Radio astronomers detect electromagnetic radiation at 50.0 MHz from an interstellar gas cloud. They suspect this radiation is emitted by electrons spiraling in a magnetic field. What is the magnetic field strength inside the gas cloud?

Respuesta :

Answer:

0.00178 T

Explanation:

f = Frequency = 50 MHz

m = Mass of electron = [tex]9.11\times 10^{-31}\ kg[/tex]

q = Charge of electron = [tex]1.6\times 10^{-19}\ C[/tex]

In circular motion the magnetic field is given by

[tex]B=\dfrac{2\pi fm}{q}\\\Rightarrow B=\dfrac{2\pi 50\times 10^6\times 9.11\times 10^{-31}}{1.6\times 10^{-19}}\\\Rightarrow B=0.00178\ T[/tex]

The magnetic field strength inside the gas cloud is 0.00178 T

The magnetic field strength inside the interstellar gas cloud is 1.79 × 10⁻³T.

Given the data in the question;

Frequency; [tex]f = 50.0 MHz = 5.0 * 10^7 Hz[/tex]

To get the magnetic field strength inside the gas cloud, we use the expression for the frequency of the cyclotron:

[tex]f = \frac{qB}{2\pi m}[/tex]

Where;

  • f is the frequency
  • q is the charge of the electron ( [tex]1.602*10^{-19} C[/tex] )
  • m is the mass of electron ( [tex]9.11*10^{-31} kg[/tex] )
  • B is the Electric Field

Let make "B" the subject of the formula

[tex]B = \frac{2\pi fm }{q}[/tex]

We substitute our values into the equation

[tex]B= \frac{2*\pi * ( 5.0*10^7Hz)* (9.11*10^{-31}kg)}{1.602*10^{-19C}}\\\\B = \frac{2.86199*10^{-22}Kg.Hz}{1.602*10^{-19C}}\\\\B = 1.79 * 10^{-3}T[/tex]

Therefore, the magnetic field strength inside the interstellar gas cloud is 1.79 × 10⁻³T.

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Universidad de Mexico