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  2. Messier 81 - Wikipedia

    en.wikipedia.org/wiki/Messier_81

    Messier 81 (also known as NGC 3031 or Bode's Galaxy) is a grand design spiral galaxy about 12 million light-years away in the constellation Ursa Major. It has a D 25 isophotal diameter of 29.44 kiloparsecs (96,000 light-years ).

  3. List of nearest galaxies - Wikipedia

    en.wikipedia.org/wiki/List_of_nearest_galaxies

    This is a list of known galaxies within 3.8 megaparsecs (12.4 million light-years) of the Solar System, in ascending order of heliocentric distance, or the distance to the Sun. This encompasses about 50 major Local Group galaxies, and some that are members of neighboring galaxy groups , the M81 Group and the Centaurus A/M83 Group , and some ...

  4. M81 Group - Wikipedia

    en.wikipedia.org/wiki/M81_Group

    The M81 Group is a galaxy group in the constellations Ursa Major and Camelopardalis that includes the galaxies Messier 81 and Messier 82, as well as several other galaxies with high apparent brightnesses. [1] The approximate center of the group is located at a distance of 3.6 Mpc, making it one of the nearest groups to the Local Group. [1]

  5. Lagoon Nebula - Wikipedia

    en.wikipedia.org/wiki/Lagoon_Nebula

    The Lagoon Nebula (catalogued as Messier 8 or M8, NGC 6523, Sharpless 25, RCW 146, and Gum 72) is a giant interstellar cloud in the constellation Sagittarius. It is classified as an emission nebula and has an H II region .

  6. List of the most distant astronomical objects - Wikipedia

    en.wikipedia.org/wiki/List_of_the_most_distant...

    2.6 AU when Mars is diametrically opposed to Earth Kepler correctly characterized Mars and Earth's orbits in the publication Astronomia nova. It had been conjectured that the fixed stars were much farther away than the planets. Sun: Star 3rd century BC — 1609 380 Earth radii (very inaccurate, true=16000 Earth radii)

  7. Ursa Major - Wikipedia

    en.wikipedia.org/wiki/Ursa_Major

    M81 is a nearly face-on spiral galaxy 11.8 million light-years from Earth. Like most spiral galaxies, it has a core made up of old stars, with arms filled with young stars and nebulae. Along with M82, it is a part of the galaxy cluster closest to the Local Group. M82 is a nearly edgewise galaxy that is interacting gravitationally with M81.

  8. Messier 87 - Wikipedia

    en.wikipedia.org/wiki/Messier_87

    The disk rotates at velocities of up to roughly 1,000 km/s (2,200,000 mph) [75] and spans a maximum diameter of 25,000 AU (3.7 trillion km; 2.3 trillion mi). [76] By comparison, Pluto averages 39 AU (5.8 billion km; 3.6 billion mi) from the Sun. Gas accretes onto the black hole at an estimated rate of one solar mass every ten years (about 90 ...

  9. Apparent magnitude - Wikipedia

    en.wikipedia.org/wiki/Apparent_magnitude

    seen from 1 AU away would be over 2 × 10 16 (20 quadrillion) times as bright as the Sun when seen from the Earth −43.27 star NGC 2403 V14: seen from 1 AU away −41.82 star NGC 2363-V1: seen from 1 AU away −41.39 star Cygnus OB2-12: seen from 1 AU away −40.67 star M33-013406.63: seen from 1 AU away −40.17 star η Carinae A seen from 1 ...