Star 2M1207distance = 55 AUPlanet 2M12076 Exoplanet orbital period (b)For the system pictured in the previous problem (and using data given there), suppose that the starhas a mass of 0.025 solar masses, and the planet's mass is very small in comparison. Compute theplanet's orbit period. Assume the orbit is circular with a radius given by the distance listed in thefigure. Express your answer in years.[Hint: this is a mildly challenging problem that requires plugging into a single formula but usingmultiple unit conversions. You will need to use Kepler's 3rd law in its **general** form (not thesimplified form that is only applicable to objects orbiting our Sun). You will need to look up thevalue of the constant G. Convert solar masses to kg, AU to m, and everything else to base Sl units;find the period in seconds; then convert seconds to years.]

Answered: Image /qna-images/answer/2bc8a81d-c315-4dec-99cc-1368c1ad46b5.jpg

Exoplanet orbital period (b) For the system pictured in the previous problem (and using data given there), suppose that the star has a mass of 0.025 solar masses, and the planet's mass is very small in comparison. Compute the planet's orbit period. Assume the orbit is circular with a radius given by the distance listed in the figure. Express your answer in years.

Exoplanet orbital period (b) For the system pictured in the previous problem (and using data given there), suppose that the star has a mass of 0.025 solar masses, and the planet's mass is very small in comparison. Compute the planet's orbit period. Assume the orbit is circular with a radius given by the distance listed in the figure. Express your answer in years.