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Scientific American|February 1, 1988
How climate evolved on the terrestrial planetsJ F Kasting, O B Toon, J B PollackIcarus|February 1, 1997
Radiative heating of interstellar grains falling toward the solar nebula: 1-D diffusion calculationsD P Simonelli, J B Pollack, C P McKayIcarus|January 1, 1984
Water loss on Venus: the role of carbon monoxideS M Richardson, J B Pollack, R T ReynoldsIcarus|January 1, 1987
The case for a wet, warm climate on early MarsJ B Pollack, J F Kasting, S M Richardson, et al.Science (New York, N.Y.)|July 6, 1979
Laboratory corroboration of the pioneer venus gas chromatograph analysesV I Oyama, G C Carle, F Woeller, et al.Science (New York, N.Y.)|February 23, 1979
Venus lower atmospheric composition: analysis by gas chromatographyV I Oyama, G C Carle, F Woeller, et al.Science (New York, N.Y.)|September 13, 1991
The dark side of Venus: near-infrared images and spectra from the Anglo-Australian observatoryD Crisp, D A Allen, D H Grinspoon, et al.Icarus|March 1, 1993
Coupled atmosphere-ocean models of Titan's pastC P McKay, J B Pollack, J I Lunine, et al.American Journal of Science|May 1, 1986
A hybrid model of the CO2 geochemical cycle and its application to large impact eventsJ F Kasting, S M Richardson, J B Pollack, et al.Science (New York, N.Y.)|March 1, 1974
Wind tunnel simulations of light and dark streaks on MarsR Greeley, J D Iversen, J B Pollack, et al.Pageof 6