Blackbody Radiation, Wein’s Law, and BrightnessIt is believed that some white dwarf stars could host planets.
(a) If the white dwarf has a luminosity ofLW D= 10−2L, how far from it must one of its’ planets besuch that the planet receives the same flux as the Earth does from our Sun (FEarth= 1360W/m2)?
(b) If this white dwarf has a surface temperature ofTeff= 15000 K, then what is the peak wavelengthof its’ blackbody radiation?
(c) Sketch the blackbody radiation curve for this white dwarf, assuming no spectral lines.
If you still have any confusion anywhere then please let me know in the comments section.
Thank you.
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