Some people have reported seeing more semivolatile elements in a class of interplanetary dust particles (IDPs) called “chondritic porous” IDPs.

曾有人报告在一类被作“多孔球粒石”的行尘埃颗粒（IDPs）中见到了较多的半挥发性元素。

If you look over the element ratios we measured, you might conclude that our comet particles look more like chondritic porous IDPs than CI chondrite meteorites.

如果查看我们测定的元素，将得出结论——我们的彗颗粒看上去更接近多孔球粒石IDPs而不是CI球粒石。

Some people have reported seeing more semivolatile elements in a class of interplanetary dust particles (IDPs) called “chondritic porous” IDPs.

曾有人报告在一类被作“多孔球陨石”的行尘埃（IDPs）中见到了较多的半挥发性元素。

If you look over the element ratios we measured, you might conclude that our comet particles look more like chondritic porous IDPs than CI chondrite meteorites.

如果你查看我们测定的元素比率，你将得出结论——我们的彗看上去更接近多孔球陨石IDPs而不是CI球陨石。

Some people have reported seeing more semivolatile elements in a class of interplanetary dust particles (IDPs) called “chondritic porous” IDPs.

有人报告在一类被作“多孔球粒陨石”尘埃颗粒（IDPs）中见到了较多半挥发性元素。

If you look over the element ratios we measured, you might conclude that our comet particles look more like chondritic porous IDPs than CI chondrite meteorites.

如果你查看我们测定元素比率，你将得出结论——我们彗颗粒看上去更接近多孔球粒陨石IDPs而不是CI球粒陨石。

Some people have reported seeing more semivolatile elements in a class of interplanetary dust particles (IDPs) called “chondritic porous” IDPs.

曾有人报告在一类被作“多孔球粒陨石”行星尘埃颗粒（IDPs）中见到了较多发性元素。

If you look over the element ratios we measured, you might conclude that our comet particles look more like chondritic porous IDPs than CI chondrite meteorites.

如果你查看我们测定元素比率，你将得出结论——我们彗星颗粒看上去更接近多孔球粒陨石IDPs而不是CI球粒陨石。

Some people have reported seeing more semivolatile elements in a class of interplanetary dust particles (IDPs) called “chondritic porous” IDPs.

曾有人报告在一类被作“多孔球粒”的行星尘埃颗粒（IDPs）中见到了较多的半挥发性元素。

If you look over the element ratios we measured, you might conclude that our comet particles look more like chondritic porous IDPs than CI chondrite meteorites.

如果你查看我们测定的元素比率，你将得出结论——我们的彗星颗粒看上去更接近多孔球粒IDPs不是CI球粒。

Some people have reported seeing more semivolatile elements in a class of interplanetary dust particles (IDPs) called “chondritic porous” IDPs.

曾有人报告在一类被作“多孔球粒陨石”的行尘埃颗粒（IDPs）中见到了较多的半挥发性元素。

If you look over the element ratios we measured, you might conclude that our comet particles look more like chondritic porous IDPs than CI chondrite meteorites.

如果你查测定的元素比率，你将得出结论——的颗粒上去更接近多孔球粒陨石IDPs而不是CI球粒陨石。

Some people have reported seeing more semivolatile elements in a class of interplanetary dust particles (IDPs) called “chondritic porous” IDPs.

曾有人报告在一“孔球粒陨石”的行星尘埃颗粒（IDPs）中见到了较的半挥发性元素。

If you look over the element ratios we measured, you might conclude that our comet particles look more like chondritic porous IDPs than CI chondrite meteorites.

如果你查看我们测定的元素比率，你将得出结论——我们的彗星颗粒看上去更接近孔球粒陨石IDPs而不是CI球粒陨石。

Some people have reported seeing more semivolatile elements in a class of interplanetary dust particles (IDPs) called “chondritic porous” IDPs.

曾有人报告在一类被作“多孔球粒陨石”的行星尘埃颗粒（IDPs）中见到了较多的半挥素。

If you look over the element ratios we measured, you might conclude that our comet particles look more like chondritic porous IDPs than CI chondrite meteorites.

如果你查看我们测定的素比率，你将得出结论——我们的彗星颗粒看上去更接近多孔球粒陨石IDPs而不是CI球粒陨石。

Some people have reported seeing more semivolatile elements in a class of interplanetary dust particles (IDPs) called “chondritic porous” IDPs.

曾有人报告在一类被作“多孔球陨石”的行尘埃（IDPs）中见到了较多的半挥发性元素。

If you look over the element ratios we measured, you might conclude that our comet particles look more like chondritic porous IDPs than CI chondrite meteorites.

如果你查看我们测定的元素比率，你将得出结论——我们的彗看上去更接近多孔球陨石IDPs而不是CI球陨石。