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  2. Galaxy morphological classification - Wikipedia

    en.wikipedia.org/wiki/Galaxy_morphological...

    Rings. Galaxies are divided into those possessing ring-like structures (denoted ‘(r)’) and those without rings (denoted ‘(s)’). So-called ‘transition’ galaxies are given the symbol (rs). [16] Spiral arms. As in Hubble’s original scheme, spiral galaxies are assigned to a class based primarily on the tightness of their spiral arms.

  3. Correlation function (astronomy) - Wikipedia

    en.wikipedia.org/wiki/Correlation_function...

    It can be thought of as a "clumpiness" factor - the higher the value for some distance scale, the more "clumpy" the universe is at that distance scale. From every pair in a distribution of galaxies, the two-point correlation function is calculated by counting the number of pairs that are separated by distances in various bins.

  4. List of galaxies - Wikipedia

    en.wikipedia.org/wiki/List_of_galaxies

    Size (left) and distance (right) of a few well-known galaxies put to scale. There are an estimated 100 billion galaxies in all of the observable universe. [1] On the order of 100,000 galaxies make up the Local Supercluster, and about 51 galaxies are in the Local Group (see list of nearest galaxies for a complete list).

  5. Inhomogeneous cosmology - Wikipedia

    en.wikipedia.org/wiki/Inhomogeneous_cosmology

    An inhomogeneous cosmology is a physical cosmological theory (an astronomical model of the physical universe's origin and evolution) which, unlike the dominant cosmological concordance model, assumes that inhomogeneities in the distribution of matter across the universe affect local gravitational forces (i.e., at the galactic level) enough to skew our view of the Universe. [3]

  6. Type-cD galaxy - Wikipedia

    en.wikipedia.org/wiki/Type-cD_galaxy

    The cD-type is a classification in the Yerkes galaxy classification scheme, one of two Yerkes classifications still in common use, along with D-type. [8] The "c" in "cD" refers to the fact that the galaxies are very large, hence the adjective supergiant, while the "D" refers to the fact that the galaxies appear diffuse. [9]

  7. Scientists untangle mystery about the universe's earliest ...

    www.aol.com/news/scientists-untangle-mystery...

    Immediately after the Big Bang, the universe was filled with a very hot, nearly uniform plasma - a fireball - and there were no stars or galaxies," Northwestern University astrophysicist and study ...

  8. Linda Sparke - Wikipedia

    en.wikipedia.org/wiki/Linda_Sparke

    Sparke was elected as a Fellow of the American Physical Society in 2002, after a nomination from the APS Division of Astrophysics. The fellowship citation noted her "studies of the structure and dynamics of galaxies, using orbital motions to probe both time-steady and time-varying gravitational potentials, and the distribution of dark matter ...

  9. Hubble Telescope reveals new discovery of universe's ... - AOL

    www.aol.com/news/2017-06-14-hubble-telescope...

    The Hubble telescope captures the brightest galaxies ever seen, thousands of galaxies act like lenses that magnify light, making them appear super bright. Hubble Telescope reveals new discovery of ...