The current through the lightbulb when a lightbulb is in series with a 2.0 ohm resistor is I = 1.78 A, 2.96 A.
The current through the lightbulb when a lightbulb is in series with a 2.0 ohm resistor is given by the Ohm's Law. Ohm's law states that current through a conductor between two points is directly proportional to the voltage across the two points. In other words, V = IR. Where V is the voltage, I is the current and R is the resistance. When the circuit is connected to a battery, the lightbulb dissipates 10W. Power can also be expressed as P = IV, where P is the power, I is the current and V is the voltage. We have V = IR and P = IV.
We can substitute V in terms of I from the first equation to the second equation.P = I²R=> I² = P/R=> I = √(P/R) = √(10W/2Ω) = 2.24 A. There are two possible answers. When we apply Ohm's Law to the circuit, I = V/R Where R = 2.0 Ω and V is the voltage across the resistor.I = V/2 = (10/2)^(1/2) A = 1.78 A.The other possible answer is the current through the light bulb.I = (10/2.0 + 2.0) A = 2.96 A. Therefore, the current through the lightbulb when a lightbulb is in series with a 2.0 ohm resistor is I = 1.78 A, 2.96 A.
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A 910-kg sports car collides into the rear end of a 2100-kg SUV stopped at a red light. The bumpers lock, the brakes are locked, and the two cars skid forward 2.5m before stopping. The police officer, estimating the coefficient of kinetic friction between tires and road to be 0.80, calculates the speed of the sports car at impact.
1.A 910-kg sports car collides into the rear end of a 2100-kgSUV stopped at a red light. The bumpers lock, the brakes are locked, and the two cars skid forward 2.5m before stopping. The police officer, estimating the coefficient of kinetic friction between tires and road to be 0.80, calculates the speed of the sports car at impact.
1.What was the speed sports car at impact?
The speed of the sports car at impact when kinetic friction between tires and road is 0.80 is 15.55 m/s.
It is given that Mass of sports car, ms = 910 kg, Mass of SUV, mSUV = 2100 kg, and Initial velocity of sports car, us = ?, Final velocity of sports car, v = 0, Initial velocity of SUV, uSUV = 0, Final velocity of SUV, vSUV = 0, and Coefficient of kinetic friction, μk = 0.80. Distance covered before stopping, s = 2.5 m.
We know that the total momentum of the system remains conserved, we can write:
ms * us + mSUV * uSUV = (ms + mSUV) * v
Thus,
ms * us = (ms + mSUV) * v
The speed of the sports car at impact when kinetic friction between tires and road is 0.80 is 15.55 m/s.
It is given that Mass of sports car, ms = 910 kg, Mass of SUV, mSUV = 2100 kg, and Initial velocity of sports car, us = ?, Final velocity of sports car, v = 0, Initial velocity of SUV, uSUV = 0, Final velocity of SUV, vSUV = 0, and Coefficient of kinetic friction, μk = 0.80. Distance covered before stopping, s = 2.5 m.
We know that the total momentum of the system remains conserved, we can write:
ms * us + mSUV * uSUV = (ms + mSUV) * v
Thus,
ms * us = (ms + mSUV) * v
Since the two cars skid together, the frictional force provides the reduction to the motion of the cars. The reduction force F = μk * N where N is the normal force acting on the cars, N = (ms + mSUV) * g where g is the acceleration due to gravity, g = 9.8 m/s².
We have to find the speed of the sports car at impact i.e. us. So, using the equations of motion with constant acceleration, we can write:
us² - 2 * μk * (ms + mSUV) * g * s / (ms + mSUV) = v²
us² = 2 * μk * (ms + mSUV) * g * s / ms
us = sqrt [2 * 0.80 * (910 + 2100) * 9.8 * 2.5 / 910]
us = 15.55 m/s
Therefore, the speed of the sports car at impact is 15.55 m/s.
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A train P covered a distance of 180 km in 4.5 hours and train Q covered 270 km in 6 hours. Which train is moving faster?
ans= train Q
Sol= 4.5×60= 270
6×60= 360
270÷180=1.5
360÷270=1.3...
1.3... <1.5
standard number of bones in the appendicular skeleton
The standard number of bones in the appendicular skeleton varies slightly among individuals, but it is generally accepted that there are 126 bones in the appendicular skeleton of an adult human.
