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Beta Circini, HD135379, HIP74824, HR5670

Beta Circini (Beta Circini) Location in Circinus

Beta Circini is a blue main sequence dwarf star that can be located in the constellation of Circinus. 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. It is calculated at being .367 Billion Years old. This information comes from ExoPlanet. Beta Circini has at least 1 Extrasolar Planets believed to be in orbit around the star.

Beta Circini's Alternative Names

Beta Circini (Bet Cir) is the Bayer Classification for the star. The Id of the star in the Yale Bright Star Catalogue is HR5670. HIP74824 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD135379. The Gliese ID of the star is GL 580.1. The star was part of the original catalogue devised by German Astronomer Wilheim Gliese of stars located within 20 parsecs of Earth. Star Names

Beta Circini has alternative name(s) :- , Beta Cir.

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

Location of Beta Circini

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 Beta Circini, the location is 15h 17m 30.96 and -58° 48` 03.2 .

Proper Motion of Beta Circini

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 -134.15 ± 0.13 miliarcseconds/year towards the north and -97.74 ± 0.19 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 9.60000 km/s with an error of about 2.70 km/s .

Beta Circini 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 19.02 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, Age, Mass) of Beta Circini

Beta Circini has a spectral type of A3V. This means the star is a blue main sequence dwarf star. The star is 7,376.00 Parsecs from the Galactic Centre or terms of Light Years is 24,057.81 s. The star has a B-V Colour Index of 0.08 which means the star's temperature has been calculated using information from Morgans @ Uni.edu at being 8,626 Kelvin.

Beta Circini Radius has been calculated as being 1.90 times bigger than the Sun.The Sun's radius is 695,800km, therefore the star's radius is an estimated 1,323,585.91.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 1.96. The figure is derived at by using the formula from SDSS and has been known to produce widely incorrect figures. The star's solar mass is 1.96 times that of the Sun's. The Sun's Mass is 1,989,100,000,000,000,000,000 billion kg. which to calculate using this website is too large. To give idea of size, the Sun is 99.86% the mass of the solar system. The star's Iron Abundance is 0.16 with an error value of 9.99 Fe/H with the Sun has a value of 1 to put it into context.

The star is believed to be about 0.37 Billion years old. To put in context, the Sun is believed to be about five billion years old and the Universe is about 13.8 billion years old.

Beta Circini Apparent and Absolute Magnitudes

Beta Circini has an apparent magnitude of 4.07 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 1.71 If you used the 2007 Parallax value, you would get an absolute magnitude of 1.64. 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 Beta Circini

Using the original Hipparcos data that was released in 1997, the parallax to the star was given as 33.75 which gave the calculated distance to Beta Circini as 96.64 light years away from Earth or 29.63 parsecs. It would take a spaceship travelling at the speed of light, 96.64 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 32.73 which put Beta Circini at a distance of 99.65 light years or 30.55 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 7,376.00 Parsecs or 24,057.81 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.

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Beta Circini Facts

Visual Facts

Primary / Proper / Traditional NameBeta Circini
Alternative NamesBet Cir, HD 135379, HIP 74824, HR 5670, Gliese 580.1, Beta Cir
Spectral TypeA3V
Multiple Star SystemNo / Unknown
Star Type main sequence Dwarf Star
Colour blue
GalaxyMilky Way
Age0.37 Billion Years Old
Absolute Magnitude1.71 / 1.64
Visual / Apparent Magnitude4.07
Naked Eye VisibleYes - Magnitudes
Right Ascension (R.A.)15h 17m 30.96
Declination (Dec.)-58° 48` 03.2
Galactic Latitude-1.12 degrees
Galactic Longitude320.89 degrees
1997 Distance from Earth33.75 Parallax (milliarcseconds)
 96.64 Light Years
 29.63 Parsecs
2007 Distance from Earth32.73 Parallax (milliarcseconds)
 99.65 Light Years
 30.55 Parsecs
Galacto-Centric Distance24,057.81 Light Years / 7,376.00 Parsecs
Proper Motion Dec.-134.15 ± 0.13 milliarcseconds/year
Proper Motion RA.-97.74 ± 0.19 milliarcseconds/year
B-V Index0.08
Radial Velocity9.60 ± 2.70 km/s
Iron Abundance0.16 ± 9.99 Fe/H
Semi-Major Axis6789.00
Stellar Luminosity (Lsun)19.02

Companions (Multi-Star and Exoplanets) Facts

Exoplanet Count1

Estimated Facts

Calculated Effective Temperature8,626 Kelvin
Mass Compared to the Sun1.96

Sources and Links

SIMBAD SourceLink

List of Extrasolar Planets orbiting Beta Circini

NameStatusMass (Jupiters)Orbital Period (Days)EccentricityDiscoveredSemi-Major AxisPeriastronInclination
beta Cir bConfirmed7.0201566562015.000

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