Dating Basalts using the $^{40}$Ar/$^{39}$Ar Method- Improvements Based on Electron Microprobe Evaluation of Samples
AU: * Dunbar, N W
EM: nelia@nmt.edu
AF: New Mexico Bureau of Geology and Mineral Resources, 801 Leroy Place, Socorro,
NM 87801 United States
AU: McIntosh, W C
EM: mcintosh@nmt.edu
AF: New Mexico Bureau of Geology and Mineral Resources, 801 Leroy Place, Socorro,
NM 87801 United States
AU: Love, D
EM: dave@gis.nmt.edu
AF: New Mexico Bureau of Geology and Mineral Resources, 801 Leroy Place, Socorro,
NM 87801 United States
A study of 85 samples of basaltic lava and cinders from the Los Lunas volcano,
central New Mexico, demonstrates that the accuracy and precision of $^{40}$Ar/$^{39}$Ar
dates for young basalts can be maximized by selecting samples that contain K-feldspar
as a late-crystallized phase, and contain little or no glass or alteration phases.
On the basis of optical observations of thin sections, it has long been recognized
that abundant groundmass glass is detrimental to K-Ar and $^{40}$Ar/$^{39}$Ar
dating of basalts. The electron microprobe offers a means of assessing and quantitatively
analyzing basaltic groundmass features that are too small to be assessed optically.
X-ray mapping and quantitative analyses accurately distinguish among crystal
and glass phases as small as 2 $\mu$m. The crystallinity of smaller areas can
be qualitatively assessed by multiple analyses, where homogeneous compositions
indicate glass and heterogeneous composition indicates multiple crystal phases.
Samples from Los Lunas volcano were examined by electron microprobe, with the
first step in the evaluation process being collection of potassium x-ray maps
of polished surfaces. Once the locations of K-bearing phases were determined,
the compositions of the phases were measured using quantitative analysis. Some
otherwise well-crystallized samples were found to contain small amounts of groundmass
glass in interstices between crystals; in these cases, virtually all K was concentrated
within the glass. In other samples the groundmass was fully crystallized. In
these cases K resided in K-feldspar, either as thin ($<$10 $\mu$m) rims on
plagioclase or as fine ($<$15 $\mu$m) groundmass crystals intergrown with
albite. This K-feldspar would be impossible to identify optically due to the
small grain size and intergrown nature of the crystals. Samples were rated on
the basis of glass content versus K-feldspar content. After excluding samples
containing abundant ($>$10\%) glass, 19 samples were dated by the $^{40}$Ar/$^{39}$Ar
resistance furnace incremental heating method. The shape of spectra and the
accuracy and precision of plateau and isochron ages correspond closely to the
ranking assigned based on the microprobe evaluation. Glass-free, K-feldspar-rich
samples have generally flat spectra, relatively high radiogenic yields (\%$^{40}$Ar*),
and ages with precision values ($\pm$2 $\sigma$) ranging from 1-5\%. These ages
agree well with stratigraphic order. Samples with increasing amounts of groundmass
glass have increasingly disturbed spectra, reduced radiogenic yields, and low
precision ($\pm$5-20\%) plateau or isochron ages, which in some cases violate
stratigraphic order. The consequences of even small amounts of groundmass glass
are attributed to various combinations of atmospheric argon acquired during
hydration, $^{40}$Ar or K$_{2}$0 loss, and $^{39}$Ar recoil artifacts . $^{40}$Ar/$^{39}$Ar
results from higher ranking samples indicate that Los Lunas volcano consists
of a 3.81 $\pm$ 0.10 Ma southern cone overlapped by a 1.25 $\pm$ 0.02 Ma northern
cone; this relationship agrees with geologic map patterns. Within the northern
cone, geologic mapping has delineated a sequence of five eruptive events. The
ages of high ranking samples from the northern cone all agree within analytical
error, suggesting that the entire period of eruptive activity spanned less than
30,000 years. The precision and accuracy of data in this study was much enhanced
by using microprobe observations of groundmass glass and K-feldspar to aid in
the sample selection process. Sample selection based on only thin section observations
would have yielded lower quality data.
DE: 1035 Geochronology
DE: 8494 Instruments and techniques
DE: 9350 North America
DE: 9604 Cenozoic
SC: V
MN: 2001 AGU Fall Meeting