Answer:
is equal to approximately 2.898 x 10 -3 meter-kelvin (0.2898 centimeter-kelvin). The product of the thermodynamic temperature of a black body in kelvin s, and the wavelength of its peak energy output in meter s, is equal to Wien's constant
ɪᴛ ɪs ᴇϙᴜᴀʟ ᴛᴏ ᴀᴘᴘʀᴏxɪᴍᴀᴛᴇʟʏ 2.898 x 10 -3 ᴍᴇᴛᴇʀ-ᴋᴇʟᴠɪɴ (0.2898 ᴄᴇɴᴛɪᴍᴇᴛᴇʀ-ᴋᴇʟᴠɪɴ). ᴛʜᴇ ᴘʀᴏᴅᴜᴄᴛ ᴏғ ᴛʜᴇ ᴛʜᴇʀᴍᴏᴅʏɴᴀᴍɪᴄ ᴛᴇᴍᴘᴇʀᴀᴛᴜʀᴇ ᴏғ ᴀ ʙʟᴀᴄᴋ ʙᴏᴅʏ ɪɴ ᴋᴇʟᴠɪɴ s, ᴀɴᴅ ᴛʜᴇ ᴡᴀᴠᴇʟᴇɴɢᴛʜ ᴏғ ɪᴛs ᴘᴇᴀᴋ ᴇɴᴇʀɢʏ ᴏᴜᴛᴘᴜᴛ ɪɴ ᴍᴇᴛᴇʀ s, ɪs ᴇϙᴜᴀʟ ᴛᴏ ᴡɪᴇɴ's ᴄᴏɴsᴛᴀɴᴛ...
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Answer:
is equal to approximately 2.898 x 10 -3 meter-kelvin (0.2898 centimeter-kelvin). The product of the thermodynamic temperature of a black body in kelvin s, and the wavelength of its peak energy output in meter s, is equal to Wien's constant
Answer:
ɪᴛ ɪs ᴇϙᴜᴀʟ ᴛᴏ ᴀᴘᴘʀᴏxɪᴍᴀᴛᴇʟʏ 2.898 x 10 -3 ᴍᴇᴛᴇʀ-ᴋᴇʟᴠɪɴ (0.2898 ᴄᴇɴᴛɪᴍᴇᴛᴇʀ-ᴋᴇʟᴠɪɴ). ᴛʜᴇ ᴘʀᴏᴅᴜᴄᴛ ᴏғ ᴛʜᴇ ᴛʜᴇʀᴍᴏᴅʏɴᴀᴍɪᴄ ᴛᴇᴍᴘᴇʀᴀᴛᴜʀᴇ ᴏғ ᴀ ʙʟᴀᴄᴋ ʙᴏᴅʏ ɪɴ ᴋᴇʟᴠɪɴ s, ᴀɴᴅ ᴛʜᴇ ᴡᴀᴠᴇʟᴇɴɢᴛʜ ᴏғ ɪᴛs ᴘᴇᴀᴋ ᴇɴᴇʀɢʏ ᴏᴜᴛᴘᴜᴛ ɪɴ ᴍᴇᴛᴇʀ s, ɪs ᴇϙᴜᴀʟ ᴛᴏ ᴡɪᴇɴ's ᴄᴏɴsᴛᴀɴᴛ...