Chemical elements are formed in the Universe by stellar nucleosynthesis.
The presence of elements heavier than iron in Iran can be hypothesized to result from the region's geological history, particularly through processes like supernova nucleosynthesis and the subsequent formation of heavy elements during stellar explosions. Additionally, tectonic activity could have facilitated the concentration and exposure of these elements through natural processes such as erosion and sedimentation. Furthermore, the area's unique mineral deposits and volcanic activity may contribute to the abundance of heavier elements found in its geology.
The presence of elements heavier than helium in stars is important because they provide crucial information about the star's age, composition, and evolutionary history. These heavier elements, also known as metals, are created through nuclear fusion processes in the cores of stars and are dispersed into space when the star dies. By studying the abundance of these elements in a star, scientists can gain insights into its formation and evolution.
Older age might account for it. As a star ages, it uses up the simplest elements (hydrogen . . . helium . . .) then starts fusing heavier and heavier elements. Our Sun will get to the point of fusing iron, which is pretty heavy, but the truly large stars out there will fuse elements much heavier than Iron. These heavier and heavier elements may account for some stars having more complex elements in their spectra.
Elements heavier than iron are formed in super-nova explosions.
They were formed in supernovae.
Heavier elements are formed through nuclear fusion reactions in the core of a star. Hydrogen atoms are fused together under high pressure and temperature to form helium. Further fusion reactions involving helium nuclei lead to the formation of heavier elements like carbon, oxygen, and up to iron. These elements are produced through a series of nuclear reactions that occur as the star evolves.
Lighter elements are composed of fewer protons and neutrons compared to heavier elements. They tend to have fewer total nucleons and lower atomic numbers. Lighter elements are typically found at the beginning of the periodic table, while heavier elements are found towards the end.
Heavier atoms which could not be formed as a result of fusion are produced as the result of a star that has run out of fuel exploding. It essentially forces atoms which do not release energy to fuse together.
This process is known as nuclear fusion. It occurs in stars like the sun when lighter elements such as hydrogen are combined to form heavier elements like helium, releasing a large amount of energy in the process.
Heavier elements in the universe were primarily formed through nuclear fusion processes in stars. During their lifecycles, stars fuse lighter elements, like hydrogen and helium, into heavier elements in their cores. When massive stars exhaust their nuclear fuel, they undergo supernova explosions, which scatter these heavier elements into space, enriching the interstellar medium. Additionally, processes like neutron capture during these explosive events contribute to the creation of even heavier elements.
Almost all solid elements are heavier than air. This is why these elements do not float under normal atmospheric situations.
After using up its hydrogen-1, the star becomes a red giant. It will start fusing helium-4 into heavier elements. It may also fuse heavier elements, to get other elements that are yet heavier.