How Can I Identify Elements in Jupiter's Absorption Spectrum?

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SUMMARY

The discussion focuses on identifying elements in Jupiter's absorption spectrum using spectral analysis. The user has successfully calibrated their spectral analysis program to obtain wavelength per pixel and generate an intensity vs. wavelength graph. They seek a catalog of wavelengths to correlate absorption lines with specific elements or molecules present in Jupiter's atmosphere. A recommended resource for this purpose is the University of Texas library's spectral database.

PREREQUISITES
  • Understanding of spectral analysis techniques
  • Familiarity with wavelength measurement units (angstroms and nanometers)
  • Knowledge of Jupiter's atmospheric composition
  • Experience with data calibration in spectral imaging software
NEXT STEPS
  • Research the University of Texas spectral database for wavelength catalogs
  • Learn about the specific absorption lines of elements in planetary atmospheres
  • Explore software tools for spectral analysis and data visualization
  • Investigate the chemical composition of Jupiter's atmosphere through scientific literature
USEFUL FOR

Astronomers, astrophysicists, and researchers interested in planetary atmospheres and spectral analysis techniques.

Jahne7
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I've recently taken a spectral image (visible wavelengths) of Jupiter. After calibrating my spectral analysis program I've been able to get wavelength per pixel and produce a graph of intensity vs wavelength.
I have an absorption spectra of Jupiter, but I am unaware on how to correlate which absorption lines go to which element, molecule, etc. Is there a general catalog of wavelengths(angstroms or nm) i.e. where I can just view say, the elements or molecules with spectral lines from 460nm to 500nm and then correlate with the known composition of Jupiter;s atmosphere?
 
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Try here http://www.lib.utexas.edu/chem/info/spectra.html
 

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