HD 133683

HD 133683 is a yellow dwarf star located approximately 144 light-years away in the constellation Boötes. It is of spectral type G0V, indicating that it is a main-sequence star similar to our Sun, though perhaps slightly hotter and more massive. Its apparent magnitude is around 7.6, meaning it is not visible to the naked eye and requires binoculars or a telescope to be observed.

The star is notable for being a relatively bright and Sun-like star in the solar neighborhood. Its proximity and similarity to the Sun make it a target of interest for astronomers studying stellar properties and the search for exoplanets.

Studies of HD 133683 have investigated its metallicity (the abundance of elements heavier than hydrogen and helium), age, and rotation rate. Such parameters are important for understanding the star's evolution and potential for harboring planetary systems. While no planets have been definitively confirmed orbiting HD 133683 as of the current date, its status as a Sun-like star makes it a continuing target in exoplanet searches. Future observations using more precise radial velocity or transit photometry techniques may reveal the presence of planets around this star.