1) Use the data above to verify Kepler's third Law, T² = r3 for the orbit of the moon GM around the Earth. You have multiple choices for T, M and r in the table above. Explain why you choose the values you did from the table for this formula.

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Chapter4: The Origin Of Modern Astronomy
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1) Use the data above to verify Kepler's third Law, T² =
r3 for the orbit of the moon
GM
around the Earth. You have multiple choices for T, M and r in the table above. Explain
why you choose the values you did from the table for this formula.
Transcribed Image Text:1) Use the data above to verify Kepler's third Law, T² = r3 for the orbit of the moon GM around the Earth. You have multiple choices for T, M and r in the table above. Explain why you choose the values you did from the table for this formula.
Feel free to use the following data to complete your calculations:
Nm2
G = 6.67 × 10-11,
kg?
Msun = 1.989 × 1030 kg
Мoon:
Earth:
Tmoon around Earth = 27.3 days
Mmoon = 7.34 × 102²kg
"Moon to Earth = 3.84 × 108 m
"Moon center to Moon surface = 1.74 × 106 m
TEarth around Sun = 365.25 days
MEarth = 5.97 × 10²4 kg
TEarth to Moon = 3.84 × 10® m
TEarth center to Earth surface = 6.37 × 106 m
Transcribed Image Text:Feel free to use the following data to complete your calculations: Nm2 G = 6.67 × 10-11, kg? Msun = 1.989 × 1030 kg Мoon: Earth: Tmoon around Earth = 27.3 days Mmoon = 7.34 × 102²kg "Moon to Earth = 3.84 × 108 m "Moon center to Moon surface = 1.74 × 106 m TEarth around Sun = 365.25 days MEarth = 5.97 × 10²4 kg TEarth to Moon = 3.84 × 10® m TEarth center to Earth surface = 6.37 × 106 m
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