Answer:
•So he stays healthy.
•He has energy and time to do it.
An airplane is flying at a constant speed along with a constant height of 3 km that will take it directly over an observer at ground level. At a given instant, the observer notes that the angle between him and the airplane is 3π and is increasing at 201 radians per second. Find the speed of the airplane, in km/hr. b. Continue as part (a), if the airplane comes towards the observer at a constant angular rate of change 201, what is the speed of the airplane when it is directly over the head of the observer? c. Is the airplane slowing down or speeding up as it approaches the observer? Justify your conclusion.
A- The speed of the airplane is approximately 201 km/hr.
b. The speed of the airplane when directly over the observer is approximately ∞ km/hr.
c. The airplane is slowing down as it approaches the observer.
a. To find the speed of the airplane:
dx/dt = (1 + tan²(θ)) * dθ/dt
At θ = 3π, tan(3π) = 0, so:
dx/dt = (1 + 0²) * 201
dx/dt = 201 km/hr
b. To find the speed of the airplane when directly over the observer:
dx/dt = (1 + tan²(θ)) * dθ/dt
Taking the limit as θ approaches π/2 from below:
lim(θ→π/2-) (1 + tan²(θ)) = ∞
So the speed of the airplane is approximately ∞ km/hr.
c. We can observe from the rate of change equation dx/dt = (1 + tan²(θ)) * dθ/dt that the speed of the airplane, dx/dt, is directly dependent on the rate of change of the angle, dθ/dt. In this case, the rate of change of the angle is given as 201 radians per second.
Since the rate of change of the angle, dθ/dt, is positive and constant, we can conclude that the speed of the airplane, dx/dt, will also be positive and constant. This means that the airplane is moving forward at a constant speed.
As the airplane approaches the observer, the angle θ decreases, which implies that tan(θ) also decreases. Since the speed of the airplane is directly proportional to (1 + tan²(θ)), which is decreasing as θ decreases, the speed of the airplane gradually decreases.
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If a rock is thrown downward with an initial speed 6ms then what is the rocks velocity after 4 sec
Answer:
\(\huge\boxed{\sf V_f=45.2 \ m/s}\)
Explanation:
Given Data:Initial velocity = \(V_i\) = 6 m/s
Time = t = 4 sec
Acceleration due to gravity = g = 9.8 m/s²
Required:Final velocity = \(V_f\) = ?
Formula:\(v_f=v_i+gt\)
Solution:Put the givens in the formula
\(V_f=6 +(9.8)(4)\\\\V_f=6+39.2\\\\V_f=45.2 \ m/s\\\\\rule[225]{225}{2}\)
the apparatus represented in the (figure 1) consists of five identical balls mounted on elastic rods. each elastic rod is connected to a base. the (unlabeled) ball and rod on the far left are pulled towards the screen (that is, toward you) and released. which of the ball-and-rod combinations will have the largest amplitude of oscillation?
The correct option is D. This is due to the fact that the rod in D has the same length as the vibrating rod (unlabeled), making it more likely for it to enter into resonance and generate a more pronounced oscillation.
In a complex mixture of chemical compounds that are reacting, a chemical oscillator is one in which the concentration of one or more components changes on a regular basis.
A trustworthy point level sensor for high and low level indication or plugged chute detection is a vibrating rod, also known as a vibrating level switch. Bulk densities of as little as 1.25 lb/ft3 can be used for their use in light, fluffy powders and flakes.
Therefore, option (d) is correct-This is because, the rod in D has same length as the vibrating rod (unlabeled) so its more likely to get in resonance with that that's why it oscillates more vigorously.
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How do astronomers know that stars are not all the same distance from us?
Answer:
'brightness' and 'place' (?)
Explanation:
You can tell the distance in both simple and complicated ways; for instance, some methods like using luminosity don't work for all stars*
quote for better understanding:
"Farther methods are usually based on identifying what type of star a given star is, and estimating its luminosity .."
"..We then measure its apparent brightness (how bright it looks)* and do some math to figure out how far away it is."
(more detailed quote):
"By knowing the actual brightness and comparing it to the apparent brightness seen from Earth (that is, by looking at how dim the star has become once its light reaches Earth), they can determine the distance to the star."
Alternatively by observing the position of the star or its place a similar technique is used:
quote:
"Earth orbits the Sun, so it is in a slightly different position in January than in July. Nearby stars will seem to slightly shift in position in our sky relative to far-away stars."