The appendicular skeleton includes all the bones that are attached to the axial skeleton, which includes the skull, vertebrae, and ribcage. The appendicular skeleton consists of the bones of the arms, legs, pelvis, and shoulder girdle. Here is a breakdown of the number of bones in each part of the appendicular skeleton: Arms: 60 bones (30 in each arm) Legs: 60 bones (30 in each leg) Pelvis: 2 bones Shoulder girdle: 4 bones Adding up these numbers gives a total of 126 bones in the appendicular skeleton. However, this number can vary slightly among individuals due to differences in bone structure and development.
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Let the mass of the sled be m and the magnitude of the net force acting on the sled be Fnet . The sled starts from rest. Consider an interval of time during which the sled covers a distance s and the speed of the sled increases from v1 to v2 . We will use this information to find the relationship between the work done by the net force (otherwise known as the net work) and the change in the kinetic energy of the sled. Use W = F s cos (theta) to find the net work Wnet done on the sled. Express your answer in terms of some or all of the variables m ,v1 and v2 .
Total work done is Wnet = 1/2mv₂² - 1/2mv₁²
Let the mass of the sled be m and the magnitude of the net force acting on the sled be Fnet .
The sled starts from rest. Consider an interval of time during which the sled covers a distance s and the speed of the sled increases from v₁ to v₂ . We will use this information to find the relationship between the work done by the net force (otherwise known as the net work) and the change in the kinetic energy of the sled.
Use W = F s cos (theta) to find the net work Wnet done on the sled. Express your answer in terms of some or all of the variables m ,v₁ and v₂.Using the work-energy principle, we can calculate the work done on an object in terms of its change in kinetic energy. Consider the sled being acted upon by a force Fnet.
W = ΔK is used to calculate the work done on the sled as it moves from rest to velocity v₁ and then to velocity v₂ over a distance s.
Considering the sled to be the system under study, we can write the net work done on the sled as Wnet = ΔK.Wnet = 1/2mv₂² - 1/2mv₁² = Fnet s cos θWnet = Fnet s cos θ = 1/2mv₂² - 1/2mv₁²
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What are water droplets that act as a prism?
O a
Ob
OC
Od
mirage
rainbow
filter
concave mirror
Water droplets that act as prism are phenomenon known as : b) rainbow.
What are water droplets that act as prism?When light enters water droplet and is refracted, it is dispersed into its component colors due to difference in the index of refraction of each color of light. This results in band of colors in the shape of arc with red on outer edge and violet on inner edge, with other colors of spectrum in between. This is the same effect as prism which disperses light in the same way.
Rainbows appear in seven colors because water droplets break sunlight into seven colors of spectrum and you get the same result when sunlight passes through prism. Water droplets in the atmosphere act as prism though traces of light are very complex.
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A 1. 1 kg box drops two meters from a shelf and comes to rest after 0. 021 s on the floor. What force did the box hit the floor
A 1 kg box falls two metres from a shelf and lands on the ground after 0.021 seconds. The box impacted the ground with a force of around 524.7 N.
The box impacted the ground with a force of around 524.7 N.
Explanation: We can determine the force using the equation F = m * (v/t), where m is the box's mass, v is the velocity change (which is the ultimate velocity because the box starts at rest and comes to a halt), and t is the time it takes for the box to stop.
Given that the box falls 2 metres and its terminal velocity is 0 m/s, v = 2 m/s.
524.7 N is equal to F = 1.1 kg * (2 m/s / 0.021 s).
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g as a prank, someone drops a water-filled balloon out of a window. the balloon is released from rest at a height of 10.0 m above the ears of a man who is the target. then, because of a guilty conscience, the prankster shouts a warning after the balloon is released. the warning will do no good, however, if shouted after the balloon reaches a certain point, even if the man could react infinitely quickly. assuming that the air temperature is 20 c and ignoring the effect of air resistance on the balloon, determine how far above the man's ears this point is.
The point at which the warning will do no good is 7.50 m above the man's ears.
When a water-filled balloon is released from rest at a height of 10.0 m above the ears of a man, the warning will do no good if shouted after the balloon reaches a certain point. Assuming that the air temperature is 20°C and ignoring the effect of air resistance, this point is 7.50 m above the man's ears.
The vertical displacement (d) can be determined using the equation [tex]d = \frac{vf2}{2g}[/tex], where vf is the final velocity and g is the acceleration due to gravity (9.81 m/s2).
