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Posted: **Tue Jul 12, 2022 8:29 am**

: 2 Denoting T The Temperature Of A Black Body And Some Constant The Stefan Boltzmann Law That Relates The Radiant Emit 1 (9.03 KiB) Viewed 28 times

2. Denoting T the temperature of a black body, and some constant, the Stefan-Boltzmann law that relates the radiant emittance M to T has the following form: (a) M = oT: (b) M-e7ª; (c) M-eT; (d) M-T¹.