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41 Arietis - HD17573 - HIP13209

41 Arietis is a blue main sequence dwarf 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.

HIP13209 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD17573.

41 Arietis has alternative name(s), 41 Arietis , 41 Ari.

Location of 41 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 41 Arietis, the location is 02h 49m 58.99 and +27d15`38.8 .

Proper Motion of 41 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 -116.52 ± 0.10 miliarcseconds/year towards the north and 66.81 ± 0.19 miliarcseconds/year east if we saw them in the horizon.

41 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 73.0000000 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 41 Arietis

41 Arietis has a spectral type of B8Vn. This means the star is a blue main sequence dwarf star. The star is 7440.00000000 Parsecs from the Galactic Centre or terms of Light Years is 24266.5527936000000000s. The star has a B-V Colour Index of -0.1 which means the star's temperature has been calculated using information from Morgans @ Uni.edu at being 11,677 Kelvin.

41 Arietis Radius has been calculated as being 2.12 times bigger than the Sun.The Sun's radius is 695,800km, therefore the star's radius is an estimated 1,474,767.98.km. However with the 2007 release of updated Hipparcos files, the radius is now calculated at being round 2.20. The figure is derived at by using the formula from SDSS and has been known to produce widely incorrect figures.

41 Arietis Apparent and Absolute Magnitudes

41 Arietis has an apparent magnitude of 3.61 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 0.16 If you used the 2007 Parallax value, you would get an absolute magnitude of 0.08. 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 41 Arietis

Using the original Hipparcos data that was released in 1997, the parallax to the star was given as 20.45 which gave the calculated distance to 41 Arietis as 159.49 light years away from Earth or 48.90 parsecs. It would take a spaceship travelling at the speed of light, 159.49 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 19.69 which put 41 Arietis at a distance of 165.65 light years or 50.79 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 7,440.00 Parsecs or 24,266.55 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.

41 Arietis Facts

Alternative Names

Traditional/Proper Name41 Arietis
Short Name41 Ari
Alternative Name(s)41 Arietis
Hipparcos Library I.D.13209
Bonner DurchmusterungBDD+26 471
Henry Draper Designation17573

Visual Facts

Star Typemain sequence dwarf star
Absolute Magnitude0.16 / 0.08
Visual / Apparent Magnitude3.61
Naked Eye VisibleYes - Ref: Wiki
Right Ascension (R.A.)02h 49m 58.99
Declination (Dec.)+27d15`38.8
Galactic Latitude-28.61 degrees
Galactic Longitude152.98 degrees
1997 Distance from Earth20.45 Parallax (milliarcseconds)
 159.49 Light Years
 48.90 Parsecs
2007 Revised Distance from Earth19.69 Parallax (milliarcseconds)
 165.65 Light Years
 50.79 Parsecs
Galacto-Centric Distance24,266.55 Light Years / 7,440.00 Parsecs
Proper Motion Dec.-116.52 ± 0.10 milliarcseconds/year
Proper Motion RA.66.81 ± 0.19 milliarcseconds/year
B-V Index-0.10
Radial Velocity4.00 ± 4.10 km/s
Spectral TypeB8Vn
Colour(B) blue

Estimated Facts

Luminosity (x the Sun)73.0000000
Calculated Effective Temperature11,677 Kelvin

Sources and Links

SIMBAD SourceLink

Related Stars

Multi-Star System

The star has been identified as being a multi-star system, one in which there is at least one star in close orbit to another star or two or more stars orbiting a central point. The stars may be of equal mass, unequal mass where one star is stronger than the other or be in groups orbiting a central point which doesn't necessarily have to be a star. More information can be found on my dedicated multiple star systems page. The source of the info is Simbad. The file is dated 2000 so any differences between this and any other source will be down to the actual source from where the information came from.


Proper Motion mas/yr
H.D. IdB.D. IdStar CodeMagnitudeR.A.Dec.SpectrumColourYear
17573+26 471.0A3.7000067.00000-112.00000B8Blue/White
B10.800001922
C10.600001922
+26 470.0D9.1000027.00000-18.000001922

Location of 41 Arietis in Aries


41 Arietis Location in Aries

The map was generated using Night Vision, an awesome free application by Brian Simpson.


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