Ned Nikolov has kindly sent me the freshly published paper by Vavasada et al which adds a lot more detail to the plot of Lunar equatorial temperature he passed our way recently. This is technical, but worth getting your head around, because it reveals and elucidates matters highly relevant to ideas and misconceptions regarding theoretical grey body temperature, both for the Moon and Earth. Get it while it’s hot.
JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 117, E00H18, doi:10.1029/2011JE003987, 2012
Lunar equatorial surface temperatures and regolith properties
from the Diviner Lunar Radiometer Experiment
Ashwin R. Vasavada,1 Joshua L. Bandfield,2 Benjamin T. Greenhagen,1 Paul O. Hayne,3
Matthew A. Siegler,4 Jean-Pierre Williams,4 and David A. Paige4
Received 30 September 2011; revised 20 February 2012; accepted 20 February 2012; published 4 April 2012.
[1] The Diviner Lunar Radiometer Experiment onboard the Lunar Reconnaissance Orbiter
has measured solar reflectance and mid-infrared radiance globally, over four diurnal cycles,
at unprecedented spatial and temporal resolution. These data are used to infer the radiative
and bulk thermophysical properties of the near-surface regolith layer at all longitudes
around the equator. Normal albedos are estimated from solar reflectance measurements.
Normal spectral emissivities relative to the 8-mm Christiansen Feature are computed from
brightness temperatures and used along with albedos as inputs to a numerical thermal
model. Model fits to daytime temperatures require that the albedo increase with solar
incidence angle. Measured nighttime cooling is remarkably similar across longitude and
major geologic units, consistent with the scarcity of rock exposures and with the
widespread presence of a near-surface layer whose physical structure and thermal response
are determined by pulverization through micrometeoroid impacts. Nighttime temperatures
are best fit using a graded regolith model, with a ~40% increase in bulk density and an
eightfold increase in thermal conductivity (adjusted for temperature) occurring within
several centimeters of the surface.
Citation: Vasavada, A. R., J. L. Bandfield, B. T. Greenhagen, P. O. Hayne, M. A. Siegler, J.-P. Williams, and D. A. Paige
(2012), Lunar equatorial surface temperatures and regolith properties from the Diviner Lunar Radiometer Experiment,
J. Geophys. Res., 117, E00H18, doi:10.1029/2011JE003987.
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