METHOD AMODIFIED FROM ANDERS ET AL. (1971)

PROCEEDINGS OF THE FOURTH LUNAR SCIENCE CONFERENCE

ANCIENT METEORITIC COMPONENTS IN LUNAR HIGHLAND ROCKS: CLUES FROM TRACE ELEMENTS IN APOLLO 15 AND 16 SAMPLES

TRACE ELEMENTS IN APOLLO 15 SAMPLES (PPB; NI, CO, ZN, RB, PPM)

APOLLO 15

SPUR CRATER

UNSPECIFIED ROCK MATERIAL, WHOLE ROCK OR GLASS

LUNAR SAMPLES

REGOLITH BRECCIA

COMBUSTION (NEW LINE, YIELDING LOW BLANKS)

THE APOLLO 15 LUNAR SAMPLES

ISOTOPIC COMPOSITION OF CARBON AND HYDROGEN IN SOME APOLLO 14 AND 15 SAMPLES

RESULTS OF HEATING AND COMBUSTION

PROC. LUNAR SCI. CONF. 5TH

THE CHEMICAL DEFINITION AND INTERPRETATION OF ROCK TYPES RETURNED FROM THE NON-MARE REGIONS OF THE MOON

ANORTHOSITIC ROCKS. ALL DATA ARE BY ISOTOPE DILUTION EXCEPT NA, WHICH IS BY ATOMIC ABSORPTION

0,Si, Al, Mg, AND Fe WERE DETERMINED BY USING 14 MeV NEUTRON ACTIVATION ANALYSIS,SEE EHMANN AND MORGAN (1971). THE ELEMENTS Ti, Ca, Mn AND Na ARE DETERMINED BY 252 Cf THERMAL NEUTRON ACTIVATION SEE JANGHORBANI ET AL.,1973). THE Ca ABUNDANCES ARE DETERMINED BY A CYCLIC ACTIVATION TECHNIQUE AND WHILE THE ABUNDANCES OF Ti,Mn AND Na ARE TYPICALLY BASED ON THREE REPLICATE ANALYSES. ABUNDANCES OF TRACE ELEMENTS WERE DETERMINED IN SOME OF THE SAMPLES BY INSTRUMENTAL REACTOR NEUTRON ACTIVATION. FOR A NUMBER OF SAMPLES,Fe WAS DETERMINED BOTH BY 14 MeV AND REACTOR THERMAL NEUTRON ACTIVATION. SPLITS OF STANDARD ROCKS BCR-1 AND W-1 WERE USED AS STANDARDS FOR THE TRACE ELEMENT DETERMINATIONS. SELECTED ABUNDANCES IN THE STANDARD ROCKS WERE TAKEN FROM FLANAGAN (1969) AND FLEISCHER (1969)

PROCEEDINGS OF LUNAR AND PLANETARY SCIENCE CONFERENCE

OXYGEN AND OTHER ELEMENTAL ABUNDANCE DATA FOR APOLLO 14, 15, 16 AND 17 SAMPLES

ELEMENTAL ABUNDANCES IN APOLLO 15 SAMPLES

PROCEEDINGS OF THE LUNAR SCIENCE CONFERENCE

LUNAR ROCK TYPES: THE ROLE OF PLAGIOCLASE IN NON-MARE AND HIGHLAND ROCK TYPES

CHEMICAL DATA FOR KNOWN OR PROPOSED PRIMARY LUNAR ROCK TYPES. ALL DATA ARE FROM ION EXCHENGE PROCEDURE FOLLOWED BY COLORIMETRY (AL2O3), ATOMIC ABSORPTION (FEO, MGO, CAO AND NA2O) AND STABLE ISOTOPE DILUTION MASS SPECTROMETRY (ALL ELSE)

ZIRCONIUM AND HAFNIUM ABUNDANCES IN SOME LUNAR MATERIALS AND IMPLICATIONS OF THEIR RATIOS

ZR AND HF ABUNDANCES IN SOME LUNAR SAMPLES AND TERRESTRIAL STANDARD ROCKS

SIMILAR TO NYQUIST ET AL., 1972, PROCEEDING THIRD LUNAR SCI. CONF., SUPPL. 3

RB-SR SYSTEMATICS FOR CHEMICALLY DEFINED APOLLO 15 MATERIALS

RB AND SR  ANALYTICAL RESULTS FOR APOLLO 15 MATERIALS

PROCEEDINGS OF THE 18TH LUNAR AND PLANETARY SCIENCE CONFERENCE

APENNINE FRONT REVISITED-DIVERSITY OF APOLLO 15 HIGHLAND ROCK TYPES

COMPOSITIONS OF APENNINE FRONT IGNEOUS AND METAMORPHIC ROCKS

Major element analysis of fused beads and INAA. PROCEDURES OF JACOBS, 1977

BULK ANALYSES OF FE NORITES

COMPOSITIONS OF APPENINE FRONT IMPACT MELTS AND GLASSES

LUNAR HIGHLANDS COMPOSITION: APENNINE FRONT

APOLLO 15 (HIGHLAND BRECCIAS). DATA IN PPM EXCEPT WHERE SHOWN IN WT%.

PROCEEDINGS OF THE 19TH LUNAR AND PLANETARY SCIENCE CONFERENCE

APOLLO 15 MG-AND FE-NORITES-A REDEFINITION OF THE MG-SUITE DIFFERENTIATION TREND

Compositions of Apollo 15 norites

LUNAR AND PLANETARY SCIENCE CONFERENCE PROCEEDINGS

AR39-AR40 AGES AND AR37-AR38 EXPOSURE AGES OF LUNAR ROCKS

Ar39-Ar40 ages, exposure ages, and calcium and potassium concentrations of lunar rocks

THE DISTRIBUTION OF K, TI, ZR, U, AND HF IN APOLLO 14 AND 15 MATERIALS

ANALYTICAL RESULTS

METHOD AS IN KOROTEV (1987) WITH AN ADDITIONAL SHORT IRRADIATION AND COUNTING FOR Al2O3, TiO2, AND MgO FOR TWO SPLITS AT THE UNIVERSITY OF MISSOURI REACTOR.

CHEMICAL AND ISOTOPIC CONSTRAINTS ON THE PETROGENESIS OF THE LARGE MARE BASALT CLAST IN BRECCIA 15459

BULK COMPOSITIONS OF APOLLO 15 PICRITIC BASALTS

JSC NBS 6" MASS SPECTROMETER USING THE TRIPLE FILAMENT TECHNIQUE. ALL ANALYSES ON THE FINNIGAN-MAT 261 WERE OBTAINED BY STATIC MULTICOLLECTION.

Astromat

15459

Metadata

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Analysis