Math Problem Statement
Compute the energy per cm squared for a ideal blackbody at 300K
Compute the energy a photon at 0.55 microns carries
Compute the number of photons from an LED emitting 10W of light at 0.65 microns (see the in class example from Week 2)
Compute the average emissivity of an opaque object with an average albedo of 0.5 in the visible spectrum
Compute the peak wavelength for a blackbody at 2000K, 5000K, and 10000
Solution
Let's compute each of these values step by step:
1. Energy per cm² for a blackbody at 300 K
We can use the Stefan-Boltzmann law to calculate the energy per unit area emitted by a blackbody: Where:
- is the Stefan-Boltzmann constant,
Since the question asks for energy per cm², we need to convert the result from m² to cm² (1 m² = 10,000 cm²).
Let me compute this for you.
2. Energy of a photon at 0.55 microns
The energy of a photon is given by: Where:
- is Planck's constant
- is the speed of light
- is the wavelength
Substitute the values into the equation to find the energy.
3. Number of photons from an LED emitting 10W of light at 0.65 microns
First, we calculate the energy of a single photon at 0.65 microns using the same formula: Where .
Next, we calculate the total number of photons emitted
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Math Problem Analysis
Mathematical Concepts
Thermodynamics
Photon Energy
Blackbody Radiation
Electromagnetic Spectrum
Albedo and Emissivity
Formulas
Stefan-Boltzmann law: E = σT^4
Photon energy: E = hc / λ
Emissivity: ε = 1 - albedo
Wien's displacement law: λ_max = b / T
Theorems
Stefan-Boltzmann law
Wien's displacement law
Suitable Grade Level
Undergraduate Physics
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