HD 136418 – a Star Located in the Constellation Boötes

HD 136418 is a star located 340 light-years away from Earth in the constellation Boötes. It, like Jupiter, has a planet orbiting it. It is a gas giant exoplanet in the habitable zone of a K-type star. It has a mass of 2.14 Jupiters, takes 464.3 days to complete one orbit around its star, and is 1.29 AU away from it.

HD 136418 is a star with a mass 1.48 times that of the Sun and a radius of 3.78 times that of the Sun. It is 343.01 light-years away from the solar system and is thought to be 4 billion years old, as opposed to the Sun’s 4.6 billion years. It is known that it has one exoplanet in orbit around it. The star and its planet will be named after something from Canadian culture. Its discovery was announced in 2009.

HD 136418 is a star with 1.48 times the mass of the Sun and 3.78 times its radius. It is a gas giant exoplanet that orbits a K-type star. It is located 343.01 light-years away from the solar system.

HD 136418 b was discovered using the radial velocity method by the W. M. Keck Observatory observatory in 2010-05. Its semi-major axis is 1.29 astronomical units, whereas Earth’s is 1 astronomical unit. HD 136418 b has a mass that is 680.520 times that of Earth. HD 136418 b has a radius that is 13.300 times that of Earth. HD 136418 b, with a mass of more than 50 Earth masses, is a gas giant, a planet whose mass is mostly made up of hydrogen and helium, similar to Jupiter and Saturn in our solar system.

It’s an extrasolar planet that orbits the star Nikawiy in the Bootes constellation. Exoplanets are planets that orbit stars other than the Sun. According to the most recent parallax records, the star is 320.40 light-years or 98.23 parsecs from Earth.

The mass and radius are calculated in relation to Jupiter. Jupiters denotes that it has ten times the mass of Jupiter and is equivalent to Mass. All of the figures have a variation that I have not included here for the time being; if you need them, you can find them at the source site.

The planet’s orbital period, or, to put it another way, its year, is 464.3 days. By the end of a full year, the Earth will have completed 0.79 orbits around its star. The semi-major axis is the point in the orbit that is farthest from the star. The Earth orbits the Sun with a semi-major axis of just over 1 A.U. (1.00000011). The average distance between the Earth and the Sun is one A.U. The planet orbits its star at a closer distance to the Sun than Mars does.