How long does it take an electron to complete a circular orbit perpendicular to a 1.4 g magnetic field?

=255 ns

The centripetal force of circular motion must be equal to the magnetic force:  

qvB = mv^2/r  

=> v/r = Bq/m  

Remember angular speed is:  

ω = v/r = 2π/T  

Where T is the period of a single orbit.

Thus:  

2π/T = B(q/m)  

=> T = 2π/(B(q/m))  

q/m = 1.76x10^11 C/kg for an electron, and

B = 1.4 G = 1.4 (1x10^-4) T = 1.4x10^-4 T (T in this case is obviously the SI unit Tesla, unrelated to the period T, sorry 'bout that).

So we have the period:

T = 2π/(1.4x10^-4 x 1.76x10^11)

   = 2.55 x10^-7 s  

   = 255 ns .

Therefore period is 255 ns

T = 2π/(1.4x10^-4 x 1.76x10^11) = 2.55x10^-7 s  

Explanation

1. The centripetal force must be equal.

The centripetal force of circular motion must be equal to the magnetic force hence:

qvB = mv^2/r  

v = (qBr)/m  

Since angular speed is: ω = v/r = 2π/T  

2. v = 2πr/T  

Where T is the period of a single orbit. Thus substituting equation 2 in equation 1 and making T the subject:

3. T = 2π/(B(q/m))  

Substituting B = 1.4 G => 1.4 x 10^-4 T

and q/m = 1.76x10^11 C/kg in equation 3

T = 2π/(1.4x10^-4 x 1.76x10^11) = 2.55x10^-7 s  

hi,

what occurs during a solar eclipse?

there are small tides across earth.

the moon is between earth and the sun.

p.s. im not sure if the first answer is correct because during a solar ecliphse there are spring tides and i dont know if they are the same.