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  2. Angular diameter - Wikipedia

    en.wikipedia.org/wiki/Angular_diameter

    The angular diameter, angular size, apparent diameter, or apparent size is an angular separation (in units of angle) describing how large a sphere or circle appears from a given point of view. In the vision sciences , it is called the visual angle , and in optics , it is the angular aperture (of a lens ).

  3. Minute and second of arc - Wikipedia

    en.wikipedia.org/wiki/Minute_and_second_of_arc

    The arcsecond is also often used to describe small astronomical angles such as the angular diameters of planets (e.g. the angular diameter of Venus which varies between 10″ and 60″); the proper motion of stars; the separation of components of binary star systems; and parallax, the small change of position of a star or Solar System body as ...

  4. Proper motion - Wikipedia

    en.wikipedia.org/wiki/Proper_motion

    The first is the direction of the proper motion on the celestial sphere (with 0 degrees meaning the motion is north, 90 degrees meaning the motion is east, (left on most sky maps and space telescope images) and so on), and the second is its magnitude, typically expressed in arcseconds per year (symbols: arcsec/yr, as/yr, ″/yr, ″ yr −1) or ...

  5. File:Comparison angular diameter solar system.svg - Wikipedia

    en.wikipedia.org/wiki/File:Comparison_angular...

    English: Comparison of angular diameter of the Sun, Moon and planets with the International Space Station (as seen from the surface of the Earth), the 20/20 row of the Snellen eye chart at the proper viewing distance and typical human visual acuity. The dotted circles represent the minimum angular size (when the celestial bodies are farthest ...

  6. Template:Solar radius calculator - Wikipedia

    en.wikipedia.org/wiki/Template:Solar_radius...

    All radii, once calculated, are divided by 6.957 × 10 8 to convert from m to R ☉.. AD radius determined from angular diameter and distance =, (/) =, = D is multiplied by 3.0857 × 10 19 to convert from kpc to m

  7. Surface brightness - Wikipedia

    en.wikipedia.org/wiki/Surface_brightness

    However, a star is so small it is effectively a point source in most observations (the largest angular diameter, that of R Doradus, is 0.057 ± 0.005 arcsec), whereas a galaxy may extend over several arcseconds or arcminutes. Therefore, the galaxy will be harder to see than the star against the airglow background light. Apparent magnitude is a ...

  8. Astronomical seeing - Wikipedia

    en.wikipedia.org/wiki/Astronomical_seeing

    The diameter of the seeing disk is the full width at half maximum of its optical intensity. An exposure time of several tens of milliseconds can be considered long in this context. The Fried parameter describes the size of an imaginary telescope aperture for which the diffraction limited angular resolution is equal to the resolution limited by ...

  9. Jupiter - Wikipedia

    en.wikipedia.org/wiki/Jupiter

    The angular diameter of Jupiter likewise varies from 50.1 to 30.5 arc seconds. [2] Favourable oppositions occur when Jupiter is passing through the perihelion of its orbit, bringing it closer to Earth. [ 138 ]