Answer:
The wave phenomenon that you are describing is known as the Doppler effect. The Doppler effect occurs when a wave, such as a sound wave, passes by an observer and the pitch of the wave seems to change. This is because the frequency of the wave changes as it moves closer to or farther away from the observer. The pitch of a sound wave is directly related to its frequency, so when the frequency of the wave changes, the pitch will also change. This effect is commonly observed with sound waves, but it can also occur with other types of waves, such as light waves.
if you measured the bouyancy force on an object submerged in molasses instead of water how would the bouyancy force differ
The buoyancy force when measured on an object submerged in molasses instead of water the buoyancy force does not differ.
Buoyancy is the force that is applied by any fluid on the body which is submerged in it.
The buoyancy force on any body is given by the relation,
B = Vpg
Where,
V is the volume of the fluid displaced,
p is the density of the fluid,
g is the acceleration due to gravity.
If we assume that the object is floating on the surface of the fluid then the buoyancy force will be equal to the weight of the body.
So, if the buoyancy force is measured on molasses instead of water the boils force will not differ in magnitude because it will be equal to the weight of the body in both the cases.
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as light reflected off an object reaches your eye, it passes through several structures before it reaches the retina. describe the functions of the following structures:.
Eye's cornea, are in front, bends and concentrates light rays. The pupil serves as the eyeball's entry for light, while the lens, a transparent behind pupil that may change form, aids in focusing images on the retina.
What else do you call reflecting?The verbs cogitate, deliberate, reason, conjecture, and think are some frequent synonyms for reflect. All of these phrases refer to "using one's faculties of conceptualization, judgment, or inference," but reflect denotes thoughtful reflection on a memory.
What comes when you suspect about this at all?You can enjoy each small victory if you take the time to think back on life you did well and your triumphs. You are able to see how much of your selflessness and life accomplishments you have accomplished. Without introspection, it's all too simple to lose sight of these things and concentrate only on our gaps.
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Which of the following describes the independent variable?
It is called the respondent variable.
It is plotted on the vertical axis when graphed.
It refers to a quantity changed by the experimenter.
It is something that remains controlled during trials.
The one that describes the independent variable is it is something that remains controlled during trials. The correct option is D.
What is an independent variable?A variable that is independent is precisely what it sounds like. It is a stand-alone variable that is unaffected by the other variables you are attempting to assess.
On the abscissa, the independent variable is plotted (also called the x-axis or horizontal axis), It is not the respondent variable because it does not respond to changes.
Therefore, the correct option is D, It is something that remains controlled during trials.
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The spring in the figure (Figure 1)/ (a) is compressed by length delta x . It launches the block across a frictionless surface with speed v0. The two springs in the figure (Figure 2) (b) are identical to the spring of the figure (a). They are compressed by the same length delta x and used to launch the same block. What is the block's speed now?
The speed from two springs is √2 times the speed with one spring.
The rate of change in position of an object in any course. Speed is measured because the ratio of distance to the time wherein the distance became included. Speed is a scalar amount because it has handiest route and no significance.
A quick-moving object has a high speed and covers a notably big distance in a given amount of time, whilst a sluggish-shifting item covers a relatively small amount of distance in the same amount of time.
The primary unit or the S.I. unit of speed is m/s or ms?¹.
Calculation :
The energy stored in the spring is 0.5*k*∆x²; this must equal the kinetic energy of the released block. 0.5*m*v0²:
0.5*m*v0² = 0.5*k*∆x²
v0 = ∆x*√[k/m]
Two springs will store twice the energy, so the stored energy in the two springs is k*∆x²
0.5*k*∆x² = k*∆x²
v0 = ∆x*√[2*k/m]
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find ds in terms of dv and approximate the change in the surface when the volume change from 1,000 m3 to 999 m3 .
Terms of dv and approximate the change in the surface when the volume change from 1,000 m3 to 999 m3 is 2.9 M2.
