超大質量ブラックホール周辺での巨大系外惑星形成が可能
イメージ ブラックホールは破壊機構ではなく複雑な時空領域であり、適切な条件下ではAGNディスク内に巨大惑星が形成される可能性がある。
出典：Universe Today ／ 自動翻訳のため訳文が不正確な場合があります
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