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Nu2 Bootis, 53 Bootis, HD138629, HIP76041, HR5774

Nu2 Bootis is a blue main sequence dwarf star that can be located in the constellation of Bootes. Nu2 Bootis is the brightest star in Bootes based on the Hipparcos 2007 apparent magnitude. The star can be seen with the naked eye, that is, you don't need a telescope/binoculars to see it.

Nu2 Bootis is the Bayer Classification for the star. The Id of the star in the Yale Bright Star Catalogue is HR5774. HIP76041 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD138629.

Location of Nu2 Bootis

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 Nu2 Bootis, the location is 15h 31m 46.99 and +40d 53` 57.7 .

Proper Motion of Nu2 Bootis

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 -13.00 ± 0.60 miliarcseconds/year towards the north and -13.71 ± 0.77 miliarcseconds/year east if we saw them in the horizon.

Nu2 Bootis 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 11.0000000 that I have given is based on the Spectral Types page that I have found on the Internet. You might find a different figure, one that may have been calculated rather than generalised that I have done. The figure is always the amount times the luminosity of the Sun. It is an imprecise figure because of a number of factors including but not limited to whether the star is a variable star and distance.

Physical Properties (Colour, Temperature, Radius) of Nu2 Bootis

Nu2 Bootis has a spectral type of A5V. This means the star is a blue main sequence dwarf star. The star is 7370.00000000 Parsecs from the Galactic Centre or terms of Light Years is 24038.2384528000000000s. The star has a B-V Colour Index of 0.08 which means the star's temperature has been calculated using information from Morgans @ Uni.edu at being 8,626 Kelvin.

Nu2 Bootis Radius has been calculated as being 5.56 times bigger than the Sun.The Sun's radius is 695,800km, therefore the star's radius is an estimated 3,870,570.74.km. However with the 2007 release of updated Hipparcos files, the radius is now calculated at being round 5.03. The figure is derived at by using the formula from SDSS and has been known to produce widely incorrect figures.

Nu2 Bootis Apparent and Absolute Magnitudes

Nu2 Bootis has an apparent magnitude of 4.98 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 -0.62 If you used the 2007 Parallax value, you would get an absolute magnitude of -0.40. 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 Nu2 Bootis

Using the original Hipparcos data that was released in 1997, the parallax to the star was given as 7.59 which gave the calculated distance to Nu2 Bootis as 429.73 light years away from Earth or 131.75 parsecs. It would take a spaceship travelling at the speed of light, 429.73 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 8.40 which put Nu2 Bootis at a distance of 388.29 light years or 119.05 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 7,370.00 Parsecs or 24,038.24 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.

Nu2 Bootis Facts

Alternative Names

Flamsteed Name53 Bootis
Flamsteed Short Name53 Boo
Bayer DesignationNu2 Bootis
Hipparcos Library I.D.76041
Yale Bright Star Catalogue (HR) Id5774
Bonner DurchmusterungBD+41 2611
Henry Draper Designation138629

Visual Facts

Star Typemain sequence dwarf star
Absolute Magnitude-0.62 / -0.40
Visual / Apparent Magnitude4.98
Naked Eye VisibleYes - Magnitudes
Right Ascension (R.A.)15h 31m 46.99
Declination (Dec.)+40d 53` 57.7
Galactic Latitude54.41 degrees
Galactic Longitude66.17 degrees
1997 Distance from Earth7.59 Parallax (milliarcseconds)
 429.73 Light Years
 131.75 Parsecs
2007 Revised Distance from Earth8.40 Parallax (milliarcseconds)
 388.29 Light Years
 119.05 Parsecs
Galacto-Centric Distance24,038.24 Light Years / 7,370.00 Parsecs
Proper Motion Dec.-13.00 ± 0.60 milliarcseconds/year
Proper Motion RA.-13.71 ± 0.77 milliarcseconds/year
B-V Index0.08
Radial Velocity-16.60 ± 3.70 km/s
Spectral TypeA5V
Colour(A) blue

Estimated Facts

Luminosity (x the Sun)11.0000000
Calculated Effective Temperature8,626 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
138629+41 2611.0A5.80000-26.00000-16.00000A2White

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