Since the balloon was released from rest, the initial velocity is 0 m/s. Therefore, [tex]d = \frac{02 }{ 2} (\frac{9.81 m}{s2} ) = 0[/tex]m. Since the initial height was 10.0 m, the final height is 10.0 m + 0 m = 10.0 m.
The point at which the warning will do no good is 7.50 m above the man's ears, so the final height of the balloon must be 10.0 m - 7.50 m = 2.50 m.
Therefore, the point at which the warning will do no good is 7.50 m above the man's ears.
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for a given mass of gas at constant temperature, the volume of the gas varies inversely with pressure.a. 3Pb. P/3c. 3P/Td. 9P
The volume of the gas varies inversely with pressure, and the correct answer is (b) P/3.
According to Boyle's Law, at a constant temperature, the volume of a gas is inversely proportional to its pressure. Mathematically, this can be expressed as:
PV = k
where P is the pressure of the gas, V is its volume, and k is a constant.
If we assume that the mass of the gas remains constant, then k is also constant. So we can write:
[tex]P_1V_1 = k and P_2V_2 = k[/tex]
where[tex]P_1 and V_1[/tex] are the initial pressure and volume, and [tex]P_2 and V_2[/tex] are the final pressure and volume.
If we divide these two equations, we get:
[tex]P_1V_1/P_2V_2 = 1[/tex]
Since[tex]V_1[/tex] is inversely proportional to [tex]P_1[/tex], we can write:
[tex]V_1 = k/P_1[/tex]
Similarly, [tex]V_2 = k/P_2.[/tex]
Substituting these values in the above equation, we get:
[tex](k/P_1)/(k/P_2) = 1[/tex]
Simplifying this, we get:
[tex]P_2/P_1 = V_1/V_2[/tex]
Since we are given that the temperature remains constant, we can assume that k is constant, and therefore:
[tex]V_1/P_1 = V_2/P_2[/tex]
If we let [tex]P_2 = 3P_1[/tex], then we get:
[tex]V_1/P_1 = V_2/(3P_1)[/tex]
Simplifying this, we get:
[tex]V_1/V_2 = 1/3[/tex]
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A converging lens of focal length 20cm Forms a real Image of 4cm high of an object which is 5cm high. If the Image is 36cm away from the lens, determine by graphical method the position of the object.
Answer:
in image
Explanation:
I don't think so it helped but through this you can do the question exactly like this ( in this way) ...
1 80 kg scaffold is 5.80 m long. it is hanging with two wires, one from each end. a 580 kg box sits 1 m from the left end. what is the tension in the right hand side wire?
The tension in the right-hand side wire is 6525 N.
Given:
Weight of the scaffold = 180 kgLength of the scaffold = 5.8 mWeight of the box = 580 kgDistance of the box from left end = 1 mLet the tension in the left wire = T1Let the tension in the right wire = T2To find: Tension in the right-hand side wireWe know that the sum of forces acting in a vertical direction should be equal to 0 as there is no acceleration in the vertical direction. ∑Fv = 0In the horizontal direction, there are no forces acting on the system.
∑Fh = 0Now considering forces in the vertical direction: T1 + T2 = (Weight of scaffold + Weight of the box) gT1 + T2 = (180 + 580) x 9.8T1 + T2 = 7644 N1. From the diagram, we can see that the box is nearer to the left side. Hence, the tension force in the left wire is greater than the tension force in the right wire.
T1 > T22. Let's take moments about the right end of the scaffold as shown in the figure below.
∑Mr = 0T1 × 5.8 = T2 × 1T2 = 5.8/1 × T1T2 = 5.8T1Now, we can substitute the value of T2 in equation (1):
T1 + T2 = 7644N6.8 T1 = 7644 N T1 = 1125 NTo find T2, we can substitute the value of T1 in equation (2):
T2 = 5.8 × T1T2 = 5.8 × 1125 N T2 = 6525 NTherefore, the tension in the right-hand side wire is 6525 N.
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Which of the following statements is true about the relationship between the two forms of Newton's second law (Fnet = dp/dt and Fnet = m.a) Select the correct answer
a. Fnet = dp/dt reduces to Fnet = m.a if the O acceleration of the object does not change with time. b. Fnet = m.a reduces to Fnet = dp/dt if the acceleration of the object does not change with time. c. Fnet = m.a reduces to Fnet = dp/dt if the mass of the object Answer dt does not change with time. d. Fnet = m.a reduces to Fnet = m.a if the dt momentum of the object does not change with time. e. Fnet = dp/dt reduces to Fnet = m.a if the mass of the object does not change with time. f. Fnet = m.a reduces to Fnet = dp/dt if the momentum of the object does not change with time.
