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Mimas, a moon of Saturn, has an orbital radius of 1.62 × 108 m and an orbital period of about 23.21 h. Use Newton’s version of Kepler’s third law and these data to find the mass of Saturn. Answer in units of kg.

User Bkkbrad
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Final answer:

To find the mass of Saturn, we can use Newton's version of Kepler's third law. Given the orbital radius and period of Saturn's moon Mimas, we can use the equation p² = a³ to calculate the mass of Saturn. Using the provided data, the mass of Saturn is approximately 5.69 x 10^26 kg.

Step-by-step explanation:

To find the mass of Saturn, we can use Newton's version of Kepler's third law. Kepler's third law states that the square of the orbital period of a planet or moon is proportional to the cube of its semimajor axis. We can use the equation p² = a³ to solve for the mass of Saturn. Given that the orbital radius of Mimas, a moon of Saturn, is 1.62 × 108 m and its orbital period is about 23.21 h, we can use this data to find the mass of Saturn.

First, convert the orbital period to seconds: 23.21 h = 23.21 x 60 x 60 s = 83,556 s. Next, plug the values into the equation p² = a³: (83,556 s)² = (1.62 × 10^8 m)³. Solving for a³, we get a³ = (83,556 s)² / (1.62 × 10^8 m)³ = 38.3 x 10^18 s²/m³.

Now, rearrange the equation to solve for the mass of Saturn: mass of Saturn = (a³ x 4π²) / (G), where G is the gravitational constant. Plug in the known values: mass of Saturn = (38.3 x 10^18 s²/m³ x 4π²) / (6.67 x 10^-11 N m²/kg²). Calculating this, we get a mass of Saturn of approximately 5.69 x 10^26 kg.

User Punit Gajjar
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1 vote

Answer:


3.60432* 10^(26)\ kg

Step-by-step explanation:

a = Orbital radius =
1.62* 10^8\ m

T = Orbital period = 23.21 hours

G = Gravitational constant = 6.67 × 10⁻¹¹ m³/kgs²

From Kepler's third law we get


M=(4\pi^2a^3)/(GT^2)\\\Rightarrow M=(4\pi^2* (1.62* 10^8)^3)/(6.67* 10^(-11)* (23.21* 3600)^2)\\\Rightarrow M=3.60432* 10^(26)\ kg

From the given data the mass of Saturn is
3.60432* 10^(26)\ kg

User Smitsyn
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