Beta Ursae Minoris

Beta Ursae Minoris
Observation data
Epoch J2000      Equinox J2000
Constellation Ursa Minor
Right ascension 14h 50m 42.3s
Declination +74° 09′ 20″
Apparent magnitude (V) 2.07[1]
Characteristics
Spectral type K4 III[1]
U−B color index 1.77
B−V color index 1.47[1]
Variable type ?
Astrometry
Radial velocity (Rv) +16.8 km/s
Proper motion (μ) RA: -32.29 mas/yr
Dec.: 11.91 mas/yr
Parallax (π) 25.79 ± 0.52 mas
Distance 126 ± 3 ly
(38.8 ± 0.8 pc)
Absolute magnitude (MV) -0.88
Details
Mass 4.4[1] M
Radius 41 R
Luminosity 500 L
Temperature 4,000 K
Metallicity ?
Rotation ~17 km/s.
Age ? years
Other designations
Kochab, Kocab, Kochah, 7 Ursae Minoris, Al Kaukab al Shamaliyy, HR 5563, BD +74 595, HD 131873, GCTP 3373.00, SAO 8102, FK5 550, HIP 72607.

Beta Ursae Minoris (β UMi, β Ursae Minoris) is the brightest star in the bowl of the "Little Dipper" (which is part of the constellation Ursa Minor), and only slightly fainter than Polaris, the northern pole star and brightest star in Ursa Minor. It has the traditional name Kochab. Kochab's magnitude is 2.07.[1] It is 16 degrees from Polaris. The star is an orange giant and is 126.4 ± 2.5 light years from Earth.[1] It is 130 times more luminous than the Sun. Kochab has a surface temperature of approximately 4,000 K.

Kochab and its neighbor Pherkad are both naked eye stars and are sometimes referred to as the "Guardians of the Pole". They served as twin pole stars, Earth's North pole stars, from 1500 BC until 500 AD. Neither star was as proximitous to the pole as Polaris is now. Due to precession of the equinoxes, the previous holder of the title was Thuban, and the next was the present-day Polaris. This succession of pole stars is a result of earth's precessional motion.

The origin of the name Kochab is unclear. It comes from the Hebrew word for star, "kokhav"[2], כוכב. It appears to be cognate with Arabic الكوكب al-kawkab "the star", short for الكوكب الشمالي al-kawkab al-šamāliyy "the north star" (lit. heavenly body), named when it was still the pole star.

In Chinese, 北極 (Běi Jí), meaning North Pole, refers to an asterism consisting of β Ursae Minoris, γ Ursae Minoris, 5 Ursae Minoris, 4 Ursae Minoris and Σ 1694.[3] Consequently, β Ursae Minoris itself is known as 北極二 (Běi Jí èr, English: the Second Star of North Pole.),[4] representing (), meaning Emperor.[5]

References

  1. ^ a b c d e f eSky. "Kochab (Beta Ursae Minoris)". http://www.glyphweb.com/esky/stars/kochab.html. Retrieved 2008-02-21. 
  2. ^ "Star in Proto-Semitic language". http://en.wiktionary.org/wiki/Appendix:Proto-Semitic/kabkab-. Retrieved 15 September 2011. 
  3. ^ (Chinese) 中國星座神話, written by 陳久金. Published by 台灣書房出版有限公司, 2005, ISBN 978-986-7332-25-7.
  4. ^ (Chinese)http://zh.wikipedia.org/wiki/%E5%8C%97%E6%A5%B5_%28%E6%98%9F%E5%AE%98%29
  5. ^ (Chinese) 香港太空館 - 研究資源 - 亮星中英對照表, Hong Kong Space Museum. Accessed on line November 23, 2010.

Mythology: Bx Times Reporter, New York http://www.webspawner.com/users/cosmic/

Preceded by
Thuban
Pole Star
1900 BC500
Succeeded by
Polaris

Coordinates: 14h 50m 42.3s, +74° 09′ 20″