Terahertz/Far Infrared beamlines assisted investigation into possible composition of lower atmosphere of Saturn’s moon Titan.
Although firmly located on earth, the Australian Synchrotron’s Terahertz/Far Infrared beamline (THz/Far IR) is one of three synchrotron facilities in the word able to simulate the extreme conditions of distant planetary worlds.
The most recently reported research using the beamline published in Earth and Space Chemistry, involved recreating the pressure and temperatures environments in the hazy atmosphere surrounding Saturn’s moon Titan.
“We are interested in Titan because it is the most Earth-like of the planetary bodies possessing an atmosphere of mostly nitrogen and methane,” said co-author Rebecca Auchettl (pictured above), a PhD candidate who was supervised by Dr Courtney Ennis, formerly of La Trobe University now at the University of Otago in New Zealand.
Image: Co-author Rebecca Auchettl, PhD candidate.