Yes.
See related question.
From the outer layers emitted by a supernova.outer layer of a supernova.
for making elements from helium to nickel and iron, thermonuclear fusionfor making elements past nickel and iron a supernova explosion is needed to force nuclei to fuse more, this destroys the star
The interstellar medium is enriched with heavy elements by the remnants of supernova explosions. Supernovae are massive stellar explosions that release heavy elements such as carbon, oxygen, and iron into space, enriching the surrounding interstellar medium with these elements.
Such elements are formed within stars. The heavy elements which are currently here on Earth were formed in stars some time ago, and then they were blown into space in supernova explosions.
The elements on the periodic table were created by stars through nuclear fusion. We use the term stellar nucleosynthesis to describe what stars are doing through fusion. Stars fuse hydrogen into helium, and then start making heavier elements by a different fusion process. But stars can only make elements up through iron. They can't make the heavier elements. Enter the supernova. A supernova is that "big blast" that occurs at the end of the life of some stars. In a supernova, the trans-iron elements are formed. That is, all the elements heavier than iron are formed in a supernova. Because the elements heavier than iron are formed in a supernova, we can say that there is a relationship between the supernova and the periodic table of elements.
Supernova explosions are responsible for producing elements with atomic masses greater than iron through nucleosynthesis processes. During these violent events, heavy elements are forged from lighter elements through rapid fusion reactions.
for making elements from helium to nickel and iron, thermonuclear fusionfor making elements past nickel and iron a supernova explosion is needed to force nuclei to fuse more, this destroys the star
In a supernova explosion, heavy elements (metals) such as iron, nickel, gold, and uranium are created through nucleosynthesis. These elements are formed from the fusion of lighter elements under extreme temperature and pressure conditions during the explosive event.
Heavy elements in the universe were primarily formed through processes such as stellar nucleosynthesis and supernova explosions. In stars, lighter elements fuse under extreme temperatures and pressures to create heavier ones, with elements beyond iron typically formed during supernova events when massive stars explode. Additionally, neutron capture processes, like the r-process and s-process, contribute to the formation of various heavy elements. These processes occur over cosmic timescales, contributing to the elemental diversity observed in the universe today.
Iron is formed in nature through a process called supernova nucleosynthesis, where heavy elements are created during the explosion of massive stars. This process involves the fusion of lighter elements in the star's core, eventually leading to the formation of iron.
Astronomers consider elements beyond hydrogen and helium, such as carbon, oxygen, nitrogen, and iron, as heavy elements. These elements are created through processes like nuclear fusion in stars and supernova explosions.
Elements with more protons and neutrons than iron are believed to have formed through processes like supernova explosions. These heavy elements, such as gold and uranium, are created in the intense conditions of these cosmic events.