Meteoritics and Planetary Science Supplement

Multiple Breakup of ALH 85085-like and CR Group Chondrites

MetBase 2457 Compilation

Antarctica

METEORITES

ANGRITE

Cameca SX100, 20 kV, 40 nA, 1 μm beam for pyroxene, chromite and ilmenite, and 15 kV, 20 nA, 1 μm beam for plagioclase

Meteoritics and Planetary Science

Ibitira: A basaltic achondrite from a distinct parent asteroid and implications for the Dawn mission

Average Na, Ca, Ti, and Hf data and Na/Ca and Ti/Hf ratios for the asteroidal basalts shown in Fig. 3.

GEOCHIMICA ET COSMOCHIMICA ACTA

GEOCHEMISTRY AND GENESIS OF THE ANGRITES

Major and trace clement compositions of angrites and BHVO-1 determined by  fused-bead electron microprobe (FB) and lNAA

PETROGENESIS OF ANGRITES

Representative elemental concentrations in plagioclase and glass

Representative elemental concentrations in clinopyroxene

Representative elemental concentrations in olivine (including kirschsteinite)

REE concentrations in phosphate

JEOL 733 electron probe (Ocean ResearchInstitute,University of Tokyo), a JEOL JCM 733 mkIImicroprobe (Geological Institute,University of Tokyo) and a Cameca SX-100 automated electron microprobe (NASA/Johnson Space Center); 15 kV; beam current was 12 or 30 nA

Antarctic Meteorite Research

Mineralogical study of angrite Asuka-881371: Its possible relation to angrite LEW87051

Chemical compositions of LEW87051 olivines

Astromat

LEW 87051

Metadata

More Resources About Sample LEW 87051

Analysis