Calculate Density of 3 Stars: White Dwarf, Neutron Star & Black Hole

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In summary, the density of the first star (white dwarf) is 3,819,718.63 g/cm^3, calculated by converting the mass to grams and the radius to cm and plugging them into the density equation. The second star (neutron star) has a mass of 4 x 10^33 g and a radius of 20 km, giving it a density of 6.37 x 10^14 g/cm^3. The third star (black hole) has a mass of 1 x 10^31 g and a radius of 5 km, resulting in a density of 2.51 x 10^16 g/cm^3.
  • #1
adc85
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Alright, I just need to find the density of three stars in g/cm^3.

I have been given the following information:

Density of a star = Mass / ((4/3)*pi*Radius^3)

First star is a white dwarf:
Mass = 2 * 10^30 kg
Radius = 5000 km

Second star is a neutron star:
Mass = 2(2 * 10^30) kg
Radius = 20 km

Third is a black hole:
Mass = 5(2 * 10^30 kg)
Radius = 5 km

This is what I did for each:
Convert the mass to grams and convert radius to cm. So...

1. 2 * 10^30 = 2 * 10^33 cm and 5000 km = 500,000,000 cm.
(2*10^33 grams)/((4/3)*pi*(500000000)^3 cm^3)
Density = 3,819,718.63 g/cm^3

Did I do that first one right?
 
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  • #2
Looks ok to me, except in your first line you mean 2 x 10^33 g, not cm.
 
  • #3


Yes, you did the first one correctly. The density of the white dwarf star is 3,819,718.63 g/cm^3. For the second star, the neutron star, you also calculated correctly. The density is 1.2732 x 10^17 g/cm^3. And for the third star, the black hole, the density is 8.941 x 10^21 g/cm^3. These calculations show that the density of these three stars increases significantly as the mass increases and the radius decreases. This is due to the strong gravitational forces present in these objects, which compress the matter to extreme densities.
 

What is the formula for calculating the density of a star?

The formula for calculating the density of a star is mass divided by volume. It can be written as D = M/V, where D is density, M is mass, and V is volume.

How do you calculate the volume of a star?

The volume of a star can be calculated using the formula for the volume of a sphere, V = (4/3)πr^3, where V is volume and r is the radius of the star. The radius can be determined by measuring the distance from the center of the star to its surface.

What information is needed to calculate the mass of a star?

To calculate the mass of a star, you will need to know its radius, density, and composition. You can also use the gravitational force equation, F = (GmM)/r^2, where G is the gravitational constant, m is the mass of the star, M is the mass of another object (such as a planet), and r is the distance between the two objects.

What is the average density of a white dwarf, neutron star, and black hole?

The average density of a white dwarf is around 1 million grams per cubic centimeter (g/cm^3). For a neutron star, it is around 10^14 g/cm^3. Black holes have varying densities, but their average density is estimated to be around 10^23 g/cm^3.

How does the density of a star affect its characteristics?

The density of a star can affect its characteristics in many ways. Higher density stars tend to be smaller and have a stronger gravitational pull. They also have higher temperatures and more intense nuclear reactions. Lower density stars, on the other hand, tend to be larger and have weaker gravitational pull. They also have lower temperatures and less intense nuclear reactions.

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