VUV and EUV irradiation of CH4+NH3 ice mixtures
碩士 === 國立中央大學 === 物理學系 === 106 === We never stop the exploration of the outer space. Since 1900s, as- tronomers have observed all over the sky to seek origin of life. Apart from observing stars, we may simulate the outer space environments and make some simple molecules in laboratories on the earth...
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| Format: | Others |
| Language: | en_US |
| Published: |
2018
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| Online Access: | http://ndltd.ncl.edu.tw/handle/5673dd |
| Summary: | 碩士 === 國立中央大學 === 物理學系 === 106 === We never stop the exploration of the outer space. Since 1900s, as- tronomers have observed all over the sky to seek origin of life. Apart from observing stars, we may simulate the outer space environments and make some simple molecules in laboratories on the earth now. To investigate the formation of CN−, we deposite CH4 and NH3 (mechanism proposed by Kim and Kaiser (2011)[1]) to simulate the surface of Charon. We provide VUV and EUV irradiations as energy sources and mainly use Fourier Transform Infrared Spectrometer (FTIR) and Quadrupole Mass Spectrometer (QMS) to study different concentrations of CH4 to NH3 ice mixtures.
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