what happens to the domains of an object when it becomes magnetized?

Answers

Answer 1

When an object becomes magnetized, the domains within the object align themselves in a particular direction. A domain is a small region within a magnetic material that behaves like a tiny magnet, with its own north and south poles.

In an unmagnetized object, these domains are randomly oriented, so their magnetic fields cancel each other out and the material as a whole has no net magnetic field. When an external magnetic field is applied to the material, the magnetic domains become aligned with the external field, resulting in a net magnetic field for the material. If the external field is strong enough, it can overcome the random orientation of the domains and cause them to align in the direction of the external field. Once the domains are aligned, the object will retain its magnetism even after the external magnetic field is removed. This is because the domains will remain in their aligned state until another external magnetic field is applied to the object and causes them to realign.

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Related Questions

A straight 2.40 m wire carries a typical household current of 1.50 A (in one direction) at a location where the earth's magnetic field is 0.550 gauss from south to north. *I know there's a lot of questions, but I will rate the you-know-what out of you a) Find the direction of the force that our planet's magnetic field exerts on this cord if is oriented so that the current in it is running from west to east. b) Find the magnitude of the force that our planet's magnetic field exerts on this cord if is oriented so that the current in it is running from west to east. c) Find the direction of the force that our planet's magnetic field exerts on this cord if is oriented so that the current in it is running vertically upward. d) Find the magnitude of the force that our planet's magnetic field exerts on this cord if is oriented so that the current in it is running vertically upward. e) Find the direction of the force that our planet's magnetic field exerts on this cord if is oriented so that the current in it is running from north to south. f) Find the magnitude of the force that our planet's magnetic field exerts on this cord if is oriented so that the current in it is running from north to south. g) Is the magnetic force ever large enough to cause significant effects under normal household conditions?

Answers

a) If the current is running from west to east, the force that our planet's magnetic field exerts on this cord is directed upwards
b) The magnitude of the force that our planet's magnetic field exerts on this cord if it is oriented so that the current in it is running from west to east is F =2.64 x 10^-4 N
c) If the current is running vertically upward, the force that our planet's magnetic field exerts on this cord is directed to the left.  west
d) The magnitude of the force that our planet's magnetic field exerts on this cord if it is oriented so that the current in it is running vertically upward is F = 0 zero
e) If the current is running from north to south, the force that our planet's magnetic field exerts on this cord is directed east.
f) The magnitude of the force that our planet's magnetic field exerts on this cord if it is oriented so that the current in it is running from north to south is F = 2.64 x 10^-4 N
g) The magnetic force is not large enough to cause significant effects under normal household conditions.

EXPLANATION

a) The direction of the force that our planet's magnetic field exerts on the cord is perpendicular to both the direction of the current and the direction of the magnetic field, according to the right-hand rule. In this case, if the current is running from west to east, and the magnetic field is from south to north, the force will be directed upwards.

b) The magnitude of the force can be calculated using the formula:

F = BIL sin(theta)

where B is the magnitude of the magnetic field, I is the current, L is the length of the wire, and theta is the angle between the direction of the current and the direction of the magnetic field. In this case, theta is 90 degrees, so sin(theta) = 1. Substituting the given values, we get:

F = (0.550 x 10^-4 T) x (1.50 A) x (2.40 m) x 1

= 2.64 x 10^-4 N

Therefore, the magnitude of the force is 2.64 x 10^-4 N.

c) If the current in the wire is running vertically upward, the force will be directed towards the west.

d) Using the same formula as in part (b), we can calculate the magnitude of the force:

F = (0.550 x 10^-4 T) x (1.50 A) x (2.40 m) x sin(90)

= 0

Therefore, the magnitude of the force is zero.

e) If the current in the wire is running from north to south, the force will be directed towards the east.

f) Using the same formula as in part (b), we can calculate the magnitude of the force:

F = (0.550 x 10^-4 T) x (1.50 A) x (2.40 m) x 1

= 2.64 x 10^-4 N

Therefore, the magnitude of the force is 2.64 x 10^-4 N.

g) The magnitude of the magnetic force in this case is quite small, and under normal household conditions, it is unlikely to cause significant effects. However, in some situations, such as in electrical power transmission systems, the effects of the magnetic force may need to be taken into account.

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An object is 29cm away from a concave mirror's surface along the principal axis.If the mirror's focal length is 9.50 cm, how far away is thecorresponding image?
a.12
b.14
c.29
d.36

Answers

The image's distance from the concave mirror's surface is 12 cm. The correct option is B.

How to calculate the distance of the image?

A concave mirror is a mirror that has a reflective surface that curves inward like a part of a sphere. Concave mirrors are also known as "converging mirrors."When a ray of light falls on a concave mirror, the light rays converge at a point in front of the mirror.

This point is known as the focal point of the concave mirror. The distance between the focal point and the concave mirror's surface is referred to as the focal length of the concave mirror. It is negative for concave mirrors because they converge in light rays.

An object is 29 cm away from a concave mirror's surface along the principal axis. The mirror's focal length is 9.50 cm, so the image's distance from the mirror can be calculated using the mirror formula.

The mirror formula is:

1/v + 1/u = 1/f

where u is the object's distance from the mirror, v is the image's distance from the mirror, and f is the focal length of the mirror.

In this case, u = -29 cm, f = -9.5 cm, and we want to solve for v.

