434 Hungaria

434 Hungaria
Lightcurve-based 3D model of 434 Hungaria
Discovery
Discovered byMax Wolf
Discovery date11 September 1898
Designations
Pronunciation/hʌŋˈɡɛəriə/
Named after
Hungary
1898 DR
Asteroid belt (Hungaria)
Orbital characteristics
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc117.58 yr (42946 d)
Aphelion2.0878 AU (312.33 Gm)
Perihelion1.8011 AU (269.44 Gm)
1.9444 AU (290.88 Gm)
Eccentricity0.073725
2.71 yr (990.34 d)
221.145°
0° 21m 48.636s / day
Inclination22.511°
175.332°
123.80°
Physical characteristics
Dimensions~11 km
26.521 h (1.1050 d)
0.428
E
11.21

434 Hungaria is a relatively small asteroid orbiting in the inner asteroid belt that is approximately 11 kilometers in diameter. It is an E-type (high-albedo) asteroid. It is the namesake of the Hungaria asteroids, which orbit the Sun on the inside of the 1:4 Kirkwood gap, standing out of the core of the asteroid belt.

It was discovered by Max Wolf on 11 September 1898 at the University of Heidelberg. It was named after Hungary, which hosted an astronomical meeting in 1898 in Budapest.

It is thought that 434 Hungaria, 3103 Eger and the aubrite meteorites may share a common origin.

Orbit of 434 Hungaria

See also

References

  1. 1 2 3 4 5 "JPL Small-Body Database Browser: 434 Hungaria (1898 DR)" (last observation: 2015-11-21). Jet Propulsion Laboratory. Retrieved 10 May 2016.
  2. ↑ Shepard, Michael K.; Kressler, Karelyn M. (2008). "Radar observations of E-class Asteroids 44 Nysa and 434 Hungaria". Icarus. 195 (1): 220–225. Bibcode:2008Icar..195..220S. doi:10.1016/j.icarus.2007.12.018.
  3. ↑ Spratt, Christopher E. (April 1990). "The Hungaria group of minor planets". Journal of the Royal Astronomical Society of Canada (abstract). 84 (2): 123–131. Bibcode:1990JRASC..84..123S. ISSN 0035-872X.
  4. 1 2 Kelley, Michael S.; Gaffey, Michael J. (December 2002). "High-albedo asteroid 434 Hungaria: Spectrum, composition and genetic connections". Meteoritics & Planetary Science (abstract). 37 (12): 1815–1827. Bibcode:2002M&PS...37.1815K. doi:10.1111/j.1945-5100.2002.tb01165.x.