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A moon is orbiting the planet Jupiter, rp is the shortest distance between the moon and its planet and ra is the longest distan...Question
For a moon orbiting its planet, rp
is the shortest distance between the moon and its planet and ra
is the longest distance between the moon and its planet. What is a moon's orbital eccentricity if rp
is equal to 0.27ra
?(1 point)
Responses
0.48
0.48
0.57
0.57
0.65
0.65
0.27
is the shortest distance between the moon and its planet and ra
is the longest distance between the moon and its planet. What is a moon's orbital eccentricity if rp
is equal to 0.27ra
?(1 point)
Responses
0.48
0.48
0.57
0.57
0.65
0.65
0.27
Answers
There are no human answers yet.
Answered by
GPT-4o mini
To find the orbital eccentricity (e) of a moon given the relationship \( r_p = 0.27 r_a \), we can use the formula that relates the periapsis (rp), apoapsis (ra), and eccentricity:
\[
e = \frac{r_a - r_p}{r_a + r_p}
\]
First, let's express \( r_p \) in terms of \( r_a \):
\[
r_p = 0.27 r_a
\]
Now we can substitute this into the equation for eccentricity:
1. Calculate \( r_a + r_p \):
\[
r_a + r_p = r_a + 0.27 r_a = 1.27 r_a
\]
2. Calculate \( r_a - r_p \):
\[
r_a - r_p = r_a - 0.27 r_a = 0.73 r_a
\]
3. Now substitute these values back into the formula for eccentricity:
\[
e = \frac{r_a - r_p}{r_a + r_p} = \frac{0.73 r_a}{1.27 r_a} = \frac{0.73}{1.27}
\]
Now, calculate \( \frac{0.73}{1.27} \):
\[
e \approx 0.575
\]
This is approximately \( 0.57 \) when rounded to two decimal places.
Therefore, the orbital eccentricity of the moon is **0.57**.
\[
e = \frac{r_a - r_p}{r_a + r_p}
\]
First, let's express \( r_p \) in terms of \( r_a \):
\[
r_p = 0.27 r_a
\]
Now we can substitute this into the equation for eccentricity:
1. Calculate \( r_a + r_p \):
\[
r_a + r_p = r_a + 0.27 r_a = 1.27 r_a
\]
2. Calculate \( r_a - r_p \):
\[
r_a - r_p = r_a - 0.27 r_a = 0.73 r_a
\]
3. Now substitute these values back into the formula for eccentricity:
\[
e = \frac{r_a - r_p}{r_a + r_p} = \frac{0.73 r_a}{1.27 r_a} = \frac{0.73}{1.27}
\]
Now, calculate \( \frac{0.73}{1.27} \):
\[
e \approx 0.575
\]
This is approximately \( 0.57 \) when rounded to two decimal places.
Therefore, the orbital eccentricity of the moon is **0.57**.
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