Lambda Cephei is a blue star that can be located in the constellation of Cepheus. Lambda Cephei is the brightest star in Cepheus based on the Hipparcos 2007 apparent magnitude. The star can be seen with the naked eye, that is, you don't need a telescope/binoculars to see it.
Lambda Cephei is the Bayer Classification for the star. The Id of the star in the Yale Bright Star Catalogue is HR8469. HIP109556 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD210839.
Lambda Cephei has alternative name(s), NSV 14069.
The location of the star in the galaxy is determined by the Right Ascension (R.A.) and Declination (Dec.), these are equivalent to the Longitude and Latitude on the Earth. The Right Ascension is how far expressed in time (hh:mm:ss) the star is along the celestial equator. If the R.A. is positive then its eastwards. The Declination is how far north or south the star is compared to the celestial equator and is expressed in degrees. For Lambda Cephei, the location is 22h 11m 30.58 and +59d 24` 52.3 .
All stars like planets orbit round a central spot, in the case of planets, its the central star such as the Sun. In the case of a star, its the galactic centre. The constellations that we see today will be different than they were 50,000 years ago or 50,000 years from now. Proper Motion details the movements of these stars and are measured in milliarcseconds. The star is moving -11.09 ± 0.16 miliarcseconds/year towards the north and -7.46 ± 0.22 miliarcseconds/year east if we saw them in the horizon.
Lambda Cephei has a spectral type of O6e. This means the star is a blue star. The star is 7564.00000000 Parsecs from the Galactic Centre or terms of Light Years is 24670.9953401600000000s. The star has a B-V Colour Index of 0.19 which means the star's temperature has been calculated using information from Morgans @ Uni.edu at being 7,480 Kelvin.
Lambda Cephei Radius has been calculated as being 27.49 times bigger than the Sun.The Sun's radius is 695,800km, therefore the star's radius is an estimated 19,125,759.98.km. However with the 2007 release of updated Hipparcos files, the radius is now calculated at being round 32.90. The figure is derived at by using the formula from SDSS and has been known to produce widely incorrect figures. The star's Iron Abundance is 0.03 with an error value of 9.99 Fe/H with the Sun has a value of 1 to put it into context.
Lambda Cephei has an apparent magnitude of 5.05 which is how bright we see the star from Earth. Apparent Magnitude is also known as Visual Magnitude. If you used the 1997 Parallax value, you would get an absolute magnitude of -3.47 If you used the 2007 Parallax value, you would get an absolute magnitude of -3.86. Magnitude, whether it be apparent/visual or absolute magnitude is measured by a number, the smaller the number, the brighter the Star is. Our own Sun is the brightest star and therefore has the lowest of all magnitudes, -26.74. A faint star will have a high number.
Using the original Hipparcos data that was released in 1997, the parallax to the star was given as 1.98 which gave the calculated distance to Lambda Cephei as 1647.29 light years away from Earth or 505.05 parsecs. It would take a spaceship travelling at the speed of light, 1647.29 years to get there. We don't have the technology or spaceship that can carry people over that distance yet.
In 2007, Hipparcos data was revised with a new parallax of 1.65 which put Lambda Cephei at a distance of 1976.75 light years or 606.06 parsecs. It should not be taken as though the star is moving closer or further away from us. It is purely that the distance was recalculated.
The star's Galacto-Centric Distance is 7,564.00 Parsecs or 24,671.00 Light Years. The Galacto-Centric Distance is the distance from the star to the Centre of the Galaxy which is Sagittarius A*. Lambda Cephei brightness ranges from a magnitude of 5.148 to a magnitude of 5.111 over its variable period. The smaller the magnitude, the brighter the star. Its variable/pulsating period lasts for 0.0 days (variability).
The source of the information if it has a Hip I.D. is from Simbad, the Hipparcos data library based at the University at Strasbourg, France. Hipparcos was a E.S.A. satellite operation launched in 1989 for four years. The items in red are values that I've calculated so they could well be wrong. Information regarding Metallicity and/or Mass is from the E.U. Exoplanets. The information was obtained as of 12th Feb 2017.
|Flamsteed Name||22 Cephei|
|Flamsteed Short Name||22 Cep|
|Short Name||NSV 14069|
|Bayer Designation||Lambda Cephei|
|Hipparcos Library I.D.||109556|
|Yale Bright Star Catalogue (HR) Id||8469|
|Bonner Durchmusterung||BD+58 2402|
|Henry Draper Designation||210839|
|Absolute Magnitude||-3.47 / -3.86|
|Visual / Apparent Magnitude||5.05|
|Naked Eye Visible||Yes - Magnitudes|
|Right Ascension (R.A.)||22h 11m 30.58|
|Declination (Dec.)||+59d 24` 52.3|
|Galactic Latitude||2.61 degrees|
|Galactic Longitude||103.83 degrees|
|1997 Distance from Earth||1.98 Parallax (milliarcseconds)|
|1647.29 Light Years|
|2007 Revised Distance from Earth||1.65 Parallax (milliarcseconds)|
|1976.75 Light Years|
|Galacto-Centric Distance||24,671.00 Light Years / 7,564.00 Parsecs|
|Proper Motion Dec.||-11.09 ± 0.16 milliarcseconds/year|
|Proper Motion RA.||-7.46 ± 0.22 milliarcseconds/year|
|Radial Velocity||-75.10 ± 0.90 km/s|
|Iron Abundance||0.03 ± 9.99 Fe/H|
|Mean Variability Period in Days||0.024|
|Variable Magnitude Range (Brighter - Dimmer)||5.111 - 5.148|
|Calculated Effective Temperature||7,480 Kelvin|