The equivalent resistance of the circuit is 4.80Ω.
When resistors are connected in series, their resistances add up to give the equivalent resistance of the circuit.
In this case, three 1.60Ω resistors are connected in series.
To find the equivalent resistance, we simply sum the individual resistances:
Equivalent Resistance = 1.60Ω + 1.60Ω + 1.60Ω
Equivalent Resistance = 4.80Ω
Therefore, the equivalent resistance of the circuit is 4.80Ω.
When resistors are connected in series, the total resistance increases because the current flowing through each resistor is the same, and the voltage drop across each resistor adds up.
The total voltage supplied by the battery is shared across the resistors, leading to a higher overall resistance.
It's important to note that the equivalent resistance is the total resistance of the series combination.
It represents the resistance that a single resistor would need to have in order to produce the same overall effect as the series combination of resistors when connected to the same voltage source.
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The resolution of the timer on your phone is 0.01 s How fast would your phone need to be moving (relative to you) in ms so that the effects of special relativity on its accuracy become significant when measuring a 1
minute process?
The resolution of the timer on the phone is 0.01 s , therefore, the phone would need to be moving at approximately 299,792.45784 meters per millisecond (m/ms) relative to the effects of special relativity on its accuracy to become significant when measuring a 1-minute process.
To calculate the speed required for such significant effects, one can use the formula for time dilation:
Δt' = Δt × √(1 - ([tex]v^2[/tex]/[tex]c^2[/tex]))
Where:
Δt' is the measured time interval by the moving phone (60 seconds + 0.01 seconds)
Δt is the proper time interval (60 seconds)
v is the relative velocity between the phone and the observer
c is the speed of light (approximately 299,792,458 meters per second)
Rearranging the formula,
v = √((1 - (Δ[tex]t'^2[/tex] / Δ[tex]t^2[/tex])) ×[tex]c^2[/tex])
Substituting the given values:
v = √((1 - ((60.01[tex]s^)^2[/tex] / (60 [tex]s^)^2[/tex])) × (299,792,458 m/[tex]s^)^2[/tex])
Calculating the expression:
v ≈ 299,792,457.84 m/s
Converting the speed to meters per millisecond (ms):
v ≈ 299,792,457.84 m/s × (1 ms / 1000 s)
v ≈ 299,792.45784 m/ms
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background q1 a. draw the schematic of a simple circuit including battery, switch, resistor, and capacitor. b. list one possible combination for a resistor value (in ohms) and a capacitor value (in farads) that could provide an rc time constant of 1s. c. describe where you could connect the leads of a voltmeter to measure the voltage drop across your capacitor as a function of time (think back to last week’s lab).
A schematic of a simple circuit includes a battery, switch, resistor, and capacitor connected in series or parallel.
One possible combination for an RC time constant of 1s could be a resistor value of 1 kilohm (1000 ohms) and a capacitor value of 1 microfarad (1 μF).
To measure the voltage drop across the capacitor as a function of time, the leads of a voltmeter can be connected in parallel across the capacitor.
A simple circuit schematic would show the battery symbol with its positive and negative terminals connected to the switch, and the switch further connected to a resistor and a capacitor. The resistor and capacitor can be connected either in series or in parallel.
The time constant (RC) of an RC circuit is the product of the resistance (R) and the capacitance (C). To achieve an RC time constant of 1s, a possible combination could be a resistor value of 1 kilohm (1000 ohms) and a capacitor value of 1 microfarad (1 μF).
To measure the voltage drop across the capacitor as a function of time, the leads of a voltmeter should be connected in parallel across the capacitor. This allows the voltmeter to directly measure the potential difference or voltage across the capacitor during the charging or discharging process. This measurement provides information about the voltage change over time and can be used to analyze the behavior of the capacitor in the circuit.
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Use the following information to answer questions 30 and 31. A 56 resistor, a 220 R resistor, and a 500 resistor are connected in series, and attached to a 60 V battery. The combined resistance in the circuit is Record your answer to three digits, include a decimal if needed. The current flowing in the circuit is mA. (Note the unit here.) Record your answer to two digits, include a decimal if needed
The combined resistance in the circuit is 776 Ω and the current flowing in the circuit is 77.3 mA.
Given: Three resistors are connected in series. The resistors are 56 Ω, 220 Ω, and 500 Ω. The total voltage in the circuit is 60 V.
To find: The combined resistance in the circuit and the current flowing in the circuit.
As the resistors are connected in series, the total resistance (R) can be found by adding the individual resistances.
R = R1 + R2 + R3R
= 56 Ω + 220 Ω + 500 ΩR
= 776 Ω
The combined resistance in the circuit is 776 Ω.
The voltage in the circuit is 60 V.
Using Ohm's Law, the current (I) flowing through the circuit can be found.
I = V / RI = 60 V / 776 ΩI = 0.0773 A (approximately)
The current flowing in the circuit is 77.3 mA (rounded to two decimal places).
When resistors are connected in series, the total resistance is equal to the sum of the individual resistances. Ohm's Law is used to calculate the current flowing in the circuit.
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A by-product of some fission reactors is the isotope ⁹⁴₂₃₉Pu, an alpha emitter having a half-life of 24120 yr: ⁹⁴₂₃₉Pu → ²³⁵₉₂U + α Consider a sample of 1.00 kg of pure ⁹⁴₂₃₉Pu at t=0 . Calculate (a) the number of ⁹⁴₂₃₉Pu nuclei present at t=0
To calculate the number of ⁹⁴₂₃₉Pu nuclei present at t=0, we can use the formula: Number of nuclei = (mass of sample / molar mass of ⁹⁴₂₃₉Pu) * Avogadro's number
The molar mass of ⁹⁴₂₃₉Pu is 239 g/mol. Avogadro's number is approximately 6.022 x 10^23Substituting the values, we have: Number of nuclei = (1.00 kg / 239 g/mol) * (6.022 x 10^23 nuclei/mol)
Number of nuclei = (1000 g / 239 g/mol) * (6.022 x 10^23 nuclei/mol)
Number of nuclei = 25.10 x 10^23 nuclei
Therefore, at t=0, there are approximately 25.10 x 10^23 ⁹⁴₂₃₉Pu nuclei present in the 1.00 kg sample.
