The Exit Light Co power failure lights provide reassurance in those times when a natural disaster or your utility company is responsible for a power outage in your home. Safer than candles, the Exit Light Co range of battery powered lighting helps you get life back to normal and light back into your home.

Near-infraredwavelength

The electromagnetic spectrum spans a wide range of wavelengths from very short wavelength and highly energetic gamma rays to very long wavelength and low-energy radio waves. The visible part of the spectrum is only a small portion. Infrared light is the same as the light that we can see except that the wavelength is longer and outside the range that our eyes can sense.

Clearly, depending on what it is that we want to observe, we need to look in different parts of the spectrum, and no one part will tell us everything. The Earth’s atmosphere transmits well in the visible and radio regions, but it blocks out everything from gamma rays to ultraviolet and most of the infrared.  So to study the Universe at those wavelengths we need to launch space-borne observatories.

Infrared frequency

The Sun has a surface temperature of nearly 6000 Kelvin (where the Kelvin temperature scale is the same as the familiar Centigrade scale except that the zero degrees C is about 273 degrees Kelvin). Its radiation peaks in the visible part of the spectrum at wavelengths of about half a micron, as shown by the yellow-green line in the graph above.

Infrared waves

In fact all objects glow (emit electromagnetic radiation), and they do this in the part of the electromagnetic spectrum that depends on their temperature. The diagram below shows how bright objects of different temperatures appear at difference wavelengths.

These lights provide reassurance for anyone who doesn't like the dark. Power failure nightlights automatically switch on during a power outage, and motion sensors switch on the light when movement is detected.

The whole region with wavelengths ranging from 1 micron to 1 mm is loosely called the “infrared”, but astronomers tend to break this up into sub-regions:  the “near infrared” (from 1 to 5 microns); the “mid infrared” (5 to 30 microns), the “far infrared” (from 30 to 300 microns) and the “submillimetre” (from 300 microns to 1 mm).  The exact boundaries are somewhat arbitrary, and the exact definitions can vary.

Clouds of interstellar gas and dust that form stars are typically at temperatures of about 50 K (that’s about –220oC). They glow at far infrared wavelengths and are brightest at about 100 microns (red line in the graph above).  And the universe itself is filled with radiation corresponding to a temperature of just less than 3 K – very cold indeed – with peak emission in the millimetre wavelength range (blue line in the graph above).

Infrared uses

How do you do that FAST? Sure, you can light candles, but try resting easy knowing there are open flames burning in your home. For peace of mind and that all-important light during a power failure, there's a better solution:

Don’t be left in the dark during the next power outage from either the utility company or any number of natural disasters that can strike at any time. Our collection of Power Outage Flashlights, Nightlights and Lanterns have been manufactured with Emergency Safety in mind.

It is interesting that the basic technique used by Herschel to discover infrared radiation is still used in modern instruments today, including instruments on board the Herschel satellite – the only real difference is a factor a billion or so in sensitivity.

Infraredwavelengthrange in m

Ir light wavelengthin nm

Infraredlight

Infrared radiation was discovered by William Herschel in 1800. He was studying the heating effect of different colours of light by using a prism to produce a spectrum of colours and thermometers to measure their heating effect. He noticed that the heating effect got stronger as he went from the blue end of the spectrum to the red. In a moment of inspiration, he moved the thermometer beyond the visible red end and found that the heating effect was even greater.

These lights provide bigger and stronger sources of portable light than flashlights to bring light to larger areas of your home.

We humans, slightly warmer than room temperature, glow in the mid infrared and we’re brightest at about 10 microns wavelength (black line in the graph).   These days we are all familiar with infrared imaging, which allows us to see in the dark using electronic detectors that record infrared light emitted by warm objects such as people.  The pictures below show SPIRE team member Prof. Peter Ade in visible light (wavelength about 0.5 micron) and infrared light (about 10 microns).

Our businesses, schools, hospitals and everywhere else you look have Power Failure Emergency Lighting Systems. Why shouldn’t your home?

In 2019, 15 million Americans experienced a power outage in their home. Having your home thrown into sudden darkness can be DISTURBING, SCARY, and DISCONCERTING, especially for the very young or old. When the lights go out, life goes on-hold until you can get light back into your life.