Center of mass of astroid

In summary, the center of mass of an asteroid is the point where the asteroid's mass is evenly distributed in all directions. It is calculated by taking into account the mass and position of all its individual components. The center of mass is important in studying asteroids as it helps us understand their overall structure and movement. It can change over time due to collisions or other factors. The center of mass is related to the asteroid's orbit as it is the point around which it orbits and influences its motion and trajectory.
  • #1
skrat
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Homework Statement


Find the center of mass of Astroid ##x^{\frac{2}{3}}+y^{\frac{2}{3}}=a^{\frac{2}{3}} ## for ##x,y\geq 0## and ##a>0##.

Homework Equations



##x_T=\frac{\int x\left | \dot{\vec{r}}(t) \right |}{\int \left | \dot{\vec{r}}(t) \right |}##

The Attempt at a Solution



##x^{\frac{2}{3}}+y^{\frac{2}{3}}=a^{\frac{2}{3}}##

##(\frac{x}{a})^{\frac{2}{3}}+(\frac{y}{a})^{\frac{2}{3}}=1##

Now is it ok to say that ##\frac{x}{a}=\cos^3t## and ##\frac{y}{a}=\sin^3t## for ##t\in \left [ 0,\frac{\pi }{2} \right ]##?

Now ##\left | \dot{\vec{r}}(t) \right |=3a \sint \cost##.

Than ##x_T=\frac{\int x\left | \dot{\vec{r}}(t) \right |}{\int \left | \dot{\vec{r}}(t) \right |}## can be written as

##x_T=\frac{\int_{0}^{\frac{\pi }{2}} 3a^2\cos^4t\sint}{\int_{0}^{\frac{\pi }{2}} 3a\cost\sint}=\frac{2}{5}a##

or... is that parameterization wrong?
 
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  • #2
skrat said:

Homework Statement


Find the center of mass of Astroid ##x^{\frac{2}{3}}+y^{\frac{2}{3}}=a^{\frac{2}{3}} ## for ##x,y\geq 0## and ##a>0##.


Homework Equations



##x_T=\frac{\int x\left | \dot{\vec{r}}(t) \right |}{\int \left | \dot{\vec{r}}(t) \right |}##

The Attempt at a Solution



##x^{\frac{2}{3}}+y^{\frac{2}{3}}=a^{\frac{2}{3}}##

##(\frac{x}{a})^{\frac{2}{3}}+(\frac{y}{a})^{\frac{2}{3}}=1##

Now is it ok to say that ##\frac{x}{a}=\cos^3t## and ##\frac{y}{a}=\sin^3t## for ##t\in \left [ 0,\frac{\pi }{2} \right ]##?

Now ##\left | \dot{\vec{r}}(t) \right |=3a \sint \cost##.

Than ##x_T=\frac{\int x\left | \dot{\vec{r}}(t) \right |}{\int \left | \dot{\vec{r}}(t) \right |}## can be written as

##x_T=\frac{\int_{0}^{\frac{\pi }{2}} 3a^2\cos^4t\sint}{\int_{0}^{\frac{\pi }{2}} 3a\cost\sint}=\frac{2}{5}a##

or... is that parameterization wrong?

Looks fine to me.
 

1. What is the center of mass of an asteroid?

The center of mass of an asteroid is the point where the asteroid's mass is evenly distributed in all directions.

2. How is the center of mass of an asteroid calculated?

The center of mass of an asteroid is calculated by taking into account the mass and position of all its individual components, such as rocks, dust, and gases.

3. Why is the center of mass important in studying asteroids?

The center of mass is important in studying asteroids because it helps us understand their overall structure and how they move through space.

4. Does the center of mass of an asteroid stay in the same place?

No, the center of mass of an asteroid can change over time as the asteroid's shape and composition can change due to collisions or other factors.

5. How is the center of mass of an asteroid related to its orbit?

The center of mass of an asteroid is related to its orbit because it is the point around which the asteroid orbits. It also influences the asteroid's motion and trajectory through space.

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