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19 Lyncis, HD57102, HIP35783, HR2783

19 Lyncis is a blue main sequence dwarf star that can be located in the constellation of Lynx. The star can not be seen by the naked eye, you need a telescope to see it.

19 Lyncis's Alternative Names

The Id of the star in the Yale Bright Star Catalogue is HR2783. HIP35783 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD57102.

Flamsteed designations are named after the creator, Sir John Flamsteed. Sir John numbered the stars in the constellation with a number and the latin name, this star's Flamsteed designation is 19 Lyncis with it shortened to 19 Lyn.

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

Location of 19 Lyncis

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 19 Lyncis, the location is 07h 22m 50.85 and +55° 17` 03.8 .

Physical Properties (Colour, Temperature) of 19 Lyncis

19 Lyncis has a spectral type of B9V. This means the star is a blue main sequence dwarf star. The star has a B-V Colour Index of -0.05 which means the star's temperature has been calculated using information from Morgans @ Uni.edu at being 10,395 Kelvin.

19 Lyncis Radius has been calculated as being 1.37 times bigger than the Sun.The Sun's radius is 695,800km, therefore the star's radius is an estimated 949,998.54.km. The figure is derived at by using the formula from SDSS and has been known to produce widely incorrect figures.

19 Lyncis Apparent and Absolute Magnitudes

19 Lyncis has an apparent magnitude of 6.86 which is how bright we see the star from Earth. Apparent Magnitude is also known as Visual Magnitude. Using the supplied Parallax value, you would get an absolute magnitude of 1.62 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 19 Lyncis

Using the original Hipparcos data that was released in 1997, the parallax to the star was given as 8.94 which gave the calculated distance to 19 Lyncis as 364.84 light years away from Earth or 111.86 parsecs. It would take a spaceship travelling at the speed of light, 364.84 years to get there. We don't have the technology or spaceship that can carry people over that distance yet.

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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19 Lyncis Facts

Visual Facts

Alternative NamesHD 57102, HIP 35783, HR 2783, 19 Lyn
Star Type main sequence Dwarf Star
GalaxyMilky Way
Visual / Apparent Magnitude6.86
Naked Eye VisibleRequires a 7x50 Binoculars - Magnitudes
Right Ascension (R.A.)07h 22m 50.85
Declination (Dec.)+55° 17` 03.8
Galactic Latitude26.36 degrees
Galactic Longitude161.96 degrees
Distance from Earth8.94 Parallax (milliarcseconds)
 364.84 Light Years
 111.86 Parsecs
B-V Index-0.05
Radial Velocity10.00 ± 3.70 km/s
Spectral TypeB9V
Associated / Clustered Stars19 Lyncis B
Colour(B) blue

Estimated Facts

Calculated Effective Temperature10,395 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

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