How Much Would You Weigh on a Neutron Star?

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SUMMARY

The discussion focuses on calculating weight on a neutron star, specifically one with the mass of the sun and a diameter of 16.0 km, such as the neutron star at the center of the Crab Nebula. The relevant gravitational formula is mg = (G * M * m_E) / (R_E)^2, which needs to be adapted for the neutron star by substituting M_E with M_n (mass of the neutron star) and R_E with R_n (radius of the neutron star). The gravitational constant G is given as 6.67×10-11 m3kg-1s-2, and the mass of the sun is 1.99×1030 kg. The weight on the neutron star can be calculated using these parameters.

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  • Understanding of gravitational force equations
  • Knowledge of mass and radius of celestial bodies
  • Familiarity with the gravitational constant (G)
  • Basic physics concepts related to weight and mass
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  • Calculate weight on a neutron star using the formula mg = (G * M_n * m) / (R_n)^2
  • Research the properties of neutron stars and their gravitational effects
  • Explore the differences between gravitational forces on Earth and neutron stars
  • Learn about the implications of extreme gravity on physical objects
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Students studying astrophysics, physics enthusiasts, and anyone interested in the effects of extreme gravitational forces on weight and mass.

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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 675 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 16.0 km?


Take the mass of the sun to be = 1.99×1030kg , the gravitational constant to be G= 6.67×10−11 , and the acceleration due to gravity at the Earth's surface to be g = 9.81


Homework Equations



mg=(Gmm_E)/(R_E)^2

I think??




The Attempt at a Solution



well I have not attempted it because the equation I have doesn't make sense when you include R_E^2 so I am unsure of the proper formulas??
 
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You need to change the M_e to M_n, the mass of the neutron star, and R_e to R_n, the radius of the neutron star. Everything should then work out fine.
 

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