he weight of a star is usually balanced by two forces: the gravitational force, acting inward, and the force created by nuclear reaction, acting outward. Over a long period of time, the force due to nuclear reactions gets weaker, causing the gravitational collapse of the star and crushing atoms out of existence. Under such extreme conditions, protons and electrons are squeezed to form neutrons, giving birth to a neutron star. Neutron stars are massively heavy-a teaspoon of the substance of a neutron star would weigh 100 million metric tons on the Earth. What is the value of g at the surface of this star? (You may enter your calculation using scientific notation.)
Question
he weight of a star is usually balanced by two forces: the gravitational force, acting inward, and the force created by nuclear reaction, acting outward. Over a long period of time, the force due to nuclear reactions gets weaker, causing the gravitational collapse of the star and crushing atoms out of existence. Under such extreme conditions, protons and electrons are squeezed to form neutrons, giving birth to a neutron star. Neutron stars are massively heavy-a teaspoon of the substance of a neutron star would weigh 100 million metric tons on the Earth. What is the value of g at the surface of this star? (You may enter your calculation using scientific notation.)
Solution
I'm sorry, but the question doesn't provide enough information to calculate the value of g (gravitational acceleration) at the surface of the neutron star. To calculate this, we would need to know the mass and radius of the neutron star. The formula to calculate the gravitational acceleration is g = GM/r^2, where G is the gravitational constant, M is the mass of the neutron star, and r is the radius of the neutron star.
Similar Questions
he weight of a star is usually balanced by two forces: the gravitational force, acting inward, and the force created by nuclear reaction, acting outward. Over a long period of time, the force due to nuclear reactions gets weaker, causing the gravitational collapse of the star and crushing atoms out of existence. Under such extreme conditions, protons and electrons are squeezed to form neutrons, giving birth to a neutron star. Neutron stars are massively heavy-a teaspoon of the substance of a neutron star would weigh 100 million metric tons on the Earth. Consider a neutron star whose mass is twice the mass of the Sun and whose radius is 12.1 km. (The mass of the Sun is 1.99 ⋅ 1030 kg1.99 · 1030 kg ) If it rotates with a period of 1.73 s, what is the speed of a point on the Equator of this star? (You may enter your calculation using scientific notation.) 4.395E4 Numeric ResponseEdit Unavailable. 4.395E4 correct.m/s
What is the value of g at the surface of this star? (You may enter your calculation using scientific notation
Whether or not a neutron star or a pulsar form depends on ...*1 pointThe mass of the original starWhether or not a supernova occurredWhether or not the object emits light and spinsNone of the above
Massive stars can become neutron stars, pulsars, or black holes.
The mass of the neutron is approximately equal to the mass of the: protonelectronnucleus
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