Category:Main Belt asteroids

Category:Main Belt asteroids - Factbites
Where results make sense
About us | Why use us? | Reviews | PR | Contact us

Topic: Category:Main Belt asteroids

Note: these results are not from the primary (high quality) database.

	E-class asteroid
		E-class asteroids dominate the Hungaria group of the main belt, though some, including the two largest, (44) Nysa (see Nysa-Polana family and (64) Angelina, are found scattered further out.
		A rare category of asteroid, slightly red in color and spectrally similar to M-class asteroids and P-class asteroids, but of higher albedo (in the range 0.25-0.60).
		Their flat reflectance spectra in the 0.3 to 1.0 micron region and high albedos suggest a connection with the aubrite (otherwise known as enstatite achondrite, hence the "E") category of meteorite.
	daviddarling.info /encyclopedia/E/Easter.html (207 words)

	E-class asteroid
		E-class asteroids dominate the Hungaria group of the main belt, though some, including the two largest, (44) Nysa (see Nysa-Polana family and (64) Angelina, are found scattered further out.
		A rare category of asteroid, slightly red in color and spectrally similar to M-class asteroids and P-class asteroids, but of higher albedo (in the range 0.25-0.60).
		Their flat reflectance spectra in the 0.3 to 1.0 micron region and high albedos suggest a connection with the aubrite (otherwise known as enstatite achondrite, hence the "E") category of meteorite.
	www.daviddarling.info /encyclopedia/E/Easter.html (207 words)

	163 Erigone - Result for 163 Erigone - Meaning of 163 Erigone - Definition of 163 Erigone - Dictionary of Meaning - www.mauspfeil.net
		Perrotin, 1876} '''163 Erigone''' is a dark-coloured, fairly big Asteroid belt Main belt asteroid, the namesake of the Erigone family of asteroids.
		{{MinorPlanets_Footer}} Category:Erigone asteroids Erigone de:Erigone (Asteroid) es:(163) Erigona
		There you find a list of all editors and the possibility to edit the original text of the article 163 Erigone.
	www.mauspfeil.net /163_Erigone.html (207 words)

	E-class asteroid
		E-class asteroids dominate the Hungaria group of the main belt, though some, including the two largest, (44) Nysa (see Nysa-Polana family and (64) Angelina, are found scattered further out.
		Their flat reflectance spectra in the 0.3 to 1.0 micron region and high albedos suggest a connection with the aubrite (otherwise known as enstatite achondrite, hence the "E") category of meteorite.
		However, this link is problematic because aubrites are clearly of igneous origin, whereas some E-class asteroids (including Nysa) show an absorption feature at 3 microns that points to water- and/or hydroxyl-bearing minerals and a non-igneous history.
	www.daviddarling.info /encyclopedia/E/Easter.html (207 words)

	A/CC Catalog: Asteroids 80000-89999
		The NEODyS NEO database entry for NT7, at last check, shows only one coming planetary encounter, with Main Belt asteroid 2 Pallas in the year 2020 at about ten lunar distances.
		Very different orbital elements were announced in June 2002 that put it into the somewhat less exotic Centaur category.
		NT7 had only just recently been removed from low priority status on the Spaceguard Central Node's Priority List, where it had been since a couple of weeks after it was pulled from the JPL and NEODyS risk pages in early Aug. 2002.
	www.hohmanntransfer.com /cat/an10.htm (767 words)

Try your search on: Qwika (all wikis)

Topic: Category:Main Belt asteroids

Ads by Google