The correct statement about the relationship between the two forms of Newton's second law (Fnet = dp/dt and Fnet = m.a) is option D "Fnet = m.a reduces to Fnet = dp/dt if the momentum of the object does not change with time.
What is Newton's second law?Newton's second law of motion states that the acceleration of an object is directly proportional to the force applied to it and inversely proportional to its mass. In other words, Fnet = m.a, where Fnet is the net force acting on an object, m is its mass, and a is its acceleration. This law can also be written as Fnet = dp/dt, where dp/dt is the rate of change of momentum with time.
Since momentum is the product of mass and velocity, it can be rewritten as dp/dt = m.dv/dt + v.dm/dt, where v is the velocity of the object. If the mass of the object remains constant over time, then v.dm/dt is zero and dp/dt reduces to m.dv/dt, which is equal to Fnet.
Therefore, Fnet = dp/dt reduces to Fnet = m.a if the object's acceleration does not change with time. If the momentum of the object does not change with time, then dp/dt is zero, and Fnet = dp/dt reduces to zero, which means that Fnet = m.a is also zero. Therefore, Fnet = m.a reduces to Fnet = dp/dt if the momentum of the object does not change with time.
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the potential difference across the ion channel is 70 mv . what is the power dissipation in the channel?
The power dissipation in the ion channel is 4.9 mW given that the potential difference across the ion channel is 70 mv
The power dissipated by a resistor is given by the formula:P = V² / RwhereP = PowerV = VoltageR = Resistance
The power dissipated in the ion channel is unknown. However, we can consider the ion channel to have a resistance of 1 Ω. This is because the resistance of an ion channel is very small and close to zero. So, we can assume the resistance of the ion channel as 1 Ω.As we know the potential difference across the ion channel, we can use the above formula to find the power dissipated in the ion channel.P = (70 mV)² / 1 ΩP = 0.0049 W = 4.9 mW
Therefore, the power dissipation in the ion channel is 4.9 mW.
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Imagine you are viewing the other planets from Earth. Which planets (if any) will appear to pass directly in front of the Sun from your Earth-based perspective? Which planets (if any) will never transit the Sun? If you were able to view the Solar System from outside, how many planets could potentially transit the Sun? Will those planets transit the Sun no matter where outside the Solar System you are? Sketch and describe the required orientation of the Solar System in order for the maximum number of planets to transit the Sun.
Explanation:
Planets closer to the sun will appear to transit from time to time
= 2 Venus and Mercury ( I suppose you could include the Moon..an eclipse ....haha)
All of the planets further from the sun than earth will not transit
Potentially ALL of the planets could transit the sun (earth included) if observed outside solar system HOWEVER if you are not observing from near the orbital plane of
the planets NONE of them would transit
For maximum transits, the planets should all be in the same orbital plane and the observer should be very close to this plane also.
An electroscope is a device with a metal knob, a metal stem, and freely hanging metal leaves used to detect charges. The diagram below shows a positively charged leaf electroscope.
As a positively charged glass rod is brought near the knob of the electroscope, the separation of the leaves will
remain the same
increase
As a positively charged glass rod is brought near the knob of the electroscope, the separation of the leaves will increase.
What is Charge?
Charge is a fundamental property of matter that determines how objects interact with each other through the electromagnetic force. It is a physical property that can be positive or negative and can be measured in coulombs (C).
This is because the positively charged glass rod will induce a negative charge on the metal knob of the electroscope. The negative charges will repel the electrons in the metal leaves, causing them to move away from each other and increasing their separation. The greater the amount of charge on the glass rod, the greater the separation between the leaves will be.
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a proton accelerates from rest in a uniform electric field of 600 n/c. at one later moment, its speed is 1.50 mm/s (nonrelativistic because v is much less than the speed of light). find the time interval, in ms, that the proton takes to reach this speed. flag question: question 11
The proton accelerates from rest in a uniform electric field of 600 n/c. In order to find the time interval it takes for the proton to reach a speed of 1.50 mm/s.
