As the speed of a fluid increases, ____.a. the pressure decreases
c. the force decreases
b. the pressure increases
d. the volume decreases

Answers

Answer 1
Answer: The correct answer for the question that is being presented above is this one: "a. the pressure decreases." As the speed of a fluid increases, the pressure decreases." The relationship of the speed and the pressure is inversely proportional. As the pressure increases, the speed decreases.
Answer 2
Answer:

I think the answer is A.


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Nicolaus Copernicus believed that the: sun revolved around the earth sun was the center of the solar system movement of planets could explain weather stars and planets represented spirits

Answers

Nicolaus Copernicus spearheaded the idea of heliocentrism, that is, that the sun was the center of the solar system. Back in his time, a lot of astronomers and scientists believed that the earth was the center of the solar system. This so called belief was called geocentrism. Nicolaus was one fo the first few who pushed heliocentrism.

Answer:

B. Sun was the center of the solar system.

You are asked to measure the density of a cube that has a side of 10 centimeters, and weighs 1 kg nominally. The tools you have are a ruler with the smallest reading at 1 mm, and a scale with a precision down to 0.1 g. Both tools are calibrated. Please estimate the final error on the density of the object that you measure. ​

Answers

Answer:

To estimate the final error on the density of the cube, we can consider the errors introduced by both the measurement of its volume and its weight.

1. Volume Measurement:

- The side length of the cube is given as 10 centimeters, and your ruler can measure to 1 mm accuracy.

- So, the error in measuring the side length is ±0.05 cm (half of the smallest measurement unit).

- To calculate volume, you need to cube the side length: Volume = (10 cm)^3 = 1000 cm^3.

- Using the error propagation rule, the relative error in volume is ±0.05 cm / 10 cm = ±0.005.

2. Weight Measurement:

- The weight is given as 1 kg nominally, which is equivalent to 1000 g.

- Your scale has a precision down to 0.1 g.

- So, the error in measuring the weight is ±0.1 g / 1000 g = ±0.0001 (0.01%) relative error.

Now, to calculate the final error in density, you need to consider both errors in volume and weight:

Density = Weight / Volume

Relative Error in Density = (Relative Error in Weight) + (Relative Error in Volume)

Relative Error in Density = (0.0001) + (0.005) = 0.0051 or 0.51%

So, the final estimated error on the density of the cube is approximately ±0.0051 g/cm^3 or ±0.51%.

Final answer:

The density of the cube is calculated using its mass and volume, with potential errors from the measurements of these quantities leading to a total estimated density error of approximately ±3.01%.

Explanation:

The density of an object is given by the formula density = mass/volume. In this case, the mass of the cube is given as 1 kg (or 1000 g for consistency with the scale's precision), and the volume of the cube can be calculated from the given side length using the formula for the volume of a cube, volume = side³, which equals 1000 cm³.

However, there are measurement errors associated with both the ruler and scale. The ruler can measure to the nearest mm (or 0.1 cm), so the error is ±0.1 cm on each measurement of the cube's sides, leading to a volume error of about ±3%. The scale can measure to the nearest 0.1 g, which gives a mass error of about ±0.01%. The total error in the density, obtained by summing these errors, is therefore approximately ±3.01%.

Learn more about Error Estimation here:

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An object falls freely from height H. if it takes one second to travel last half of total displacement find height H priop to the fall.​

Answers

Answer:9.82 m

Explanation:

As we know from equation of motion

S=v*t +0.5 a t^2

Know s=H/2

a =9.82

t=1

V=0

Plugging the values

H*0.5=0+0.5*9.82*1^2

H=9.82 m

Sandra's target heart rate zone is 135bpm—172bpm. Marissa's target heart rate zone is 143bpm—176bpm. They stop playing basketball and take their pulse, and both count the heart rate at 144bpm. If they decrease their heart rates by 20bpm, who will be in her THR zone?

Answers

Answer: Neither Sandra nor Marissa will be in her THR zone.


Explanation:


1) Actual pulse of both Sandra and Marissa : 144 bpm


2) Decrease of 20 bpm ⇒ 144 bpm - 20 bpm = 124 bpm


3) Sandra's TRH is in the range 135 - 172 bpm.


Since 124 < 135, she will be below the range.


4) Marissa's TRH range is 143 - 176 bpm.


Since, 124 < 143, she is below the range


In conlusion, neither Sandra nor Marissa will be in her THR zone.


Sandra's pulse is 144 bpm.  If she decreases it by 20 bpm,
it will be 124 bpm.  Her TRH is the range  of 135 - 172 bpm,
so she will be below it.

Marissa's pulse is 144 bpm.  If she decreases it by 20 bpm,
it will be 124 bpm.  Her TRH is the range  of 143 - 176 bpm,
so she will be below it.

Neither girl will be in her THR.

A person drops a brick from the top of a building. The height of the building is 400 m and the mass of the brick is 2.00 kg. What will be the speed of the brick right before it touches the ground? Use g=10.0 m/s^2.

Answers

This question involves the conservation of energy. There are two energy in this case, potential energy and kinetic energy. Let's divid the energy into three status. 
1. Before dropping, all potential energy 
2.dropping, potential energy transformed to kinetic energy
3. before hitting the ground, all Kinetic energy.

Recall the formula for both energy, which are U=mgh, and K=1/2mv^2

Since the energy is conserved in this case ( b/c otherwise it will say in the problem), the amount of energy at the beginning should equal to the energy at the end. Therefore we have, mgh=1/2mv^2

plug the number in and solve for velocity.

2x400x10=1/2 x 2 x v^2
v^2=8000
v=√(8000)
v=40√(5)

The term angle of deviation is used in reference to A. a polarizer.
B. a prism.
C. a lens.
D. an analyzer.

Answers

B. a prism.

This is because the term "angle of deviation" is used to describe the angle at which the light bends compared to the normal of the ray of light