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agasfer [191]
3 years ago
12

If two forces are in the same direction then do they cancel each other out

Physics
1 answer:
stellarik [79]3 years ago
3 0
Im pretty sure that they do

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A 54.0-kg projectile is fired at an angle of 30.0° above the horizontal with an initial speed of 126 m/s from the top of a cliff
Nikolay [14]

Answer:

a) The initial total mechanical energy of the projectile is 498556.296 joules.

b) The work done on the projectile by air friction is 125960.4 joules.

c) The speed of the projectile immediately before it hits the ground is approximately 82.475 meters per second.

Explanation:

a) The system Earth-projectile is represented by the Principle of Energy Conservation, the initial total mechanical energy (E) of the project is equal to the sum of gravitational potential energy (U_{g}) and translational kinetic energy (K), all measured in joules:

E = U_{g} + K (Eq. 1)

We expand this expression by using the definitions of gravitational potential energy and translational kinetic energy:

E = m\cdot g\cdot y + \frac{1}{2}\cdot m\cdot v^{2} (Eq. 1b)

Where:

m - Mass of the projectile, measured in kilograms.

g - Gravitational acceleration, measured in meters per square second.

y - Initial height of the projectile above ground, measured in meters.

v - Initial speed of the projectile, measured in meters per second.

If we know that m = 54\,kg, g = 9.807\,\frac{m}{s^{2}}, y = 132\,m and v = 126\,\frac{m}{s}, the initial mechanical energy of the earth-projectile system is:

E = (54\,kg)\cdot \left(9.807\,\frac{m}{s^{2}}\right)\cdot (132\,m)+\frac{1}{2}\cdot (54\,kg)\cdot \left(126\,\frac{m}{s} \right)^{2}

E = 498556.296\,J

The initial total mechanical energy of the projectile is 498556.296 joules.

b) According to this statement, air friction diminishes the total mechanical energy of the projectile by the Work-Energy Theorem. That is:

W_{loss} = E_{o}-E_{1} (Eq. 2)

Where:

E_{o} - Initial total mechanical energy, measured in joules.

E_{1} - FInal total mechanical energy, measured in joules.

W_{loss} - Work losses due to air friction, measured in joules.

We expand this expression by using the definitions of gravitational potential energy and translational kinetic energy:

W_{loss} = E_{o}-K_{1}-U_{g,1}

W_{loss} = E_{o} -\frac{1}{2}\cdot m\cdot v_{1}^{2}-m\cdot g\cdot y_{1} (Eq. 2b)

Where:

m - Mass of the projectile, measured in kilograms.

g - Gravitational acceleration, measured in meters per square second.

y_{1} - Maximum height of the projectile above ground, measured in meters.

v_{1} - Current speed of the projectile, measured in meters per second.

If we know that E_{o} = 498556.296\,J, m = 54\,kg, g = 9.807\,\frac{m}{s^{2}}, y_{1} = 297\,m and v_{1} = 89.3\,\frac{m}{s}, the work losses due to air friction are:

W_{loss} = 498556.296\,J -\frac{1}{2}\cdot (54\,kg)\cdot \left(89.3\,\frac{m}{s} \right)^{2} -(54\,kg)\cdot \left(9.807\,\frac{m}{s^{2}} \right)\cdot (297\,m)

W_{loss} = 125960.4\,J

The work done on the projectile by air friction is 125960.4 joules.

c) From the Principle of Energy Conservation and Work-Energy Theorem, we construct the following model to calculate speed of the projectile before it hits the ground:

E_{1} = U_{g,2}+K_{2}+1.5\cdot W_{loss} (Eq. 3)

K_{2} = E_{1}-U_{g,2}-1.5\cdot W_{loss}

Where:

E_{1} - Total mechanical energy of the projectile at maximum height, measured in joules.

U_{g,2} - Potential gravitational energy of the projectile, measured in joules.

K_{2} - Kinetic energy of the projectile, measured in joules.

W_{loss} - Work losses due to air friction during the upward movement, measured in joules.

We expand this expression by using the definitions of gravitational potential energy and translational kinetic energy:

\frac{1}{2}\cdot m \cdot v_{2}^{2} = E_{1}-m\cdot g\cdot y_{2}-1.5\cdot W_{loss} (Eq. 3b)

m\cdot v_{2}^{2} = 2\cdot E_{1}-2\cdot m \cdot g \cdot y_{2}-3\cdot W_{loss}

v_{2}^{2} = 2\cdot \frac{E_{1}}{m}-2\cdot g\cdot y_{2}-3\cdot \frac{W_{loss}}{m}

v_{2} = \sqrt{2\cdot \frac{E_{1}}{m}-2\cdot g\cdot y_{2}-3\cdot \frac{W_{loss}}{m}  }

If we know that E_{1} = 372595.896\,J, m = 54\,kg, g = 9.807\,\frac{m}{s^{2}}, y_{2} =0\,m and W_{loss} = 125960.4\,J, the final speed of the projectile is:

v_{2} =\sqrt{2\cdot \left(\frac{372595.896\,J}{54\,kg}\right)-2\cdot \left(9.807\,\frac{m}{s^{2}} \right)\cdot (0\,m)-3\cdot \left(\frac{125960.4\,J}{54\,kg}\right)  }

v_{2} \approx 82.475\,\frac{m}{s}

The speed of the projectile immediately before it hits the ground is approximately 82.475 meters per second.

7 0
3 years ago
A solid steel sphere of density 7.86 g/cm3 and mass 1 kg spin on an axis through its center with a period of 2.3 s. given vspher
Alenkasestr [34]

<span>The solution for this problem is:</span>

density = mass / volume <span>
7860 = 1 / ((4/3) pi r^3) 
r^3 = 1 / (7860 * 4/3*pi) 
r = (1 / (7860 * 4/3*pi))^(1/3)</span>

= 0.067 m <span>

Inertia = (2/5)mr^2</span>

= (2/5) x 1 x 0.067^2

= 0.0017956 kg-m^2 <span>

1/2.3 = 0.4348 rev/s 

0.4348 x 2pi = 2.732 rad/s 

Angular momentum = Inertia x rad/s 

0.0017956 x 2.732 = 0.00490557 kg m^2/s</span>

4 0
3 years ago
You are building a uniform to protect workers from all types of nuclear radiation. If you use material that blocks _____ radiati
bearhunter [10]
If a material blocks gamma radiation, then it will probably protect against alpha and beta radiation. Alpha particles are large and slow-moving, thus having very little penetrating power. Beta particles are fast-moving, and can penetrate the human flesh up to 1 or 2 centimeters. Gamma particles, however, have great penetration and can easily pass through the human flesh.
3 0
3 years ago
What will happen two temperatures if you increase particle motion
nalin [4]

If the temperature is increased the particles gain more kinetic energy or vibrate faster. This means that they move faster and take more space.

8 0
3 years ago
Can someone give me 4 examples of comparing stars life cycle to mans life cycle
dexar [7]

Answer:

After formation, a star uses its fuel and burns brightly; however, upon the consumption of all of its fuel, the star is unable to maintain itself, just as the human body is. This causes the star to either collapse in on itself or burn out completely. Similarly, the life cycle of a human reaches its peak phase after a certain period of maturity and then becomes unable to maintain itself and deteriorates.  

Explanation:

3 0
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