Chowist Web Search

  1. Ad

    related to: 3d milky way map ariadne arm

Search results

  1. Results From The WOW.Com Content Network
  2. Orion Arm - Wikipedia

    en.wikipedia.org/wiki/Orion_Arm

    The Orion Arm, also known as the Orion–Cygnus Arm, is a minor spiral arm within the Milky Way Galaxy spanning 3,500 light-years (1,100 parsecs) in width and extending roughly 10,000 light-years (3,100 parsecs) in length. [2] This galactic structure encompasses the Solar System, including Earth.

  3. Radcliffe wave - Wikipedia

    en.wikipedia.org/wiki/Radcliffe_wave

    The Radcliffe wave is a neighbouring coherent gaseous structure in the Milky Way, dotted with a related high concentration of interconnected stellar nurseries. It stretches about 8,800 light years. This structure runs with the trajectory of the Milky Way arms.

  4. A new, incredibly detailed 3D map of the Milky Way has revealed that its central disk is wavy, much like an enormous potato chip.This new picture of the galactic disk — the central region of the ...

  5. Perseus Arm - Wikipedia

    en.wikipedia.org/wiki/Perseus_Arm

    The Perseus Arm is one of two major spiral arms of the Milky Way galaxy. The second major arm is called the Scutum–Centaurus Arm. The Perseus Arm begins from the distal end of the long Milky Way central bar. [1]

  6. Galactic quadrant - Wikipedia

    en.wikipedia.org/wiki/Galactic_quadrant

    A galactic quadrant, or quadrant of the Galaxy, is one of four circular sectors in the division of the Milky Way Galaxy. Numbered quadrants and sectors of constellations. Quadrants as starcharts, with most prominent stars marked.

  7. Local Bubble - Wikipedia

    en.wikipedia.org/wiki/Local_Bubble

    The Local Bubble, or Local Cavity, is a relative cavity in the interstellar medium (ISM) of the Orion Arm in the Milky Way. It contains the closest of celestial neighbours and among others, the Local Interstellar Cloud (which contains the Solar System ), the neighbouring G-Cloud , the Ursa Major moving group ( the closest stellar moving group ...

  8. Milky Way - Wikipedia

    en.wikipedia.org/wiki/Milky_Way

    Two spiral arms, the Scutum–Centaurus arm and the Carina–Sagittarius arm, have tangent points inside the Sun's orbit about the center of the Milky Way. If these arms contain an overdensity of stars compared to the average density of stars in the Galactic disk, it would be detectable by counting the stars near the tangent point.

  9. Galactic coordinate system - Wikipedia

    en.wikipedia.org/wiki/Galactic_coordinate_system

    Artist's depiction of the Milky Way Galaxy, showing the galactic longitude. A vector matching the plane of the galaxy, at 0° longitude, notably has the Galactic Center and intersects arms directly beyond.

  10. Gould Belt - Wikipedia

    en.wikipedia.org/wiki/Gould_Belt

    Mesh map of the inner Gould Belt created from Gaia observatory data. The Gould Belt is a local ring of stars in the Milky Way, tilted away from the galactic plane by about 16–20 degrees, first reported by John Herschel and Benjamin Gould in the 19th century.

  11. File:Milky Way Spiral Arm.svg - Wikipedia

    en.wikipedia.org/wiki/File:Milky_Way_Spiral_Arm.svg

    A composite map of the Milky Way's Spiral Structure showing several arms of the Milky Way. The obscured region is known as the Zone of Avoidance (ZOA) as the light, gas and dust obscure the region from sight.