NASA figures out how to cause supernova (Should we be worried?)

From DVICE: NASA, for some reason that the agency has chosen not to share, is quite interested in just exactly what it takes to set off a Type Ia supernova. Thanks to a series of X-ray and ultraviolet observations from the SWIFT satellite, NASA says that "we have a clearer picture of what's required to blow up these stars." Oh, good.

Type Ia supernovae are a specific type of stellar explosion that are very, very important because astronomers can use them as what's called "standard candles."

Standard candles (there are only a few different kinds and they're all very rare) are things that we can see with a telescope and know how far away they are. Usually, if you see something through a telescope, there's no reliable way of knowing whether it's a bright thing that's far away or a dim thing that's up close. A standard candle has a luminosity (or, an intrinsic brightness) that doesn't ever change, so based on how bright or dim it looks to us here on Earth, we can figure out how far away it (and everything around it) actually is.

This post originally appeared on DVICE, a sister blog of Blastr all about technology that really matters. To read the rest of it, click here.

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