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sveta [45]
4 years ago
7

Kepler's third law relates the period of a planet

Physics
1 answer:
sammy [17]4 years ago
6 0

Answer:

√(r³ / (MG))

Explanation:

The dimensions of each variable are:

r = [m]

G = [m³/kg/s²]

M = [kg]

Multiplying M and G eliminates kilograms:

MG = [m³/s²]

The radius cubed divided by MG eliminates meters:

r³ / (MG) = [s²]

The square root gives us seconds:

√(r³ / (MG)) = [s]

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You’ll need 4H20 molecules to balance the equation.
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The tendency of an object to resist a change in its motion
Olenka [21]

Answer:

Inertia Newtons First law

Explanation:

 

3 0
3 years ago
A tortoise and hare start from rest and have a race. As the race begins, both accelerate forward. The hare accelerates uniformly
never [62]

Answer:

1) Vf = 3.36 m/s

2) v = 6.86 m/s

3) s = 92.3 m

4) a = - 0.23 m/s²

Explanation:

1)

We use first equation of motion in this case:

Vf = Vi + at

where,

Vf = Final velocity = ?

Vi = Initial velocity = 0 m/s

a = acceleration = 1.4 m/s²

t = time = 2.4 s

Therefore,

Vf = 0 m/s + (1.4 m/s²)(2.4 s)

<u>Vf = 3.36 m/s</u>

2)

We again use first equation of motion but with t= 4.9 s now:

Vf = 0 m/s + (1.4 m/s²)(4.9 s)

Vf = 6.86 m/s

Now, this velocity remained constant for net 11 seconds. Hence, the velocity of hare after 8.9 s is:

<u>v = 6.86 m/s</u>

3)

First we use second equation of motion to find distance covered in accelerated motion:

s₁ = Vi t + (0.5)at²

s₁ = (0 m/s)(4.9 s) + (0.5)(1.4 m/s²)(4.9 s)²

s₁ = 16.8 m

Now, we calculate the distance covered in uniform motion:

s₂ = vt

s₂ = (6.86 m/s)(11 s)

s₂ = 75.5 m

Now, total distance covered before slowing down is given as:

s = s₁ + s₂ = 16.8 m + 75.5 m

<u>s = 92.3 m</u>

3)

Using third equation of motion for the decelerated motion:

2as = Vf² - Vi²

where,

a = deceleration = ?

s = distance covered = 102 m

Vf = Final Speed = 0 m/s

Vi = Initial Speed = 6.86 m/s

Therefore,

(2)(a)(102 m) = (0 m/s)² - (6.86 m/s)²

a = - (47.06 m²/s²)/(204 m)

<u>a = - 0.23 m/s²</u>

3 0
4 years ago
A person, whose eye has a lens-to-retina distance of 2.0 cm, can only clearly see objects that are closer than 1.0 m away. what
shutvik [7]

To calculate the strength of the eye lens, we use the formula

\frac{P}{100} = \frac{1}{f} =\frac{1}{u} +\frac{1}{v}  ( thin lens formula)

Here, u is the object distance and v is image distance.

Given, u =1 m=100cm and v = 2 cm

Therefore,

\frac{1}{f} =\frac{1}{100} + \frac{1}{2}

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Thus, strength of the eye lens is

P= \frac{100}{f} =\frac{100}{\frac{1}{0.51} } = 51 D



5 0
3 years ago
A monochromatic light passes through a narrow slit and forms a diffraction pattern on a screen behind the slit. As the slit widt
Musya8 [376]

As the slit width increases, the diffraction pattern gets narrower and vice versa.

<h3>Relationship between width and diffraction pattern</h3>

The increase in silt width leads to the narrowing of diffraction pattern of the  light because the increase of width reduces the space for the passing of light wave.

So we can conclude that as the slit width increases, the diffraction pattern gets narrower and vice versa.

Learn more about diffraction here: brainly.com/question/16749356

3 0
2 years ago
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