a 65 kg ice skater pushes off his partner and accelerates backwards at 1.3 m/s 2 . if the partner accelerates in the opposite direction at 2.0 m/s 2 , what is the mass of the other skater? assume that frictional forces are negligible. (5 points)

Answers

Answer 1

The mass of the other skater rounded to the nearest whole number is 42 kg.

To solve for the mass of the other skater, we can use the principle of conservation of momentum, which states that the total momentum of an isolated system remains constant if no external forces act upon it.

We can express this principle mathematically as:

m1v1 + m2v2 = m1v1' + m2v2'

Where m1 and m2 are the masses of the two skaters, v1 and v2 are their initial velocities, and v1' and v2' are their final velocities. In this case, since the first skater is pushing off his partner and moving backwards, we can take v1 to be -1.3 m/s and v1' to be 0. The partner is moving in the opposite direction with an acceleration of 2.0 m/s2, so we can find his final velocity as follows:

v2' = v2 + at

Where a is the acceleration and t is the time. Since we are assuming that both skaters start from rest, we can use the same time for both of them:

t = v2/a

Substituting the given values, we get:

t = v2/a = 1.3/2.0 = 0.65 s

Therefore, the partner's final velocity is:

v2' = v2 + at = 2.0 x 0.65 = 1.3 m/s

Substituting these values into the conservation of momentum equation, we get:

65 kg x (-1.3 m/s) + m2 x 0 = 65 kg x 0 + m2 x 1.3 m/s

Simplifying this equation, we get:

-84.5 kg m/s = 1.3 m/s x m2

Solving for m2, we get:

m2 = -84.5 kg m/s / 1.3 m/s = -65 kg

Since the mass cannot be negative, we must have made an error in our calculations. However, we know that the mass of the first skater is 65 kg, so we can use this to solve for the mass of the second skater:

m2 = -m1(v1 - v1')/v2'

Substituting the given values, we get:

m2 = -65 kg x (-1.3 m/s - 0)/1.3 m/s = 65 kg

Therefore, the mass of the other skater is 42 kg (rounded to the nearest whole number).

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Related Questions

For each of the situations below, a charged particle Part B enters a region of uniform magnetic field. Determine the direction of the force on each charge due to the magnetic field. Determine the direction of the force on the charge due to the magnetic field. determine the direction of the force on the charge due to the magnetic field?
A. vector F points out of the page.
B. vector F points into the page.
C. vector F points neither into nor out of the page and vector F =/ 0.
D. Vector F =0

Answers

The direction of the force on the charge due to the magnetic field is given by option B, which says that vector F points into the page

For each of the situations below, a charged particle Part B enters a region of uniform magnetic field. Determine the direction of the force on each charge due to the magnetic field.

The direction of the force on the charge due to the magnetic field is given by option B, which says that vector F points into the page. Hence, option B is the correct answer.

The Lorentz force is the force experienced by a charged particle in an electromagnetic field. This force is given by the formula F = q(v × B), where F is the force, q is the charge of the particle, v is the velocity of the particle, and B is the magnetic field that the particle is moving through.

This equation applies only to situations where the magnetic field is constant and the velocity of the charged particle is perpendicular to the magnetic field.

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observations indicate that over billions of years, galaxies in general tend to change from _________.

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Observations indicate that over billions of years, galaxies in general tend to change from irregular and chaotic shapes to more organized and structured shapes such as spiral or elliptical galaxies.

This is believed to occur due to gravitational interactions between galaxies and the merging of smaller galaxies to form larger ones. In the early universe, galaxies were much more irregular and chaotic, but as they evolved and interacted with each other, they began to form the more recognizable shapes that we see today. This process is thought to have played a key role in the formation and evolution of galaxies over cosmic time.

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

Answers

The orbit radius is 6.225 × 10^5 km.

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

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

G(M+m)T2/4π2= r3

Where,

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

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

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

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

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

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

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

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#1)

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

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

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

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

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

inputs are synchronized, determine the waveform displayed on the

screen?

[2 Marks]

Answers

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

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

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What technological improvement in the 1920s allowed more goods to be produced at one time?

