Calculate gravitational acceleration in a vacuum?

In summary: The uncertainty in f can be computed using either absolute or statistical uncertainty. To compute absolute uncertainty, use the total difference equation given. To compute statistical uncertainty, use a root-sum-square formula.
  • #1
rockchalk1312
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The gravitational acceleration in vacuum varies with latitude, elevation, and local inhomogeneities in the Earth's crust. Use the following equation to find g in Lawrence based on a latitude of λ=38°57' ±3' and an elevation of H=259±10m. Calculate the uncertainty using the total difference.g = 9.780556m/s2[1+0.0052885sin2λ-0.0000059sin2(2λ)]-0.0000020s-2HHow do you include latitude when it's at three different dimensions? And I know the total difference formula but how would you put it in here exactly? Thank you very much for any help!
 
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  • #2
rockchalk1312 said:
The gravitational acceleration in vacuum varies with latitude, elevation, and local inhomogeneities in the Earth's crust. Use the following equation to find g in Lawrence based on a latitude of λ=38°57' ±3' and an elevation of H=259±10m. Calculate the uncertainty using the total difference.


g = 9.780556m/s2[1+0.0052885sin2λ-0.0000059sin2(2λ)]-0.0000020s-2H


How do you include latitude when it's at three different dimensions? And I know the total difference formula but how would you put it in here exactly? Thank you very much for any help!

The latitude is being expressed in degrees (°), arcminutes ('), and arcseconds ("), where:

1 arcmin = (1/60) degrees

1 arcsec = (1/60) arcmins
 
  • #3
I assume that's a formula you've been given, so it's obvious how to use the latitude and altitude in computing g. That leaves me not knowing what you're asking. Are you puzzled as to how the formula can be valid?
When asked to compute an uncertainty in f=f(x,y,..), given the uncertainties in x, y..., there are two principal methods producing different answers: absolute uncertainty and statistical uncertainty. The first is appropriate when the given uncertainties are absolute uncertainties with uniform distributions (as often is the case with instrumental measurements), there are only two or three parameters, and the answer is to be relied on absolutely, as may be the case in structural engineering. In this method, just plug in all the combinations of extreme values for the parameters and see what f values come out.
For statitical uncertainty you assume the given uncertainties are some number of standard deviations, the same number in each parameter, or otherwise convert to that form. You may then be able to use a root-sum-square formula to combine them, and the answer will represent the same number of standard deviations for f.
E.g. if f=x*y, Δf = xΔy+yΔx; E[(Δf)2] = E[x2]Δy2+E[y2]Δx2; σ(f)/f = √((σ(x)/x)2+(σ(y)/y)2).
More generally, Δf = (∂f/∂x)Δx+(∂f/∂y)Δy, etc.
 

1. What is gravitational acceleration in a vacuum?

Gravitational acceleration in a vacuum is a constant value that represents the rate at which objects accelerate towards each other due to the force of gravity. It is denoted by the symbol "g" and is approximately equal to 9.8 m/s^2 on Earth.

2. How do you calculate gravitational acceleration in a vacuum?

To calculate gravitational acceleration in a vacuum, you can use the formula g = G * M / r^2, where G is the universal gravitational constant, M is the mass of the larger object, and r is the distance between the two objects. Alternatively, you can also use the formula g = F / m, where F is the force of gravity and m is the mass of the object.

3. What is the difference between gravitational acceleration in a vacuum and on Earth?

The main difference between gravitational acceleration in a vacuum and on Earth is that the former is a constant value, while the latter may vary depending on the location and mass of the objects involved. In a vacuum, there are no external factors affecting the acceleration, whereas on Earth, factors such as air resistance and the planet's rotation can impact the value of gravitational acceleration.

4. Why is gravitational acceleration in a vacuum important?

Gravitational acceleration in a vacuum is important because it helps us understand and predict the motion of objects in space. It also plays a crucial role in the laws of motion and the theory of gravity formulated by Sir Isaac Newton. Additionally, it is necessary for many scientific calculations and experiments related to space exploration.

5. Does gravitational acceleration in a vacuum vary in different parts of the universe?

Yes, gravitational acceleration in a vacuum can vary in different parts of the universe due to the presence of different masses and distances between objects. For example, the value of g on the surface of the moon is approximately 1.6 m/s^2, while on the surface of Jupiter it is around 24.8 m/s^2. However, it is considered a constant value in a specific location in space, known as the standard gravitational parameter.

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