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A rogue planet 620 light-years away called Cha 1107 is devouring six billion tons of material every second, blurring the line between planets and stars and forcing astronomers to rethink how worlds form.

Source: https://arxiv.org/abs/2510.01747

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9Comments

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  1. 2
    @tttpppbbbaaa

    It could be the missing link of star formation. First is a Jupiter like planet is formed then over time it slowly get bigger and bigger till it becomes a protostar till finally it has enough mass to ignite through fusion.

  2. 7
    @EdStauffer-n2i

    Do some planets form in the dark due to streams of dark matter that overflowed their gravity wells. As the dark matter stream moves through space escaping the gravity well it’s gravity stream begins to collect additional dust. The collected dust slows in its progress through space due to accretion until finally it begins to orbit the next dust ball that has collected. This causes the two to move out of the Center of the stream. The comet tail of planetessimals that it has collected as the dust turns into spheres which eventually catch up to and orbit the two biggest masses. When the dark matter stream and the largest sphere of dusts combined gravity is enough it ignites into a Star or maybe two. The other masses would follow in decreasing size due to less gas and dust to collect. How many millions of different pieces would come trailing in over the next 500 million years. Each one of these pieces having slowed the dark matter through gravity interactions they were tugged into the gravity train. The majority of these due to wider orbits ending up in the Kuiper belt and the Oort Cloud or miss and continue on. The bulk of the overflowing dark matter would continue to stream on potentially continuing to add dust to the developing solar system. This would also explain how there is more matter than the original disk of dust would account for. The incoming dark matter stream would also follow the accretion to the star possibly still circulating today kept going by the planetary rotations.

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