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HIP 64532, HD115043

HIP 64532 is a white to yellow main sequence dwarf star that can be located in the constellation of Ursa Major. The description is based on the spectral class. HIP 64532 is not part of the constellation but is within the borders of the constellation.

The star can not be seen by the naked eye, you need a telescope to see it. The star has an estimated age of 5.60 Billion of Years but could be as young as 1.20 to 9.80 according to Hipparcos.

HIP 64532's Alternative Names

HIP64532 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD115043. The Gliese ID of the star is GL 503.2. The star was part of the original catalogue devised by German Astronomer Wilheim Gliese of stars located within 20 parsecs of Earth. Star Names

BD number is the number that the star was filed under in the Durchmusterung or Bonner Durchmusterung, a star catalogue that was put together by the Bonn Observatory between 1859 to 1903. The star's BD Number is BD+57 1425.

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

Location of HIP 64532

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 64532, the location is 13h 13m 36.89 and +56° 42` 29.9 .

Radial Velocity and Proper Motion of HIP 64532

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 -18.02 ± 0.34 miliarcseconds/year towards the north and 111.91 ± 0.41 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 the Sun is -8.70 km/s with an error of about 0.20 km/s . When the value is negative then the star and the Sun are getting closer to one another, likewise, a positive number means that two stars are moving away. Its nothing to fear as the stars are so far apart, they won't collide in our life-time, if ever.

HIP 64532 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 1.13 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, Age) of HIP 64532

HIP 64532 has a spectral type of G1V. This means the star is a white to yellow main sequence dwarf star. The star is 7,406.00 Parsecs from the Galactic Centre or terms of Light Years is 24,155.66 s. The star has a B-V Colour Index of 0.6 which means the star's temperature has been calculated using information from Morgans @ Uni.edu at being 5,895 Kelvin.

HIP 64532 Radius has been calculated as being 1.00 times bigger than the Sun.The Sun's radius is 695,800km, therefore the star's radius is an estimated 692,426.02.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 0.98. The figure is derived at by using the formula from SDSS and has been known to produce widely incorrect figures. The star's Iron Abundance is 0.05 with an error value of 0.04 Fe/H with the Sun has a value of 1 to put it into context.

The stars age according to Hipparcos data files put the star at an age of about 5.60 Billion years old but could be between 1.20 and 9.80 Billion years old. In comparison, the Sun's age is about 4.6 Billion Years Old.

HIP 64532 Apparent and Absolute Magnitudes

HIP 64532 has an apparent magnitude of 6.82 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 4.77 If you used the 2007 Parallax value, you would get an absolute magnitude of 4.80. 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 64532

Using the original Hipparcos data that was released in 1997, the parallax to the star was given as 38.92 which gave the calculated distance to HIP 64532 as 83.80 light years away from Earth or 25.69 parsecs. It would take a spaceship travelling at the speed of light, 83.80 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 39.53 which put HIP 64532 at a distance of 82.51 light years or 25.30 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.

Using the 2007 distance, the star is roughly 5,218,463.24 Astronomical Units from the Earth/Sun give or take a few. An Astronomical Unit is the distance between Earth and the Sun. The number of A.U. is the number of times that the star is from the Earth compared to the Sun.

The star's Galacto-Centric Distance is 7,406.00 Parsecs or 24,155.66 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 64532 Facts

Visual Facts

Primary / Proper / Traditional NameHIP 64532
Alternative NamesHD 115043, HIP 64532, BD+57 1425, Gliese 503.2
Spectral TypeG1V
Constellation's Main StarNo
Multiple Star SystemYes
Star Type main sequence Dwarf Star
Colour white to yellow
GalaxyMilky Way
ConstellationUrsa Major
Age5.60 Billion Years Old
Age Range1.20 - 9.80 Billion Years Old
Absolute Magnitude 4.77 / 4.80
Visual / Apparent Magnitude6.82
Naked Eye VisibleRequires a 7x50 Binoculars - Magnitudes
Right Ascension (R.A.)13h 13m 36.89
Declination (Dec.)+56° 42` 29.9
Galactic Latitude60.16 degrees
Galactic Longitude116.81 degrees
1997 Distance from Earth38.92 Parallax (milliarcseconds)
 83.80 Light Years
 25.69 Parsecs
2007 Distance from Earth39.53 Parallax (milliarcseconds)
 82.51 Light Years
 25.30 Parsecs
 5,218,463.24 Astronomical Units
Galacto-Centric Distance24,155.66 Light Years / 7,406.00 Parsecs
Proper Motion Dec.-18.02 ± 0.34 milliarcseconds/year
Proper Motion RA.111.91 ± 0.41 milliarcseconds/year
B-V Index0.60
Radial Velocity-8.70 ± 0.20 km/s
Iron Abundance0.05 ± 0.04 Fe/H
Semi-Major Axis8880.00
Stellar Luminosity (Lsun)1.13

Companions (Multi-Star and Exoplanets) Facts

Exoplanet CountNone/Unaware

Estimated Facts

Calculated Effective Temperature5,895 Kelvin

Sources and Links

SIMBAD SourceLink

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