Astronomical Spectroscopy

Astronomical spectroscopy is the study which is used to measure three major bands of radiation: visible spectrum, radio, and X-ray. Though all spectroscopy looks at specific areas of the spectrum, different approaches are required to acquire the signal depending upon the frequency. Ozone (O3) and the molecular oxygen (O2) absorb light with wavelengths only under 300 nm, that means meaning the X-ray and ultraviolet spectroscopy requires the use of a satellite telescope or rocket mounted detectors. Radio signals have much longer wavelengths than of the optical signals and it requires the use of antennas or radio dishes.

  • Emission spectrum
  • Photometry
  • Prism
  • Quasars
  • 3D Image
  • Helium Spectra
  • Astrometry
  • Celestial Mechanics
  • Telescopes

Related Conference of Astronomical Spectroscopy

October 06-07, 2025

6th International Conference on Physics

Paris, France
December 01-02, 2025

9th International Meeting on Fluid Dynamics & Fluid Mechanics

Vancouver, Canada
December 15-16, 2025

13th World Congress on Physical and Theoretical Chemistry

Amsterdam, Netherlands
February 09-10, 2026

9th World Congress On Cardiology and Heart Failure

London, UK
April 29-30, 2026

4th World Congress on Quantum Physics

Dubai, UAE

Astronomical Spectroscopy Conference Speakers

    Recommended Sessions

    Related Journals

    Are you interested in