The peak wavelength for Betelgeuse is 828 nm
Explanation:
Wien's law describes how the surface temperature relates to a star’s peak wavelength:
where
represents the peak wavelength
T is the surface temperature
is Wien's constant
For Betelgeuse, the surface temperature is roughly
T = 3500 K
Consequently, its peak wavelength can be determined as:
Learn more about wavelength:
Answer:
20.353125 V
Explanation:
m = Mass of proton =
q = Charge of proton =
= Velocity of proton at point A = 50 km/s
= Velocity of proton at point B = 80 km/s
The relationship derived from energy conservation is as follows:
The determined potential difference is 20.353125 V
Solution:
/ Em₀ = 0.30
Explanation:
In this problem, we apply the connection between mechanical energy, kinetic energy, and gravitational potential energy.
K = ½ m v²
U = mgh
We assess the mechanical energy at two positions:
Initial. Lower
Em₀ = K = ½ m v²
At its highest point
= U = mg and
Now let's compute
Em₀ = ½ m 3.6²
Em₀ = m 6.48
= m 9.8 × 0.2
= m 1.96
Thus the energy lost is given by:
/ Em₀ = m 1.96 / m 6.48
/ Em₀ = 0.30
This means that 30% of the sun's energy is transformed into potential energy.
There are various conversion possibilities.
This energy changes into thermal energy affecting the spores and air, since it cannot be regained.