Observation data Epoch J2000 Equinox | |
---|---|
Constellation | Ursa Minor |
Pronunciation | /pəˈlɛərɪs, -ˈlær-/; UK: /pəˈlɑːrɪs/[1] |
α UMi A | |
Right ascension | 02h 31m 49.09s[2] |
Declination | +89° 15′ 50.8″[2] |
Apparent magnitude (V) | 1.98[3] (1.86 – 2.13)[4] |
α UMi B | |
Right ascension | 02h 30m 41.63s[5] |
Declination | +89° 15′ 38.1″[5] |
Apparent magnitude (V) | 8.7[3] |
Characteristics | |
α UMi A | |
Spectral type | F7Ib + F6V[6] |
U−B color index | 0.38[3] |
B−V color index | 0.60[3] |
Variable type | Classical Cepheid[4] |
α UMi B | |
Spectral type | F3V[3] |
U−B color index | 0.01[7] |
B−V color index | 0.42[7] |
Variable type | suspected[4] |
Astrometry | |
Radial velocity (Rv) | −17[8] km/s |
Proper motion (μ) | RA: 198.8±0.20[2] mas/yr Dec.: −15±0.30[2] mas/yr |
Parallax (π) | 7.54±0.11 mas[2] |
Distance | 446.5±1.1 ly (136.90±0.34 pc)[9] |
Absolute magnitude (MV) | −3.6 (α UMi Aa)[3] 3.6 (α UMi Ab)[3] 3.1 (α UMi B)[3] |
Position (relative to α UMi Aa) | |
Component | α UMi Ab |
Epoch of observation | 2005.5880 |
Angular distance | 0.172″ |
Position angle | 231.4° |
Position (relative to α UMi Aa) | |
Component | α UMi B |
Epoch of observation | 2005.5880 |
Angular distance | 18.217″ |
Position angle | 230.540° |
Orbit[9] | |
Primary | α UMi Aa |
Companion | α UMi Ab |
Period (P) | 29.416±0.028 yr |
Semi-major axis (a) | 0.12955±0.00205" (≥2.90±0.03 AU[10]) |
Eccentricity (e) | 0.6354±0.0066 |
Inclination (i) | 127.57±1.22° |
Longitude of the node (Ω) | 201.28±1.18° |
Periastron epoch (T) | 2016.831±0.044 |
Argument of periastron (ω) (primary) | 304.54±0.84° |
Semi-amplitude (K1) (primary) | 3.762±0.025 km/s |
Details | |
α UMi Aa | |
Mass | 5.13±0.28[9] M☉ |
Radius | 46.27±0.42[9] R☉ |
Luminosity (bolometric) | 1,260[11] L☉ |
Surface gravity (log g) | 2.2[12] cgs |
Temperature | 6015[7] K |
Metallicity | 112% solar[13] |
Rotation | 119 days[6] |
Rotational velocity (v sin i) | 14[6] km/s |
Age | 45 - 67[14] Myr |
α UMi Ab | |
Mass | 1.316[9] M☉ |
Radius | 1.04[3] R☉ |
Luminosity (bolometric) | 3[3] L☉ |
Age | >500[14] Myr |
α UMi B | |
Mass | 1.39[3] M☉ |
Radius | 1.38[7] R☉ |
Luminosity (bolometric) | 3.9[7] L☉ |
Surface gravity (log g) | 4.3[7] cgs |
Temperature | 6900[7] K |
Rotational velocity (v sin i) | 110[7] km/s |
Age | 1.5[14] Gyr |
Other designations | |
Polaris, North Star, Cynosura, Alpha UMi, α UMi, ADS 1477, CCDM J02319+8915 | |
α UMi A: 1 Ursae Minoris, BD+88°8, FK5 907, GC 2243, HD 8890, HIP 11767, HR 424, SAO 308 | |
α UMi B: NSV 631, BD+88°7, GC 2226, SAO 305 | |
Database references | |
SIMBAD | α UMi A |
α UMi B |
Polaris is a star in the northern circumpolar constellation of Ursa Minor. It is designated α Ursae Minoris (Latinized to Alpha Ursae Minoris) and is commonly called the North Star or Pole Star. With an apparent magnitude that fluctuates around 1.98,[3] it is the brightest star in the constellation and is readily visible to the naked eye at night.[15] The position of the star lies less than 1° away from the north celestial pole, making it the current northern pole star. The stable position of the star in the Northern Sky makes it useful for navigation.[16]
As the closest Cepheid variable its distance is used as part of the cosmic distance ladder. The revised Hipparcos stellar parallax gives a distance to Polaris of about 433 light-years (133 parsecs), while the successor mission Gaia gives a distance of about 448 light-years (137 parsecs). Calculations by other methods vary widely.
Although appearing to the naked eye as a single point of light, Polaris is a triple star system, composed of the primary, a yellow supergiant designated Polaris Aa, in orbit with a smaller companion, Polaris Ab; the pair is in a wider orbit with Polaris B. The outer pair AB were discovered in August 1779 by William Herschel, where the 'A' refers to what is now known to be the Aa/Ab pair.
hipparcos2
was invoked but never defined (see the help page).
Gaia_DR3
was invoked but never defined (see the help page).
evans2024
was invoked but never defined (see the help page).
Anderson2019
was invoked but never defined (see the help page).
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