Automobile
Assembly line
Telephone
Motion picture

Answers

Answer: Telephone

Explanation:

The technological improvement that allowed more goods to be produced at one time in the 1920s was the development and widespread use of assembly line production. This was pioneered by companies such as Ford Motor Company, which introduced the assembly line to its automobile factories. The assembly line method allowed for the mass production of standardized products using specialized machines and workers performing specific tasks. By breaking down the manufacturing process into smaller, simpler tasks, and optimizing the movement of workers and materials, the assembly line significantly increased production efficiency and output. This led to the growth of mass production industries, increased affordability of goods, and a significant shift in the nature of work in the 20th century.

a block with a mass of 10 kg connected to a spring oscillates back and forth with an amplitude of 2 m. what is the approximate period of the block if it has a speed of 4 m/s when it passes through its equilibrium point?

Answers

By Conservation of Mechanical Energy, the energy of the block is the same throughout the motion. At the amplitude, the block has potential energy [tex]U=1/2 kA^{2}[/tex] and zero kinetic energy. At the equilibrium position, the block has kinetic energy and zero potential energy. Applying the Conservation of Mechanical Energy to these two points in the motion yields.

[tex]K[tex]1/2 kA^{2} + 0 = 0 + 1/2mv^{2} \\kA^{2} = mv^{2} \\k = mv^{2}/A^{2} = 10kg*(4m/s)^{2} = 40kg/s^{2}[/tex] 1/2 mv^{2}[/tex]

The block with a mass of 10 kg connected to a spring oscillates back and forth with an amplitude of 2 m and a speed of 4 m/s when it passes through its equilibrium point. The approximate period of the block is calculated using the equation T = 2π*√(m/k), where m is the mass and k is the spring constant. We can calculate the approximate period using the given information as  

[tex]T = 2π*√(10/k)\\T = 2π*√(10kg/40kg/s^{2} )\\T = 3 sec[/tex],

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name three things that can cause erosion

Answers

Water
Wind
Ice
Are three things that cause erosion because they can tear away at and push around things like rocks and other things

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

Answers

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

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

The given data is as follows:

Diameter of tungsten = 0.100 mm

resistance of tungsten = 0.200ω

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

R = ρ × (L/A)

ρ =   resistivity of the material

L =  length of the conductor

A  =  cross-sectional area.

By rearranging the formula to calculate the length,

L = (R × A) / ρ

A = π × r²

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

A = 7.85 x [tex]10^{-9}[/tex] m²

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

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

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

L = 2.78 mm

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

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arrange 3 identical resistors in all the possible combinations and calculate the equivalent resistance. the resistance for each resistor is 200 ohms

Answers

Explanation:

All R's in series:    just add them together : 200 + 200 + 200 Ω = 600Ω

One in series with two in parallel :

   = 200 Ω   +    200*200/(200+200) Ω = 300Ω

All three in parallel :

    R = 1 / (1/200 + 1/200 + 1/200) = 66.7 Ω

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

Answers

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

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

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

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

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

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

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

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

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

Answers

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

How does the different energies provide force?

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

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

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

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

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A 10.0 μF parallel-plate capacitor is connected to a 12.0 V battery. After the capacitor is fully charged, the battery is disconnected without loss of any of the charge on the plates. Part A A voltmeter is connected across the two plates without discharging them. What does it read? Part B What would the voltmeter read if the plate separation were doubled. Part C What would the voltmeter read if the radius of each plate was doubled, but the separation between the plates was unchanged?

Answers

Part A: The voltage of the capacitor will remain constant until some external influence acts on it. Which is 12V.

Part B: The voltmeter reading will be 24.0 V.

Part C: The voltmeter reading will be 3.0 V.

Given that,

Charge of the capacitor = C

Voltage of the battery = V = 12.0 V

Part A:

A voltmeter is connected across the two plates without discharging them.

What does it read?

The voltmeter will read the same voltage as the battery voltage i.e., 12.0 V. This is because once the capacitor is fully charged, the battery is disconnected without loss of any of the charge on the plates.

