Meteoritics & Planetary Science 40, Nr 3, 431–443 (2005) Abstract available online at http://meteoritics.org Primordial noble gases in a graphite-metal inclusion from the Canyon Diablo IAB iron meteorite and their implications Jun-ichi MATSUDA,1* Miwa NAMBA,1 Teruyuki MARUOKA,1† Takuya MATSUMOTO,1 and Gero KURAT2 1Department of Earth and Space Science, Graduate School of Science, Osaka University, Toyonaka, Osaka 560–0043, Japan 2Institut f¸r Geologische Wissenschaften, Universit‰t Wien, Althanstrasse 14, A-1090 Vienna, Austria †Present address: Graduate School of Life and Environmental Sciences, University of Tsukuba, Tsukuba, Ibaraki 305–8572, Japan *Corresponding author. E-mail:
[email protected] (Received 01 July 2004; revision accepted 29 December 2004) Abstract–We have carried out noble gas measurements on graphite from a large graphite-metal inclusion in Canyon Diablo. The Ne data of the low-temperature fractions lie on the mixing line between air and the spallogenic component, but those of high temperatures seem to lie on the mixing line between Ne-HL and the spallogenic component. The Ar isotope data indicate the presence of Q in addition to air, spallogenic component and Ar-HL. As the elemental concentration of Ne in Q is low, we could not detect the Ne-Q from the Ne data. On the other hand, we could not observe Xe-HL in our Xe data. As the Xe concentration and the Xe/Ne ratio in Q is much higher than that in the HL component, it is likely that only the contribution of Q is observed in the Xe data.