Universe Guide
HomeAliensConstellationsTelevision and Films ListFact ListGames ListWarcraftSearchTwitterFacebook

Keid, Omicron-2 Eridani, 40 Eridani, HD26965, HIP19849, HR1325

Keid (Omicron-2 Eridani) Location in Eridanus

Keid (Omicron-2 Eridani) is a orange to red main sequence dwarf star that can be located in the constellation of Eridanus. The description is based on the spectral class. The star can be seen with the naked eye, that is, you don't need a telescope/binoculars to see it.

There are two stars in Eridanus with similar sounding names, Beid and Keid so make sure you get the right one. Both star are close to one another when you look up at the star but are light years apart. Keid although on the shore of the river is the more famous of the two stars. It has the designation name of 40 Eridani which is the star that Gene Roddenberry said was host star for the Vulcan homeworld. ref: N.A.S.A.

Keid is a multi-star system and any planet would have an skyline similar to Tatooine in the rival Star Wars entertainment franchise. As the article mentioned above, there have been no planets discovered in orbit round the star as yet, the article was written on August 5th 2016. Its not to say there aren`t any, its just that there`s been discovered so far. It is a relatively near star compared to some other stars so the interest in it is greater than other stars.

As the star is dimmer than our Sun, any exoplanet would be closer into the star to ge the necessary heat and light that is needed for life to exist.

Keid's Alternative Names

Omicron-2 Eridani (Omi02 Eri) is the Bayer Classification for the star. The Id of the star in the Yale Bright Star Catalogue is HR1325. HIP19849 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD26965. The Gliese ID of the star is GL 166A. The star was part of the original catalogue devised by German Astronomer Wilheim Gliese of stars located within 20 parsecs of Earth. Star Names

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 40 Eridani with it shortened to 40 Eri.

The Gould star designation is one that was designed by American astronomer, Benjamin Apthorp Gould. Gould stars are predominantly in the Southern and Equatorial constellations but do appear in northern constellations such as Bootes and Orion. The star has the designation 197 G. Eridani. There are no stars with a Gould designation in Ursa Major for example.

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-07 780.

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

Location of Keid

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 Keid, the location is 04h 15m 17.64 and -07° 38` 40.4 .

Proper Motion of Keid

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 -3,420.27 ± 0.14 miliarcseconds/year towards the north and -2,240.12 ± 0.23 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 us is -42.32000 km/s with an error of about 0.08 km/s .

Keid 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 0.44 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 Keid

Keid has a spectral type of K1V. This means the star is a orange to red main sequence dwarf star. The star is 7,404.00 Parsecs from the Galactic Centre or terms of Light Years is 24,149.13 s. The star has a B-V Colour Index of 0.82 which means the star's temperature has been calculated using information from Morgans @ Uni.edu at being 5,236 Kelvin.

Keid Radius has been calculated as being 0.74 times bigger than the Sun.The Sun's radius is 695,800km, therefore the star's radius is an estimated 516,809.44.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 0.74. 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 -0.24 with an error value of 9.99 Fe/H with the Sun has a value of 1 to put it into context.

Keid Apparent and Absolute Magnitudes

Keid has an apparent magnitude of 4.43 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 5.92 If you used the 2007 Parallax value, you would get an absolute magnitude of 5.94. 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 Keid

Using the original Hipparcos data that was released in 1997, the parallax to the star was given as 198.24 which gave the calculated distance to Keid as 16.45 light years away from Earth or 5.04 parsecs. It would take a spaceship travelling at the speed of light, 16.45 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 200.62 which put Keid at a distance of 16.26 light years or 4.98 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 7,404.00 Parsecs or 24,149.13 Light Years. The Galacto-Centric Distance is the distance from the star to the Centre of the Galaxy which is Sagittarius A*. Keid brightness ranges from a magnitude of 4.587 to a magnitude of 4.554 over its variable period. The smaller the magnitude, the brighter the star. Its variable/pulsating period lasts for 0.1 days (variability).

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.

Hide Explanations
Show GridLines

Keid Facts

Visual Facts


 Keid
Alternative NamesOmicron-2 Eridani, Omi02 Eri, HD 26965, HIP 19849, HR 1325, 197 G. Eridani, 40 Eridani, 40 Eri, BD-07 780, Gliese 166A
Spectral TypeK1V
Multiple Star SystemYes
Star Type main sequence Dwarf Star
Colour orange to red
GalaxyMilky Way
ConstellationEridanus
Absolute Magnitude5.92 / 5.94
Visual / Apparent Magnitude4.43
Naked Eye VisibleYes - Magnitudes
Right Ascension (R.A.)04h 15m 17.64
Declination (Dec.)-07° 38` 40.4
Galactic Latitude-38.04 degrees
Galactic Longitude200.75 degrees
1997 Distance from Earth198.24 Parallax (milliarcseconds)
 16.45 Light Years
 5.04 Parsecs
2007 Distance from Earth200.62 Parallax (milliarcseconds)
 16.26 Light Years
 4.98 Parsecs
Galacto-Centric Distance24,149.13 Light Years / 7,404.00 Parsecs
Proper Motion Dec.-3420.27 ± 0.14 milliarcseconds/year
Proper Motion RA.-2240.12 ± 0.23 milliarcseconds/year
B-V Index0.82
Radial Velocity-42.32 ± 0.08 km/s
Iron Abundance-0.24 ± 9.99 Fe/H
Eccentricity0.54
Semi-Major Axis9239.00
Stellar Luminosity (Lsun)0.44
Associated / Clustered Stars40 Eridani B
Omicron-02 Eridani C

Companions (Multi-Star and Exoplanets) Facts


Exoplanet CountNone/Unaware

Variable Star Details


Mean Variability Period in Days0.054
Variable Magnitude Range (Brighter - Dimmer)4.554 - 4.587

Estimated Facts


Calculated Effective Temperature5,236 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
26965-07 780.0A4.50000-2245.00000-3419.00000G5Yellow
26976-07 781.0B9.70000-2182.00000-3440.00000AWhite1940
BC11.700001959
D12.200001907
E12.500001907

Related Stars


Add a Comment


Name:
Email: (Optional)
Comment: