title: Instrumental neutron activation analyses of lunar specimens.
abstract: Ten Apollo 11 specimnens were divided into 24 samtples. Sodillim contents of 8 diverse specimens clluster tightly abolit 0.3 percent. Plagioclase separated from sample 10044 contains aboltt 1.09 percent Na; barium is not enriched in the plagioclase separate. Contents of the rare earths are strikingly high, and relative abtmndances resemble those of calcium-rich achondrites or abyssal basalts but are depleted in Eu by factors of 2 to 3 and in La by about 20 percent. The plagioclase separate is enriched in Eu and pyroxenes (and opaqtte minerals are Eu-depleted. Fine fractions of 10044 are abotit 20 to 40 percent richer in most rare earths (50 percent for Eu) than coarse fractions, probably becaitse of the presence of small grains in which rare earths are mnarkedly concentrated. "Microgabbro" 10045 is imnpoverished, relative to the soil, in rare eartlhs and Hf. Ratios by mass of Zr to Hf are comlparatively low. Abttndances of Mn, Co, Fe, Sc and Cr stiggest systematic differences between igneous rocks on one hanid and breccias and "soil" on the other. Fromn the Co abuindances, no more than about 3 percent of the present "soil" can consist of chondritic mleteorite conitamination.
authors.forename: G G
authors.initials: GG
authors.lastname: Golescaron
authors.forename: M
authors.initials: M
authors.lastname: Osawa
authors.forename: K
authors.initials: K
authors.lastname: Randle
authors.forename: R L
authors.initials: RL
authors.lastname: Beyer
authors.forename: D Y
authors.initials: DY
authors.lastname: Jerome
authors.forename: D J
authors.initials: DJ
authors.lastname: Lindstrom
authors.forename: M R
authors.initials: MR
authors.lastname: Martin
authors.forename: S M
authors.initials: SM
authors.lastname: McKay
authors.forename: T L
authors.initials: TL
authors.lastname: Steinborn