Cooling rates of lunar orange glass beads

1Hejiu Hui(惠鹤九), 2Kai-Uwe Hess, 3Youxue Zhang(张有学), 4Alexander R.L.Nichols, 5Anne H.Peslier, 3Rebecca A.Lange, 2Donald B.Dingwell, 6Clive R.Neal
Earth and Planetary Science Letters 503, 88-94 Link to Article []
1State Key Laboratory for Mineral Deposits Research & Lunar and Planetary Science Institute, School of Earth Sciences and Engineering, Nanjing University, Nanjing, Jiangsu 210023, China
2Department of Earth and Environmental Sciences, LMU-University of Munich, Theresienstrasse 41/III, 80333 Munich, Germany
3Department of Earth and Environmental Sciences, University of Michigan, Ann Arbor, MI 48109, USA
4Department of Geological Sciences, University of Canterbury, Christchurch 8140, New Zealand
5Jacobs, NASA-Johnson Space Center, Mail Code X13, Houston, TX 77058, USA
6Department of Civil and Environmental Engineering and Earth Sciences, University of Notre Dame, Notre Dame, IN 46556, USA
Copyright Elsevier

It is widely accepted that the Apollo 17 orange glass beads are of volcanic origin. The degree of degassing of the glass beads depends on their cooling rates, so the estimation of volatile contents in the parental magmas of these lunar pyroclastic glasses also depends on the cooling rates. The cooling rate can be estimated using the calorimetric properties of the glass across the glass transition. In this study, a series of heat capacity measurements were carried out on hand-picked lunar volcanic orange glass beads during several cycles of heating to temperatures above their glass transition using a differential scanning calorimeter. The cooling rate of orange glass beads (sample 74220,867) was calculated to be 101 K/min using the correlation between glass cooling rates and fictive temperatures estimated from their heat capacity–temperature paths. This cooling rate is close to the lower end of the range that best fits the diffusion profiles of several volatile species in the glass beads, and at the upper end of the cooling-rate range recorded in glasses quenched subaerially on Earth. The cooling rate is likely to be controlled by the cooling environment (cooling medium) such that the lunar volcanic glass beads could have been cooled in a gaseous medium released from volcanic eruptions on the Moon, but not during “free flight” in vacuum. The existence of a gas medium suggests, in turn, that there may have been at least a short-lived or episodic atmosphere on the early Moon at around 3.5 Ga.


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