1/v + 1/-29 = 1/-9.5

Multiply both sides of the equation by

v x -29 x -9.5:-9.5v + -29(-9.5) = v(-29)(-9.5)285.5 = v(275.5)

v = -285.5/275.5

v ≈ -1.0378 cm

The negative sign indicates that the image is inverted, which is common for concave mirrors. The image is also closer to the mirror than the object, which is another characteristic of concave mirrors. The distance from the mirror's surface to the image is given by:-1.0378 - (-9.5) = 8.46 cm this is the same as 8.46 cm from the surface of the mirror.

Therefore, the image's distance from the concave mirror's surface is 12 cm. Option (a) 12 is correct.

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Help asaaap it's about doppler effect

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The frequency that the bad guy hear is 12000 hz when the police car is moving with speed of 80m/s.

Frequencyfo=fs(vvov), where fo is the observed frequency, fs is the source frequency, v is the speed of sound, vo is the observer's speed, the top sign indicates the observer is approaching the source, and the bottom sign indicates the observer is leaving the source.Equation fo=800(80-65) fo = 12000 after substituting the variablesThe apparent change in frequency of a wave as a result of an observer moving with respect to the wave source is known as the Doppler effect or Doppler shift. It bears the name of the Austrian physicist Christian Doppler, who first described the phenomenon in 1842.

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does air move from areas of high pressure to low pressure

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Explanation:  Gases move from high-pressure areas to low-pressure areas. And the bigger the difference between the pressures, the faster the air will move from the high to the low pressure.

Given the definition of EER, find the EER of an 8000 Btu/hour air conditioner that requires a power input of 1500 W. Express your answer numerically in British thermal units per hour per watt. EER = __________(Btu/hour)/W

Answers

EER is defined as the Energy Efficiency Ratio which is the ratio of cooling capacity in BTU/hr to the power input in watts.

The EER of the given 8000 Btu/h air conditioner is 5.33 Btu/hour per watt.

In the case of the given 8000 Btu/h air conditioner that requires a power input of 1500 W, the EER can be calculated as follows:

EER = (cooling capacity in Btu/hr) / (power input in watts)

EER = 8000 Btu/hour / 1500 W = 5.33 Btu/hour per wat.

Energy efficiency ratio (EER) is used in the USA and is defined as the system output in Btu/h per watt of electrical energy.

Coefficient of performance (COP) is the equivalent measure using SI units, which is widely used in the UK. A COP of 1.0 equates to an EER of 3.4.

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a cross section across a diameter of a long cylindrical conductor of radius a=2 cm carrying uniform current 170 A. What is the magnitude of the current's magnetic field at radial distance (a) 0, (b) 1 cm, (c) 2 cm (wire's surface), and (d) 4 cm

Answers

The magnitude of the current's magnetic field at radial distances (a) 0, (b) 1cm, (c) 2cm (wire's surface), and (d) 4cm are undefined, 1.7 * 10^-3 Tesla, 1.7 * 10^-3 Tesla, and 8.5 * 10^-4 Tesla, respectively. 

The question is about finding the magnitude of magnetic fields at different radial distances across a diameter of a long cylindrical conductor of radius a=2 cm carrying uniform current 170A.

Let's solve it step by step.

(a) At radial distance 0:

At the center of the conductor, r = 0, the magnetic field is zero.

It can be found by using the formula for the magnetic field at the center of the wire: 

B = (μ_0 * I) / (2 * π * r)

= (4π * 10^-7 * 170) / (2π * 0)

= undefined.

Therefore, the magnetic field at r = 0 is undefined. 

(b) At radial distance 1cm:

Using the formula for the magnetic field at a point P located at a radial distance r from the center of the wire: 

B = (μ_0 * I) / (2 * π * r)

= (4π * 10^-7 * 170) / (2π * 0.01)

= 1.7 * 10^-3 Tesla.

(c) At radial distance 2cm:

The magnetic field at r = a (i.e., the surface of the wire) can be determined by substituting the value of r = 2cm into the magnetic field formula:

B = (μ_0 * I) / (2 * π * r)

= (4π * 10^-7 * 170) / (2π * 0.02)

= 1.7 * 10^-3 Tesla.

(d) At radial distance 4cm:

Again, we use the formula for the magnetic field at a point P located at a radial distance r from the center of the wire:

B = (μ_0 * I) / (2 * π * r)

= (4π * 10^-7 * 170) / (2π * 0.04)

= 8.5 * 10^-4 Tesla.

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A small block with mass 0.0400 kg slides in a vertical circle of radius R = 0.500 m on the inside of a circular track. During one of the revolutions of the block, when the block is at the bottom of its path, point A, the normal force exerted on the block by the track has magnitude 3.95 N. In this same revolution, when the block reaches the top of its path, point B, the normal force exerted on the block has magnitude 0.680 N. How much work is done on the block by friction during the motion of the block from point A to point B?

Answers

The work done on the block by friction during the motion of the block from point A to point B is 2.49 J.

The normal force acting on the block at point A and point B is different. We can find the weight of the block at points A and point B using the following formula:

Weight = mg,

where m is the mass of the block and g is the acceleration due to gravity.

Weight at point A = m × g

Weight at point B = m × g

Now, the normal force acting on the block at point A is given as 3.95 N.

Therefore, we can write the equation for the weight and normal force as:

Weight at point A - Normal force at point A = m × a

Now, at point A, the acceleration acting on the block is the centripetal acceleration a = v²/R where v is the velocity of the block at point A.

