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g100num [7]
3 years ago
10

UniformDefine, velocity with an encomple.​

Physics
1 answer:
spin [16.1K]3 years ago
8 0
I’m a bit confused on your question but i believe you’re asking to define uniform velocity, which is the condition which a body covers equal distance in an equal interval of the time is known as uniform velocity. an example would be when a truck travels in equal distances in equal intervals of time then we say the body has a uniform velocity
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50 points!!! Kinetics
iris [78.8K]

Answer:

98 m √

Explanation:

How about s = Vo * t + ½at² ?

s = h = Vo * 2s - 4.9m/s² * (2s)² = 2Vo - 19.6

and

h = Vo * 10s - 4.9m/s² * (10s)² = 10Vo - 490

Subtract 2nd from first:

0 = -8Vo + 470.4

Vo = 58.8 m/s

h = 58.8m/s * 2s - 4.9m/s² * (2s)² = 98 m

3 0
3 years ago
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What is an atom? Give three 3 examples.​
Assoli18 [71]

Answer:

<u>Atom</u><u> </u><u>is </u><u>particle</u><u> </u><u>of </u><u>matter</u><u> </u><u>that </u><u>uniquely</u><u> </u><u>defines</u><u> </u><u>a</u><u> </u><u>chemical</u><u> </u><u>element</u><u>.</u>

Examples of atom:

  • Hydrogen [ H]
  • Neon [Ne]
  • Argon [A]
  • Iron [Fe]
  • Calcium [Ca]

<h3>About Atom:</h3>

Atom consists of a central nucleus that is usually surrounded by one or more electrons .Each electron is negatively charged. The nucleus is positively charged and contains one or more relatively heavy particles known as protons and neutrons.

An early model of the atom was developed by the physicist Ernest Rutherford in 1913. He was the first to suggest that atoms are like miniature solar systems except that the attractive force is not caused by gravity, but by opposing electrical charged.

Hope this helps....

Good luck on your assignment...

8 0
3 years ago
If a layer was deposited but does not appear in the rock record, what has occured
nalin [4]
I think you forgot to give the choices along with the question. I am answering the question based on my research and knowledge. <span>If a layer was deposited but does not appear in the rock record, the thing that happened is erosion. I hope that this is the ans wer that has actually come to your desired help.</span>
5 0
3 years ago
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Why so much space in the solar system?
polet [3.4K]

Answer:

To avoid collision, you know.

4 0
2 years ago
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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
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