Calculate the force of gravity between Earth (mass = 6.0 * 10^24 kg) and the Sun (mass = 2.0×10^30 kg). The average Earth-Sun distance is 1.5×10^11 m..

F=G(m1xm2)/r^2=

=6.67•10^-11•(6•10^24•2•10^30)/(1.5•10^11)^1=3.56•10^22 N

Well, gravity between Earth and the Sun is no joke! But here's the punchline... To calculate the force of gravity, we can use the formula F = G * (m1 * m2) / r^2, where G is the gravitational constant, m1 and m2 are the masses of the two objects, and r is the distance between them.

So, plugging in the numbers, we get:

F = (6.67 × 10^(-11) N*(m^2)/(kg^2)) * (6.0 × 10^24 kg) * (2.0 × 10^30 kg) / (1.5 × 10^11 m)^2

Now, let me grab my calculator... Tada! After doing the math, we find that the force of gravity between Earth and the Sun is approximately 3.5 × 10^22 Newtons.

Now, that's one strong gravitational pull! But don't worry, the Sun doesn't steal Earth away... It's just playing a friendly cosmic game of tug-of-war!

To calculate the force of gravity between Earth and the Sun, you can use Newton's Law of Universal Gravitation formula:

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

Where:
F = force of gravity
G = gravitational constant (6.67430 × 10^-11 N(m/kg)^2)
m1 = mass of object 1 (Earth)
m2 = mass of object 2 (Sun)
r = distance between the centers of the two objects

Plugging in the given values:
m1 = 6.0 * 10^24 kg
m2 = 2.0 * 10^30 kg
r = 1.5 * 10^11 m

Let's calculate it step-by-step:

1. Calculate the product of the masses (m1 * m2):
m1 * m2 = (6.0 * 10^24 kg) * (2.0 * 10^30 kg)
= 1.2 * 10^55 kg^2

2. Calculate the square of the distance (r^2):
r^2 = (1.5 * 10^11 m)^2
= 2.25 * 10^22 m^2

3. Calculate the product of the gravitational constant and the product of the masses (G * m1 * m2):
G * m1 * m2 = (6.67430 × 10^-11 N(m/kg)^2) * (1.2 * 10^55 kg^2)
= 8.009160 × 10^44 N(m^2/kg)

4. Divide the product of G * m1 * m2 by the square of the distance to get the force of gravity:
F = (8.009160 × 10^44 N(m^2/kg)) / (2.25 * 10^22 m^2)

Simplifying the expression:
F = 3.559627 × 10^22 N

Therefore, the force of gravity between Earth and the Sun is approximately 3.56 × 10^22 Newtons.

To calculate the force of gravity between the Earth and the Sun, you can use Newton's Law of Universal Gravitation. According to this law, the force of gravity (F) between two objects is given by the equation:

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

Where:
- F is the force of gravity between the objects
- G is the gravitational constant (approximately 6.674 × 10^-11 N m^2 / kg^2)
- m1 and m2 are the masses of the two objects
- r is the distance between the centers of the two objects

Let's substitute the given values into the equation:

m1 = 6.0 × 10^24 kg (mass of the Earth)
m2 = 2.0 × 10^30 kg (mass of the Sun)
r = 1.5 × 10^11 m (distance between the Earth and the Sun)

Plugging in these values, we get:

F = (6.674 × 10^-11 N m^2 / kg^2) * (6.0 × 10^24 kg) * (2.0 × 10^30 kg) / (1.5 × 10^11 m)^2

Calculating this expression will give you the force of gravity between the Earth and the Sun.