The ring extends much further out than Saturn's other rings, and is tilted at a different angle to the rest in relation to the planet's axis of rotation.
Saturn's rings are known to be composed of dust, ice and other debris caught up in orbit around the planet.
Scientists believe the newly discovered ring is so tenuous because its particles of ice and dust are thinly dispersed in space. This means they do not reflect much light, making the ring hard to see.
Spitzer's infra-red camera was able to detect the "glow" of the band's cool dust, which only manages to reach a temperature of minus 193C. Even at such low temperatures, the dust gives off enough infra-red light to be picked up by Spitzer, the $800m space observatory launched in 2003. "By focusing on the glow of the ring's cool dust, Spitzer made it easy to find," said Anne Verbiscer, an astronomer at the University of Virginia. "[But] the particles are so far apart that if you were to stand in the ring, you wouldn't even know it. This is one supersized ring. If you could see [it], it would span the width of two full-moons' worth of sky, one on either side of Saturn."
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