Solar analogs

triple star system in the constellation Centaurus, where one of the three stars, Proxima Centauri, being the closest star to the Earth

binary star

star in the constellation Pegasus

star in the southern dog portion of the constellation Canes Venatici

star in the constellation Reticulum

star in constellation Fornax

star in the constellation Coma Berenices

a star that is particularly similar to the Sun

star in the constellation Ursa Major

star in the constellation Orion

star in the constellation Scorpius

binary star system in the constellation Ophiuchus

star

star and planetary system in the Milky Way galaxy

star in the constellation Tucana

Star in the constellation Centaurus

binary star system in the constellation Andromeda

star in the constellation Corona Borealis

star in the constellation Phoenix

star in the Ursa Major constellation

star

binary star system in the constellation Cassiopeia

binary star system in the constelaltion Hydra

binary star system in the constellation Leo Minor

star in the constellation Coma Berenices

star in the constellation Capricornus

star in the constellation Cassiopeia

Kepler-51 is a Sun-like star that is about 500 million years old. It is orbited by four planets—Kepler-51b, c, d and e—first three of which are super-puffs and have the lowest known densities of any known exoplanet. The transiting planets in the system (b, c and d) are similar in radius to gas giants like Jupiter, but have unusually small masses for their size, only a few times greater than Earth's.

star in the constellation Serpens

g-type star located in the constellation of Hercules

star in the constellation Cygnus

star

star in the constellation Auriga

star in the constellation Eridanus

star in the constellation Pegasus

star in the constellation Auriga

star in the constellation Fornax

star

star

triple star system in the constellation Phoenix

star in the constellation Cancer

Kepler-84 is a Sun-like star 3,339 light-years from the Sun. It is a G-type star. The stellar radius measurement has a large uncertainty of 48% as in 2017, complicating the modelling of the star. The Kepler-84 star has two suspected stellar companions. Four stars, all more than four magnitudes fainter than Kepler-84, are seen within a few arcseconds and at least one is probably gravitationally bound to Kepler-84. Another, which has only a 0.005% chance of being a background star, is a yellow star with mass at a projected separation of 0.18″ or 0.26″ (213.6 AU).

star

star in the constellation Draco

sun-like star the constellation Gemini

star in the constellation Crater

WASP-56 is a sun-like star of spectral type G6 about 1,070 light-years away in the constellation of Coma Berenices. It has an apparent magnitude of 11.48. Observations at the Calar Alto Observatory using the lucky imaging technique detected a candidate companion star located 3.4 arcseconds away, however it was not known if this is an actual binary companion or an optical double. It was confirmed in 2019 using Gaia DR2 data.

star in the constellation Pegasus

star