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Behavior of Long-Chain Hydrocarbons at High Pressures and Temperatures
Abhisek Basu1, Mainak Mookherjee1, Ericka McMahan1
1Earth Materials Laboratory, Department of Earth, Ocean and Atmospheric Science, Florida State University, Tallahassee, Florida 32306, United States.
The origin of long-chain hydrocarbons in meteorites remains unclear. This study reveals how high pressures and temperatures alter their molecular structure, suggesting potential extraterrestrial origins.
Area of Science:
- Geochemistry
- Astrochemistry
- Materials Science
Background:
- Long-chain aliphatic hydrocarbons are found in meteorites, but their origin (pristine extraterrestrial or terrestrial alteration) is debated.
- Understanding their stability under extreme conditions is crucial for determining their indigenous nature.
Purpose of the Study:
- To investigate the behavior of aliphatic hydrocarbons under simultaneous high pressure and temperature.
- To explore the effects of thermal changes on molecular structure, bridging a gap in current research.
Main Methods:
- Utilized a resistively heated diamond anvil cell to subject aliphatic hydrocarbons to simultaneous high pressure and temperature.
- Employed Raman spectroscopy to monitor structural changes via vibrational modes.
Main Results:
- Observed new low-energy vibrational modes upon compression, consistent with chain bending.
- Documented softening of these modes upon heating to ~220 °C, indicating molecular unbending and anharmonicity.
Conclusions:
- High pressure and temperature significantly alter the molecular structure of long-chain aliphatic hydrocarbons.
- These findings provide insights into the potential for indigenous extraterrestrial organic molecules in meteorites.
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