What is volume?Volume is a measure of the amount of three-dimensional space occupied by a solid, liquid, gas, or plasma. It is measured in cubic meters, liters, or milliliters. Volume is an important measurement when dealing with liquids and other substances since it determines the amount of material that can fit in a given container. Volume also has an effect on pressure and temperature, as the pressure and temperature of a substance increase when its volume decreases.
The change in the surface of a given volume can be found by taking the derivative of the volume in terms of the surface. The derivative of V (volume) with respect to S (surface) is S = 3√V. Therefore, the change in surface when the volume changes from 1000 m3 to 999 m3 is approximately 3√999 - 3√1000 = 2.9 m2.
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For finding the distances to globular clusters, Harlow Shapley used
A. eclipsing binaries
B. planetary nebulae
C. Type I supernovae
D. RR Lyrae variables
E. Population I classical Cepheidsd
Harlow Shapley used RR Lyrae variables.
RR Lyrae variables are periodic variable stars, normally found in globular clusters. they're used as preferred candles to degree galactic distances, supporting the cosmic distance ladder. This elegance is named after the prototype and brightest example, RR Lyrae.
RR Lyrae is a variable, horizontal branch star with periods starting from a few hours to 2 days, and optical brightnesses that commonly vary from zero. They lie within the instability strip of the Hertzsprung-Russell diagram and suffer instabilities that purpose their length to periodically trade.
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A ruby laser emits light of wavelength 694.3 nm. If this light is due to transitions from the n = 2 state to the n = 1 state of an electron in a box, find the width of the box.
If the wavelength of the ruby laser light is 694.3 nm then the width of the box is 0.795 nm .
In the question ,
it is given that ,
the wavelength (λ) is = 694.3 × 10⁻⁹ m ,
transition from n = 2 to n = 1 .
then the energy Eₙ = (h²n²/8mL²)
where "L" is the width of box ,
The transition energy is related to emitted (light) photon wavelength by
ΔE = (h²n²/8mc²L²) × (2² - 1²) = hc/λ ....equation(1)
Rewriting for the width "L" ,
we get ,
L = √[(3hcλ)/8mc²]
Substituting the values in equation(1) ,
we get ,
L = √[(3×1.24×10³×694.3)/8×511×10³]
Simplifying further ,
we get ,
L = 0.795 × 10⁻⁹ m
= 0.795 nm .
Therefore , the width of the box is 0.795 nm .
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Which of the following atmospheric characterization techniques allow for 2D mapping of an exoplanet's atmospheric temperature and circulation patterns?
Measuring phase curves
Direct imaging
Measuring transits at different wavelengths
Measuring Doppler (velocity) curves
Astronomers can learn important details about the atmosphere, surface temperature, and size of transiting planets.
A transiting planet that is the size of a brown dwarf often only dims the brightness of Sun-like stars by a few percent or less. The transit technique has been used to find the majority of known exoplanets. When a planet passes in front of an observer and a star, it is said to be transiting. Transits in our solar system can be seen from Earth as Venus or Mercury pass in front of the Sun. The atmosphere of a transiting exoplanet can be seen backlit by the star when it passes its host star. As exoplanets pass in front of and behind their stars, one can do further atmosphere observations.
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a 80 kg student is standing atop a spring in an elevator that is accelerating upward at 3.0m/s2. the spring constant is 2700 n/m .
According to the question, the spring will be compressed by 0.3413 m.
What are the physics applications of springs?Springs are crucial because they provide as straightforward models for numerous complex physical processes. In physics, objects that behave like springs exhibit what has known as a simple harmonic motion (SHM), which you will encounter again. k is referred to as the spring constant.
Briefing:acceleration of elevator=3 m/s²
mass of student= 80 Kg
spring constant=3 x 10³ N/m
the force on the student is given by F = m ( g +a)
F=80 (9.8+3)
F=1024 N
now the formula for spring force is given by
F= k x
1024= 3 x 10³ (x)
x=0.3413 m
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eudora ran from her home to her secret laboratory at an average speed of 12\text{ km/h}12 km/h12, start text, space, k, m, slash, h, end text. she then took one of her jetpacks and flew to her school at an average speed of 76\text{ km/h}76 km/h76, start text, space, k, m, slash, h, end text. eudora traveled a total distance of 120120120 kilometers, and the entire trip took 222 hours.
