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HD 48766

HD 48766 Facts

HD 48766's Alternative Names

HIP32609 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD48766.

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+55 1122.

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

Location of HD 48766

The location of the main sequence 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 object is compared to the celestial equator and is expressed in degrees. For HD 48766, the location is 06h 48m 12.23 and +55° 42` 16.0 .

Radial Velocity and Proper Motion of HD 48766

Proper Motion

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 -105.83 ± 0.46 miliarcseconds/year towards the north and 56.40 ± 0.73 miliarcseconds/year east if we saw them in the horizon.

Radial Velocity

The Radial Velocity, that is the speed at which the star is moving away/towards the Sun is 7.94 km/s with an error of about 0.19 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.

Physical Properties (Colour, Age) of HD 48766

HD 48766 Colour and Temperature

HD 48766 has a spectral type of F5V:+.... This means the star is a blue to white main sequence star. The star's Iron Abundance is 0.05 with an error value of 0.08 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 1.80 Billion years old but could be between 1.70 and 1.90 Billion years old. In comparison, the Sun's age is about 4.6 Billion Years Old.

HD 48766 Apparent and Absolute Magnitudes

HD 48766 has an apparent magnitude of 5.54 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 2.18 If you used the 2007 Parallax value, you would get an absolute magnitude of 2.31. 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 HD 48766

Using the original Hipparcos data that was released in 1997, the parallax to the star was given as 21.26 which gave the calculated distance to HD 48766 as 153.42 light years away from Earth or 47.04 parsecs. It would take a spaceship travelling at the speed of light, 153.42 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 22.59 which put HD 48766 at a distance of 144.38 light years or 44.27 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 9,131,279.34 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 7,439.00 Parsecs or 24,263.29 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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Additional HD 48766 Facts and Figures

Visual Facts


Primary / Proper / Traditional NameHD 48766
Alternative NamesHD 48766, HIP 32609, BD+55 1122
Spectral TypeF5V:+...
Constellation's Main StarNo
Multiple Star SystemYes
Star Type Main Sequence Dwarf Star
ColourYellow - White
GalaxyMilky Way
ConstellationLynx
Age1.80 Billion Years Old
Age Range1.70 - 1.90 Billion Years Old
Absolute Magnitude 2.18 / 2.31
Visual / Apparent Magnitude5.54
Naked Eye VisibleYes - Magnitudes
Right Ascension (R.A.)06h 48m 12.23
Declination (Dec.)+55° 42` 16.0
Galactic Latitude21.69 degrees
Galactic Longitude160.26 degrees
1997 Distance from Earth21.26 Parallax (milliarcseconds)
 153.42 Light Years
  47.04 Parsecs
2007 Distance from Earth22.59 Parallax (milliarcseconds)
 144.38 Light Years
 44.27 Parsecs
 9,131,279.34 Astronomical Units
Galacto-Centric Distance24,263.29 Light Years / 7,439.00 Parsecs
Proper Motion Dec.-105.83 ± 0.46 milliarcseconds/year
Proper Motion RA.56.40 ± 0.73 milliarcseconds/year
B-V Index-99.00
Radial Velocity7.94 ± 0.19 km/s
Iron Abundance0.05 ± 0.08 Fe/H
Eccentricity0.05
Semi-Major Axis7051.00

Companions (Multi-Star and Exoplanets) Facts


Exoplanet CountNone/Unaware

Sources and Links


SIMBAD SourceLink

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
48767+55 1122.0A6.3000064.00000-113.00000F5Yellow/White
48766B6.3000057.00000-102.00000F5Yellow/White1830
BC11.200001880

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