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RR Lacertae, HD240024, HIP112026

RR Lacertae is a blue to white pulsating variable star that can be located in the constellation of Lacerta. 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.

RR Lacertae's Alternative Names

HIP112026 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD240024.

RR Lacertae has alternative name(s) :- , RR Lac.

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+55 2789.

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

Location of RR Lacertae

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 RR Lacertae, the location is 22h 41m 26.53 and +56° 25` 58.1 .

Proper Motion of RR Lacertae

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 -2.14 ± 0.78 miliarcseconds/year towards the north and -3.66 ± 1.08 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 -38.40000 km/s with an error of about 0.20 km/s .

Physical Properties (Colour, Temperature) of RR Lacertae

RR Lacertae has a spectral type of F9. This means the star is a blue to white variable star. The star has a B-V Colour Index of 0.83 which means the star's temperature has been calculated using information from Morgans @ Uni.edu at being 5,353 Kelvin.

RR Lacertae Radius has been calculated as being 19.40 times bigger than the Sun.The Sun's radius is 695,800km, therefore the star's radius is an estimated 13,496,020.01.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 11.69. The figure is derived at by using the formula from SDSS and has been known to produce widely incorrect figures.

RR Lacertae Apparent and Absolute Magnitudes

RR Lacertae has an apparent magnitude of 8.87 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 -1.26 If you used the 2007 Parallax value, you would get an absolute magnitude of -0.16. 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 Lacertae

Using the original Hipparcos data that was released in 1997, the parallax to the star was given as 0.94 which gave the calculated distance to RR Lacertae as 3469.82 light years away from Earth or 1063.83 parsecs. It would take a spaceship travelling at the speed of light, 3469.82 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 1.56 which put RR Lacertae at a distance of 2090.79 light years or 641.03 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 RR Lacertae

The star is a pulsating Delta Cepheid 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. RR Lacertae brightness ranges from a magnitude of 9.379 to a magnitude of 8.571 over its variable period. The smaller the magnitude, the brighter the star. Its variable/pulsating period lasts for 6.4 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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RR Lacertae Facts

Visual Facts


Primary / Proper / Traditional NameRR Lacertae
Alternative NamesHD 240024, HIP 112026, BD+55 2789, RR Lac
Spectral TypeF9
Multiple Star SystemNo / Unknown
Star TypeVariable Star
Colour blue to white
GalaxyMilky Way
ConstellationLacerta
Absolute Magnitude-1.26 / -0.16
Visual / Apparent Magnitude8.87
Naked Eye VisibleRequires a 7x50 Binoculars - Magnitudes
Right Ascension (R.A.)22h 41m 26.53
Declination (Dec.)+56° 25` 58.1
Galactic Latitude-2.01 degrees
Galactic Longitude105.64 degrees
1997 Distance from Earth0.94 Parallax (milliarcseconds)
 3469.82 Light Years
 1063.83 Parsecs
2007 Distance from Earth1.56 Parallax (milliarcseconds)
 2090.79 Light Years
 641.03 Parsecs
Proper Motion Dec.-2.14 ± 0.78 milliarcseconds/year
Proper Motion RA.-3.66 ± 1.08 milliarcseconds/year
B-V Index0.83
Radial Velocity-38.40 ± 0.20 km/s

Companions (Multi-Star and Exoplanets) Facts


Exoplanet CountNone/Unaware

Variable Star Details


Variable Star ClassPulsating
Variable Star TypeDelta Cepheid
Mean Variability Period in Days6.416
Variable Magnitude Range (Brighter - Dimmer)8.571 - 9.379

Estimated Facts


Calculated Effective Temperature5,353 Kelvin

Sources and Links


SIMBAD SourceLink

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