Eudora used her jetpack for around 1.5 hours of flying and 0.5 hours of jogging.
Given: Eudora moved at an average pace of 12 km/h as she sprinted from her house to her underground laboratory. She then hopped into one of her jetpacks and soared 76 km/h to her school. Eudora covered 120 kilometres in all, and the journey took her two hours.
To determine: How much time Eudora spent running and how much time she spent using her jetpack to fly
Solution:
If she utilised the jet pack for x seconds, then
76x + 12 (2-x) = 120
76x + 24 – 12x = 120
x = 96/64
x= 1.5
She spent 0.5 hours running, thus when we simplify, x = 1.5 hours.
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Bill Lauer, retired UT professor who holds six.national swimming records in the 80-84 age group, drops one of his medals in the swimming pool. He shines a flashlight into the pool onto his medal. The index of refraction of the water is 1.33. All dimensions are given in meters STATS-HELP ? NOTES T IMAGES | i Discuss. I Ulis art Description Answer Chk History Try 2-your answer of 3.44 m is not correct. How far is the medal from the edge 3.44m A of the pool? (include units with answer) 13.2 pts. 106% Angles must be measured from normal, not from water surface. try penalty tries: 2. how Detais Hints: 0.1
Using Snell's Law we got the distance from the edge to be 4.678 m.
Snell's law (also known as Snell–Descartes law and the law of refraction) is a formula used to describe the relationship between the angles of incidence and refraction, when referring to light or other waves passing through a boundary between two different isotropic media, such as water, glass, or air.
Snell's law is used for refraction of light
It is a formula used to describe the relationship between the angles of incidence and refraction, when referring to light or other waves passing through a boundary between two different isotropic media.
From Snell's Law,
n₁ sin i = n₂ sin r
1 * [1.6 /√(1.6² + 1.1²)] = 1.33 * [P / √(P² + 3.9²)]
P² = 0.3838P² + 0.3838(3.9)²
P = 3.078 m
Now, with the solution of Snell's Law, we can easily find the distance from the edge.
Distance from the edge = (1.6 + 3.078) = 4.678 m
Therefore, using Snell's Law we got the distance from the edge to be 4.678 m.
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Q1: A pupil fires an elastic band gun. Just before it is released the band is at its most stretched point. If the band is extended by 0.36m and the band is fired with 412J of energy, what is the spring constant of the band?
The spring constant of the given band is equal to 6.36 × 10³ N/m.
What is Hooke's law?Hooke's law can be demonstrated as a law that states that the force (F) required to extend or compress a spring by displacement linearly w.r.t. that distance along a straight line.
The spring force can be represented in the form of mathematical equation:
F = -kx,
where k is a spring constant and x is the deformation of the spring. The negative sign shows that the spring returns to its original position.
The energy stored in the spring when it is extended is given by:
E = (1/2)kx²
Given, the energy stored in the band when it is extended, E = 412 J
The distance by which the band is extended, x = 0.36 m
412 = (1/2)×k (0.36)²
k = 6.36 × 10³ N/m
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Jane, looking for Tarzan, is running at top speed (4.5 m/s) and grabs a vine hanging vertically from a tall tree in the jungle. How high can she swing upward?
Does the length of the vine affect your answer?
Jane could swing 1.03316 m high and the length of the vine does not affect the answer .
In the question ,
it is given that ,
the top speed of Jane is = 4.5 m/s .
she grabs a vine that is hanging vertically from a tall tree in the jungle .
