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EG Leonis

EG Leonis Facts

EG Leonis's Alternative Names

HIP46570 is the reference name for the star in the Hipparcos Star Catalogue.

EG Leonis has alternative name(s) :- , EG Leo.

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+19 2219.

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

Location of EG Leonis

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 EG Leonis, the location is 09h 29m 50.09 and +19° 05` 57.9 .

Physical Properties (Colour, Temperature) of EG Leonis

EG Leonis Colour and Temperature

EG Leonis has a spectral type of M2. This means the star is a red variable star. 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.

EG Leonis Apparent and Absolute Magnitudes

EG Leonis has an apparent magnitude of 8.88 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 EG Leonis

Using the original Hipparcos data that was released in 1997, the parallax to the star was given as -0.11 which gave the calculated distance to EG Leonis as 0 light years away from Earth or 0 parsecs. If you want that in miles, it is 0.

Variable Type of EG Leonis

The star is a eruptive Irregular 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. EG Leonis brightness ranges from a magnitude of 8.965 to a magnitude of 8.781 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.

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Additional EG Leonis Facts and Figures

Visual Facts


Primary / Proper / Traditional NameEG Leonis
Alternative NamesHIP 46570, BD+19 2219, EG Leo
Spectral TypeM2
Constellation's Main StarNo
Multiple Star SystemNo / Unknown
Star TypeVariable Star
ColourRed
GalaxyMilky Way
ConstellationLeo
Visual / Apparent Magnitude8.88
Naked Eye VisibleRequires a 7x50 Binoculars - Magnitudes
Right Ascension (R.A.)09h 29m 50.09
Declination (Dec.)+19° 05` 57.9
Galactic Latitude43.26 degrees
Galactic Longitude211.63 degrees
Distance from Earth-0.11 Parallax (milliarcseconds)
 0 Light Years
 0 Parsecs
 0.00 Astronomical Units
B-V Index1.42

Companions (Multi-Star and Exoplanets) Facts


Exoplanet CountNone/Unaware

Variable Star Details


Variable Star ClassEruptive
Variable Star TypeIrregular
Mean Variability Period in Days0.147
Variable Magnitude Range (Brighter - Dimmer)8.781 - 8.965

Estimated Calculated Facts


Effective Temperature4,172 Kelvin

Sources and Links


SIMBAD SourceLink

Related Stars


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