Polaris | has declination +89 15 51 | |
has right ascension 2 31 50.5 | |
has period 3.97 days | |
has primary F8 Ib | |
has spectral type F7:Ib-IIv | |
has V magnitude 2.02 | |
is a part of Ursa Minor | |
has distance 330 light-years | |
has synonym HR 424 | |
has synonym Pole star | |
has synonym North Star | |
has synonym alpha UMi | |
has B-V magnitude 0.60 | |
has use The star that lies near the direction in the sky toward which the North Pole of the Earth points. | |
has definition A supergiant F8 Ib, F3 V visual binary, with an orbital period of thousands of years. The primary (a Cepheid with a pulsation period of 3.97 days) is itself a single-lined spectroscopic double with a period of 29.6 years. There are at least two more faint (12th mag) components of the system. | |
is an instance of Population I Cepheid | |
is an instance of F star | |
is an instance of supergiant | |
is an instance of naked eye star | |
is an instance of binary star | |
F star | has color yellow-white | |
has surface temperature 6000 to 7500 K | |
naked eye star | has been observed for many centuries | |
is usually part of asterism | |
is a part of celestial sphere | |
is a part of Milky Way | |
has apparent magnitude brighter than 5 | |
binary star | has number of stars 2 | |
has orbital period | |
Population I Cepheid | has absolute magnitude <Mv> = -0.5 to -6 | |
supergiant | has luminosity class I | |
star | has star surface temperature | |
has B magnitude | |
has U magnitude | |
has position on celestial sphere from the point of view of Earth | |
has parallax from the point of view of Earth's orbit | |
has proper motion | |
has radiation at surface which is diffused out from the hotter core | |
has energy source gravitational contraction and or fusion | |
has energy production which takes place primarily within the core | |
has surface density which depends on luminosity class | |
has age | |
has catalog star catalog | |
has material hydrogen, helium | |
has velocity determined from proper motion and radial velocity | |
has mass greater than 0.08 the sun's mass | |
star system | has abundance half the stars in the solar neighborhood are members of star systems | |
Population I star | has author Baade (1944) | |
is a part of disk | |
Cepheid | has prototype delta Cephei | |
celestial body | has spectra | |
physical object | has location or center of gravity | |
has angular momentum | |
has momentum | |
has temperature | |
has volume | |
has extent | |
variable | has name designated with - R, S, T, U, V, W, X, Y, or Z and the genitive of the latin constellation name
- RR, RS, RT, RU, RV, RW, RX, RY, or RZ and the genitive of the latin constellation name when the single letter designations are exhausted
- AA...AZ, BB...BZ, etc. (omitting J), which ends with QQ...QZ and the genitive of the latin constellation namewhen the RR...RZ designations are exhausted
- V 335, V 336, etc., when the double letter designations are exhausted
| |
has observational problem some difficulty in distinguishing between various kinds | |
has observable variation time scale within a period of decades | |
has light curve | |
has optical brightness variation 0.2 magnitudes or greater | |
has amplitude | |