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Topic: 704 Interamnia

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	704 Interamnia (Site not responding. Last check: 2007-09-07)
		704 Interamnia ("IN ter AM nee uh") is a very large asteroid with a diameter of 350 kilometres.
		It was discovered on October 2, 1910 by Vincenzo Cerulli, and named after the Latin name for Teramo, Italy, where Cerulli worked.
		Interamnia is the sixth largest known asteroid within Jupiter's orbit and was discovered surprisingly late for such a large object.
	pedia.newsfilter.co.uk /wikipedia/7/70/704_interamnia.html (89 words)

	Vincenzo Cerulli - Wikipedia, the free encyclopedia
		He also observed Mars and developed the theory that the Martian canals were not real but an optical illusion, a theory that was later confirmed.
		He discovered one asteroid, 704 Interamnia, which is named after the Latin name for Teramo, and is notable for its relatively large diameter of approximately 350 km, which makes it one of the largest bodies in the traditional asteroid belt.
		A crater on Mars is named after Cerulli, as is the asteroid 366 Vincentina.
	www.wikipedia.org /wiki/Vincenzo_Cerulli (133 words)

	Interamnia (Site not responding. Last check: 2007-09-07)
		Interamnia was discovered on October 2, 1910 by Vincenzo Cerulli.
		The asteroid was given the Latin name for the town in which it was discovered, Teramo, Italy.
		It is approximately 3.07 AU from the sun, placing it well within the boundaries of the asteroid belt.
	physics.bgsu.edu /~layden/Anim/Asteroids/interamnia.htm (170 words)

	interamnia_japan (Site not responding. Last check: 2007-09-07)
		Occultation of HIP 36189 by 704 Interamnia, 2003 March 23
		Interamnia was estimated to have a 316 km diameter.
		The predicted maximum length of occultation was 62.8 seconds with a magnitude change of 3.9.
	tufi.alphalink.com.au /astro/interamnia_japan.htm (240 words)

	No Title (Site not responding. Last check: 2007-09-07)
		Occultation of GSC 23450183 by (704) Interamnia on 1996 December 17
		The sixth largest of the known asteroids, (704) Interamnia, was observed to occult GSC 23450183 (from the HST Guide Star Catalog) by 10 teams of observers.
		This lightcurve structure supports the presence of topography on the object as seen in the limb fit to the occultation chords.
	www.lpi.usra.edu /meetings/dps97/html/H0710/H0710.html (304 words)

	Buie: Occultation Prediction for (704) Interamnia, 96/12/17 (Site not responding. Last check: 2007-09-07)
		Asteroid (704) Interamnia will occult a 10th magnitude star in the early morning hours of 1996 Dec 17, as discovered by Edwin Goffin and reported by David Dunham.
		At the time of the event, Interamnia will be 40 degrees above the horizon as seen from Flagstaff.
		The prediction team consists of Ron Stone at the US Naval Observatory providing transit measurements, Larry Wasserman at Lowell Observatory is processing the measurements and generating the predictions and plots, and Marc Buie, also Lowell Obs., is coordinating the collection and dissemination of information (like this WWW page).
	www.lowell.edu /~buie/occ/704pred.html (370 words)

	704 Interamnia - Encyclopedia, History, Geography and Biography
		704 Interamnia ("IN ter AM nia") is a very large asteroid with a diameter of 350 kilometres.
		This page was last modified 03:24, 19 Jun 2005.
		This encyclopedia, history, geography and biography article about 704 Interamnia contains research on
	www.arikah.net /encyclopedia/704_Interamnia (135 words)

	Catalogo Articoli (Site not responding. Last check: 2007-09-07)
		New masses of eight asteroids: (6) Hebe, (10) Hygiea, (15) Eunomia, (52) Europa, (88) Thisbe, (444) Gyptis, (511) Davida, and (704) Interamnia, were determined.
		In most cases, the masses were calculated by means of the least-squares method as the weighted means of the values found separately from the perturbations on several single asteroids.
		The masses of Hebe, Hygiea, Eunomia, Europa, Thisbe, Gyptis, Davida and Interamnia were determined from perturbations on, respectively, 2, 8, 3, 4, 1, 1, 2 and 3 asteroids.
	serials.cib.unibo.it /cgi-ser/start/it/spogli/df-s.tcl?prog_art=4132313&language=ITALIANO&view=articoli (311 words)

