What is Stephen-Boltzman law of heating?
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ꜱᴛᴇᴩʜᴇɴ - ʙᴏʟᴛᴢᴍᴀɴ ʟᴀᴡ , ꜱᴛᴀᴛᴇᴍᴇɴᴛ ᴛʜᴀᴛ ᴛʜᴇ ᴛᴏᴛᴀʟ ʀᴀᴅɪᴀɴᴛ ʜᴇᴀᴛ ᴇɴᴇʀɢy ᴇᴍɪᴛᴛᴇᴅ ꜰʀᴏᴍ ᴀ ꜱᴜʀꜰᴀᴄᴇ ɪꜱ ᴩʀᴏᴩᴏʀᴛɪᴏɴᴀʟ ᴏꜰ ᴛʜᴇ ꜰᴏᴜʀᴛʜ ᴩᴏᴡᴇʀ ᴏꜰ ɪᴛꜱ ᴀʙꜱᴏʟᴜᴛᴇ ᴛᴇᴍᴩᴇʀᴀᴛᴜʀᴇ... ᴛʜᴇ ʟᴀᴡ ᴀᴩᴩʟɪᴇꜱ ᴏɴʟy ᴛᴏ ʙʟᴀᴄᴋ ʙᴏᴅɪᴇꜱ .
ʜᴏᴩᴇ ɪᴛ ʜᴇʟᴩꜱ yᴏᴜ..!
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✍Stefan-Boltzman law , Statement that the total radiant heat energy emitted from a surface is proportional to the fourth power of its absolute temperature.
✍The law only applies to backbodies , theorthical surface that absorb all incident heat radiation.
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