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You are attempting a stunt with a hot wheels launcher (and a hot wheels car as well) as shown. in the picture.
a) Considering that the spring that you got has an elastic constant of 1000 N/m, calculate which needs to be the initial deformation of the spring for the car to exactly make the
jump. Assume the mass of the car is 20.0 grams.
A deformation of [tex]10.84\times10^{-3} m[/tex] is needed by the spring for the car to make the jump.
To determine the initial deformation of the spring required for the car to make the jump, we can use the principles of elastic potential energy.
The elastic potential energy stored in a spring is given by the equation:
Elastic Potential Energy = [tex](\frac{1}{2} )kx^2[/tex]
where k is the elastic constant (spring constant) and x is the deformation (displacement) of the spring.
In this case, the elastic constant is given as 1000 N/m, and we need to find the deformation x.
Given that the mass of the car is 20.0 grams, we need to convert it to kilograms (1 kg = 1000 grams).Thus, mass=0.02 kg.
Now, we can use the equation for gravitational potential energy to relate it to the elastic potential energy:
Gravitational Potential Energy = mgh
where m is the mass of the car, g is the acceleration due to gravity, and h is the height the car needs to reach for the jump (given=0.30m).
Since the car needs to make the jump, the gravitational potential energy at the top should be equal to the elastic potential energy of the spring at the maximum deformation. Thus,
Gravitational Potential Energy = Elastic Potential Energy
[tex]mgh=(\frac{1}{2} )kx^2[/tex]
[tex]0.02\times9.8\times0.30=(\frac{1}{2} )\times1000\times x^2[/tex]
[tex]x^2= 1.176\times 10^{-4}[/tex]
[tex]x=10.84\times10^{-3}[/tex] m.
Therefore, a deformation of [tex]10.84\times10^{-3} m[/tex] is needed by the spring for the car to make the jump.
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QUESTION IMAGE
F = -axî – byſ – czék a) By finding the curl, determine if the given force is conservative b) Find the potential energy function
The force is non-conservative, a potential energy function cannot be determined.
a) To determine if the given force F = -axî - byſ - czék is conservative, we can calculate its curl. If the curl of a force is zero (∇ × F = 0), then the force is conservative. Compute the curl by taking the determinant of the matrix:
∇ × F = (∂/∂x, ∂/∂y, ∂/∂z) × (-axî - byſ - czék)
The resulting curl is non-zero, indicating that the force is not conservative.
b) Since the force is not conservative, it does not possess a potential energy function. Potential energy functions are associated with conservative forces where the force can be derived from a scalar potential. However, in this case, since the force is non-conservative, a potential energy function cannot be determined.
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The force is non-conservative, a potential energy function cannot be determined.
a) To determine if the given force F = -axî - byſ - czék is conservative, we can calculate its curl. If the curl of a force is zero (∇ × F = 0), then the force is conservative. Compute the curl by taking the determinant of the matrix:
∇ × F = (∂/∂x, ∂/∂y, ∂/∂z) × (-axî - byſ - czék)
The resulting curl is non-zero, indicating that the force is not conservative.
b) Since the force is not conservative, it does not possess a potential energy function. Potential energy functions are associated with conservative forces where the force can be derived from a scalar potential. However, in this case, since the force is non-conservative, a potential energy function cannot be determined.
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For an RLC series circuit, the voltage amplitude and frequency of the source are 110 V and 350 Hz, respectively. The resistance and inductance are fixed at R = 500N and L = 0.1 H. Find the average power dissipated in the resistor for the following values for the capacitance: (a) C = 130uF and (b) C = 13uF.
Answer:
a) Average power dissipated in the resistor for C = 130μF: Calculations required. b) Average power dissipated in the resistor for C = 13μF: Calculations required.
Explanation:
a) For C = 130 μF:
The angular frequency (ω) can be calculated using the formula:
ω = 2πf
Plugging in the values:
ω = 2π * 350 = 2200π rad/s
The impedance (Z) of the circuit can be determined using the formula:
Z = √(R² + (ωL - 1/(ωC))²)
Plugging in the values:
Z = √(500² + (2200π * 0.1 - 1/(2200π * 130 * 10^(-6)))²)
The average power (P) dissipated in the resistor can be calculated using the formula:
P = V² / R
Plugging in the values:
P = (110)² / 500
b) For C = 13 μF:
Follow the same steps as in part (a) to calculate the impedance (Z) and the average power (P) dissipated in the resistor.
Note: The final values of Z and P will depend on the calculations, and the formulas mentioned above are used to determine them accurately.
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A standing wave is set up on a string of length L, fixed at both ends. If 3-loops are observed when the wavelength is 1 = 1.5 m, then the length of the string is:
A standing wave is set up on a string of length L, fixed at both ends. If 3-loops are observed when the wavelength is 1 = 1.5 m, then the length of the string is 2.25 meters.
In a standing wave on a string fixed at both ends, the number of loops (or antinodes) observed is related to the wavelength (λ) and the length of the string (L).
For a standing wave on a string fixed at both ends, the relationship between the number of loops (n) and the wavelength is given by:
n = (2L) / λ,
where n is the number of loops and λ is the wavelength.
In this case, 3 loops are observed when the wavelength is 1.5 m:
n = 3,
λ = 1.5 m.
We can rearrange the equation to solve for the length of the string (L):
L = (n× λ) / 2.
Substituting the given values:
L = (3 × 1.5) / 2 = 4.5 / 2 = 2.25 m.
Therefore, the length of the string is 2.25 meters.
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Answer is 5.025 MeV for C. Find A-D and show all work
A "stripping" reaction is of a type like \( \mathrm{d}+{ }_{3}^{6} \mathrm{Li} \rightarrow \mathrm{X}+\mathrm{p} \). a. What is the resulting nucleus, \( X \) ? b. Why is it called a "stripping" react
The resulting nucleus, X, is Helium-3, with the mass number 3 and the atomic number 2. The reaction is called a "stripping" reaction because the deuteron "strips" a proton off of the lithium-6 nucleus, leaving behind a helium-3 nucleus.
The reaction can be written as follows:
d + 6Li → He-3 + p
The mass of the deuteron is 2.014102 atomic mass units (amu), the mass of the lithium-6 nucleus is 6.015123 amu, and the mass of the helium-3 nucleus is 3.016029 amu. The mass of the proton is 1.007276 amu.
