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  2. 20 Leonis Minoris - Wikipedia

    en.wikipedia.org/wiki/20_Leonis_Minoris

    0.967 ± 0.010 [8] MRadius: ... The two stars are currently separated by 14.5 arc seconds, corresponding to a projected separation of 2016 ...

  3. Parsec - Wikipedia

    en.wikipedia.org/wiki/Parsec

    By the 2015 definition, 1 au of arc length subtends an angle of 1″ at the center of the circle of radius 1 pc. That is, 1 pc = 1 au/tan(1″) ≈ 206,264.8 au by definition. [9] Converting from degree/minute/second units to radians,

  4. Mu Leonis - Wikipedia

    en.wikipedia.org/wiki/Mu_Leonis

    1.5 ± 0.1 [7] MRadius: ... Based upon an annual parallax shift of 0.02628 arc seconds as measured by the Hipparcos satellite, [1] this system is 124 light-years ...

  5. Surface brightness - Wikipedia

    en.wikipedia.org/wiki/Surface_brightness

    A truly dark sky has a surface brightness of 2 × 10 −4 cd m −2 or 21.8 mag arcsec −2. [9] [clarification needed] The peak surface brightness of the central region of the Orion Nebula is about 17 Mag/arcsec 2 (about 14 milli nits) and the outer bluish glow has a peak surface brightness of 21.3 Mag/arcsec 2 (about 0.27 millinits). [10]

  6. AT Microscopii - Wikipedia

    en.wikipedia.org/wiki/AT_Microscopii

    Position measurements of the pair made with the Hipparcos spacecraft show an annual parallax shift of 0.0935 seconds of arc, which is equivalent to a distance of about 35 ly (11 pc) from the Sun. [2] It is a binary star system with an angular separation of 4.0 arcseconds. [12]

  7. 11 Cephei - Wikipedia

    en.wikipedia.org/wiki/11_Cephei

    The star has a relatively high proper motion, traversing the celestial sphere at the rate of 0.153 arc seconds per annum. [9] It is moving closer to the Earth with a heliocentric radial velocity of −38 km/s. [2] This is an aging giant star with a stellar classification of K0.5 III, [4] having exhausted the hydrogen at its core and expanded.

  8. Lalande 21185 - Wikipedia

    en.wikipedia.org/wiki/Lalande_21185

    The second mark shows each's distance from Sol, with the concentric circles indicating the distance in steps of one ly. Lalande 21185 is a typical type-M main-sequence star with about 39% of the mass and radius of the Sun. It is also much cooler than the Sun with a surface temperature of 3,550 K.

  9. Groombridge 34 - Wikipedia

    en.wikipedia.org/wiki/Groombridge_34

    The star system has a relatively high proper motion of 2.9 arc seconds per year, [13] and is moving away from the Solar System at a velocity of 11.6 km/s. [6] It achieved perihelion some 15,000 years ago when it came within 11 ly (3.5 pc) of the Sun. [ 13 ]