Matches in DBpedia 2016-04 for { <http://wikidata.dbpedia.org/resource/Q151102> ?p ?o }
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- Q151102 subject Q19795229.
- Q151102 subject Q3919730.
- Q151102 subject Q7299791.
- Q151102 subject Q7607653.
- Q151102 subject Q8273192.
- Q151102 absoluteMagnitude "6.82".
- Q151102 abstract "324 Bamberga is one of the largest asteroids in the asteroid belt. It was discovered by Johann Palisa on February 25, 1892 in Vienna. It is the 14th largest asteroid in the asteroid belt. Apart from the near-Earth asteroid Eros, it was the last asteroid which is ever easily visible with binoculars to be discovered.Although its very high orbital eccentricity means its opposition magnitude varies greatly, at a rare opposition near perihelion Bamberga can reach a magnitude of +8.0, which is as bright as Saturn's moon Titan. Such near-perihelion oppositions occur on a regular cycle every twenty-two years, with the last occurring in 2013 and the next in 2035, when attaining magnitude 8.1 on September 13. Its brightness at these rare near-perihelion oppositions makes Bamberga the brightest C-type asteroid, roughly one magnitude brighter than 10 Hygiea's maximum brightness of around +9.1. At such an opposition Bamberga can in fact be closer to Earth than any main-belt asteroid with magnitude above +9.5, getting as close as 0.78 AU. For comparison, 7 Iris never comes closer than 0.85 AU and 4 Vesta never closer than 1.13 AU (when it becomes visible to the naked eye in a light pollution-free sky).Overall Bamberga is the tenth brightest main-belt asteroid after, in order, Vesta, Pallas, Ceres, Iris, Hebe, Juno, Melpomene, Eunomia and Flora. Its high eccentricity (for comparison 36% higher than that of Pluto), though, means that at most oppositions other asteroids reach higher magnitudes.The 29 hour rotation period is unusually long for an asteroid more than 150 km in diameter. Its spectral class is intermediate between the C-type and P-type asteroids.10µ radiometric data collected from Kitt Peak in 1975 gave a diameter estimate of 255 km. An occultation of Bamberga was observed on 8 December 1987, and gave a diameter of about 228 km, in agreement with IRAS results. In 1988 a search for satellites or dust orbiting this asteroid was performed using the UH88 telescope at the Mauna Kea Observatories, but the effort came up empty.".
- Q151102 albedo "0.0628".
- Q151102 apoapsis "5.37241E11".
- Q151102 averageSpeed "65448.0".
- Q151102 discovered "1892-02-25".
- Q151102 discoverer Q78486.
- Q151102 epoch "30 January 2005 (JD2453400.5)".
- Q151102 escapeVelocity "396.0".
- Q151102 formerName "none".
- Q151102 orbitalPeriod "1.3870630079999998E8".
- Q151102 periapsis "2.65576E11".
- Q151102 rotationPeriod "105926.40000000001".
- Q151102 rotationPeriod "105948.0".
- Q151102 temperature "172.0".
- Q151102 thumbnail 324_Bamberga.gif?width=300.
- Q151102 wikiPageWikiLink Q102626.
- Q151102 wikiPageWikiLink Q107486.
- Q151102 wikiPageWikiLink Q107495.
- Q151102 wikiPageWikiLink Q107509.
- Q151102 wikiPageWikiLink Q107528.
- Q151102 wikiPageWikiLink Q11579.
- Q151102 wikiPageWikiLink Q117550.
- Q151102 wikiPageWikiLink Q124313.
- Q151102 wikiPageWikiLink Q1333532.
- Q151102 wikiPageWikiLink Q14267.
- Q151102 wikiPageWikiLink Q1659605.
- Q151102 wikiPageWikiLink Q16711.
- Q151102 wikiPageWikiLink Q1741.
- Q151102 wikiPageWikiLink Q175821.
- Q151102 wikiPageWikiLink Q180644.
- Q151102 wikiPageWikiLink Q1811.
- Q151102 wikiPageWikiLink Q185981.
- Q151102 wikiPageWikiLink Q193.
- Q151102 wikiPageWikiLink Q19795229.
- Q151102 wikiPageWikiLink Q217208.
- Q151102 wikiPageWikiLink Q2179.
- Q151102 wikiPageWikiLink Q2373252.
- Q151102 wikiPageWikiLink Q2565.
- Q151102 wikiPageWikiLink Q2640.
- Q151102 wikiPageWikiLink Q265392.
- Q151102 wikiPageWikiLink Q3002.
- Q151102 wikiPageWikiLink Q3009.
- Q151102 wikiPageWikiLink Q3030.
- Q151102 wikiPageWikiLink Q339.
- Q151102 wikiPageWikiLink Q3863.
- Q151102 wikiPageWikiLink Q3919730.
- Q151102 wikiPageWikiLink Q3936.
- Q151102 wikiPageWikiLink Q4052125.
- Q151102 wikiPageWikiLink Q506254.
- Q151102 wikiPageWikiLink Q5193851.
- Q151102 wikiPageWikiLink Q596.
- Q151102 wikiPageWikiLink Q724913.
- Q151102 wikiPageWikiLink Q729623.
- Q151102 wikiPageWikiLink Q7299791.
- Q151102 wikiPageWikiLink Q7607653.
- Q151102 wikiPageWikiLink Q78486.
- Q151102 wikiPageWikiLink Q8273192.
- Q151102 wikiPageWikiLink Q831790.
- Q151102 absMagnitude "6.82".
- Q151102 albedo "0.0628".
- Q151102 altNames "none".
- Q151102 aphelion "537.241".
- Q151102 avgSpeed "18.18".
- Q151102 discovered "1892-02-25".
- Q151102 discoverer Q78486.
- Q151102 epoch "2005-01-30".
- Q151102 escapeVelocity "0.11".
- Q151102 name "324".
- Q151102 perihelion "265.576".
- Q151102 period "1.3870630079999998E8".
- Q151102 rotation "105926.40000000001".
- Q151102 singleTemperature "~172 K".
- Q151102 type Place.
- Q151102 type CelestialBody.
- Q151102 type Location.
- Q151102 type Place.
- Q151102 type Planet.
- Q151102 type Thing.
- Q151102 type Q634.
- Q151102 comment "324 Bamberga is one of the largest asteroids in the asteroid belt. It was discovered by Johann Palisa on February 25, 1892 in Vienna. It is the 14th largest asteroid in the asteroid belt.".
- Q151102 label "324 Bamberga".
- Q151102 depiction 324_Bamberga.gif.
- Q151102 name "324 Bamberga".
