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AstroAlert: The Sun’s long-lost twin?

Hi everyone,
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Stars, like puppies, are born in litters. Although humans usually give birth to one offspring at a time, multiple births are the norm for stars. In fact, it’s unusual for a star to be born without siblings.
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Stellar birth takes place in giant clouds of gas and dust that are slowly squeezed by gravity until they fragment into stars. Depending on its size, a single cloud can spawn dozens to millions of stars. These litters usually disperse over time as siblings drift apart, tugged this way and that by the gravitational pull of other passing stars, star clusters and gas clouds. Yet most stars manage to hang onto a sibling or two, becoming lifelong companions locked in an endless gravitational hug.
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The Sun was probably born in such a litter nearly five billion years ago. But nobody knows where our star’s siblings are today. Like a litter of puppies all adopted by different homes, the Sun’s brother and sister stars have dispersed to parts unknown. Somewhere out there, the Sun’s long-lost siblings wander through space, oblivious to our yellow star and the planets huddled around it.
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But now astronomers think they might have found one of the Sun’s siblings, maybe even an identical twin. Just as human siblings share similar genetic traits inherited from their parents, stars born to the same parent gas cloud share the same ages and same proportions of different types of atoms, which provides a sort of cosmic DNA test to identify stellar siblings.
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By carefully sifting through data for about 17,000 stars, a team of astronomers in Europe found that one of them, named HD 186302, turns out to be the spitting image of our Sun. Not only does it have the same atomic composition and age as the Sun, its size, temperature and luminosity are also nearly identical. An image of this solar doppelgänger is shown below.
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Located just 184 light years away – practically in our neighborhood – it’s possible that HD 186302 could even Earth-like planets with conditions suitable for life. Perhaps future Earthlings will someday travel to HC 186302 to invite our cousins over for a barbecue.
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If you’d like to know more, just click here.
If you’d like to read the full (technical) scientific paper about this discovery, you’ll find it here.
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Best regards,
Michael
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