Science. 1989 Jul 21;245(4915):283-6. doi: 10.1126/science.245.4915.283.
The quantity and physical state of methane and nitrogen in the atmosphere of Neptune's satellite Triton and on the surface are evaluated by means of new telescopic data and laboratory measurements of these volatiles. Methane ice is seen in some spectral regions, indicating that the atmosphere is sufficiently transparent to permit sunlight penetration to the surface. Some of the molecular nitrogen absorption occurs in the atmosphere, though some must occur in condensed nitrogen (liquid or solid) on Triton's surface, or in a thin cloud of condensed nitrogen. The Voyager spacecraft cameras should see the surface of Triton.
利用新的望远镜数据和这些挥发物的实验室测量结果,评估了海王星卫星特里顿的大气中甲烷和氮气的数量和物理状态。在一些光谱区域观察到甲烷冰,表明大气足够透明,可以让阳光穿透到表面。一些分子氮的吸收发生在大气中,尽管一些必须发生在特里顿表面的冷凝氮(液体或固体)中,或者在一层稀薄的冷凝氮云中。航海者号飞船的摄像机应该可以看到特里顿的表面。