In conclusion-- luminosity is commonly how astronomers know that stars are not all the same distance away from us.
There are ________ protons, ________ electrons, and ________ neutrons in an atom of 1315413154xe.
In an atom of ¹³¹⁵⁴¹³¹⁵⁴Xe, there are 54 protons, 54 electrons, and 77 neutrons.
The atomic symbol ¹³¹⁵⁴¹³¹⁵⁴Xe represents a specific isotope of the element xenon, denoted by Xe. The number ¹³¹⁵⁴ indicates the total number of nucleons (protons and neutrons) in the nucleus of the atom.
The atomic number of an element represents the number of protons in its nucleus. In this case, xenon (Xe) has an atomic number of 54, indicating it has 54 protons. Since atoms are electrically neutral, the number of protons is equal to the number of electrons. Therefore, there are 54 electrons in an atom of ¹³¹⁵⁴Xe.
To determine the number of neutrons, we subtract the atomic number from the total number of nucleons. In this case, ¹³¹⁵⁴Xe has a total of 131 nucleons (protons + neutrons). Subtracting 54 (the atomic number) from 131 gives us 77 neutrons.
An atom of ¹³¹⁵⁴Xe contains 54 protons, 54 electrons, and 77 neutrons.
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Laboratory experiments here on Earth have determined that each element in the periodic table emits photons only at certain wavelengths. These photons are apparent to astronomers as either emission or absorption lines in the spectrum of an astronomical object, like stars in galaxies. Astronomers can, by measuring the position of these spectral lines, determine which elements are present in the star itself or along the line of sight. When astronomers perform this analysis, they note that for most astronomical bodies, the observed spectral lines are all shifted to longer (redder) wavelengths. This is known as cosmological redshift and is analogous to the Doppler redshift. What does this redshift indicate to us about the universe in general?
A) The age of the universe.
B) The universe is expanding.
C) How much longer the universe should exist.
D) The universe is contracting into a black hole.
Answer: answer is B
Explanation:
Mumtaz chooses TWO two digit numbers and divided one by the other. His answe was 2. 12121212121
find the two numbers he used
The two numbers that Mumtaz used are:
15 and 75
27 and 81
39 and 99
21 and 10
Let's assume the two-digit numbers chosen by Mumtaz are represented by "AB" and "CD," where A, B, C, and D are digits.
According to the given information, Mumtaz divided one number by the other and obtained a result of 2.12121212121.
We can express this division as:
(AB) / (CD) = 2.12121212121
To solve this problem, we'll examine the possible values of A, B, C, and D.
First, let's focus on the integer part of the division (before the decimal point). Since the division result is 2, it implies that AB divided by CD must be equal to 2.
So, we have:
(AB) / (CD) = 2
This equation suggests that AB should be twice the value of CD. Let's consider the possible cases:
Case 1: AB = 2 * CD
To find the possible values, we can iterate through all two-digit numbers and check if AB is equal to twice CD.
The possible values for A and C are:
A = 1, C = 5
A = 2, C = 7
A = 3, C = 9
For each value of A and C, we need to find the corresponding values of B and D.
For A = 1 and C = 5, AB = 15, and CD = 75 (since 15 / 75 = 0.2).
For A = 2 and C = 7, AB = 27, and CD = 81 (since 27 / 81 = 0.333...).
For A = 3 and C = 9, AB = 39, and CD = 99 (since 39 / 99 = 0.3939...).
Case 2: AB = 20 * CD
In this case, the value of AB would be twenty times the value of CD.
The only possible values for A and C are:
A = 2, C = 1
For A = 2 and C = 1, AB = 21, and CD = 10 (since 21 / 10 = 2.1).
Therefore, the two numbers that Mumtaz used are:
15 and 75
27 and 81
39 and 99
21 and 10
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A 0.50-kilogram frog is at rest on the bank surrounding a pond of water. As the frog leaps from the bank, the magnitude of the acceleration of the frog is 4.0 meters per second².
Complete question:
A 0.50 kilogram frog is at rest on the bank surrounding a pond of water. As the frog leaps from the bank, the magnitude of the acceleration of the frog is 4.0 meters per second^2. Calculate The magnitude of the net force exerted on the frog as it leaps.
Answer:
2.0N
Explanation:
Given that,
Mass, m of the frog = 0.5 kg
The acceleration of the frog = 4.0 m/s².
