Here’s What The Solar System Looked Like As A ‘Toddler,’ According To Astronomers


What did the solar system look like in its early days, and exactly how did it evolve? No one knows for sure, because no one was around billions of years ago to snap a photo or watch the action unfold.

But astronomers are crowing about the recent discovery of a distant star system that–particularly in its outer regions–looks a lot like what the solar system must have looked like early in its evolution.

“It’s almost like looking at the outer solar system when it was a toddler,” Dr. Thayne Currie, an astronomer at the Subaru Observatory in Hawaii and the principal investigator of a new study about the star system, said in a written statement.

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This composite image of the newly discovered star (HD 115600) shows a bright debris ring viewed nearly edge-on and located just beyond a Pluto-like distance to the star (left); and a model of the star’s debris ring on the same scale (right).

The newfound system, which was detected with the help of the Gemini South telescope in Chile, is located 360 light-years away in the constellation Centaurus. It features a star slightly more massive than the sun that has a disc-like field of dust and ice surrounding it at a distance of 3.4 to 5.1 billion miles.

That’s roughly the same distance as the sun to the Kuiper Belt, the region of space just beyond Neptune that contains icy debris left over from the formation of the solar system more than four billion years ago. The debris ranges in size from a speck of dust to moon-sized objects like Pluto, which is now considered a dwarf planet.

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Diagram showing Kuiper belt.

No planets were detected around HD 115600, although the fact that its disc —> Read More