			15min:

A SEARCH FOR THE 8.5 µm VIBRATIONAL SPECTRUM OF C₆₀ IN THE LABORATORY AND SPACE.

SUSANNA L. WIDICUS WEAVER, Departments of Chemistry and Astronomy, University of Illinois at Urbana-Champaign, Urbana, IL 61801; BRIAN E. BRUMFIELD AND ANDREW A. MILLS, Department of Chemistry, University of Illinois at Urbana-Champaign, Urbana, IL 61801; SCOTT HOWARD AND CLAIRE GMACHL, Department of Electrical Engineering, and the Princeton Institute for the Science and Technology of Materials, Princeton University, Princeton, New Jersey 08544; BENJAMIN J. MCCALL, Departments of Chemistry and Astronomy, University of Illinois at Urbana-Champaign, Urbana, IL 61801.

\hspace0.25in Buckminsterfullerene (C₆₀) was discovered during experiments designed to simulate the conditions of carbon star outflows. C₆₀ is stable against photodissociation, is expected to be present in the interstellar medium, and has been detected in craters on NASA's Long Duration Exposure Facility and in sediments related to meteorite impacts. C₆₀ has four infrared active modes that should be observationally detectable, and we have conducted searches for the 8.5 µm mode toward three molecular cloud sources and the variable star R Coronae Borealis with the Texas Echelon Cross Echelle Spectrograph (TEXES) instrument at NASA's Infrared Telescope Facility (IRTF).

\hspace0.25in In the laboratory, gas phase emission spectra of C₆₀ have been obtained at high temperatures, and infrared absorption studies in a parahydrogen matrix have also been conducted. Yet a cold, rotationally resolved gas phase spectrum is required for direct comparison to observational spectra. To this end we are utilizing continuous-wave cavity ringdown spectroscopy (cw-CRDS) to investigate the rovibrational spectrum of C₆₀ using an 8.5 µm continuous-wave quantum cascade laser (cw-QCL). Solid C₆₀ is heated to > 600 ^\circC and the resultant vapor is supersonically expanded with argon through a 0.030'' pinhole. Using this supersonic expansion source, we have observed a rotational temperature of < 30 K (with N₂⁺ in the near IR), and a residual Doppler linewidth of 60 MHz (with this QCL, using CH₂Br₂). The results of the cw-CRDS laboratory study and observational work on C₆₀ will be presented.