Calculating the gravitational field due to a horizontal uniform thin disk

Click For Summary
SUMMARY

The gravitational field due to a horizontal uniform thin disk with thickness D, radius R, and density ρ at a distance h above its center is calculated using the formula 2πGρD(1-h/(R²+h²)¹/²). The discussion also addresses the effect of a 1cm thick lead layer (density 11350 kg/m³) on the timekeeping of a pendulum clock, specifically how many seconds it will gain per year. The gravitational potential is defined as φ=-Gdm/R, where dm=2πRDρdR, and the gravitational field is derived from the potential using g= -∇φ.

PREREQUISITES
  • Understanding of gravitational fields and potentials
  • Familiarity with calculus, specifically integration techniques
  • Knowledge of Newton's law of gravitation
  • Basic concepts of density and mass distribution
NEXT STEPS
  • Study the derivation of gravitational fields from mass distributions
  • Learn about the integration of functions in cylindrical coordinates
  • Explore the effects of density on gravitational potential
  • Investigate the relationship between gravitational fields and timekeeping in pendulum clocks
USEFUL FOR

Students in physics, particularly those studying gravitational fields, as well as educators and anyone interested in the practical implications of gravitational effects on timekeeping mechanisms.

AaronKnight
Messages
10
Reaction score
0

Homework Statement


Show that the gravitational field due to a horizontal uniform thin disc (thickness D, radius R and density r) at a distance h vertically above the centre of the disc has magnitude

2πGρd(1-h/(R2+h2)1/2)

A pendulum clock in the centre of a large room is observed to keep correct time. How many
seconds per year will the clock gain if the floor is covered by a 1cm thick layer of lead of density
11350kgm−3?
[Newton’s gravitational constant is G = 6.67×10−11Nm2 kg−2.]


Homework Equations


Gravitational potential, \phi=-Gdm/R
Where dm=2πRDρ.dR
Gravitational field, g= -\nabla\phi

The Attempt at a Solution


I have got to \phi=-2πDρGdR and I know I need to integrate with respect to R, then use the g= -\nabla\phi but I am unsure what my integration limits should be? I think I need to integrate between 0 and R but then I can't see how I would get the h/(R2+h2)1/2 term?
Any hints would be very useful.
 
Physics news on Phys.org
In the relevant equations sections ϕ=-Gdm/R should be dϕ=-Gdm/R
 

Similar threads

  • · Replies 17 ·
Replies
17
Views
2K
  • · Replies 5 ·
Replies
5
Views
3K
  • · Replies 23 ·
Replies
23
Views
5K
  • · Replies 8 ·
Replies
8
Views
2K
  • · Replies 5 ·
Replies
5
Views
3K
  • · Replies 2 ·
Replies
2
Views
2K
  • · Replies 1 ·
Replies
1
Views
1K
  • · Replies 15 ·
Replies
15
Views
2K
  • · Replies 7 ·
Replies
7
Views
4K
  • · Replies 16 ·
Replies
16
Views
2K