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  2. Stellar parallax - Wikipedia

    en.wikipedia.org/wiki/Stellar_parallax

    Giuseppe Calandrelli noted stellar parallax in 1805-6 and came up with a 4-second value for the star Vega which was a gross overestimate. [3] The first successful stellar parallax measurements were done by Thomas Henderson in Cape Town South Africa in 1832–1833, where he measured parallax of one of the closest stars, Alpha Centauri.

  3. Parallax in astronomy - Wikipedia

    en.wikipedia.org/wiki/Parallax_in_astronomy

    A parsec is the distance from the Sun to an astronomical object that has a parallax angle of one arcsecond (not to scale). The parsec (symbol: pc) is a unit of length used to measure the large distances to astronomical objects outside the Solar System, approximately equal to 3.26 light-years or 206,265 astronomical units (AU), i.e. 30.9 trillion kilometres (19.2 trillion miles).

  4. Parallax - Wikipedia

    en.wikipedia.org/wiki/Parallax

    Parallax is a displacement or difference in the apparent position of an object viewed along two different lines of sight and is measured by the angle or half-angle of inclination between those two lines. [1] [2] Due to foreshortening, nearby objects show a larger parallax than farther objects, so parallax can be used to determine distances.

  5. Parsec - Wikipedia

    en.wikipedia.org/wiki/Parsec

    The parallax method is the fundamental calibration step for distance determination in astrophysics; however, the accuracy of ground-based telescope measurements of parallax angle is limited to about 0.01″, and thus to stars no more than 100 pc distant. [12] This is because the Earth's atmosphere limits the sharpness of a star's image.

  6. Astronomical unit - Wikipedia

    en.wikipedia.org/wiki/Astronomical_unit

    The parsec (parallax arcsecond) is defined in terms of the astronomical unit, being the distance of an object with a parallax of 1″. The light-year is often used in popular works, but is not an approved non-SI unit and is rarely used by professional astronomers. [28]

  7. Parallax (character) - Wikipedia

    en.wikipedia.org/wiki/Parallax_(character)

    The Hal Jordan incarnation of Parallax as depicted in Green Lantern (vol. 3) #50 (March 1994). Art by Darryl Banks.. In 1994, in an effort to generate interest in its Green Lantern comics, DC replaced Hal Jordan, who had been the primary Green Lantern since the late 1950s, with the character Kyle Rayner, and eliminated the Green Lantern Corps which had served as supporting characters in the ...

  8. Gliese 777 - Wikipedia

    en.wikipedia.org/wiki/Gliese_777

    Parallax (π) 62.4865 ± 0.34 ... Initially therefore, the planet was believed to be a true "Jupiter-twin" but was later redefined as being more like an "eccentric ...

  9. Autostereoscopy - Wikipedia

    en.wikipedia.org/wiki/Autostereoscopy

    Comparison of parallax-barrier and lenticular autostereoscopic displays. Note: The figure is not to scale. Autostereoscopy is any method of displaying stereoscopic images (adding binocular perception of 3D depth) without the use of special headgear, glasses, something that affects vision, or anything for eyes on the part of the viewer.