10 Hygiea ⯚ (The tradeetional astronomical seembol for 10 Hygiea)

Animated orbit o Hygiea relative tae the orbits o the terrestrial planets an Jupiter.
Discovery
Discovered biA. de Gasparis
Discovery dateAprile 12, 1849
Designations
Pronunciation/hˈə/ hy-JEE
Named after
Hygieia
Alternative names
none
Minor planet category
Main belt (Hygiea family)
AdjectivesHygiean
Orbital chairactereestics[1]
Epoch November 30, 2008 (JD 2454800.5)
Aphelion3.507 AU
(524.63 Gm) (Q)
Perihelion2.770 AU
(414.38 Gm) (q)
3.139 AU
(469.58 Gm)
Eccentricity0.117
Orbital period
5.56 yr
(2031.01 d)
Average orbital speed
16.76 km/s
Mean anomaly
197.96° (M)
Inclination3.842°
Longitude o ascendin node
283.45°
Argument o perihelion
313.19°
Proper orbital elements[2]
3.1417827 AU
Proper eccentricity
0.1356315
Proper inclination
5.1039060°
Proper mean motion
64.621768 deg / yr
Proper orbital period
5.57088 yr
(2034.763 d)
Precession o perihelion
128.543611 arcsec / yr
Precession of the ascending node
−96.902395 arcsec / yr
Pheesical chairacteristics
Dimensions530×407×370 ±7 km[3]
431 km (mean)
Surface area
837,080.744 km2 (323,198.682 sq mi)
Mass(8.67 ±0.15)×1019 kg[3]
Mean density
2.08 ± 0.10 g/cm³[3]
Surface gravity
0.091 m/s²
Escape velocity
0.21 km/s
27.623 h (1.15 d)[1]
Albedo0.0717 (geometric)[1]
Temperatur≈164 K
max: 247 K (−26°C) [4]
Spectral teep
C-type asteroid[1]
Apparent magnitude
9.0[5] to 11.97
5.43[1]
Angular diameter
0.321″ tae 0.133″

10 Hygiea is the fowert lairgest asteroid in the Solar Seestem bi volume an mass, an it is locatit in the asteroid belt.

References

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  1. a b c d e "JPL Small-Body Database Browser: 10 Hygiea". Retrieved 7 September 2008.
  2. "AstDyS-2 Hygiea Synthetic Proper Orbital Elements". Department of Mathematics, University of Pisa, Italy. Retrieved 1 October 2011.
  3. a b c Jim Baer (2010). "Recent Asteroid Mass Determinations". Personal Website. Archived frae the original on 21 October 2013. Retrieved 2 September 2011.
  4. L.F. Lim; McConnochie, T; Belliii, J; Hayward, T (2005). "Thermal infrared (8–13 µm) spectra of 29 asteroids: the Cornell Mid-Infrared Asteroid Spectroscopy (MIDAS) Survey". Icarus. 173 (2): 385. Bibcode:2005Icar..173..385L. doi:10.1016/j.icarus.2004.08.005.
  5. "AstDys (10) Hygiea Ephemerides". Department of Mathematics, University of Pisa, Italy. Retrieved 26 Juin 2010.