DL Camelopardalis is a blue giant star that can be located in the constellation of Camelopardalis. The star can be seen with the naked eye, that is, you don't need a telescope/binoculars to see it.
The Id of the star in the Yale Bright Star Catalogue is HR1417. HIP21148 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD28446.
DL Camelopardalis has alternative name(s) :- , DL Cam.
Flamsteed designations are named after the creator, Sir John Flamsteed. Sir John numbered the stars in the constellation with a number and the latin name, this star's Flamsteed designation is 1 Camelopardalis with it shortened to 1 Cam.>
BD number is the number that the star was filed under in the Durchmusterung or Bonner Durchmusterung, a star catalogue that was put together by the Bonn Observatory between 1859 to 1903. The star's BD Number is BD+53 779.
More details on star alternative names can be found at Star Names.
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 DL Camelopardalis, the location is 04h 32m 01.84 and +53 ° 54` 39.0 .
DL Camelopardalis has a spectral type of B0III SB. This means the star is a blue giant star. The star has a B-V Colour Index of 0.11 which means the star's temperature has been calculated using information from Morgans @ Uni.edu at being 8,375 Kelvin. The figure is derived at by using the formula from SDSS and has been known to produce widely incorrect figures.
DL Camelopardalis has an apparent magnitude of 5.78 which is how bright we see the star from Earth. Apparent Magnitude is also known as Visual Magnitude. Using the supplied Parallax value, you would get an absolute magnitude of 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 -2.00 which gave the calculated distance to DL Camelopardalis as -1630.82 light years away from Earth or -500 parsecs. It would take a spaceship travelling at the speed of light, -1630.82 years to get there. We don't have the technology or spaceship that can carry people over that distance yet. DL Camelopardalis brightness ranges from a magnitude of 5.850 to a magnitude of 5.810 over its variable period. The smaller the magnitude, the brighter the star. Its variable/pulsating period lasts for 0.1 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.
|Alternative Names||HD 28446, HIP 21148, HR 1417, 1 Camelopardalis, 1 Cam, BD+53 779, DL Cam|
|Star Type||Giant Star|
|Visual / Apparent Magnitude||5.78|
|Naked Eye Visible||Yes - Magnitudes|
|Right Ascension (R.A.)||04h 32m 01.84|
|Declination (Dec.)||+53 ° 54` 39.0|
|Galactic Latitude||3.95 degrees|
|Galactic Longitude||151.91 degrees|
|Distance from Earth||-2.00 Parallax (milliarcseconds)|
|-1630.82 Light Years|
|Radial Velocity||-7.00 ± 4.30 km/s|
|Spectral Type||B0III SB|
|Mean Variability Period in Days||0.052|
|Variable Magnitude Range (Brighter - Dimmer)||5.810 - 5.850|
|Calculated Effective Temperature||8,375 Kelvin|
The star has been identified as being a multi-star system, one in which there is at least one star in close orbit to another star or two or more stars orbiting a central point. The stars may be of equal mass, unequal mass where one star is stronger than the other or be in groups orbiting a central point which doesn't necessarily have to be a star. More information can be found on my dedicated multiple star systems page. The source of the info is Simbad. The file is dated 2000 so any differences between this and any other source will be down to the actual source from where the information came from.
|Proper Motion mas/yr|
|H.D. Id||B.D. Id||Star Code||Magnitude||R.A.||Dec.||Spectrum||Colour||Year|