Question

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 the box.

3. By what factor would a star's radiated power per square meter of surface area increase as a result of its temperature increasing such that its peak wavelength emitted at its surface went from 510 to 360 nm? Your answer will be unitless (it's a ratio).

Homework Answers

Answer #1

Hello Dear,

Hope this helps.. cheers

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...
A star whose surface temperature is 4000 K has a peak wavelength of 725 nm, according...
A star whose surface temperature is 4000 K has a peak wavelength of 725 nm, according to Wien’s Law. If this star is in the Andromeda Galaxy, which is moving toward Earth at about 120 km/s, what would an observer on Earth see as the peak wavelength for this star?
Infrared observations of a star show that it is most intense at a wavelength of 920...
Infrared observations of a star show that it is most intense at a wavelength of 920 nm (9.20  102 nm). What is the temperature of the star's surface? _________________________K If one star has a temperature of 6300 K and another star has a temperature of 7800 K, how much more energy per second will the hotter star radiate from each square meter of its surface? ______________________________times
A star has a surface temperature of 4500 K. a. Calculate the peak wavelength of its...
A star has a surface temperature of 4500 K. a. Calculate the peak wavelength of its brightness vs. wavelength curve. [1.5 points] b. What color does this wavelength correspond to? (Note: See p. 5-7 of the textbook for a list of colors corresponding to different wavelength ranges. If the wavelength is in the infrared or ultraviolet range, state “IR” or “UV” as the color.) [0.5 points] c. Now imagine that the star is moving away from us at 0.15c, where...
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?
The wavelength of peak emission from any star is related to the temperature of its photosphere...
The wavelength of peak emission from any star is related to the temperature of its photosphere (i.e., the emitting surface) by Wien’s Law, given by λ = 2,900/T, where λ is the wavelength in micrometers (1 µm = 10-6 m), and T is the temperature of the star in Kelvin (see textbook’s figure 3.27 for help). Answer the following questions using the above equation. 2.1. The most massive star ever observed is a Wolf-Rayet type-star, named R136a1. It is so...
As the temperature of a backbody increases, the wavelength of the peak in the emitted intensity...
As the temperature of a backbody increases, the wavelength of the peak in the emitted intensity remains the same. shifts to higher values. shifts to lower values. becomes unstable. QUESTION 2 Max Planck discovered the theoretical reasoning necessary to understand the spectrum of the electromagnetic radiation emitted by a blackbody. What was this reasoning based on? A careful consideration of the possible physical effects. Guessing until he found an expression which led to the correct result. Don't select this answer....
What is the peak wavelength of light coming from a star with a temperature of 10,250...
What is the peak wavelength of light coming from a star with a temperature of 10,250 k? (submit your answer in nanometers. Remember 1nm=10^-9m)
Parallax angle for a star is 195 mas. Its surface temperature is 7500 K and diameter...
Parallax angle for a star is 195 mas. Its surface temperature is 7500 K and diameter of 4 times solar radius. Calculate apparent magnitude , absolute magnitude, luminosity, wavelength of peak emission and flux received on surface of the earth.
The sun is a main sequence G5 type star with a surface temperature TMS = 5800...
The sun is a main sequence G5 type star with a surface temperature TMS = 5800 K. When the sun exhausts its Hydrogen supply it will evolve into a red giant with a surface temperature TRG = 3000 K and a radius of 100 times its present value. What is the peak wavelength of the sun in its main sequence and red giant phases? How many times larger will the sun’s radiative power be in the red giant phase? Assume...