Calculating Mass and Density of Planets in Our Solar System

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In summary, the mass and density of planets in our solar system can be calculated using their orbits and the orbits of any moons they may have. This can be achieved by measuring the distance between the planet and its moon, and the time it takes for the moon to orbit. The mass of the planet can then be determined using the formula: time = 2π√(radius^3 / GM). However, to measure the mass of a moon, an object must be put into orbit around it.
  • #1
bassist_13
How do we know the mass and density of the planets in our solar system?
My physics teacher at college said that they were calculated using their orbits and the orbits of any moons they may have, but did not go into any more detail than that.
 
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  • #2
You can easily measure the mass of an object if anything else is orbiting around it.
All you need to know is the distance between the planet and it's moon and the time it takes the moon to go around.
You don't need to know the mass of the moon (assuming it's much less than the planet), this means you can't use the orbit to work out the mass of the orbiting object.
so we can use the Earth's orbit around the sun to work out the mass of the Sun but not the mass of the Earth, we can then use the Moon's orbit around the Earth to work out the mass of the Earth but not the moon. To measure the mass of the moon we have to put something else in orbit around it - like a spaceship

If your interested the formula is
time =[tex] 2\pi \sqrt{radius^3 / GM }[/tex]

Where M is the mass of the planet
 
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  • #3
Thank you, that has cleared that up for me :smile:
 

1. How do you calculate the mass of a planet?

The mass of a planet can be calculated by using Newton's law of gravitation: M = (r3 * G) / (4π2 * T2), where M is the mass of the planet, r is its average distance from the Sun, G is the gravitational constant, and T is its orbital period around the Sun.

2. What is the formula for calculating density of a planet?

The formula for calculating density of a planet is: D = M / V, where D is density, M is mass, and V is volume. The mass of a planet can be calculated using the formula mentioned in the previous question, and its volume can be determined by measuring its diameter and assuming it is a perfect sphere.

3. How do you measure the diameter of a planet?

The diameter of a planet can be measured using a variety of methods, including spacecraft flybys, radar measurements, and telescopic observations. These methods allow for accurate measurements of a planet's size and shape.

4. Why is calculating mass and density of planets important?

Calculating the mass and density of planets is important because it helps us understand the composition and structure of our solar system. It also allows us to compare and contrast different planets, and can provide insights into their formation and evolution.

5. What is the average density of planets in our solar system?

The average density of planets in our solar system varies greatly, with gas giants like Jupiter having a low density of 1.33 g/cm3 and terrestrial planets like Earth having a higher density of 5.51 g/cm3. The average density of all the planets in our solar system is approximately 1.32 g/cm3.

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