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42 Persei, HD23848, HIP17886, HR1177

42 Persei is a blue eclipsing binary system main sequence dwarf star that can be located in the constellation of Perseus. The description is based on the spectral class. The star can be seen with the naked eye, that is, you don't need a telescope/binoculars to see it.

42 Persei's Alternative Names

The Id of the star in the Yale Bright Star Catalogue is HR1177. HIP17886 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD23848.

42 Persei has alternative name(s) :- , V467 Per.

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 42 Persei with it shortened to 42 Per.

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+32 667.

More details on star alternative names can be found at Star Names .

Location of 42 Persei

The location of the 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 star is compared to the celestial equator and is expressed in degrees. For 42 Persei, the location is 03h 49m 32.70 and +33° 05` 29.0 .

Proper Motion of 42 Persei

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 -1.47 ± 0.41 miliarcseconds/year towards the north and -18.63 ± 0.70 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 us is -12.40000 km/s with an error of about 1.70 km/s .

42 Persei Luminosity

Luminosity is the amount of energy that a star pumps out and its relative to the amount that our star, the Sun gives out. The figure of 52.89 that I have given is based on the value in the Simbad Hipparcos Extended Catalogue at the University of Strasbourg from 2012.

Physical Properties (Colour, Temperature) of 42 Persei

42 Persei has a spectral type of A3V. This means the star is a blue main sequence dwarf star. The star is 7,474.00 Parsecs from the Galactic Centre or terms of Light Years is 24,377.45 s. The star has a B-V Colour Index of 0.05 which means the star's temperature has been calculated using information from Morgans @ Uni.edu at being 8,917 Kelvin.

42 Persei Radius has been calculated as being 3.35 times bigger than the Sun.The Sun's radius is 695,800km, therefore the star's radius is an estimated 2,327,806.94.km. If you need the diameter of the star, you just need to multiple the radius by 2. However with the 2007 release of updated Hipparcos files, the radius is now calculated at being round 3.02. The figure is derived at by using the formula from SDSS and has been known to produce widely incorrect figures.

42 Persei Apparent and Absolute Magnitudes

42 Persei has an apparent magnitude of 5.14 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 0.34 If you used the 2007 Parallax value, you would get an absolute magnitude of 0.56. 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.

Distance to 42 Persei

Using the original Hipparcos data that was released in 1997, the parallax to the star was given as 10.96 which gave the calculated distance to 42 Persei as 297.59 light years away from Earth or 91.24 parsecs. It would take a spaceship travelling at the speed of light, 297.59 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 12.15 which put 42 Persei at a distance of 268.45 light years or 82.30 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 7,474.00 Parsecs or 24,377.45 Light Years. The Galacto-Centric Distance is the distance from the star to the Centre of the Galaxy which is Sagittarius A*.

Variable Type of 42 Persei

The star is a eclipsing binary system Beta Lyrae (Sheliak) 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. 42 Persei brightness ranges from a magnitude of 5.206 to a magnitude of 5.149 over its variable period. The smaller the magnitude, the brighter the star. Its variable/pulsating period lasts for 1.8 days (variability).

Source of Information

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.

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42 Persei Facts

Visual Facts

Primary / Proper / Traditional Name42 Persei
Alternative NamesN Per, HD 23848, HIP 17886, HR 1177, 42 Per, BD+32 667, V467 Per
Spectral TypeA3V
Multiple Star SystemNo / Unknown
Star Type main sequence Dwarf Star
Colour blue
GalaxyMilky Way
Absolute Magnitude0.34 / 0.56
Visual / Apparent Magnitude5.14
Naked Eye VisibleYes - Magnitudes
Right Ascension (R.A.)03h 49m 32.70
Declination (Dec.)+33° 05` 29.0
Galactic Latitude-16.42 degrees
Galactic Longitude160.70 degrees
1997 Distance from Earth10.96 Parallax (milliarcseconds)
 297.59 Light Years
 91.24 Parsecs
2007 Distance from Earth12.15 Parallax (milliarcseconds)
 268.45 Light Years
 82.30 Parsecs
Galacto-Centric Distance24,377.45 Light Years / 7,474.00 Parsecs
Proper Motion Dec.-1.47 ± 0.41 milliarcseconds/year
Proper Motion RA.-18.63 ± 0.70 milliarcseconds/year
B-V Index0.05
Radial Velocity-12.40 ± 1.70 km/s
Semi-Major Axis9000.00
Stellar Luminosity (Lsun)52.89

Companions (Multi-Star and Exoplanets) Facts

Exoplanet CountNone/Unaware

Variable Star Details

Variable Star ClassEclipsing binary system
Variable Star TypeBeta Lyrae (Sheliak)
Mean Variability Period in Days1.765
Variable Magnitude Range (Brighter - Dimmer)5.149 - 5.206

Estimated Facts

Calculated Effective Temperature8,917 Kelvin

Sources and Links

SIMBAD SourceLink

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