the vector gravitational force acting on block 2 due to block 1 is approximately 1.2674 x 10^(-7) N in magnitude.
To determine the vector gravitational force acting on block 2 due to block 1, we can use Newton's law of universal gravitation:
F = G * (m1 * m2) / r^2
where F is the gravitational force, G is the gravitational constant (approximately 6.67430 x 10^(-11) N m^2/kg^2), m1 and m2 are the masses of the two blocks, and r is the distance between their centers of mass.
Given that the mass of block 1 is 37 kg and its position is (4, 11, 0) m, and the mass of block 2 is 1140 kg and its position is (22, 11, 0) m, we can calculate the distance between their centers of mass:
r = √((x2 - x1)^2 + (y2 - y1)^2 + (z2 - z1)^2)
r = √((22 - 4)^2 + (11 - 11)^2 + (0 - 0)^2)
r = √(18^2 + 0^2 + 0^2)
r = 18 m
Now we can calculate the gravitational force:
F = (6.67430 x 10^(-11) N m^2/kg^2) * (37 kg * 1140 kg) / (18 m)^2
F ≈ 1.2674 x 10^(-7) N
Therefore, the vector gravitational force acting on block 2 due to block 1 is approximately 1.2674 x 10^(-7) N in magnitude.
For the second part of the question, to determine the momentum of block 2 at 4.55 seconds after noon, we need to know its velocity. Without that information, we cannot calculate the momentum. Please provide the velocity of block 2 at that time so that we can assist you further.
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The gravitational force acting on block 2 from block 1 depends on the distances between them but can't be calculated with the given information. The momentum of block 2 at any given time would be zero due to no external forces. The comparison of speed of block 1 and block 2 can't be made without information about their velocities.
Explanation:The gravitational force acting on block 2 due to block 1 can be calculated using Newton's law of gravitation. This law states that every particle of matter in the universe attracts every other particle with a force that is directly proportional to the product of their masses and inversely proportional to the square of the distance between their centers.
To calculate the vector force, we would need to know the exact position of these two blocks in three dimensional space. This would involve calculating the distance vector from block 1 to block 2, then use this to calculate the force vector by multiplying the magnitude of the gravitational force (calculated using Newton's law) by the unit vector in the direction of the distance vector. However, given the current details, a precise calculation can't be performed.
As for the momentum of block 2 at 4.55 seconds after noon, it can be calculated using the equation p = mv , where p is momentum, m is mass and v is velocity. Since no external forces are mentioned, block 2 would remain at rest, meaning its velocity is 0 and thus its momentum is also 0.
The question about whether block 1 is moving faster than block 2, or vice versa or both have the same speed, cannot be answered without knowing details about their velocities.
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1, Describe one scientific discovery or principle that has been
especially important to your life and why you chose that discovery
over others.
The principle of conservation of energy has been an important scientific discovery that has helped me appreciate the value of energy and the need to use it wisely and efficiently.
The scientific discovery that has been especially important to my life is the principle of conservation of energy. This principle states that energy cannot be created or destroyed but can only be converted from one form to another, and the total amount of energy in a closed system remains constant.
Conservation of energy has been important to my life because it has helped me understand the importance of conserving resources. It has helped me appreciate the importance of renewable energy sources such as wind, solar, and hydroelectric power, and the need to reduce our dependence on non-renewable sources such as coal, oil, and gas.
Conservation of energy has also helped me understand the concept of energy efficiency. By using energy-efficient appliances and reducing energy wastage, we can reduce our energy consumption and save money on utility bills. Overall, the principle of conservation of energy has been an important scientific discovery that has helped me appreciate the value of energy and the need to use it wisely and efficiently.
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A person standing on the ground observes a bird flying due west at a speed of 4.10 m/s. At the same time, a passenger in a car moving due north at 22.0 m/s observes the same bird. Determine the magnitude and direction of the bird's velocity relative to the car's passenger. (Assume north and east are along the positive y - and x-axes, respectively.)
magnitude
direction
m/s
∘W of S
Question 3.2b: Radar mounted on a northbound police motorcycle detects an oncoming car's speed to be 37.0 m/s. The car is traveling south with a speed of 17.0 m/s relative to the ground. Determine the speed of the police motorcycle relative to the ground. (Assume north is along the positive y-axis.) m/s
The magnitude of the bird's velocity relative to the car's passenger is 22.4 m/s, and the direction is 10.7° W of S.
Given data:
Velocity of bird in x-direction: Vbx = 4.10 m/s
Velocity of car in y-direction: Vcy = 22.0 m/s
The magnitude of bird's velocity relative to the car's passenger, Vbc, is given as:
Vbc = sqrt((Vbx)² + (Vcy)²)
Vbc = sqrt((4.10 m/s)² + (22.0 m/s)²)
Vbc = sqrt(16.81 + 484)
Vbc = sqrt(500.81)
Vbc = 22.4 m/s (approx)
The direction of bird's velocity relative to the car's passenger is given as:
tanθ = (Vbx)/(Vcy)
θ = tan⁻¹(Vbx)/(Vcy)
θ = tan⁻¹(4.10/22.0)
θ = 10.7° W of S (approx)
Answer:
Therefore, the magnitude of the bird's velocity relative to the car's passenger is 22.4 m/s, and the direction is 10.7° W of S.
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Question: The average speed of a car which covers half the distance with a speed of 20 m/s and other half with a speed of 30 m/s in equal intervals of time is 125 m/s
2
0 m/s
3
24 m/s 424 m/s
The average speed of a car that covers half the distance with a speed of 20 m/s and the other half with a speed of 30 m/s in equal intervals of time is 24 m/s.
Lets x be the total distance covered by the car.
Half of the distance covered with a speed of 20m/s at time t1
t1 = [tex]x/20*2[/tex]
t1 = [tex]x/40[/tex]
The half distance covered with the speed of 30m/s at time t2
t2 = [tex]x/30*2[/tex]
t2 = [tex]x/60[/tex]
Total time = t1 + t2
Total time = [tex]x/40 + x/60[/tex]
Total time = [tex]x/24\\[/tex]
The average speed is given by
[tex]v=x/t\\v= x/x/24\\v=24[/tex]
Therefore, the average speed is 24 m/s.
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Two equipotential surfaces surround a +2.10×10
−8
−C point charge. How far is the 240−V surface from the 57.0−V surface? Number Units
The electric potential difference between the two equipotential surfaces equals the difference between the potential of the 240-V surface and the potential of the 57.0-V surface, and is given by:∆V=V_1−V_2=240−57=183 V The electric potential difference is related to the work done per unit charge by a source that moves a charge between two points in an electric field by the equation: ∆V=W/q, where W is the work done and q is the amount of charge.
