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Psi1 Cancri, 13 Cancri, HD67690, HIP40007

Psi1 Cancri is a orange to red star that can be located in the constellation of Cancer. Psi1 Cancri is the brightest star in Cancer 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.

Psi1 Cancri is the Bayer Classification for the star. HIP40007 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD67690.

Location of Psi1 Cancri

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 Psi1 Cancri, the location is 08h 10m 13.12 and +25d50`40.4 .

Proper Motion of Psi1 Cancri

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 -28.89 ± 0.33 miliarcseconds/year towards the north and -16.23 ± 0.62 miliarcseconds/year east if we saw them in the horizon.

Physical Properties (Colour, Temperature, Radius) of Psi1 Cancri

Psi1 Cancri has a spectral type of K0. This means the star is a orange to red star. The star is 7614.00000000 Parsecs from the Galactic Centre or terms of Light Years is 24834.0770121600000000s. The star has a B-V Colour Index of 1.42 which means the star's temperature has been calculated using information from Morgans @ Uni.edu at being 4,172 Kelvin.

Psi1 Cancri Radius has been calculated as being 29.12 times bigger than the Sun.The Sun's radius is 695,800km, therefore the star's radius is an estimated 20,263,274.95.km. However with the 2007 release of updated Hipparcos files, the radius is now calculated at being round 23.89. The figure is derived at by using the formula from SDSS and has been known to produce widely incorrect figures.

Psi1 Cancri Apparent and Absolute Magnitudes

Psi1 Cancri has an apparent magnitude of 6.44 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 -1.06 If you used the 2007 Parallax value, you would get an absolute magnitude of -0.63. 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 Psi1 Cancri

Using the original Hipparcos data that was released in 1997, the parallax to the star was given as 3.16 which gave the calculated distance to Psi1 Cancri as 1032.16 light years away from Earth or 316.46 parsecs. It would take a spaceship travelling at the speed of light, 1032.16 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 3.86 which put Psi1 Cancri at a distance of 844.98 light years or 259.07 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 7,614.00 Parsecs or 24,834.08 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.

Psi1 Cancri Facts

Alternative Names

Flamsteed Name13 Cancri
Flamsteed Short Name13 Cnc
Bayer DesignationPsi1 Cancri
Hipparcos Library I.D.40007
Bonner DurchmusterungBD+26 1728
Henry Draper Designation67690

Visual Facts

Star Type star
Absolute Magnitude-1.06 / -0.63
Visual / Apparent Magnitude6.44
Naked Eye VisibleYes - Magnitudes
Right Ascension (R.A.)08h 10m 13.12
Declination (Dec.)+25d50`40.4
Galactic Latitude27.95 degrees
Galactic Longitude196.51 degrees
1997 Distance from Earth3.16 Parallax (milliarcseconds)
 1032.16 Light Years
 316.46 Parsecs
2007 Revised Distance from Earth3.86 Parallax (milliarcseconds)
 844.98 Light Years
 259.07 Parsecs
Galacto-Centric Distance24,834.08 Light Years / 7,614.00 Parsecs
Proper Motion Dec.-28.89 ± 0.33 milliarcseconds/year
Proper Motion RA.-16.23 ± 0.62 milliarcseconds/year
B-V Index1.42
Radial Velocity4.52 ± 15.32 km/s
Spectral TypeK0
Colour(K) Orange to Red

Estimated Facts

Calculated Effective Temperature4,172 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
67690+26 1728.0A6.80000-12.00000-37.00000K0Orange
+26 1729.0B9.80000-81.00000-44.000001910

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