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  2. Timeline of knowledge about galaxies, clusters of galaxies ...

    en.wikipedia.org/wiki/Timeline_of_knowledge...

    1978 – Vera Rubin, Kent Ford, N. Thonnard, and Albert Bosma measure the rotation curves of several spiral galaxies and find significant deviations from what is predicted by the Newtonian gravitation of visible stars. 1978 – Leonard Searle and Robert Zinn theorize that galaxy formation occurs through the merger of smaller groups.

  3. Galaxy formation and evolution - Wikipedia

    en.wikipedia.org/wiki/Galaxy_formation_and_evolution

    In cosmology, the study of galaxy formation and evolution is concerned with the processes that formed a heterogeneous universe from a homogeneous beginning, the formation of the first galaxies, the way galaxies change over time, and the processes that have generated the variety of structures observed in nearby galaxies. Galaxy formation is ...

  4. Galaxy groups and clusters - Wikipedia

    en.wikipedia.org/wiki/Galaxy_groups_and_clusters

    MACS J0152.5-2852 is a massive galaxy cluster. Almost every pixel seen in the image is a galaxy, each containing billions of stars. [1]Galaxy groups and clusters are the largest known gravitationally bound objects to have arisen thus far in the process of cosmic structure formation. [2]

  5. New James Webb telescope pictures zoom in on various ... - AOL

    www.aol.com/james-webb-telescope-pictures-zoom...

    The fifth galaxy in the quintet is much closer to Earth and only looks like it is part of the group. To really absorb the different shapes and structures of galaxies, JWST just released a mosaic ...

  6. International astronomy team reveal images of star-forming ...

    www.aol.com/international-astronomy-team-reveal...

    The light from the galaxies has been travelling for billions of years to reach the Earth. Skip to main content. Sign in. Mail. 24/7 Help. For premium support please call: ...

  7. Galactic orientation - Wikipedia

    en.wikipedia.org/wiki/Galactic_orientation

    Spiral galaxies range from S0, the lenticular galaxies, to Sb, which have a bar across the nucleus, to Sc galaxies which have strong spiral arms. In total count, ellipticals amount to 13%, S0 to 22%, Sa, b, c galaxies to 61%, irregulars to 3.5%, and peculiars to 0.9%. At the center of most galaxies is a high concentration of older stars.

  8. Supercluster - Wikipedia

    en.wikipedia.org/wiki/Supercluster

    A supercluster is a large group of smaller galaxy clusters or galaxy groups; [1] they are among the largest known structures in the universe. The Milky Way is part of the Local Group galaxy group (which contains more than 54 galaxies), which in turn is part of the Virgo Supercluster , which is part of the Laniakea Supercluster , which is part ...

  9. Outline of galaxies - Wikipedia

    en.wikipedia.org/wiki/Outline_of_galaxies

    Many galaxies are thought to have black holes at their active centers. The Milky Way's central black hole, known as Sagittarius A* , has a mass four million times greater than the Sun. As of March 2016, GN-z11 is the oldest and most distant observed galaxy with a comoving distance of 32 billion light-years from Earth, and observed as it existed ...