We have been asked To find,
The magnitude of the net force exerted on the frog as it leaps.
So
We calculate this using the formula below :
F = ma
When we insert the values into the formula, we have:
F = 0.5 kg × 4 m/s²
F = 2.0 N
Therefore, the magnitude of net force is 2.0 N.
when the protostar has the following temperatures, what is its luminosity? what is the radius of a protostar with these temperatures and luminosities compared to the radius of the sun? what is happening to the protostar at 200 k? what is happening to the protostar at 1000 k?
The first stage in the evolution of stars is the protostellar phase. It lasts roughly 500,000 years for a low-mass star (sun-mass or less).
When a star is still gaining mass from its parent molecular cloud, it is referred to as a protostar. The first stage in the evolution of stars is the protostellar phase. It lasts roughly 500,000 years for a low-mass star (sun-mass or less). A molecular cloud fragment first experiences self-gravity-induced collapse before entering the phase, where an opaque, pressure-supported core develops inside the fragment. It comes to an end when the gas that is descending outruns it, leaving a pre-main-sequence star that subsequently contracts to become a main-sequence star at the start of hydrogen fusion that produces helium. Since the protostar is still contracting, its diameter and surface area are extremely large, and its luminosity may be approximately 100 times greater than when it is fully formed.
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Trey is skiing on a circular ski trail that has a radius 0.8 km long. Trey starts at the 3-o'clock position (the easternmost point on the trail) and travels 2.75 km in a counterclockwise direction. Imagine an angle with its vertex at the center of the circular trail that subtends the path Trey skis. a. What is the angle's measure in radians?
The length of the subtended arc divided by the circle's radius, r, is the radian measurement of the angle.
For instance, if the circle's radius is two and the arc's length is three, the radian measurement is 1.5.
To find the angle's measure in radians, we need to use the formula:
angle (in radians) = distance traveled / radius
In this case, Trey traveled 2.75 km along the circular ski trail with a radius of 0.8 km. So the angle's measure in radians is:
angle (in radians) = 2.75 km / 0.8 km = 3.4375 radians
Therefore, the angle's measure in radians is approximately 3.4375 radians.
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In Concept Simulation 17.2 you can explore the concepts that are important in this problem. A 421-Hz tuning fork is sounded together with an out-of- tune guitar string, and a beat frequency of 5 Hz is heard. When the string is tightened, the frequency at which it vibrates increases, and the beat frequency is heard to decrease. What was the original frequency of the guitar string? Number i Units
The original frequency of the guitar string was 416 Hz.
The original frequency of the guitar string can be determined by using the formula for beat frequency:
Beat frequency = |f1 - f2|
Where f1 and f2 are the frequencies of the two sounds producing the beat.
In this case, the beat frequency is 5 Hz and the frequency of the tuning fork is 421 Hz. We can plug these values into the formula and solve for the original frequency of the guitar string (f2):
5 Hz = |421 Hz - f2|
There are two possible solutions for this equation:
f2 = 421 Hz + 5 Hz = 426 Hz
or
f2 = 421 Hz - 5 Hz = 416 Hz
Since the problem states that the guitar string is out of tune and the frequency increases when it is tightened, the original frequency of the guitar string must be lower than the frequency of the tuning fork. Therefore, the original frequency of the guitar string is 416 Hz.
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The mass of each loaf of bread produced by a bakery follows a normal distribution with the mean of 400g and standard deviation of 18g. Find the probability that a loaf of bread chosen at random will have a mass of more than 450g.
The probability that a loaf of bread chosen at random will have a mass of more than 450g is 0.0026 or 0.26%.
The probability that a loaf of bread chosen at random will have a mass of more than 450g is found by first standardizing the random variable, using the standard normal distribution. We can then use the standard normal table or calculator to find the area to the right of the standardized value. The standardized random variable can be found using the formula
Z = (X - μ) / σ,
where X is the given value, μ is the mean, and σ is the standard deviation.
Substituting the given values, we get:
Z = (450 - 400) / 18 = 2.78
Using the standard normal table or calculator, we can find the area to the right of 2.78. This area represents the probability that a loaf of bread chosen at random will have a mass of more than 450g.
Using a standard normal table or calculator, we find that this area is 0.0026 or 0.26%.
Hence, the probability that a loaf of bread chosen at random will have a mass of more than 450g is 0.0026 or 0.26%.
