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Formation of Heavier Elements

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H. Manishankar (KV Pattom) Asked

Question: Iron is the heaviest element that can be formed by nuclear reactions in a star.So how the heavier elements after iron were formed?And could there be further heavier elements out there in the cosmos?

Answer:

Nuclear fusion inside a star is not the only process my which new elements are created. There are many others too.

During a supernova explosion many unpredictable nuclear transmutations occur, fusing elements and forming heavier elements.

But however, the amount of elements heavier than iron is less.

It’s a good idea to think back (say from the time of BigBang)

Every explosion has a consequent implosion resulting in creation of heavier elements

Remember that birth and death of stars are taking place everyday in some part or other of the universe. The earlier stars had relatively lighter elements in their core. As they die, the remains form part of other stars and other celestial bodies thereby forming heavier elements in the universe.

(I don’t claim that this is a complete answer. Visitors are requested to suggest amendments to this Answer via comments)

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Comments

  1. Earth and most of the other planets were formed from the same raw material, but the constituents of different planets differ. The differentiation process changed the constitution. In undifferentiated planets, the constituents will be almost the same as the initial ones.

  2. am still nt clear abt if there could be further heavier elements than wat we can presently find on earth?

    1. There are certain things which inhibit the creation of still heavier elements (on earth at least). As more and more nucleons are added to the nucleus, the size of the nucleus increases. As nuclear force is a short range force, the Coulomb repulsion force between the farther nucleons overpowers the nuclear force and this decreases the stability of the nucleus. So, elements of higher atomic weight (AND ATOMIC NO) are rare. The percentage of transuranic elements are very small.

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