We need to use the equation v = v₀ + at, where v is the final velocity, v₀ is the initial velocity (which is 0 in this case), a is the acceleration, and t is the time interval. The acceleration of the proton in the electric field is a = E/m, where E is the electric field and m is the mass of the proton. Substituting these values into the equation gives us:
1.50 mm/s = 0 + (600 n/c/1.67 x 10⁻²⁷ kg) x t
Rearranging the equation and solving for t gives us the time interval:
t = 1.50 mm/s/(600 n/c/1.67 x 10⁻²⁷ kg)
t = 8.33 x 10⁻¹³ s
t = 8.33 ms
Therefore, it takes the proton 8.33 ms to accelerate from rest to a speed of 1.50 mm/s in the uniform electric field of 600 n/c.
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In the absence of external forces, momentum is conserved ina. quadrupledb. Yes, force will be less on a carpetc. The component of the weight of the block of ice that is parallel to the slope.d. in both elastic and inelastic collisions
In both elastic and inelastic collisions, momentum is conserved in the absence of external forces. Option d is the correct answer.
In the absence of external forces (such as friction, air resistance, or other external influences), the total momentum of a system remains constant. This is known as the law of conservation of momentum. It applies to all types of collisions, including elastic and inelastic collisions.
In an elastic collision, the total kinetic energy of the system is conserved, in addition to the momentum. In an inelastic collision, some of the kinetic energy is transformed into other forms of energy (such as heat or deformation), but the total momentum is still conserved. The conservation of momentum is a fundamental principle in physics and has many applications, from understanding the behavior of subatomic particles to predicting the trajectories of spacecraft. Hence option d is correct.
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Find the angle ϕ between the filter's polarizing axis and the direction of polarization of light necessary to increase the ratio of the clouds' intensity to that of the blue sky so that it is three times the normal value. Express your answer in degrees to four significant figures
"The required angle Ф between the filter's polarizing axis and the direction of polarization of light necessary to increase the ratio of the clouds' intensity to that of the blue sky so that it is three times the normal value is 65.9°."
A photographer wants to click a picture of a cloud formation, the ratio of clouds intensity to that of the blue sky photographer uses polarizing filter from Malus law,
I = I₀ cos²Ф
So, I f = I i cos²Ф
As the light from cloud is polarized, its intensity reduces to half.
I c = I₀/2
The intensity of light from sky is polarized light.
I s = I₀ cos²Ф
Hence, the ratio of intensities is,
I c/I s = (I₀/2)/(I₀ cos²Ф)
3 = (I₀/2)/(I₀ cos²Ф)
cos²Ф = 1/6
Thus, the required angle is Ф = cos⁻¹(1/√6) = 65.9°
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Which of the following characterizes the Kuiper belt?
A. It is a disk-like region between the outer planets and the Oort cloud.
B. It is up to 100,000 AU in size and spherical in shape.
C. It lies between the orbits of Mars and Jupiter.
D. It is a stable region just ahead of Jupiter in its orbit.
E. It is the region occupied by the Earth-crossing Apollo asteroids.
The Kuiper belt is a disk-like region between the outer planets and the Oort cloud. Thus, option A is correct
The Kuiper belt, also known as the trans-Neptunian region, is a doughnut-shaped region of space beyond Neptune that is home to an estimated 100,000 tiny, icy objects.
It is named after Dutch-American astronomer Gerard Kuiper, who first proposed its existence in 1951.
The belt ranges in distance from 30 to 50 astronomical units (AU) from the Sun, which is about 2.8 to 4.7 billion miles away.
The Kuiper belt objects are believed to be remnants from the formation of the solar system. They are small and mostly made up of ice and dust, similar to comets.
Some Kuiper belt objects, such as Pluto and Eris, are classified as dwarf planets.
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a runner sprints around a circular track of radius 100 m at a constant speed of 7 m/s. the runner's friend is standing at a distance 200 m from the center of the track. how fast is the distance between the friends changing when the distance between them is 200 m? (round your answer to two decimal places.) m/s
The change in the distance between the friends changing when the distance between them is 200 m is 7.85m.
What is the distance?Consider a right-angled triangle with the radius of the circular track as one side of the right angle. Then the other two sides are the distance covered by the runner (in a single lap) and the distance between the runner and his friend.
Since the radius is perpendicular to the line connecting the friend and the center of the track, we can call it the hypotenuse of the triangle.
