Thermogravimetric thermal analyzer PERSEUS® STA 509 Jupiter®

Evolved Gas Analysis (EGA) is the perfect tool for characterizing the thermal behavior of organics, inorganics or polymers in more detail, elucidating the chemistry behind the processes. The PERSEUS® STA 509 Jupiter® is an unmatched alliance between two successful instruments: the NETZSCH STA 509 Jupiter® and the FT-IR spectrometer by Bruker Optics. Its design is unprecedented and sets a benchmark for state-of-the-art coupling systems. Due to its robustness, high performance, compactness and attractive price, this combination instrument has the potential to find its way into any laboratory – be it in universities or industry, across the spectrum from inorganics to polymers. Affordable Gas Analysis The unrivaled instrument alliance serves as an innovative coupling technique, even for a narrow budget. It has what it takes to become an integral part of any laboratory and indispensible for its future needs. No Liquid Nitrogen required The DLaTGS (DLaTGS = deuterated L-alanine doped triglycine sulphate) detector used does not require any liquid nitrogen cooling. This system is therefore particularly well-suited for test runs with an autosampler (ASC) or for measurements of longer duration. No Separate Transfer Line The built-in heated gas cell is directly connected to the gas outlet of the furnace via a heated tube. The low volume of this short gas path guarantees fast response and is quite advantageous in cases where condensable evolved gases are present. Space-Saving Design No separate FT-IR spectrometer is necessary, the footprint of the PERSEUS® STA 509 Jupiter® coupling is identical to that of an STA 509 Jupiter® alone.