We can write the equation for the weight and normal force as:

m × g - 3.95 = m × v²/R

Similarly, at point B, we can write the equation for the weight and normal force as:

m × g - 0.680 = m × v²/R

Now, we can solve both the equations for the velocity of the block at point A and point B:

Velocity at point A, v₁ = √(gR - 3.95/m)

Velocity at point B, v₂ = √(gR - 0.680/m)

The change in kinetic energy during the motion from point A to point B is given by:

∆KE = KE₂ - KE₁

= (1/2)mv₂² - (1/2)mv₁²

We know that work done, W = ∆KE

So, the work done on the block by friction during the motion of the block from point A to point B is given by:

W = (1/2)m(v₂² - v₁²)

Substituting the values in the above equation:

W = (1/2) × 0.0400 × ((√(9.81 × 0.500 - 0.680/0.0400))² - (√(9.81 × 0.500 - 3.95/0.0400))²)

W = 2.49 J

Therefore, the work done on the block by friction is 2.49 J.

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(3)
Four particles are located at points (1,4), (2,3), (3,3), (4,1).?
Find the moments Mx and My and the center of mass of the system, assuming that the particles have equal mass m.
Mx=
My=
xCM=
yCM=
Find the center of mass of the system, assuming the particles have mass 3, 2, 5, and 7, respectively.
xCM=
yCM=

Answers

Given that four particles are located at points (1,4), (2,3), (3,3), (4,1).

The moments Mx and My and the center of mass of the system can be determined as follows:

For equal mass m, the moment Mx is obtained by summing the product of the mass of each particle and the perpendicular distance from the line y=0.

Similarly, the moment My is obtained by summing the product of the mass of each particle and the perpendicular distance from the line x=0.

My = Σ mi*yiMy = (m(1)+m(2)+m(3)+m(4))(4+3+3+1)/4My = 11m

Hence, the moments Mx and My are 10m and 11m, respectively.

For particles with mass 3, 2, 5, and 7 respectively, the x-coordinate and y-coordinate of the center of mass of the system are given by:

xCM = (Σ mixi)/Mx= (3*1+2*2+5*3+7*4)/17= (3+4+15+28)/17= 50/17yCM = (Σ miyi)/My= (3*4+2*3+5*3+7*1)/17= (12+6+15+7)/17= 40/17

Hence, the center of mass of the system is at (50/17, 40/17).

The center of mass of the system with the following coordinates will be (2.76, 2.76). This can be calculated by the sum of the moments of each particle around the x-axis.

What is the center of mass of the system?

Here, we are given four particles that are located at points (1,4), (2,3), (3,3), (4,1). To calculate the moments Mx and My and the center of mass of the system, let us assume that the particles have equal mass m.

Moment Mx is defined as the sum of the moments of each particle around the y-axis. The moment of the ith particle around the y-axis is given by Mx,i = yim, where yi is the y-coordinate of the ith particle. Therefore, the total moment Mx of the system is: Mx = Mx,1 + Mx,2 + Mx,3 + Mx,4 = 4m + 3m + 3m + 1m = 11m

Therefore, Mx = 11m.

Moment My is defined as the sum of the moments of each particle around the x-axis. The moment of the ith particle around the x-axis is given by My, i = xim, where xi is the x-coordinate of the ith particle. Therefore, the total moment My of the system is: My = My,1 + My,2 + My,3 + My,4 = 1m + 2m + 3m + 4m = 10m

Therefore, My = 10m.

The coordinates of the center of mass (xCM, yCM) are given by:

xCM = Σmixi / ΣmiyCM = Σmiyi / Σmi

where, Σmi is the sum of the masses and Σmixi and Σmiyi are the sums of the moments around the y-axis and x-axis, respectively.

If the particles have equal mass m, then Σmi = 4m + 3m + 3m + 1m = 11m.

xCM = (1×4 + 2×3 + 3×3 + 4×1) / 11 = 2.45

yCM = (1×4 + 2×3 + 3×3 + 4×1) / 11 = 2.45

Therefore, the center of mass of the system is (2.45, 2.45).

If the particles have mass 3, 2, 5, and 7, respectively, then Σmi = 3 + 2 + 5 + 7 = 17.

xCM = (1×3 + 2×2 + 3×5 + 4×7) / 17 = 2.76

yCM = (4×3 + 3×2 + 3×5 + 1×7) / 17 = 2.76

Therefore, the center of mass of the system is (2.76, 2.76).

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what is the minimum angular velocity (in rpm ) for swinging a bucket of water in a vertical circle without spilling any? the distance from the handle to the bottom of the bucket is 35 cm . express your answer in revolutions per minute.

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The minimum angular velocity (in rpm) for swinging a bucket of water in a vertical circle without spilling any is 5.56 rpm.

The minimum angular velocity (in rpm) for swinging a bucket of water in a vertical circle without spilling any is given by the formula; Vmin=√g/R

where:

Vmin = minimum angular velocity (in rpm)g = acceleration due to gravity (9.81 m/s²)R = radius of the circular path or distance from the handle to the bottom of the bucket (35 cm)

To express the answer in revolutions per minute, the radius of the circle must be converted to meters;R = 35 cm = 0.35 m

Substituting the values given above into the formula;

Vmin=√g/R Vmin=√9.81/0.35 Vmin = 5.56 rpm

Therefore, the minimum angular velocity (in rpm) for swinging a bucket of water in a vertical circle without spilling any is 5.56 rpm.

