HD 50281

HD 50281 is a G-type main-sequence star located in the constellation Columba. It is approximately 79 light-years from Earth. The star is notable for its relatively high metallicity compared to the Sun.

Properties:

HD 50281 is slightly more massive and luminous than the Sun. Its effective temperature is similar to that of the Sun, giving it a yellowish-white appearance. The star's age is estimated to be several billion years.

Planetary System:

As of the current date, no planets have been confirmed orbiting HD 50281. However, radial velocity measurements have shown a long-term trend, indicating the possible presence of a distant, massive companion, potentially a brown dwarf or long-period planet. Further observations are needed to confirm the existence and properties of any potential companions.

Observation:

HD 50281 is visible through binoculars or a small telescope under dark sky conditions. Its apparent magnitude is around 7.8.