enow.com Web Search

Search results

  1. Results from the WOW.Com Content Network
  2. Milky Way - Wikipedia

    en.wikipedia.org/wiki/Milky_Way

    In Meteorologica, Aristotle (384–322 BC) states that the Greek philosophers Anaxagoras (c. 500 –428 BC) and Democritus (460–370 BC) proposed that the Milky Way is the glow of stars not directly visible due to Earth's shadow, while other stars receive their light from the Sun, but have their glow obscured by solar rays. [72]

  3. Location of Earth - Wikipedia

    en.wikipedia.org/wiki/Location_of_Earth

    Initially, Earth was believed to be the center of the Universe, which consisted only of those planets visible with the naked eye and an outlying sphere of fixed stars. [1] After the acceptance of the heliocentric model in the 17th century, observations by William Herschel and others showed that the Sun lay within a vast, disc-shaped galaxy of ...

  4. Galactic orientation - Wikipedia

    en.wikipedia.org/wiki/Galactic_orientation

    The Milky Way Galaxy [4] is only one of the billions of galaxies in the known universe. Galaxies are classified into spirals, [5] ellipticals, irregular, and peculiar. Sizes can range from only a few thousand stars (dwarf irregulars) to 10 13 stars in giant ellipticals. Elliptical galaxies are spherical or elliptical in appearance.

  5. Astronomical coordinate systems - Wikipedia

    en.wikipedia.org/wiki/Astronomical_coordinate...

    In astronomy, coordinate systems are used for specifying positions of celestial objects (satellites, planets, stars, galaxies, etc.) relative to a given reference frame, based on physical reference points available to a situated observer (e.g. the true horizon and north to an observer on Earth's surface). [1]

  6. Galactic coordinate system - Wikipedia

    en.wikipedia.org/wiki/Galactic_coordinate_system

    The anisotropy of the star density in the night sky makes the galactic coordinate system very useful for coordinating surveys, both those that require high densities of stars at low galactic latitudes, and those that require a low density of stars at high galactic latitudes.

  7. Local Group - Wikipedia

    en.wikipedia.org/wiki/Local_Group

    The term "The Local Group" was introduced by Edwin Hubble in Chapter VI of his 1936 book The Realm of the Nebulae. [11] There, he described it as "a typical small group of nebulae which is isolated in the general field" and delineated, by decreasing luminosity, its members to be M31, Milky Way, M33, Large Magellanic Cloud, Small Magellanic Cloud, M32, NGC 205, NGC 6822, NGC 185, IC 1613 and ...

  8. Stellar parallax - Wikipedia

    en.wikipedia.org/wiki/Stellar_parallax

    Created by the different orbital positions of Earth, the extremely small observed shift is largest at time intervals of about six months, when Earth arrives at opposite sides of the Sun in its orbit, giving a baseline (the shortest side of the triangle made by a star to be observed and two positions of Earth) distance of about two astronomical ...

  9. Galactic plane - Wikipedia

    en.wikipedia.org/wiki/Galactic_plane

    The Galactic Center is located at position angle 31.72° (B1950) or 31.40° (J2000) east of north. This edge-on view of the galaxy NGC 4452 from Earth shows its galactic plane, with the nucleus at the center.