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What happens to the reaction rate when the concentration (absorbance) of the reactants is doubled? Determine the reaction order by solving the following equations. Show a sample computation in your lab notebook. rate; – [CV3]* = CV.x = x= _ rate4 _ [CV4]* Ox= ratez [CV]* rates _ [CVs]* rates CV.* rate, x=

Answers

The reaction rate will double when the concentration of the reactants is doubled. The reaction order can be determined by solving the equations provided.
For example, if the initial rate is given by:
Rate = [CV3]* = CV.x = x = rate4 [CV4]* Ox= ratez [CV]* rates [CVs]* rates CV.* rate,
Then the reaction order can be calculated by rearranging the equation to:
[CV3]* = CV.x/x = rate4 [CV4]* Ox/x = ratez [CV]* rates [CVs]* rates CV.* rate
Since [CV3]*, [CV4]*, [CV]* and [CVs]* are all constants, the equation simplifies to:
x/x = rate4 Ox/x = ratez rates rates rate
Hence, the reaction order is 4.

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X-ray pulses from Cygnus X-1, a celestial x-ray source, have been recorded during high-altitude rocket flights. The signals can be interpreted as originating when a blob of ionized matter orbits a black hole with a period of 7.84 ms. If the blob were in a circular orbit about a black hole whose mass is 13.5 times the mass of the Sun, what is the orbit radius? The value of the gravitational constant is 6.67259×10−11N⋅m2/kg2 and the mass of the Sun is 1.991×1030 kg. Answer in units of km.

Answers

The orbit radius is 6.225 × 10^5 km.

The x-ray pulses from Cygnus X-1, a celestial x-ray source, have been recorded during high-altitude rocket flights. The signals can be interpreted as originating when a blob of ionized matter orbits a black hole with a period of 7.84 ms. And also, it is given that the blob were in a circular orbit about a black hole whose mass is 13.5 times the mass of the Sun. We need to determine the orbit radius.

The formula to be used to find the orbit radius is given by:

G(M+m)T2/4π2= r3

Where,

G = Gravitational constant = 6.67259×10−11 N⋅m2/kg2
M = Mass of the black hole
m = Mass of the blob
T = Time period of the orbit = 7.84 ms = 7.84 × 10^-3 s
r = Orbit radius

Substitute the given values in the above formula, we get:

r3 = G(M+m)T2/4π2
r3 = 6.67259×10−11 * [13.5(1.991×10^30) + m] * (7.84×10−3)2 / 4π2
r3 = 5.7919 × 10^15 m^3
Taking cube root on both sides, we get:
r = [5.7919 × 10^15 m^3] 1/3
r = 6.225 × 10^8 m
1 km = 1000 m

Therefore, the orbit radius in km is:
r = 6.225 × 10^8 m * 1 km / 1000 m
r = 6.225 × 10^5 km

Hence, the orbit radius is 6.225 × 10^5 km.

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A student standing on the ground throws a ball straight up. The ball leaves the student's hand with a speed of 11 m/s when the hand is 1.8 m above the ground. How long is the ball in the air before it hits the ground? (The student moves her hand out of the way.)

Answers

The ball is in the air for about 1.8 seconds before it hits the ground after it leaves the student's hand with a speed of 11 m/s when the hand is 1.8 m above the ground.

Projectile motion is a kind of movement experienced by an object or particle (a projectile) that is projected near the Earth's surface and moves along a curved path under the gravity of the Earth. In general, projectile motion refers to a free-body's motion influenced only by gravity. A student throws a ball straight up while standing on the ground. When her hand is 1.8 m above the ground, the ball leaves her hand at a speed of 11 m/s. The time the ball is in the air before it hits the ground is calculated as follows:Using the equation:

∆y = v0yt + 1/2gt² Where ∆y is the displacement (in this case, -1.8 m) of the projectile along the vertical axis, v0y is the initial vertical velocity (in this case, 11 m/s), t is the time of flight, and g is the acceleration due to gravity (9.81 m/s²):-1.8 m = (11 m/s)t + (1/2)(-9.81 m/s²)t².Rearranging the equation, we get:-4.905t² + 11t - 1.8 = 0.

Using the quadratic formula, we get:t = (-11 ± sqrt(11² - 4(-4.905)(-1.8))) / (2(-4.905))= 1.77 s or t = 0.20 s. Since the ball is in the air for approximately 1.77 s before it hits the ground, and the student's hand is 1.8 m above the ground, the ball is in the air for about 1.8 seconds before it hits the ground. Therefore, the correct answer is the option C, 1.8 seconds.

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A battery-powered toy car pushes a stuffed rabbit across the floor.Part ADraw a free-body diagram for a car (assume that it is moving from left to the right).Draw the force vectors with their tails at the dot. The orientation of your vectors will be graded. The exact length of your vectors will not be graded but the relative length of one to the other will be graded.Part BDraw a free-body diagram for a rabbit.Draw the force vectors with their tails at the dot. The orientation of your vectors will be graded. The exact length of your vectors will not be graded but the relative length of one to the other will be graded.

Answers

Part A: Thrust acts on the right in the direction of motion. Gravity acts downward.

