A planet has two satellite moons. Moon X has an orbital period of 2.27 days. Moon Y has an orbital period of about 3.40 days. Both moons have nearly circular orbits. Use Kepler's third law to find the distance of each satellite from the planet's center. The planet's mass is 1.60 1027 kg.

distance from Moon X to the planet's center__ km
distance from Moon Y to planet's center ___ km

For the first problem (Moon X), I keep getting 8.09but that answer is wrong. What am I doing wrong? I get K= 3.69x10^-16. Then 1.96x10^5s for the planets orbital and plug it into the cubed root equation. Any suggestions?

Use Kepler's Third Law, in Newton's modified frm.

You can find the formula at

http://easycalculation.com/physics/classical-physics/learn-keplers-law.php

To find the distance of each satellite moon from the planet's center using Kepler's third law, we need to use the equation:

T^2 = (4π^2/GM)r^3

Where:
T is the orbital period of the moon in seconds,
G is the gravitational constant (approximately 6.674 × 10^(-11) N m^2/kg^2),
M is the mass of the planet in kilograms, and
r is the distance from the moon to the planet's center.

Let's start with Moon X:
Given:
T (orbital period of Moon X) = 2.27 days = 2.27 × 24 × 60 × 60 seconds = 196,560 seconds
M (mass of the planet) = 1.60 × 10^27 kg

Substituting these values into the equation, we have:

(196,560)^2 = (4π^2/G(1.60 × 10^27))r^3

To find the distance r, we need to rearrange the equation:

r^3 = [(196,560)^2 * G(1.60 × 10^27)/(4π^2)]

Now, calculate the right-hand side of the equation using the given values for G and M:

r^3 ≈ [(196,560)^2 * (6.674 × 10^(-11))(1.60 × 10^27)/(4π^2)]

r^3 ≈ 2.31 × 10^18

To get the distance r, take the cube root of both sides:

r ≈ ∛(2.31 × 10^18)
r ≈ 1337900 km

Therefore, the distance from Moon X to the planet's center is approximately 1,337,900 km.

Now, let's move on to Moon Y:
Given:
T (orbital period of Moon Y) = 3.40 days = 3.40 × 24 × 60 × 60 seconds = 293,760 seconds

Substituting these values into the equation, we have:

(293,760)^2 = (4π^2/G(1.60 × 10^27))r^3

Following the same steps as above, you should find that the distance from Moon Y to the planet's center is approximately 1,834,400 km.

I hope this clears up any confusion and gives you the correct answers for the distances of Moon X and Moon Y from the planet's center.