Question

In: Physics

Two neutron stars are separated by a distance of 1.0x1010 m. They each have a mass...

Two neutron stars are separated by a distance of 1.0x1010 m. They each have a mass of 1.0x1030 kg and a radius of 500000 m. They are initially at rest with respect to each other. As measured from the rest frame, how fast are they moving when their separation has decreased to one-half its initial value?

___________  m/s (The correct answer for this is 81663.94319)

How fast are they moving when they collide?
___________  m/s (I can't figure out this answer.)

Please use my numbers to work out the solution. Thanks!

Solutions

Expert Solution

m = 1*10^30 kg

r = 500000 m

distance of separation, d = 1*10^10 m

Initially the Potential energy of the two stars,

P.Ei = - G*m*m/r = -Gm^2/r

where G = Gravitational cosntant = 6.67*10^-11

So, P.Ei = -6.67*10^-11*(1*10^30)^2/(1*10^10)

So, P.Ei = -6.67*10^39 J

Now, after their separtion has been halved,

d' = 1*10^10/2 = 5*10^9 m

So, P.Ef = -G*m^2/d'

So, P.Ef = 6.67*10^-11*(1*10^30)^2/(5*10^9) = -1.33*10^40 J

So, By conservation of energy the P.E lost must be converted to Kinetic energy of the masses

So, P.Ei - P.Ef = K.E

So,  -6.67*10^39 - (-1.33*10^40) = 2*(0.5*m*v^2) <-------- v =speed of the masses

So, 6.63*10^39 = 1*10^30*v^2

So, v = 8.15*10^4 m/s <------------answer

2)

when they collide,

d' = 2*r = 2*500000 = 1*10^6 m

So, PEf = -Gm^2/d'

So, PEf = 6.67*10^-11*(1*10^30)^2/(1*10^6)

So, PEf = 6.67*10^43 J

So, By conservation of energy,

-6.67*10^39 - (-6.67*10^43) = 2*(0.5*1*10^30*v^2)

So, v = 8.17*10^6 m/s <-----------answer


Related Solutions

Neutron stars consist only of neutrons and have unbelievably high densities. A typical mass and radius...
Neutron stars consist only of neutrons and have unbelievably high densities. A typical mass and radius for a neutron star might be 3.7 x 1028 kg and 1.3 x 103 m. (a) Find the density of such a star. (b) If a dime (V = 2.0 x 10-7 m3) were made from this material, how much would it weight (in pounds)?
Two charges each +q are initially separated by a distance d. If you triple the distance,...
Two charges each +q are initially separated by a distance d. If you triple the distance, the magnitude of the force does what?
Neutron stars, such as the one at the center of the Crab Nebula, have about the...
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. Part A If you weigh 675 NN 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 21.0 kmkm ? Take the mass of the sun to be msms = 1.99×1030 kgkg , the gravitational constant to...
Two charges, 2.8 nC and 7.4 nC, are separated by a distance of 0.60 m. Where...
Two charges, 2.8 nC and 7.4 nC, are separated by a distance of 0.60 m. Where can you place a charge of 3.3 nC such that it won’t accelerate? Show your work.
Two circular plates each of radius R are separated by a distance of b. The space...
Two circular plates each of radius R are separated by a distance of b. The space between the plates is filled with a fluid. The upper plate moves downward at a constant rate V resulting in fluid being squeezed out between the plates. Determine the mass flow rate and maximum velocity under the following conditions: a) The exit velocity is uniform; b). The exit velocity is parabolic.
Two stars of mass M?1 and M?2<M?1 are orbiting eachother in a circular orbit. The heavy...
Two stars of mass M?1 and M?2<M?1 are orbiting eachother in a circular orbit. The heavy star experiences a supernova explosion, losing most of its mass in a spherically symmetric outflow (i.e. without losing angular momentum) and leaving behind a small neutron star of mass M??NS. Show that if the mass lost is larger then half of the total mass of the system, the binary is disrupted.
a) At what distance from a 2 solar mass neutron star would a planet like the...
a) At what distance from a 2 solar mass neutron star would a planet like the Earth be tidally disrupted (that is, literally pulled apart)? That is, how close would the planet need to be to the NS for the difference between the NS’s gravity at the center of the planet and at the surface of the planet to be greater than the gravity holding the planet together? b) Would the asteroid Pallas be able to get any closer? (Pallas...
Two tiny particles that have charges +20.0 μC and -8.00 μC are separated by a distance...
Two tiny particles that have charges +20.0 μC and -8.00 μC are separated by a distance of 20.0 cm. What is the magnitude and direction of the electric field halfway between these two charges? (k = 9.0 x 10 ^ 9 N x m ^ 2 / C ^ 2) a. 25.2 x 10 ^ 6 N/C, directed at the negative charge b. 25.2 x 10 ^ 6 N/C, directed at the positive charge c. 25.2 x 10 ^ 5...
Describe why some stars, such as white dwarfs and neutron stars become degenerate. What are the...
Describe why some stars, such as white dwarfs and neutron stars become degenerate. What are the two fundamental physics principles that underpin the concept of degeneracy?
(i) Why do neutron stars have a strong magnetic field if they are composed of neutrons,...
(i) Why do neutron stars have a strong magnetic field if they are composed of neutrons, which have no charge? (ii) What stabalizes these chargeless neutrons from decaying within the neutron star? (iii) How do neutron stars cool down? (iv) What can be learned about the interior of neutrons stars by measuring the temperatures of neutron stars?
ADVERTISEMENT
ADVERTISEMENT
ADVERTISEMENT