DBpedia – Linked Data Fragments

Matches in DBpedia 2016-04 for { <http://wikidata.dbpedia.org/resource/Q431499> ?p ?o }

• Q431499 subject Q19795229.
• Q431499 subject Q8273453.
• Q431499 subject Q8300362.
• Q431499 subject Q8380129.
• Q431499 subject Q8527668.
• Q431499 absoluteMagnitude "14.2".
• Q431499 absoluteMagnitude "14.4".
• Q431499 abstract "9069 Hovland, provisional designation 1993 OV, is a stony binary asteroid from the inner regions of the asteroid belt, about 3 kilometers in diameter. It was discovered by American female astronomer Eleanor Helin at the U.S. Palomar Observatory in California, on 16 July 1993.The bright E-type asteroid is a member of the Hungaria family, which form the innermost dense concentration of asteroids in the Solar System. It orbits the Sun at a distance of 1.7–2.1 AU once every 2 years and 8 months (966 days). Its orbit shows an eccentricity of 0.12 and an inclination of 20 degrees from the plane of the ecliptic.Several photometric light-curve analysis from the Spitzer Space Telescope and other ground-based observations including the U.S Palmer Divide Observatory (PDO), Colorado, rendered a well-defined rotation period of 7000421580000000000♠4.2158±0.0001 hours (most recent observation) with a very low brightness amplitude in the range between 0.008 and 0.011 in magnitude. Such a low amplitude typically means that the asteroid has a nearly spheroidal shape. In 2004, PDO reported the discovery of an asteroid moon making the asteroid a binary system. The moon's orbital period has since been measured to take 30.292, 30.34 and 30.35 hours, respectively, for a full orbit around its primary.While Spitzer and others gave it a high albedo of 0.373, with a corresponding diameter of 2.9 kilometers, the Collaborative Asteroid Lightcurve Link assumes a more typical albedo of 0.30, calculating therefore a somewhat larger diameter of 3.5 kilometers, as the lower the body's reflectivity (albedo), the larger its diameter for a given absolute brightness (magnitude).The minor planet was named in honor of Larry E. Hovland (b. 1947), who is a senior engineer at the Jet Propulsion Laboratory responsible for the Raman spectrometer electronics and the Mars 2005 Op-Nav camera electronics. He generously provided his expertise to the discoverer in her early efforts to convert from photographic to electronic detection methods.".
• Q431499 albedo "0.3".
• Q431499 apoapsis "3.1995992585316E11".
• Q431499 discovered "1993-07-16".
• Q431499 discoverer Q58962.
• Q431499 epoch "27 June 2015 (JD2457200.5)".
• Q431499 formerName "1993 OV".
• Q431499 orbitalPeriod "228960.0".
• Q431499 periapsis "2.5238656765797E11".
• Q431499 rotationPeriod "15181.199999999999".
• Q431499 wikiPageExternalLink page_cou.html.
• Q431499 wikiPageExternalLink GenerateALCDEFPage_Local.php?AstInfo=9069%7CHovland.
• Q431499 wikiPageExternalLink NumberedMPs005001.html.
• Q431499 wikiPageExternalLink lcdbsummaryquery.php.
• Q431499 wikiPageExternalLink lightcurvedatabase.html.
• Q431499 wikiPageExternalLink books?id=aeAg1X7afOoC&pg.
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• Q431499 wikiPageWikiLink Q8273453.
• Q431499 wikiPageWikiLink Q8300362.
• Q431499 wikiPageWikiLink Q8380129.
• Q431499 wikiPageWikiLink Q8527668.
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• Q431499 absMagnitude "14.2".
• Q431499 absMagnitude "14.4".
• Q431499 albedo "0.3".
• Q431499 altNames "1993".
• Q431499 aphelion "2.1388".
• Q431499 discovered "1993-07-16".
• Q431499 discoverer Q58962.
• Q431499 epoch "2015-06-27".
• Q431499 name "9069".
• Q431499 perihelion "1.6871".
• Q431499 period "8.362764E7".
• Q431499 rotation "15181.199999999999".
• Q431499 rotation "h".
• Q431499 type Place.
• Q431499 type CelestialBody.
• Q431499 type Location.
• Q431499 type Place.
• Q431499 type Planet.
• Q431499 type Thing.
• Q431499 type Q634.
• Q431499 comment "9069 Hovland, provisional designation 1993 OV, is a stony binary asteroid from the inner regions of the asteroid belt, about 3 kilometers in diameter. It was discovered by American female astronomer Eleanor Helin at the U.S. Palomar Observatory in California, on 16 July 1993.The bright E-type asteroid is a member of the Hungaria family, which form the innermost dense concentration of asteroids in the Solar System.".
• Q431499 label "9069 Hovland".
• Q431499 name "9069 Hovland".