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Theta Arietis, 22 Arietis, HD14191, HIP10732, HR669

Theta Arietis is a blue star that can be located in the constellation of Aries. The star can be seen with the naked eye, that is, you don't need a telescope/binoculars to see it.

Theta Arietis is the Bayer Classification for the star. The Id of the star in the Yale Bright Star Catalogue is HR669. HIP10732 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD14191.

Location of Theta Arietis

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 Theta Arietis, the location is 02h 18m 07.55 and +19d 54` 04.2 .

Proper Motion of Theta Arietis

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 0.72 ± 0.16 miliarcseconds/year towards the north and -13.19 ± 0.29 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 2.30000 km/s with an error of about 0.80 km/s .

Theta Arietis 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 20.0000000 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.

Physical Properties (Colour, Temperature, Radius) of Theta Arietis

Theta Arietis has a spectral type of A1Vn. This means the star is a blue star. The star is 7493.00000000 Parsecs from the Galactic Centre or terms of Light Years is 24439.4193659200000000s. The star has a B-V Colour Index of 0.01 which means the star's temperature has been calculated using information from Morgans @ Uni.edu at being 9,392 Kelvin.

Theta Arietis Radius has been calculated as being 3.20 times bigger than the Sun.The Sun's radius is 695,800km, therefore the star's radius is an estimated 2,227,766.15.km. However with the 2007 release of updated Hipparcos files, the radius is now calculated at being round 3.71. The figure is derived at by using the formula from SDSS and has been known to produce widely incorrect figures.

Theta Arietis Apparent and Absolute Magnitudes

Theta Arietis has an apparent magnitude of 5.58 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 0.21 If you used the 2007 Parallax value, you would get an absolute magnitude of -0.11. 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 Theta Arietis

Using the original Hipparcos data that was released in 1997, the parallax to the star was given as 8.42 which gave the calculated distance to Theta Arietis as 387.37 light years away from Earth or 118.76 parsecs. It would take a spaceship travelling at the speed of light, 387.37 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 7.29 which put Theta Arietis at a distance of 447.41 light years or 137.17 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 7,493.00 Parsecs or 24,439.42 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.

Theta Arietis Facts

Alternative Names

Flamsteed Name22 Arietis
Flamsteed Short Name22 Ari
Bayer DesignationTheta Arietis
Hipparcos Library I.D.10732
Yale Bright Star Catalogue (HR) Id669
Bonner DurchmusterungBD+19 340
Henry Draper Designation14191

Visual Facts

Star Type star
Absolute Magnitude0.21 / -0.11
Visual / Apparent Magnitude5.58
Naked Eye VisibleYes - Magnitudes
Right Ascension (R.A.)02h 18m 07.55
Declination (Dec.)+19d 54` 04.2
Galactic Latitude-38.50 degrees
Galactic Longitude149.27 degrees
1997 Distance from Earth8.42 Parallax (milliarcseconds)
 387.37 Light Years
 118.76 Parsecs
2007 Revised Distance from Earth7.29 Parallax (milliarcseconds)
 447.41 Light Years
 137.17 Parsecs
Galacto-Centric Distance24,439.42 Light Years / 7,493.00 Parsecs
Proper Motion Dec.0.72 ± 0.16 milliarcseconds/year
Proper Motion RA.-13.19 ± 0.29 milliarcseconds/year
B-V Index0.01
Radial Velocity2.30 ± 0.80 km/s
Spectral TypeA1Vn
Colour(A) blue

Estimated Facts

Luminosity (x the Sun)20.0000000
Calculated Effective Temperature9,392 Kelvin

Sources and Links

SIMBAD SourceLink

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