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  2. Magnitude (astronomy) - Wikipedia

    en.wikipedia.org/wiki/Magnitude_(astronomy)

    An illustration of light sources from magnitude 1 to 3.5, in 0.5 increments. In astronomy, magnitude is a measure of the brightness of an object, usually in a defined passband. An imprecise but systematic determination of the magnitude of objects was introduced in ancient times by Hipparchus. Magnitude values do not have a unit.

  3. Astronomical object articles need an infobox to show basic data about them. A complete list of the templates to be used is at Wikipedia:WikiProject Astronomical objects/Infoboxes. When filling in scientific data, you may find the following templates useful: {{±|pos|neg}} which produces: +pos −neg used thus: 500 +35 −22 km. (Avoid using it ...

  4. Star chart - Wikipedia

    en.wikipedia.org/wiki/Star_chart

    SFA Star ChartsFree star charts; Geody Star ChartsFree (CC-by-sa) printer friendly star charts for several latitudes and times of the year; An online star chart; Monthly sky maps for every location on Earth Archived 2007-09-13 at the Wayback Machine; The Evening Sky Map – Free monthly star charts and calendar for northern hemisphere ...

  5. Template:POTD/2010-01-12 - Wikipedia

    en.wikipedia.org/wiki/Template:POTD/2010-01-12

    An illustration of relative astronomical orders of magnitude, starting with the terrestrial planets of the Solar System in image 1 (top left) and ending with the largest known star, VY Canis Majoris, at the bottom right. The biggest celestial body in each image is shown on the left of the next frame.Image credit: Dave Jarvis

  6. Apparent magnitude - Wikipedia

    en.wikipedia.org/wiki/Apparent_magnitude

    The absolute magnitude M, of a star or astronomical object is defined as the apparent magnitude it would have as seen from a distance of 10 parsecs (33 ly). The absolute magnitude of the Sun is 4.83 in the V band (visual), 4.68 in the Gaia satellite's G band (green) and 5.48 in the B band (blue).

  7. AB magnitude - Wikipedia

    en.wikipedia.org/wiki/AB_magnitude

    The monochromatic AB magnitude is defined as the logarithm of a spectral flux density with the usual scaling of astronomical magnitudes and a zero-point of about 3 631 janskys (symbol Jy), [1] where 1 Jy = 10 −26 W Hz −1 m −2 = 10 −23 erg s −1 Hz −1 cm −2 ("about" because the true definition of the zero point is based on magnitudes as shown below).

  8. Celestial cartography - Wikipedia

    en.wikipedia.org/wiki/Celestial_cartography

    "Astronomy: Star Atlases, Charts, and Maps", a collection of more than 60 star atlas volumes. "Astronomy: Selected Images , a collection of high-resolution star map images. "History of Cosmology: Views of the Stars" , high-resolution scans of prints relating to the study of the structure of the cosmos.

  9. Template:Units of length used in Astronomy - Wikipedia

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

    Create account; Log in; Pages for ... (Top) 1 See also. Toggle the table of contents. Template: Units of length used in Astronomy. ... Template documentation See also ...