Conventional cooling is all about moving heat from a place where you don’t want it to a place that you care about slightly less. Your refrigerator, for example, cools itself by pumping heat into your house. Your house cools itself by pumping heat into the outdoors. It takes a significant amount of energy to keep this up—15 percent of the energy consumption of most buildings is spent just on air conditioning—meaning that the work put into transferring the heat generates even more heat. And then it’s not like the heat just vanishes when it gets outside: in urban areas, all of this waste heat builds up to increase local temperatures as part of the urban heat island effect.
In Nature this week, Stanford researchers describe a passive radiator system that can lower the temperature of anything that it’s placed on by up to five degrees Celsius by absorbing heat and sending it directly into outer space, and it even works in direct sunlight.
Radiative cooling is a way of passively moving heat from one place to another through thermal radiation, without the need for any additional energy (like electricity). If you have a hot thing, it will radiate its heat into whatever cooler thing is most convenient. In your house, this is probably the air outside, and in your car, it’s also the air outside, by way of the water in your radiator.
Since the general approach here is to use the atmosphere as the final heat sink, radiative cooling doesn’t work if you’re trying to end up at a temperature lower than the ambient temperature outside, which is why completely passive air conditioning isn’t a thing.
The clever thing about the passive radiative cooling system that Stanford came with is that it skips the atmosphere completely, and uses the entire Universe as a place to dump heat. The entire Universe, being mostly empty space, has an average temperature of just under three Kelvin, meaning that it’ll happily absorb just about as much heat as you can possibly throw at it, making it a heat sink that’s nearly, you know, universal.
To use outer space as a heat sink, you need to have access to outer space, which sounds like it’s probably a difficult thing to achieve. But fundamentally, it just means being able to transfer heat straight through Earth’s atmosphere. Stanford’s cooling system emits thermal radiation in a very specific infrared wavelength that the Earth’s atmosphere is completely transparent to, between 8 and 13 micrometers.
So, this is great, but the other part of the problem with radiative cooling is that we really need it to work during the day, when the sun is out and it’s hot. But if the sun is warming the radiator more than the radiator can cool itself, the system isn’t going to accomplish much. Stanford’s radiator also functions as a mirror that can reflect 97 percent of incident sunlight, enabling the radiator to cool itself (or something underneath it) by up to five degrees Celsius even during the heat of the day. In a three-story commercial building with a 1600 square meter roof, using the radiative cooler would save an estimated 118,500 kWh annually, the engineers calculate.
The radiator itself is composed of seven layers of silicon dioxide and hafnium oxide on top of a thin layer of silver. The structure has been tuned to only radiate at the specific infrared wavelengths that can pass through the atmosphere. It’s just 1.8 microns thick in total, and the researchers say that it can be fabricated at production scales in existing facilities. Otherwise, the only remaining issue is to figure out how to conduct the heat from inside a building through to the exterior walls, to where the radiator could do its job.
These problems both seem surmountable, and even surmountable in the near future, as opposed to the “five to ten years” void that many technologies like this fall into. If this radiative cooler material can in fact be produced inexpensively and efficiently, it could have a significant impact on energy usage, especially in the developing world where off-grid cooling is often the only option in rural areas.