Most stars shine in ultraviolet and infrared colours that are blocked by the Earth’s atmosphere, as well as the colours our eyes evolved to see.

Extra colours are useful. For example, we can weigh stars on the other side of our galaxy because massive stars are bright in infrared, while smaller ones are faint – and they stay that way throughout their lifetimes. However, we know where stars are being born because only young stars emit ultraviolet light.

In addition, independent measurements of the same thing are vital for rigorous science. Infrared telescopes, for example, can work together and have already made surprising discoveries. But it’s not great for diversity that the Webb, Euclid and Roman space telescopes all see infrared colours.