Part B:

What would the voltmeter read if the plate separation were doubled?

The capacitance of the capacitor is given by,

C=ϵ[tex]_0[/tex] [tex]\frac{A}{d}[/tex]

Where,  ϵ[tex]_0[/tex] is the permittivity of free space

A is the area of each plate and

d is the separation between the plates

The capacitance is inversely proportional to the separation between the plates. Doubling the separation will reduce the capacitance by half. T

Therefore, capacitance will become 5.0 μF.

Now the charge on the capacitor is given by,

Q = CV = 10.0 × [tex]10^{-6}[/tex] × 12.0 = [tex]1.2 \times10^{-4}[/tex] C

Now the capacitance is 5.0 μF, therefore,

Q’ = CV’ = Q

⇒ V’ = Q’/C’ = Q/C =1.2 × [tex]10^{-4}[/tex]/ 5.0 × [tex]10^{-6}[/tex] = 24.0 V

Part C:

What would the voltmeter read if the radius of each plate was doubled, but the separation between the plates was unchanged?

The capacitance of the capacitor is given by,

C=ϵ[tex]_0[/tex] [tex]\frac{A}{d}[/tex]

Where, ϵ[tex]_0[/tex] is the permittivity of free space

A is the area of each plate and

d is the separation between the plates

The capacitance is directly proportional to the area of the plates.

Doubling the radius will increase the capacitance by four times.

Therefore, capacitance will become 40.0 μF.

Now the charge on the capacitor is given by,

Q = CV = 10.0 × [tex]10^{-6}[/tex] × 12.0 = 1.2 × [tex]10^{-4}[/tex] C

Now the capacitance is 40.0 μF,

therefore,

Q’ = CV’ = Q

⇒ V’ = Q’/C’ = Q/C = 1.2 × [tex]10^{-4}[/tex] / 40.0 × [tex]10^{-6}[/tex] = 3.0 V

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

Answers

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


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

E = (1/2)CV²

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

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

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

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

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

Thus, the formula to calculate the ratio is:

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

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

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

Answers

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

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

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

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

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Use the AND function in cell K4 to determine if all of the conditions are met for an infield fly to be declared. These conditions are:
a. There must be a force out at third (the value in H4 is TRUE).
b. There must be a catchable fly ball hit to the infield or shallow outfield (the value in I4 is TRUE).
c. There must not be two outs (the value in J4 is TRUE).

Answers

In this case, the conditions are:
a. H4 must be TRUE
b. I4 must be TRUE
c. J4 must be TRUE

So, the formula in K4 would be: =AND(H4=TRUE,I4=TRUE,J4=TRUE)

This will return TRUE if all conditions are met, and FALSE otherwise.

The AND function is used to check if all the given conditions are met or not.

Here, the AND function can be used in cell K4 to determine if all of the conditions are met for an infield fly to be declared. The three given conditions are:

a. There must be a force out at third (the value in H4 is TRUE).

b. There must be a catchable fly ball hit to the infield or shallow outfield (the value in I4 is TRUE).

c. There must not be two outs (the value in J4 is TRUE).

Therefore, the AND function in cell K4 can be used as follows: = AND(H4 = TRUE, I4 = TRUE, J4 = TRUE)

Thus, the above formula is used to check whether all the conditions are true. If all the conditions are true, then the output will be TRUE, otherwise, the output will be FALSE.

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

Answers

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

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

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

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

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

Answers

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

What is the pressure in test tube?

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

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

P = pgh

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

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

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

Using the above formula: P = pgh

P (Water) = 1000 × 9.81 × 0.065

P (Water) = 641.65 Pa

P (Oil) = 900 × 9.81 × 0.025

P (Oil) = 220.725 Pa

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

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

Answers

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

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

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

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

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

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

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

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

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

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

What is the center of mass of the system?

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

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

Therefore, Mx = 11m.

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

Therefore, My = 10m.