Therefore, the amount of work done on a unit charge by a field between two equipotential surfaces equals the electric potential difference between them.If the potential of the +2.10×10-8-C point charge is zero at infinity, then its potential at a distance r from it is given by:V=kq/r, where k = 9×109 N·m2/C2 is Coulomb's constant. Thus, the potential of the +2.10×10-8-C point charge at the 240-V surface is:240=k(2.10×10-8)/r_1r_1=k(2.10×10-8)/240 = 8.75 m The potential of the +2.10×10-8-C point charge at the 57.0-V surface is:57=k(2.10×10-8)/r_2r_2=k(2.10×10-8)/57.0 = 31.47 m
The distance between the two equipotential surfaces is the difference between their distances from the +2.10×10-8-C point charge:d=r_1-r_2=8.75-31.47=−22.72 m = -2.272×10² mThus, the distance between the two equipotential surfaces is 2.272×10² m or -227.2 m (since it is negative, it means that the 240-V surface is closer to the +2.10×10-8-C point charge than the 57.0-V surface).Answer: -227.2 m.
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An electric field given by
E
=7.5
i−8.1(y
2
+6.7)
j
^
^
pierces the Gaussian cube of edge length 0.920 m and positioned as shown in the figure. (The magnitude E is in newtons per coulomb and the position x is in meters.) What is the electric flux through the (a) top face, (b) bottom face, (c) left face, and (d) back face? (e) What is the net electric flux through the cube?
The electric flux through the top face of the cube is 27.31 Nm²/C, through the bottom face of the cube is -1.507 Nm²/C, through the left face of the cube is -6.35 Nm²/C, and through the back face of the cube is -6.86 Nm²/C. The net electric flux through the cube is 12.59 Nm²/C.
Electric field given by E=7.5i−8.1(y^2+6.7)j^ pierces the Gaussian cube of edge length 0.920 m.
The cube is positioned as shown in the figure.
Find the electric flux through the top face of the cube.Given data,Edge length of the cube, l = 0.920 m.
Area of the cube, A = l² = (0.920 m)² = 0.8464 m².
The electric field given by E=7.5i−8.1(y^2+6.7)j^ pierces through the cube of edge length 0.920 m.
Therefore, flux through the cube can be calculated using the formulaφ = EA.Cosθ.
The angle θ is the angle between the normal to the face and the electric field vector. Here, we consider the normal perpendicular to each face of the cube.Now, we need to find the flux for each face of the cube.
(a) The top face of the cube:For the top face, the normal vector will be in the upward direction, that is, k^= 0i + 0j + k^, where k^ is the unit vector along z-axis.Cosθ = Cos90° = 0.
Substituting the given values in the formula,φ = EA.Cosθ = 0.8464 × (8.1 + 6.7) = 27.31 Nm²/C
(b) The bottom face of the cube:For the bottom face, the normal vector will be in the downward direction, that is, -k^ = 0i + 0j – k^, where k^ is the unit vector along z-axis.Cosθ = Cos90° = 0.
Substituting the given values in the formula,φ = EA.Cosθ = 0.8464 × (-8.1 + 6.7) = -1.507 Nm²/C
(c) The left face of the cube:For the left face, the normal vector will be in the left direction, that is, -i^ = -i^ + 0j + 0k^, where i^ is the unit vector along the x-axis.Cosθ = Cos0° = 1.
Substituting the given values in the formula,φ = EA.Cosθ = 0.8464 × (-7.5) = -6.35 Nm²/C
(d) The back face of the cube:For the back face, the normal vector will be in the left direction, that is, -j^ = 0i^ - j^ + 0k^, where j^ is the unit vector along the y-axis.Cosθ = Cos0° = 1.
Substituting the given values in the formula,φ = EA.Cosθ = 0.8464 × (-8.1) = -6.86 Nm²/C.
Electric flux through the cube:Net flux = Sum of all fluxesφ_net = φ_top + φ_bottom + φ_left + φ_back= 27.31 - 1.507 - 6.35 - 6.86= 12.59 Nm²/C.
Thus, the electric flux through the top face of the cube is 27.31 Nm²/C, through the bottom face of the cube is -1.507 Nm²/C, through the left face of the cube is -6.35 Nm²/C, and through the back face of the cube is -6.86 Nm²/C. The net electric flux through the cube is 12.59 Nm²/C.
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A 60 lb man slides sides down a slide at a water park, and his path is given in the from of cylindrical coordinates,
r(t) = 0.04 t^3 m
θ(t) = 1.8 t rad
z(t) = (120 - 5t) m
If you ignore the size of the man,
a) How long does it take for the man to reach the bottom at z = 0?
b) When the man is at the bottom, what is the velocity vectorr in cylindrical coordinates?
c) Using the force balance equation for the z direction, what is the force the slide must exert in the z direction so that the man does not fall off or through the slide?
a). It takes the man 24 seconds to reach the bottom at z = 0.
b). The velocity vector in cylindrical coordinates when the man is at the bottom is approximately (69.12, 298.56, -5) m/s.
c). The force the slide must exert in the z-direction to prevent the man from falling off or through the slide is 267.1968 N.
a) To find the time it takes for the man to reach the bottom at z = 0, we can set the z-coordinate equation equal to zero and solve for t:
z(t) = 120 - 5t
= 0
Solving this equation, we have:
5t = 120
t = 120 / 5
= 24 seconds
Therefore, it takes the man 24 seconds to reach the bottom at z = 0.
b) To find the velocity vector in cylindrical coordinates when the man is at the bottom, we differentiate the position vector with respect to time:
r(t) = 0.04t³ m
θ(t) = 1.8t rad
z(t) = (120 - 5t) m
Taking the derivatives:
r'(t) = 0.12t² m/s
θ'(t) = 1.8 rad/s
z'(t) = -5 m/s
Therefore, the velocity vector at the bottom can be written as:
v = (r'(t), rθ'(t), z'(t))
= (0.12t², 0.12t² * 1.8, -5)
Plugging in t = 24 seconds (at the bottom), we have:
v = (0.12 * 24², 0.12 * 24² * 1.8, -5)
= (69.12, 298.56, -5) m/s
So, the velocity vector in cylindrical coordinates when the man is at the bottom is approximately (69.12, 298.56, -5) m/s.
c). To determine the force the slide must exert in the z-direction to prevent the man from falling off or through the slide, we can use the force balance equation in the z-direction:
ΣFz = m * az
Since the man is not accelerating in the z-direction (az = 0), the sum of forces in the z-direction should be zero:
ΣFz = 0
The forces acting in the z-direction are gravity (mg) and the normal force (N) exerted by the slide.
At the bottom of the slide, the normal force must balance the weight of the man, so we have:
mg - N = 0
Solving for N, we find:
N = mg
Given that the weight of the man is 60 lb, we need to convert it to Newtons:
m = 60 lb
= 60 lb * 0.4536 kg/lb
= 27.216 kg
Therefore, the force the slide must exert in the z-direction to prevent the man from falling off or through the slide is
N = mg
= 27.216 kg * 9.8 m/s²
= 267.1968 N (approximately 267.2 N).
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the movement of one object around another object is called
The movement of one object around another object is called orbit.
If an object moves around a circular path, it is said to be in orbit. An orbit is a stable path of a celestial body, such as the Moon around Earth, or Earth around the sun. A satellite may also orbit another satellite in space.
