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  2. Redshift - Wikipedia

    en.wikipedia.org/wiki/Redshift

    Similarly, small redshifts and blueshifts detected in the spectroscopic measurements of individual stars are one way astronomers have been able to diagnose and measure the presence and characteristics of planetary systems around other stars and have even made very detailed differential measurements of redshifts during planetary transits to ...

  3. Quasars, Redshifts and Controversies - Wikipedia

    en.wikipedia.org/wiki/Quasars,_Redshifts_and...

    Arp also argued that some galaxies showed unusual redshifts, and that redshifts themselves could be quantized. These are controversial views which do not accord with the standard model of physical cosmology. It also contradicts the accepted model that quasars are bright nuclei of very distant galaxies. Most astronomers reject Arp's ...

  4. Gravitational redshift - Wikipedia

    en.wikipedia.org/wiki/Gravitational_redshift

    In astronomy, the magnitude of a gravitational redshift is often expressed as the velocity that would create an equivalent shift through the relativistic Doppler effect. In such units, the 2 ppm sunlight redshift corresponds to a 633 m/s receding velocity, roughly of the same magnitude as convective motions in the Sun, thus complicating the ...

  5. Redshift survey - Wikipedia

    en.wikipedia.org/wiki/Redshift_survey

    In astronomy, a redshift survey is a survey of a section of the sky to measure the redshift of astronomical objects: usually galaxies, but sometimes other objects such as galaxy clusters or quasars. Using Hubble's law , the redshift can be used to estimate the distance of an object from Earth .

  6. Redshift quantization - Wikipedia

    en.wikipedia.org/wiki/Redshift_quantization

    Redshift quantization, also referred to as redshift periodicity, [1] redshift discretization, [2] preferred redshifts [3] and redshift-magnitude bands, [4] [5] is the hypothesis that the redshifts of cosmologically distant objects (in particular galaxies and quasars) tend to cluster around multiples of some particular value.

  7. Photometric redshift - Wikipedia

    en.wikipedia.org/wiki/Photometric_redshift

    A photometric redshift is an estimate for the recession velocity of an astronomical object such as a galaxy or quasar, made without measuring its spectrum.The technique uses photometry (that is, the brightness of the object viewed through various standard filters, each of which lets through a relatively broad passband of colours, such as red light, green light, or blue light) to determine the ...

  8. Astronomers Finally Know How Black Holes ‘Spaghettify’ Stars

    www.aol.com/lifestyle/astronomers-finally-know...

    Insights from a stellar death 215 million light-years from Earth show a black hole blowing the star away—not just sucking it in. Astronomers Finally Know How Black Holes ‘Spaghettify’ Stars ...

  9. Rossiter–McLaughlin effect - Wikipedia

    en.wikipedia.org/wiki/Rossiter–McLaughlin_effect

    As the main star rotates on its axis, one quadrant of its photosphere will be seen to be coming towards the viewer, and the other visible quadrant to be moving away. These motions produce blueshifts and redshifts, respectively, in the star's spectrum, usually observed as a broadening of the spectral lines. When the secondary star or planet ...