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

March 09-10, 2020

International Conference on Physics

Rome, Italy
March 09-10, 2020

International Conference on Physics

Rome, Italy
MARCH 20-21, 2020

World Congress on Physics

Paris, France
September 22-23, 2020

International Conference on Optometry

Dubai, UAE
September 22-23, 2020

International Conference on Nucleic Acids

Dubai, UAE
October 19-20, 2020

18th International Expo on Optics,Lasers and Photonics

Paris, France
November 02-03, 2020

GlobaL Meet on Optoelectronics and Quantum Physics

Sydney, Australia
November 12-13, 2020

European Meet on Laser, Optics & Photonics

Budapest, Hungary

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