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 object is compared to the celestial equator and is expressed in degrees. For Kepler 99, the location is 19 49 25 and 41 18 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 -3.22 milliarcseconds/year towards the north and 1.38 milliarcseconds/year east if we saw them in the horizon.
The Radial Velocity, that is the speed at which the star is moving away/towards the Sun is -23.00000 km/s . When the value is negative then the star and the Sun are getting closer to one another, likewise, a positive number means that two stars are moving away. Its nothing to fear as the stars are so far apart, they won't collide in our life-time, if ever.
|Primary / Proper / Traditional Name||Kepler 99|
|Constellation's Main Star||No|
|Multiple Star System||No / Unknown|
|Age||1.47 Billion Years Old|
|Right Ascension (R.A.)||19 49 25|
|Declination (Dec.)||41 18 00|
|Distance from Earth||4.77040 Parallax (milliarcseconds)|
|683.72 Light Years|
|43,238,990.04 Astronomical Units|
|Proper Motion Dec.||-3.22000 milliarcseconds/year|
|Proper Motion RA.||1.37900 milliarcseconds/year|
|Radial Velocity||-23.00000 km/s|
|Radius (x the Sun)||0.73|
|Calculated Temperature Range||0.00 - 0.00|
|Mass Compared to the Sun||0.79|
|Name||Status||Mass (Jupiters)||Orbital Period (Days)||Eccentricity||Discovered||Semi-Major Axis||Periastron|
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