Thus, the answer is orbit.
Movement:
The act or process of moving is known as movement. One of the most essential things in life is movement. It's the method we move from one location to another. We utilize it to accomplish our everyday tasks and hobbies. We also move our muscles when we engage in physical activity.
One object:
The term one object refers to a physical entity that can be observed. It is an individual thing that can exist physically, be touched, and have boundaries. It can be seen, felt, and measured as well.
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"Two parallel conducting plates are separated by a distance
d = 10.8 cm.
Plate B, which is at a higher potential has a value of
620 V. The potential at x = 7.50 cm from plate B
is 67.9 V. See diagram b"
First, we find the electric field between the parallel plates, which can be done using the following formula:E = (V/d)where E is the electric field strength, V is the potential difference between the plates and d is the distance between them.
Therefore, E = (620 - 67.9) / 0.108 = 4980 V/m.Next, we use the formula for electric potential, which is given by:V = Edwhere d is the distance from the higher potential plate. Therefore, the potential at x = 7.5 cm from plate B is V = 4980 x 0.075 = 373.5 V.
Given that two parallel conducting plates are separated by a distance of d = 10.8 cm, plate B, which is at a higher potential has a value of 620 V and the potential at x = 7.50 cm from plate B is 67.9 V. In order to find the electric field between the parallel plates, we use the formula:E = (V/d)where E is the electric field strength, V is the potential difference between the plates and d is the distance between them. We can substitute the given values to get:E = (620 - 67.9) / 0.108 = 4980 V/m.
This means that the electric field strength is 4980 V/m.Next, we use the formula for electric potential, which is given by:V = Edwhere d is the distance from the higher potential plate. In this case, the distance is x = 7.5 cm. Therefore, the potential at x = 7.5 cm from plate B is given by:V = 4980 x 0.075 = 373.5 V.This means that the potential at x = 7.5 cm from plate B is 373.5 V. Hence, the potential at x = 7.5 cm from plate B is 373.5 V.
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A proton accelerates from rest in a uniform electric field of 602 N/C. At some later time, its speed is 1.00×10
6
m/s. (a) Find the magnitude of the acceleration of the proton. You appear to have made an error in keeping track of exponents.m/s 2 (b) How long does it take the proton to reach this speed? 115 (c) How far has it moved in that interval? m (d) What is its kinetic energy at the later time?
The kinetic energy of the proton at the later time is 8.35 × 10-12 J. The electric field is defined as the force per unit charge acting on a charged particle in the field. Acceleration is defined as the rate of change of velocity per unit time. In this problem, a proton is accelerated from rest in a uniform electric field of 602 N/C.
Given, Uniform electric field, E = 602 N/C
Initial velocity of proton, u = 0
Speed of proton, v = 1.00 × 106 m/s
(a) Acceleration of proton: The initial velocity of the proton is zero, and it accelerates at a uniform rate, resulting in the following formula: v2 - u2 = 2as
where, v = final velocity = 1.00 × 106 m/s
u = initial velocity = 0
a = acceleration of proton = ?
s = distance traveled by proton = ?
The electric field, E = F/q
where, F = force acting on proton
q = charge of proton = 1.6 × 10-19 CE = ma, where m = mass of proton = 1.67 × 10-27 kg (given)
Thus, a = E(m/q)
The charge on proton = 1.6 × 10-19 C
Acceleration of proton, a = E(m/q)= (602 N/C) [1.67 × 10-27 kg / (1.6 × 10-19 C)]= 6.27 × 1014 m/s2
Therefore, the magnitude of the acceleration of the proton is 6.27 × 1014 m/s2.
(b) Time taken to reach the speed, v: We can use the following formula to calculate the time, t taken by the proton to reach its final velocity, v:
v = u + at
Here, u = 0
a = 6.27 × 1014 m/s2
v = 1.00 × 106 m/s
t = ?
Substituting the given values in the above equation, we get,1.00 × 106 m/s = 0 + (6.27 × 1014 m/s2)t
Time, t taken by the proton to reach 1.00 × 106 m/s = 1.59 × 10-9 s
Therefore, the time taken by the proton to reach its final velocity is 1.59 × 10-9 s.
(c) Distance moved by proton in this time: We can use the following formula to calculate the distance, s traveled by the proton during this time: t = time taken
u = initial velocity
v = final velocity
a = acceleration of proton
Thus, s = ut + 1/2at2
Substituting the given values, we get, s = 0 + 1/2 (6.27 × 1014 m/s2) (1.59 × 10-9 s)2= 1.58 × 10-8 m
Therefore, the distance moved by the proton in this time is 1.58 × 10-8 m.
(d) Kinetic energy of the proton at the later time: We can use the following formula to calculate the kinetic energy, K of the proton: K = 1/2 mv2
Where, m = mass of proton = 1.67 × 10-27 kg
v = velocity of proton = 1.00 × 106 m/s
Therefore, K = 1/2 (1.67 × 10-27 kg) (1.00 × 106 m/s)2= 8.35 × 10-12 J
Thus, the kinetic energy of the proton at the later time is 8.35 × 10-12 J. The electric field is defined as the force per unit charge acting on a charged particle in the field. Acceleration is defined as the rate of change of velocity per unit time. In this problem, a proton is accelerated from rest in a uniform electric field of 602 N/C. In order to determine the acceleration of the proton, we can use the equation a = E(m/q), where E is the electric field strength, m is the mass of the proton, and q is the charge of the proton. The charge on the proton is 1.6 × 10-19 C.
After finding the acceleration, we can calculate the time taken for the proton to reach its final velocity using the equation v = u + at. The distance moved by the proton in that interval can be calculated using the formula s = ut + 1/2at2. Finally, the kinetic energy of the proton at the later time can be calculated using the formula K = 1/2 mv2.
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A bicyclist is finishing his repair of a flat tire when a friend rides by with a constant speed of 3.9 m/s. Two seconds iater the bicyclist hops on his bike and accelerates at 2.1 m/s
2
until the catches his friend. Part A How much time does it take until he catches his friend (atter his friend passes him)? Express your answer using two significant figures. Part B How far has he traveled in this time? Express your answer using two significant figures. Part C What is his speed when he catches up? Express your answer using two significant figure
A) The time it takes for the cyclist to catch his friend (after his friend passes him) is approximately 3.7 seconds.
B) The distance traveled by the cyclist in that time is approximately 28.5 meters.
C) The speed of the cyclist, when he catches up to his friend, is approximately 7.8 m/s.