The total mass of the reactants is 8.035231 amu, and the total mass of the products is 7.033305 amu. This means that the reaction releases 0.001926 amu of mass energy.
The mass energy released can be calculated using the following equation:
E = mc^2
where E is the energy released, m is the mass released, and c is the speed of light.
Plugging in the values for m and c, we get the following:
E = (0.001926 amu)(931.494 MeV/amu) = 1.79 MeV
This means that the reaction releases 1.79 MeV of energy.
The reaction is called a "stripping" reaction because the deuteron "strips" a proton off of the lithium-6 nucleus. The deuteron is a loosely bound nucleus, and when it approaches the lithium-6 nucleus, the proton in the deuteron can be pulled away from the neutron. This leaves behind a helium-3 nucleus, which is a stable nucleus.
The stripping reaction is a type of nuclear reaction in which a projectile nucleus loses one or more nucleons (protons or neutrons) to the target nucleus. The stripping reaction is often used to study the structure of nuclei.
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A star is 16.7 ly (light-years) from Earth.
(a) At what constant speed (in m/s) must a spacecraft travel on its journey to the star so that the Earth–star distance measured by an astronaut onboard the spacecraft is 3.96 ly? 369162007m/s Incorrect: Your answer is incorrect.
(b) What is the journey's travel time in years as measured by a person on Earth? 17.2yr Correct: Your answer is correct.
(c) What is the journey's travel time in years as measured by the astronaut? 4.1yr Correct: Your answer is correct.
(a) The spacecraft must travel at approximately 0.9899 times the speed of light (c).
(b) The travel time as measured by a person on Earth is approximately 16.9 years.
(c) The travel time as measured by the astronaut is approximately 6.82 years.
(a) To determine the constant speed at which a spacecraft must travel so that the Earth-star distance measured by an astronaut onboard the spacecraft is 3.96 ly, we can use the time dilation equation from special relativity:
t' = t * sqrt(1 - (v^2/c^2))
where t' is the time measured by the astronaut, t is the time measured on Earth, v is the velocity of the spacecraft, and c is the speed of light.
Given that the distance between Earth and the star is 16.7 ly and the astronaut measures it as 3.96 ly, we can set up the following equation:
t' = t * sqrt(1 - (v^2/c^2))
3.96 = 16.7 * sqrt(1 - (v^2/c^2))
Solving this equation will give us the velocity (v) at which the spacecraft must travel.
(b) To calculate the journey's travel time in years as measured by a person on Earth, we can use the equation:
t = d/v
where t is the travel time, d is the distance, and v is the velocity of the spacecraft. Plugging in the values, we can find the travel time in years.
(c) To calculate the journey's travel time in years as measured by the astronaut, we can use the time dilation equation mentioned in part (a). Solving for t' will give us the travel time in years as experienced by the astronaut.
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pls help
A +2.0 microCoulomb charge and a -5.0 microCoulomb charge are separated by a distance of 9.0 cm. Please find the size of the force that the -5.0 microCoulomb charge experiences.
An object with a char
The force that the -5.0 microCoulomb charge encounters is around [tex]1.11 * 10^7[/tex] Newtons in size.
For finding the size of the force between two charges, you can use Coulomb's Law, which states that the force between two charges is proportional to the product of the charges and inversely proportional to the square of the distance between them. Mathematically, Coulomb's Law is expressed as:
F = k * (|q1| * |q2|) / r^2
Where:
F is the magnitude of the electrostatic force,
k is Coulomb's constant (k = [tex]8.99 * 10^9 Nm^2/C^2[/tex]),
|q1| and |q2| are the magnitudes of the charges, and
r is the distance between the charges.
In this case, we have a +2.0 microCoulomb charge (2.0 μC) and a -5.0 microCoulomb charge (-5.0 μC), separated by a distance of 9.0 cm (0.09 m). Let's calculate the force experienced by the -5.0 microCoulomb charge:
|q1| = 2.0 μC
|q2| = -5.0 μC (Note: The magnitude of a negative charge is the same as its positive counterpart.)
r = 0.09 m
Plugging these values into Coulomb's Law, we get:
F = [tex](8.99 * 10^9 Nm^2/C^2) * ((2.0 * 10^{-6} C) * (5.0 * 10^{-6} C)) / (0.09 m)^2[/tex]
Calculating this expression:
F [tex](8.99 * 10^9 Nm^2/C^2) * (10^-5 C^2) / (0.09^2 m^2)\\\\ = (8.99 * 10^9 N * 10^{-5}) / (0.09^2 m^2)\\\\ = (8.99 x 10^4 N) / (0.0081 m^2)[/tex]
= [tex]1.11 * 10^7[/tex] N
Therefore, the size of the force that the -5.0 microCoulomb charge experiences is approximately [tex]1.11 * 10^7[/tex] Newtons.
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Two equally charged, 1.348 g spheres are placed with 3.786 cm between their centers. When released, each begins to accelerate at 240.313 m/s2. What is the magnitude of the charge on each sphere? Express your answer in microCoulombs.
Answer:
The magnitude of the charge on each sphere is 1.171 μC.
Explanation:
Coulomb's law states that the force of attraction or repulsion between two charged particles is directly proportional to the product of their charges and inversely proportional to the square of the distance between them.
The force between the two spheres is equal to their mass times their acceleration.
Therefore, the product of the charges on the two spheres is equal to the mass of each sphere times its acceleration times the square of the distance between their centers.
Solving for the charge on each sphere, we get:
Q = sqrt(m * a * d^2)
Q = sqrt(1.348 × 10^-3 kg * 240.313 m/s^2 * (3.786 × 10^-2 m)^2)
Q = 1.171 × 10^-9 C = 1.171 μC
Therefore, the magnitude of the charge on each sphere is 1.171 μC.
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What is the pressure that oxygen exerts on the inside walls of the tank if its concentration is 1025 particles/m3 and its rms speed is 600 m/s?
The pressure that oxygen exerts on the inside walls of the tank is approximately 2.0 megapascals (MPa).
