93 Minerva

Last updated

93 Minerva
93 Minerva.png
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 by James Craig Watson
Discovery site Ann Arbor, Michigan
Discovery date24 August 1867
Designations
(93) Minerva
Pronunciation /mɪˈnɜːrvə/ [1]
Named after
 Minerva
1949 QN2, A902 DA
Main belt
Adjectives Minervian, Minervean /mɪˈnɜːrviən/
Orbital characteristics [2]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc 146.14 yr (53379 d)
Aphelion 3.1429  AU (470.17  Gm)
Perihelion 2.3711 AU (354.71 Gm)
2.7570 AU (412.44 Gm)
Eccentricity 0.13998
4.58 yr (1672.0 d)
Average orbital speed
~17.86 km/s
262.022°
0° 12m 55.116s / day
Inclination 8.56143°
4.06265°
274.543°
Physical characteristics
154.155±1.298  km (IRAS) [2]
156 km [3]
Mass 3.8×1018 kg (calculated) [a]
Mean density
1.9 g/cm3 [3]
Equatorial surface gravity
4.139 cm/s2 (0.004221 g) [4]
Equatorial escape 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 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]

    Contents

    Satellites

    93 Minerva Lightcurve model. 93Minerva (Lightcurve Inversion).png
    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] ( /ˈiːdʒɪs/ ) [9] and Gorgoneion [8] ( /ˌɡɔːrɡəˈnaɪən/ ). [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. 1 2 3 4 5 6 "JPL Small-Body Database Browser: 93 Minerva" (2011-12-29 last obs). Jet Propulsion Laboratory . Retrieved 13 May 2016.
    3. 1 2 3 Franck Marchis (7 October 2011). "Is the triple Asteroid Minerva a baby-Ceres?". NASA blog (Cosmic Diary). Retrieved 28 January 2012.
    4. 1 2 "HEC:Exoplanets Calculator/Planet Density, Surface Gravity, and Escape Velocity". Planetary Habitability Laboratory. University of Puerto Rico at Arecibo. Archived from the original on 24 August 2017. Retrieved 10 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. Retrieved 3 September 2020.
    7. 1 2 Franck Marchis (21 August 2009). "The discovery of a new triple asteroid, (93) Minerva". Cosmic Diary Blog. Retrieved 25 October 2009.
    8. 1 2 Franck Marchis (26 December 2013). "Asteroid Minerva finds its magical weapons in the sky". The Planetary Society. Retrieved 7 April 2023.
    9. ↑ "aegis". Lexico UK English Dictionary. Oxford University Press. Archived from the original on 23 March 2020.
    10. ↑ "gorgoneion". Lexico UK English Dictionary UK English Dictionary. Oxford University Press. Archived from the original on 23 March 2020.
    This page is based on this Wikipedia article
    Text is available under the CC BY-SA 4.0 license; additional terms may apply.
    Images, videos and audio are available under their respective licenses.