Part B:  The direction of air resistance is opposite to the direction of motion, which is shown towards the left. Gravity acts downwards.

Part A:

A free-body diagram for a car is as follows:

The direction of friction is opposite to the direction of motion, which is shown towards the left.
The diagram shows three forces acting on the toy car that is battery-powered, which is as follows:
The force due to friction is labeled as [tex]f_K[/tex].

The force of thrust is labeled as [tex]f_T[/tex]. The force of gravity is labeled as [tex]f_g[/tex].
Part B:

A free-body diagram for a rabbit is as follows:
The diagram shows three forces acting on the stuffed rabbit that is being pushed by a toy car that is battery-powered, which is as follows:

The direction of friction is opposite to the direction of motion, which is shown towards the right.
The force due to friction is labeled as [tex]f_K[/tex]. The force due to air resistance is labeled as fair. The force of gravity is labeled as [tex]f_g[/tex].
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Which term describes the energy an object has due to the motion of its
particles?
A. Magnetic energy
B. Chemical energy
C. Elastic energy
D. Thermal energy

Answers

Answer: The answer is D. Thermal Energy.

Explanation:

Thermal energy is a type of kinetic energy owing to the fact that it results from the movement of particles.

as a source of blackbody radiation becomes hotter, the peak in its radiation spectrum moves from the visible to the ultraviolet and beyond. does this imply that the object can no longer be seen by the unaided human eye

Answers

Yes, it is correct that when the source of blackbody radiation becomes hotter, the peak in its radiation spectrum shifts from the visible to the ultraviolet and beyond. Blackbody radiation is electromagnetic radiation emitted from a blackbody or perfect absorber. This is due to the fact that hotter objects emit shorter wavelengths of electromagnetic radiation, which correspond to higher energy photons. Therefore, when an object gets hot enough to emit mostly ultraviolet or X-ray radiation, it will no longer be visible to the unaided human eye because the human eye can only detect radiation within the visible spectrum of about 400 nm (violet) and 700 nm (red). Therefore, a blackbody that emits radiation beyond this range will no longer be seen by the unaided human eye.

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why can't we fall safely with the help of parachute towards the moon?​

Answers

Answer:

The Moon has no atmosphere so there is no drag on the capsule to slow its descent; parachutes will not work. Lunar landing vehicles were equipped with rocket engines that were fired by the pilot to provide lift — thrust in the opposite direction of descent — during the rapid descent to the Moon's surface.

The moon does not harbor any appreciable atmosphere. Therefore no parachute, no matter how large, will operate properly on the moon. Air is required in order to inflate the parachute and slow down the descending object. Remember geologist Harrison Schmidt, the ONLY scientist to visit the moon? He was one of the last two people to ever touch the lunar surface. (Apollo 17). He demonstrated what would happen when two objects of different masses were dropped simultaneously from about five feet above the moon’s surface. He dropped a hammer and a feather. They fell at the same rate and hit the surface at exactly the same instant! There was no atmosphere to cause the feather to flutter. Note: Careful observers may notice that in videos of the the descending Apollo Lunar Lander (“The Eagle has landed”) lunar dust is kicked up by the craft’s engines. The dust moves out in straight lines, not in billowing clouds! PROOF that the film was made in the airless void of the moon and NOT in some clandestine film studio on Earth. No moon landing hoax!

lab 4: newton's second law: the atwood machine pre-lab questions: 1. what happens to the acceleration of our system when the mass of the system increases but the net force stays constant? 2. what happens to the acceleration of our system when the net applied force increases but the mass of the system does not change? 3. explain, in your own words, potential sources of error in today's experiment.

Answers

According to Newton's second law, the acceleration of a system is directly proportional to the net force applied to it and inversely proportional to its mass. Therefore, if the net force stays constant but the mass of the system increases, the acceleration of the system will decrease.

Similarly, if the mass of the system remains constant but the net applied force increases, the acceleration of the system will increase.

There are several potential sources of error in the Atwood machine experiment. For example, friction in the pulley or air resistance could cause the system to accelerate at a different rate than predicted by theory. Additionally, the masses used in the experiment may not be perfectly accurate, which could introduce small errors into the measurements. The string connecting the two masses could also stretch or have varying elasticity, which could affect the results. Finally, human error in measuring the time or the distances traveled by the masses could lead to inaccuracies in the calculated values of acceleration or tension in the string.

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hydroelectric, wind, geothermal, and parabolic solar collection all rely on spinning turbines (connected to a generator) to produce electricity. explain how each provides the force to do so.

Answers

Hydroelectric energy is generated by capturing the energy of flowing water. As water flows through a turbine, the blades of the turbine spin and generate electricity.

How does the different energies provide force?

Wind energy is generated by capturing the kinetic energy of the wind. As wind passes through the turbine, the blades spin and generate electricity.

Geothermal energy is generated by harnessing the natural heat of the Earth’s core. Heat from the Earth’s core is used to generate steam, which is then used to spin a turbine and generate electricity.

Parabolic solar collection is a method of collecting the sun’s energy using large reflective mirrors. The mirrors focus the sunlight onto a central point, which is then used to spin a turbine and generate electricity.

Thus, all of these power sources rely on spinning turbines connected to a generator to produce electricity.

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b) If the observation point on the z axis is far enough away from the center of this ring, the ring should start to look and behave as a particle of charge Q at the origin. How far out on the +z axis must the observation point lie if the result for Vring (Eq. A) and for the potential of a particle with the same charge Vparticle agree to within 5%?

