/mɪˈnɜːrviən/
Orbital characteristics[2]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc146.14 yr (53379 d)
Aphelion3.1429 AU (470.17 Gm)
Perihelion2.3711 AU (354.71 Gm)
2.7570 AU (412.44 Gm)
Eccentricity0.13998
4.58yr (1672.0d)
~17.86 km/s
262.022°
0° 12m 55.116s / day
Inclination8.56143°
4.06265°
274.543°
Physical characteristics
154.155±1.298 km(IRAS)[2]
156 km[3]
Mass3.8×1018 kg (calculated)[a]
1.9 g/cm3[3]
4.139 cm/s2 (0.004221g)[4]
Equatorialescape velocity
81 m/s[4]
5.982 h (0.2493 d)[2]
0.056±0.008[2]
C[2]
G?[3]
7.91[2]

93 Minerva is a largetriplemain-belt asteroid. It is aC-type asteroid, meaning that it has a dark surface and possibly a primitivecarbonaceous composition. It was discovered byJ. C. Watson on 24 August 1867, and named afterMinerva, theRoman equivalent ofAthena, goddess of wisdom. Anoccultation of astar by Minerva was observed inFrance,Spain and theUnited 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 estimatedmean diameter of ~150 km.[5][6]

Satellites

[edit]
93 Minerva Lightcurve model.

On 16 August 2009, at 13:36UT, theKeck Observatory'sadaptive 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 namedAegis[8] (/ˈɪs/)[9] andGorgoneion[8] (/ˌɡɔːrɡəˈnən/).[10]

Notes

[edit]
  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

[edit]
  1. ^Noah Webster (1884)A Practical Dictionary of the English Language
  2. ^abcdef"JPL Small-Body Database Browser: 93 Minerva" (2011-12-29 last obs).Jet Propulsion Laboratory. Retrieved13 May 2016.
  3. ^abcFranck Marchis (7 October 2011)."Is the triple Asteroid Minerva a baby-Ceres?". NASA blog (Cosmic Diary). Retrieved28 January 2012.
  4. ^ab"HEC:Exoplanets Calculator/Planet Density, Surface Gravity, and Escape Velocity".Planetary Habitability Laboratory. University of Puerto Rico at Arecibo. Archived fromthe original on 24 August 2017. Retrieved10 January 2014.
  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,Bibcode:1985Icar...61..124M,doi:10.1016/0019-1035(85)90159-9,hdl:2060/19840022996
  6. ^"Observed minor planet occultation events". astro.cz. 26 July 2005. Retrieved3 September 2020.
  7. ^abFranck Marchis (21 August 2009)."The discovery of a new triple asteroid, (93) Minerva". Cosmic Diary Blog. Retrieved25 October 2009.
  8. ^abFranck Marchis (26 December 2013)."Asteroid Minerva finds its magical weapons in the sky". The Planetary Society. Retrieved7 April 2023.
  9. ^"aegis".Lexico UK English Dictionary.Oxford University Press. Archived fromthe original on 23 March 2020.
  10. ^"gorgoneion".Lexico UK English Dictionary UK English Dictionary.Oxford University Press. Archived fromthe original on 23 March 2020.

External links

[edit]
Minor planets
Asteroid
Distant minor planet
Comets
Other
Authority control databasesEdit this at Wikidata
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