The kinetic energy of running Jane can be converted into gravitational potential energy, and
the highest point is reached when all the Kinetic Energy has been changed to Potential energy .
we know , KE = 1/2mv²
PE = mgh
So Equating KE = PE
and solving for h:
we get , h = v²/2g
So , h = 4.5²/(2*9.8)
= 1.03316 m
also we can conclude that , the length of the vine does not affect the answer .
Therefore , the Jane could swing 1.03316 m high .
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Part A Which of the following statements are true? Check all that apply. View Available Hint(s) Mechanical energy is conserved because no dissipative forces perform work on the ball. The forces of gravity and the spring have potential energies associated with them. No conservative forces act in this problem after the ball is released from the spring gun.
The statement that is true is Mechanical energy is conserved because no dissipative forces perform work on the ball. The correct option is A.
What is mechanical energy?Mechanical energy, also known as kinetic energy or potential energy, is the energy that an object possesses when it is in motion or the energy that an object stores due to its location.
Renewable energy is also fueled by mechanical energy. In order to efficiently produce electricity or convert energy, many sources of renewable energy depend on mechanical energy.
Therefore, the correct option is A, Mechanical energy is conserved because no dissipative forces perform work on the ball.
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A star's absolute magnitude is its apparent brightness as seen from
A. Alpha Centauri.
B. 10 light-years distance.
C. 10 parsecs distance.
D. 100 parsecs distance.
E. Pluto.
Answer: C
The absolute significance of a star is 10 parsecs distance , M is the significance the big name could have if it become located at a distance of 10 parsecs from Earth.
By thinking about stars at a set distance, astronomers can evaluate the real (intrinsic) brightnesses of various stars.Apparent significance is the brightness of a celebrity because it seems to the observer. This is what stargazers look at after they study the sky and spot that a few stars are brighter than others. Absolute significance is the brightness of a celebrity from a distance of 10 parsecs away. A parsec is same to 32.6 light-years.
Astronomers outline big name brightness in phrases of obvious significance — how shiny the big name seems from Earth — and absolute significance — how shiny the big name seems at a popular distance of 32.6 light-years, or 10 parsecs.
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The starships of the Solar Federation are marked with the symbol of the Federation, a circle, whereas starships of the Denebian Empire are marked with the Empire's symbol, an ellipse whose major axis is n times its minor axis (a = nb in the figure (Figure 1)). How fast, relative to an observer, does an Empire ship have to travel for its markings to be confused with those of a Federation ship? Use c for the speed of light in a vacuum. Express your answer in terms of n and c.
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The speed at which an Empire ship must travel for its markings to be confused with those of a Federation ship is sqrt(c^2 - 1/n^2) * c, where n is the ratio of the major axis to the minor axis of the ellipse and c is the speed of light in a vacuum.
The appearance of an object changes when it moves at a significant fraction of the speed of light due to the phenomenon of relativistic length contraction. This effect causes the length of the object to appear shorter to an observer, and also causes any features on the surface of the object to be distorted.
In the case of the Empire ship and the Federation ship, the appearance of the symbols on their hulls would be affected by relativistic length contraction. If the Empire ship is moving fast enough, its ellipse-shaped symbol may appear to an observer as a circle, similar to the symbol on the Federation ship.
To determine the speed at which this would occur, we can use the equation for relativistic length contraction: L' = L / sqrt(1 - v^2/c^2), where L' is the length of the object as observed by the observer, L is the actual length of the object, v is the speed of the object, and c is the speed of light in a vacuum.
By setting L' equal to the length of the minor axis of the ellipse (b) and L equal to the length of the major axis (a), and solving for v, we can determine the speed at which the Empire ship must travel for its markings to be confused with those of the Federation ship. This speed is given by the equation v = sqrt(c^2 - b^2/a^2) * c, where n is the ratio of the major axis to the minor axis of the ellipse and c is the speed of light in a vacuum.
