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quester [9]
4 years ago
6

Find a numerical value for ρearth, the average density of the earth in kilograms per cubic meter. use 6378km for the radius of t

he earth, g=6.67×10−11m3/(kg⋅s2), and a value of g at the surface of 9.80m/s29.80m/s2.

Physics
2 answers:
Rufina [12.5K]4 years ago
5 0

The average density of the earth is about 5.50 × 10³ kg/m³

\texttt{ }

<h3>Further explanation</h3>

Let's recall the Gravitational Force formula:

\boxed {F = G\ \frac{m_1 m_2}{R^2}}

<em>where:</em>

<em>F = Gravitational Force ( N )</em>

<em>G = Gravitational Constant ( = 6.67 × 10⁻¹¹ Nm²/kg² )</em>

<em>m = mass of object ( kg )</em>

<em>R = distance between object ( m )</em>

Let us now tackle the problem!

\texttt{ }

<u>Given:</u>

Radius of The Earth = R = 6378 km = 6378000 m

Gravitational Constant = G = 6.67 × 10⁻¹¹ Nm²/kg²

Gravitational Acceleration = g = 9.90 m/s²

<u>Asked:</u>

Average Density of the Earth = ρ = ?

<u>Solution:</u>

<em>Firstly , we will calculate the mass of the Earth as follows:</em>

g = G \frac{M}{R^2}

\boxed {M = \frac{g R^2}{G} } → <em>Equation 1</em>

\texttt{ }

<em>Next , we could calculate the average density of the Earth as follows:</em>

\rho = M \div V

\rho = (\frac{g R^2}{G}) \div ( \frac{4}{3} \pi R^3 )  ← <em>Equation 1</em>

\rho = \frac{3gR^2}{4 \pi G R^3}

\rho = \frac{3g}{4 \pi G R}

\rho = \frac{3 \times 9.80}{ 4 \pi \times 6.67 \times 10^{-11} \times 6378000 }

\boxed {\rho \approx 5.50 \times 10^3 \texttt{ kg/m}^3}

\texttt{ }

<h3>Learn more</h3>
  • Unit of G : brainly.com/question/1724648
  • Velocity of Runner : brainly.com/question/3813437
  • Kinetic Energy : brainly.com/question/692781
  • Acceleration : brainly.com/question/2283922
  • The Speed of Car : brainly.com/question/568302

\texttt{ }

<h3>Answer details</h3>

Grade: High School

Subject: Mathematics

Chapter: Gravitational Force

Andre45 [30]4 years ago
4 0

Answer:

5501 kg/m^3

Explanation:

The value of g at the Earth's surface is

g=\frac{GM}{R^2}=9.70 m/s^2

where G is the gravitational constant

M is the Earth's mass

R=6378km = 6.378 \cdot 10^6 m is the Earth's radius

Solving the formula for M, we find the value of the Earth's mass:

M=\frac{gR^2}{G}=\frac{(9.81 m/s^2)(6.378\cdot 10^6 m)^2}{6.67\cdot 10^{-11}}=5.98\cdot 10^{24}kg

The Earth's volume is (approximating the Earth to a perfect sphere)

V=\frac{4}{3}\pi r^3 = \frac{4}{3}\pi (6.378\cdot 10^6 m)^3=1.087\cdot 10^{21} m^3

So, the average density of the Earth is

\rho = \frac{M}{V}=\frac{5.98\cdot 10^{24} kg}{1.087\cdot 10^{21} m^3}=5501 kg/m^3

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Answer:

29.396988 m/s

Explanation:

Really, it depends on where the child is when he drops the ball - e.g., which planet he is on, and his distance from the center of that planet.

I'll assume that the child is on Earth at sea level at the equator, so that his distance from the geocenter is 6378000 meters.

The acceleration, g, is found from

g = GM/r²

G = 6.6743e-11 m³ kg⁻¹ sec⁻²

M = 5.9724e+24 kg

r = 6.378e+6 m

g = 9.799086 m sec⁻²

An approximate answer is found from an equation from constant acceleration kinematics:

v = gt

t = 3.0 sec

v = 29.397259 m/s

Now, the above method is an approximation that makes the technically incorrect assumption that the acceleration of gravity is a constant throughout the entire fall. You get away with it because the drop is very short. In another situation, it might not be. So it would be nice to develop a more accurate method that does not assume constant gravitational acceleration. For that, we begin with the Vis Viva equation:

v = √[GM(2/r − 1/a)]

Here,

a = the semimajor axis of a plunge orbit, which is equal to half of the apoapsis distance of 6378000+h, where

h = the altitude from which the ball is dropped

We can (using some math) develop the following equation:

t − t₀ = √[d/(2GM)] { √(rd−r²) + d arctan √(d/r−1) }

t − t₀ = 3 sec

r = 6378000 meters

d = r + h

Using an iterative method (e.g. Newton's or Danby's), we can determine that the altitude,

h = 44.0954 meters

So,

d = 6378044.09538 meters

a = d/2 = 3189022.04769 meters

Now we can calculate that

v = 29.396988 m/s

This is the more nearly correct answer because it takes into account the variability of the gravitational acceleration during the fall.

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