804 Hispania

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804 Hispania
Discovery
Discovered byJ. Comas Solá
Discovery date20 March 1915
Designations
(804) Hispania
Pronunciation/hɪˈspniə/[1][2]
Named after
Spain
1915 WT
Main belt
AdjectivesHispanian[2]
Orbital characteristics[3]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc39,655 d (108.57 yr)
Aphelion3.2343 AU (483.84 Gm)
Perihelion2.4418 AU (365.29 Gm)
2.8381 AU (424.57 Gm)
Eccentricity0.13961
4.78 yr (1746.3 d)
17.60 km/s
277.552°
0° 12m 22.104s / day
Inclination15.395°
347.611°
344.626°
Earth MOID1.43481 AU (214.645 Gm)
Jupiter MOID2.16034 AU (323.182 Gm)
TJupiter3.244
Physical characteristics
Dimensions157.30 km[citation needed]
78.79±2.9 km[3]
74.125±2.04 km[4]
Mass(5.00±1.78)×1018 kg[4]
Mean density
2.93±1.06 g/cm3[4]
Equatorial surface gravity
~0.107m/s2
Equatorial escape velocity
~129.9m/s
14.845 h (0.6185 d)[3]
7.405±0.010 h[5]
0.0520±0.004
Temperature~167.4K
P
7.84

804 Hispania is a minor planet orbiting the Sun. It was discovered from Barcelona (Spain) on 20 March 1915 by Josep Comas Solá (1868–1937), the first asteroid to be discovered by a Spaniard. Hispania is a carbonaceous C-type asteroid. Busarev and Taran (2002) classed it as CP type with a spectrum that shows a highly hydrated body.[6] It has a diameter of 122 kilometers according to measurements made with the W. M. Keck Observatory. This is 30% smaller than the size estimated from the IRAS observatory data. It has a size ratio of 1.16 between its major and minor axes.[7] Two alternate rotation periods have been found for this asteroid: 7.4 hours and double that at 14.8 hours. To explain this discrepancy, it is possible the asteroid has a peculiar shape or it may be a double asteroid.[4]

References

  1. Webster, Noah (1884), A Practical Dictionary of the English Language
  2. 2.0 2.1 "Hispanian". Oxford English Dictionary (Online ed.). Oxford University Press. (Subscription or participating institution membership required.)
  3. 3.0 3.1 3.2 "804 Hispania (1915 WT)". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. Retrieved 4 May 2016.
  4. 4.0 4.1 4.2 4.3 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.
  5. Calabresi, M.; Roselli, G. (April 2001), "The rotation period of 804 Hispania: Some considerations on its nature", Astronomy and Astrophysics, 369: 305–307, Bibcode:2001A&A...369..305C, doi:10.1051/0004-6361:20010114.
  6. Busarev, V. V.; Taran, M. N. (November 2002), "On the spectral similarity of carbonaceous chondrites and some hydrated and oxidized asteroids", Asteroids, Comets, and Meteors, 500: 933–936, Bibcode:2002ESASP.500..933B.
  7. Marchis, F.; et al. (November 2006), "Shape, size and multiplicity of main-belt asteroids. I. Keck Adaptive Optics survey", Icarus, vol. 185, no. 1, pp. 39–63, Bibcode:2006Icar..185...39M, doi:10.1016/j.icarus.2006.06.001, PMC 2600456, PMID 19081813, retrieved 27 March 2013.

External links