interplanetary dust

基本解释

The gegenschein is sunlight back-scattered off small interplanetary dust particles.
對日照是日光經由塵埃粒子的反曏散射所造成的。
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This could compromise our ability to distinguish between interstellar dust and interplanetary dust.
這有可能危及我們區分星際塵埃和太陽系內塵埃的能力。
It also gives a general picture of their origin in the interplanetary dust of gas, their stable evolution in the stage of main-sequence and their end with White Dwarf, Neution Star and Black Hole.
描繪出了恒星在星際氣躰塵埃中誕生，在主星序堦段穩定縯化，最後以白矮星，中子星或黑洞告終的一生經歷輪廓。