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for universes with no dark energy ( ) composed of pressureless matter , what does this imply for an upper limit on , if is equal to 70 km/s/mpc? curvature is determined by the value of , you mustn't simply assume it is flat, obviously
The value of the Hubble constant, denoted H0, represents the expansion rate of the universe. It is defined as the ratio of the speed at which a galaxy is receding from an observer to its distance from the observer. In a universe with no dark energy and composed of pressureless matter, the expansion rate is determined by the density of matter in the universe.
If the Hubble constant is equal to 70 km/s/Mpc, this implies that the expansion rate of the universe is 70 km/s per megaparsec of distance. It does not directly provide information about the curvature of the universe, as the curvature depends on the amount and distribution of matter and energy in the universe, as well as the expansion rate. To determine the curvature of the universe, you would need to know the density of matter in the universe and the expansion rate. If the density of matter in the universe is high enough, the expansion rate will be slowed down and the universe will be closed and have positive curvature. If the density of matter in the universe is low enough, the expansion rate will be accelerated and the universe will be open and have negative curvature. If the density of matter in the universe is just right, the expansion rate will remain constant and the universe will be flat. Without knowing the density of matter in the universe, it is not possible to determine the curvature of the universe based on the value of the Hubble constant alone.
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3. A ballon of weight 300 N is moving upward. Volume of
ballon is 30m³ and displacing air of density 1.2kg/m³ 11.A
then the upward force acting in the ballon is?
The upward force acting in the ballon is -352.8N
What is upward force?This refers to a force exerted by a fluid that opposes the weight of a partially or fully immersed object. In a column of fluid, pressure increases with depth as a result of the weight of the overlying fluid. the upward force is also known as upthrust. It operates under Archimedes' principle.
The formula for calculating upward force:
Fb = -ρ g V
Where,
Fb = buoyant force
ρ = fluid density
g = acceleration due to gravity
V = fluid volume
From the question:
V= 30m³
ρ = 1.2kg/m³
W = 300 N
g = 9.8m/s
To calculate buoyant force, Fb:
Fb = -ρ g V
Fb = - 1.2kg/m³ * 9.8m/s * 30m³
Fb = -352.8N
Note: Negative upward force suggests that the immersed object is denser than the fluid displaced which results in the sinking of the object. Neutral buoyancy takes place when the weight of the immersed object is equivalent to the fluid displaced. The dive taken by the scuba diver is a perfect example of neutral buoyancy.
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in the circuit at right, the bulbs are identical, and the battery is ideal. rank the brightness of the bulbs in the ircuit at right
Brightest resistor is the one with the most current. The current via bulb C is the highest since it receives the same amount of current as the battery.
What is an example of a resistor?Digital potentiometers and rheostats are variable resistors. Electrical parts called rheostats are constructed from resistive thin wire around for a ceramic core. They were once employed to regulate the quantity of power utilized by ovens, heaters, and motors.
How do resistors function?By decreasing the voltage and obstructing the passage of electricity, the resistance absorbs the electrical energy, which is then released as heat. The heat dissipation in electronic circuits today is typically a few hundredths of a watt.
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9. A 0.25 kg steel ball experiences a net force of 1.15 N as it rolls down a ramp. What is the
acceleration of the ball?
a. 0.29 m/s²
b. 0.90 m/s²
c. 1.4 m/s²
d. 4.6 m/s²
Answer:
4.6 option d
Explanation:
from second Newton law of motion
F=ma
to find acceleration
a= F/m
a= 1.15/0.25
a = 4.6
a 2000 hz sound wave passes through a wall with two narrow openings 30 cm apart. if sound travels on average 352 m/s, find the following. (a) what is the angle of the first order maximum?
Angle of the first order maximum is 35.1°.