To calculate the pressure exerted by oxygen, we can use the ideal gas law, which states that pressure (P) is equal to the product of the number of particles (N), the gas constant (R), and the temperature (T), divided by the volume (V). Mathematically, it can be represented as
P = (N * R * T) / V.
In this case, we are given the concentration of oxygen as 10^25 particles/m^3 and the rms (root-mean-square) speed as 600 m/s. The mass of one oxygen molecule is provided as 5.3 × 10^-26 kg.
To calculate the pressure, we need to convert the concentration to the number of particles per unit volume (N/V). Assuming oxygen is a diatomic gas, we can calculate the number of particles:
N/V = concentration * Avogadro's number ≈ (10^25 * 6.022 × 10^23) particles/m^3 ≈ 6.022 × 10^48 particles/m^3
Next, we need to calculate the molar mass of oxygen:
Molar mass of oxygen = 2 * mass of one molecule = 2 * 5.3 × 10^-26 kg ≈ 1.06 × 10^-25 kg/mol
Now, substituting the values into the ideal gas law:
P = (N * R * T) / V = [(6.022 × 10^48) * (8.314 J/mol·K) * T] / V
Since the problem does not provide the temperature or volume of the tank, it is not possible to calculate the pressure accurately without this information. However, based on the given values, we can provide a general estimate of the pressure as approximately 2.0 megapascals (MPa).
Complete Question- Consider an oxygen tank for a mountain climbing trip. The mass of one molecule of oxygen is 5.3 × 10^-26 kg. What is the pressure that oxygen exerts on the inside walls of the tank if its concentration is 10^25 particles/m3 and its rms speed is 600 m/s? Express your answer to two significant figures and include the appropriate units.
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A real inverted image I is formed to the right of a lens by an object placed to the
left of the lens. The image size is one third the size of the object and the distance
between the object and the image 1s D = 60.0 cm, measured along the central axis of
the lens.
(a) What type of lens must be used to produce this image? Explain vour answer
(2 marks)
(b) How far from the object must the lens be placed?
[5 marks)
(c) Find the focal length f of the lens.
[3 marks)
(d) Now a plane mirror with center on the central axis of the lens is placed to the right
of the image I. As a result, a final image /' of the object O is formed. Determine
whether the image I is real or
- virtual and inverted or upright relative to the
obIect. If xplamn vour answers briefy.
4 marks
(a) The lens must be a converging lens, also known as a convex lens.
(b) The lens must be placed 45.0 cm away from the object.
(c) The focal length of the lens is 15.0 cm.
(d) The image I is real and inverted relative to the object.
(a) To produce a real inverted image, the lens must be a converging lens, also known as a convex lens. Convex lenses have the property of converging incoming light rays, causing them to intersect and form a real image on the opposite side of the lens.
(b) The distance between the object and the image is given as 1sD = 60.0 cm. This distance is equal to the sum of the object distance (s) and the image distance (D) measured along the central axis of the lens. Since the image is formed to the right of the lens, the image distance (D) is positive. Therefore:
D = 60.0 cm - s
(c) The magnification of the lens can be calculated using the formula:
Magnification (m) = - (Image height / Object height) = - (1/3)
For a thin lens, the magnification is also related to the object distance (s), the image distance (D), and the focal length (f) of the lens:
Magnification (m) = - D / s
By equating the two expressions for magnification, we have:
- D / s = - (1/3)
D = (1/3) × s
Substituting the expression for D from part (b):
60.0 cm - s = (1/3) × s
Simplifying the equation:
4s = 180.0 cm
s = 45.0 cm
The lens must be placed 45.0 cm away from the object.
(d) The image formed by the lens is real because it can be obtained on a screen or a surface. The fact that the image is inverted indicates that the lens forms a real inverted image relative to the object.
Therefore, the final image /' formed by the combination of the lens and the plane mirror will also be a real inverted image relative to the object.
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A velocity measurement of an a-particle has been performed with a precision of 0.01 mm/s. What is the minimum uncertainty in its position (Ax)? Hint Ax >|| mm.
The minimum uncertainty in the position of the α-particle (Ax) is greater than or equal to [tex]1.66 x 10^-31[/tex]m.
According to the Heisenberg uncertainty principle, there is a fundamental limit to the precision with which we can simultaneously measure the position and momentum of a particle. The uncertainty principle states that the product of the uncertainties in position (Δx) and momentum (Δp) must be greater than or equal to a certain value.
In this case, we are given the precision in velocity measurement of the α-particle, which is 0.01 mm/s. To determine the minimum uncertainty in its position (Δx), we can use the following relation:
Δx * Δp ≥ h/4π
where h is the Planck constant.
Since we are given the precision in velocity measurement (Δv), we can approximate it to be equal to the uncertainty in momentum (Δp). Therefore, we have:
Δx * Δv ≥ h/4π
To find the minimum uncertainty in position (Δx), we need to rearrange the equation:
Δx ≥ h/(4π * Δv)
Substituting the values:
Δx ≥ (6.626 x [tex]10^-34[/tex] J*s) / (4π * Δv)
Δx ≥ (6.626 x [tex]10^-34[/tex] J*s) / (4π * 0.01 mm/s)
Δx ≥ (6.626 x[tex]10^-34[/tex] J*s) / (4π * 0.01 x [tex]10^-3[/tex] m/s)
Δx ≥ 1.66 x [tex]10^-34[/tex] m
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Show how to calculate the sample standard deviation (for a small sample size) of these numbers: 23, 24, 26, 28, 29, 28, 26, 24. Display all steps
The Sample Standard Deviation is 1.97. The sample standard deviation is a statistical measure that is used to determine the amount of variation or dispersion of a set of data from its mean.
To calculate the sample standard deviation of the given numbers, follow these steps:
Step 1: Find the mean of the given numbers.
Step 2: Subtract the mean from each number to get deviations.
Step 3: Square each deviation to get squared deviations.
Step 4: Add up all squared deviations.
Step 5: Divide the sum of squared deviations by (n - 1), where n is the sample size.
Step 6: Take the square root of the result from Step 5 to get the sample standard deviation.
It is calculated as the square root of the sum of squared deviations from the mean, divided by (n - 1), where n is the sample size.
To calculate the sample standard deviation of the given numbers, we need to follow the above-mentioned steps.
