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  2. Stellar kinematics - Wikipedia

    en.wikipedia.org/wiki/Stellar_kinematics

    Barnard's Star, showing position every 5 years in the period 1985–2005.Barnard's Star is the star with the highest proper motion. [1]In astronomy, stellar kinematics is the observational study or measurement of the kinematics or motions of stars through space.

  3. Hubble's law - Wikipedia

    en.wikipedia.org/wiki/Hubble's_law

    The result assumes Ω m = 0.3, Ω Λ = 0.7 and a sound horizon of 149.3 Mpc, a value taken from Anderson et al. (2014). [101] 2020-09-29 67.6 +4.3 −4.2: S. Mukherjee et al. [102] Gravitational waves, assuming that the transient ZTF19abanrh found by the Zwicky Transient Facility is the optical counterpart to GW190521. Independent of distance ...

  4. 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.

  5. Olbers's paradox - Wikipedia

    en.wikipedia.org/wiki/Olbers's_Paradox

    If the universe is homogeneous at a large scale, then there would be four times as many stars in a second shell between 2,000,000,000 and 2,000,000,001 light years away. However, the second shell is twice as far away, so each star in it would appear one quarter as bright as the stars in the first shell.

  6. Cepheid variable - Wikipedia

    en.wikipedia.org/wiki/Cepheid_variable

    (Between two such observations 2 AU apart, a star at a distance of 7500 light-years = 2300 parsecs would appear to move an angle of 2 / 2300 arc-seconds = 2 x 10-7 degrees, the resolution limit of the available telescopes.) [55]

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  8. Stellar parallax - Wikipedia

    en.wikipedia.org/wiki/Stellar_parallax

    Stellar parallax is most often measured using annual parallax, defined as the difference in position of a star as seen from Earth and Sun, i.e. the angle subtended at a star by the mean radius of Earth's orbit around the Sun. The parsec (3.26 light-years) is defined as the distance for which the annual parallax is 1 arcsecond. Annual parallax ...

  9. Breaking down the 1.3 seconds of mayhem before every NFL ...

    www.aol.com/news/breaking-down-1-3-seconds...

    This has been a weird season for NFL kickers. So far, they have made about 72% of their tries from 50 or more yards, a big improvement from 58% five years ago.