Given,
frequency f= 2000 Hz
sound travels average 352 m/s
The speed of the sound wave is 352 meters per second, and the Frequency is 2000. The slate is separated by 30 cm. The position of the first order needs to be found. There is a maximum for interference.
a) wavelength = v/f = 352/2000
λ = d sinФ
Ф = si[tex]n^-^1[/tex]( (352/2000)/.3)= 35.4°
The speed of sound can be written as 52 meter per second if the Frequency is 2000 times one over the separation. The first order's maximum is 35.4 degrees.
b) then λ/d
=(352/2000)/.3 = 2.85E-2/d
d=0.0496 m
c) (352/3000)/.3 = (352/f)/1.0E-6
f= 9.0E8 Hz
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The proper time between two events is measured by clocks at rest in a reference frame in which the two events: A. occur at the same time B. occur at the same coordinates C. are separated by the distance a light signal can travel during the time interval D. occur in Boston E. satisfy none of the above
The proper time between two events is measured by clocks at rest in a reference frame in which the two events occur at the same coordinates. (Option B)
In physics and astronomy, a frame of reference or reference frame refer to an abstract coordinate system whose origin, orientation, and scale are specified by a set of reference points which are geometric points whose position is identified both mathematically (with numerical coordinate values) and physically (signaled by conventional markers). Hence, the proper time between two events is measured by clocks at rest in a reference frame in which the two events occur at the same coordinates.
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A rocket on Earth experiences an upward applied force from its thrusters. As a result of this force, the rocket accelerates upward at 2 m/s2. Assume that there are no other upward forces exerted on the rocket and that wind resistance is negligible. Which of the following combinations of the rocket mass Mrocket and force from its thrusters FThrusters would result in an upward acceleration of 2 m/s2? Select two answers.
A. Mrocket 1 kg, FThrusters 12N
B. Mrocket 2 kg, FThrusters 4 N
C. Mrocket 3 kg, FThrusters 6 N
D. Mrocket 3 kg, FThrusters 36 N
The combinations of the rocket mass Mrocket and force from its thrusters FThrusters would result in an upward acceleration of 2 m/s2 are
A. Mrocket 1 kg, FThrusters 12 N
C. Mrocket 3 kg, FThrusters 6 N
Using Newton's Second Law, F = ma, we can determine the force needed to accelerate a rocket at a given rate. Since the mass of the rocket is given, we can calculate the force by rearranging the equation to F = m*a, where m is the mass and a is the acceleration. Therefore, for a mass of 1 kg, the force needed to achieve an acceleration of 2 m/s2 is 12 N. Similarly, for a mass of 3 kg, the force needed to achieve an acceleration of 2 m/s2 is 6 N.
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Classical physics defines the vacuum as a state of absence: a vacuum is said to exist in a region of space if there is nothing in it. In the quantum field theories that describe the physics of elementary particles, the vacuum becomes somewhat more complicated. Even in empty space, particles can appear spontaneously as a result of fluctuations of the vacuum. For example, an electron and a positron, or antielectron, can be created out of the void. Particles created in this way have only a fleeting existence; they are annihilated almost as soon as they appear, and their presence can never be detected directly. They are called virtual particles in order to distinguish them from real particles, whose lifetimes are not constrained in the same way, and which can be detected. Thus it is still possible to define the vacuum as a space that has no real particles in it.
The Vacuum - Its Fluctuations and Decay.
Vacuum is not the problem. The reason space is almost a complete vacuum is not because it is attracted to you, but because it is almost empty.
This emptiness results in extremely low pressure. This is an approach to theoretical physics and quantum mechanics that views the underlying physical vacuum as a superfluid or Bose-Einstein condensate.
A vacuum is a space devoid of matter, or a space in which the pressure is so low that the particles in the space do not affect the processes taking place therein. This is a state well below normal atmospheric pressure and is measured in units of pressure. There is no perfect vacuum because it is impossible to remove all air or particles from space. However, partial vacuums are common.
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You are to measure the rotational speed of a crank shaft. The available angular velocity meter has a display with resolution of 2 rpm (revolutions/minute). The meter specifications indicate that the device accuracy is 1.5% of the velocity reading. Find the design stage uncertainty for each of the following velocities
You are required to gauge a crank shaft's rotational speed. The device's level of uncertainty will be 0%.
