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RR Pictoris

RR Pictoris Facts

RR Pictoris's Alternative Names

HIP31481 is the reference name for the star in the Hipparcos Star Catalogue.

RR Pictoris has alternative name(s) :- , RR Pic.

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

Location of RR Pictoris

The location of the main sequence 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 object is compared to the celestial equator and is expressed in degrees. For RR Pictoris, the location is 06h 35m 36.06 and -62° 38` 24.3 .

Physical Properties of RR Pictoris

RR Pictoris Colour and Temperature

RR Pictoris has a spectral type of pec(NOVA).

RR Pictoris Apparent and Absolute Magnitudes

RR Pictoris has an apparent magnitude of 12.39 which is how bright we see the star from Earth. Apparent Magnitude is also known as Visual Magnitude. Using the supplied Parallax value, you would get an absolute magnitude of 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 RR Pictoris

Using the original Hipparcos data that was released in 1997, the parallax to the star was given as -2.46 which gave the calculated distance to RR Pictoris as -1325.87 light years away from Earth or -406.50 parsecs. If you want that in miles, it is -889,150,469,892.

RR Pictoris brightness ranges from a magnitude of 12.604 to a magnitude of 12.153 over its variable period. The smaller the magnitude, the brighter the star. Its variable/pulsating period lasts for 0.3 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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Additional RR Pictoris Facts and Figures

Visual Facts


Primary / Proper / Traditional NameRR Pictoris
Alternative NamesHIP 31481, RR Pic
Spectral Typepec(NOVA)
Constellation's Main StarNo
Multiple Star SystemYes
Star Type Main Sequence Dwarf Star
GalaxyMilky Way
ConstellationPictor
Visual / Apparent Magnitude12.39
Naked Eye VisibleRequires a 4.5 - 6 Inch Telescope - Magnitudes
Right Ascension (R.A.)06h 35m 36.06
Declination (Dec.)-62° 38` 24.3
Galactic Latitude-25.67 degrees
Galactic Longitude272.35 degrees
Distance from Earth-2.46 Parallax (milliarcseconds)
 -1325.87 Light Years
 -406.50 Parsecs
 -83,846,059.49 Astronomical Units
B-V Index-99.00

Companions (Multi-Star and Exoplanets) Facts


Exoplanet CountNone/Unaware

Variable Star Details


Mean Variability Period in Days0.329
Variable Magnitude Range (Brighter - Dimmer)12.153 - 12.604

Sources and Links


SIMBAD SourceLink

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
A-49.00000-18.00000
B1935
C1935

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