DOES MARS HAVE A PRISTINE, -2 CUMULATIVE POWER LAW DISTRIBUTION FOR CRATERS >5 KM IN DIAMETER? K.L. Tanaka1, J.A. Skinner, Jr.1, and N.G. Barlow2. 1Astrogeology Team, U.S. Geological Survey, Flagstaff, AZ[removed]ktanaka@ - Alba Mons - Document - PDFSEARCH.IO

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	DOES MARS HAVE A PRISTINE, -2 CUMULATIVE POWER LAW DISTRIBUTION FOR CRATERS >5 KM IN DIAMETER? K.L. Tanaka1, J.A. Skinner, Jr.1, and N.G. Barlow2. 1Astrogeology Team, U.S. Geological Survey, Flagstaff, AZ[removed]ktanaka@ Add to Reading List Document Date: 2004-10-06 14:26:31 Open Document File Size: 155,42 KB Share Result on Facebook City Flagstaff / / Company Frey H.V. (2003) Sixth Intl / / / IndustryTerm power-law slope / slope power law / impact energy / power law slope / / NaturalFeature km craters / / OperatingSystem Elysium / / Organization Vastitas Borealis and Arcadia Formations / Northern Arizona Univ. / / Person J.A. Skinner / Jr. / Alba Patera / / / ProvinceOrState Arizona / / Region Northern Arizona / / SocialTag Mars Hesperian Noachian Impact crater Alba Mons Yuty Geology Planetary science Planetary geology

DOES MARS HAVE A PRISTINE, -2 CUMULATIVE POWER LAW DISTRIBUTION FOR CRATERS >5 KM IN DIAMETER? K.L. Tanaka1, J.A. Skinner, Jr.1, and N.G. Barlow2. 1Astrogeology Team, U.S. Geological Survey, Flagstaff, AZ[removed]ktanaka@Add to Reading List