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758 Mancunia is a minor planet orbiting the Sun. It was discovered in 1912 from Johannesburg by H. E. Wood, a Mancunian. This object is orbiting at a distance of 3.19 AU with a period of 5.70 years and an eccentricity (ovalness) of 0.15. The orbital plane is inclined at an angle of 5.61° to the plane of the ecliptic.[2]

758 Mancunia
Discovery
Discovered byH. E. Wood
Discovery siteJohannesburg
Discovery date18 May 1912
Designations
MPC designation
(758) Mancunia
Pronunciation/mænˈkjuːniə/[1]
Alternative designations
1912 PE
Orbital characteristics[2]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc101.39 yr (37034 d)
Aphelion3.6704 AU (549.08 Gm)
Perihelion2.7081 AU (405.13 Gm)
Semi-major axis
3.1893 AU (477.11 Gm)
Eccentricity0.15086
Orbital period (sidereal)
5.70 yr (2080.3 d)
Mean anomaly
260.973°
Mean motion
0° 10m 22.98s / day
Inclination5.6102°
Longitude of ascending node
106.200°
Argument of perihelion
314.999°
Earth MOID1.72323 AU (257.792 Gm)
Jupiter MOID1.66575 AU (249.193 Gm)
TJupiter3.172
Physical characteristics
Mean radius
42.74±3.35 km[2]
43.54 ± 0.655 km[3]
Mass(9.31 ± 0.80) × 1017 kg[3]
Mean density
2.69 ± 0.26 g/cm3[3]
Synodic rotation period
12.7253 h (0.53022 d)
Geometric albedo
0.1317±0.023
Absolute magnitude (H)
8.16

    Observation of this asteroid in 1996 suggested a rotation period of 6.902 hours. However, radar observations from Arecibo indicated this may be in error. Independent photometry measurements made during December 2006 were combined to determine an estimated period nearly double that of the original, or 12.7253±0.0006 h with a brightness variation amplitude of 0.26±0.02 in magnitude.[4] A high radar albedo indicates this object is most likely metallic. Dips in the radar echo suggests there are large concavities on both sides. It is classified as an X-type asteroid in the Tholen taxonomy and spans a girth of 85±7 km.[5]


    References


    1. "Mancunian". Oxford English Dictionary (Online ed.). Oxford University Press. (Subscription or participating institution membership required.)
    2. "758 Mancunia (1912 PE)". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. Retrieved 5 May 2016.
    3. Carry, 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. Warner, Brian D.; Behrend, Raoul; Poncy, Raymond; Coliac, Jean-Francois (March 2008), "Lightcurve Analysis of 758 Mancunia", Bulletin of the Minor Planets Section of the Association of Lunar and Planetary Observers, 35 (1): 25, Bibcode:2008MPBu...35...25W.
    5. Shepard, Michael K.; et al. (May 2008), "A radar survey of M- and X-class asteroids", Icarus, 195 (1): 184–205, Bibcode:2008Icar..195..184S, doi:10.1016/j.icarus.2007.11.032.




    На других языках


    [de] (758) Mancunia

    (758) Mancunia ist ein Asteroid des Hauptgürtels, der am 18. Mai 1912 vom südafrikanischen Astronomen Harry Edwin Wood in Johannesburg entdeckt wurde.
    - [en] 758 Mancunia

    [es] (758) Mancunia

    (758) Mancunia es un asteroide que forma parte del cinturón de asteroides y fue descubierto el 18 de mayo de 1912 por Harry Edwin Wood desde el observatorio Union de Johannesburgo, República Sudaficana.

    [ru] (758) Манкуния

    (758) Манкуния (лат. Mancunia) — небольшой астероид из группы главного пояса, который был открыт 18 мая 1912 года южноафриканским астрономом Гарри Вудом в обсерватории Йоханнесбурга и назван в честь латинского названия английского города Манчестер[2].



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