Universe Guide
AliensAliensConstellationsTelevision and Films ListFact ListGames ListWarcraftSearchTwitterFacebook


HR 239, HD4849, HIP3903

HR 239 is a blue giant star that can be located in the constellation of Phoenix. The star can be seen with the naked eye, that is, you don't need a telescope/binoculars to see it.

HR 239's Alternative Names

The Id of the star in the Yale Bright Star Catalogue is HR239. HIP3903 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD4849.

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

Location of HR 239

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 HR 239, the location is 00h 50m 03.76 and -43° 23` 41.8 .

Proper Motion of HR 239

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 6.24 ± 0.67 miliarcseconds/year towards the north and 14.92 ± 0.94 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 11.90000 km/s with an error of about 1.80 km/s .

HR 239 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 24.1400000 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 HR 239

HR 239 has a spectral type of A9/F0III. This means the star is a blue giant star. The star is 7384.00000000 Parsecs from the Galactic Centre or terms of Light Years is 24083.9013209600000000s. The star has a B-V Colour Index of 0.2 which means the star's temperature has been calculated using information from Morgans @ Uni.edu at being 7,767 Kelvin.

HR 239 Radius has been calculated as being 2.51 times bigger than the Sun.The Sun's radius is 695,800km, therefore the star's radius is an estimated 1,749,306.48.km. However with the 2007 release of updated Hipparcos files, the radius is now calculated at being round 2.82. The figure is derived at by using the formula from SDSS and has been known to produce widely incorrect figures.

HR 239 Apparent and Absolute Magnitudes

HR 239 has an apparent magnitude of 6.49 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 1.56 If you used the 2007 Parallax value, you would get an absolute magnitude of 1.31. 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 HR 239

Using the original Hipparcos data that was released in 1997, the parallax to the star was given as 10.31 which gave the calculated distance to HR 239 as 316.36 light years away from Earth or 96.99 parsecs. It would take a spaceship travelling at the speed of light, 316.36 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 9.21 which put HR 239 at a distance of 354.14 light years or 108.58 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 7,384.00 Parsecs or 24,083.90 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.

Hide Explanations.

HR 239 Facts

Visual Facts

Alternative NamesHD 4849, HIP 3903, HR 239
Star TypeGiant Star
GalaxyMilky Way
Absolute Magnitude1.56 / 1.31
Visual / Apparent Magnitude6.49
Naked Eye VisibleYes - Magnitudes
Right Ascension (R.A.)00h 50m 03.76
Declination (Dec.)-43° 23` 41.8
Galactic Latitude-73.73 degrees
Galactic Longitude303.82 degrees
1997 Distance from Earth10.31 Parallax (milliarcseconds)
 316.36 Light Years
 96.99 Parsecs
2007 Revised Distance from Earth9.21 Parallax (milliarcseconds)
 354.14 Light Years
 108.58 Parsecs
Galacto-Centric Distance24,083.90 Light Years / 7,384.00 Parsecs
Proper Motion Dec.6.24 ± 0.67 milliarcseconds/year
Proper Motion RA.14.92 ± 0.94 milliarcseconds/year
B-V Index0.20
Radial Velocity11.90 ± 1.80 km/s
Semi-Major Axis8409.00
Stellar Luminosity (Lsun)24.14
Spectral TypeA9/F0III
Colour(A) blue

Estimated Facts

Calculated Effective Temperature7,767 Kelvin

Sources and Links

SIMBAD SourceLink

Related Stars

Add a Comment

Email: (Optional)