Qatar-8

The topic of this article may not meet Wikipedia's notability guideline for astronomical objects. Please help to demonstrate the notability of the topic by citing reliable secondary sources that are independent of the topic and provide significant coverage of it beyond a mere trivial mention. If notability cannot be shown, the article is likely to be merged, redirected, or deleted. Find sources: "Qatar-8" – news · newspapers · books · scholar · JSTOR (May 2021) (Learn how and when to remove this message)

Qatar-8 is a faint solar analog located in the northern circumpolar constellation Ursa Major. With an apparent magnitude of 11.71, it is impossible to detect with the naked eye, but can be located with a powerful telescope. Qatar-8 is currently 924 light-years (283 parsecs) away from the Solar System, but is drifting further away, with a radial velocity of 5.06 km/s.

Qatar-8 is a relatively old star, with an age of 8.3 billion years. At this rate, it is on the final stages of the main sequence. It has a similar effective temperature to the Sun at 5,738 K. Despite that, it has a 69% greater luminosity than the Sun. Qatar-8 has a radius 31.5% greater than the Sun, and has a similar metallicity to the Sun despite its age.

In 2019, the Qatar Exoplanet Survey (QES) discovered planets around Qatar-9, itself, and Qatar-10. However, Qatar-8b is a puffy Hot Saturn unlike the other planets discovered. ^[3]

Since Qatar-8b is a puffy planet, it only has 37.1% the mass of Jupiter. Due to that, it puffs up to a radius that is 28.5% larger than the latter's. It also has an effective temperature of 1,457 K. Qatar-8b is ten times closer to its star than Mercury is to the Sun, which corresponds to a typical four-day orbit. ^[3]

Qatar-8 was suspected to have a stellar companion, which makes it a binary star. However, a study in 2020 after analysis of many other stars show no stellar companion at all.^[4]