"Phad" redirects here. For scroll painting style, see
Phad painting.
Phecda , also called Gamma Ursae Majoris (γ Ursae Majoris, abbreviated Gamma UMa, γ UMa),[12][13] is a star in the constellation of Ursa Major. Since 1943, the spectrum of this star has served as one of the stable anchor points by which other stars are classified.[14] Based upon parallax measurements with the Hipparcos astrometry satellite,[15][16] it is located at distance of around 83.2 light-years (25.5 parsecs) from the Sun.[1]
Quick Facts Observation data Epoch J2000 Equinox J2000, Constellation ...
Phecda
Location of Phecda (circled) |
Observation data Epoch J2000 Equinox J2000 |
Constellation |
Ursa Major |
Right ascension |
11h 53m 49.84732s[1] |
Declination |
+53° 41′ 41.1350″[1] |
Apparent magnitude (V) |
2.438[2] |
Characteristics |
Spectral type |
A0 Ve + K2 V[3] |
U−B color index |
+0.008[2] |
B−V color index |
–0.013[2] |
Astrometry |
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|
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Radial velocity (Rv) | −12.6[4] km/s |
Proper motion (μ) | RA: +107.68[1] mas/yr Dec.: +11.01[1] mas/yr |
Parallax (π) | 39.21 ± 0.40 mas[1] |
Distance | 83.2 ± 0.8 ly (25.5 ± 0.3 pc) |
Absolute magnitude (MV) | 0.4[5] |
|
Orbit[5] |
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Period (P) | 20.5 ± 1 yr |
Semi-major axis (a) | 0.460″ |
Eccentricity (e) | 0.3 ± 0.3 |
Inclination (i) | 51 ± 15° |
Longitude of the node (Ω) | 6 ± 61° |
Periastron epoch (T) | B 1984.0 ± 2.0 |
Argument of periastron (ω) (secondary) | 185 ± 37° |
Details |
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γ UMa A |
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Mass | 2.94[3] M☉ |
Radius | 3.04 ± 0.08[6] R☉ |
Luminosity | 65.255[3] L☉ |
Surface gravity (log g) | 3.79[7] cgs |
Temperature | 9,355[7] K |
Rotational velocity (v sin i) | 178[8] km/s |
Age | 0.3[9] Gyr |
γ UMa B |
---|
Mass | 0.79[3] M☉ |
Luminosity | 0.397[3] L☉ |
Temperature | 4,780[3] K |
Other designations |
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Phad, Phecda, Phekda, Phegda, Phekha, Phacd, Fekda, [10] γ Ursae Majoris, γ UMa, Gamma UMa, 64 Ursae Majoris, BD+54 1475, FK5 447, GC 16268, HD 103287, HIP 58001, HR 4554, PPM 33292, SAO 28179. [11] |
Database references |
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SIMBAD | data |
Close
It is more familiar to most observers in the northern hemisphere as the lower-left star forming the bowl of the Big Dipper, together with Alpha Ursae Majoris (Dubhe, upper-right), Beta Ursae Majoris (Merak, lower-right) and Delta Ursae Majoris (Megrez, upper-left). Along with four other stars in this well-known asterism, Phecda forms a loose association of stars known as the Ursa Major moving group.[7] Like the other stars in the group, it is a main sequence star, as the Sun is, although somewhat hotter, brighter and larger.
Phecda is located in relatively close physical proximity to the prominent Mizar–Alcor star system. The two are separated by an estimated distance of 8.55 ly (2.62 pc); much closer than the two are from the Sun. The star Beta Ursae Majoris is separated from Gamma Ursae Majoris by 11.0 ly (3.4 pc).[17]
γ Ursae Majoris (Latinised to Gamma Ursae Majoris) is the star's Bayer designation.
It bore the traditional names Phecda or Phad, derived from the Arabic phrase فخذ الدب fakhth al-dubb ('thigh of the bear').[18] In 2016, the International Astronomical Union organized a Working Group on Star Names (WGSN)[19] to catalog and standardize proper names for stars. The WGSN's first bulletin of July 2016[20] included a table of the first two batches of names approved by the WGSN, which included Phecda for this star.
To the Hindus this star was known as Pulastya, one of the seven rishis.[10]
In Chinese, 北斗 (Běi Dǒu), meaning Northern Dipper, refers to an asterism equivalent to the Big Dipper. Consequently, the Chinese name for Gamma Ursae Majoris itself is 北斗三 (Běi Dǒu sān, English: the Third Star of Northern Dipper) and 天璣 (Tiān Jī, English: Star of Celestial Shining Pearl).[21]
Oja, T. (1986), "UBV photometry of stars whose positions are accurately known. III", Astronomy and Astrophysics Supplement Series, 65 (2): 405–4, Bibcode:1986A&AS...65..405O Wielen, R.; et al. (1999), "Sixth Catalogue of Fundamental Stars (FK6). Part I. Basic fundamental stars with direct solutions", Veröff. Astron. Rechen-Inst. Heidelb, 35 (35), Astronomisches Rechen-Institut Heidelberg: 1, Bibcode:1999VeARI..35....1W Royer, F.; Zorec, J.; Gómez, A. E. (February 2007), "Rotational velocities of A-type stars. III. Velocity distributions", Astronomy and Astrophysics, 463 (2): 671–682, arXiv:astro-ph/0610785, Bibcode:2007A&A...463..671R, doi:10.1051/0004-6361:20065224, S2CID 18475298 Kunitzsch, Paul; Smart, Tim (2006). A Dictionary of Modern star Names: A Short Guide to 254 Star Names and Their Derivations (2nd rev. ed.). Cambridge, Massachusetts: Sky Pub. ISBN 978-1-931559-44-7. Perryman, M. A. C.; Lindegren, L.; Kovalevsky, J.; et al. (July 1997), "The Hipparcos Catalogue", Astronomy and Astrophysics, 323: L49–L52, Bibcode:1997A&A...323L..49P