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Kinetic Energy HELP! Brainly included
Answer:
A
Explanation:
When you dropping the swing, it increases the kinetic energy. In the middle, that is when it is at it's fullest potential. As it makes its way up, it pushes again the gravitational force, and soon, the swing will stop at the top for a VERY SHORT AND SMALL period of time. That is when it is at it's very weakest point, making the answer, indeed, A.
explain why it is important to keep the weight over the pulley constant ( Newton 's second law)
Newton's second law of motion states that the acceleration of an object is directly proportional to the net force acting on it and inversely proportional to its mass. In other words, the larger the net force acting on an object, the greater its acceleration, and the larger the object's mass, the smaller its acceleration for a given force.
Why is it important to keep the weight over the pulley constant?When a weight is placed over a pulley, the net force acting on it is equal to the weight of the object, and the acceleration of the object depends on its mass. However, if the weight over the pulley is not constant, the net force acting on the object changes, which affects its acceleration.
For example, if the weight over the pulley increases, the net force acting on the object also increases, and the object's acceleration increases. Conversely, if the weight over the pulley decreases, the net force acting on the object decreases, and the object's acceleration decreases.
Keeping the weight over the pulley constant ensures that the net force acting on the object remains constant, which allows for accurate and predictable calculations of the object's acceleration. This is especially important in scientific and engineering applications where precise measurements and calculations are necessary.
Therefore, it is important to keep the weight over the pulley constant to ensure that Newton's second law of motion can be applied accurately and consistently.
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Your job is to order and connect lead-acid cells used to supply an uninterruptible power supply (UPS). The battery output voltage must be 126 V and have a current capacity of not less than 250 A-hr. Each cell has a rating of 2 V and 100 A-hr. How many cells must be ordered and how would you connect them?
In order to achieve an output of 126 Volts and a current capacity of at least 250 Ahr, the three sets of 63 lead acid cells that were connected in series should be connected in parallel, which means that a total of 189 solar cells are needed to connect in series and parallel.
What is cell?
An electrical current can be produced by a cell, a unit structure, in addition to a conductor moving through a magnetic field. For instance, a semiconductor junction in a solar cell turns sunlight directly into energy.
As is well known, when cells are connected in series, their voltages are increased while maintaining the same current capacities, and when cells are connected in parallel, their voltages are maintained while increasing the current capacities.
The quantity of lead-acid cells that must be connected in parallel in order to generate 126 Volts is,
126 / 2 = 63
The no of lead acid cells required to connect in parallel to produce 250 Ahrs is,
250 / 100 = 2.5 ≈ 3
Therefore, three sets of 63 lead acid cells that were connected in series should be connected in parallel are required.
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if vector A=2i+3j-k and vector B=4i+6j-2k. The angle between them will be: a) 0°b)45°c)90°d)60°
Notice that
B = 4i + 6j - 2k = 2 (2i + 3j - k) = 2A
so both vectors point in the same direction and the angle between them is (A) 0°.
The Hale telescope on Mount Palomar has a diameter of 5.08 m (200 in.). Hint (a) If the smallest crater diameter the telescope can resolve on the Moon is 54.2 m, what wavelength light is being used? (Give your answer in nm. Assume the crater is 3.76 x 108 m from the telescope.) nm (b) What diameter crater (in m) could the Hubble telescope resolve using this wavelength, assuming the same distance as the Mount Palomar telescope. (The Hubble telescope's aperture diameter is 2.40 m.)
The wavelength is 568 nm. The Hubble telescope could resolve a crater with a diameter of approximately 108.6 m using this wavelength and assuming the same distance as the Mount Palomar telescope.
(a) To find the wavelength of light being used, we can use the angular resolution formula for a telescope:
θ = 1.22 * (λ/D)
where θ is the angular resolution, λ is the wavelength, and D is the diameter of the telescope. We know the diameter (D) of the Hale telescope is 5.08 m, and the smallest crater diameter it can resolve on the Moon is 54.2 m. We can use the small-angle approximation:
θ = crater diameter/distance to the Moon
θ = 54.2 m / 3.76 x 10^8 m ≈ 1.44 x 10^-7 rad
Now, we can solve for the wavelength (λ):
1.44 x 10^-7 rad = 1.22 * (λ / 5.08 m)
λ ≈ 5.68 x 10^-7 m
Converting to nanometers (1 m = 10^9 nm):
λ ≈ 568 nm
(b) To find the diameter of the crater that the Hubble telescope can resolve using the same wavelength, we use the same formula and the Hubble telescope's aperture diameter (D) of 2.40 m:
θ_Hubble = 1.22 * (568 nm / 2.40 m)
θ_Hubble ≈ 2.89 x 10^-7 rad
Now, we can use the small-angle approximation to find the diameter of the crater:
crater diameter = θ_Hubble * distance to the Moon
crater diameter ≈ 2.89 x 10^-7 rad * 3.76 x 10^8 m ≈ 108.6 m
So, the Hubble telescope could resolve a crater with a diameter of approximately 108.6 m using this wavelength and assuming the same distance as the Mount Palomar telescope.