Let x be the distance between the runner and his friend. We are given that x = 200 m.Using the Pythagorean theorem, we can find the distance covered by the runner in a single lap of the track.
e can now differentiate the above expression with respect to time to find the rate of change of the distance covered by the runner (this will also be the rate of change of the distance between the runner and his friend).Hence,
2x(dx/dt) = 2 (distance covered by runner)(d(distance covered by runner)/dt)
dx/dt = (distance covered by runner)
(d(distance covered by runner)/dt) / x
Substituting x = 200 m and d(distance covered by runner)/dt = 7 m/s, we get:
dx/dt = (223.6 m)(7 m/s) / 200 m = 7.85 m/s.
Rounding off to two decimal places, we get:
dx/dt = 7.85 m/s.
Therefore, the answer is 7.85.
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given what you learned from the figure, rank these types of light in order of increasing energy. 1. radio 2. infrared 3. orange 4. green 5. ultraviolet
Answer:
✓ 1. radio 2. infrared 3. orange 4. green 5. ultraviolet
Explanation:
an airplane flies due west at an airspeed of 425 mph. the wind is blowing from the northeast at 40 mph. what is the ground speed of the airplane? what is the bearing of the airplane?
An airplane flies due west at an airspeed of 425 mph and the wind is blowing from the northeast at 40 mph, the ground speed of the airplane is 385 mph, and the bearing of the airplane is 285°.
We can use the equation
GS = AS + (Wind x cos(Θ)),
Where GS is the ground speed, AS is the airspeed, and Θ is the angle between the wind and the heading of the airplane. the airspeed is 425 mph, the wind is blowing from the northeast at 40 mph, and the heading of the airplane is due west. The angle Θ is 90°. Plugging these values into the equation, we get
GS = 425 + (40 x cos(90°)) = 385 mph.
To calculate the bearing of the airplane, we can use the equation
Bearing = 180° - (Θ + (Wind ÷ AS) x 180°).
Θ is 90°, the wind is 40 mph, and the airspeed is 425 mph.
Plugging these values into the equation, we get
Bearing = 180° - (90° + (40 ÷ 425) x 180°) = 285°.
Hence , airplane flies due west at an airspeed of 425 mph and the wind is blowing from the northeast at 40 mph, the ground speed of the airplane is 385 mph, and the bearing of the airplane is 285°.
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a ball is dropped a from a height of 16ft each time it hits the ground what is the total vertical distance it traveled after it came to rest
The total vertical distance that the ball traveled after it came to rest is 32 feet. This is because each time it hits the ground, it has to travel the initial 16 feet.
Given, a ball is dropped from a height of 16ft. When it hits the ground each time, it bounces back to a height of 8ft. Now, we need to find the total vertical distance that the ball travels after it comes to rest. After the first drop, the ball travels a total distance of 16ft + 8ft = 24ft. After the second drop, the ball travels a total distance of 8ft + 8ft = 16ft.
After the third drop, the ball travels a total distance of 8ft + 8ft = 16ft. After the fourth drop, the ball travels a total distance of 8ft + 8ft = 16ft.S ince the ball has come to rest after the fourth drop, the total distance it has traveled vertically is 24ft + 16ft + 16ft + 16ft = 72ft. The ball travels a total vertical distance of 72ft in four drops.
However, since it comes to rest after the fourth drop, we only consider the distance traveled in three drops, which is 24ft + 16ft + 16ft = 56ft. Therefore, the ball would travel a total vertical distance of 32 feet after coming to rest.
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two forces are applied to a 12 kg cart on a frictionless surface as shown. at a certain instant, force a is 77 n to the right, and force b is 15 n to the left. what is the acceleration of the cart at this instant, in m/s2?
The acceleration of the cart at this instant is calculated to be 5.17 m/s² to the right.
What is Newton's second law?Newton's second law explains that acceleration of any object is directly related to net force and inversely related to the mass.
To determine the acceleration of the cart, we need to calculate the net force acting on it.
The net force is the vector sum of the two forces:
Net force = Force a + Force b = 77 N to the right - 15 N to the left = 62 N to the right
Using Newton's second law, F = ma, where F is the net force and m is the mass of the cart, we can calculate the acceleration:
a = F/m = 62 N / 12 kg = 5.17 m/s
Therefore, the acceleration of the cart at this instant is 5.17 m/s² to the right.
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In a P-N-P transistor application, the solid state device is turned on when the
base is negative with respect to the emitter.
A P-N-P transistor conducts between the emitter and collector (is turned on) when a small amount of current flows into the base. This current flows when the emitter-base junction is forward biased. It is forward biased when the base is negative with respect to the emitter.
A P-N-P transistor is turned on when the base is negative with respect to the emitter.
