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We use newly developed spectroscopic methods for determining FeO and TiO 2 abundances to study the huge (2500 km diameter) South Pole‐Aitken basin. The floor of this basin shows iron and titanium values which are weakly correlated and largely range from 7 to 14 wt % FeO and from 0.5 to 1.5 wt % TiO 2 . This composition is consistent with an approximate 1:1 mixture of lower crustal material like that found elsewhere on the Moon and mantle rock containing 10–16 wt % FeO and <0.1 wt % TiO 2 . Although mantle rock appears to compose about 50% of the floor deposits, models of the formation of large impact basins predict that virtually all the floor materials ought to be derived from the mantle.
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Lucey et al. (1998) studied this question.
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