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

August 02-03, 2019

Global Summit on Applied Physics and Computational Mathematics

Chicago, Illinois, USA
August 02-03, 2019

5th International Conference on Atomic and Nuclear Physics

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August 02-03, 2019

2nd International Meeting on Quantum Mechanics and Applications

Chicago, Illinois, USA
August 19-20, 2019

Asia Pacific Physics Conference

Tokyo, Japan
September 16-17, 2019

Global Meet on Astrophysics & Space Science

Amsterdam, Netherlands
October 14-15, 2019

5th International Conference on Physics

London, UK
October 18-19, 2019

European Meet on Laser, Optics & Photonics

Paris, France
December 16-17, 2019

International Conference on Bio and Medical Physics

Dubai, UAE
March 09-10, 2020

International Conference on Physics

Rome, Italy
MARCH 20-21, 2020

World Congress on Physics

Paris, France
April 20-21, 2020

16th International Conference on Optics, Lasers & Photonics


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