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Topic: 324 Bamberga

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324 Bamberga

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	Bamberga discovery
		Bamberga also catalogued with number 324 is a small asteroid that it orbits between the Mars orbits and Jupiter that I could locate with the small telescope which I have, refractor of 90mm.
		Bamberga has an eccentricity of 0,3379, typical one of asteroids and a greater semiaxis of 2,6844 UA, therefore, in the perihelion or point next in its orbit to the Sun is to 1.78UA, and in the aphelion or point more moved away to 3.59UA.
		Bamberga has an orbital period of 4,40 years and a period of rotation of 29,43 hours.
	www.mallorcaweb.net /masm/Bamberga1.htm (437 words)

	Radar aperture synthesis observations of asteroids (Site not responding. Last check: 2007-10-16)
		We report results of Goldstone-VLA, radar aperture-synthesis observations of the mainbelt asteroids 324 Bamberga and 7 Iris and the near-Earth asteroids 1991 EE and 4179 Toutatis.
		Simultaneous resolution of echoes in both angle and Doppler frequency provide new constraints on the mainbelt asteroids' pole directions: Bamberga's spin vector is within 40 deg.
		For Bamberga, monostatic and bistatic radar echoes and VLA thermal-emission measurements, also reported here, are consistent with radiometric estimates of Bamberga's size and with the hypothesis that the asteroid is overlain by a regolith having a porosity of ~50%.
	echo.jpl.nasa.gov /publications/radar_aperture_synthesis_abs.html (190 words)

	Astron. Astrophys. 331, 1113-1118 (1998)
		Two minor planets (2) Pallas and (324) Bamberga have been selected for the application of the method.
		The meridian observations of Pallas and all the observations of Bamberga were selected and given weights in the same way as detailed in Viateau and Rapaport (1997).
		Observed minus calculated positions O-C for (2) Pallas and (324) Bamberga over the period 1984-1994, using the orbital elements given in the "Ephemerides of Minor Planets for 1995".
	aa.springer.de /papers/8331003/2301113/sc3.htm (426 words)

	324 Bamberga -- Facts, Info, and Encyclopedia article (Site not responding. Last check: 2007-10-16)
		324 Bamberga -- Facts, Info, and Encyclopedia article
		324 Bamberga is the 16th largest (Any of numerous small celestial bodies composed of rock and metal that move around the sun (mainly between the orbits of Mars and Jupiter)) asteroid in the (Click link for more info and facts about Main asteroid belt) Main asteroid belt.
		It was discovered by (Click link for more info and facts about Johann Palisa) Johann Palisa on February 25, 1892 in (The capital and largest city of Austria; located on the Danube in northeastern Austria; was the home of Beethoven and Brahms and Haydn and Mozart and Schubert and Strauss) Vienna.
	www.absoluteastronomy.com /encyclopedia/3/32/324_bamberga.htm (132 words)

	324 BC - Encyclopedia Glossary Meaning Explanation 324 BC (Site not responding. Last check: 2007-10-16)
		324 BC - Encyclopedia Glossary Meaning Explanation 324 BC 324 BC - Encyclopedia Glossary Meaning Explanation 324 BC.
		Informations for 324 BC Centuries: 5th century BC - 4th century BC - 3rd century BC Decades: 370s BC 360s BC 350s BC 340s BC 330s BC - 320s BC - 310s BC 300s BC 290s BC 280s BC 270s BC Births
		The orginal 324 BC article can be editet
	www.encyclopedia-glossary.com /en/324-BC.html (151 words)

	Radar Observation Support (Site not responding. Last check: 2007-10-16)
		On 2000 Sept 8-14 we will be observing some MBAs: 88 Thisbe, 336 Lacadiera 914 Palisana 111 Ate 324 Bamberga.
		All of those have periods, but it would be nice to have a phased-up lightcurve for Bamberga, for which we should get decent images (unless it is known so well that it isn't necessary to take more data).
		For the rest we will probably only get bandwidth and integrated surface properties, and the period is sufficient.
	www.minorplanetobserver.com /_astlc/00000017.htm (115 words)

	Update for (324) Bamberga - June 18, 2002
		IOTA/IOTA-ES occultation update for (324) Bamberga / TYC 0256-00656-1 on June 18, 2002 visible from north Africa Summary
		In evening of June 18, 2002 a faint 11.9 mag star TYC 0256-00656-1 will be occulted by a 228 km asteroid (324) Bamberga.
		This update is based on USNO/Flagstaff and TMO astrometry for the asteroid and recent UCAC star position.
	sorry.vse.cz /~ludek/mp/updates/2002/0618bam.html (374 words)

	Asteroids and Remote Planets Section (Site not responding. Last check: 2007-10-16)
		Ephemerides of bright objects are given in the Association's Handbook and tracking charts may be available on the Section web pages.
		All apart from 12, 324 and 654 come to opposition in 2001.
		The minor Solar System bodies share many characteristics in common.
	yan.open.ac.uk /~ajh47/arps.htm (641 words)

	SHARCII User's Manual
		Some asteroids can be used for pointing and, if good models are available, flux calibration.
		The following asteroids are available in the UIP, at least through 2005: AMPHITRITE (29), BAMBERGA (324), CERES (1), DAVIDA (511), DESIDERATA (344), EGERIA (13), EUNOMIA (15), EUROPA52 (52), HERCULINA (532), HYGIEA (10), INTERAMNIA (704), JUNO (3), PALLAS (2), PROKNE (194), PSYCHE (16), VESTA (4).
		Some asteroids are only useful when near closest approach to the Earth.
	www.submm.caltech.edu /~sharc/operating/manual.htm (3631 words)

	COMMISSION 15: PHYSICAL STUDY OF COMETS, MINOR PLANETS AND METEORITES
		(1994, 92) reported on Goldstone-VLA, radar aperture-synthesis observations of the mainbelt asteroids 324 Bamberga and 7 Iris and the near-Earth asteroids 1991 EE and 4179 Toutatis.
		From these observations they concluded that Bamberga's spin vector is within 40
		Their results are consistent with radiometric estimates of Bamberga's size and with the hypothesis that the asteroid is overlain by a regolith having a porosity of approximately 50%.
	www.ss.astro.umd.edu /IAU/comm15/trirep97/Report97.html (13752 words)

	A.L.P.O. MINOR PLANETS SECTION - MAP ALERTS FOR 2004
		***********************************************************************= MAP Alert #324**, December 6, 2004: Greetings MAP Observers: Lone observations of NEO 2004 RZ164 highlight this brief call for = observations MAP Alert.
		Observing myself last night, = December 5-6 UT, I found 2004 = RZ164 not visible despite its predicted Mv 13.1.
		During the trip, I observed 324 Bamberga (mag 9.5) with a small Celestron 90, in the low parts of the Sagittarius for the fun, on August 15.
	www.lpl.arizona.edu /~rhill/alpo/minplan/alert2004.html (5602 words)

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