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Answer on Question #61300 - Physics - Mechanics | Relativity
Question:
1. IF a small planet were discovered whose orbital period was twice that of Earth, how many time
farther
from
the
Sun
would
this
planet
be?
2. Determine Kepler's constant for any satellite of Earth.
Solution:
1.
The third Kepler’s law is:
𝑇12
=
𝑇22
π‘Ž13
π‘Ž23
𝑇12 π‘Ž13
π‘Ž1 3 𝑇12
=
β‡’
= √ 2,
π‘Ž2
𝑇22 π‘Ž23
𝑇2
where π‘Ž2 is the radius of Earth's orbit and π‘Ž1 is the radius of planet's orbit, 𝑇2 and 𝑇1 are orbital
periods of Earth and planet.
1
π‘Ž1 3 𝑇12 3 (2𝑇2 )2
= √ 2 = √ 2 = 43 β‰ˆ 1.5874 …
π‘Ž2
𝑇2
𝑇2
2.
Kepler’s constant is: 𝐾 =
For Earth: 𝐾 =
𝐺𝑀
4πœ‹2
=
π‘Ž3
𝑇2
=
𝐺𝑀
4πœ‹2
6.67βˆ™10βˆ’11 βˆ™6βˆ™1024
4πœ‹2
π‘š3
β‰ˆ 1.014 βˆ™ 1013 (
𝑠2
)
Answer:
1)
π‘Ž1
π‘Ž2
β‰ˆ 1.5874 …
2) 𝐾 β‰ˆ 1.014 βˆ™ 1013
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