Universe Guide

DI Ceti

DI Ceti Facts

DI Ceti's Alternative Names

HIP8646 is the reference name for the star in the Hipparcos Star Catalogue.

DI Ceti has alternative name(s) :- , DI Cet.

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-16 320.

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

Location of DI Ceti

The location of the variable 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 object is compared to the celestial equator and is expressed in degrees. For DI Ceti, the location is 01h 51m 28.29 and -15° 27` 18.5 .

Physical Properties (Colour, Temperature) of DI Ceti

DI Ceti Colour and Temperature

DI Ceti has a spectral type of K5. This means the star is a orange to red variable star. The star has a B-V Colour Index of 1.5 which means the star's temperature is about 4,014 Kelvin. The temperature was calculated using information from Morgans @ Uni.edu at being .

DI Ceti Apparent and Absolute Magnitudes

DI Ceti has an apparent magnitude of 9.43 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 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 DI Ceti

Using the original Hipparcos data that was released in 1997, the parallax to the star was given as -1.73 which gave the calculated distance to DI Ceti as -1885.34 light years away from Earth or -578.03 parsecs. If you want that in miles, it is -1,264,340,355,319.

Variable Type of DI Ceti

The star is a pulsating Semi-Regular Star w variable type which means that its size changes over time. The Variable Type is usually named after the first star of that type to be spotted. DI Ceti brightness ranges from a magnitude of 9.724 to a magnitude of 9.419 over its variable period. The smaller the magnitude, the brighter the star. Its variable/pulsating period lasts for 0.2 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.

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Additional DI Ceti Facts and Figures

Visual Facts

Primary / Proper / Traditional NameDI Ceti
Alternative NamesHIP 8646, BD-16 320, DI Cet
Spectral TypeK5
Constellation's Main StarNo
Multiple Star SystemNo / Unknown
Star TypeVariable Star
ColourOrange to Red
GalaxyMilky Way
Visual / Apparent Magnitude9.43
Naked Eye VisibleRequires a 7x50 Binoculars - Magnitudes
Right Ascension (R.A.)01h 51m 28.29
Declination (Dec.)-15° 27` 18.5
Galactic Latitude-71.82 degrees
Galactic Longitude176.04 degrees
Distance from Earth-1.73 Parallax (milliarcseconds)
 -1885.34 Light Years
 -578.03 Parsecs
 -119,226,415.17 Astronomical Units
B-V Index1.50

Companions (Multi-Star and Exoplanets) Facts

Exoplanet CountNone/Unaware

Variable Star Details

Variable Star ClassPulsating
Variable Star TypeSemi-Regular Star w
Mean Variability Period in Days0.244
Variable Magnitude Range (Brighter - Dimmer)9.419 - 9.724

Estimated Calculated Facts

Effective Temperature4,014 Kelvin

Sources and Links

SIMBAD SourceLink

Related Stars

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