b) An exoplanet orbits a non-rotating, 1.79019x 1030 kg star. Analysing through the use of geodesics, determine the time period of the planet to complete one orbit around the G-tyne star where the eccentricity of the orbit is approximately (O and the
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![b) An exoplanet orbits a non-rotating, 1.79019x 100 kg star. Analysing through the use
of geodesics, determine the time period of the planet to complete one orbit around
the G-type star where the eccentricity of the orbit is approximately 0 and the
distance between the star and planet is 3.41382 x 10° m.](/v2/_next/image?url=https%3A%2F%2Fcontent.bartleby.com%2Fqna-images%2Fquestion%2Fc0602eaa-79a9-4455-9bd8-2642a3c0ae64%2Ffafc1b65-9c98-4035-81c0-bd86c2e99b95%2Fwbceok_processed.jpeg&w=3840&q=75)
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