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By Radu D. Rugescu

ISBN-10: 9533070528

ISBN-13: 9789533070520

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Mars is damned cold. At night, in the winter, temperatures on Mars get down to about -160 degrees! ) But there’s an easy fix for this: add greenhouse gases. This has the effect of letting sunlight in, but preventing the heat from escaping. In order to keep Mars at about the same temperature as Earth, all we’d have to do is add enough Carbon Dioxide, Methane, and Water Vapor to Mars’ atmosphere. Want to know something neat? If we’re going to move 20% of our atmosphere over there, we may want to move 50% of our greenhouse gases with it, solving some of our environmental problems in the process.

In addition, the proposed technological principles can be used for producing photovoltaic devices based on thin films of cadmium telluride. 7. Acknowledgements This research was supported in part by the Ministry for Education and Science (Ukraine) through the financing provided for the scientific projects carried out at the Department of Optoelectronics, Department of Energy Engineering and Electronics, as well as at the Science and Education Center “Semiconductor Material Science and Energy-Efficient Technology” at the Chernivtsi National University, Research Project #SU/447-2009 for the years 2009-2010.

Tulita, S. Raghunathan, E. Benard, Control of Steady Transonic Periodic Flow on NACA-0012 Aerofoil by Contour Bumps, Department of Aeronautical Engineering, The Queen’s University of Belfast, Belfast, Northern Ireland, United Kingdom, 2002; Synge, J. , and Griffith, B. , New York, Toronto, London. , and Redfield, S. (2005) New mass-loss measurements from astrospheric Ly-α absorption, Astrophys. , 628:L143–L146. S. (1993), Oxygen ionization rates at Mars and Venus: relative contributions of impact ionization and charge exchange.

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Solar Energy by Radu D. Rugescu

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