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R Octantis, HD40857, HIP25412

R Octantis is a red pulsating variable star that can be located in the constellation of Octans. The description is based on the spectral class. The star can not be seen by the naked eye, you need a telescope to see it.

R Octantis's Alternative Names

HIP25412 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD40857.

R Octantis has alternative name(s) :- , R Oct.

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

Location of R Octantis

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 R Octantis, the location is 05h 26m 06.18 and -86° 23` 18.0 .

Proper Motion of R Octantis

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 28.97 ± 0.76 miliarcseconds/year towards the north and 1.26 ± 0.73 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 46.00000 km/s with an error of about 4.70 km/s .

Physical Properties (Colour, Temperature) of R Octantis

R Octantis has a spectral type of Md. This means the star is a red variable star. The star has a B-V Colour Index of 1.5 which means the star's temperature has been calculated using information from Morgans @ Uni.edu at being 4,014 Kelvin.

R Octantis Radius has been calculated as being 5.78 times bigger than the Sun.The Sun's radius is 695,800km, therefore the star's radius is an estimated 4,019,827.08.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 11.42. The figure is derived at by using the formula from SDSS and has been known to produce widely incorrect figures.

R Octantis Apparent and Absolute Magnitudes

R Octantis has an apparent magnitude of 10.04 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 2.62 If you used the 2007 Parallax value, you would get an absolute magnitude of 1.14. 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 R Octantis

Using the original Hipparcos data that was released in 1997, the parallax to the star was given as 3.28 which gave the calculated distance to R Octantis as 994.40 light years away from Earth or 304.88 parsecs. It would take a spaceship travelling at the speed of light, 994.40 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 1.66 which put R Octantis at a distance of 1964.84 light years or 602.41 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.

Variable Type of R Octantis

The star is a pulsating Omicron Ceti 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. R Octantis brightness ranges from a magnitude of 11.370 to a magnitude of 7.371 over its variable period. The smaller the magnitude, the brighter the star. Its variable/pulsating period lasts for 412.4 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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R Octantis Facts

Visual Facts

Primary / Proper / Traditional NameR Octantis
Alternative NamesHD 40857, HIP 25412, R Oct
Spectral TypeMd
Multiple Star SystemNo / Unknown
Star TypeVariable Star
Colour red
GalaxyMilky Way
Absolute Magnitude2.62 / 1.14
Visual / Apparent Magnitude10.04
Naked Eye VisibleRequires a 4.5 - 6 Inch Telescope - Magnitudes
Right Ascension (R.A.)05h 26m 06.18
Declination (Dec.)-86° 23` 18.0
Galactic Latitude-28.39 degrees
Galactic Longitude299.11 degrees
1997 Distance from Earth3.28 Parallax (milliarcseconds)
 994.40 Light Years
 304.88 Parsecs
2007 Distance from Earth1.66 Parallax (milliarcseconds)
 1964.84 Light Years
 602.41 Parsecs
Proper Motion Dec.28.97 ± 0.76 milliarcseconds/year
Proper Motion RA.1.26 ± 0.73 milliarcseconds/year
B-V Index1.50
Radial Velocity46.00 ± 4.70 km/s

Companions (Multi-Star and Exoplanets) Facts

Exoplanet CountNone/Unaware

Variable Star Details

Variable Star ClassPulsating
Variable Star TypeOmicron Ceti
Mean Variability Period in Days412.400
Variable Magnitude Range (Brighter - Dimmer)7.371 - 11.370

Estimated Facts

Calculated Effective Temperature4,014 Kelvin

Sources and Links

SIMBAD SourceLink

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