HIP 57087 is a red star that can be located in the constellation of Leo. HIP57087 is the reference name for the star in the Hipparcos Star Catalogue. HIP 57087 has alternative name(s), Gliese 436 , . HIP 57087 has at least 3 Extrasolar Planets believed to be in orbit around the star.
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 HIP 57087, the location is 11h 42m 10.51 and +26d42`30.8 .
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 -813.54 ± 001.63 towards the north and 896.07 ± 002.33 east if we saw them in the horizon.
HIP 57087 has a spectral type of M3. This means the star is a red star. The star has a B-V Colour Index of 1.49 which means the star's temperature has been calculated using information from Morgans @ Uni.edu at being 4,035 Kelvin.
HIP 57087 has been calculated as 0.14 times bigger than the Sun.The Sun's radius is 695,800km, therefore the star's radius is an estimated 99,907.13.km.
HIP 57087 has an apparent magnitude of 10.67 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 10.62 If you used the 2007 Parallax value, you would get an absolute magnitude of 10.64. 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 97.73 which gave the calculated distance to HIP 57087 as 33.37 light years away from Earth or 10.23 parsecs. It would take a spaceship travelling at the speed of light, 33.37 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 98.61 which put HIP 57087 at a distance of 33.08 light years or 10.14 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 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 Stellar Age, Metallicity or Mass is from the E.U. Exoplanets. The information was obtained as of 12th Feb 2017.
|Traditional Name||HIP 57087|
|Alternative Name(s)||Gliese 436|
|Hipparcos Library I.D.||57087|
|Absolute Magnitude||10.62 / 10.64|
|Right Ascension (R.A.)||11h 42m 10.51|
|1997 Distance from Earth||97.73 Parallax (milliarcseconds)|
|33.37 Light Years|
|2007 Revised Distance from Earth||98.61 Parallax (milliarcseconds)|
|33.08 Light Years|
|Proper Motion Dec.||-813.54 ± 1.63 milliarcseconds/year|
|Proper Motion RA.||896.07 ± 2.33 milliarcseconds/year|
|Radius (x the Sun)||0.14|
|Calculated Effective Temperature||4,035 Kelvin|
|Name||Status||Mass (Jupiters)||Orbital Period (Days)||Eccentricity||Discovered||Semi-Major Axis||Periastron||Inclination|
|Gliese 436 B||Confirmed||0.07||2.644||0.1912||2004||0.02887||354.000||86.000|
|Gliese 436 C||Unconfirmed||0.0009||1.366||2012||0.0185||87.000|
|Gliese 436 D||Unconfirmed||0.00085||2012|