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Topic: 808 Merxia

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	808 merxia - OneLook Dictionary Search (Site not responding. Last check: 2007-10-31)
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	www.onelook.com /?w=808+merxia (99 words)

	Abstracts Vol. 39, Issue 8, August 2004
		Our analyses of high quality spectra of several S-type asteroids (17 Thetis, 847 Agnia, 808 Merxia, and members of the Agnia and Merxia families) reveal that they include both low- and high calcium pyroxene with minor amounts of olivine (<20%).
		High-calcium pyroxene is a spectrally detectable and petrologically important indicator of igneous history and may prove critical in future studies aimed at understanding the history of asteroidal bodies.
		The silicate mineralogy inferred for Thetis and the Merxia and Agnia family members requires that these asteroids experienced igneous differentiation, producing broadly basaltic surface lithologies.
	meteoritics.org /Abst_39-8.htm (2584 words)

	Minor planet - beginner-guide-to-online-day-trading.info (Site not responding. Last check: 2007-10-31)
		Adeona asteroids, named after 145 Adeona, ~65 members.
		Merxia asteroids, named after 808 Merxia, ~25-30 members.
		Misa asteroids, named after 569 Misa, ~26 members.
	beginner-guide-to-online-day-trading.info /Minor_planet (2469 words)

	NORTHWEST AFRICA 011 PHOTO
		Other differentiated and disrupted parent bodies have been identified in the central main belt (Bottke et al.
		These include the S-type, high-Ca pyroxene asteroids 17 Thetis, 847 Agnia, and 808 Merxia, as well as some possible exposed iron cores such as 16 Psyche and 216 Kleopatra.
		A very small amount of mantle material would be expected to survive the long journey from this distant region of the asteroid belt.
	www.meteoritestudies.com /protected_NWA011.HTM (1199 words)

	[No title]
		We consider the constraints that various source models impose on F(E), and we present explicit forms for an illustrative F(E) corresponding to the injection of a power-law spectrum of electrons into a thick target with a nonuniform ionization level.
		Title: Lightcurve photometry of asteroid 808 Merxia Authors: Koff, Robert A.; Brown, Janel; Menke, John Journal: The Minor Planet Bulletin (ISSN 1052-8091).
		Asteroid 808 Merxia was found to have a synodic period of 30.631 hours ± 0.001 hours and an amplitude of 0.81 ± 0.02 magnitude.
	www.phys.uu.nl /~rutten/rrtex/bibfiles/ads/abs/brown-john.txt (11533 words)

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