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单词 Iron peak
释义

Iron peak

中文百科

铁峰顶

化学元素的丰度:太阳系的丰度。

铁峰顶 — 化学元素丰度图上,在 Fe(V、Cr、Mn、Fe、Co和Ni)元素邻近的局部极大。

在铁之前的元素进行核融合释放能量,比铁重的元素需要消耗能量才能进行核融合,取代的是以核分裂发布能量。化学元素的恒星核合成因而很正常的产生了铁峰顶。重的元素只有在超新星核合成才会产生,因此在我们邻近的区域有着较多的铁峰顶元素。

英语百科

Iron peak 铁峰顶

Abundances of the chemical elements in the Solar System. Hydrogen and helium are most common, from the Big Bang. The next three elements (Li, Be, B) are rare because they are poorly synthesized in the Big Bang and also in stars. The two general trends in the remaining stellar-produced elements are: (1) an alternation of abundance in elements as they have even or odd atomic numbers, and (2) a general decrease in abundance, as elements become heavier. The

The iron peak is a local maximum in the vicinity of Fe (V, Cr, Mn, Fe, Co and Ni) on the graph of the abundances of chemical elements, as seen below.

For elements lighter than iron on the periodic table, nuclear fusion releases energy. For iron, and for all of the heavier elements, nuclear fusion consumes energy, but nuclear fission releases it. Chemical elements up to the iron peak are produced in ordinary stellar nucleosynthesis. Heavier elements are produced only during supernova nucleosynthesis. This is why we have more iron peak elements than in its neighbourhood.

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更新时间:2025/6/22 6:19:22