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Lambda Coronae Borealis - HD142908 - HIP78012

Lambda Coronae Borealis is a blue to white subgiant star that can be located in the constellation of CoronaBorealis. Lambda Coronae Borealis is the Bayer Classification for the star. HIP78012 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD142908. Lambda Coronae Borealis has alternative name(s), 12 Coronae Borealis , 12 CrB.

Location of Lambda Coronae Borealis

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 Lambda Coronae Borealis, the location is 15h 55m 47.57 and +37d56`48.3 .

Proper Motion of Lambda Coronae Borealis

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 080.14 ± 000.19 towards the north and 029.28 ± 000.24 east if we saw them in the horizon.

Physical Properties (Colour, Temperature, Radius) of Lambda Coronae Borealis

Lambda Coronae Borealis has a spectral type of F0IV. This means the star is a blue to white subgiant star. The star has a B-V Colour Index of 0.35 which means the star's temperature has been calculated using information from Morgans @ Uni.edu at being 6,967 Kelvin.

Lambda Coronae Borealis has been calculated as 2.18 times bigger than the Sun.The Sun's radius is 695,800km, therefore the star's radius is an estimated 1,518,005.12.km.

Lambda Coronae Borealis Apparent and Absolute Magnitudes

Lambda Coronae Borealis has an apparent magnitude of 5.43 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 2.34 If you used the 2007 Parallax value, you would get an absolute magnitude of 2.34. 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 Lambda Coronae Borealis

Using the original Hipparcos data that was released in 1997, the parallax to the star was given as 24.12 which gave the calculated distance to Lambda Coronae Borealis as 135.23 light years away from Earth or 41.46 parsecs. It would take a spaceship travelling at the speed of light, 135.23 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 24.06 which put Lambda Coronae Borealis at a distance of 135.56 light years or 41.56 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.

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 Stellar Age, Metallicity or Mass is from the E.U. Exoplanets. The information was obtained as of 12th Feb 2017.

Lambda Coronae Borealis Facts

Alternative Names

Short Name12 CrB
Bayer DesignationLambda Coronae Borealis
Alternative Name(s)12 Coronae Borealis
Hipparcos Library I.D.78012
Bonner DurchmusterungBD+38 2712
Henry Draper Designation142908

Visual Facts

Star Typesubgiant star
Absolute Magnitude2.34 / 2.34
Apparent Magnitude5.43
Right Ascension (R.A.)15h 55m 47.57
Declination (Dec.)+37d56`48.3
1997 Distance from Earth24.12 Parallax (milliarcseconds)
 135.23 Light Years
 41.46 Parsecs
2007 Revised Distance from Earth24.06 Parallax (milliarcseconds)
 135.56 Light Years
 41.56 Parsecs
Proper Motion Dec.80.14 ± 0.19 milliarcseconds/year
Proper Motion RA.29.28 ± 0.24 milliarcseconds/year
B-V Index0.35
Spectral TypeF0IV
Colour(F) blue to white

Estimated Facts

Radius (x the Sun)2.18
Calculated Effective Temperature6,967 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
142908+38 2712.0A5.5000025.0000078.00000F2Yellow/White

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