研究者已经在寻找那些距离其母恒星的引力足够远，以致可能庇护安定的卫星的巨型行星。

Already researchers are locating giant planets far enough from the gravitational pull of their host star to potentially harbor stable satellites.

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来自这些凝聚的硬块所带来引力的扰动，反过来能够推动这些在早期所形成行星进入到更为靠近其母恒星的运行轨道上。

Gravitational perturbations from the clumps, in turn, can push the nascent planets into orbits closer to the parent star.

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其母体恒星就像是一个红色的小矮人——比起太阳来实在是又小又模糊。

Its parent star is a red dwarf--a far smaller and fainter object than the sun.

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