Finding period of revolution of stars?

In summary, the conversation discusses the calculation of the period of revolution for two stars in a binary-star system. The stars have the same mass, which is 7.5 times that of the Sun, and they orbit around their center of mass. The distance between them is 7.5 times the distance between the Earth and the Sun. The equation used to calculate the period is T2=(4∏2/(GM))r3, where T is the period, G is the gravitational constant, M is the mass of the stars, and r is the distance between them. The correct answer for the period is 7.54 years. The confusion in the conversation arises from the fact that the orbital radius is not the same as
  • #1
rockchalk1312
38
0

Homework Statement


In a certain binary-star system, each star has the same mass which is 7.5 times of that of the Sun, and they revolve about their center of mass. The distance between them is the 7.5 times the distance between Earth and the Sun. What is their period of revolution in years?


Homework Equations


T2=(4∏2/(GM))r3


The Attempt at a Solution



multiplied mass of sun by 7.5 to get M, multiplied 1 amu by 7.5 to get r

T2=(4∏2/(6.67E-11)(1.491E31))x(1.125E12)3
T=2.38E8 seconds

changed this to years and got 7.54 years but this was the wrong answer.

Can anyone point out what I'm doing wrong? Thank you!
 
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  • #2
..."and they revolve about their center of mass"...
 
  • #3
...I wish I knew what that implies...
 
  • #4
The orbital radius is not the distance between the stars. They orbit about the center of mass.
 
  • #5
Doesn't that mean you have to know the radius of the stars themselves?
 
  • #6
rockchalk1312 said:
Doesn't that mean you have to know the radius of the stars themselves?

No. You need their masses and their separation...
 
  • #7
gneill said:
You need their masses and their separation.

But I used their masses--7 x that of the earth--and their separation is 7x the distance between the sun and the Earth (1 amu).
 
  • #8
Draw a picture. What point do they mutually orbit?
 

1. What is the period of revolution of a star?

The period of revolution of a star is the amount of time it takes for the star to complete one full orbit around its center of mass. This can vary depending on the mass of the star and its distance from its center of mass.

2. How is the period of revolution of a star calculated?

The period of revolution of a star can be calculated using Kepler's Third Law, which states that the square of a planet's orbital period is directly proportional to the cube of its average distance from the sun. This can be applied to stars as well, using the mass of the star and its distance from its center of mass.

3. Can the period of revolution of a star change over time?

Yes, the period of revolution of a star can change over time due to factors such as interactions with other stars or planets, changes in the star's mass or structure, and external influences like gravitational forces.

4. Why is it important to know the period of revolution of a star?

Knowing the period of revolution of a star can provide valuable information about its characteristics, such as its mass and distance from its center of mass. It can also help us understand the dynamics of the star's orbit and its interactions with other bodies in its system.

5. How do scientists measure the period of revolution of a star?

Scientists can measure the period of revolution of a star by observing its position and movement over time using telescopes and other instruments. They can also use data from observations of other bodies in the star's system to calculate the period of revolution. Additionally, data from satellite missions can provide more precise measurements of a star's period of revolution.

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