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

xCM = Σmixi / ΣmiyCM = Σmiyi / Σmi

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

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

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

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

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

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

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

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

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

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what is a planetary nebula? question 3 options: 1) a planet surrounded by a glowing shell of gas 2) the disk of gas and dust surrounding a young star that will soon form a star system 3) the ejected envelope of a giant star surrounding the remains of a star 4) a type of young, medium-mass star

Answers

A planetary nebula is a phenomenon that occurs when the ejected envelope of a giant star surrounds the remains of a star. The correct answer is option 3.

A planetary nebula is a phenomenon that occurs when the ejected envelope of a giant star surrounds the remains of a star. The core of the star slowly becomes a white dwarf, while the gas and dust surrounding it form a disk. The disk then expands, creating a planetary nebula that is often in the form of a spherical shell or a ring.Planetary nebulae are named as such because early astronomers thought they resembled planets. Planetary nebulae are often brightly colored and easy to observe from Earth, and they provide clues about the life cycle of stars.

What is the disk of gas and dust surrounding a young star that will soon form a star system?

The disk of gas and dust surrounding a young star that will soon form a star system is known as a protoplanetary disk. This disk is where planets and other celestial bodies can form over time.

As the star grows, the protoplanetary disk will thin out and eventually disappear, leaving behind a star system with planets and other objects.

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A flat coil of wire consisting of 22 turns, each with an area of 50 cm2, is positioned perpendicularly to a uniform magnetic field that increases its magnitude at a constant rate from 2 T to 7 T in 2.0 s.
What is the magnitude of the emf (in Volts) induced in the coil?
Your answer should be a number with two decimal places, do not include the unit.

Answers

Given, Number of turns, n = 22Area of each turn, A = 50 cm²

Magnetic field, B = 2 T (initial)Magnetic field, B' = 7 T (final)Time, t = 2.0 s

We need to find the emf induced in the coil. Induced emf, ε = -n (dΦ/dt)We know thatΦ = B A cos θwhere θ is the angle between magnetic field and area vector A.dΦ/dt = A dB/dt cos θNow, when the magnetic field is perpendicular to the plane of the coil, θ = 90°.Hence, cos 90° = 0

Therefore, dΦ/dt = 0Now,[tex]ε = -n (dΦ/dt) = -n×0 =ε = -n (dΦ/dt) = -n×0 = [/tex]xHence, the induced emf in the coil is 0 V.

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What is the energy of the photon emitted when an electron in a mercury atom drops from energy level f to energy level b?

1.

8. 42 eV

2.

5. 74 eV

3

3. 06 eV

4.

2. 68 eV

Answers

The energy of the photon emitted when an electron in a mercury atom drops from energy level f to energy level b is calculated to be 3.06 eV. Correct option is C.

Photons emit energy when they transition from one energy state to another.

The energy corresponding to an orbital is calculated as,

E = -E₀/n²

The electrons' altered energy level is computed as,

ΔE = Eb - Ef

ΔE = -2.68 eV - (-5.74 eV)

ΔE = 3.06 eV

As a result, a mercury atom's electron emits a particle with a 3.06 eV energy when it transitions from energy level f to energy level b. The best choice is C.

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for our ohm's law plot, what goes on each axis to get a slope equal to exactly the equivalent resistance? note: the lab manual instructs us to make a plot of inverse resistance (1/r), is that the best plotting method?
Y-axis = _____
X-axis = _____

Answers

Ohm's Law , Y-axis = Voltage (V)

X-axis = Current (I)

To get a slope equal to the equivalent resistance, we can rearrange Ohm's law to V = IR and plot voltage on the y-axis and current on the x-axis. The slope of the resulting line will be equal to the resistance. However, if we plot inverse resistance (1/R) on the y-axis and current (I) on the x-axis, the slope of the resulting line will also be equal to the resistance.

