Universe Guide


49 Herculis, HD152308, HIP82526

49 Herculis is a blue rotating star that can be located in the constellation of Hercules. The star can not be seen by the naked eye, you need a telescope to see it.

HIP82526 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD152308.

49 Herculis has alternative name(s), V823 Her.

Location of 49 Herculis

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 49 Herculis, the location is 16h 52m 04.84 and +14d58`27.1 .

Proper Motion of 49 Herculis

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 5.59 ± 0.26 miliarcseconds/year towards the north and 16.44 ± 0.43 miliarcseconds/year east if we saw them in the horizon.

Physical Properties (Colour, Temperature, Radius) of 49 Herculis

49 Herculis has a spectral type of B9.5p (Cr). This means the star is a blue star. The star is 7314.00000000 Parsecs from the Galactic Centre or terms of Light Years is 23855.5869801600000000s. The star has a B-V Colour Index of -0.03 which means the star's temperature has been calculated using information from Morgans @ Uni.edu at being 11,122 Kelvin.

49 Herculis Radius has been calculated as being 1.74 times bigger than the Sun.The Sun's radius is 695,800km, therefore the star's radius is an estimated 1,210,637.70.km. However with the 2007 release of updated Hipparcos files, the radius is now calculated at being round 1.56. The figure is derived at by using the formula from SDSS and has been known to produce widely incorrect figures.

49 Herculis Apparent and Absolute Magnitudes

49 Herculis has an apparent magnitude of 6.51 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 0.80 If you used the 2007 Parallax value, you would get an absolute magnitude of 1.04. 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 49 Herculis

Using the original Hipparcos data that was released in 1997, the parallax to the star was given as 7.21 which gave the calculated distance to 49 Herculis as 452.38 light years away from Earth or 138.70 parsecs. It would take a spaceship travelling at the speed of light, 452.38 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 8.06 which put 49 Herculis at a distance of 404.67 light years or 124.07 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 7,314.00 Parsecs or 23,855.59 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 49 Herculis

The star is a rotating Alpha2 Canum Venaticorum 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. 49 Herculis brightness ranges from a magnitude of 6.518 to a magnitude of 6.492 over its variable period. The smaller the magnitude, the brighter the star. Its variable/pulsating period lasts for 0.9 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.

49 Herculis Facts

Alternative Names

Traditional/Proper Name49 Herculis
Flamsteed Name49 Herculis
Flamsteed Short Name49 Her
Short NameV823 Her
Hipparcos Library I.D.82526
Bonner DurchmusterungBD+15 3066
Henry Draper Designation152308

Visual Facts

Star Type star
Absolute Magnitude0.80 / 1.04
Visual / Apparent Magnitude6.51
Naked Eye VisibleRequires a 7x50 Binoculars - Magnitudes
Right Ascension (R.A.)16h 52m 04.84
Declination (Dec.)+14d58`27.1
Galactic Latitude33.07 degrees
Galactic Longitude33.67 degrees
1997 Distance from Earth7.21 Parallax (milliarcseconds)
 452.38 Light Years
 138.70 Parsecs
2007 Revised Distance from Earth8.06 Parallax (milliarcseconds)
 404.67 Light Years
 124.07 Parsecs
Galacto-Centric Distance23,855.59 Light Years / 7,314.00 Parsecs
Proper Motion Dec.5.59 ± 0.26 milliarcseconds/year
Proper Motion RA.16.44 ± 0.43 milliarcseconds/year
B-V Index-0.03
Radial Velocity-22.80 ± 3.00 km/s
Spectral TypeB9.5p (Cr)
Colour(B) blue

Variable Star Details

Variable Star ClassRotating
Variable Star TypeAlpha2 Canum Venaticorum
Mean Variability Period in Days0.937
Variable Magnitude Range (Brighter - Dimmer)6.492 - 6.518

Estimated Facts

Calculated Effective Temperature11,122 Kelvin

Sources and Links

SIMBAD SourceLink

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