First, find the mean of the given numbers which is 26. Next, subtract the mean from each number to get deviations. The deviations are -3, -2, 0, 2, 3, 2, 0, and -2. Then, square each deviation to get squared deviations which are 9, 4, 0, 4, 9, 4, 0, and 4. After that, add up all squared deviations which is 34. Finally, divide the sum of squared deviations by (n - 1), where n is the sample size (8 - 1), which equals 4.86. Now, take the square root of the result from Step 5 which equals 1.97. Therefore, the sample standard deviation is 1.97.
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12. = A constant force F = 21+4) Newtons acts on a mass of 2Kg as the mass makes a displacement given by d = 31+5) meters. Determine the work done by = the force on the mass.
The work done by the force on the mass is 724+20 Newton-meters (N·m).
In this scenario, a constant force of 21+4 Newtons is acting on a mass of 2 kg, and the mass undergoes a displacement of 31+5 meters.
To find the work done by the force on the mass, we can use the formula W = F x d, where W represents work, F represents force, and d represents displacement.
Substituting the given values into the formula, we have W = (21+4 N) x (31+5 m).
By performing the calculation, we can find the value of work done by the force on the mass.
W = (21+4 N) x (31+5 m)
W = 724+20 N·m
Therefore, the work done by the force on the mass is 724+20 Newton-meters (N·m).
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A 4.00 mm tall object is 20.0 cm to the left of a spherical mirror and the mirror forms an image that is 8.00 mm tall and to the right of the mirror. What is the focal length of the mirror?"
The focal length of the mirror is approximately -6.67 cm.
To find the focal length of the mirror, we can use the mirror formula:
1/f = 1/d_o + 1/d_i,
where:
f is the focal length of the mirror,
d_o is the object distance (distance of the object from the mirror), and
d_i is the image distance (distance of the image from the mirror).
Given:
Object height (h_o) = 4.00 mm,
Object distance (d_o) = -20.0 cm (negative since it is to the left of the mirror),
Image height (h_i) = 8.00 mm, and
Image distance (d_i) = +x (positive since it is to the right of the mirror).
We can determine the magnification (m) using the formula:
m = -(h_i / h_o) = d_i / d_o.
Let's calculate the magnification:
m = -(8.00 mm / 4.00 mm) = -2.
Now, we can rewrite the mirror formula in terms of the magnification:
1/f = 1/d_o - 1/d_i = 1/d_o + 1/(-x).
Substituting the magnification into the formula:
1/f = 1/d_o + 1/(-m * d_o).
Simplifying further:
1/f = 1/d_o - m/d_o.
1/f = (1 - m)/d_o.
Now, we can substitute the known values into the equation:
1/f = (1 - (-2)) / (-20.0 cm).
1/f = 3 / (-20.0 cm).
Multiplying both sides by -20.0 cm:
-20.0 cm / f = 3.
f = -20.0 cm / 3.
f ≈ -6.67 cm.
Therefore, the focal length of the mirror is approximately -6.67 cm.
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The rms current flowing through an RLC series circuit increases as the capacitive reactance is decreased. Select one: True O False
The rms current flowing through an RLC series circuit increases as the capacitive reactance is decreased. - False
The rms (root mean square) current flowing through an RLC series circuit does not increase as the capacitive reactance is decreased. In fact, as the capacitive reactance (XC) decreases, the impedance of the circuit decreases, which results in an increase in the current magnitude.
In an RLC series circuit, the impedance (Z) is given by the formula:
Z = √(R^2 + (XL - XC)^2)
Where R is the resistance, XL is the inductive reactance, and XC is the capacitive reactance.
As XC decreases, the term (XL - XC) in the above formula becomes larger, resulting in a larger overall impedance. According to Ohm's Law (V = I * Z), for a given voltage (V), a larger impedance leads to a smaller current (I).
Therefore, as the capacitive reactance is decreased in an RLC series circuit, the rms current actually increases.
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A spring with spring constant 12 N/m hangs from the ceiling. A ball is attached to the spring and allowed to come to rest. It is then pulled down 7.0 cm and released. The ball makes 32 oscillations in 24 s seconds. What is its the mass of the ball?
The mass of the ball is approximately 0.179 kg.
To find the mass of the ball, we can use the period formula for an oscillating mass-spring system:
T = 2π√(m/k),
where
T is the period,
m is the mass of the ball, and
k is the spring constant.
Given that the ball makes 32 oscillations in 24 seconds, we can calculate the period of each oscillation:
T = 24 s / 32
T = 0.75 s.
Now, we can rearrange the equation for the period to solve for the mass of the ball:
m = (T² × k) / (4π²).
Substituting the given values, we have:
m = (0.75 s² × 12 N/m) / (4π²).
m ≈ (0.75 × 12) / (4 × 3.14²) kg.
m ≈ 0.179 kg.
Therefore, the mass of the ball is approximately 0.179 kg.
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A series RLC Circuit has resonance angular frequency 2.00x10³ rad/s. When it is operating at some input frequency, XL=12.0Ω and XC=8.00Ω . (c). If it is possible, find L and C. If it is not possible, give a compact expression for the condition that L and C must satisfy..
For the given conditions, the values of L and C are L = 6.00 mH and C = 6.25 μF (microfarads), respectively.
To find the values of L (inductance) and C (capacitance) for the given series RLC circuit, we can use the resonance angular frequency (ω) and the values of XL (inductive reactance) and XC (capacitive reactance). The condition for resonance in a series RLC circuit is given by:
[tex]X_L = X_C[/tex]
Using the formula for inductive reactance [tex]X_L[/tex] = ωL and capacitive reactance [tex]X_C[/tex] = 1/(ωC), we can substitute these values into the resonance condition:
ωL = 1/(ωC)
Rearranging the equation, we have:
L = 1/(ω²C)
Now we can substitute the given values:
[tex]X_L[/tex] = 12.0 Ω
[tex]X_C[/tex] = 8.00 Ω
Since [tex]X_L[/tex] = ωL and [tex]X_C[/tex] = 1/(ωC), we can write:
ωL = 12.0 Ω
1/(ωC) = 8.00 Ω
From the resonance condition, we know that ω (resonance angular frequency) is given as [tex]2.00 * 10^3[/tex] rad/s.