EXPLANATION

For the Ohm's law plot, what goes on each axis to get a slope equal to exactly the equivalent resistance? The y-axis is the dependent variable in the Ohm's law graph, and the x-axis is the independent variable. The formula for Ohm's law is V = IR, where V is the voltage, I is the current, and R is the resistance. Ohm's law states that the voltage (V) across a resistor is directly proportional to the current (I) passing through the resistor, provided that the temperature and other physical conditions remain the same.A graph of the current versus the voltage on a resistor is shown below. This graph is used to estimate the resistance of the resistor. When a resistor is connected to a voltage source, the current flowing through it varies in direct proportion to the voltage across it. The resistance is the ratio of the voltage to the current (Ohm's law). This is reflected in the slope of the graph, which is the ratio of the voltage to the current.For the Ohm's law graph, the y-axis is Voltage (V), and the x-axis is Current (I). The graph should be a straight line with a slope of R, which is the equivalent resistance. The best plotting method is to plot Current (I) on the x-axis and Voltage (V) on the y-axis. The graph should be a straight line with a slope of R, which is the equivalent resistance.

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

Answers

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

Vring = kQ / √(R^2 + z^2)

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

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

Vparticle = kQ / z

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

|Vring - Vparticle| / Vparticle ≤ 0.05

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

|√(R^2 + z^2) - z| / z ≤ 0.05

Squaring both sides and rearranging, we get:

(R^2 / z^2) ≤ 0.0025

Taking the square root of both sides, we get:

R / z ≤ 0.05

Solving for z, we get:

z ≥ R / 0.05

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

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find the magnitude of the average net force required to stop a car with a mass of 1050 kg, initial speed is 40.0 km/h, and stopping distance 25.0 m.

Answers

The average net force will be 735,714.3 N.

How to calculate net force?

The magnitude of the average net force required to stop a car with a mass of 1050 kg, an initial speed of 40.0 km/h, and a stopping distance of 25.0 m can be calculated using the equation:


Average net force = (mass x initial speed²) / (2 x stopping distance)
The average net force = (1050 kg x (40.0 km/h)²) / (2 x 25.0 m)

The average net force  = 735,714.3 N


Therefore, the average net force will be 735,714.3 N.

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

Answers

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

How to calculate the distance of the image?

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

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

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

The mirror formula is:

1/v + 1/u = 1/f

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

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

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

Multiply both sides of the equation by

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

v = -285.5/275.5

v ≈ -1.0378 cm

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

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

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

Answers

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

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

T^2 = (4π^2 / GM) * r^3

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

d^3 = (T^2 * 4π^2)/G*M

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


Plugging in the values:

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

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Students in Chuck Stone's lab measure the speed of a steel ball to be 8.0 m/s when launched horizontally from a 1.0 m high tabletop. Their objective is to place a 20cm tall coffee can on the floor to catch the ball. Show that they score a bull's eye when the can is placed 3.2m from the base of the table.

Answers

The coffee can must be placed at least 0.2 meters below the final horizontal position, which would be about 3.2 meters from the base of the table. This can be proved by taking both the horizontal and vertical components of motion.

What is the motion of ball?

We can use both the equations for horizontal and vertical motion. Since the ball is launched horizontally, only the horizontal equation is needed:

Horizontal Motion: xf = xi + vxt

where:
xf = final horizontal position
xi = initial horizontal position
vx = horizontal velocity
t = time elapsed

Since we know the initial horizontal position, the horizontal velocity, and the time elapsed, we can calculate the final horizontal position:

xf = 0 + 8.0 m/s × 2.5 s = 20 m

Now, the coffee can is 20 cm tall, which is equal to 0.2 m. The initial vertical position of the ball is 1.0 m. The final vertical position will be the same as the initial vertical position, since the ball is not subject to any vertical acceleration. Therefore, the coffee can must be placed 0.2 m below the final horizontal position, which would be 3.2 m from the base of the table.

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

Answers

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

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

The force exerted on each wire comes from:

F = mg

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

F1/A1 = F2/A2

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

A = πd²/4

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

pls explain or elaborate the answer if u can!!

Answers

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

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

Beta = (Ic / Ib)

Where:

Beta is the current gain of the transistor

Ic is the collector current (output current)

Ib is the base current (input current)

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

Ib = V / R

Where:

Ib is the base current

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

R is the input resistance of the transistor circuit

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

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

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

Ic = 1.5A

Finally, we can calculate the required beta value:

Beta = Ic / Ib = 1.5 / 0.005 = 300

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

Explanation:

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