Diphda (Beta Ceti) is a orange to red star that can be located in the constellation of Cetus. Diphda is the 1st brightest star in Cetus 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.
Beta Ceti is the Bayer Classification for the star. The Id of the star in the Yale Bright Star Catalogue is HR188. HIP3419 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD4128. The Id of the star in the Gould Star Catalogue is 70. Stars in the southern hemisphere are more likely to have a Gould Id than the northern hemisphere. For example, there are no Gould classified stars in Ursa Major. The Gliese ID of the star is GL 31. The star was part of the original catalogue devised by German Astronomer Wilheim Gliese of stars located within 20 parsecs of Earth. Ref : Star Names.
Diphda has alternative name(s), 16 Ceti, Deneb Kaitos , NSV 00272. In Arabic, it is known as Ad-Difdi'.
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 Diphda, the location is 00h 43m 35.23 and -17d 59` 12.1 .
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 31.99 ± 0.12 miliarcseconds/year towards the north and 232.55 ± 0.16 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 13.10000 km/s with an error of about 0.10 km/s .
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 96.0000000 that I have given is based on the Spectral Types page that I have found on the Internet. You might find a different figure, one that may have been calculated rather than generalised that I have done. The figure is always the amount times the luminosity of the Sun. It is an imprecise figure because of a number of factors including but not limited to whether the star is a variable star and distance.
Diphda has a spectral type of K0III. This means the star is a orange to red star. The star is 7402.00000000 Parsecs from the Galactic Centre or terms of Light Years is 24142.6107228800000000s. The star has a B-V Colour Index of 1 which means the star's temperature has been calculated using information from Morgans @ Uni.edu at being 4,849 Kelvin.
Diphda Radius has been calculated as being 15.19 times bigger than the Sun.The Sun's radius is 695,800km, therefore the star's radius is an estimated 10,570,277.95.km. However with the 2007 release of updated Hipparcos files, the radius is now calculated at being round 15.26. 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 0.02 with an error value of 9.99 Fe/H with the Sun has a value of 1 to put it into context.
Diphda has an apparent magnitude of 2.04 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 -0.30 If you used the 2007 Parallax value, you would get an absolute magnitude of -0.31. 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.
Using the original Hipparcos data that was released in 1997, the parallax to the star was given as 34.04 which gave the calculated distance to Diphda as 95.82 light years away from Earth or 29.38 parsecs. It would take a spaceship travelling at the speed of light, 95.82 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 33.86 which put Diphda at a distance of 96.33 light years or 29.53 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 7,402.00 Parsecs or 24,142.61 Light Years. The Galacto-Centric Distance is the distance from the star to the Centre of the Galaxy which is Sagittarius A*. Diphda brightness ranges from a magnitude of 2.226 to a magnitude of 2.195 over its variable period. The smaller the magnitude, the brighter the star. Its variable/pulsating period lasts for 0.0 days (variability).
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.
|Short Name||NSV 00272|
|English Meaning||The frog|
|Bayer Designation||Beta Ceti|
|Alternative Name(s)||16 Ceti, Deneb Kaitos|
|Hipparcos Library I.D.||3419|
|Yale Bright Star Catalogue (HR) Id||188|
|Bonner Durchmusterung||BD-18 115|
|Gliese ID||GL 31|
|Henry Draper Designation||4128|
|Absolute Magnitude||-0.30 / -0.31|
|Visual / Apparent Magnitude||2.04|
|Naked Eye Visible||Yes - Magnitudes|
|Right Ascension (R.A.)||00h 43m 35.23|
|Declination (Dec.)||-17d 59` 12.1|
|Galactic Latitude||-80.68 degrees|
|Galactic Longitude||111.33 degrees|
|1997 Distance from Earth||34.04 Parallax (milliarcseconds)|
|95.82 Light Years|
|2007 Revised Distance from Earth||33.86 Parallax (milliarcseconds)|
|96.33 Light Years|
|Galacto-Centric Distance||24,142.61 Light Years / 7,402.00 Parsecs|
|Proper Motion Dec.||31.99 ± 0.12 milliarcseconds/year|
|Proper Motion RA.||232.55 ± 0.16 milliarcseconds/year|
|Radial Velocity||13.10 ± 0.10 km/s|
|Iron Abundance||0.02 ± 9.99 Fe/H|
|Colour||(K) Orange to Red|
|Mean Variability Period in Days||0.017|
|Variable Magnitude Range (Brighter - Dimmer)||2.195 - 2.226|
|Luminosity (x the Sun)||96.0000000|
|Calculated Effective Temperature||4,849 Kelvin|
The map was generated using Night Vision, an awesome free application by Brian Simpson.