21 January 2023

The Second Evolution

Darwinian principles have shaped life on Earth. We know today that life is controlled by DNA. DNA is present in every cell of every living organism, whether animal or plant. Life began 3.5 billion years ago with simple cells and probably some kind of RNA or even less sophisticated information retention capabilities. The evolution of life is nothing short of staggering. One major step is the start of collaboration between several cells to form a superior entity. Multicellular organisms appeared quite late, probably only half a billion years ago.

Darwin's On the Origin of Species and the discovery of DNA as the repository of life information put the theory of evolution on very solid grounds. Life on Earth is evolving, and this means that gradual changes have appeared that make all living species adapted to their environment. Two ingredients are necessary: the randomness of the rare DNA mutations and the natural selection process that filters out the un-adapted ones. 

The human species is no more special than any other and is completely relevant to the life of Earth. It is simply the end of a non-unique branch in the evolutionary tree.


 

It is, in fact, just one species. There is only one species alive today. However, evolution is limited by the generational renewal. A new trend will emerge after at least a hundred generations. For example, the lactose-tolerant adults in Europe appeared only after several thousand years of selective pressure.

We are convinced that this second evolution is being swamped by a new one, simply because the third evolution is going much faster. I will explain more about this later.

08 January 2023

The First Evolution

The Universe as we see it today was very different in the past. Evolution is a gradual change over time, and the Universe has been evolving. It is still changing now.

Compare this image of colliding galaxies (the Stephan Quintet as recently observed by the JWST) in a nearby region of the Universe:

 
with the state of the Universe 13.8 billion years ago (as revealed by the Planck satellite) :

When the Universe was 380 thousand years old, it was much smoother or more homogeneous: we see relative temperature differences of about one part in a hundred million. Then, gravitation and the electromagnetic force have shaped the world into galaxies, stars, and so on. Even before this first photo of the infant Universe, the simple atomic elements (hydrogen, helium, and lithium) were formed in the first minutes, by the strong and weak forces. But no carbon was created at all.

Since then, new elements have been synthesised in stars, including carbon, and at the end of their lives. These elements were then distributed throughout the galaxies. This is chemical evolution.

The fate of the Universe is clear: it will go into dilution, with neighbouring regions moving further and further apart, and stars dying. Small pockets of the Universe will continue their "life" - a constant struggle against entropy.