How the Rubin observatory could detect thousands of 'failed stars'

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How the Rubin observatory could detect thousands of 'failed stars'
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Robert Lea is a science journalist in the U.K. whose articles have been published in Physics World, New Scientist, Astronomy Magazine, All About Space, Newsweek and ZME Science. He also writes about science communication for Elsevier and the European Journal of Physics. Rob holds a bachelor of science degree in physics and astronomy from the U.K.

The Milky Way could be hold a sea of faint,"failed stars," or brown dwarfs, that an upcoming astronomical survey called the Legacy Survey of Space and Time could detect. This type of discovery could help us better understand the processes that shaped our galaxy into the realm it is today.. Rubin is currently under construction on the mountain Cerro Pachón, high in the dry atmosphere of northern Chile.

That cool nature means brown dwarfs don't emit a great deal of light within the visible region of the electromagnetic spectrum. As a result, theseBreaking space news, the latest updates on rocket launches, skywatching events and more!Receive email from us on behalf of our trusted partners or sponsorsthe LSST camera, it will scan the entire visible sky every few nights.

That considerable increase in distance means a proportional increase in the total volume of space available to be scoured for brown dwarfs.

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