Infrared Incandescence: How Hot Does It Need To Be?

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SUMMARY

This discussion centers on the principles of infrared (IR) radiation and its detection by various cameras, specifically comparing thermal cameras like FLIR with standard commercial security cameras. It is established that all objects above absolute zero emit IR radiation, with the intensity and wavelength depending on their temperature, as described by Wien's Law. A normal incandescent bulb operates around 3,000 Kelvin, emitting significant IR radiation, which is often wasted. The conversation also highlights practical experiments using electric stoves and digital cameras to observe IR emissions before they become visible.

PREREQUISITES
  • Understanding of infrared radiation and its spectrum
  • Familiarity with thermal imaging technology, specifically FLIR cameras
  • Knowledge of Wien's Law and black-body radiation principles
  • Basic experience with digital cameras and their functionalities
NEXT STEPS
  • Research the principles of Wien's Law and its application in thermal imaging
  • Explore the differences between thermal cameras and standard IR-sensitive cameras
  • Conduct experiments with black-body radiation using interactive simulations
  • Investigate energy efficiency in lighting, focusing on incandescent versus compact fluorescent lamps (CFLs)
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Individuals interested in physics, engineers working with thermal imaging, and anyone looking to understand the principles of infrared radiation and its practical applications in technology.

ricardo7890
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From what i understand thermal cameras like flir can see "heat" because objects at room temperature release Ir light like hot metal would visible light. But most cameras like commercial security cameras can see IR but don't work like thermal cameras because they aren't sensitive to the right range of the IR spectrum.
But if an object was hot enough would it give off IR light that a normal ir sensitive camera could see it, but not produce visible light, and if that is the case how hot would say a piece of iron have to be to give of this wavelength of IR but not visible light.
 
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ricardo7890 said:
But if an object was hot enough would it give off IR light that a normal ir sensitive camera could see it, but not produce visible light, and if that is the case how hot would say a piece of iron have to be to give of this wavelength of IR but not visible light.
Hi ricardo7890. http://img96.imageshack.us/img96/5725/red5e5etimes5e5e45e5e25.gif

You can experiment with IR at home, using your electric stove and digital camera. In the dark of night, set one of the stove's top elements to medium heat and as it warms up watch it on the monitor of your digital camera. Does it show up on the screen as green-grey well before it's visible to the unaided eye?

At night, while monitoring the screen of your digital camera, you can illuminate things using your tv remote control as an IR flashlight.

If you want to read up on the topic, see radiation from hot bodies and Wien's Law. http://www.egglescliffe.org.uk/physics/astronomy/blackbody/bbody.html
 
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ricardo7890 said:
From what i understand thermal cameras like flir can see "heat" because objects at room temperature release Ir light like hot metal would visible light. But most cameras like commercial security cameras can see IR but don't work like thermal cameras because they aren't sensitive to the right range of the IR spectrum.

Yes, the security cameras have to illuminate their field of view with special LED's that emit the required frequency range of the camera I believe.

But if an object was hot enough would it give off IR light that a normal ir sensitive camera could see it, but not produce visible light, and if that is the case how hot would say a piece of iron have to be to give of this wavelength of IR but not visible light.

Yes and no. The effect you are referring to is known as "thermal" or "black-body" radiation. http://en.wikipedia.org/wiki/Black-body_radiation
Any object above absolute zero in temperature will emit a broad spectrum of radiation. This emission is random, but follows a relationship based on the temperature of the object. Simply put, hotter objects emit more radiation at higher frequencies (higher frequencies are more energetic) than colder objects. A normal incandescent light bulb that you screw into your lamp or whatever uses a filament that is heated to about 3,000 kelvin. At this temperature objects emit a range of wavelengths that includes the visible and infrared, with the amount of radiation peaking in the infrared range. That's right, a normal light bulb puts out more power in the INFRARED range of the spectrum than in the visible range! This means a large amount of power is wasted, which is the reason for the push to change to compact fluorescent lamps (CFL's).

Here is an interactive graph you can use to see the output of an object at a certain temperature. It's designed for use with stars, but the same rules apply to any object. Drag the bar to whatever temperature gives you the right range and you can see for yourself.
http://www.pas.rochester.edu/~afrank/A105/mha/Blackbody_Nav.swf

That one only goes down to 2500 k, so here's one where you can enter whatever temperature you want.
http://homepages.ius.edu/kforinas/physlets/thermo/blackbody.html

In any case, the radiation emitted at higher frequencies drops off, BUT IS NEVER ZERO! So every so often the wall of your room may emit a red or blue photon, but the frequency at which this happens is so incredibly low you'd never be able to see it. It's like...really REALLY low...
 

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