Note to users. If you're seeing this message, it means that your browser cannot find this page's style/presentation instructions -- or possibly that you are using a browser that does not support current Web standards. Find out more about why this message is appearing, and what you can do to make your experience of our site the best it can be.


Science 26 November 1965:
Vol. 150. no. 3700, pp. 1156 - 1158
DOI: 10.1126/science.150.3700.1156

Articles

Mars: Compatible Determinations of Surface Pressure through Particle Scattering

J. A. Greenspan 1

1 Astro Sciences Center, IIT Research Institute, Chicago, Illinois 60616

The number of scattering particles required to bring the visual polarimetric and ultraviolet photometric estimates of the surface pressure of Mars into agreement are calculated. Concentrations of 108 to 109 ice particles,0.2 micron in diameter, per square-centimeter column are obtained. Based on concentrations of Aitken nuclei in the atmosphere of Earth, a layer less than 100 meters thick would contain the required number of particles. The compatible pressures obtained in this manner for various N2-CO2 and Ar-CO2 atmospheric models lie within the range of pressures determined spectroscopically.





To Advertise     Find Products


Science. ISSN 0036-8075 (print), 1095-9203 (online)