DY Persei has alternative name(s) :- DY Per.
More details on objects' alternative names can be found at Star Names .
The location of the carbon star in the night sky 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 object is compared to the celestial equator and is expressed in degrees. For DY Persei, the location is 02 35 17.1273531147 and 2 35 17.1273531147 .
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 -0.83 miliarcseconds/year towards the north and 2.34 miliarcseconds/year east if we saw them in the horizon.
The Radial Velocity, that is the speed at which the star is moving away/towards the Sun is -38.00 km/s . When the value is negative then the star and the Sun are getting closer to one another, likewise, a positive number means that two stars are moving away. Its nothing to fear as the stars are so far apart, they won't collide in our life-time, if ever.
DY Persei has a spectral type of C-R4+ B. This means the star is a carbon red carbon star.
The Parallax of the star is given as 0.83 which gives a calculated distance to DY Persei of 3929.68 light years from the Earth or 1204.82 parsecs. It would take a spaceship travelling at the speed of light, 3929.68 years to get there. We don't have the technology or spaceship that can carry people over that distance yet.
The star is roughly 248,510,232.22 Astronomical Units from the Earth/Sun give or take a few. An Astronomical Unit is the distance between Earth and the Sun. The number of A.U. is the number of times that the star is from the Earth compared to the Sun.
The star is a eruptive R Coronae Borealis variable type which means that its size changes over time. The Variable Type is usually named after the first star of that type to be spotted.
|Primary / Proper / Traditional Name||DY Persei|
|Alternative Names||DY Per|
|Spectral Type||C-R4+ B|
|Constellation's Main Star||No|
|Multiple Star System||No / Unknown|
|Star Type||Carbon Star|
|Right Ascension (R.A.)||02 35 17.1273531147|
|Declination (Dec.)||2 35 17.1273531147|
|Distance from Earth||0.83 Parallax (milliarcseconds)|
|3929.68 Light Years|
|248,510,232.22 Astronomical Units|
|Proper Motion Dec.||-0.83 milliarcseconds/year|
|Proper Motion RA.||2.34 milliarcseconds/year|
|Radial Velocity||-38.00 km/s|
|Variable Star Class||Eruptive|
|Variable Star Type||R Coronae Borealis|
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