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Recent Progress in Laboratory Astrophysics Achieved with NASA Ames’ COSmIC Facility

Published online by Cambridge University Press:  04 September 2018

Farid Salama
Affiliation:
NASA-Ames Research Center, Space Science & Astrobiology Division, Moffett Field, California, USA
Ella Sciamma-O’Brien
Affiliation:
NASA-Ames Research Center, Space Science & Astrobiology Division, Moffett Field, California, USA Bay Area Environmental Research Institute, Petaluma, California, USA
Cesar S. Contreras
Affiliation:
NASA-Ames Research Center, Space Science & Astrobiology Division, Moffett Field, California, USA Bay Area Environmental Research Institute, Petaluma, California, USA
Salma Bejaoui
Affiliation:
NASA-Ames Research Center, Space Science & Astrobiology Division, Moffett Field, California, USA
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Abstract

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We describe the characteristics and the capabilities of the laboratory facility, COSmIC, that was developed at NASA Ames to generate, process and analyze interstellar, circumstellar and planetary analogs in the laboratory. COSmIC stands for ’Cosmic Simulation Chamber’ and is dedicated to the study of neutral and ionized molecules and nanoparticles under the low temperature and high vacuum conditions that are required to simulate various space environments such as diffuse interstellar clouds, circumstellar outflows and planetary atmospheres. Recent results obtained using COSmIC will be highlighted. In particular, the progress that has been achieved in the domain of the diffuse interstellar bands (DIBs) and in monitoring, in the laboratory, the formation of circumstellar dust grains and planetary atmosphere aerosols from their gas-phase molecular precursors. Plans for future laboratory experiments on interstellar and planetary molecules and grains will also be addressed, as well as the implications of the studies underway for astronomical observations and past and future space mission data analysis.