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  2. File:Navigational-stars-above-30-degrees-north.svg - Wikipedia

    en.wikipedia.org/wiki/File:Navigational-stars...

    The northern stars above declination 30 degrees north of navigational astronomy. Date: 4 September 2010, 17:13 (UTC) Source: Navigational-stars-north.svg; Author: Navigational-stars-north.svg: U.S. National Imagery and Mapping Agency/User:Haus; derivative work: Haus (talk) Other versions: Derivative works of this file: Navigational-stars-below ...

  3. Polaris - Wikipedia

    en.wikipedia.org/wiki/Polaris

    Polaris is a star in the northern circumpolar constellation of Ursa Minor. It is designated α Ursae Minoris (Latinized to Alpha Ursae Minoris) and is commonly called the North Star or Pole Star. With an apparent magnitude that fluctuates around 1.98, [3] it is the brightest star in the constellation and is readily visible to the naked eye at ...

  4. Template:Northern Stars - Wikipedia

    en.wikipedia.org/wiki/Template:Northern_Stars

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  5. Pole star - Wikipedia

    en.wikipedia.org/wiki/Pole_star

    Northern Hemisphere circumpolar stars around Polaris, with a long-exposure producing a star trail photo. A pole star is a visible star that is approximately aligned with the axis of rotation of an astronomical body; that is, a star whose apparent position is close to one of the celestial poles.

  6. Northern Star - Wikipedia

    en.wikipedia.org/wiki/Northern_Star

    Northern star is a term for the star Polaris. Northern star(s) may also refer to: Books and newspapers. The Northern Star, a newspaper in New South Wales, Australia;

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  8. List of stars for navigation - Wikipedia

    en.wikipedia.org/wiki/List_of_stars_for_navigation

    The two brightest northern stars are Vega and Capella. In the star chart to the right, declination is shown by the radial coordinate, starting at 90° north in the center and decreasing to 30° north at the outer edge. Sidereal hour angle is shown as the angular coordinate, starting at 0° at the left of the chart, and increasing counter-clockwise.

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