Part A:
When the cyclist is repairing his bike, his friend is moving away from him at a speed of 3.9 m/s for 2 seconds. During this time, the distance covered by the friend can be found by:
S = v × t
S = 3.9 × 2
S = 7.8 meters
After 2 seconds, the cyclist hops on his bike and accelaterates to catch his friend. When the cyclist catches his friend, they will have covered the same distance. The distance covered by both can be calculated using the following formula:
s = (u × t) + (1/2 × a × t²)
For friend:
When the cyclist starts moving, the friend will already be ahead of him by a distance of 7.8 meters.
s = (u × t) + (1/2 × a × t²)
s = (3.9 × t)
For cyclist:
u = 0 (since he was stationary while repairing his bike)
a = 2.1 m/s²
s = (u × t) + (1/2 × a × t²)
s = (0 × t) + (1/2 × 2.1 × t²)
s = 1.05t²
When the cyclist catches his friend, they will have covered the same distance. Therefore, we can equate both distances:
3.9t = 1.05t²
2.11t = 7.8
t = 3.7 seconds (approx)
Part B:
The distance traveled by the cyclist when he catches up with his friend can be calculated using the formula:
s = (u × t) + (1/2 × a × t²)
s = (0 × 3.7) + (1/2 × 2.1 × 3.7²)
s = 28.5 meters (approx)
Part C:
The speed of the cyclist when he catches his friend can be calculated using the formula:
v = u + at
v = 0 + (2.1 × 3.7)
v = 7.8 m/s (approx)
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Consult Multiple Concept Example9 in preparation for this problem. A golfer, putting on a green, requires three strokes to "hole the ball," During the first putt, the ball rolls 3.7 m due east. For the second putt, the ball travels 1.1 m at an angle of 20.0
∘
north of east. The third putt is 0.33 m due north. What displacement ((a) magnitude and (b) direction relative to due east) would have been needed to "hole the ball' on the very first putt? (a) Number Units (b) Number Units
Answer:
Answer: (a) 3 m (to 1 d.p.) (b) 137° (to 1 d.p.) east of south.
Given
The first putt distance,
s1 = 3.7 m
The second putt distance,
s2 = 1.1 m
The second putt angle,
θ2 = 20.0° north of east
The third putt distance,
s3 = 0.33 m
To find the displacement (magnitude and direction) required to hole the ball on the very first putt:
Let the required displacement = x
Let the angle between the required displacement and due east be θx.
θx = tan-1(Δy/Δx)θx
= tan-1(0/ x)θx
= 0° (θx = 0° because the required displacement is due east)
(a) Magnitude of the required displacement, |x|:
The total displacement, s = x + s2 + s3s
= 3.7 m – 1.1 m cos 20.0° + 0.33 m cos 90°s
= 3.7 m – 1.044 m + 0.33 m
≈ 3 m (to 1 d.p.)
Therefore, the magnitude of the required displacement, |x| ≈ 3 m (to 1 d.p.)
(b) Direction of the required displacement, θx:
The total displacement, s = x + s2 + s3s
= 3.7 m – 1.1 m cos 20.0° + 0.33 m cos 90°s
= 3.7 m – 1.044 m + 0.33 m
≈ 3 m (to 1 d.p.)
Therefore, the direction of the required displacement relative to due east, θx ≈ 137° (to 1 d.p.) east of south.
Answer: (a) 3 m (to 1 d.p.) (b) 137° (to 1 d.p.) east of south.
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Required information From the edge of the rooftop of a building, a boy throws a stone at an angle 25.0
∘
above the horizontal. The stone hits the ground 4.20 s later, 143 m away from the base of the building. (Ignore air resistance.) Find the maximum height reached by the stone. m above the ground
The maximum height reached by the stone is 26.6 m above the ground.
Given: Angle of projection (θ) = 25°Time of flight (t) = 4.20 s
Horizontal range (R) = 143 m
To find: Maximum height (H)Formula: Horizontal Range = R = U cos θ × t (as there is no vertical acceleration)
U = R / (cos θ × t)
Putting values we get,U = 143 / (cos 25° × 4.20)U = 143 / 3.7443U = 38.12 m
Now, Maximum height (H) = U sin θ × (t/2) - 1/2 × g × (t/2)²Where g = 9.8 m/s²
Putting values we get,H = 38.12 × sin 25° × (4.20/2) - 1/2 × 9.8 × (4.20/2)²H = 26.6 m
Thus, the maximum height reached by the stone is 26.6 m above the ground.
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A bridge rectifier is supplied with 120 V
pesk-topeak
sinusoidal signal. If each diode has a junction voltage of 0.3 V, determine: (i) The peak voltage at the output of the rectifier. [2 marks] (ii) A suitable peak inverse voltage rating of each diode. [5 marks] (iii) The average output voltage of the bridge rectifier network [2 marks]
A bridge rectifier is a circuit used to convert alternating current (AC) to direct current (DC). In this case, the bridge rectifier is supplied with a 120 V peak-to-peak sinusoidal signal.
(i) To determine the peak voltage at the output of the rectifier, we need to find the peak voltage of the sinusoidal signal. The peak voltage is equal to the peak-to-peak voltage divided by 2. In this case, the peak voltage is 120 V / 2 = 60 V.
(ii) To determine a suitable peak inverse voltage (PIV) rating of each diode, we need to consider the maximum voltage that will be applied across each diode in the bridge rectifier circuit. The PIV rating of each diode should be greater than or equal to the maximum voltage applied across it. In this case, the maximum voltage across each diode is the peak voltage of the sinusoidal signal plus the junction voltage of the diode. So the PIV rating of each diode should be more than 60 V + 0.3 V = 60.3 V.
(iii) The average output voltage of the bridge rectifier network can be calculated using the formula Vavg = (2/π) * Vpk, where Vpk is the peak voltage. Substituting the value, Vavg = (2/π) * 60 V ≈ 38.19 V.
Therefore, the answers to the questions are:
(i) The peak voltage at the output of the rectifier is 60 V.
(ii) A suitable peak inverse voltage rating of each diode is more than 60.3 V.
(iii) The average output voltage of the bridge rectifier network is approximately 38.19 V.
Note: The calculations provided are based on ideal conditions and assume the diodes are ideal. In real-world scenarios, there might be some voltage drops and losses due to diode characteristics and other factors.
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When ultraviolet light of wavelength 380 nm shines on a certain metal surface, the maximum kinetic energy of the ejected photoelectrons from the metal is 1.50eV. 36. What is the value of the work function of this metal? A. 1.77eV B. 2.54eV C. 3.45eV D. 4.78eV 37. What is the maximum wavelength of light that will eject photoelectrons from this metal? A. 403 nm B. 524 nm C. 615 nm D. 702 nm
the maximum wavelength of light that will eject photoelectrons from this metal is approximately 702 nm.
To find the value of the work function of the metal and the maximum wavelength of light that will eject photoelectrons, we can use the following equations:
1. The energy of a photon (E) is given by E = hf, where h is Planck's constant and f is the frequency of light. We can convert this equation to relate energy and wavelength using the speed of light (c): E = (hc) / λ, where λ is the wavelength of light.
2. The work function (Φ) is the minimum energy required to remove an electron from the metal surface.
3. The maximum kinetic energy of the ejected photoelectrons (KEmax) is given by KEmax = E - Φ, where E is the energy of the incident photon and Φ is the work function.