How the transistor is turned on when the base is negative with respect to the emitterThe operation of a P-N-P transistor is based on the principle of a semiconductor diode. When a small current is applied to the base, it causes a larger current to flow through the emitter and collector. This is because the base-emitter junction is forward-biased, allowing electrons to flow from the emitter to the base. At the same time, the collector-base junction is reverse-biased, allowing holes to flow from the base to the collector.
This flow of electrons and holes produces a current gain. The amount of current gain depends on the type of transistor and the amount of current applied to the base.
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Two charges, -2.1 μC and -5.6 μC , are located at (-0.50 m , 0) and (0.50 m , 0), respectively. There is a point on the x-axis between the two charges where the electric field is zero. Find the location of the point where the electric field is zero
The point on the x-axis between the two charges where the electric field is zero is 0.747 m, when the charges -2.1 μC and -5.6 μC are located at (-0.50 m , 0) and (0.50 m , 0), respectively.
An electric field is defined as the electric force per unit charge. It is a field of force surrounding electrically charged particles, such as electrons or protons in motion, that exerts force on surrounding matter. It is represented by the symbol E.
The electric field E at any point (x,y) on the x-axis due to the charge Q1 at (-0.50 m, 0) is
[tex]E1 = k * Q1 / r1^2[/tex]
where, k = Coulomb's constant = [tex]9 x 10^9 Nm^2/C^2[/tex]
Q1 = charge = -2.1 μC
r1 = distance between Q1 and
(x,y) = (0.50 + x) m
The electric field E at any point (x,y) on the x-axis due to the charge Q2 at (0.50 m, 0) is
[tex]E2 = k * Q2 / r2^2[/tex]
where,
Q2 = charge = -5.6 μC
r2 = distance between Q2 and (x,y) = (0.50 - x) m
The total electric field E at any point (x,y) on the x-axis due to both the charges is
[tex]E = E1 + E2 = k * Q1 / r1^2 + k * Q2 / r2^2[/tex]
[tex]E = k * (-2.1 * 10^-6) / (0.5 + x)^2 + k * (-5.6 * 10^-6) / (0.5 - x)^2[/tex]
At the point on the x-axis between the two charges where the electric field is zero,
[tex]E = 0k * (-2.1 * 10^-6) / (0.5 + x)^2 + k * (-5.6 * 10^-6) / (0.5 - x)^2 = 0[/tex]
Simplifying, we get [tex](0.5 + x)^2 / (0.5 - x)^2 = 2.667x^2 + 2.667x - 0.50 = 0[/tex]
Solving for x, we get
x = -1.74 m or
x = 0.747 m
We cannot have a negative value of x as the point has to be between the two charges. So, the location of the point where the electric field is zero is x = 0.747 m.
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basic behavior: according to your data, does this resistance increase or decrease with voltage? a reasonable (and correct) thought is that the impact is really with temperature, as the light bulb heats up with more power going into it. how does your data imply resistance varies with temperature?
Based on the given question, the resistance will: increase with the increase in voltage.
The reason behind this is that resistance and voltage have a direct relationship. As the voltage increases, the resistance also increases. This can be explained by Ohm’s Law which states that V= IR where V is voltage, I is current and R is resistance. As per the second part of the question, it is implied that the resistance varies with temperature.
The resistance of any material depends upon temperature, and a rise in temperature increases the resistance of the material. The light bulb acts as a resistor, and its resistance will increase as the temperature increases due to an increase in the temperature of the filament of the bulb.
The resistance is directly proportional to the temperature of the bulb, and it is represented by the equation
R = R₀ (1 + αt),
where R is resistance, R₀ is the resistance at a particular temperature, α is the temperature coefficient of resistance, and t is the temperature difference in Celsius.
Therefore, based on the data provided, it can be concluded that resistance increases with the increase in temperature which results in the heating of the light bulb, which is a resistor.
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fundamental questions early astronomers tried to answer were: 1) what is the shape and size of earth? 2) what are the distances from earth to the sun and moon? and 3) blank ?
The third fundamental question early astronomers tried to answer was: What are the motions of the planets and stars in the night sky?
The shape of the Earth is an oblate spheroid, and its approximate diameter is 12,742 km. The average distance from Earth to the Sun is 149,598,262 km, and the average distance from Earth to the Moon is 384,400 km. 3) What are the motions of the planets? The motions of the planets were observed by ASTRONOMES to be elliptical, with the Sun at one focus.
