Mass of a star given orbital radius and period

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Homework Help Overview

The problem involves determining the mass of a star based on the orbital radius and period of a planet orbiting it. The context is rooted in celestial mechanics and gravitational interactions.

Discussion Character

  • Exploratory, Assumption checking, Conceptual clarification

Approaches and Questions Raised

  • Participants express uncertainty about how to begin the problem, particularly regarding the relevance of the planet's mass. There are discussions about the forces acting on the planet and the relationship between orbital motion and forces. Some participants suggest considering centripetal force and its relation to orbital parameters.

Discussion Status

The discussion is active, with participants exploring different angles of the problem. Some guidance has been offered regarding the use of centripetal force and Kepler's laws, though there is no explicit consensus on the approach yet.

Contextual Notes

Participants note the potential oversight of prior knowledge regarding Kepler's laws, which may be necessary for solving the problem. There is also a mention of the relative insignificance of the planet's mass compared to that of the star.

disque
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Homework Statement


In recent years, a number of nearby stars have been found to possesses planets. Suppose, the orbital radius of such a planet is found to be 4.3 times 1011 m, with a period of 1080 days. Find the mass of the star.


Homework Equations


?


The Attempt at a Solution


I don't even know where to start with this question. Without the mass of the planet I am clueless. ANy help would be much appreciated, Thanks a lot.
 
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disque said:

Homework Statement


In recent years, a number of nearby stars have been found to possesses planets. Suppose, the orbital radius of such a planet is found to be 4.3 times 1011 m, with a period of 1080 days. Find the mass of the star.


Homework Equations


?


The Attempt at a Solution


I don't even know where to start with this question. Without the mass of the planet I am clueless. ANy help would be much appreciated, Thanks a lot.
Let's start by looking at what interactions are relevant. So erm what are the relevant interactions? Or more to the point, what forces are acting on our planet?
After that we'll need to see what the motion of the planet means in terms of forces. So again can you think of a relation between the period, mass and radius for an object in circular motion to the force exerted on it?
after that we should be at a point to get an answer after a bit of algebra
 
(mv^2)/r
am i on the right track?
 
disque said:
(mv^2)/r
am i on the right track?

So that's the equation for the centripetal force, you will need to relate v to the period and radius. Also you need to recognize what force is causing the circular motion and what the equation for that force is
 
Look up "Kepler's third law" in the index of your book. You are given numbers to substitute into the formula.
 
I'm surprised they've not covered Kepler's laws first? Did you skip a chapter?

Seems a little advanced to expect you to know how to find mass without it?

You don't really need to know the mass of the planet since it will be much smaller than the star generally so you can approximate it ignoring the planets mass to all intents and purposes.

Even Jupiter's mass is only ~1/1000 of the Suns.
 
Last edited:

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