What Are the Escape Velocities for Callisto and a Neutron Star?

In summary, the escape speed from (a) Jupiter’s moon Callisto is 2438.73 m/s, calculated using the equation v=sqrt(2GM/r) with G=6.67 x 10^-11, M=1.07 × 10^23 kg, and r=2.4 x 10^6 m. The escape speed from (b) a neutron star with twice the mass of the sun and a radius of 6 km is 297403171.9 m/s, calculated using the same equation with G=6.67 x 10^-11, M=3.9782 x 10^30 kg, and r=6000 m. It should also be noted
  • #1
warmfire540
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Determine the escape speed from (a) Jupiter’s moon Callisto with a mass of 1.07 × 10^23 kg and radius 2.4 Mm and (b) a neutron star twice the mass of the sun and a radius of 6 km.

I want to make sure I'm doing this and have the correct equations..

For part a)
Okay, so escape speed is found using the equation
v=sqrt(2GM/r)
G=6.67 x 10^-11
M=1.07 × 10^23
r=2.4 x 10^6

v=sqrt(1.427 x 10^13/2.4 x 10^6)
v=srt(5947416.667)
v=2438.73 m/s

For part b)
v=sqrt(2GM/r)
G=6.67 x 10^-11
M=2(1.9891 ×10^30) = 3.9782 x 10^30
r=6000

v=sqrt(5.301 x 10^20/6000)
v=sqrt(8.845 x 10^16)
v=297403171.9 m/s
 
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  • #2
Yep, you have the right formulae, and the right answers too.

and incase it is mentioned, your neutron star is VERY nearly a black hole too.
 
  • #3


Your calculations for both parts are correct. The escape velocity from Callisto is 2438.73 m/s and from the neutron star is 297403171.9 m/s. These calculations are important in understanding the minimum speed an object needs to escape the gravitational pull of a celestial body. It is also useful in spacecraft missions, as the escape velocity determines the amount of energy and fuel needed to leave a planet or moon's orbit. Additionally, these equations can also be used to calculate the escape velocity for other celestial bodies, providing valuable information for future space exploration.
 

1. What is escape velocity?

Escape velocity is the minimum speed that an object needs to achieve in order to escape the gravitational pull of a massive body, such as a planet or a star. It is the speed at which the object's kinetic energy is equal to its potential energy due to the gravitational force.

2. How is escape velocity calculated?

The escape velocity of an object can be calculated using the escape velocity equation:
Ve = √(2GM/r)
where Ve is the escape velocity, G is the gravitational constant, M is the mass of the massive body, and r is the distance from the center of the massive body to the object.

3. What is the significance of escape velocity?

Escape velocity is important because it determines whether an object can escape the gravitational pull of a massive body. If an object does not reach escape velocity, it will remain in orbit around the massive body. If an object exceeds escape velocity, it will leave the orbit and continue on its own trajectory.

4. Does escape velocity vary for different objects?

Yes, the escape velocity for an object depends on the mass and size of the massive body it is trying to escape from. For example, the escape velocity for Earth is 11.2 km/s, while the escape velocity for the Moon is only 2.4 km/s.

5. Can escape velocity be exceeded?

Yes, an object can exceed escape velocity if it receives an additional boost of energy, such as from a rocket. This will allow the object to escape the gravitational pull of the massive body and enter into space.

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