Answers

The potential due to a ring of charge at a point on the z-axis a distance z away from the center of the ring is given by the equation:

Vring = kQ / √(R^2 + z^2)

where k is Coulomb's constant, Q is the charge on the ring, R is the radius of the ring, and z is the distance from the center of the ring to the observation point.

If the ring behaves like a point particle of charge Q at the origin, the potential at the same observation point on the z-axis would be:

Vparticle = kQ / z

To find the distance z where these two potentials agree to within 5%, we can set up the following equation:

|Vring - Vparticle| / Vparticle ≤ 0.05

Substituting the expressions for Vring and Vparticle and simplifying, we get:

|√(R^2 + z^2) - z| / z ≤ 0.05

Squaring both sides and rearranging, we get:

(R^2 / z^2) ≤ 0.0025

Taking the square root of both sides, we get:

R / z ≤ 0.05

Solving for z, we get:

z ≥ R / 0.05

Therefore, the observation point on the +z axis must be at a distance z of at least R / 0.05 from the center of the ring, where R is the radius of the ring, for the ring to behave like a point particle of charge Q at the origin to within 5%.

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We always see the same side of the Moon because a. the Moon does not rotate on its axis. b. the Moon rotates on its axis once for each revolution around Earth. c. when t…
We always see the same side of the Moon because
a. the Moon does not rotate on its axis.
b. the Moon rotates on its axis once for each revolution around Earth.
c. when the other side of the Moon is facing Earth, it is unlit.
d. when the other side of the Moon is facing Earth, it is on the opposite side of Earth.
e. none of the above

Answers

We always see the same side of the Moon because the "Moon rotates on its axis once for each revolution around Earth." Thus, the correct option will be B.

How does the Moon rotates?

When the Moon rotates on its axis once for each revolution around Earth, then we always see the same side of the Moon. The reason behind this is that the moon's rotation takes almost the same time as it takes to orbit the Earth.

When the same side of the moon is facing the Earth, it appears to be unchanging. That is why we always see the same side of the moon from Earth. The other side of the Moon is known as the far side, which was first observed by the Soviet spacecraft Luna 3 in 1959.

Therefore, the correct option will be B.

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The capacity of a battery to deliver charge, and thus power, decreases with temperature. The same is not true of capacitors. For sure starts in cold weather, a truck has a 500 F capacitor alongside a battery. The capacitor is charged to the full 13.8 V of the truck's battery. How much energy does the capacitor store? What is the ratio between the energy density per unit mass of the 9.0 kg capacitor system and the 130,000 J/kg of the truck's battery.

Answers

The energy stored in the capacitor is calculated as 630150 J. The ratio between the energy density per unit mass of the 9.0 kg capacitor system and the 130,000 J/kg of the truck's battery is 70.17


The formula to calculate the energy stored in a capacitor is expressed by the formula: 

E = (1/2)CV²

where E is energy, C is capacitance, and V is voltage.

The question mentions that the capacitor is fully charged to 13.8 V. Therefore, the energy stored in the capacitor is given by the formula:

[tex]E = (1/2)CV^2 \\= (1/2)\times (500 F)\times {(13.8 V)}^2\\= 630150 J[/tex]

The ratio between the energy density per unit mass of the 9.0 kg capacitor system and the 130,000 J/kg of the truck's battery can be computed by dividing the energy density of the capacitor system by the energy density of the truck's battery.

We know that energy density = energy / mass of the system.

Thus, the formula to calculate the ratio is:

[tex]Ratio = \dfrac{energy density per unit mass of capacitor system}{ energy density per unit mass of truck's battery}\\Ratio= \dfrac{630150 J / 9 kg}{ 130,000 J / 1 kg}= 70.017[/tex]

Therefore, the ratio of energy density per unit mass of the capacitor system to that of the truck's battery is 70.017.

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a test tube standing verticslly in a test tube rack contains 2.5 cm of oil and 6.5 cm of water. what is the pressur eon the bottom of the tube

Answers

The pressure on the bottom of the test tube which contain both the oil and water molecules is about 641.65 Pa + 220.725 Pa = 862.375 Pa.

What is the pressure in test tube?

The pressure at the bottom of the test tube is the result of two factors: the weight of the oil and the weight of the water molecules. The pressure is equal to the density of each liquid multiplied by the height of each liquid, multiplied by the gravitational acceleration (g).

The pressure at the bottom of the test tube is given by the density of the fluids and also the height of the column above the bottom region. The pressure at the bottom of the test tube is calculated by multiplying the density of the fluids by the height of the column above the bottom. Here's how to calculate the pressure:

P = pgh

where P = Pressure, p = Density of fluid, g = Acceleration due to gravity, and h = Height of the column.

The pressure at the bottom of the test tube is the pressure which is exerted by the water and oil above it. The water is more dense than that of the oil, therefore it exerts more pressure on the bottom of the test tube. The pressure at the bottom of the test tube is given by the formula

The density of water is 1000 kg/m³, and the density of oil is 900 kg/m³. The height of the column of water is 6.5 cm, and the height of the column of oil is 2.5 cm.

Using the above formula: P = pgh

P (Water) = 1000 × 9.81 × 0.065

P (Water) = 641.65 Pa

P (Oil) = 900 × 9.81 × 0.025

P (Oil) = 220.725 Pa

Therefore, the pressure on the bottom of the tube is 641.65 Pa + 220.725 Pa = 862.375 Pa.

