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

May 02-03, 2019

3rd International Conference on Astronomy and Space Science

Park Inn by Radisson Hotel Heathrow, London, UK
May 13-14, 2019

6th World Congress on Physics

Paris, France
May 16-17, 2019

6th International Conference on Theoretical and Applied Physics

Hotel Holiday Inn, Aurelia Rome, Italy
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

Chicago, Illinois, USA
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 14-16, 2019

5th International Conference on Physics

London, UK
October 18-19, 2019

World Congress on Physics

Paris, France
October 18-19, 2019 |

European Meet on Laser, Optics & Photonics

Paris, France
October 28-29, 2019

International Conference on Physics

Rome, Italy
December 16-17, 2019

International Conference on Bio and Medical Physics

Dubai, UAE

Astronomical Spectroscopy Conference Speakers

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