Path: utzoo!censor!geac!torsqnt!news-server.csri.toronto.edu!cs.utexas.edu!swrinde!ucsd!ucbvax!pasteur!miro.Berkeley.EDU!ph From: ph@miro.Berkeley.EDU (Paul Heckbert) Newsgroups: comp.graphics Subject: Re: Lambert's Law & the Moon Message-ID: <9237@pasteur.Berkeley.EDU> Date: 27 Nov 90 05:54:50 GMT References: <27331@cs.yale.edu> Sender: news@pasteur.Berkeley.EDU Reply-To: ph@miro.Berkeley.EDU (Paul Heckbert) Organization: University of California at Berkeley Lines: 18 musgrave-forest@CS.YALE.EDU (F. Ken Musgrave) writes: > Am I correct in a vague memory I seem to have, that the (Earth's) moon is >supposedly a near-ideal Lambertian reflector? As others have mentioned, the moon and other dusty surfaces are not Lambertian. Blinn, in the paper cited below, says they follow the Hapke-Irvine illumination model more closely. %A James F. Blinn %T Light Reflection Functions for Simulation of Clouds and Dusty Surfaces %J Computer Graphics (SIGGRAPH '82 Proceedings) %V 16 %N 3 %D July 1982 %P 21-29 %K shading %Z Hapke-Irvine illumination model