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a rocket starts from rest and moves upward from the surface of the earth for the first 10.0 s of its motion the vertical acceleration of the rocket is given by ay 2.90m s3 t where the y direction is upward. Part A: What is the height of the rocket above the surface of the earth at t = 10.0 s? Part B: What is the speed of the rocket when it is 205 m above the surface of the earth?

Answers

At t = 10.0 s, the height of the rocket above the surface of the earth is 200 m. the speed of the rocket when it is 205 m above the surface of the earth is 20.64 m/s.

To calculate height of the rocket, we can use the equation of motion: s = 1/2*a*t^2. Therefore, the height of the rocket is: s = 1/2*2.90m/s^2*(10.0s)^2 = 200 m

To calculate the speed of the rocket when it is 205 m above the surface of the earth, we can use the equation of motion: v^2 = 2as

Therefore, the speed of the rocket when it is 205 m above the surface of the earth is v = sqrt(2*2.90m/s^2*205m) = 20.64 m/s.

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If the 0. 100-mm diameter tungsten filament in a light bulb is to have a resistance of 0. 200 ω at 20. 0oc , how long should it be?

Answers

The length is 2.78 mm if the 0. 100-mm diameter tungsten filament in a light bulb is to have a resistance of 0. 200 ω at 20 degrees.

The length tungsten filament is 2.78 mm to have a resistance of 0. 200 ω at 20. degrees.

The given data is as follows:

Diameter of tungsten = 0.100 mm

resistance of tungsten = 0.200ω

The resistance (R) of a conductor is calculated by using the formula,

R = ρ × (L/A)

ρ =   resistivity of the material

L =  length of the conductor

A  =  cross-sectional area.

By rearranging the formula to calculate the length,

L = (R × A) / ρ

A = π × r²

A = 3.14 × (5.0 x [tex]10^{-5}[/tex])²

A = 7.85 x [tex]10^{-9}[/tex] m²

The resistivity of tungsten at 20.0°C  =  5.6 x [tex]10^{-8}[/tex] Ωm

L = (0.200 × 7.85 x [tex]10^{-9}[/tex]) / (5.6 x [tex]10^{-8}[/tex])

L = 2.78 x [tex]10^{-3}[/tex] m

L = 2.78 mm

Therefore we can conclude that the length is 2.78 mm to have a resistance of 0. 200 ω at 20 degrees.

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A student wants to use the output from the aux port on their phone to play music from their speakers. The aux port supplies 5v and a max current of 0.015A, but the speakers need 12v and a max current of 1.5A. You decide to use a power transistor to amplify the signal from the aux port. What does the beta value of your chosen transistor need to be to amplify the current enough?

pls explain or elaborate the answer if u can!!

Answers

Answer:The beta value of a transistor represents the current gain, which is the ratio of the collector current to the base current. In this case, we want to use the transistor as an amplifier to increase the current from the 0.015A supplied by the phone to the 1.5A required by the speakers.

The required current gain can be calculated using the following formula:

Beta = (Ic / Ib)

Where:

Beta is the current gain of the transistor

Ic is the collector current (output current)

Ib is the base current (input current)

To find the required beta value, we need to first calculate the base current required to drive the transistor. We can use Ohm's Law to do this:

Ib = V / R

Where:

Ib is the base current

V is the voltage supplied by the phone (5V)

R is the input resistance of the transistor circuit

Assuming an input resistance of 1kΩ, the base current required is:

Ib = V / R = 5 / 1000 = 0.005A (5mA)

Now, we can calculate the required collector current using the maximum current required by the speakers:

Ic = 1.5A

Finally, we can calculate the required beta value:

Beta = Ic / Ib = 1.5 / 0.005 = 300

Therefore, we need to choose a power transistor with a beta value of at least 300 to amplify the current from the aux port enough to drive the speakers.

Explanation:

At a major league baseball game, a pitcher delivers a 45 m/s (100.7 mph) fastball to the first player at bat, who bunts (meets the pitch with a loosely held stationary bat) so that the ball leaves the bat at only 5 m/s (11.2 mph) directly back towards the pitcher. The second player at bat also receives a 45 m/s fastball from the pitcher, but he swings his bat hard and sends the ball in a fast line drive directly back towards the pitcher at 50 m/s (111.8 mph). The mass of a standard baseball is 0.145 kg.
Calculate the impulse delivered to the baseball by the baseball bat for the first player (who bunts the ball). Assume the initial pitch is in the positive x-direction, and the ball moves in the negative x-direction after it strikes the bat.
Calculate the impulse delivered to the baseball by the baseball bat for the second player (who hits the fast line drive). Assume the initial pitch is in the positive x-direction, and the ball moves in the negative x-direction after it strikes the bat.
Calculate the magnitude of the work done by the baseball bat on the baseball for the first player (who bunts the ball). Report your answer as a positive number for positive work done on the ball or a negative number for negative work done on the ball.
Calculate the work done by the baseball bat on the baseball for the second player (who hits the fast line drive). Report your answer as a positive number for positive work done on the ball or a negative number for negative work done on the ball.

Answers

1) The impulse delivered to the baseball by the baseball bat is 40 kg-m/s.

2) The impulse delivered to the baseball by the baseball bat is 5 kg-m/s.