	Interamnia Occultation Mar. 23 timed in Hawaii & Japan (Site not responding. Last check: 2007-09-07)
		The 2003 March 23rd occultation is the best-observed one involving (704) Interamnia, but it's not the first!
		Below is a quick reply to Jim Bedient giving him (and now you) an expanded account of the successful observations of the Saturday March 23rd occultation of SAO 96908 by (704) Interamnia.
		The link below shows the outline of Interamnia determined from several of the Japanese observations, and a map of central Japan locating the observers and the actual path there (the map there does not show the Maui observers like Hirose's map below).
	iota.jhuapl.edu /mp704327.htm (544 words)

	Ephemerides of the Largest Asteroids (Site not responding. Last check: 2007-09-07)
		Except for Davida and Interamnia all of the asteroids are fit to substantially more data over substantially more oppositions than the ephemerides described in Table 2.
		The perturbing asteroids included in the ephemeris of each asteroid are given in Table 4.The mass for Interamnia was the mean of two values determined by Landgraff (1992).
		The mass for Davida is the estimate used by Viateau & Rapaport(1997).
	aa.usno.navy.mil /hilton/ephemerides/asteroid_ephemerides.html (9264 words)

	Asteroid_News.htm (Site not responding. Last check: 2007-09-07)
		654 Zelinda 1263 Varsavia 469 Argentina 85 Io 704 Interamnia 856 Backlunda 95 Arethusa
		The large "F" class asteroid 704 Interamnia occulted a m = 6.6 star on March 23, 2003.
		Interamnia was discovered October 2, 1910 by V. Cerulli in Teramo, Italy.
	weblore.com /richard/Asteroid_News.htm (4476 words)

	Determination of asteroid masses
		(6) Hebe, (10) Hygiea, (15) Eunomia, (52) Europa, (88) Thisbe, (444) Gyptis, (511) Davida and (704) Interamnia
		A discussion on individual mass determinations is also presented.
		planets and satellites: individual: 6 Hebe, 10 Hygiea, 15 Eunomia, 52 Europa, 88 Thisbe, 444 Gyptis, 511 Davida, 704 Interamnia
	www.edpsciences.org /articles/aa/abs/2001/29/aa10228/aa10228.html (258 words)

	DDA Newsletter January 2000
		These are the asteroid ephemerides which will appear in the Astronomical Almanac beginning with the edition for the year 2000.
		USNO/AE98 includes the asteroids 1 Ceres, 2 Pallas, 3 Juno, 4 Vesta, 6 Hebe, 7 Iris, 8 Flora, 9 Metis, 10 Hygiea, 15 Eunomia, 16 Psyche, 52 Europa, 65 Cybele, 511 Davida, and 704 Interamnia.
		USNO/AE98 is based on the JPL DE405 planetary ephemerides and covers the period 1799 November 16 (JD 2378450.5) through 2100 February 1 (JD 2488100.5).
	dda.harvard.edu /newsletters/ddanews85.html (1492 words)

	BAA Asteroids and Remote Planets Section - Recent News (Site not responding. Last check: 2007-09-07)
		You can see for yourself how unlucky mainland European observers were for this one!
		REPORT on 704 Interamnia Occultation Event of 1997 Mar 02
		A short report of the event on 1997 March 02 20:43 UT follows:
	www.ast.cam.ac.uk /~baa/arpsnews.html (2990 words)

	Cambridge Conference Correspondence
		(15) Eunomia, (52) Europa, (88) Thisbe, (444) Gyptis, (511) Davida and (704)
		Europa, (88) Thisbe, (444) Gyptis, (511) Davida, and (704) Interamnia, were
		Hygiea, Eunomia, Europa, Thisbe, Gyptis, Davida and Interamnia were
	abob.libs.uga.edu /bobk/ccc/cc083001.html (6469 words)

	British Astronomical Association News Page (Site not responding. Last check: 2007-09-07)
		Two Starlight Xpress SX-M CCD images of Comet 1997T1 (Utsunomiya) in Cepheus contributed by Maurice Gavin using 500mm f8 Maksutov.
		Below (courtesy of Maurice Gavin) is a series of CCD images of the recent occultation event involving the asteroid, 704 Interamnia.
		The occultation was predicted to take place at 20:43 UT on March 02 and be visible from the UK.
	www.ast.cam.ac.uk /~baa/baanews.html (5143 words)

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