4.1 Article

Lunar meteorites from northern Africa

Journal

METEORITICS & PLANETARY SCIENCE
Volume 56, Issue 2, Pages 206-240

Publisher

WILEY
DOI: 10.1111/maps.13617

Keywords

-

Funding

  1. NASA [NNX14AI65G]
  2. McDonnell Center for the Space Sciences
  3. NASA [681688, NNX14AI65G] Funding Source: Federal RePORTER

Ask authors/readers for more resources

The study found that approximately 27% of African meteorites are typical feldspathic lunar rocks with similar bulk compositions. These meteorites have a wide range of whole-rock mole% Mg/[Mg + Fe] and do not correlate with albite content of plagioclase or concentrations of incompatible elements. Some of these meteorites are believed to originate from different regions of the lunar highlands.
We report bulk composition data for 235 stones of similar to 77 lunar meteorites from northern Africa and 33 lunar meteorites from elsewhere. About 27% of the African meteorites are typical feldspathic lunar rocks, all breccias of similar bulk composition, for example, 3-5% FeO and low concentrations of incompatible elements. Nevertheless, these meteorites have a large range in Mg' (whole-rock mole% Mg/[Mg + Fe]), 57-77 (mean: 65.5), and this parameter does not correlate with either albite content of the plagioclase or concentrations of incompatible elements. From this observation, we conclude that feldspathic lunar meteorites do not support the hypotheses that the anorthositic, precursor plutonic rocks of the meteorite breccias all crystallized from a common magma. Among feldspathic lunar meteorites, Mg' increases with normative olivine abundance but is uncorrelated with normative pyroxene abundance, that is, high-Mg' feldspathic rocks of the early lunar crust were troctolitic, not noritic. The NWA 5744 (Northwest Arica) clan of lunar meteorites are anorthositic troctolites (59-75% plagioclase, 15-26% olivine, Fo(77-80)) with very low concentrations of incompatible elements (2.6 x CI) compared to troctolites in the Apollo collection. They may represent the lower feldspathic crust or differentiated impact melt from portions of the highlands distant from the PKT (Procellarum KREEP Terrane). About 31% of the lunar meteorites from northern Africa, all breccias, are, by lunar standards, moderately mafic (5-13% FeO) but more magnesian than mixtures of typical feldspathic meteorite and mare basalt, implying that they represent moderately mafic regions of the highlands or originate from the South Pole-Aitken basin. With similar to 6 mu g g(-1) Th, two NWA meteorites likely originate from the PKT. Including the unique NWA 773 clan, at least six of the northern Africa meteorites are, or are dominated by, unbrecciated basalts and gabbros of mare affinity. We estimate that the similar to 341 lunar meteorite stones (Africa and elsewhere) for which there are data represent 131-147 terrestrially unpaired meteorites and 109-134 lunar launch sites.

Authors

I am an author on this paper
Click your name to claim this paper and add it to your profile.

Reviews

Primary Rating

4.1
Not enough ratings

Secondary Ratings

Novelty
-
Significance
-
Scientific rigor
-
Rate this paper

Recommended

No Data Available
No Data Available