ER Vulpeculae is a white to yellow eclipsing giant star that can be located in the constellation of Vulpecula. The star can not be seen by the naked eye, you need a telescope to see it. The star has an estimated age of 8.70 Billion of Years but could be as young as 8.00 to 9.40 according to Hipparcos.
HIP103833 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD200391.
ER Vulpeculae has alternative name(s), ER_Vul.
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 ER Vulpeculae, the location is 21h 02m 25.85 and +27d48`26.4 .
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 5.88 ± 0.40 miliarcseconds/year towards the north and 87.95 ± 0.60 miliarcseconds/year east if we saw them in the horizon.
ER Vulpeculae has a spectral type of G0IIIvar. This means the star is a white to yellow giant star. The star is 7386.00000000 Parsecs from the Galactic Centre or terms of Light Years is 24090.4245878400000000s. The star has a B-V Colour Index of 0.61 which means the star's temperature has been calculated using information from Morgans @ Uni.edu at being 5,859 Kelvin.
ER Vulpeculae Radius has been calculated as being 1.55 times bigger than the Sun.The Sun's radius is 695,800km, therefore the star's radius is an estimated 1,075,729.64.km. However with the 2007 release of updated Hipparcos files, the radius is now calculated at being round 1.61. 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 -0.20 with an error value of 9.99 Fe/H with the Sun has a value of 1 to put it into context.
The stars age according to Hipparcos data files put the star at an age of about 8.70 Billion years old but could be between 8.00 and 9.40 Billion years old. In comparison, the Sun's age is about 4.6 Billion Years Old.
ER Vulpeculae has an apparent magnitude of 7.33 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 3.84 If you used the 2007 Parallax value, you would get an absolute magnitude of 3.75. 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 20.06 which gave the calculated distance to ER Vulpeculae as 162.59 light years away from Earth or 49.85 parsecs. It would take a spaceship travelling at the speed of light, 162.59 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 19.23 which put ER Vulpeculae at a distance of 169.61 light years or 52.00 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 7,386.00 Parsecs or 24,090.42 Light Years. The Galacto-Centric Distance is the distance from the star to the Centre of the Galaxy which is Sagittarius A*.
The star is a eclipsing W Ursae Majoris/RS Canum Venaticorum-type binary systems (subtype) 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. ER Vulpeculae brightness ranges from a magnitude of 8.000 to a magnitude of 7.000 over its variable period. The smaller the magnitude, the brighter the star. Its variable/pulsating period lasts for 1.0 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.
|Traditional/Proper Name||ER Vulpeculae|
|Short Name||ER Vul|
|Hipparcos Library I.D.||103833|
|Bonner Durchmusterung||BDD+27 3952|
|Henry Draper Designation||200391|
|Star Type||giant star|
|Age||8.70 Billion Years Old|
|Age Range||8.00 - 9.40 Billion Years Old|
|Absolute Magnitude||3.84 / 3.75|
|Visual / Apparent Magnitude||7.33|
|Naked Eye Visible||Requires a 7x50 Binoculars - Ref: Wiki|
|Right Ascension (R.A.)||21h 02m 25.85|
|Galactic Latitude||-12.31 degrees|
|Galactic Longitude||73.34 degrees|
|1997 Distance from Earth||20.06 Parallax (milliarcseconds)|
|162.59 Light Years|
|2007 Revised Distance from Earth||19.23 Parallax (milliarcseconds)|
|169.61 Light Years|
|Galacto-Centric Distance||24,090.42 Light Years / 7,386.00 Parsecs|
|Proper Motion Dec.||5.88 ± 0.40 milliarcseconds/year|
|Proper Motion RA.||87.95 ± 0.60 milliarcseconds/year|
|Radial Velocity||-24.60 ± 0.50 km/s|
|Iron Abundance||-0.20 ± 9.99 Fe/H|
|Colour||(G) White to Yellow|
|Variable Star Class||Eclipsing|
|Variable Star Type||W Ursae Majoris/RS Canum Venaticorum-type binary systems (subtype)|
|Mean Variability Period in Days||1.000|
|Variable Magnitude Range (Brighter - Dimmer)||7.000 - 8.000|
|Calculated Effective Temperature||5,859 Kelvin|