There are plenty of fun space simulations out there, but this model serves an important purpose. Dust can block out blue light in favor of red light, giving us inaccurate information through our telescopes. That means astronomers need to know the chemical makeup, shape and size of the dust grains in order to correct for their effect, according to an article published by a team of American scientists today in The Astrophysical Journal. The outcome—how the dust affects the light we measure—is described by an equation called the extinction curve.

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The scientists created extinction curves from data collected by the Pan-STARRS telescopes in Hawaii and the Sloan Digital Sky Survey, which operates out of a telescope at Apache Point Observatory in New Mexico. Combined with another research group’s distance estimates to the dust, and yet another’s Milky Way dust map, you get the trippy visuals above, which show actual dust in a region of the Milky Way thousands of light-years wide.

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And we need the data for lots of reasons other than entertaining your stoned friend Chad. Scientists are trying to make 3D maps of the entire universe with experiments like the Dark Energy Spectroscopic Instrument (DESI), and dust can distort that map. Efforts like this can help identify regions of space where the light we’re seeing isn’t an accurate reflection of what’s really out there.

Anyway, it’s Wednesday. Take it easy and take solace in the fact that you’re just a dust grain in our vast Milky Way. Mind blown, my dudes.

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Correction: We updated the headline after a commenter pointed out that this is not a simulation but a real model with real data.

[Astrophysical Journal]