Given:
Wavelength of incident light (λ) = 380 nm = 380 × 10^(-9) m
KEmax = 1.50 eV = 1.50 × 1.6 × 10^(-19) J (1 eV = 1.6 × 10^(-19) J)
To find the work function (Φ), we can rearrange the equation for KEmax:
Φ = E - KEmax
First, let's find the energy (E) of the incident photon using the equation E = (hc) / λ:
E = (6.63 × 10^(-34) J·s * 3.00 × 10^8 m/s) / (380 × 10^(-9) m)
E ≈ 5.23 × 10^(-19) J
Now, we can find the work function (Φ):
Φ = 5.23 × 10^(-19) J - 1.50 × 1.6 × 10^(-19) J
Φ ≈ 2.54 × 10^(-19) J
Therefore, the value of the work function of this metal is approximately 2.54 eV.
To find the maximum wavelength of light that will eject photoelectrons, we need to find the minimum energy required, which is the sum of the work function and the maximum kinetic energy of the ejected photoelectrons:
Emin = Φ + KEmax
Let's calculate Emin:
Emin = 2.54 × 10^(-19) J + 1.50 × 1.6 × 10^(-19) J
Emin ≈ 5.34 × 10^(-19) J
Now, we can rearrange the equation for energy to find the maximum wavelength (λmax):
λmax = (hc) / Emin
Substituting the values:
λmax = (6.63 × 10^(-34) J·s * 3.00 × 10^8 m/s) / (5.34 × 10^(-19) J)
λmax ≈ 702 nm
Therefore, the maximum wavelength of light that will eject photoelectrons from this metal is approximately 702 nm.
In summary:
37. The maximum wavelength of light that will eject photoelectrons from this metal is D. 702 nm.
36. The value of the work function of this metal is B. 2.54 eV.
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Q1.An electron is exposed to its Lorentz coefficient acceleration field equal to 4, if the mass is equal to 9.1 * 10-31kg, calculate the velocity of the electron when it comes out of this field if you know that the speed of light 3*108 m/s .
Q2.A Photon hit a free electron, gaining him a speed of 0.5c moved for two minutes and then crashed into another particle, losing most of its energy, how long is the time of an observer on Earth's surface
An electron is exposed to its Lorentz coefficient acceleration field equal to 4,
if the mass is equal to 9.1 * 10-31kg, calculate the velocity of the electron when it comes out of this field if you know that the speed of light 3*108 m/s.
The acceleration of an electron due to the Lorentz force in the uniform magnetic field can be given by the formula:
Acceleration
a = e E/m,
Where, e is the charge of electron,
E is the uniform electric field,
m is the mass of electron
Here,
Given,
Lorentz coefficient
acceleration field = a = 4
Mass of electron m = [tex]9.1 * 10^-31 kg[/tex]
Speed of light = c = 3*10^8 m/s
The acceleration of an electron is given by Lorentz force.
f = q (v x B)
Where,
f is the force acting on the particle,
q is the charge of particle,
v is the velocity of the particle
B is the magnetic field strength
The force acting on an electron,
f = ma
Where,
m is the mass of the electrona is the acceleration of the electron
Thus,
we have
f = ma = q (v x B)
The velocity v of the electron in the magnetic field can be given by:
v = (f/qB)
The energy gained by the electron as it is accelerated through the Lorentz coefficient acceleration field can be given by,
KE = (1/2) mv²
The velocity of the electron when it comes out of the Lorentz coefficient acceleration field can be given as
[tex]v = √[2KE / m][/tex]
To find v,
Let's put the given values in the above equation.
[tex]v = √[2 * f * d / m][/tex]
the time of an observer on Earth's surface is approximately 142 seconds.
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Suppose a clay model of a koala bear has a mass of 0.20 kg and slides on ice at a speed of 0.75 m/s. It runs into another clay model, which is initially motionless and has a mass of 0.35 kg. Both being soft clay, they naturally stick together.
What is their final velocity?
The final velocity of the combined clay models after collision is approximately 0.273 m/s.
To solve this problem, we can apply the principle of conservation of momentum. According to this principle, the total momentum before the collision is equal to the total momentum after the collision, assuming no external forces are involved.
The momentum of an object is given by the product of its mass and velocity:[tex]\(p = mv\).[/tex]
Before the collision, the first clay model (with mass 0.20 kg) is moving with a speed of 0.75 m/s, while the second clay model (with mass 0.35 kg) is initially at rest. Therefore, the initial momentum of the system is:
[tex]\(p_{\text{initial}} = (0.20 \, \text{kg}) \times (0.75 \, \text{m/s}) + (0.35 \, \text{kg}) \times (0 \, \text{m/s})\)\\\(p_{\text{initial}} = 0.15 \, \text{kg m/s}\)[/tex]
After the collision, the two clay models stick together and move as a single object. Let's denote the final velocity of the combined system as[tex]\(v_{\text{final}}\).[/tex]
The total mass of the system after the collision is the sum of the masses of the two clay models: 0.20 kg + 0.35 kg = 0.55 kg.
Using the conservation of momentum, we can set up the equation:
[tex]\(p_{\text{initial}} = p_{\text{final}}\)\\\\\(0.15 \, \text{kg m/s} = (0.55 \, \text{kg}) \times (v_{\text{final}})\)\\\\Solving for \(v_{\text{final}}\), we find:\\\\\(v_{\text{final}} = \frac{0.15 \, \text{kg m/s}}{0.55 \, \text{kg}}\)\\\\\(v_{\text{final}} \approx 0.273 \, \text{m/s}\)[/tex]
Therefore, the final velocity of the combined clay models after the collision is approximately 0.273 m/s.
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A proton is released near the equator and falls toward the earth under the influence of gravity. The magnetic force on the proton will be toward the west. The magnetic force will be zero. east. north. south.
The magnetic force on the proton will be zero.
When a proton falls toward the Earth under the influence of gravity, it experiences only gravitational force and not magnetic force. The magnetic force on a charged particle depends on its velocity and the presence of a magnetic field. In this scenario, the proton is only subjected to the gravitational force directed towards the center of the Earth. Therefore, there is no magnetic force acting on the proton, resulting in a magnetic force of zero
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4. Aluminum is a very light metal, with a density of 2.7 g/cm3. What is the dough in pounds of A solid aluminum sphere of a radius equal to 50 cm ?. (Density = mass/volume and mass = densityxvolume); (Sphere volume =v=4/3 tr^3 where tt(pi)=3,1416) A C
The density of aluminum is 2.7 g/cm3, and a solid aluminum sphere has a radius of 50 cm. The volume of a sphere can be calculated using the formula `V = (4/3)πr³` where `r` is the radius of the sphere and `π` is a constant approximately equal to 3.
The volume of the aluminum sphere is given by:`
V = (4/3)π(50 cm)³ = 5.24 x 10⁵ cm³`
Now we can use the formula `mass = density x volume` to calculate the mass of the sphere. Substituting the values,
we get:`
mass = 2.7 g/cm³ x 5.24 x 10⁵ cm³ = 1.4148 x 10⁶ g`
To convert grams to pounds, we can use the conversion factor 1 lb = 453.592 g.
