HD 25274

HD 25274 is a G-type main-sequence star located approximately 155 light-years away in the constellation Taurus. It is slightly more massive and luminous than the Sun. The star is also known by its Henry Draper Catalogue designation, indicating its inclusion in the massive stellar catalog compiled in the early 20th century.

HD 25274 has been the subject of studies related to stellar evolution, activity, and the search for exoplanets. Although no confirmed planets have been detected orbiting HD 25274 as of the current date, it remains a target of interest for radial velocity and transit surveys. Further investigation is necessary to fully characterize any potential planetary systems around this star. Its spectral type indicates a temperature and color similar to the Sun, suggesting a similar stage in its life cycle. Precise measurements of its stellar properties, such as its effective temperature, surface gravity, and metallicity, are used to compare it to other stars and to refine models of stellar structure and evolution.