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sergey [27]
3 years ago
10

Two blocks of masses mA and mB are connected by a massless spring. The blocks are moved apart, stretching the spring, and subseq

uently released from rest. Find (a) the ratio of velocities 7of the blocks at any point of their ensuing motion (when their velocities are non-zero) and (b) the ratio of the kinetic energies of the blocks.
Physics
1 answer:
WINSTONCH [101]3 years ago
7 0

Answer:

Part a)

\frac{v_A}{v_B} = -\frac{m_B}{m_A}

Part b)

\frac{K_A}{K_B} = \frac{m_B}{m_A}

Explanation:

Part a)

As we know that initially the two blocks are connected by a spring and initially stretched by some amount

Since the two blocks are at rest initially so its initial momentum is zero

since there is no external force on this system so final momentum is also zero

m_Av_{1i} + m_Bv_{2i} = m_Av_A + m_Bv_B

now for initial position the speed is zero

0 = m_Av_A + m_Bv_B

now we have

\frac{v_A}{v_B} = -\frac{m_B}{m_A}

Part b)

now for ratio of kinetic energy we know that the relation between kinetic energy and momentum is given as

K = \frac{P^2}{2m}

now for the ratio of energy we have

\frac{K_A}{K_B} = \frac{P^2/2m_A}{P^2/2m_B}

since we know that momentum of two blocks are equal in magnitude so we have

now we have

\frac{K_A}{K_B} = \frac{m_B}{m_A}

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The sun's intensity for an outer planet located at a distance 6r from the sun is 5.55 W/m². The result is obtained by using the inverse square law formula.

<h3>What is the Inverse Square Law formula?</h3>

The Inverse Square Law formula describes the intensity of light is inversely proportional to the square of the distance. It can be expressed as

\frac{I_{1} }{I_{2} } = \frac{d_{2}^{2} }{d_{1}^{2}}

Where

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  • I₂ = Intensity at distance 2 (W/m²)
  • d₁ = distance 1 from a light source (m)
  • d₂ = distance 2 from a light source (m)

Given the case the sun's intensity is 200 W/m² for an inner planet at the distance r. If an outer planet is at a distance 6r, what is the sun's intensity?

By using the inverse square law formula, the sun's intensity for an outer planet is

\frac{I_{1} }{I_{2} } = \frac{d_{2}^{2} }{d_{1}^{2}}

\frac{200 }{I_{2} } = \frac{(6r)^{2} }{r^{2}}

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Hence, the sun's intensity for a planet at a distance 6r from the sun is 5.55 W/m².

Learn more about intensity of light here:

brainly.com/question/13155277

#SPJ4

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