Experimental Study of Ethylene Evaporites under Titan Conditions

Titan has an abundance of lakes and seas, as confirmed by Cassini. Major components of these liquid bodies include methane (\(CH_4\)) and ethane (\(C_2H_6\)); however, evidence indicates that minor components such as ethylene (\(C_2H_4\)) may also exist in the lakes. As the lake levels drop, 5 \(\mu...

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Veröffentlicht in:	arXiv.org 2020-02
Hauptverfasser:	Czaplinski, E C, Gilbertson, Woodrow A, Farnsworth, Kendra K, Chevrier, Vincent F
Format:	Artikel
Sprache:	eng
Schlagworte:	Absorption spectra Cassini mission Ethane Ethylene Evaporation Evaporation rate Fourier transforms Infrared analysis Methane Physics - Earth and Planetary Astrophysics Physics - Instrumentation and Methods for Astrophysics Solvents Titan
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