Question

3. A star in a distant galaxy approaches the Sun at 3 X 10? m/s. It emits a photon with a wave- length of 0.4 microns. Apply the Doppler Effect to estimate the observed wavelength of this pho- ton. 4. An object is 2 meters from a thin lens with a focal length of 50 cm. Apply the thin-lens equa- tion to calculate the image distance from the lens and magnification.

          3. A star in a distant galaxy approaches the Sun at 3 X 10? m/s. It emits a photon with a wave-
length of 0.4 microns. Apply the Doppler Effect to estimate the observed wavelength of this pho-
ton.

4. An object is 2 meters from a thin lens with a focal length of 50 cm. Apply the thin-lens equa-
tion to calculate the image distance from the lens and magnification.

3. A star in a distant galaxy approaches the Sun at 3 X 10? m/s. It emits a photon with a wave-
length of 0.4 microns. Apply the Doppler Effect to estimate the observed wavelength of this pho-
ton.

4. An object is 2 meters from a thin lens with a focal length of 50 cm. Apply the thin-lens equa-
tion to calculate the image distance from the lens and magnification.

Added by Kevin W.

University Physics with Modern Physics

Hugh D. Young 14th Edition

Instant Answer

Solved by Expert Penny Riley

04/12/2022

Step 1

Given: - Wavelength of emitted photon (λ₀) = 0.4 microns - Speed of star approaching the Sun (V) = 3 x 10^6 m/s - Speed of light (c) = 3 x 10^8 m/s Using the Doppler effect formula: Δλ = λ₀ * V / c Plugging in the values: Δλ = 0.4 * (1 + 3 x 10^6 / 3 x Show more…

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3. A star in a distant galaxy approaches the Sun at 3 X 106 m/s. It emits a photon with a wave- length of 0.4 microns. Apply the Doppler Effect to estimate the observed wavelength of this pho- ton. 4. An object is 2 meters from a thin lens with a focal length of 50 cm. Apply the thin-lens equa- tion to calculate the image distance from the lens and magnification.