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x | New tab x | 4 Home | Mt. San Antonio College X Files X DE Blackbody Radiation Sheet.pdf X + Users/cryst/Downloads/Blackbody%20Radiation%20Sheet.pdf 2 | | A | at | Ask Copilot 2 of 4 | 2 | CD The two most important features of a star's spectral curve (also known as a blackbody curve) are: . its maximum height or peak - where the energy output is greatest; and . the corresponding wavelength at which this peak occurs - which indicates the star's temperature. If the peak occurs at a long wavelength the star is cooler than a star that gives off most of its light (peaks) at a shorter wavelength. For example, if Star E and Star F are the same size and temperature, they will have identical blackbody curves. However, if Star F is the same size as star E, but is cooler, its energy output is less at all wavelengths and the peak occurs at a longer wavelength (toward the red end of the spectrum) Visible Range Sur E 1 80 Ranger Sur D 8090" : Energy Output (per second) Energy Output (per second) Star F 1 4000'K TTTTTT TTT TTT VIBOYOR Wavelength Use Figure 2a to answer questions 6 - 9. Assume stars E and F are the same size. 6) Which star gives off more red light? Explain your reasoning. 7) Which star gives off more blue light? Explain your reasoning. Search ENG (4) F3 F5 F6 F8 F9 F12 Insert Delete Backspace Num 5 6 Lock E R P Hicakes D F G K A Enter