Carl Sagan, one of the most charismatic figures of later-twentieth century Astrophysics, has been the first to inform the common man that - "Our Sun is a second- or third-generation star. All of the rocky and metallic material we stand on, the iron in our blood, the calcium in our teeth, the carbon in our genes were produced billions of years ago in the interior of a red giant star. We are made of star-stuff (The Cosmic Connection: An Extraterrestrial Perspective, 1973)".
Yes, starstuff. Quite literally. According to the currently accepted cosmological models, the Universe started in an incredibly hot and dense state, about 14 billion years ago in a singular event known as the `Big Bang'. As the Universe expanded, it cooled and within the first three minutes matter, as we know it, formed. However, it was mostly hydrogen (76%) and helium (24%), with a rather small fraction of other material like lithium etc. It was not till the first stars were born that heavier elements could be formed through fusion of lighter elements in a process now known as 'stellar nucleosynthesis'.
Even though this appears to be rather obvious now, there was considerable uncertainty regarding stellar nucleosynthesis in the early part of the twentieth century when scientists were not sure if stellar interiors were hot enough for such fusion processes. Eventually, the day was won and Arthur Eddington proclaimed from Cambridge - "We do not argue with the critic who urges that the stars are not hot enough for this process; we tell him to go and find a hotter place (The Internal Constitution of Stars, 1926)". The story would be completed a couple of decades later by another Cambridge man, Sir Fred Hoyle, when he and his collaborators would work out the details of stellar nucleosynthesis in the celebrated BBFH (Burbidge, Burbidge, Fowler, Hoyle, 1957) paper.
However, stellar nucleosynthesis goes only as far as iron and nickel. Manufacturing elements heavier than iron require other more energetic processes like - a supernova explosion or merger of neutron stars. Jennifer A. Johnson of Ohio State University has now created a rather clever 'astrophysical' periodic table to indicate the origin of all the elements we commonly (or not so commonly) encounter around us.
But this is just for the show. :) In reality, astrophysicists mostly refer to another, far less complex version of the periodic table. Because, we basically deal with only three elements - Hydrogen, Helium and everything else. And in an ingenuous fashion this 'everything else' is called 'metal'. This is not as crazy as it sounds. This 'astrophysical' periodic table actually reflects the composition of the Universe, the fractional amount of a particular elements being proportional to the area under its symbol.
Dmitri Ivanovich Mendeleev, father of the periodic table, used a balloon to ascend above the cloud cover to observe an eclipse on this day in 1887. I am sure, when he dabbled in his passion for Astronomy, he had no inclination that one day his periodic table would become such a favourite of Astronomers. :)



