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  2. Milky Way - Wikipedia

    en.wikipedia.org/wiki/Milky_Way

    The Milky Way is the galaxy that includes the Solar System, with the name describing the galaxy's appearance from Earth: a hazy band of light seen in the night sky formed from stars that cannot be individually distinguished by the naked eye.

  3. Andromeda–Milky Way collision - Wikipedia

    en.wikipedia.org/wiki/Andromeda–Milky_Way...

    A NASA conception of the collision using computer-generated imagery. The AndromedaMilky Way collision is a galactic collision predicted to occur in about 4.5 billion years between the two largest galaxies in the Local Group —the Milky Way (which contains the Solar System and Earth) and the Andromeda Galaxy.

  4. Great Debate (astronomy) - Wikipedia

    en.wikipedia.org/wiki/Great_Debate_(astronomy)

    Arguments. The "Great Spiral Nebula" in the constellation Andromeda (1902 photograph). The Debate was over whether this was a cloud of gas and dust or a distant galaxy. Shapley was arguing in favor of the Milky Way as the entirety of the universe. [2]

  5. Galaxy rotation curve - Wikipedia

    en.wikipedia.org/wiki/Galaxy_rotation_curve

    A model of galaxy based on a general relativity metric was also proposed, showing that the rotation curves for the Milky Way, NGC 3031, NGC 3198 and NGC 7331 are consistent with the mass density distributions of the visible matter, avoiding the need for a massive halo of exotic dark matter.

  6. Galactocentrism - Wikipedia

    en.wikipedia.org/wiki/Galactocentrism

    In astronomy, galactocentrism is the theory that the Milky Way Galaxy, home of Earth ' s Solar System, is at or near the center of the Universe. Thomas Wright and Immanuel Kant first speculated that fuzzy patches of light called nebulae were actually distant "island universes" consisting of many stellar systems.

  7. MilkyWay@home - Wikipedia

    en.wikipedia.org/wiki/MilkyWay@home

    Purpose and design. MilkyWay@home is a collaboration between the Rensselaer Polytechnic Institute 's departments of Computer Science and Physics, Applied Physics and Astronomy and is supported by the U.S. National Science Foundation. It is operated by a team that includes astrophysicist Heidi Jo Newberg and computer scientists Malik Magdon ...

  8. Galaxy formation and evolution - Wikipedia

    en.wikipedia.org/wiki/Galaxy_formation_and_evolution

    In the Local Group, the Milky Way and the Andromeda Galaxy are gravitationally bound, and currently approaching each other at high speed. Simulations show that the Milky Way and Andromeda are on a collision course, and are expected to collide in less than five billion years.

  9. Density wave theory - Wikipedia

    en.wikipedia.org/wiki/Density_wave_theory

    Density wave theory or the Lin–Shu density wave theory is a theory proposed by C.C. Lin and Frank Shu in the mid-1960s to explain the spiral arm structure of spiral galaxies. [1] [2] The Lin–Shu theory introduces the idea of long-lived quasistatic spiral structure (QSSS hypothesis). [1]

  10. Heliocentrism - Wikipedia

    en.wikipedia.org/wiki/Heliocentrism

    William Herschel's model of the Milky Way, 1785. In 1783, amateur astronomer William Herschel attempted to determine the shape of the universe by examining stars through his handmade telescopes. Herschel was the first to propose a model of the universe based on observation and measurement.

  11. William Herschel - Wikipedia

    en.wikipedia.org/wiki/William_Herschel

    William Herschel's model of the Milky Way, 1785 Herschel also studied the structure of the Milky Way and was the first to propose a model of the galaxy based on observation and measurement. [92] He concluded that it was in the shape of a disk , but incorrectly assumed that the Sun was in the centre of the disk.