Problem 33
Question
\(320 \mathrm{~km}\) above the surface of earth, the value of acceleration due to gravity is nearly \(90 \%\) of its value on the surface of the earth. Its value will be \(95 \%\) of the value on the earth's surface (a) nearly \(160 \mathrm{~km}\) below the earth's surface (b) nearly \(80 \mathrm{~km}\) below the earth's surface (c) nearly \(640 \mathrm{~km}\) below the earth's surface (d) nearly \(320 \mathrm{~km}\) below the earth's surface
Step-by-Step Solution
Verified Answer
Option (d): nearly 320 km below the Earth's surface.
1Step 1: Understanding gravity above the surface
The acceleration due to gravity at a height above the Earth's surface, like 320 km, is given by the formula \( g_h = g_0 \left(\frac{R}{R+h}\right)^2 \) where \( g_0 \) is the gravitational acceleration on the surface, \( R \) is the Earth's radius, and \( h \) is the height above the surface. For 320 km, \( g_h = 0.9g_0 \). This is our reference point.
2Step 2: Understanding gravity below the surface
The acceleration due to gravity below the Earth's surface can be approximated by \( g_d = g_0 \left(1- \frac{d}{R} \right) \) where \( d \) is the depth below the surface. At this point, we know \( g_d = 0.95 g_0 \).
3Step 3: Set up the equation for below the surface
Using the formula \( g_d = g_0 \left(1- \frac{d}{R} \right) = 0.95 g_0 \), we can set up the equation \( 1- \frac{d}{R} = 0.95 \).
4Step 4: Solve for the depth (d)
From the equation \( 1 - \frac{d}{R} = 0.95 \), we rearrange to find \( \frac{d}{R} = 0.05 \). Therefore, \( d = 0.05R \). Assuming \( R \approx 6400 \text{ km} \), the depth \( d \approx 0.05 \times 6400 = 320 \text{ km} \).
5Step 5: Identify the correct option
The calculated depth of 320 km below the Earth's surface matches the condition where gravity is 95% of its surface value. Hence, option (d) nearly matches our calculation.
Key Concepts
gravity variationsEarth's radiusgravitational formulas
gravity variations
Gravity doesn't remain constant across different locations on Earth and changes based on several factors. These variations can happen due to changes in elevation, latitude, and local geological structures. When you are above or below the Earth's surface, the gravitational pull could be weaker or stronger, respectively.
- **Above the surface**: Higher altitudes, such as those experienced in high mountains or airplanes, mean you are further from Earth's center. Here, gravity weakens and you weigh a tiny bit less.
- **Below the surface**: When you dig deeper into Earth, you get closer to the massive central core. As a result, gravity can become stronger because there is more mass above you exerting a pull.
Understanding these gravity variations helps explain why certain locations on Earth have slightly different gravitational forces. This is crucial for applications in geophysics and engineering.
- **Above the surface**: Higher altitudes, such as those experienced in high mountains or airplanes, mean you are further from Earth's center. Here, gravity weakens and you weigh a tiny bit less.
- **Below the surface**: When you dig deeper into Earth, you get closer to the massive central core. As a result, gravity can become stronger because there is more mass above you exerting a pull.
Understanding these gravity variations helps explain why certain locations on Earth have slightly different gravitational forces. This is crucial for applications in geophysics and engineering.
Earth's radius
The radius of Earth is an essential parameter for calculating gravitational acceleration. Earth's average radius is approximately 6400 kilometers. This value is fundamental for applying the gravitational formula to predict how gravity changes with altitude and depth.
- At **sea level**, the radius is typically measured from the center of Earth to that point on the surface.
- When you travel **above** the surface, the radius becomes the distance from Earth's center to the point of interest above the surface.
- Similarly, **under the surface**, the radius still extends from the center to where you are below the surface level.
Using Earth's radius in our calculations helps determine how the gravitational force diminishes with height or increases with depth. This knowledge is utilized by scientists and engineers in fields such as satellite launching and underground exploration.
- At **sea level**, the radius is typically measured from the center of Earth to that point on the surface.
- When you travel **above** the surface, the radius becomes the distance from Earth's center to the point of interest above the surface.
- Similarly, **under the surface**, the radius still extends from the center to where you are below the surface level.
Using Earth's radius in our calculations helps determine how the gravitational force diminishes with height or increases with depth. This knowledge is utilized by scientists and engineers in fields such as satellite launching and underground exploration.
gravitational formulas
Gravitational formulas play a vital role in evaluating how gravity differs with position relative to Earth. The two key formulas are for calculating gravity above and below the surface.
### Above the SurfaceThe formula to calculate gravity above the surface is \[ g_h = g_0 \left(\frac{R}{R+h}\right)^2 \] where:
### Below the SurfaceWhen you're below the surface, gravity is computed using the formula:\[ g_d = g_0 \left(1 - \frac{d}{R} \right) \] with:
### Above the SurfaceThe formula to calculate gravity above the surface is \[ g_h = g_0 \left(\frac{R}{R+h}\right)^2 \] where:
- \(g_h\) is the gravity at height \(h\)
- \(g_0\) is the gravity at Earth's surface
- \(R\) is Earth's radius, and
- \(h\) is the height above the surface
### Below the SurfaceWhen you're below the surface, gravity is computed using the formula:\[ g_d = g_0 \left(1 - \frac{d}{R} \right) \] with:
- \(g_d\) as gravity at depth \(d\)
- \(g_0\) as surface gravity
- \(d\) as depth beneath the surface
Other exercises in this chapter
Problem 32
If \(M\) mass of the square plate before cutting the holes, then mass of portion of each hole. $$ m=\frac{M}{16 R^{2}} \times \pi R^{2}=\frac{\pi}{16} M $$ \(\t
View solution Problem 32
A spaceship is stationed on mars. How much energy must be expended on the spaceship to rocket it out of the solar system? Mass of the spaceship \(=1000 \mathrm{
View solution Problem 33
A planet of mass \(m\) is revolving round the sun (of mass \(m_{s}\) ) in an elliptical orbit. If \(\mathbf{v}\) is the velocity of the planet when its position
View solution Problem 34
The acceleration due to gravity at a height \(1 / 20\) th of the radius of the earth above the earth surface is \(9 \mathrm{~ms}^{-2}\). Its value at a point at
View solution