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Tseen Kee, Phi Velorum, HD86440, HIP48774, HR3940

Tseen Kee Location in Vela

Primary Facts on Tseen Kee

  • Tseen Kee's star type is supergiant star that can be located in the constellation of Vela. The description is based on the spectral class.
  • Tseen Kee is a main star of the constellation outline.
  • Based on the spectral type (B5Ib) of the star, the star's colour is blue .
  • Phi Velorum is the Bayer name for the star. It was assigned this name by Johann Bayer in 1603. The closer to the start of the Greek Alphabet the name, the brighter the star is. Alpha stars tend to be the brightest in the constellation. A notable exception is Pollux (Beta Geminorum) which is the brighest star in the Gemini constellation.
  • The star can be seen with the naked eye, that is, you don't need a telescope/binoculars to see it.
  • Using the most recent figures given by the 2007 Hipparcos data, the star is 1591.04 light years away from us.

Tseen Kee's Alternative Names

Phi Velorum (Phi Vel) is the Bayer Classification for the star. The Id of the star in the Yale Bright Star Catalogue is HR3940. HIP48774 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD86440.

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

Location of Tseen Kee

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 Tseen Kee, the location is 09h 56m 51.75 and -54° 34` 04.1 .

Radial Velocity and Proper Motion of Tseen Kee

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 3.55 ± 0.09 miliarcseconds/year towards the north and -13.08 ± 0.11 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 13.90 km/s with an error of about 0.70 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.

Tseen Kee 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 11,757.00 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 Tseen Kee

Tseen Kee has a spectral type of B5Ib. This means the star is a blue supergiant star. The star is 7,336.00 Parsecs from the Galactic Centre or in terms of Light Years is 23,927.34 s. The star has a B-V Colour Index of -0.06 which means the star's temperature has been calculated using information from Morgans @ Uni.edu at being 12,136 Kelvin.

Tseen Kee Radius has been calculated as being 24.71 times bigger than the Sun.The Sun's radius is 695,800km, therefore the star's radius is an estimated 17,190,524.21.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 20.36. The figure is derived at by using the formula from SDSS and has been known to produce widely incorrect figures.

Tseen Kee Apparent and Absolute Magnitudes

Tseen Kee has an apparent magnitude of 3.52 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 -5.34 If you used the 2007 Parallax value, you would get an absolute magnitude of -4.92. 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 Tseen Kee

Using the original Hipparcos data that was released in 1997, the parallax to the star was given as 1.69 which gave the calculated distance to Tseen Kee as 1929.96 light years away from Earth or 591.72 parsecs. It would take a spaceship travelling at the speed of light, 1929.96 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 2.05 which put Tseen Kee at a distance of 1591.04 light years or 487.80 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 100,615,271.39 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 7,336.00 Parsecs or 23,927.34 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 Tseen Kee Facts and Figures

Visual Facts


Primary / Proper / Traditional NameTseen Kee
Alternative NamesPhi Velorum, Phi Vel, HD 86440, HIP 48774, HR 3940
Spectral TypeB5Ib
Constellation's Main StarYes
Multiple Star SystemYes
Star Type very luminous Supergiant Star
Colour blue
GalaxyMilky Way
ConstellationVela
Absolute Magnitude -5.34 / -4.92
Visual / Apparent Magnitude3.52
Naked Eye VisibleYes - Magnitudes
Right Ascension (R.A.)09h 56m 51.75
Declination (Dec.)-54° 34` 04.1
Galactic Latitude0.11 degrees
Galactic Longitude279.35 degrees
1997 Distance from Earth1.69 Parallax (milliarcseconds)
 1929.96 Light Years
 591.72 Parsecs
2007 Distance from Earth2.05 Parallax (milliarcseconds)
 1591.04 Light Years
 487.80 Parsecs
 100,615,271.39 Astronomical Units
Galacto-Centric Distance23,927.34 Light Years / 7,336.00 Parsecs
Proper Motion Dec.3.55 ± 0.09 milliarcseconds/year
Proper Motion RA. -13.08 ± 0.11 milliarcseconds/year
B-V Index-0.06
Radial Velocity13.90 ± 0.70 km/s
Eccentricity0.04
Semi-Major Axis7076.00
Stellar Luminosity (Lsun)11,757.00

Companions (Multi-Star and Exoplanets) Facts


Exoplanet CountNone/Unaware

Estimated Facts


Calculated Effective Temperature12,136 Kelvin

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
86440-53 3075.4A3.70000-12.000005.00000B7Blue/White
B12.000001901

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