What does rotational speed mean?The number of rotations a rotating system completes in a predetermined amount of time is the measure of rotational speed, also known as speed or speed of rotation. Pump speed is often expressed in min-1, while rotational speed is measured in s-1 (rev/s) (rpm).
What about angular velocity in rotation?The term "angular velocity" or "rotational velocity" ( or ), also known as "angular frequency vector," refers to a pseudovector that expresses how quickly an item spins or circles in relation to a point or axis or changes its angular location or orientation over time.
Briefing:The velocity meter's resolution = 2 rpm.
accuracy = 1.5%.
40 rpm = 1.5%.
The speed can change at 40 rpm = 39.7 to 40.3 rpm.
The device's resolution = 2 rpm.
uncertainty = 0%.
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Problems 2-3 refer to the following situation. A lake has a depth of
27.5 m
. The lake is filled with water, with has a density of
1000 kg/m^3
. Since the top of the lake is open to the air, the pressure at the top of the lake is the atmospheric pressure,
P 0​ =1.0×10^5
. Problem 2: What is the pressure at the bottom of the lake? a.
1.7×10^5 Pa
b.
3.7×10^5 Pa
c.
5.7×10^5 Pa
d.
7.7×10^5 Pa
Problem 3: An underwater vehicle is at the bottom of the lake. The vehicle has a circular window of radius
0.175 m
. What is the force on this window, due to the water? a.
1.6×10^4 N
b.
3.6×10^4 N
c.
5.6×10^4 N
d.
7.6×10^4 N
A pressure at the bottom of the lake of: P = 3.7 x 10^5 Pa So the answer to problem 2 is 3.7 x 10^5 Pa the answer to problem 3 is 3.6 x 10^4 N.
To find the pressure at the bottom of the lake, you can use the formula for hydrostatic pressure: P = P0 + rho * g * h Where P is the pressure at the bottom of the lake, P0 is the atmospheric pressure at the top of the lake, rho is the density of the water, g is the acceleration due to gravity, and h is the depth of the lake. Plugging in the given values, you get: P = 1.0 x 10^5 Pa + 1000 kg/m^3 * 9.8 m/s^2 * 27.5 m This gives a pressure at the bottom of the lake of: P = 3.7 x 10^5 Pa. To find the force on the circular window, you can use the formula for the force exerted by a fluid on a surface: F = P * A Where F is the force on the window, P is the pressure at the bottom of the lake, and A is the area of the window. The area of the window can be calculated using the formula for the area of a circle: A = pi * r^2 Where A is the area of the window, pi is the mathematical constant pi (approximately 3.14), and r is the radius of the window. Plugging in the values, you get: F = 3.7 x 10^5 Pa * (pi * (0.175 m)^2) This gives a force on the window of: F = 3.6 x 10^4 N So the answer to problem 3 is b. 3.6 x 10^4 N.
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as a jet is taking off, it is accelerating down the runway with acceleration , with . you are sitting inside the jet and holding a simple pendulum consisting of a bob of mass attached to a string of length . the pendulum comes to rest in the equilibrium position where the string makes an angle with respect to the vertical. when the bob is in the equilibrium position, which of the following free-body force diagrams on the bob is correct in a reference frame fixed to the accelerating jet.
A jet plane's acceleration is a critical phase of flight that necessitates intense focus on the part of both pilots.
On the ground, things can get hectic and demand a lot of situational awareness, especially when there is little traffic separation, a runway is wet, visibility is poor, and there are heavy winds. Nevertheless, you start to relax a little and take in the beauty of flying as the engines begin to accelerate and you take off and break through the clouds. We have put up this essay with all you need to know so that you may master the takeoff phase in complete confidence.
You must commit to memory three call-outs for the acceleration and takeoff phases of your flight. You will first check your instruments at 80 knots. When you push the nose of your aircraft upward and rotate in V1, you are too quick to abort the takeoff.
This was merely a succinct justification. In order to help you mentally prepare, we will go over every important stage of a jet plane's acceleration.