The mass of the sphere in pounds is given by:`
mass = 1.4148 x 10⁶ g x (1 lb/453.592 g) = 3115.2 lb`
Thus, the dough of the solid aluminum sphere is 3115.2 lb.
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A jogger that is initially running in a straight line on level ground at 3.0 m/s uniformly accelerates at 2.0 m/s
2
for a time of 3.0 s. How far does the jogger run in this time interval? a. 16 m b. 20 m c. 12 m d. 14 m e. 18 m
The jogger runs a distance of 18.0 meters in the given time interval.
Hence, the correct answer is e. 18 m.
To determine the distance the jogger runs in the given time interval, we can use the equation of motion for uniformly accelerated motion:
s = ut + (1/2)at^2,
where s is the distance, u is the initial velocity, a is the acceleration, and t is the time. Velocity is a vector quantity that describes the rate of change of an object's position with respect to time.
Mathematically, velocity (v) is calculated using the formula:
v = Δx / Δt,
Given:
Initial velocity, u = 3.0 m/s
Acceleration, a = 2.0 m/s^2
Time, t = 3.0 s
Substituting these values into the equation, we get:
s = (3.0 m/s)(3.0 s) + (1/2)(2.0 m/s^2)(3.0 s)^2
s = 9.0 m + (1/2)(2.0 m/s^2)(9.0 s^2)
s = 9.0 m + 9.0 m
s = 18.0 m
Therefore, the jogger runs a distance of 18.0 meters in the given time interval.
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A bicyclist can coast down a 8.0
∘
hill at a steady 9.5 km/h. The mass of the cyclist plus bicycle is 85.0 kg. If the drag force is proportional to the Part A square of the speed v, so that F
D
=−cv
2
. Calculate the value of the constant c. Express your answer using two significant figures. Part B Calculate the average force that must be applied in order to descend the hill at 20 km/h. Ignore other types of friction. Express your answer using two significant figures.
The constant c in the drag force equation is approximately 278 kg/m. The average force required to descend the hill at 20 km/h is approximately -84.7 N.
To find the value of the constant c in the drag force equation FD = -cv^2, we can use the given information. At a steady 9.5 km/h, the drag force is balanced by the gravitational force down the hill.
Let's convert the speed to meters per second (m/s):
9.5 km/h = 9.5 * 1000 / 3600 = 2.64 m/s
At this speed, the drag force is equal to the gravitational force:
-mg = -cv^2
Substituting the values:
-(85.0 kg)(9.8 m/s^2) = -c(2.64 m/s)^2
Solving for c:
c = (85.0 kg)(9.8 m/s^2) / (2.64 m/s)^2 ≈ 278 kg/m
Thus, the value of the constant c is approximately 278 kg/m.
For Part B, to calculate the average force required to descend the hill at 20 km/h, we follow a similar approach. Convert the speed to m/s:
20 km/h = 20 * 1000 / 3600 = 5.56 m/s
Since the cyclist is descending the hill, the drag force opposes the motion, so the average force required is equal to the drag force:
Favg = -cv^2
Substituting the values:
Favg = -(278 kg/m)(5.56 m/s)^2 ≈ -84.7 N
Therefore, the average force that must be applied to descend the hill at 20 km/h is approximately -84.7 N.
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Assigned resistance (ohms)
Measured Voltage (volts)
Theoretical Voltage (volts)
Measured Current (amps)
Theoretical Current (amps)
Resistor 1
10
0.45
0.04
Resistor 2
8
2.55
0.81
Resistor 3
3
6.45
0.85
Using Kirchhoff’s loop and current rules, create equations for the circuit so that you can solve for the currents passing through each resistor. Show work on separate piece of paper and attach to this lab report as your calculations page. Record these currents in the "Theoretical Current" results in the table provided.
From Ohm’s law, calculate the voltages using the currents that you just found. Show work on your calculations page. Record these voltages in the "Theoretical Voltage" results in the table provided.
The equations of the currents passing through each resistor using Kirchhoff’s loop and current rules is:
For Resistor 1: 0.45 = I1 * 10
For Resistor 2: 2.55 = I2 * 8
For Resistor 3: 6.45 = I3 * 3
The voltages of three resistors using Ohm's Law is:
For Resistor 1: I1 * 10
For Resistor 2: I2 * 8
For Resistor 3: I3 * 3
To solve for the currents passing through each resistor, we can apply Kirchhoff's current rule (also known as Kirchhoff's junction rule) at each junction in the circuit. According to this rule, the sum of currents entering a junction is equal to the sum of currents leaving the junction.
Let's denote the currents passing through Resistor 1, Resistor 2, and Resistor 3 as I1, I2, and I3, respectively. The current entering the junction where Resistor 1, Resistor 2, and Resistor 3 meet is the same as the current leaving that junction.
Equation 1: I1 = I2 + I3
Now, we can use Ohm's law to relate the voltage across each resistor to its current and resistance. Ohm's law states that V = I * R, where V is the voltage, I is the current, and R is the resistance.
For Resistor 1:
Equation 2: 0.45 = I1 * 10
For Resistor 2:
Equation 3: 2.55 = I2 * 8
For Resistor 3:
Equation 4: 6.45 = I3 * 3
By solving Equations 1, 2, 3, and 4 simultaneously, we can find the values of I1, I2, and I3.
After obtaining the values of I1, I2, and I3, we can calculate the theoretical voltages across each resistor using Ohm's law.
For Resistor 1:
Theoretical Voltage for Resistor 1 = I1 * 10
For Resistor 2:
Theoretical Voltage for Resistor 2 = I2 * 8
For Resistor 3:
Theoretical Voltage for Resistor 3 = I3 * 3
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as an aid in solving this problem. A portable electric heater uses 16.2 A of current. The manufacturer recommends that an extension cord attached to the heater receive no more than 2.92 W of power per meter of length. What is the smallest radius of copper (resistivity 1.72×10
−8
Ω⋅m ) wire that can be used in the extension cord? (Note: An extension cord contains two wires.) Number Units
The smallest radius of copper wire that can be used in the extension cord is 2.0428 × 10⁻⁴ m.Current = 16.2 A Power/meter = 2.92 W Copper resistivity, ρ = 1.72×10⁻⁸ Ω⋅m.
We know that Power (P) = I²R, where P is power, I is current and R is resistance.R = P/I²For a copper wire, its resistance is given by the formula:
R = (ρL)/A, where ρ is the resistivity of copper, L is the length of the wire and A is its cross-sectional area.
Therefore, we can rewrite the equation above as follows:A = (ρL)/RA = (ρL)/((P/I²) × 2)A = (ρL×I²)/(2P).
Putting the values, we get:A = (1.72 × 10⁻⁸ × 1 × 16.2²)/(2 × 2.92) = 0.4179 × 10⁻⁶ m².
