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Topic: 135 Hertha

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	Nysa-Polana family
		Its members move in low-inclination orbits at a mean distance from the Sun of 2.4 to 2.5 AU, a region of the belt showing an unusual abundance of the fairly rare F-class asteroids.
		The two largest members of the family are (44) Nysa (the largest E-class asteroid and the brightest asteroid known) and (135) Hertha.
		For instance, it is not clear how to interpret the role of as well as the presence of several large F-type asteroids apparently not related, but very close to the clan.
	www.daviddarling.info /encyclopedia/N/Nysa-Polana_family.html (293 words)

	135 Hertha -- Facts, Info, and Encyclopedia article (Site not responding. Last check: )
		135 Hertha -- Facts, Info, and Encyclopedia article
		Hertha was discovered by (additional info and facts about C. Peters) C.
		One (One celestial body obscures another) occultation of a ((astronomy) a celestial body of hot gases that radiates energy derived from thermonuclear reactions in the interior) star by the asteroid has been observed, in 2000.
	www.absoluteastronomy.com /encyclopedia/1/13/135_hertha.htm (390 words)

	[61.02] Asteroid Observations Using the Speckle Camera at TNG (Site not responding. Last check: )
		Also in this case the agreement is reasonable, and the speckle observations may allow us to discriminate between the two pole solutions usually found for each object.
		No clear evidence of binaries was found, although the asteroid 135 Hertha turns out to be much more elongated than previously suspected.
		The results show that the TNG speckle camera can be a powerful tool to resolve relatively large main belt asteroids, and to calibrate the results of the IRAS survey.
	www.aas.org /publications/baas/v33n3/dps2001/137.htm (248 words)

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