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  2. Doppler spectroscopy - Wikipedia

    en.wikipedia.org/wiki/Doppler_spectroscopy

    Doppler spectroscopy (also known as the radial-velocity method, or colloquially, the wobble method) is an indirect method for finding extrasolar planets and brown dwarfs from radial-velocity measurements via observation of Doppler shifts in the spectrum of the planet's parent star. As of November 2022, about 19.5% of known extrasolar planets ...

  3. Minimum mass - Wikipedia

    en.wikipedia.org/wiki/Minimum_mass

    In astronomy, minimum mass is the lower-bound calculated mass of observed objects such as planets, stars, binary systems, [1] nebulae, [2] and black holes.. Minimum mass is a widely cited statistic for extrasolar planets detected by the radial velocity method or Doppler spectroscopy, and is determined using the binary mass function.

  4. Doppler parameter - Wikipedia

    en.wikipedia.org/wiki/Doppler_parameter

    The Doppler parameters of Lyman-alpha forest absorption lines are in the range 10–100 km s −1, with a median value around = that decrease with redshift (Kim et al. 1997). Analyses of the HST / COS dataset of low-redshift quasars gives a median b {\displaystyle b} parameter of around 33 k m s − 1 {\displaystyle 33\ \mathrm {km\ s} ^{-1 ...

  5. Methods of detecting exoplanets - Wikipedia

    en.wikipedia.org/wiki/Methods_of_detecting_exo...

    A separate novel method to detect exoplanets from light variations uses relativistic beaming of the observed flux from the star due to its motion. It is also known as Doppler beaming or Doppler boosting. The method was first proposed by Abraham Loeb and Scott Gaudi in 2003. [35]

  6. Binary mass function - Wikipedia

    en.wikipedia.org/wiki/Binary_mass_function

    This is the radial velocity method of detecting exoplanets. [ 5 ] [ 3 ] Using the mass function and the radial velocity of the host star, the minimum mass of an exoplanet can be determined. [ 15 ] [ 16 ] : 9 [ 12 ] [ 17 ] Applying this method on Proxima Centauri , the closest star to the solar system, led to the discovery of Proxima Centauri b ...

  7. Doppler broadening - Wikipedia

    en.wikipedia.org/wiki/Doppler_broadening

    A particular case is the thermal Doppler broadening due to the thermal motion of the particles. Then, the broadening depends only on the frequency of the spectral line, the mass of the emitting particles, and their temperature , and therefore can be used for inferring the temperature of an emitting (or absorbing) body being spectroscopically ...

  8. Electrophoretic light scattering - Wikipedia

    en.wikipedia.org/wiki/Electrophoretic_light...

    Electrophoretic light scattering (also known as laser Doppler electrophoresis and phase analysis light scattering) is based on dynamic light scattering. The frequency shift or phase shift of an incident laser beam depends on the dispersed particles mobility.

  9. Doppler imaging - Wikipedia

    en.wikipedia.org/wiki/Doppler_imaging

    Doppler imaging was first used to map chemical peculiarities on the surface of Ap stars.For mapping starspots it was first used by Steven Vogt and Donald Penrod in 1983, when they demonstrated that signatures of starspots were observable in the line profiles of the active binary star HR 1099 (V711 Tau); from this they could derive an image of the stellar surface.