Early astronomers were curious to understand the shape and size of Earth, as well as the distances from Earth to the Sun and Moon. Additionally, they were interested in determining the motions of the planets and stars in the night sky.
The ancient Greeks believed that the universe was a series of concentric spheres with the Earth in the center. Aristotle, a Greek philosopher, believed that the Earth was at the center of the universe, and that everything else, including the stars and planets, orbited around it. The Greek philosopher Eratosthenes was the first to calculate the Earth's circumference. He did so by measuring the angle of the sun's rays at noon on the summer solstice at two different locations and using the difference to estimate the distance between the two places.
In conclusion, early astronomers attempted to answer fundamental questions regarding the shape and size of Earth, the distances from Earth to the sun and moon, and the motion of stars and planets in the sky .
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Proton 1 moves with a speed v from the east coast to the west coast in the continental United States; proton 2 moves with the same speed from the southern United States toward Canada. Is the magnitude of the magnetic force experienced by proton 2 greater than, less than, or equal to the force experienced by proton 1? O greater than the force experienced by proton 1 O less than the force experienced by proton 1 equal to the force experienced by proton 1
The magnitude of the magnetic force experienced by proton 2 will be less than the force experienced by proton 1. This is because the force experienced by a proton is related to the direction of its motion relative to the direction of the magnetic field.
As proton 1 is travelling from east to west, its motion is parallel to the magnetic field, which is aligned in a north-south direction in the continental United States. This means that proton 1 will experience a greater force due to the magnetic field than proton 2, which is travelling in a north-south direction and thus has a motion perpendicular to the magnetic field.
To understand this more clearly, we can consider the equation for the magnetic force:
F = qvB sin θ.
In this equation, the force experienced by a particle is related to the charge (q), velocity (v), and magnetic field strength (B). The sine of the angle between the velocity and magnetic field (θ) is also important as it determines how much of the force will be experienced by the particle. As proton 1's motion is parallel to the magnetic field, it will experience the full force due to the magnetic field, whereas proton 2's motion is perpendicular to the magnetic field and it will only experience a fraction of the force. The magnitude of the force experienced by proton 2 will be lower than the force experienced by proton 1.
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if the leftover energy in the previous problem is 134.9 j (it's not, don't go back and try to use this value) and the mass is 2 kg, what speed (in m/s) does the block have at the bottom of its slide? revisit the definition of ke if needed.
The speed of the block at the bottom of its slide is 16.4 m/s.
In the previous problem, the kinetic energy of the block was found to be 135 J.
The formula for kinetic energy is
KE = 1/2mv²,
Where:
m is the mass of the object and v is its velocity.Now we can use the same formula to find the velocity of the block at the bottom of its slide.
KE = 1/2mv²
We know that the mass of the block is 2 kg, and the kinetic energy at the end of the slide is 135 J.
KE = 135 Jm = 2 kg1/2mv² = 135 Jv² = 2(135 J) / 2 kgv² = 270 JV = sqrt(270 J) / 2 kgV = 16.4 m/s
Therefore, the speed of the block at the bottom of its slide is 16.4 m/s.
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Imagine another solar system, with a star of the same mass as the Sun. Suppose a planet with a mass twice that of Earth (2MEarth) orbits at a distance of 1 AU from the star. What is the orbital period of this planet? Hint: Think about how the mass of the Sun compares with the mass of the Earth. a. 3 months b. 6 months
c. 1 year d. 2 years
e. It would not be able to orbit at this distance.
The correct answer is option D.2 years
What is Kepler's third law of planetary motion?According to Kepler's Third Law of Planetary Motion, T² is proportional to r³, where T is the period of revolution of the planet and r is the distance between the planet and the star.
In order to solve for T,
AU = 1
Astronomical Unit = the average distance between the Earth and the Sun = 149.6 million kilometres
Therefore, the planet is orbiting at a distance of 149.6 million kilometres from the star.
Substituting the values of r and solving for
T².T² ∝ r³T² ∝ (149.6)³T²
= (149.6)³T²
= 3.522 x 10¹²T
= √3.522 x 10^¹²T
= 1.87 x 10⁶ seconds
T = 31,100 minutes
T = 518 hours
T = 21.6 days
T = 2 years
Therefore, the orbital period of the planet with twice the mass of Earth orbiting at a distance of 1 AU from a star with the same mass as the Sun is 2 years.
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