Physics
Scientific paper
Apr 2012
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012georl..3907201k&link_type=abstract
Geophysical Research Letters, Volume 39, Issue 7, CiteID L07201
Physics
Mineralogy And Petrology: Planetary Mineralogy And Petrology (5410), Physical Properties Of Rocks: Permeability And Porosity, Planetary Sciences: Solid Surface Planets: Gravitational Fields (1221), Planetary Sciences: Solid Surface Planets: Surface Materials And Properties, Planetary Sciences: Solar System Objects: Moon (1221)
Scientific paper
Accurate lunar rock densities are necessary for constructing gravity models of the Moon's crust and lithosphere. Most Apollo-era density measurements have errors of 2–5% or more and few include porosity measurements. We report new density and porosity measurements using the bead method and helium pycnometry for 6 Apollo samples and 7 lunar meteorites, with typical grain density uncertainties of 10–30 kg m‑3 (0.3–0.9%) and porosity uncertainties of 1–3%. Comparison between igneous grain densities and normative mineral densities show that these uncertainties are realistic and that the helium fully penetrates the pore space. Basalt grain densities are a strong function of composition, varying over at least 3270 kg m‑3 (high aluminum basalt) to 3460 kg m‑3 (high titanium basalt). Feldspathic highland crust has a bulk density of 2200–2600 kg m‑3 and porosity of 10–20%. Impact basin ejecta has a bulk density of 2350–2600 kg m‑3 and porosity of ∼20%.
Britt Daniel T.
Consolmagno Guy J.
Irving Anthony J.
Kiefer Walter Scott
Macke Robert J.
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