How Would a Halved Sun Mass Alter Earth's Orbit?

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SUMMARY

If the mass of the Sun were suddenly reduced to half its current value, the Earth's orbit would transition to a parabolic trajectory. The total energy equation, E = (1/2)mv² - (GMm)/r, indicates that if the total energy equals zero, the orbit is parabolic. Calculating the escape velocity using v = √(GM/r) confirms that the Earth's average speed exceeds this value, leading to a parabolic orbit rather than a bound elliptical one. Analytical methods can further simplify the calculations by expressing the radius as a function of velocity.

PREREQUISITES
  • Understanding of gravitational potential energy and kinetic energy equations
  • Familiarity with orbital mechanics and parabolic trajectories
  • Knowledge of the escape velocity formula
  • Basic proficiency in algebra and calculus for analytical solutions
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  • Study the implications of reduced solar mass on planetary orbits using simulation tools
  • Explore the derivation of escape velocity in different gravitational contexts
  • Investigate the effects of varying mass on orbital stability and dynamics
  • Learn about the mathematical modeling of orbits using conic sections
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Astronomy students, astrophysicists, and educators interested in gravitational dynamics and orbital mechanics will benefit from this discussion.

AdkinsJr
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Homework Statement



If the mass of the sun were 1/2 it's current mass suddenly show the orbit of the Earth would be a parabola...

The Attempt at a Solution



I'm not sure what kind of approach to apply here, if the total energy equals zero then the orbit is a parabolic trajectory, if it is less than zero the the orbit is circular or elliptical, if I plug in numbers for the mass of the earth, sun, the radius and the average speed I can find escape velocity,

E=\frac{1}{2}mv^2 -\frac{GMm}{r}

and solve for the velocity v=\sqrt\frac{GM}{r}

and show that the Earth's average speed exceeds this value, but since these numbers are going to be approximations it's difficult to tell whether it should be parabola or bound orbit...E will not be exactly zero...
 
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AdkinsJr said:
and show that the Earth's average speed exceeds this value, but since these numbers are going to be approximations it's difficult to tell whether it should be parabola or bound orbit...E will not be exactly zero...
You can do it analytically, assuming Earth has a perfectly circular orbit* you can express the radius as function of the velocity (or vice versa) and calculate the total energy afterwards.

*otherwise the whole statement is not true anyway
 
That makes sense, by radius I presume you mean the orbital equations solns. Yeah I think that will simplify things down a bit. r(\theta)=\frac{\alpha}{1+e cos(\theta)}...for a circle e=o so r_c=\frac{ml^2}{k} where l=L/m and k=GMm

r_c=\frac{m(v_cr_c)^2}{GMm} if I solve for V_c I get v_c^2=\frac{GM}{r}

If I plug this into energy equation it does actually work when I plug in 1/2 M for the mass of the sun in the potential energy term.
 

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