NEO Physical Characterization: Spin Rates and Spectra Eileen V. Ryan, Ph.D. Director, 2.4-Meter Telescope, Magdalena Ridge Observatory New Mexico Institute of Mining and Technology, Socorro, NM

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Date: 2014-02-03 13:12:36 Asteroid S-type asteroid Astronomy Planetary science Planetary defense Near-Earth object		NEO Physical Characterization: Spin Rates and Spectra Eileen V. Ryan, Ph.D. Director, 2.4-Meter Telescope, Magdalena Ridge Observatory New Mexico Institute of Mining and Technology, Socorro, NM Add to Reading List Source URL: minorplanetcenter.net Download Document from Source Website File Size: 2,96 MB Share Document on Facebook

	NATIONAL NEAR-EARTH OBJECT PREPAREDNESS STRATEGY PRODUCT OF THE INTERAGENCY WORKING GROUP FOR DETECTING AND MITIGATING THE IMPACT OF EARTH-BOUND NEAREARTH OBJECTS (NEOS) (DAMIEN) DocID: 1tY00 - View Document
	Printer Sheet - Zelia copy DocID: 1qJIU - View Document
	Printer Sheet - YORP copy DocID: 1qEXt - View Document
	Printer Sheet - Itokawa copy DocID: 1qz1x - View Document
	Printer Sheet - Gaspra copy DocID: 1qprz - View Document