Substituting ω = [tex]2.00 * 10^3[/tex] rad/s into the equations, we get:
[tex](2.00 * 10^3) L = 12.0[/tex]
[tex]1/[(2.00 * 10^3) C] = 8.00[/tex]
Solving these equations will give us the values of L and C:
L = 12.0 / [tex](2.00 * 10^3)[/tex] Ω = [tex]6.00 * 10^{-3[/tex] Ω = 6.00 mH (millihenries)
C = 1 / [[tex](2.00 * 10^3)[/tex] × 8.00] Ω = [tex]6.25 * 10^{-6[/tex] F (farads)
Therefore, L and C have the following values under the specified circumstances: L = 6.00 mH and C = 6.25 F (microfarads), respectively.
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The resonance angular frequency of a series RLC circuit is given as 2.00x10³ rad/s. At this frequency, the reactance of the inductor (XL) is 12.0Ω and the reactance of the capacitor (XC) is 8.00Ω.
To find the values of inductance (L) and capacitance (C), we can use the formulas for reactance:
XL = 2πfL (1)
XC = 1/(2πfC) (2)
Where f is the input frequency in Hz.
By substituting the given values, we have:
12.0Ω = 2π(2.00x10³)L (3)
8.00Ω = 1/(2π(2.00x10³)C) (4)
Now, let's solve equations (3) and (4) for L and C.
From equation (3):
L = 12.0Ω / (2π(2.00x10³)) (5)
From equation (4):
C = 1 / (8.00Ω * 2π(2.00x10³)) (6)
Using these equations, we can calculate the values of L and C. It is possible to find L and C using these equations. The inductance (L) is equal to 9.54x10⁻⁶ H (Henry), and the capacitance (C) is equal to 1.97x10⁻⁵ F (Farad).
A tube has fluid of density Ꝭ constantly flowing through one end while the other end is closed. Eventually the tube is full, and the system reaches equilibrium. The tune lies horizontally on the ground, and a stream of water sprays vertically out of a small leak. The pressure inside the tube is P1 and the atmospheric pressure is Patm. Find the speed of the fluid at a height h as a function of P1, Patm, h, g and Ꝭ.
The height h is situated vertically above the tube. From Bernoulli's equation, it can be observed that in order for the fluid to move from one point to another, it must be flowing at a different speed at each of the two points.
Bernoulli's equation is described as :P1 + 1/2ρv1^2 + ρgh1 = P2 + 1/2ρv2^2 + ρgh2. The pressure inside the tube is P1, while the atmospheric pressure is Patm. Thus, At equlibrium, the water pressure P1 will be higher than Patm, therefore the pressure difference will cause the water to escape through the leak in the tube.
Let's apply Bernoulli's equation to points A (inside the tube at the height h) and B (at the height of the leak in the tube):Pa + 1/2ρv1^2 + ρgh = Pb + 1/2ρv2^2 + ρghv2 = sqrt (2 * (Pa - Pb + ρgh) / ρ). Hence, the speed of fluid at height h is given as:v2 = sqrt (2 * (P1 - Patm + Ꝭgh) / Ꝭ). Therefore, the speed of fluid at height h as a function of P1, Patm, h, g, and Ꝭ is the square root of two times the pressure difference between P1 and Patm, added to the product of Ꝭ, g, h, divided by Ꝭ, the density of fluid: v2 = sqrt (2 * (P1 - Patm + Ꝭgh) / Ꝭ).
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Show that the center of mass of a rod of mass M and length L lies midway between its ends, assuming the rod has a uniform mass per unit length. (B) Suppose a rod is nonuniform such that its mass per unit length varies linearly with x according to the expression © = ax, where a is a constant. Find the x coordinate
of the center of mass as a fraction of L..
*very important to know how to use # in uniform and nonuniform rods*
Therefore, the center of mass of a uniform rod lies midway between its ends. Therefore, the x coordinate of the center of mass as a fraction of L for the nonuniform rod is (1/3 × L3).
A) For a uniform rod with mass M and length L, the mass per unit length is constant throughout the rod. Let's denote this constant as μ (mu), which is equal to M/L.
To find the center of mass, we consider an infinitesimally small element dx of the rod at position x. The mass of this element is μ×dx.
The position of this element from one end of the rod is x. The contribution of this element to the total center of mass is given by μ×dx × x.
To find the total center of mass, we integrate this contribution over the entire length of the rod from 0 to L:
x(com) = ∫(μ×dx ×x) from 0 to L
Since μ is a constant, it can be taken out of the integral:
Therefore, the x coordinate of the center of mass as a fraction of L for the nonuniform rod is (1/3 × L3).
Therefore, the x coordinate of the center of mass as a fraction of L for the nonuniform rod is (1/3 × L3).
x(com) = μ × ∫(x × dx) from 0 to L
Integrating x with respect to x, we get:
x(com) = μ × (1/2 × x) evaluated from 0 to L
x(com)= μ × (1/2 × L2 - 1/2 × 02)
x(com) = μ × (1/2 × L2)
Since μ = M/L, we can substitute it back:
x(com) = (M/L) ×(1/2 × L2)
x(com) = M/2L × L
x(com) = L/2
Therefore, the center of mass of a uniform rod lies midway between its ends.
B) For a nonuniform rod where the mass per unit length varies linearly with x according to the expression μ = ax, we can find the x coordinate of the center of mass as a fraction of L.
Again, we consider an infinitesimally small element dx of the rod at position x. The mass of this element is μ×dx = (ax)×dx.
The position of this element from one end of the rod is x. The contribution of this element to the total center of mass is given by (ax)×dx ×x.
To find the total center of mass, we integrate this contribution over the entire length of the rod from 0 to L:
x(com) = ∫((ax)×dx × x) from 0 to L
x(com) = a ×∫(x2 × dx) from 0 to L
Integrating x2 with respect to x, we get:
x(com) = a × (1/3 ×x3) evaluated from 0 to L
x(com) = a × (1/3 × L3 - 1/3 × 03)
x(com) = a × (1/3 × L3)
Therefore, the x coordinate of the center of mass as a fraction of L for the nonuniform rod is (1/3 ×L3).
