434 Hungaria
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434 Hungaria is a relatively small asteroid orbiting in the inner asteroid belt. 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.[1]
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.[2]
It is thought that there may be a genetic connection between 434 Hungaria and 3103 Eger and the aubrites.[2]
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See also
References
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External links
- Lightcurve plot of 434 HungariaTemplate:Category handler[<span title="Script error: No such module "string".">usurped]Script error: No such module "Check for unknown parameters"., Palmer Divide Observatory, B. D. Warner (2011)
- SDSS image taken on 01APR2003 /Fermats Brother
- Relation between 434 Hungaria, 3103 Eger, and e-type asteroids
- Near IR-spectra of 3 Hungaria family asteroids: 4483 Petofi, 3169 Ostro and 3940 Larion
- Asteroid Lightcurve Database (LCDB), query form (info Script error: No such module "webarchive".)
- Dictionary of Minor Planet Names, Google books
- Asteroids and comets rotation curves, CdR – Observatoire de Genève, Raoul Behrend
- Discovery Circumstances: Numbered Minor Planets (1)-(5000) – Minor Planet Center
- Template:AstDys
- Template:PAGENAMEBASE at the JPL Small-Body DatabaseTemplate:EditAtWikidata
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