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  2. Right ascension - Wikipedia

    en.wikipedia.org/wiki/Right_ascension

    Over a precession cycle of 26,000 years, "fixed stars" that are far from the ecliptic poles increase in right ascension by 24h, or about 5.6' per century, whereas stars within 23.5° of an ecliptic pole undergo a net change of 0h.

  3. Equinox (celestial coordinates) - Wikipedia

    en.wikipedia.org/wiki/Equinox_(celestial...

    Since the right ascension and declination of stars are constantly changing due to precession, astronomers always specify these with reference to a particular equinox. Historically used Besselian equinoxes include B1875.0, B1900.0, B1925.0 and B1950.0.

  4. Regulus - Wikipedia

    en.wikipedia.org/wiki/Regulus

    Right ascension: 10 h 08 m 12.8/14 s [4] ... so as this cycle continues Venus will more definitely pass Regulus ... Regulus is the brightest star in the constellation ...

  5. Capella - Wikipedia

    en.wikipedia.org/wiki/Capella

    Right ascension: 05 h 17 m 23.943 s [7] Declination +45° 50′ 19.84 ... The Brightest Stars: Discovering the Universe through the Sky's Most Brilliant Stars. Wiley.

  6. Delta Cassiopeiae - Wikipedia

    en.wikipedia.org/wiki/Delta_Cassiopeiae

    δ Cassiopeiae (Latinised to Delta Cassiopeiae) is the star's Bayer designation.WDS J01258+6014A is its designation in the Washington Double Star Catalog.. It also bore the traditional names Ruchbah and Ksora; the former deriving from the Arabic word ركبة rukbah meaning "knee", [9] and the latter appeared in a 1951 publication, Atlas Coeli (Skalnate Pleso Atlas of the Heavens) by Czech ...

  7. Antares - Wikipedia

    en.wikipedia.org/wiki/Antares

    Lunar occultations of Antares are fairly common, depending on the 18.6-year cycle of the lunar nodes. The last cycle ended in 2010 and the next begins in 2023. Shown at right is a video of a reappearance event, clearly showing events for both components. Antares can also be occulted by the planets, e.g. Venus, but these events are rare.

  8. Rigel - Wikipedia

    en.wikipedia.org/wiki/Rigel

    Two stars in the system can be seen by large telescopes, and the brighter of the two is a spectroscopic binary. These three stars are all blue-white main-sequence stars, each three to four times as massive as the Sun. Rigel and the triple system orbit a common center of gravity with a period estimated to be 24,000 years. The inner stars of the ...

  9. Albireo - Wikipedia

    en.wikipedia.org/wiki/Albireo

    Albireo is the star in the head of the constellation of Cygnus (bottom). β Cygni (Latinised to Beta Cygni) is the system's Bayer designation. The brighter of the two components is designated β¹ Cygni or Beta Cygni A and the fainter β² Cygni or Beta Cygni B. The origin of the star system's traditional name Albireo is unclear.