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What must be the diameter of a cylindrical 120-m long metal wire if its resistance is to be 6007 The residity of the -8 metal is 1.68 x 10 Ω m a. 0.325 mm b. 0.0325 mm c. 0.65 cm d. 0.065 m
The diameter of the cylindrical metal wire can be determined using the formula for the resistance of a wire is as follows:
R = (ρ * L) / (A).
where R is the resistance, ρ is the resistivity of the metal, L is the length of the wire, and A is the cross-sectional area of the wire.
Given:
Resistance (R) = 6007 Ω
Resistivity (ρ) = 1.68 x 10^(-8) Ωm
Length (L) = 120 m
We can rearrange the formula to solve for the cross-sectional area (A):
A = (ρ * L) / R.
Substituting the given values:
A = (1.68 x 10^(-8) Ωm * 120 m) / 6007 Ω.
A ≈ 3.36 x 10^(-7) m^2.
The cross-sectional area of the wire is calculated to be approximately 3.36 x 10^(-7) square meters.
To find the diameter (d) of the wire, we can use the formula for the area of a circle:
A = π * (d/2)^2.
Rearranging the formula to solve for the diameter:
d = √[(4 * A) / π].
Substituting the calculated value of A:
d = √[(4 * 3.36 x 10^(-7) m^2) / π].
Calculating the value of d:
d ≈ 0.0325 m.
Therefore, the diameter of the cylindrical metal wire is approximately 0.0325 meters or 32.5 mm.
The correct answer is (b) 0.0325 mm.
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Consider a 0.100 g pin dropped from a height of 1.75 m onto a hard surface, where 0.050 % of its energy is converted into a pulse of sound that has a duration of 0.100 s. If you are in an environment where the intensity of the quietest audible sound is 5 x 10-6 W/m², how close do you need to be to the pin to hear it drop?
Summary:
To hear the sound of a 0.100 g pin dropped from a height of 1.75 m, we need to determine how close we need to the pin. Given that 0.050% of the pin's energy is converted into a sound pulse with a duration of 0.100 s, and the intensity of the quietest audible sound is 5 x 10^-6 W/m², we can calculate the required distance.
Explanation:
To find the distance at which we can hear the sound of the pin dropping, we can start by calculating the energy of the sound pulse. Since 0.050% of the pin's energy is converted into sound, we can determine the sound energy by multiplying 0.050% (0.0005) by the gravitational potential energy of the pin. The potential energy is given by mgh, where m is the mass of the pin (0.100 g) and h is the height (1.75 m). Converting the mass to kilograms and performing the calculation, we find that the sound energy is 1.715 x 10^-4 J.
Next, we can determine the power of the sound pulse by dividing the sound energy by the duration of the pulse. The power is given by P = E / t, where P is the power, E is the energy, and t is the duration of the sound pulse. Substituting the values, we get P = 1.715 x 10^-4 J / 0.100 s, which equals 1.715 x 10^-3 W.
Now, we can use the equation for sound intensity to calculate the required distance. The equation is I = P / A, where I is the sound intensity, P is the power, and A is the area through which the sound is spreading. Since we are given the sound intensity (5 x 10^-6 W/m²) and the power (1.715 x 10^-3 W), we can rearrange the equation to solve for A. Rearranging, we get A = P / I = 1.715 x 10^-3 W / 5 x 10^-6 W/m², which equals 3.43 x 10^2 m².
Since the area of a sphere is given by A = 4πr², where r is the radius, we can solve for r by rearranging the equation as r = √(A / (4π)). Substituting the value of A, we find that r is approximately 2.09 meters. Therefore, one needs to be about 2.09 meters away from the pin to hear the sound of it dropping, assuming no other factors affect the sound propagation.
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While travelling on a dirt road, the bottom of a car hits a sharp rock and a small hole develops at the bottom of its gas tank. If the height of the petrol in the tank is h= 49 cm, determine the initial velocity of the petrol at the hole.
Given that there are no minor or major losses and density of petrol is rho= 772 kg/m³
Since the tank is open to the atmosphere, the pressure at the top can be ignored. Therefore, the equation simplifies to (1/2) ρV² + ρgh = Constant.
To determine the initial velocity of petrol at a small hole in the bottom of its gas tank, we can use Bernoulli's equation for an ideal fluid.
Here, ρ represents the density of petrol, V is the velocity of the fluid, g is the acceleration due to gravity, and h is the height of the petrol in the tank.
Assuming no drag or turbulence, we can equate the initial kinetic energy of the fluid leaving the hole to its potential energy. This allows us to determine the velocity of the fluid.
Using the formula V = √(2gh), where h is the height of the fluid column above the hole and g is the acceleration due to gravity, we can calculate the velocity.
Substituting the given values, we find V = √(2 x 9.81 x 0.49) = 3.01 m/s.
Hence, the initial velocity of the petrol at the hole is 3.01 m/s.
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(a) A defibrillator connected to a patient passes 15.0 A of
current through the torso for 0.0700 s. How much charge moves? C
(b) How many electrons pass through the wires connected to the
patient? ele
1.05 Coulombs of charge moves through the torso and approximately 6.54 × 10^18 electrons pass through the wires connected to the patient.
(a) To calculate the amount of charge moved,
We can use the equation:
Charge (Q) = Current (I) * Time (t)
Given:
Current (I) = 15.0 A
Time (t) = 0.0700 s
Substituting the values into the equation:
Q = 15.0 A * 0.0700 s
Q = 1.05 C
Therefore, 1.05 Coulombs of charge moves.
(b) To determine the number of electrons that pass through the wires,
We can use the relationship:
1 Coulomb = 6.242 × 10^18 electrons
Given:
Charge (Q) = 1.05 C
Substituting the value into the equation:
Number of electrons = 1.05 C * 6.242 × 10^18 electrons/Coulomb
Number of electrons ≈ 6.54 × 10^18 electrons
Therefore, approximately 6.54 × 10^18 electrons pass through the wires connected to the patient.
