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  2. Cosmic distance ladder - Wikipedia

    en.wikipedia.org/wiki/Cosmic_distance_ladder

    The amount of shift is quite small, even for the nearest stars, measuring 1 arcsecond for an object at 1 parsec's distance (3.26 light-years), and thereafter decreasing in angular amount as the distance increases. Astronomers usually express distances in units of parsecs (parallax arcseconds); light-years are used in popular media.

  3. HD 141569 - Wikipedia

    en.wikipedia.org/wiki/HD_141569

    HD 141569 is an isolated [5] Herbig Ae/Be star [6] of spectral class A2Ve [7] approximately 364 light-years away in the constellation of Libra. The primary star has two red dwarf companions (orbiting each other) at about nine arcseconds. In 1999, a protoplanetary disk was discovered around the star.

  4. Stellar parallax - Wikipedia

    en.wikipedia.org/wiki/Stellar_parallax

    The parsec (3.26 light-years) is defined as the distance for which the annual parallax is 1 arcsecond. Annual parallax is normally measured by observing the position of a star at different times of the year as Earth moves through its orbit. The angles involved in these calculations are very small and thus difficult to measure.

  5. List of nearest stars - Wikipedia

    en.wikipedia.org/wiki/List_of_nearest_stars

    This number is likely much higher, due to the sheer number of stars needed to be surveyed; a star approaching the Solar System 10 million years ago, moving at a typical Sun-relative 20–200 kilometers per second, would be 600–6,000 light-years from the Sun at present day, with millions of stars closer to the Sun.

  6. List of star systems within 150–200 light-years - Wikipedia

    en.wikipedia.org/wiki/List_of_star_systems_within...

    Print/export Download as PDF; Printable version; In other projects ... This is a list of star systems within 150–200 light years of Earth. [1] [2] [3]

  7. Nu Orionis - Wikipedia

    en.wikipedia.org/wiki/Nu_Orionis

    Based upon an annual parallax shift of 0.00632 arcseconds, [1] the distance to this system is roughly 520 light years. This is a single-lined spectroscopic binary system, [ 9 ] which means that only the absorption line features of one of the components can be distinguished.

  8. Kappa Centauri - Wikipedia

    en.wikipedia.org/wiki/Kappa_Centauri

    As of 2007, the secondary component was separated from the primary by 0.128 arcseconds at a position angle of 156°. It has about 68% of the mass of the primary. [ 9 ] This system is a proper motion member of the Upper Centaurus–Lupus sub-group in the Scorpius–Centaurus OB association , the nearest such co-moving association of massive ...

  9. Light-year - Wikipedia

    en.wikipedia.org/wiki/Light-year

    A contemporary German popular astronomical book also noticed that light-year is an odd name. [25] In 1868 an English journal labelled the light-year as a unit used by the Germans. [26] Eddington called the light-year an inconvenient and irrelevant unit, which had sometimes crept from popular use into technical investigations. [27]