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the plane of a loop of wire is perpendicular to a magnetic field. rank, from greatest to least, the magnitudes of the loop's induced emf for each situation. a. the magnetic field strength increases from 0 t to 1 t in 6 s . b. the magnetic field strength increases from 1 t to 4 t in 2 s . c. the magnetic field strength remains at 4 t for 1 min . d. the magnetic field strength decreases from 4 t to 3 t in 4 s . e. the magnetic field strength decreases from 3 t to 0 t in 1 s . rank from greatest to least. to rank items as equivalent, overlap them.
The plane of a loop of wire is perpendicular to a magnetic field. Rank, from greatest to least, the magnitudes of the loop's induced emf for each situation will be E - B - D - A-C.
Magnetic field strength is one of two ways that the intensity of a magnetic field can be expressed. Technically, a distinction is made between magnetic field strength H, measured in amperes per meter, and magnetic flux density B, measured in Newton-meters per ampere, also called tesla.
A current I through a long, straight wire produces a magnetic field with strength H=I/2πr at a distance r from the wire. So the field strength is inversely proportional to the distance from the wire.
The unit of magnetic field strength happens to be ampere per meter or A/m. Furthermore, the symbol of the magnetic field strength happens to be H.
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Listed following is a set of statements describing individual stars or characteristics of stars. Match these to the appropriate object category.a. Red Giant or Supergiant Starts.b. Main-sequence starsc. White dwarfs1. Very cool but very luminous2. Found in the upper right of the H-R diagram3. The majority of stars in our galaxy4. The Sun, for example5. A very hot and very luminous star6. not much larger in radius than Earth7. Very hot but very dim
The five fundamental features of a star are its brightness, color, surface temperature, size, and mass.
Supergiant or Red Giant Stars are located in the upper right corner of the H-R diagram and are extremely cool but bright.
The majority of the stars in our galaxy are main-sequence stars, such as the Sun, which is an extremely hot and brilliant star.
White dwarfs are tremendously hot, but they are also quite dim. Their radii are not much larger than Earth's.
The largest and hottest stars are those in the 'O' class, with temperatures over 30,000 °C. The smallest and coldest stars are those in the 'M' class, with temperatures below 3,000 °C. The stars in the sky are not all the same color when you look attentively at them.
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when you urinate, you increase pressure in your bladder to produce the flow. for an elephant, gravity does the work. an elephant urinates at a remarkable rate of 0.0060 m3 (a bit over a gallon and a half) per second. assume that the urine exits 1.0 m below the bladder and passes through the urethra, which we can model as a tube of diameter 8.0 cm and length 1.2 m. assume that urine has the same density as water, and that viscosity can be ignored for this flow.
During urination, the pressure in the bladder increases to produce the flow hence, the speed of the flow of urine is 1.19 m/s and bernoulli's equation give for the pressure in the bladder is -9092 pa.
The Bernoulli equation is concerned with the conservation of kinetic, potential, and flow energies of a fluid stream and their conversion to each other in regions of flow where net viscous forces are negligible and where other restrictive conditions apply. The energy equation is a statement of the conservation of energy principle.
The Bernoulli equation is an approximate relation between pressure,velocity, and elevation, and is valid in regions of steady, incompressible flow where net frictional forces are negligible.
Given,
d = 8 cm = 0.08 m
Area of the tube, A = pi*d^2/4
= pi*0.08^2/4
= 0.005036 m^2
volume flow rate, dV/dt = A*v
v = (dV/dt)/A
= 0.006/0.005036
= 1.19 m/s
Now, use Bernoulli's theorem,
P_baldder + rho*g*h1 + (1/2)*rho*v1^2 = P_atm + rho*g*h2 + (1/2)*rho*v^2
P_baldder + rho*g*h + 0 = P_atm + 0 + (1/2)*rho*v^2
P_baldder - P_atm = (1/2)*rho*v^2 - rho*g*h
= (1/2)*1000*1.19^2 - 1000*9.8*1
= -9092 Pa
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