804 Hispania

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.

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 arc108.57 yr (39655 d)
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°
 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
Mean radius
78.79±2.9 km[3]
74.125 ± 2.04 km[4]
Mass(5.00 ± 1.78) × 1018 kg[4]
9.95×1018
Mean density
2.93 ± 1.06 g/cm3[4]
4.90 g/cm³
Equatorial surface gravity
~0.107m/s2
Equatorial escape velocity
~129.9m/s
14.845 h (0.6185 d)[3]
7.405 hr[5]
0.0520±0.004
Temperature~167.4K
P
7.84

    Hispania is a carbonaceous C-type asteroid and 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.[6]

    References

    1. Noah Webster (1884) A Practical Dictionary of the English Language
    2. "Hispanian". Oxford English Dictionary (3rd ed.). Oxford University Press. September 2005. (Subscription or UK public library membership required.)
    3. "804 Hispania (1915 WT)". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. Retrieved 4 May 2016.
    4. Carry, B. (December 2012), "Density of asteroids", Planetary and Space Science, 73, pp. 98–118, arXiv:1203.4336, Bibcode:2012P&SS...73...98C, doi:10.1016/j.pss.2012.03.009. See Table 1.
    5. Marchis, F.; et al. (November 2006), "Shape, size and multiplicity of main-belt asteroids. I. Keck Adaptive Optics survey", Icarus, 185 (1), pp. 39–63, Bibcode:2006Icar..185...39M, doi:10.1016/j.icarus.2006.06.001, PMC 2600456, PMID 19081813, retrieved 27 March 2013.


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