“这是我们第一次可以获得大型年轻星体周围的碟状区域内部的图像，”Kraus陈述说，“我们的观察表明所有星体的形成方式都是一样的，无论大小。”

This is the first time we could image the inner regions of the disc around a massive young star, "Kraus said in a statement."

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图片上蓝色的光点代表灼热的年轻的星体，它们从2004年起被加入观察范围。

Bright blue dots represent hot young stars in the photo, which includes observations taken from 2004.

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的碰撞。例如月亮被认为形成于火星大小的星体急速撞向我们年轻的地球时产生的碎片。

The moon, for instance, is believed to have formed from debris stirred up by a Mars-size object careening into our young planet.

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