an up-to-date (and subject to frequent change) 

in approximate order of decreasing alumina (Al₂O₃) concentration
(also see alternate list in alphanumeric order)

The list contains only those meteorites that have been announced in The Meteoritical Bulletin, described elsewhere in the scientific literature, or that I've studied myself and believe to be of lunar origin.

For the geochemically inclined: Click here (or on FeO concentration below) to see where the meteorite plots in compositional space. Plot symbols are in column 2.
  

Meteorites listed in the same box with a slash (/ ), e.g., MacAlpine Hills 88104 and MacAlpine Hills 88105 are paired, i.e., they are two or more fragments of a single object that made the Moon-Earth trip.  Other unidentified pairings may exist. 

*  It is not always possible to identify the type of breccia from a small thin section and different petrologists don't always agree on the classification. Some of these classifications might be in error.

** Total iron as FeO.

Thanks to Erich H. Haiderer, Norbert Classen, and Tony Irving for providing samples, images, and opinions that help sort out possible pairing relationships among the many Dhofar and Northwest Africa lunar meteorites

Maps: U.S. Antarctic (ANSMET) | Japanese Antarctic (NIPR)| Dhofar, Oman

NASA Lunar Meteorite Compendium