21 January 2023

The Second Evolution

 Life on Earth has been shaped by Darwinian principles. As we know it today, life is controlled by the DNA. DNA pervades all cells of living bodies, whether animals or plants. Life started about 3.5 billion years ago with simple cells and probably some kind of RNA or even less-sophisticated information retention abilities. The evolution of life is staggering. One big step is the start of collaboration between several cells to form a superior entity. Multicellular organisms appeared quite late, probably only two billion years ago. 

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

The human species has nothing special in that respect and is completely relevant to life of Earth. It is just the end of a non-peculiar twig in the evolution bushy tree. 


 

It is just one species. One species alive today. However, the speed of evolution is limited by the generational renewing. At least a hundred generations are needed to see a new trend appearing. For example, the lactose-tolerant adults in Europe appeared only after several thousand years of selective pressure.

We posit that this second evolution is being swamped by a new one, simply because the third evolution is going much faster. More on that 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 evolved. 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:

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

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

New elements have since been synthetized in stars and at the end of their lives. These elements were then dispersed in galaxies. This is the chemical evolution.

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