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HIP 25381, HD37380

HIP 25381 is a blue to white subgiant star that can be located in the constellation of Mensa. The description is based on the spectral class. The star can not be seen by the naked eye, you need a telescope to see it.

HIP 25381's Alternative Names

HIP25381 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD37380.

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

Location of HIP 25381

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 HIP 25381, the location is 05h 25m 49.06 and -79° 45` 45.7 .

Proper Motion of HIP 25381

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 32.62 ± 0.58 miliarcseconds/year towards the north and 12.40 ± 0.61 miliarcseconds/year east if we saw them in the horizon.

HIP 25381 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 13.69 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 HIP 25381

HIP 25381 has a spectral type of F8IV/V. This means the star is a blue to white subgiant star. The star is 7,334.00 Parsecs from the Galactic Centre or terms of Light Years is 23,920.82 s. The star has a B-V Colour Index of 0.58 which means the star's temperature has been calculated using information from Morgans @ Uni.edu at being 5,968 Kelvin.

HIP 25381 Radius has been calculated as being 3.23 times bigger than the Sun.The Sun's radius is 695,800km, therefore the star's radius is an estimated 2,247,548.10.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 3.49. The figure is derived at by using the formula from SDSS and has been known to produce widely incorrect figures.

HIP 25381 Apparent and Absolute Magnitudes

HIP 25381 has an apparent magnitude of 8.68 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 2.16 If you used the 2007 Parallax value, you would get an absolute magnitude of 1.99. 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 HIP 25381

Using the original Hipparcos data that was released in 1997, the parallax to the star was given as 4.96 which gave the calculated distance to HIP 25381 as 657.59 light years away from Earth or 201.61 parsecs. It would take a spaceship travelling at the speed of light, 657.59 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 4.60 which put HIP 25381 at a distance of 709.05 light years or 217.39 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 7,334.00 Parsecs or 23,920.82 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.

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HIP 25381 Facts

Visual Facts


Primary / Proper / Traditional NameHIP 25381
Alternative NamesHD 37380, HIP 25381
Spectral TypeF8IV/V
Multiple Star SystemNo / Unknown
Star TypeSubgiant Star
Colour blue to white
GalaxyMilky Way
ConstellationMensa
Absolute Magnitude2.16 / 1.99
Visual / Apparent Magnitude8.68
Naked Eye VisibleRequires a 7x50 Binoculars - Magnitudes
Right Ascension (R.A.)05h 25m 49.06
Declination (Dec.)-79° 45` 45.7
Galactic Latitude-30.43 degrees
Galactic Longitude291.87 degrees
1997 Distance from Earth4.96 Parallax (milliarcseconds)
 657.59 Light Years
 201.61 Parsecs
2007 Distance from Earth4.60 Parallax (milliarcseconds)
 709.05 Light Years
 217.39 Parsecs
Galacto-Centric Distance23,920.82 Light Years / 7,334.00 Parsecs
Proper Motion Dec.32.62 ± 0.58 milliarcseconds/year
Proper Motion RA.12.40 ± 0.61 milliarcseconds/year
B-V Index0.58
Stellar Luminosity (Lsun)13.69

Companions (Multi-Star and Exoplanets) Facts


Exoplanet CountNone/Unaware

Estimated Facts


Calculated Effective Temperature5,968 Kelvin

Sources and Links


SIMBAD SourceLink

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