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• PERSEUS® STA 509 Jupiter® Technical Datasheet

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 FTIR 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.

Any existing NETZSCH STA 509 Jupiter^®-system can be upgraded to the PERSEUS^®.

The PERSEUS^® STA 509 Jupiter^® can be employed for the following application areas:

• Decomposition
• Solid-gas reactions
• Compositional analysis
• Evaporation, outgassing

Advantages of the PERSEUS^® STA 509 Jupiter^®:

• DLaTGS detector does not require any liquid nitrogen cooling
• No separate transfer line required
• Space-saving design
• Maximum temperature range from room temperature to 2000 °C
• Maximum temperature of the transfer line: 200 °C
• Internal gas cell with KBr window (length: 70 mm; volume: 5.8 ml)
• Spectral range of FTIR data: 350 to 8000 cm^-1
• Automatic sample change is available as an option
• Additional coupling option to GC-MS or MS
• Proteus^® software (including device license)

For further information, please refer to the technical data sheet.