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.
Transcribed Image Text: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.
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