Question

The Sun’s surface temperature is about 5800 K and its spectrum peaks at 5000 Å. An O-type star’s surface temperature may be 40,000 K. (a) According to Wien’s law, at what wavelength does its spectrum peak? (b) In what part of the spectrum might that peak be? (c) Can the peak be observed with the Keck telescopes on Maunakea in Hawaii? Explai

Answer 1

(a)
`7.25\cdot 10^(-8)m`

Wien's displacement law is summarized by the equation

`\lambda = (b)/(T)`

where

`\lambda` is the peak wavelength

`b=2.898\cdot 10^(-3) m \cdot K` is Wien's displacement constant

T is the absolute temperature at the surface of the star

For an O-type star, we have

T = 40,000 K

Therefore, its peak wavelength is

`\lambda = (2.898\cdot 10^(-3))/(40000)=7.25\cdot 10^(-8)m`

(b) Ultraviolet

We can answer this part by looking at the wavelength range of the different parts of the electromagnetic spectrum:

gamma rays
`<10^(-12)m`

X-rays 1 nm - 1 pm

ultraviolet 380 nm - 1 nm

visible light 750 nm - 380 nm

infrared
`25 \mu m - 750 nm`

microwaves 1 mm -
`25 \mu m`

radio waves > 1 mm

The peak wavelength of this star is

`\lambda=7.25\cdot 10^(-8)m=72.5 nm`

Therefore, it falls in the ultraviolet region.

(c) No

The Keck telescopes is actually a system of 2 telescopes in the Keck Observatory, located in Mauna kea, Hawai.

The two telescopes, thanks to several instruments, are able to detect much of the electromagnetic radiation in the visible ligth and infrared parts of the spectrum. However, they are not able to detect light in the ultraviolet region: therefore, they cannot observe the star mentioned in the previous part of the problem.