3) The magnitude of the work done by the baseball bat on the baseball for the first player is 1800 Joules.

4) The work done by the baseball bat on the baseball for the second player is 225 Joules.

The impulse delivered to the baseball by the baseball bat for the first player (who bunts the ball) can be calculated by subtracting the final velocity of the ball (5 m/s) from the initial velocity of the ball (45 m/s). The impulse delivered to the baseball by the baseball bat is 40 kg-m/s.

The impulse delivered to the baseball by the baseball bat for the second player (who hits the fast line drive) can be calculated by subtracting the final velocity of the ball (50 m/s) from the initial velocity of the ball (45 m/s). The impulse delivered to the baseball by the baseball bat is 5 kg-m/s.

The magnitude of the work done by the baseball bat on the baseball for the first player (who bunts the ball) can be calculated by multiplying the impulse (40 kg-m/s) by the initial velocity of the ball (45 m/s). The magnitude of the work done by the baseball bat on the baseball for the first player is 1800 Joules.

The work done by the baseball bat on the baseball for the second player (who hits the fast line drive) can be calculated by multiplying the impulse (5 kg-m/s) by the initial velocity of the ball (45 m/s). The work done by the baseball bat on the baseball for the second player is 225 Joules.

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Masses m1 and m2 are supported by wires that have equal lengths when unstretched. The wire supporting m1 is an aliminum wire 0. 9 mm in diameter, and the one supporting m2 is steel wire 0. 3 mm in diameter. What is the ratio m1/m2 if the two wires stretched by the same amount?

Answers

A wire's ability to elongate (or stretch) under stress is influenced by a number of variables, including the force used, the wire's cross-sectional area, and the material's elastic modulus.

The stiffness or resistance to deformation of a material is measured by the modulus of elasticity, which varies for steel and aluminium.While supporting the masses m1 and m2, let L be the length of each wire when it is not extended, and let L be the common elongation (or stretch) of the wires.

The force exerted on each wire comes from:

F = mg

where g is the gravitational acceleration. The identical amount of stretching is applied to both wires, therefore we have:

F1/A1 = F2/A2

where the cross-sectional areas of the steel and aluminium wires, respectively, are A1 and A2, respectively. A wire of diameter d has a cross-sectional area given by:

A = πd²/4

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Rank the objects from left to right based on their average distance from the Sun, from farthest to closest. (Not to scale.)Pluto, Saturn, Jupiter, Mars, Earth, Mercury

Answers

From farthest to closest, the ranking of the planets based on their average distance from the Sun would be:

Pluto, Saturn, Jupiter, Mars, Earth, Mercury

Note that the objects are not to scale, so this ranking may not be perfectly accurate in terms of relative distances. However, it gives a general idea of the order of the planets from farthest to closest to the Sun.

The eight planets in our solar system, listed in order from the Sun, are:

Mercury

Venus

Earth

Mars

Jupiter

Saturn

Uranus

Neptune

These eight planets are also known as the "classical planets," and are the largest and most massive objects in orbit around the Sun. There are also several dwarf planets in our solar system, such as Pluto and Ceres, as well as numerous smaller objects like asteroids and comets.

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#1)

A 500 Hz triangular wave with a peak amplitude of 50 V is applied to

the vertical deflecting plates of a CRO. A 1 kHz saw tooth wave with a

peak amplitude of 100 V is applied to the horizontal deflecting plates.

The CRO has a vertical deflection sensitivity of 0. 1 cm/V and a

horizontal deflection sensitivity of 0. 02 cm/V. Assuming that the two

inputs are synchronized, determine the waveform displayed on the

screen?

[2 Marks]

Answers

The CRO (Cathode Ray Oscilloscope) will display a triangular wave that is vertically stretched and horizontally compressed.

The vertical deflection plates will cause the triangular wave to be displayed with a peak-to-peak amplitude of[tex]100 cm (50 V * 0.1 cm/V)[/tex], while the horizontal deflection plates will cause  sawtooth wave to be displayed with a peak-to-peak amplitude of [tex]5000 cm (100 V * 0.02 cm/V).[/tex] The synchronization of the two inputs will ensure that the triangular wave and the sawtooth wave are displayed in a coordinated manner, with each cycle of the sawtooth wave corresponding to five cycles of the triangular wave. The resulting display will show a pattern of diagonal lines that gradually rise and then quickly drop back to the starting position, with each line representing a cycle of the sawtooth wave.

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the orbital period of saturn is 29.46 years. determine the distance from the sun to the planet in km

Answers

The average distance from the Sun to Saturn is approximately 1,427,000,000 km. To calculate this, we can use the Third Kepler's Law of Planetary Motion, which states that the square of the orbital period of a planet is proportional to the cube of the semi-major axis of the orbit.

We can use Kepler's Third Law to relate the orbital period of a planet to its distance from the sun:

T^2 = (4π^2 / GM) * r^3

where T is the orbital period in years, G is the gravitational constant, M is the mass of the sun, and r is the average distance from the sun to the planet in astronomical units (AU).
Therefore, we can use the formula:

d^3 = (T^2 * 4π^2)/G*M

Where d is the distance, T is the orbital period, G is the gravitational constant, and M is the mass of the Sun.


Plugging in the values:

d^3 = (29.46^2 * 16π^2)/(6.67408 * 1.989 * 10^30)
d = 1,427,000,000 km

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