WASP-18 is a blue to white star that can be located in the constellation of Phoenix. 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. It is calculated at being .630 Billion Years old. This information comes from ExoPlanet. WASP-18 has at least 1 Extrasolar Planets believed to be in orbit around the star.
HIP7562 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD10069.
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 WASP-18, the location is 01h 37m 25.00 and -45° 40` 40.00 .
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 18.79 ± 0.95 miliarcseconds/year towards the north and 26.52 ± 1.07 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 2.78000 km/s with an error of about 0.20 km/s .
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 1.61 that I have given is based on the value in the Simbad Hipparcos Extended Catalogue at the University of Strasbourg from 2012.
WASP-18 has a spectral type of F6. This means the star is a blue to white star. The star is 7,395.00 Parsecs from the Galactic Centre or terms of Light Years is 24,119.78 s. The star has a B-V Colour Index of 0.49 which means the star's temperature has been calculated using information from Morgans @ Uni.edu at being 6,140 Kelvin.
WASP-18 has been calculated as 1.23 times bigger than the Sun.The Sun's radius is 695,800km, therefore the star's radius is an estimated 855,834.00.km. If you need the diameter of the star, you just need to multiple the radius by 2.
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.
The star is believed to be about 0.63 Billion years old. To put in context, the Sun is believed to be about five billion years old and the Universe is about 13.8 billion years old.
WASP-18 has an apparent magnitude of 9.30 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 4.31 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 10.06 which gave the calculated distance to WASP-18 as 324.22 light years away from Earth or 99.40 parsecs. It would take a spaceship travelling at the speed of light, 324.22 years to get there. We don't have the technology or spaceship that can carry people over that distance yet.
The star's Galacto-Centric Distance is 7,395.00 Parsecs or 24,119.78 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.
|Alternative Names||HD 10069, HIP 7562|
|Multiple Star System||No / Unknown|
|Colour||blue to white|
|Age||0.63 Billion Years Old|
|Visual / Apparent Magnitude||9.30|
|Naked Eye Visible||Requires a 7x50 Binoculars - Magnitudes|
|Right Ascension (R.A.)||01h 37m 25.00|
|Declination (Dec.)||-45° 40` 40.00|
|Galactic Latitude||-69.32 degrees|
|Galactic Longitude||279.71 degrees|
|Distance from Earth||10.06 Parallax (milliarcseconds)|
|324.22 Light Years|
|Galacto-Centric Distance||24,119.78 Light Years / 7,395.00 Parsecs|
|Proper Motion Dec.||18.79 ± 0.95 milliarcseconds/year|
|Proper Motion RA.||26.52 ± 1.07 milliarcseconds/year|
|Radial Velocity||2.78 ± 0.20 km/s|
|Stellar Luminosity (Lsun)||1.61|
|Radius (x the Sun)||1.23|
|Calculated Effective Temperature||6,140 Kelvin|
|Name||Status||Mass (Jupiters)||Orbital Period (Days)||Eccentricity||Discovered||Semi-Major Axis||Periastron||Inclination|