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When a body changes we know that its momentum changes.
Answer:
ok
Explanation:
Answer:
The change of movement depends on the force that acts and the length of time it acts.
Limits of Lorentz contraction formula - L1/1- 3. In the theory of relativity, the Lorentz contraction formula v2 LU) = L01 c2 expresses the measured length (by an observer) L of an object as a function of its velocity v with respect to an observer, where Lo is the length of the object at rest, and c is the speed of light. (a) Using the limit laws, find limo+c- L. Justify each step of your work (and don't skip any steps!). (b) Interpret the result. (c) Why is a left-hand limit necessary?
A left-hand limit is required because the formula becomes a division by zero when the observer travels at the speed of light or faster than the speed of light.
The Limits of the Lorentz contraction formula are given by the following:(a) Using the limit laws, find limo+c-L.
Justify each step of your work (and don't skip any steps!).
lim (L1/√1 - (v/c)^2)
= L0l/sqrt(1) - (0)^2lim (L1/1 - 0)
= L0l/1 = L0 + c - L0= c(b)
Interpret the result.
The answer to (a) is c. The length of the moving object will appear to be shorter than the object's actual length, L0, when measured by an observer. As a result, when a moving object moves at a speed equal to the speed of light, it appears to be compressed to an infinite amount of time.
A left-hand limit is required because the formula becomes a division by zero when the observer travels at the speed of light or faster than the speed of light.
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PLEASE HELP MEE PLEASE I BEG
Explanation: (I think)
Plug your values into the momentum equation.
So m1= 63kg
m2 = 10 kg
V1 = 12 m/s
And then plug in your values and solve for your unknown (v2)
Transcribed image text: The position of a ball rolling in a straight line is given by x = 2.0 - 3.6t + 1.7t2 where x is in meters and t in seconds, (a) What do the numbers 2.0, 3.6, and 1.7 refer to? (b) What are the units of each of these numbers? (c) Determine the position of the ball at t = 1.0 s, 2.0 s, and 3.0 s. (d) What is the average velocity over the interval t = 1.0 s to t = 3.0 s? Essay answers are limited to about 500 words (3800 characters maximum, including spaces). 3800 Character(s) remaining
a) 2.0 represents the initial position of the ball, -3.6 represents the initial velocity of the ball and 1.7 represents the acceleration of the ball.
b)The unit of 2.0 is meters, the unit of -3.6 is meters per second, and the unit of 1.7 is meters per second squared.
c) Position of of ball at t=1, 2, 3 are -1.9, 5.4 and 9.1 meters respectively
d) Average velocity is 5.5 meter per second
Part a
In the equation x = 2.0 - 3.6t + 1.7t2, the number 2.0 represents the initial position of the ball (i.e., the position of the ball at t = 0 seconds), -3.6 represents the initial velocity of the ball (i.e., the velocity of the ball at t = 0 seconds), and 1.7 represents the acceleration of the ball.
Part b
The unit of 2.0 is meters, the unit of -3.6 is meters per second, and the unit of 1.7 is meters per second squared.
Part c
To determine the position of the ball at t = 1.0 s, 2.0 s, and 3.0 s, we simply substitute these values into the equation:
When t = 1.0 s: x = 2.0 - 3.6(1.0) + 1.7(1.0)^2 = -1.9 meters
When t = 2.0 s: x = 2.0 - 3.6(2.0) + 1.7(2.0)^2 = 5.4 meters
When t = 3.0 s: x = 2.0 - 3.6(3.0) + 1.7(3.0)^2 = 9.1 meters
Part d
The average velocity over the interval t = 1.0 s to t = 3.0 s can be calculated by taking the displacement of the ball during this time interval and dividing it by the time interval:
Displacement = x(3.0) - x(1.0) = 9.1 - (-1.9) = 11.0 meters
Time interval = 3.0 s - 1.0 s = 2.0 s
Average velocity = Displacement / Time interval = 11.0 meters / 2.0 seconds = 5.5 meters per second.
