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54 Alexandra

From Wikipedia, the free encyclopedia
Main-belt asteroid

54 Alexandra
A three-dimensional model of 54 Alexandra based on itslight curve
Discovery[1]
Discovered byH. Goldschmidt
Discovery date10 September 1858
Designations
(54) Alexandra
Pronunciation/ˌælɪɡˈzændrə,-ˈzɑːn-/AL-ig-ZA(H)N-drə[2]
Named after
Alexander von Humboldt
(German explorer)
Main belt
AdjectivesAlexandrian
Orbital characteristics
Epoch December 31, 2006 (JD 2454100.5)
Aphelion485.483 Gm (3.245AU)
Perihelion326.043 Gm (2.179 AU)
405.763 Gm (2.712 AU)
Eccentricity0.196
1,631.620 d (4.47 a)
103.809°
Inclination11.804°
313.446°
345.594°
Physical characteristics
Dimensions160 × 135 km (± 1 km)
154.137 km[1]
Mass(6.16±3.50)×1018 kg[3]
3.50±2.11 g/cm3[3]
18.14h[4]
155°±[5]
17°±[5]
0.056[1][6]
Tholen =C[1]
SMASS =C[1]
7.66[1]

54 Alexandra is acarbonaceousasteroid from the intermediateasteroid belt, approximately 155 kilometers in diameter. It was discovered by German-French astronomerHermann Goldschmidt on 10 September 1858, and named after the German explorerAlexander von Humboldt; it was the first asteroid to be named after a male.[7]

Description

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On May 17, 2005, this asteroid occulted a faint star (magnitude 8.5) and the event was observed and timed in a number of locations within theU.S. andMexico. As a result, asilhouette profile was produced, yielding a roughly oval cross-section with dimensions of 160 × 135 km (± 1 km).[8] The mass of the asteroid can be estimated based upon the mutuallyperturbing effects of other bodies, yielding an estimate of(6.16±3.50)×1018 kg.[3]

Photometric observations of this asteroid during 1990–92 gave alight curve with a period of 18.14 ± 0.04 hours and a brightness variation of 0.10 inmagnitude.[4] Alexandra has been studied byradar.[9] It was the namesake and largest member of the former Alexandraasteroid family; a dynamic group ofC-type asteroids that share similarorbital elements. Other members included70 Panopaea and145 Adeona.[10] 145 Adeona was subsequently assigned to theAdeona family, with Alexandra and Panopaea being dropped.[11]

In Popular Culture

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In the Swedish filmAniara (2018) it is mentioned that 54 Alexandra is the closest celestial body which the off-course and out-of-control spacecraft will approach before it leaves the Solar System.

References

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  1. ^abcdefYeomans, Donald K."54 Alexandra".JPL Small-Body Database Browser.NASA Jet Propulsion Laboratory. Retrieved7 April 2013.
  2. ^"Alexandra".Lexico UK English Dictionary.Oxford University Press. Archived fromthe original on 22 March 2020.
    "Alexandra".Dictionary.com Unabridged (Online). n.d.
  3. ^abcCarry, B. (December 2012), "Density of asteroids",Planetary and Space Science, vol. 73, pp. 98–118,arXiv:1203.4336,Bibcode:2012P&SS...73...98C,doi:10.1016/j.pss.2012.03.009. See Table 1.
  4. ^abBelskaya, I. N.; et al. (November 1993), "Physical Studies of Asteroids. Part XXVII. Photoelectric Photometry of Asteroids 14 Irene, 54 Alexandra and 56 Melete",Astronomy and Astrophysics Supplement, vol. 101, no. 3, pp. 507–511,Bibcode:1993A&AS..101..507B.
  5. ^abHanuš, J.; et al. (May 2017), "Volumes and bulk densities of forty asteroids from ADAM shape modeling",Astronomy & Astrophysics,601: 41,arXiv:1702.01996,Bibcode:2017A&A...601A.114H,doi:10.1051/0004-6361/201629956, A114.
  6. ^"Asteroid Data Sets". Archived fromthe original on 17 December 2009. Retrieved12 January 2007.
  7. ^Schmadel, Lutz D. (2003),Dictionary of Minor Planet Names (5th ed.), Springer, p. 20,ISBN 3642297188.
  8. ^D.W. Dunham, "Upcoming Asteroid Occultations",Sky & Telescope, June, 2006, p. 63.
  9. ^"Radar-Detected Asteroids and Comets". NASA/JPL Asteroid Radar Research. Retrieved30 October 2011.
  10. ^Williams, J. G. (March 1988), "The Unusual Alexandra Family",Abstracts of the Lunar and Planetary Science Conference, vol. 19, pp. 1277–1278,Bibcode:1988LPI....19.1277W.
  11. ^Zappala, Vincenzo; et al. (December 1990), "Asteroid families. I - Identification by hierarchical clustering and reliability assessment",Astronomical Journal, vol. 100, pp. 2030–2046, 2045,Bibcode:1990AJ....100.2030Z,doi:10.1086/115658. See p. 2045 and family 44.

External links

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