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TiliK225 [7]
3 years ago
10

A cosmic ray electron moves at 7.45 â 106 m/s perpendicular to the earth's magnetic field at an altitude where field strength is

1.10 â 10â5 t. what is the radius (in m) of the circular path the electron follows?
Physics
1 answer:
kupik [55]3 years ago
6 0
The magnetic force on the electron is:
F=qvB \sin \theta
where q is the electron charge, v the electron speed, B the magnetic field intensity and \theta is the angle between v and B. Since the electron is traveling perpendicular to the magnetic field, \sin \theta = \sin 90^{\circ}=1, so we can write 
F=qvB

This force acts as centripetal force of the motion, F_c = m \frac{v^2}{r}, where m is the electron mass and r the radius of the circular orbit. So we can write:
qvB=m \frac{v^2}{r}
and by re-arranging this equation, we find the radius of the circular orbit, r:
r= \frac{mv}{qB}= \frac{(9.1 \cdot 10^{-31}kg)(7.45 \cdot 10^6 m/s)}{(1.6 \cdot 10^{-19}C)(1.10 \cdot 10^{-5}T)}=  3.85 m
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A ball rolls onto the path of your car as you drive down a quiet neighborhood street. To avoid hitting the child that runs to re
Ilya [14]

Answer:

a) F = -1035.385 N

b) Backwards

c) s = 15.60 m

Explanation:

Given information

u = Initial Speed of Car = 15.0 m/s

v = Final Speed of Car = 9.00 m/s

t_{b} = Breaking Time = 1.30 s

m = Mass of Car = 1040 kg

Part (a)

To find the force exerted on the car we use the following formula

F = ma

Where

F = Force = unknown

m = Mass of Car = 1040 kg

a = Acceleration of Car / Deceleration of Car = unknown

To find the force (F) we need to first find the deceleration rate (a)

To find the deceleration rate we use the following formula

a = \frac{v - u}{t}

Inputting the given values

a = \frac{15 - 9}{1.30} \\ a = -4.615

To find the force

F = ma \\ F = (1040)(-4.615) \\ F = (1040)(-4.615) \\ F = -1035.385 N

Part (b)

Since the value of F is negative this means the the force was opposite the direction of motion, hence the force was backwards.

Part (c)

To find the total distance the car moved while braking we use the following formula

v^2 = u^2 + 2as

Where

s = distance traveled

Inputting the values given

(9)^2 = (15)^2 + 2(-4.615)s

s = 15.60 m

6 0
3 years ago
a length of wire is cut into five equal pieces. the five pieces are then connected in parallel, with the resulting resistance be
Natali [406]
The equivalent resistance of n resistors connected in parallel is given by
\frac{1}{R_{eq}} =  \frac{1}{R_1}+ \frac{1}{R_2}+...+ \frac{1}{R_n} (1)

In our problem, the resulting resistance of the 5 pieces connected in parallel is R_{Eq}=2.00 \Omega, and since the 5 pieces are identical, their resistance R is identical, so we can rewrite (1) as
\frac{1}{R_{Eq} }= \frac{1}{2 \Omega}= \frac{1}{R}+ \frac{1}{R}   + \frac{1}{R}   + \frac{1}{R}   + \frac{1}{R}   =  \frac{5}{R}
From which we find R= 5 \cdot 2 \Omega = 10 \Omega.

So, each piece of wire has a resistance of 10 \Omega. Before the wire was cut, the five pieces were connected as they were in series. The equivalent resistance of a series of n resistors is given by
R_{Eq}=R_1 + R_2 + ...+R_n
So if we apply it at our case, we have
R_{eq}=R+R+R+R+R=5 R= 5\cdot 10 \Omega= 50 \Omega

therefore, the resistance of the original wire was 50 \Omega.
5 0
3 years ago
I believe that our solar system formed by the same process as star formation. A huge cloud of dust and gas collapsed and condens
xz_007 [3.2K]

Nebular hypothesis.

Explanation:

  • The first version of the nebula hypothesis was proposed by Immanuel Kant and Pierre Laplace.
  • Today the hypothesis has been revised to fit into more current and update realities about how our solar system emerged.
  • The hypothesis is the widely accepted explanation to the origin and evolution of the solar system.
  • It suggests that the star and the planets that makes up the solar system were products of a huge cloud of dust called the nebular.
  • The nebular is a huge mass of interstellar dusts.
  • The cloud collapsed and condensed under gravitational pull of the materials.
  • A center core that resulted in the formation of our star, sun emerged and the rest of the particles formed our planet.

Learn more:

The sun energy brainly.com/question/1140127

#learnwithBrainly

4 0
4 years ago
When designing an experiment a benefit of larger sample sizes would be more____. A.variables B.representative data C.time per gr
castortr0y [4]
<span>When designing an experiment a benefit of larger sample sizes would be more representative data. This larger sample size would lead to perfect result. The correct option among all the options that are given in the question is the second option or option "B". I hope the answer comes to your help.</span>
5 0
3 years ago
Read 2 more answers
In physics class, Carrie learns that a force, F, is equal to the mass of an object, m, times its acceleration, a. She writes the
Phantasy [73]

Answer:

2.2 m/s^2

Explanation:

Acceleration = Force / Mass

= 7.92 / 3.6 = 2.2m/s^2

Hope this help you :3

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3 years ago
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