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What is the angular position in radians of the minute hand of a clock at 6:15?Express your answer with the appropriate units.What is the angular position in radians of the minute hand of a clock at 10:35?Express your answer with the appropriate units.
At 6:15, the minute hand's angular position is π/2 radians, and at 10:35, it is 7π/6 radians. The minute hand of a clock makes a full revolution in 60 minutes, which is equivalent to 2π radians.
To find the angular position of the minute hand at a specific time, we need to calculate the fraction of the 60-minute cycle that has elapsed and multiply it by 2π. For 6:15, the minute hand has moved 15 minutes out of 60, which is equivalent to three-fourths of the cycle. Therefore, its angular position is: (3/4) * 2π = (3/4) * 6.28 ≈ 4.71 radians
For 10:35, the minute hand has moved 35 minutes out of 60, which is equivalent to seven-twelfths of the cycle. Therefore, its angular position is:
(7/12) * 2π = (7/12) * 6.28 ≈ 3.65 radians
So the answer is 3.65 radians.
In summary, the angular position in radians of the minute hand of a clock at 6:15 is 4.71 radians, and at 10:35 is 3.65 radians.
At 6:15, the minute hand is at the 3 o'clock position, which corresponds to 90 degrees. To convert this to radians, use the formula: radians = (degrees * π) / 180. In this case, the angular position of the minute hand is (90 * π) / 180, which simplifies to π/2 radians. For the second scenario, at 10:35, the minute hand is at the 7 o'clock position, corresponding to 210 degrees. Using the same formula to convert degrees to radians, we have (210 * π) / 180, which simplifies to 7π/6 radians.
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13. A student wears eyeglasses of power P=-15 diopter to correct nearsightedness. The glasses are designed to be worn d 1.2 cm in front of the eye Randomized Variables p-.1.5 diopter d 1.2 cm ? 50% Part (a) Input an expression for the far point the student can see without correction, do. Grade Summary Deductions Potential 0% 100% Submissions Attempts remaining: 5 (500 per attempt) detailed view di DELI CLEAR Submit Hint I give up! Hints: 200 deduction per hint. Hints remaining:3 Feedback: 2% deduction per feedback. D ? 50% Part (b) Numerically, what is the distance in meters?
(a) The far point that the student can see without correction is 6.7 centimeters.
(b) To convert the distance to meters, we divide by 100, giving do = 0.067 meters.
This is given by the formula do = 1/f, where f is the focal length of the eye's lens. For a nearsighted person with eyeglasses of power P, the far point is given by do = -1/P. Therefore, substituting P = -15 diopter, we get do = -1/(-15) = 0.067 meters or 6.7 centimeters.
(b) To convert the distance to meters, we divide by 100, giving do = 0.067 meters. The negative sign indicates that the far point is in front of the eye, which is expected for a nearsighted person. The eyeglasses are designed to bring this far point to infinity, so the student can see distant objects clearly.
The focal length of the eye's lens is shorter than normal for a nearsighted person, which causes light from distant objects to converge in front of the retina instead of on it, resulting in blurred vision.
The eyeglasses of appropriate power are designed to diverge the light rays before they enter the eye, allowing them to focus correctly on the retina. The far point is the maximum distance at which the eye can see objects clearly without strain.
The negative sign in the answer indicates that the far point is a virtual image formed in front of the eye due to its abnormal focusing properties.
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Use the spherical wavefronts of Equations (2.9) to derive the Lorentz transformation given in Equations (2.17). Supply all the steps. x^2 + y^2 + z^2 = c^2 t^2 x'^2+ y^'2 + z^'2 = c^2 t^2 x' = x - vt/squareroot 1 - beta^2 y' = y z' = z t' = t - (vx/c^2)/squareroot 1 - beta^2
The Lorentz transformation is: x'² + y² + z'2 = c² t'²
The Lorentz transformation can be derived from spherical wavefronts given in Equations (2.9). To do so, we can use the following steps:
1. Start with the equation x²+ y² + z²= c²t²
2. Make the change x -> x' - vt/√(1-β²) and y -> y'
3. Inserting these values into the original equation gives us x'² + y'² + z² = c² t²
4. Next, make the change z -> z' and t -> t' - (vx/c²)/√(1-β²)
5. Inserting these values into the equation from Step 3 yields the Lorentz transformation: x'² + y'² + z'² = c² t²
This completes the derivation of the Lorentz transformation given in Equations (2.17) from spherical wavefronts given in Equations (2.9).
