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Epsilon Lyrae, Epsilon1 Lyrae, 4 Lyrae, HD173582, HIP91919, HR7051

Epsilon Lyrae (Epsilon1 Lyrae) is a blue to white main sequence dwarf star that can be located in the constellation of Lyra. Epsilon Lyrae is the brightest star in Lyra 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.

Epsilon1 Lyrae is the Bayer Classification for the star. The Id of the star in the Yale Bright Star Catalogue is HR7051. HIP91919 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD173582.

Epsilon Lyrae is a double star, the primary one being this one. This page details the star that is better known as Epsilon1 Lyrae with the other is known as Epsilon2 Lyrae. Unlike other mutli-star systems, both components of the star system were studied by the Hipparcos satellite which is where are there two pages for the star.

Location of Epsilon Lyrae

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 Epsilon Lyrae, the location is 18h 44m 20.34 and +39d 40` 11.9 .

Proper Motion of Epsilon Lyrae

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 61.39 ± 0.61 miliarcseconds/year towards the north and 11.09 ± 0.78 miliarcseconds/year east if we saw them in the horizon.

Physical Properties (Colour, Temperature, Radius) of Epsilon Lyrae

Epsilon Lyrae has a spectral type of F1V. This means the star is a blue to white main sequence dwarf star. The star is 7383.00000000 Parsecs from the Galactic Centre or terms of Light Years is 24080.6396875200000000s. The star has a B-V Colour Index of 0.17 which means the star's temperature has been calculated using information from Morgans @ Uni.edu at being 7,952 Kelvin.

Epsilon Lyrae Radius has been calculated as being 2.84 times bigger than the Sun.The Sun's radius is 695,800km, therefore the star's radius is an estimated 1,978,897.98.km. However with the 2007 release of updated Hipparcos files, the radius is now calculated at being round 2.86. The figure is derived at by using the formula from SDSS and has been known to produce widely incorrect figures.

Epsilon Lyrae Apparent and Absolute Magnitudes

Epsilon Lyrae has an apparent magnitude of 4.67 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 1.19 If you used the 2007 Parallax value, you would get an absolute magnitude of 1.18. 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 Epsilon Lyrae

Using the original Hipparcos data that was released in 1997, the parallax to the star was given as 20.10 which gave the calculated distance to Epsilon Lyrae as 162.27 light years away from Earth or 49.75 parsecs. It would take a spaceship travelling at the speed of light, 162.27 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 20.09 which put Epsilon Lyrae at a distance of 162.35 light years or 49.78 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 7,383.00 Parsecs or 24,080.64 Light Years. The Galacto-Centric Distance is the distance from the star to the Centre of the Galaxy which is Sagittarius A*.

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.

Epsilon Lyrae Facts

Alternative Names

Traditional/Proper NameEpsilon Lyrae
Flamsteed Name4 Lyrae
Flamsteed Short Name4 Lyr
Bayer DesignationEpsilon1 Lyrae
Hipparcos Library I.D.91919
Yale Bright Star Catalogue (HR) Id7051
Bonner DurchmusterungBD+39 3509
Henry Draper Designation173582

Visual Facts

Star Typemain sequence dwarf star
Absolute Magnitude1.19 / 1.18
Visual / Apparent Magnitude4.67
Naked Eye VisibleYes - Magnitudes
Right Ascension (R.A.)18h 44m 20.34
Declination (Dec.)+39d 40` 11.9
Galactic Latitude18.20 degrees
Galactic Longitude68.85 degrees
1997 Distance from Earth20.10 Parallax (milliarcseconds)
 162.27 Light Years
 49.75 Parsecs
2007 Revised Distance from Earth20.09 Parallax (milliarcseconds)
 162.35 Light Years
 49.78 Parsecs
Galacto-Centric Distance24,080.64 Light Years / 7,383.00 Parsecs
Proper Motion Dec.61.39 ± 0.61 milliarcseconds/year
Proper Motion RA.11.09 ± 0.78 milliarcseconds/year
B-V Index0.17
Radial Velocity-31.20 ± 1.70 km/s
Spectral TypeF1V
Associated / Clustered StarsEpsilon2 Lyrae
Colour(F) blue to white

Estimated Facts

Calculated Effective Temperature7,952 Kelvin

Sources and Links

SIMBAD SourceLink

Related Stars

Multi-Star System

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. IdB.D. IdStar CodeMagnitudeR.A.Dec.SpectrumColourYear
173582+39 3509.0A5.1000012.0000060.00000A3White

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