The rates of many processes that control rock breakdown into transportable
particles are dependent upon rock temperature. In particular, frost-crackin
g depends largely upon the time spent within a range of subzero temperature
s I call the frost cracking window. I present simple analytic solutions, de
tailed time series of thermal data from a field site, and a numerical model
of subsurface temperatures that constrain the expected depth dependence of
frost cracking. Analytic solutions using sinusoidal surface temperature hi
stories result in predicted vertical profiles of frost-cracking intensity t
hat depend upon the location of the frost-cracking window within the range
of surface temperatures. In some cases, the expected frost cracking intensi
ty decreases monotonically with depth, while in others it displays a distin
ct maximum at depth. I use hourly temperatures measured over the I-yr inter
val April 1995 through March 1996, at 8 depths up to 42 cm into a granitic
bedrock surface in the Laramie Range, Wyoming, to constrain an in situ ther
mal diffusivity of 1.7 mm(2) s(-1). These temperature histories suggest tha
t frost cracking at this site should decrease monotonically with depth into
the rock. I also use this time series of temperatures to calibrate a numer
ical thermal model in which the top boundary condition is set by a surface
radiation balance. The data require both a low albedo of the rock surface (
0.1), and a high atmospheric transmissivity (0.9). I then explore the expec
ted near-surface temperatures at other sites by running the model with diff
erent annual mean temperatures, latitudes, and slopes. The resulting simula
tions suggest that at lower mean annual temperatures, as are found in highe
r latitude and altitude sites, the frost cracking maximum should both ampli
fy and deepen into the subsurface.