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in 1893, german physicist wilhelm wien quantified the relationship between blackbody temperature and the wavelength of the spectral peak with the following equation:
en 1893, el físic alemany wilhelm wein quantificà la relació entre la temperatura d' un cos negre i la longitud d' ona del pic espectral amb la següent equació:
& contents; & skycoords; & cequator; & cpoles; & csphere; & ecliptic; & equinox; & geocoords; & greatcircle; & horizon; & hourangle; & meridian; & precession; & zenith; & julianday; & leapyear; & sidereal; & timezones; & utime; & blackbody; & darkmatter; & flux; & luminosity; & parallax; & retrograde; & ellipgal; & spiralgal; & magnitude; & stars; & colorandtemp;
& contents; & skycoords; & cequator; & cpoles; & csphere; & ecliptic; & equinox; & geocoords; & greatcircle; & horizon; & hourangle; & meridian; & precession; & zenith; & julianday; & leapyear; & sidereal; & timezones; & utime; & blackbody; & darkmatter; & flux; & luminosity; & parallax; & retrograde; & ellipgal; & spiralgal; & magnitude; & stars; & colorandtemp;