Question

The star Rigel in the constellation Orion (the Hunter) emits its greatest intensity of radiation at...

The star Rigel in the constellation Orion (the Hunter) emits its greatest intensity of radiation at a wavelength of 239 nm.

a) Calculate the surface temperature of the star.

b) What colour is the star? Explain your answer.

Homework Answers

Answer #1

a) Solution :

From Wien's displacement law T = constant = 0.0029 mK

where = wavelength of greatest intensity of radiation = 239 nm = 239 x 10 ^-9 m

and T = surface temperature in kelvin (K)

so T = 0.0029 / = 0.0029 /(239 x 10 ^-9 ) =

so surface temperature of the star

Answer:

b) Solution:

As = 239 nm so the star cannot be seen with bare  eyes  ( visible range 380nm to 740nm )

as the wavelenght of the star lies in ultraviolet region (10 nm to 400 nm ) So the colour of the star is ultraviolet ( which cannot be seen with bare eyes)

Answer : Ultraviolet.

Thank You.

Know the answer?
Your Answer:

Post as a guest

Your Name:

What's your source?

Earn Coins

Coins can be redeemed for fabulous gifts.

Not the answer you're looking for?
Ask your own homework help question
Similar Questions
A particular star has a radius of 8.58 ✕ 108 m. The peak intensity of the...
A particular star has a radius of 8.58 ✕ 108 m. The peak intensity of the radiation it emits is at a wavelength of 682 nm. (a) What is the energy (in J) of a photon with this wavelength? J (b) What is the star's surface temperature (in K)? (Round your answer to at least the nearest integer.) K (c) At what rate (in W) is energy emitted from the star in the form of radiation? Assume the star is...
The star Rigel acts like a Blackbody. Its surface temperature is 10,000k A) Calculate the total...
The star Rigel acts like a Blackbody. Its surface temperature is 10,000k A) Calculate the total power per unit area emitted by Rigel B) Calculate the wavelength of peak intensity for Rigel's blackbody spectrum. C) Calculate the energy of a photon of wavelength given in B) above.
The human eye is most sensitive over the same wavelength range at which the Sun emits...
The human eye is most sensitive over the same wavelength range at which the Sun emits its greatest intensity of radiation. Suppose creatures were to evolve on a planet orbiting a star somewhat colder than the Sun. To what wavelengths would their vision most likely be sensitive? Explain your reasoning.
Suppose a star with radius 8.50 × 108 m has a peak wavelength of 685 nm...
Suppose a star with radius 8.50 × 108 m has a peak wavelength of 685 nm in the spectrum of its emitted radiation. Assume the star is a perfect blackbody. (A) What is the energy of a photon with this wavelength? (B) What is the surface temperature of the star? (C) At what rate is energy emitted from the star in the form of radiation?
23.   Photons and Energy      A. A certain source emits radiation of wavelength 500.0 nm. Determine...
23.   Photons and Energy      A. A certain source emits radiation of wavelength 500.0 nm. Determine its frequency. Calculate the energy associated with this photon at 500.0 nm.    B. If it takes 3.36 x 10-19 J of energy to eject an electron from the surface of a certain metal, Calculate the frequency of this energy and the longest possible wavelength in nm.       C. Ionization energy is the energy required to remove an electron from an atom in...
Chapter 14 The Size of Stars 10 of 11 Constants The hot glowing surfaces of stars...
Chapter 14 The Size of Stars 10 of 11 Constants The hot glowing surfaces of stars emit energy in the form of electromagnetic radiation. It is a good approximation to assume that the emissivity e is equal to 1 for these surfaces. Part A Find the radius RRigel of the star Rigel, the bright blue star in the constellation Orion that radiates energy at a rate of 2.7×1031W and has a surface temperature of 11,000 K. Assume that the star...
You measure the maximum wavelength of the radiation from a star as 547.0 nm, and the...
You measure the maximum wavelength of the radiation from a star as 547.0 nm, and the radius of the star to be 5.1 ×108m×108m. Find the total power emitted by the star in Watts, assuming it is a perfect black-body emitter. Use 2 sf in your answer. Hint: Use Wien's Law to find the temperature, and then Stefan's Law. You can assume the star is a sphere.
Thermal radiation: Mostly based on Section 5.4. i) Draw by hand the curves for thermal radiation...
Thermal radiation: Mostly based on Section 5.4. i) Draw by hand the curves for thermal radiation for a star like the Sun and the Earth. The x-axis is wavelength and the y-axis is intensity/power (you do not need to put numbers on your plot). Please explain the dierence in the two curves based on Wien's Law and the Stefan-Boltzman law. ii) The Earth produces thermal radiation at night. Take the temperature at the surface to be 50 F or about...
1. What is the peak wavelength emitted by a star with a surface temperature of 7070...
1. What is the peak wavelength emitted by a star with a surface temperature of 7070 K? Give your answer in nm (1 nm = 10-9 m), but enter only the numerical part in the box. 2. By how much would a star's temperature need to increase in order for its peak wavelength to decrease from 460 to 360 nm? Your answer will be the change in temperature. Give your answer in K, but enter only the numerical part in...
A small laser emits light at power 6.88 mW and wavelength 441 nm. The laser beam...
A small laser emits light at power 6.88 mW and wavelength 441 nm. The laser beam is focused (narrowed) until its diameter matches the 1255 nm diameter of a sphere placed in its path. The sphere is perfectly absorbing and has density 4.00×103kg/m3. What is the beam intensity at the sphere's location? Calculate the radiation pressure on the sphere. Calculate the magnitude of the corresponding force. Calculate the magnitude of the acceleration that force alone would give the sphere?
ADVERTISEMENT
Need Online Homework Help?

Get Answers For Free
Most questions answered within 1 hours.

Ask a Question
ADVERTISEMENT