which situation involves shear? a. convergent boundaries b. isolated rift valleys c. volcanic mountain ranges d. frequent shallow earthquakes e. new rock formations

Answers

Answer 1
Answer:

Answer:

Frequent shallow earthquakes

Explanation:

Shear is the response of a rock to deformation usually by compressive stress and forms particular textures.

During an earthquake when the earth shakes it produces a super shear earthquake in which the propagation of the rupture along the fault surface occurs at speeds in excess of the seismic shear wave (S-wave) velocity.

The mechanisms of shearing depend on the pressure and temperature of the rock and on the rate of shear which the rock is subjected to.


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The tip of a fan blade is 0.61 m from the center of the fan. The fan turns at a constant speed and completes 2 rotations every 1.0 second. What is the centripetal acceleration of the tip of the fan blade? Option 1: 6.0 m/s² Option 2: 48 m/s² Option 3: 53 m/s² Option 4: 96 m/s²

Answers

Answer: Here's my answer, I made it step-by-step so you can understand it! <3

Explanation:

To find the centripetal acceleration of the tip of the fan blade, we can use the formula for centripetal acceleration:

a = (v^2) / r

where:

a is the centripetal acceleration,

v is the linear velocity, and

r is the radius of the circular path.

Given that the fan completes 2 rotations every 1.0 second, we can find the angular velocity (ω) using the formula:

ω = (2π * n) / t

where:

ω is the angular velocity,

π is a constant (approximately 3.14),

n is the number of rotations (2),

and t is the time taken (1.0 second).

Substituting the values into the formula, we have:

ω = (2π * 2) / 1.0 = 4π rad/s

Next, we can calculate the linear velocity (v) using the formula:

v = r * ω

Substituting the given radius value (0.61 m) and the angular velocity we found earlier, we have:

v = 0.61 * 4π = 2.44π m/s

Finally, we can calculate the centripetal acceleration (a) using the formula:

a = (v^2) / r

Substituting the linear velocity and the radius, we have:

a = (2.44π)^2 / 0.61 = 5.88π^2 / 0.61 ≈ 96 m/s²

Therefore, the centripetal acceleration of the tip of the fan blade is approximately 96 m/s² (Option 4).

Make a island with all renewable energy soursws and how it works and about it but at year 9 level​

Answers

Answer:

How are we expected to make an island

What kinds of space and matter can light travel through?

Answers

Answer:

Every material and the void.

Explanation:

Light is a kind of electromagnetic wave and electromagnetic waves do not need a medium to propagate itself. Light can travel through every medium and even in void.

A skier is skiing down a slope on the mountain. Is the mechanical energy conserved? Why or why not?

Answers

yes, because mechanical energy is your total amount of energy when you add Potential and Kinetic energy together

Venus's average distance from the sun is 0.72 AU and Saturn's is 9.54 AU. Calculate the orbital velocity of Venus and Saturn around the sun. (The mass of the sun is 1.99 X 10^30 KG. an AU is 1.50 X 10^11 M.

Answers

The orbital velocity of Venus and Saturn around the sun is 8.854 x 10^8.

What is orbital velocity?

Orbital velocity is the speed required to achieve orbit around a celestial body, such as a planet or a star.

So you can compute the force of gravity on the planet

GMm/r^2

or

(6.674 * 10^(-11))(1.99 * 10^(30))m / d^2(1.5 * 10^(11))^2

Where d is the average distance of the planet from the sun and m is the mass of the planet (I will keep these as symbols so doing Saturn and Venus will be simple substitutions into one formula in the end).

Now realize that if they are in a stable circular orbit, then this force must provide the necessary centripetal force mv^2/r or mv^2 / d(1.5 * 10^(11))

So we get:

(6.674 * 10^(-11))(1.99 * 10^(30))m / d^2(1.5 * 10^(11))^2 = mv^2 / d(1.5 * 10^(11))

The m's cancel out as does one

1/d(1.5 * 10^(11))(6.674 * 10^(-11))(1.99 * 10^(30)) / d(1.5 * 10^(11)) = v^2

Evaluating and square rooting yeilds:

v = √(((8.854 * 10^8)/d))

Now plug in 0.72 for venus and 9.54 for saturn

Venus = 35067.39 m/s

Saturn = 9633.75 m/s

Some precision was lost rounding to 8.854 x 10⁸, so if more precision is required type the whole thing from before into a calculator. Anyways the process is sound.

Learn more about orbital velocity here:

brainly.com/question/24152628

#SPJ2

So you can compute the force of gravity on the planet GMm/r^2
or (6.674 X 10^−11)(1.99 X 10^30)m / d^2(1.5 X 10^11)^2
Where d is the average distance of the planet form the sun and m is the mass of the planet (I will keep these as symbols so doing Saturn and Venus will be simple substitution into one formula in the end).

Now realize that if they are in stable circular orbit, then this force must provide the necessary centripetal force mv^2/r or mv^2 / d(1.5 X 10^11)

So we get:

(6.674 X 10^−11)(1.99 X 10^30)m / d^2(1.5 X 10^11)^2 = mv^2 / d(1.5 X 10^11)
The m's cancel out as does one 1/d(1.5 X 10^11)
(6.674 X 10^−11)(1.99 X 10^30) / d(1.5 X 10^11) = v^2
Evaluating and square rooting yeilds:
v = sqrt((8.854 X 10^8)/d)

Now plug in 0.72 for venus and 9.54 for saturn

Venus = 35067.39 m/s
Saturn = 9633.75 m/s

Some precision was lost rounding to 8.854 X 10^8, so if more presion is required just type the whole thing from before into a calculator.  Anyways the process is sound

You are sitting in a chair on an elavator. The elavator accelerates downward, you and the chair land on the cround with the chair landing first and then you on the chair.Explain the Net Forces at 3 points for each object

The points are: Before the Elevator Accelerates Downward, In Freefall, At Impact

Analyze whether the Normal Force would need to increase, and where the direction of the net force is for each object.

Answers

Answer:

fdsbgdfshtrsnbfgsbnhgr

Explanation:

cdfrgresgtrshtrwhtrwhtwjhdgngdabfeahydrtgnb