The mass of Earth can be calculated using the fact that the weight of an object (in newtons) is equal to the force of gravity between the object and Earth. Given that the radius of Earth is 6.4*10^6m , determine its mass

Hmmm. Several things are missing here.

mg = GmM/R^2

M=gR^2/G,
where
g=9.8 (m/s^2) ,
gravitational constant
G = 6.67•10^-11 (m^3•kg^-1•s^-2)

To determine the mass of Earth, we can use the equation for the force of gravity:

F = (G * m1 * m2) / r^2

Where:
F is the force of gravity
G is the gravitational constant (6.67430 × 10^-11 m^3 kg^-1 s^-2)
m1 and m2 are the masses of the two objects (in this case Earth and the object)
r is the distance between the centers of the two objects (in this case the radius of Earth)

Since we want to find the mass of Earth, we can rewrite the equation as:

m2 = (F * r^2) / (G * m1)

We know the weight of the object, which is equal to the force of gravity. The weight of an object is given by:

W = m * g

Where:
W is the weight of the object
m is the mass of the object
g is the acceleration due to gravity (approximately 9.8 m/s^2)

In this case, the object is Earth, so the weight of Earth is equal to:

W = m2 * g

Rearranging the equation, we can solve for m2:

m2 = W / g

Substituting this into the previous equation, we have:

m2 = (W * r^2) / (G * m1 * g)

The mass of Earth (m1) is what we want to find. Rearranging the equation, we can solve for m1:

m1 = (W * r^2) / (G * m2 * g)

Given that the radius of Earth is 6.4 * 10^6 m, we can plug in the values:

m1 = (W * (6.4 * 10^6)^2) / (6.67430 × 10^-11 * m2 * 9.8)

To calculate the mass of Earth using this method, we need to know the weight of an object and the force of gravity between the object and Earth. However, we don't have the weight of an object mentioned here.

To determine the mass of Earth, we can use a different approach known as the Cavendish experiment. This experiment measures the gravitational force between two objects, using their masses and the distance between their centers.

Here's a step-by-step approach to calculating the mass of Earth using the Cavendish experiment:

1. Measure the gravitational force between two objects:
- Set up an experiment with two small masses (M1 and M2) suspended from a lever or torsion balance.
- Measure the deflection of the torsion balance due to the gravitational attraction between the masses.
- Measure the distance (r) between the centers of the masses.

2. Calculate the gravitational force between the masses:
- Use Newton's law of gravitation: F = (G * M1 * M2) / r^2.
- G is the gravitational constant (approximately 6.67430 × 10^-11 N(m/kg)^2).

3. Calculate the mass of Earth:
- Rearrange the equation to solve for the mass of Earth:
Mass of Earth = (F * r^2) / (G * M1).

Please note that performing the Cavendish experiment requires precise measurements and controlled conditions. It is typically done in a laboratory setting by scientists with specialized equipment.

Using this method, the mass of Earth has been estimated to be approximately 5.9722 × 10^24 kilograms.