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 |  |