Weight on a neutron star ( universal gravity)

In summary, a neutron star has the same mass as our sun but a much smaller diameter. Using the given values, a person with a weight of 650 N on Earth would have a weight of approximately 3.527 x 10^12 N on the surface of a neutron star with a diameter of 15.0 km. This was calculated using the equation F = GMm/r^2 and the given values for the mass of the sun, gravitational constant, and acceleration due to gravity on Earth. The calculation may need to be double-checked for accuracy.
  • #1
tnutty
326
1

Homework Statement



Neutron stars, such as the one at the center of the Crab Nebula, have about the same mass as our sun but a much smaller diameter.

If you weigh 650 N on the earth, what would be your weight on the surface of a neutron star that has the same mass as our sun and a diameter of 15.0 km ?

Take the mass of the sun to be = 1.99×1030 kg , the gravitational constant to be
G = 6.67×10−11 , and the acceleration due to gravity at the Earth's surface to be
g = 9.810 .

Express your weight W_star in Newtons.

Homework Equations



F = GMm/r^2

The Attempt at a Solution



mg = w
mg = 650
m = 650/g = 650 / 9.810 = mass of you

F = GMm/r^2

ma = GMm/r^2

a = GM/r^2 = acceleration in the neutron star.

F = ma;

= Mass of you * acceleration in neutron star

where

acceleration in neutron star =

[ 6.67 * 10^-11 * 1.99 * 10^30 ] / r^2--(or D/2)^2

=

6.67 * 10^-11 * 1.99*10^30 / 7500^2
~ 3.527 x 10^12


so

w = mg
= 650/9.81 * (3.527 * 10^12)

is this right, can you check my calculation?
 
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  • #2
I got it, thanks fooorrrr alll yoouuuurrrrr heeeellllppppp guuuuuuyyyysss
(cough*sarcasm*cough).
 
  • #3


Your calculations are correct. However, it is important to note that the weight on a neutron star would not be the same as the weight on Earth, as the gravitational force depends not only on mass and radius, but also on the gravitational constant. Therefore, a more accurate calculation would be to use the equation F = G(Mm)/r^2, where M is the mass of the neutron star and m is your mass. This would give a weight of approximately 2.9 x 10^12 N on the surface of the neutron star. This difference in weight is due to the much stronger gravitational pull on the surface of a neutron star compared to Earth.
 

Related to Weight on a neutron star ( universal gravity)

What is a neutron star?

A neutron star is a type of celestial object that is formed when a massive star collapses in on itself. It is incredibly dense, with a mass greater than the sun but compressed into a much smaller size, typically around 12 miles in diameter.

How does the weight on a neutron star compare to Earth?

The weight on a neutron star is incredibly high due to its immense gravitational pull. On Earth, we measure weight in terms of the force of gravity pulling on an object, and this force is dependent on the mass of the object and the distance from the center of the planet. On a neutron star, the mass is much greater and the distance from the center is much smaller, resulting in a much higher weight.

What is universal gravity?

Universal gravity is a physical law that explains the force of attraction between two objects with mass. It states that every object in the universe attracts every other object with a force that is directly proportional to the product of their masses and inversely proportional to the square of the distance between them.

How does the gravitational pull on a neutron star affect its weight?

The immense gravitational pull on a neutron star is what gives it its incredibly high weight. The force of gravity on a neutron star is more than a billion times stronger than on Earth, resulting in an enormous weight that is difficult for us to comprehend.

Can anything escape the gravitational pull of a neutron star?

No, nothing can escape the gravitational pull of a neutron star. This includes light, which is the fastest thing in the universe. The gravitational pull is so strong that it warps the fabric of space-time, making it impossible for anything to escape once it gets within a certain distance from the star's center, known as the event horizon.

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