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MakcuM [25]
2 years ago
9

After a laser beam passes through two thin parallel slits, the first completely dark fringes occur at 19.0 with the original dir

ection of the beam, as viewed on a screen far from the slits. (a) What is the ratio of the distance between the slits to the wavelength of the light illuminating the slits
Physics
1 answer:
Katarina [22]2 years ago
8 0

Answer:

$\frac{d}{\lambda} = 1.54$

Explanation:

Given :

The first dark fringe is for m = 0

$\theta_1 = \pm 19^\circ$

Now we know for a double slit experiments , the position of the dark fringes is give by :

$d \sin \theta=\left(m+\frac{1}{2}\right) \lambda$

The ratio of distance between the two slits, d to the light's wavelength that illuminates the slits, λ :

$d \sin \theta=\left(\frac{1}{2}\right) \lambda$     (since, m = 0)

$d \sin \theta=\frac{\lambda}{2}$

$\frac{d}{\lambda} = \frac{1}{2 \sin \theta}$

$\frac{d}{\lambda} = \frac{1}{2 \sin 19^\circ}$

$\frac{d}{\lambda} = 1.54$

Therefore, the ratio is $\frac{1}{1.54}$  or 1 : 1.54

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Answer:

  • <u>233 N</u>

Explanation:

The balance condition, to keep the gate from moving, requires that the net torque be zero, this is, the torques on both sides of the gate must be equal.

  • Torque equation: τ = F × d

a) <u>Torque applied by one of the children:</u>

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b) <u>Torque applied by the second child</u>:

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c) <u>Equilibrium condition</u>:

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  • 170 N × 0.590m = F × 0.430m

  • F = 170 N × 0.590 m / 0.430 m = 233 N ← answer
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What are Alpha rays <br><br><br>please its aurgent ​
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2 years ago
Explain how energy balance sets planetary temperature? Imagine a planet colder than expected for energy balance and explain why
RUDIKE [14]

The planetary temperature energy balance is obtained by radiating back the absorbed radiation energy from outer-space, by the planet and thus acquiring thermal equilibrium.

What is the process of attaining thermal equilibrium by Earth?

The Stefan-Boltzmann law states that the more the temperature a planet has, the more it will radiate out to reach thermal equilibrium.

We know that outer space contains large masses of radiative energy freely distributed in its vast expanse. A small fraction of this energy is absorbed by the Earth through the atmosphere, surface land, clouds etc.

Now, radiative balance is achieved when a planet's surface continuously warms up until it reaches its peak at which point the same amount of absorbed energy can then be radiated back to space. The relative amount of energy radiated back by a planet is dependent upon the size of the planet.

A colder planet relatively absorbs lower amount of radiation energy from space. In some time, as the planet heats up enough, the energy is radiated back to the space attaining thermal equilibrium.

Learn more about Stefan-Boltzmann law here:

<u>brainly.com/question/14919749</u>

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1 year ago
Based on the information in the graph, why is energy released during the fusion of hydrogen (H) into helium (He)?
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Answer:

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The average velocity of blood flowing in a certain 4-mm-diameter artery in the human body is 0.28 m/s. The viscosity and density
OLga [1]

Answer:

V = 3.5 x 10⁻⁶ m³/s = 3.5 cm³/s

Explanation:

The volume flow rate of the blood in the artery can be given by the following formula:

V = Av

where,

V = Volume flow rate = ?

A = cross-sectional area of artery = πd²/4 = π(0.004 m)²/4 = 1.26 x 10⁻⁵ m²

v = velcoity = 0.28 m/s

Therefore,

V = (1.26\ x\ 10^{-5}\ m^2)(0.28\ m/s)

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3 years ago
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