吸积
參考

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三裂星雲的可見光（左）與紅外線（右）影像。三裂星雲位於射手座，距地球5400光年（1700秒差距），是一團巨大的氣體和灰塵雲，其內有恆星形成。
新生恆星 HH 46/47 的分子外流的紅外線影像。若不使用此波段，此恆星將無法被觀測到。
當雙星系統中的小質量恆星進入膨脹階段，其外氣層可能落入另一個緻密恆星，形成吸積盤。
原行星盤（中心含有一顆年輕恆星）的藝術家印象。
球粒隕石中的球粒隕石顆粒。所示尺度為毫米尺度。
小行星486958（天涯海角），一個位於庫伯帶的天體，其被認為能代表最初的原行星（行星由其成長而成）。