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Planetary systems with two confirmed planets

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star in the constellation of Ara

star in the constellation Coma Berenices

red dwarf star with earth-like planet

star in the constellation Serpens

star in the constellation Aquila

star in the constellation Virgo

star in the constellation Ursa Major

Nu2 Canis Majoris

star in the constellation Pisces

star in the constellation Sextans

star in the constellation Tucana

Kepler-28 is an M-type main-sequence star about away in the northern constellation of Cygnus. With an apparent visual magnitude of 15.036, this star is too faint to be seen with the naked eye. It is orbited by two exoplanets.

star in the constellation Ursa Major

star system in the constellation Eridanus

star in the constellation Lyra

star in the constellation Cetus

star in the constellation Dorado

HAT-P-13, also known as GSC 03416-00543, is a G-type main sequence star approximately 800 light-years away in the constellation Ursa Major. In 2009 it was discovered that this star is orbited by two massive planets, the innermost of which transits the star. This was the first known example of an extrasolar transiting planet with an additional planet in the same system.

Kepler-29 is a Sun-like star in the northern constellation of Cygnus. It is located at the celestial coordinates: Right Ascension , Declination . With an apparent visual magnitude of 15.456, this star is too faint to be seen with the naked eye. It is a solar analog, having a close mass, radius, and temperature as the Sun. Currently the age of the star has not been determined due to its 2780 light-year (850 parsecs) distance. As of 2016 no Jovian exoplanets of 0.9–1.4 have been found at a distance of 5 AU.

star in the constellation Lynx

star in the constellation Centaurus

star in the constellation Ursa Major

BD−08°2823 is a star with a pair of exoplanetary companions in the faint equatorial constellation of Sextans. The star has an apparent visual magnitude of 9.86, which is too faint to be visible with the naked eye. This system is located at a distance of 135 light-years from the Sun based on parallax measurements, and is trending further away with a radial velocity of +53 km/s. It is a high proper motion star that is traversing the celestial sphere at the angular rate of  yr−1.

star in the constellation Cetus

star in the constellation Carina

star in the constellation Sagittarius

star in the constellation Corvus

star in the constellation Monoceros

star in the constellation Virgo

WASP-41 is a G-type main-sequence star about 533 light-years away in the constellation Centaurus. Its surface temperature is 5450 K. WASP-41 is similar to the Sun in its concentration of heavy elements, with a metallicity Fe/H index of −0.080, but is much younger at an age of 2.289 billion years. The star exhibits strong starspot activity, with spots covering 3% of the stellar surface.

star in the constellation Centaurus

star in the constellation Hydrus

star in the costellation Canis Major

Star system in the constellation Octans

star in the constellation Circinus

nearby star with a planetary system

red giant star in the constellation Cetus

star in the constellation Cygnus

star in the constellation Vela

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