The cross-sectional area is related to the radius of the wire by the formula: A = πr²πr² = Aπr² = (0.4179 × 10⁻⁶ m²)πr² = 1.3108 × 10⁻⁷ m²r² = 1.3108 × 10⁻⁷/πr² = 4.175 × 10⁻⁸ m².
Taking the square root of both sides gives us the radius:r = √4.175 × 10⁻⁸ m² = 2.0428 × 10⁻⁴ m
Answer: The smallest radius of copper wire that can be used in the extension cord is 2.0428 × 10⁻⁴ m.
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For a data set of chest sizes (distance around chest in inches) and weights (pounds) of six anesthetized bears that were measured, the linear correlation coefficient is r 0.144. Use the table valable below to find the critical values of r. Based on a comparison of the linear correlation coefficient r and the critical values, what do you conclude about a linear correlation?
Click the icon to view the table of critical values of r
The critical values are
(Type integers or decimals. Do not round. Use a comma to separate answers as needed.).
Since the correlation coefficient ris
there
sufficient evidence to support the claim of a linear correlation
In order to determine whether a correlation coefficient is statistically significant or not, we use the critical values of r, which can be obtained from a table of critical values of r
The critical values are ±0.811. Since the correlation coefficient r = 0.144 is less than the critical values of r which are ±0.811, there is insufficient evidence to support the claim of a linear correlation.
Hence, the correct option is
Since the correlation coefficient r is less than the critical values of r, there is insufficient evidence to support the claim of a linear correlation.
What is a linear correlation?
Linear correlation is the measure of the degree of correlation or association between two variables in a data set. If there is a strong correlation between the two variables, it indicates that there is a strong relationship between the two. If there is a weak correlation between the two variables, it indicates that there is a weak relationship between the two.
In order to determine whether a correlation coefficient is statistically significant or not, we use the critical values of r, which can be obtained from a table of critical values of r. If the correlation coefficient is greater than the critical value, it indicates that there is sufficient evidence to support the claim of a linear correlation. If the correlation coefficient is less than the critical value, it indicates that there is insufficient evidence to support the claim of a linear correlation.
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Why is there a point of maximum power output for solar cells?
Would changing ambient temperature affect the maximum power output?
The maximum power point for a solar cell occurs at the point where the load resistance is equal to the cell's internal resistance. As a result, temperature changes can have a significant effect on a solar cell's maximum power point and output. Changing ambient temperature will definitely affect the maximum power output of solar cells.
Basically, at any given time, a solar cell's power output is a product of its voltage and current. When the voltage or current output of a solar cell is plotted against the load resistance, the curve has a single maximum point. This point is where the cell's maximum power output can be achieved. As a result, the solar cell's current and voltage must be matched to the load in order to achieve maximum power output.
Because of the internal resistance of a solar cell, it generates heat when current flows through it. The amount of internal resistance, and thus the amount of heat produced, is determined by the cell's composition and design. Temperature, on the other hand, has a significant effect on the amount of heat produced. As a result, temperature changes can have a significant impact on a solar cell's maximum power point and output.
If the temperature rises, the internal resistance of the solar cell decreases, making it easier for current to flow through it. As a result, the solar cell's maximum power point shifts to a lower resistance. This can result in a lower maximum power output, which is not desirable.
On the other hand, if the temperature drops, the solar cell's internal resistance increases. As a result, the maximum power point of the solar cell shifts to a higher resistance. This can also result in a lower maximum power output.
So, changing ambient temperature will definitely affect the maximum power output of solar cells.
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A long straight wire carries a steady direct current. A circular loop of conducting wire is placed directly below the straight wire such that the wire is directly above the plane of the loop as shown
(i). The loop falls vertically below the wire due to gravity, causing a change in the magnetic field through the loop.
(ii). the direction of the induced current can be determined to be clockwise when viewed from above the loop.
(iii). The magnitude of the average e.m.f. induced in the circular loop is 70.65 volts.
(i). An electromotive force (e.m.f.) is induced in the circular loop due to the changing magnetic field caused by the current flowing through the long straight wire.
According to Faraday's law of electromagnetic induction, whenever there is a change in the magnetic field through a loop of wire, an e.m.f. is induced in the loop.
In this case, as the current in the wire is steady, there is no change in the magnetic field due to the current itself.
However, Gravity causes the loop to drop vertically below the wire, changing the magnetic field through the loop. This change in the magnetic field induces an e.m.f. in the loop.
(ii) To determine the direction of the induced current in the circular loop, we can use the right-hand rule for electromagnetic induction.
If we point the thumb of our right hand in the direction of the induced current and curl our fingers around the loop in the direction of the changing magnetic field, then the palm of our hand will point in the direction of the induced current.
In this case, when observed from above the loop, it is possible to establish that the induced current is flowing clockwise.
(iii) To calculate the magnitude of the average e.m.f. induced in the loop, we can use the formula:
e.m.f. = -N * ΔΦ/Δt
Where, N is the number of turns in the loop, ΔΦ is the change in magnetic flux, and Δt is the change in time.
As per data, the average magnetic field within the loop decreases from 120mT to 30mT in 0.040s, we can calculate the change in magnetic flux: ΔΦ = B2 - B1
= 30mT - 120mT
= -90mT
Substituting the values into the formula:
e.m.f. = -N * ΔΦ/Δt
= -N * (-90mT)/(0.040s)
= 2.25N volts.
Since the circular loop has a radius of 5.0 cm, we can calculate the number of turns using the formula:
N = 2πr
= 2π(5.0 cm)
= 31.4 turns
Substituting the value of N into the formula:
e.m.f. = 2.25N volts
= 2.25(31.4 turns)
= 70.65 volts
Therefore, the average emf induced in the circular loop is 70.65 volts in size.
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Complete question is,
A long straight wire carries a steady direct current. A circular loop of conducting wire is placed directly below the straight wire such that the wire is directly above the plane of the loop as shown in the following figure. The loop falls vertically below the wire due to gravity. 7 (i) Explain why an e.m.f. is induced in the loop. (ii) Determine and explain the direction of induced current in the circular loop. (iii) If the circular loop has a radius of 5.0 cm, and the average magnetic field within the loop decreases from 120mT to 30mT in 0.040 s. Calculate the magnitude of the average e.m.f. induced in the loop.
A ball rolls off a platform that is 8 meters above the ground. The ball's horizontal velocity as it leaves the platform is 5 m/5. NOTE: This is a multi-part question. Once an answer is submitted, you will be unable to return to this part. Using the approximate value of g=10 m/s
2
, how much time does it take for the ball to hit the ground? The time taken by the ball to hit the ground is:
The time taken by the ball to hit the ground is 0.860s.
Using the given information, we can calculate the time taken by the ball to hit the ground by using the formula of motion under constant acceleration:
h = ut + (1/2)at²
where, h = 8 meters (height of platform)
u = 5 m/s (horizontal velocity)
a = g = 10 m/s² (acceleration due to gravity)
t = time taken by the ball to hit the ground.
Since the initial vertical velocity of the ball is 0, we can neglect it in this problem.