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a cell phone weighing 80 grams is flying throgh the air at 15 m/s what is the kentic energy
Answer:
kinetic energy: \(9\) Joules
Explanation:
\(Kinetic-Energy = \frac{1}{2} m v^2\)
Here the mass is 80 grams - which should be changed to kilograms
→ 1 kg ⇔ 1000 grams
→ 80 grams ⇔ 0.08 kg
Now using the formula:
\(\frac{1}{2} mv^2\)
\(\frac{1}{2} * 0.08 * 15^2\)
\(9\) Joules
Remember the mass should be in kg and velocity in meter per second.
initially, a bowl holds 15 m^3 of water. an object is dropped into the bowl and the new volume of the water is 25 m^3. what is the buoyant force?
Explanation:
The new volume of water = 25 ml
The old volume of water = 15 ml
The difference = 25 - 15 but what are the units?
Since the question asks for force, the units must start out as 10 mL
In water 1 mL has a mass of 1 gram, so the answer is 10 grams.
Grams are units of mass, not weight. You should convert this into newtons.
10 grams = 1/1000 = 0.01 kg
1 kg has a weight of 9.81 Newtons
0.01 kg has a weight 0.081 Newtons
If you have never seen a Newton before, then the answer is 10 grams
The pages of a book are numbered 1 to 200 and each
leaf is 0.10mm thick. If each cover is 0.20 mm thick, what
is the thickness of the book?
Answer:
10.4mm
Explanation:
2 pages = 1 leaf
200 pages = 100 leaves
100 × 0.10 = 10 mm thickness
Total thickness = 2(0.20) +10 = 0.4+10 = 10.4mm
Why is it important to wear loose-fitting clothing when exercising?
It isn't best to wear loose fitting clothing when exercising, as you may not feel too comfortable. It depends on the person. However there are a few advantages.
• Tight clothing may not be comfortable as well
• Looser clothing allows easy evaporation of sweat
Then again when it says " loose - fitting " it may mean not too baggy. Baggy clothing can have an impact on your physical activity.
Answer All of the above
For people on a p e x
in this guided lab you determined the approximate depth of the mt. vesuvius crater. (round your answers to the nearest whole number.) what is the depth of the crater in meters?
In Guided Lab 1, the distance from the center of the Mt. Vesuvius crater to the coast was found and it is approximately 7 kilometers.
The distance can be determined using different methods such as using a map and a ruler, using GIS software or a mapping website, such as Maps, or using a GPS device or smartphone app.
It is important to note that this distance may vary depending on the measurement method and location, and it should be a rough estimation.
Mt Vesuvius is an active volcano located on the east coast of the Italian Peninsula, southeast of Naples, it is one of the most dangerous volcanoes in the world due to its proximity to the city of Naples, it last erupted in 1944. The volcano has a crater that is about 800 meters wide and 140 meters deep.
To learn more about the distance at
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Which of the following vehicles has the most kinetic energy? A. a 300kg motorcycle traveling 60km/h B. a 1,100kg car traveling 60km/h C. a 900kg car traveling 80km/h D. a 2000kg truck traveling 50km/h
Explanation:
Kinetic energy of an object is given by :
\(E=\dfrac{1}{2}mv^2\)
Where
m is mass and v is velocity of the object
A. Mass, m = 300 kg.
Speed, v = 60 km/h = 16.67 m/s
\(E=\dfrac{1}{2}\times 300\times 16.67^2\\\\=41683.33\ J\)
B. Mass, m = 1100 kg.
Speed, v = 60 km/h = 16.67 m/s
\(E=\dfrac{1}{2}\times 1100\times 16.67^2\\\\=152838.89\ J\)
C. Mass, m = 900 kg.
Speed, v = 80 km/h = 22.22 m/s
\(E=\dfrac{1}{2}\times 900\times 22.22^2\\\\=222177.78\ J\)
D. Mass, m = 2000 kg.
Speed, v = 50 km/h = 13.88 m/s
\(E=\dfrac{1}{2}\times 2000\times 13.88^2\\\\=192654.4\ J\)
The kinetic energy in case C is maximum.