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faltersainse [42]
3 years ago
14

The gravitational force of attraction be-

Physics
1 answer:
Sliva [168]3 years ago
4 0

Answer:

2.15 m

Explanation:

Newton's Law of Universal Gravitation:

\displaystyle F_g = G \frac{m_1 m_2}{r^2}  

  • \displaystyle F_g is the gravitational force of attraction
  • \displaystyle G is the universal gravitational constant
  • m_1 and m_2 are the two masses of the two objects
  • \displaystyle r is the distance between the centers of the two objects.

List the known values:

  • \displaystyle F_g = 3.47 \cdot 10^-^8 \ \text{N}  
  • \displaystyle G = 6.673 \cdot 10^-^1^1 \ \frac{Nm^2}{kg^2}
  • \displaystyle m_1 = 44.8 \ \text{kg} \\ m_2 = 53.9 \ \text{kg}
  • \displaystyle r =\ ?

Plug these values into the equation:

  • \displaystyle 3.47 \cdot 10^-^8 \ \text{N} = 6.673 \cdot 10^-^1^1 \ \frac{Nm^2}{kg^2} \frac{(44.8 \ \text{kg})(53.9 \ \text{kg})}{r^2}

Notice that the units \displaystyle \text{N}, \displaystyle \text{kg}^2, and \displaystyle \text{m} cancel out. We are left with the unit \displaystyle \text{m} for radius r.

Get rid of the units to make the problem easier to read.

  • \displaystyle 3.47 \cdot 10^-^8= 6.673 \cdot 10^-^1^1 \ \frac{(44.8)(53.9) \ }{r^2}  

Multiply the masses together.

  • \displaystyle 3.47 \cdot 10^-^8= 6.673 \cdot 10^-^1^1 \ \frac{(2414.72)}{r^2}

Multiply the gravitational constant and the masses together.

  • \displaystyle 3.47 \cdot 10^-^8= \frac{1.61134265\cdot 10^-^7}{r^2}

Solve for r^2 by dividing both sides by 3.47 * 10^(-8) and moving r^2 to the left.

  • \displaystyle r^2 = \frac{1.61134265\cdot 10^-^7}{3.47\cdot 10^-^8}
  • r^2 = 4.64363876

Take the square root of both sides.

  • r=2.154910383  

The students are sitting about 2.15 m apart from each other.

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Calculate the energy, wavelength, and frequency of the emitted photon when an electron moves from an energy level of -3.40 eV to
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Answer:

(a) The energy of the photon is 1.632 x 10^{-8} J.

(b) The wavelength of the photon is 1.2 x 10^{-17} m.

(c) The frequency of the photon is 2.47 x 10^{25} Hz.

Explanation:

Let;

E_{1} = -13.60 ev

E_{2} = -3.40 ev

(a) Energy of the emitted photon can be determined as;

E_{2} - E_{1} = -3.40 - (-13.60)

           = -3.40 + 13.60

           = 10.20 eV

           = 10.20(1.6 x 10^{-9})

E_{2} - E_{1} = 1.632 x 10^{-8} Joules

The energy of the emitted photon is 10.20 eV (or 1.632 x 10^{-8} Joules).

(b) The wavelength, λ, can be determined as;

E = (hc)/ λ

where: E is the energy of the photon, h is the Planck's constant (6.6 x 10^{-34} Js), c is the speed of light (3 x 10^{8} m/s) and λ is the wavelength.

10.20(1.6 x 10^{-9}) = (6.6 x 10^{-34} * 3 x 10^{8})/ λ

λ = \frac{1.98*10^{-25} }{1.632*10^{-8} }

  = 1.213 x 10^{-17}

Wavelength of the photon is 1.2 x 10^{-17} m.

(c) The frequency can be determined by;

E = hf

where f is the frequency of the photon.

1.632 x 10^{-8}  = 6.6 x 10^{-34} x f

f = \frac{1.632*10^{-8} }{6.6*10^{-34} }

 = 2.47 x 10^{25} Hz

Frequency of the emitted photon is 2.47 x 10^{25} Hz.

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Answer:

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Explanation:

Given the parallex of the star is 0.1 sec.

The distance is inversely related with the parallex of the star. Mathematically,

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Here, d is the distance to a star which is measured in parsecs, and P is the parallex which is measured in arc seconds.

Now,

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And also know that,

1 parsec=3.086\times 10^{13} km

Therefore the distance of the star  is 30.86\times 10^{13} km away.

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