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  2. Milky Way - Wikipedia

    en.wikipedia.org/wiki/Milky_Way

    The Milky Way [c] 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. Tianhe-2 - Wikipedia

    en.wikipedia.org/wiki/Tianhe-2

    Tianhe-2 or TH-2 ( Chinese: 天河-2; pinyin: tiānhé-èr; lit. 'Heavenriver-2', i.e. ' Milky Way 2') is a 3.86- petaflops supercomputer located in the National Supercomputer Center in Guangzhou, China. [3] It was developed by a team of 1,300 scientists and engineers. It was the world's fastest supercomputer according to the TOP500 lists for ...

  4. Galactic habitable zone - Wikipedia

    en.wikipedia.org/wiki/Galactic_habitable_zone

    e. In astrobiology and planetary astrophysics, the galactic habitable zone is the region of a galaxy in which life might most likely develop. The concept of a galactic habitable zone analyzes various factors, such as metallicity (the presence of elements heavier than hydrogen and helium) and the rate and density of major catastrophes such as ...

  5. Andromeda Galaxy - Wikipedia

    en.wikipedia.org/wiki/Andromeda_Galaxy

    A visible light image of the Andromeda Galaxy. Messier 32 is to the left of the galactic nucleus and Messier 110 is at the bottom right. The Andromeda Galaxy is a barred spiral galaxy and is the nearest major galaxy to the Milky Way. It was originally named the Andromeda Nebula and is cataloged as Messier 31, M31, and NGC 224.

  6. Galactic Center - Wikipedia

    en.wikipedia.org/wiki/Galactic_Center

    Galactic Center. 17 45 40.04, −29° 00′ 28.1″. The Galactic Center, as seen by one of the 2MASS infrared telescopes, is located in the bright upper left portion of the image. Marked location of the Galactic Center. The Galactic Center is the barycenter of the Milky Way and a corresponding point on the rotational axis of the galaxy.

  7. Fermi paradox - Wikipedia

    en.wikipedia.org/wiki/Fermi_paradox

    Enrico Fermi (1901–1954) The Fermi paradox is a conflict between the argument that scale and probability seem to favor intelligent life being common in the universe, and the total lack of evidence of intelligent life having ever arisen anywhere other than on Earth. The first aspect of the Fermi paradox is a function of the scale or the large ...

  8. Alpha Centauri - Wikipedia

    en.wikipedia.org/wiki/Alpha_Centauri

    Alpha Centauri ( α Centauri, α Cen, or Alpha Cen) is a triple star system in the southern constellation of Centaurus. It consists of three stars: Rigil Kentaurus ( α Centauri A ), Toliman ( α Centauri B ), and Proxima Centauri ( α Centauri C ). [14] Proxima Centauri is the closest star to the Sun at 4.2465 light-years (1.3020 pc ).

  9. Galaxy merger - Wikipedia

    en.wikipedia.org/wiki/Galaxy_merger

    The Mice Galaxies (NGC 4676 A&B) are in the process of merging. This artist's impression shows the merger between two galaxies leading to the formation of a disc galaxy. Galaxy mergers can occur when two (or more) galaxies collide. They are the most violent type of galaxy interaction. The gravitational interactions between galaxies and the ...

  10. Cosmic dust - Wikipedia

    en.wikipedia.org/wiki/Cosmic_dust

    Cosmic dust – also called extraterrestrial dust, space dust, or star dust – is dust that occurs in outer space or has fallen onto Earth. [1] [2] Most cosmic dust particles measure between a few molecules and 0.1 mm (100 μm ), such as micrometeoroids. Larger particles are called meteoroids.

  11. Stellar kinematics - Wikipedia

    en.wikipedia.org/wiki/Stellar_kinematics

    Barnard's Star is the star with the highest proper motion. [1] In astronomy, stellar kinematics is the observational study or measurement of the kinematics or motions of stars through space. Stellar kinematics encompasses the measurement of stellar velocities in the Milky Way and its satellites as well as the internal kinematics of more distant ...