By substituting the values, we obtain:
8 = 5t + (1/2) × 10 × t²
or, 8 = 5t + 5t²
Rearranging the terms, we get:
5t² + 5t - 8 = 0
Solving this quadratic equation, we get:
According to the Quadratic Formula, t , the solution for At^2+Bt+C = 0, where A, B and C are numbers, often called coefficients, is given by :
t = [- B ± √(B2-4AC)] / 2A
In our case, A = 5, B = 5, C = -8
Accordingly, B^2 - 4AC = 25 - (-160) = 185
Applying the quadratic formula :
t = (-5 ± √ 185) / 10
√ 185 , rounded to 4 decimal digits, is 13.6015
So now we are looking at:
t = ( -5 ± 13.601 ) / 10
Two real solutions:
t =(-5+√185)/10 = -1/2+1/10√ 185 = 0.860
or,
t =(-5-√185)/10 = -1/2-1/10√ 185 = -1.860
Since time cannot be negative, hence t = 0.860 s.
Therefore, it takes 0.860 seconds for the ball to hit the ground.
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If the absolute refractive index at the boundary of two media
increases by 102 %, how many times will the speed of light in the
new medium?
If the absolute refractive index at the boundary of two media increases by 102%, it means that the refractive index of the new medium is 100% + 102% = 202% of the original refractive index.
To find how many times the speed of light will be in the new medium, we need to consider the relationship between the refractive index and the speed of light. The speed of light in a medium is inversely proportional to the refractive index.
Let's assume the original speed of light in the first medium is v. Since the refractive index is proportional to 1/v, the new speed of light in the second medium (v') can be expressed as:
v' = v / (202%)
Simplifying the equation, we can rewrite 202% as a decimal value of 2.02:
v' = v / 2.02
Therefore, the speed of light in the new medium will be approximately 1/2.02 times the speed of light in the original medium.
In summary, the speed of light in the new medium will be approximately 0.495 times (or about half) the speed of light in the original medium.
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If you are carrying a heavy bag of groceries and bang your hand against the wall, the concept that best explains why you are hurt is accelecation. resistance. gravity inertia rione of the nbove
When carrying a heavy bag of groceries and banging one's hand against the wall, the concept that best explains why one gets hurt is acceleration.
Acceleration is the rate of change of velocity of an object with respect to time. It can be explained as a vector quantity which means that it is specified by both direction and magnitude. In a scenario like carrying a heavy bag of groceries and banging one's hand against the wall, acceleration occurs due to the sudden change in velocity of the hand.The hand holding the bag of groceries has a certain velocity while in motion.
The moment it collides with the wall, its velocity changes abruptly, which causes the hand to experience a force in the opposite direction. This force is transferred to the hand from the bag and can result in damage or pain. In other words, the concept that best explains why one gets hurt when they bang their hand while carrying a heavy bag of groceries against the wall is acceleration. It should be noted that the force is due to the sudden change in velocity (or acceleration) of the hand, which causes the hand to experience a force in the opposite direction that can lead to the sensation of pain or injury. So, acceleration is the concept that best explains why one is hurt.
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In a two-state system, there are only two states, one with energy 0 and the other with energy ϵ=0.4eV. What is the average energy of the system at very high temperature 3000 K ? Answer in units of eVand round to three decimal places. Unit conversion: 1eV=1.6×10−19 J Boltzmann constant: kB=1.38×10−23 J⋅K−1 A chemical reaction has an activation energy Eact of about 0.6eV. When the temperature increases from T=300 K (room temperature) to T +ΔT=310 K, how much more probable for a chemical reaction to occur? For example, you can answer the question as "the probability for the chemical reaction to occur at T+ΔT is 1.5 times the probability at T ". Answer as the ratiao of PT+ΔT/PT and round to one decimal place.
The formula for average energy is given as, average energy= Z1E1 + Z2E2/ Z1 + Z2 where E1 and E2 are the energy levels and Z1 and Z2 are their degeneracies (number of states at each energy level).Now, given that the system has two energy levels: one with energy 0 and another with energy ϵ=0.4eV. This gives E1=0 and E2=0.4eV.
Since there are only two states, Z1=1 and Z2=1.So, the average energy of the system at very high temperature 3000 K would be given as: average energy= Z1E1 + Z2E2/ Z1 + Z2= 0×1 + 0.4×1/1 + 1= 0.2eV (rounded to 3 decimal places)Therefore, the average energy of the system at very high temperature 3000 K is 0.2eV (rounded to 3 decimal places).Formula for the probability of a chemical reaction to occur is given by Arrhenius Equation: k= Ae-E act/RTN where, k is the rate constant, A is the frequency factor, R is the universal gas constant and T is the absolute temperature (in Kelvin).
So, the ratio of PT+ΔT/PT at T= 300 K and ΔT = 10 K would be given as:PT+ΔT/PT = A e-E act/RT+ΔT / A e-E act/RT= e-E act/R [1/T+ΔT - 1/T]So, the ratio of PT+ΔT/PT would be:PT+ΔT/PT = e0.6eV/kB[1/(300K + 10K) - 1/300K]= 1.5 (approx)
Therefore, the probability for the chemical reaction to occur at T+ΔT=310 K is 1.5 times the probability at T= 300 K.
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A golfer hits a shot to a green that is elevated 3.20 m above the point where the ball is struck. The ball leaves the club at a speed of 1 m/s at an angle of 33.0
∘
above the horizontal. It rises to its maximum height and then falls down to the green. Ignoring air resistance, find the speed of the ball just before it lands.
To find the speed of the golf ball just before it lands on the green, we can apply the principle of conservation of energy. Conservation of energy is a fundamental principle in physics that states the total energy of a closed system remains constant.
In this problem, the golf ball is initially at a height of zero and rises to a maximum height of H before falling to the ground at a height of 3.20 m. The total change in potential energy of the ball can be expressed as:
mgh = (1/2)mv_final^2 - (1/2)mv_initial^2
Here, m represents the mass of the ball, g is the acceleration due to gravity, h is the maximum height of the ball, v_final is the final velocity of the ball, and v_initial is the initial velocity of the ball.
Given that the initial velocity of the ball, u, is 1 m/s at an angle of 33.0° above the horizontal, we can determine its vertical and horizontal components of velocity as follows:
Vertical component: u sin θ = 1 × sin 33.0° = 0.545 m/s
Horizontal component: u cos θ = 1 × cos 33.0° = 0.853 m/s
At the highest point, the vertical component of velocity becomes zero. Thus, the total change in potential energy is given by:
mgh = (1/2)mv_final^2 + (1/2)mu^2sin^2 θ
Rearranging this equation, we can solve for v_final:-
v_final = √(2gh + u^2sin^2 θ) --(1)
Substituting the given values into equation (1), we can calculate the final velocity of the ball:
v_final = √(2 × 9.81 × 3.20 + 1^2 × sin^2 33.0°)
≈ 9.43 m/s
Therefore, the speed of the ball just before it lands on the green is approximately 9.43 m/s.
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