Hamal (Alpha Arietis) is a orange to red giant star that can be located in the constellation of Aries. The description is based on the spectral class. Hamal is a main star of the constellation.
Hamal is the 49th brightest star in the night sky and is the brightest star in Aries 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. Hamal has at least 1 Extrasolar Planets believed to be in orbit around the star.
Alpha Arietis (Alf Ari) is the Bayer Classification for the star. The Id of the star in the Yale Bright Star Catalogue is HR617. HIP9884 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD12929. The Gliese ID of the star is GL 84.3. The star was part of the original catalogue devised by German Astronomer Wilheim Gliese of stars located within 20 parsecs of Earth. Star Names
Hamal has alternative name(s) :- , Alf Ari. In Arabic, it is known as Al-Hamal.
Flamsteed designations are named after the creator, Sir John Flamsteed. Sir John numbered the stars in the constellation with a number and the latin name, this star's Flamsteed designation is 13 Arietis with it shortened to 13 Ari.
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+22 306.
More details on star alternative names can be found at Star Names .
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 Hamal, the location is 02h 07m 10.29 and +23° 27` 46.0 .
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 -148.08 ± 0.14 miliarcseconds/year towards the north and 188.55 ± 0.25 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 the Sun is -14.64 km/s with an error of about 0.02 km/s . When the value is negative then the star and the Sun are getting closer to one another, likewise, a positive number means that two stars are moving away. Its nothing to fear as the stars are so far apart, they won't collide in our life-time, if ever.
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 90.89 that I have given is based on the value in the Simbad Hipparcos Extended Catalogue at the University of Strasbourg from 2012.
Hamal has a spectral type of K2III. This means the star is a orange to red giant star. The star is 7,413.00 Parsecs from the Galactic Centre or terms of Light Years is 24,178.49 s. The star has a B-V Colour Index of 1.15 which means the star's temperature has been calculated using information from Morgans @ Uni.edu at being 4,576 Kelvin.
Hamal Radius has been calculated as being 11.91 times bigger than the Sun.The Sun's radius is 695,800km, therefore the star's radius is an estimated 8,287,262.33.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 11.86. 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 1.50 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 metallicity is -0.090000, this value is the fractional amount of the star that is not Hydrogen (X) or Helium (Y). An older star would have a high metallicity whereas a new star would have a lower one.
Hamal has an apparent magnitude of 2.01 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 0.48 If you used the 2007 Parallax value, you would get an absolute magnitude of 0.49. 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 49.48 which gave the calculated distance to Hamal as 65.92 light years away from Earth or 20.21 parsecs. It would take a spaceship travelling at the speed of light, 65.92 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 49.56 which put Hamal at a distance of 65.81 light years or 20.18 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 7,413.00 Parsecs or 24,178.49 Light Years. The Galacto-Centric Distance is the distance from the star to the Centre of the Galaxy which is Sagittarius A*.
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.
|Primary / Proper / Traditional Name||Hamal|
|Alternative Names||Alpha Arietis, Alf Ari, Al-Hamal, HD 12929, HIP 9884, HR 617, 13 Arietis, 13 Ari, BD+22 306, Gliese 84.3, Alf Ari|
|Constellation's Main Star||Yes|
|Multiple Star System||No / Unknown|
|Star Type||Giant Star|
|Colour||orange to red|
|Absolute Magnitude||0.48 / 0.49|
|Visual / Apparent Magnitude||2.01|
|Naked Eye Visible||Yes - Magnitudes|
|Right Ascension (R.A.)||02h 07m 10.29|
|Declination (Dec.)||+23° 27` 46.0|
|Galactic Latitude||-36.21 degrees|
|Galactic Longitude||144.58 degrees|
|1997 Distance from Earth||49.48 Parallax (milliarcseconds)|
|65.92 Light Years|
|2007 Distance from Earth||49.56 Parallax (milliarcseconds)|
|65.81 Light Years|
|Galacto-Centric Distance||24,178.49 Light Years / 7,413.00 Parsecs|
|Proper Motion Dec.||-148.08 ± 0.14 milliarcseconds/year|
|Proper Motion RA.||188.55 ± 0.25 milliarcseconds/year|
|Radial Velocity||-14.64 ± 0.02 km/s|
|Iron Abundance||-0.17 ± 9.99 Fe/H|
|Stellar Luminosity (Lsun)||90.89|
|Brightest in Night Sky||49th|
|Calculated Effective Temperature||4,576 Kelvin|
|Mass Compared to the Sun||1.50|
|Name||Status||Mass (Jupiters)||Orbital Period (Days)||Eccentricity||Discovered||Semi-Major Axis||Periastron||Inclination|
|alf Ari b||Confirmed||0.2||380.800||0.25||2011||1.2||89.160||2011.000|
This is a N.A.S.A. impression of what the solar system might look like. If the star is not on display, its because its so small compared to the orbits of the outer planets. The green area denotes the habital zone which if the planet is within that area, life could exist. The habital zone might not appear on the picture because its outside the area for the picture. Our planets show the orbit of the planet if its was in our solar system. For more information about the planet and other exoplanetary stuff, visit N.A.S.A.