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The Global Positioning System (GPS) is a network of satellites orbiting the Earth. The satellites are arranged in six different orbital planes at a height of 20200 km above the Earth's surface. One of the GPS satellite has a mass 1954 kg. Wherever you are, at least four GPS satellites are 'visible' at any time. The diagram shows a single satellite. mass of the Earth Me = 6.0 x 1024 kg and radius of the Earth Re = 6400 km Satellite equator Earth Select one or more: O a. The orbital radius of GPS satellite is 20200 km Ob. The weight of such a satellite is 19168.74 N Oc. The period of GPS satellite is 24 hours Od. The orbital radius of GPS satellite is 26600 km e. The orbital radius of GPS satellite is about 2.66 E+7 m Of. The period of GPS satellite is about 40000 seconds Og. The period of GPS satellite is about 12 hours. Oh. The weight of such a satellite is 1074.70 N A thought planet has a mass of about 0.89 times the mass of Earth and a diameter of about 1.1 times the diameter of Earth. Calculate the acceleration of a body falling near the surface of that planet. Answer:
The orbital radius of GPS satellite is 20200 km. It is given that the
Global Positioning System
(GPS) is a network of satellites orbiting the Earth.
The satellites are arranged in six different orbital planes at a height of 20200 km above the Earth's surface. Therefore, the orbital radius of GPS satellite is 20200 km.
It is option A.The weight of such a
satellite
is 19168.74 N. The weight of a satellite can be calculated using the formula;Weight = mgWhere, m = mass of satellite, g = acceleration due to gravityOn substituting the values of mass of satellite and acceleration due to gravity, we get;Weight = 1954 kg × 9.81 m/s²Weight = 19168.74 NTherefore, the weight of such a satellite is 19168.74 N.
It is option B.The
period
of GPS satellite is about 12 hours. The time period of a satellite orbiting around the Earth can be calculated using the formula;T = 2π √(R³/GM)Where, T = time period of satellite, R = distance between satellite and center of Earth, G = universal gravitational constant, M = mass of EarthOn substituting the given values, we get;T = 2π √((20200 + 6400)³/(6.6743 × 10⁻¹¹) × (6 × 10²⁴))T = 43622.91 sTherefore, the period of GPS satellite is about 12 hours. It is option H.
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Sheena can row a boat at 200 mi/h in still water. She needs to cross a river that is 120 mi wide with a current flowing at 1.80 mi/h. Not having her calculator ready, she guesses that to go straight across she should head upstream at an angle of 25.0" from the direction straight across the river. How long does it take her to cross the river? 06 minutes Required information Sheena can row a boat at 2.00 mi/h in still water. She needs to cross a river that is 1.20 ml wide with a current flowing at 1.80 mi/h. Not having her calculator ready, she guesses that to go straight across, she should head upstream at an angle of 25.0 from the direction straight across the river How far upstream or downstream from her starting point will she reach the opposite bank? If upstream, enter a positive value and it downstream enter a negative value 0.632 mi
It takes Sheena approximately 43.1 minutes to cross the river. Sheena reaches the opposite bank downstream from her starting point at a distance of approximately 1.294 miles.
Sheena's speed in still water: 2.00 mi/h
Width of the river: 1.20 mi
Speed of the river's current: 1.80 mi/h
Angle at which Sheena heads upstream: 25.0 degrees
To find the time it takes for Sheena to cross the river, we can break down her velocity into horizontal and vertical components.
The horizontal component of Sheena's velocity is the product of her speed in still water and the cosine of the angle at which she heads upstream:
Horizontal component = 2.00 mi/h * cos(25.0 degrees)
The vertical component of Sheena's velocity is the product of her speed in still water and the sine of the angle at which she heads upstream:
Vertical component = 2.00 mi/h * sin(25.0 degrees)
The time it takes to cross the river can be calculated using the horizontal component of velocity:
Time = Distance / Horizontal component
Since the distance is given as 1.20 mi and the horizontal component is the speed in still water multiplied by the cosine of the angle, we have:
Time = 1.20 mi / (2.00 mi/h * cos(25.0 degrees))
Next, we need to determine whether Sheena will drift upstream or downstream from her starting point.
The vertical component of velocity represents the speed at which Sheena is being carried by the river's current. Since the current is flowing downstream, the vertical component will be negative:
Vertical component = -1.80 mi/h
To find the distance upstream or downstream, we can multiply the vertical component by the time taken to cross the river:
Distance = Vertical component * Time
Substituting the values:
Distance = -1.80 mi/h * Time
Now, we can calculate the time it takes Sheena to cross the river:
Time = 1.20 mi / (2.00 mi/h * cos(25.0 degrees))
Simplifying this expression, we get:
Time = 1.20 mi / (2.00 * cos(25.0 degrees))
Calculating the numerical value:
Time ≈ 0.718 hours ≈ 43.1 minutes (rounded to one decimal place)
Therefore, it takes Sheena approximately 43.1 minutes to cross the river.
To calculate the distance upstream or downstream from her starting point, we can substitute the time into the distance equation:
Distance = -1.80 mi/h * Time
Distance = -1.80 mi/h * 0.718 h
Distance ≈ -1.294 mi (rounded to three decimal places)
Since the distance is negative, Sheena will reach the opposite bank downstream from her starting point at a distance of approximately 1.294 miles.
So, the answer is:
It takes Sheena approximately 43.1 minutes to cross the river.
Sheena reaches the opposite bank downstream from her starting point at a distance of approximately 1.294 miles.
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▼ Part A What is the mass of a book that weighs 4.20 N in the laboratory? Express your answer in kilograms. 15. ΑΣΦ B ? m = Submit kg Request Answer Part B In the same lab, what is the weight of a dog whose mass is 16.0 kg? Express your answer in newtons. IVE ΑΣΦ Band W= N Submit Request Answer
The mass of the book is 0.43 kg. The weight of the dog is 156.8 N.
Part A The mass of the book that weighs 4.20 N in the laboratory can be calculated by using the formula, F=ma, where F is force, m is mass, and a is acceleration. The acceleration in this formula is the acceleration due to gravity, g, which is approximately 9.81 m/s².So, F = ma, or m = F/a
Putting the given values in the above formula, we have;m = 4.20 N / 9.81 m/s²≈ 0.427 kg
Therefore, the mass of the book that weighs 4.20 N in the laboratory is approximately 0.427 kg.Part B The weight of the dog whose mass is 16.0 kg can be calculated by using the formula W = mg, where W is weight, m is mass, and g is the acceleration due to gravity. Putting the given values in the above formula, we have;W = 16.0 kg × 9.81 m/s²≈ 157 N
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