Main Neocene
Blue Chimera

Igor Kraj

Extraterrestrial life: “Heavy” planets

All pictures are taken from open sources and belong to their authors

Most of the currently discovered supposedly habitable worlds belong to the class of “super-earths” – planets significantly larger than Earth in mass, but not so heavy as to hold hydrogen and helium and turn to gas giants. So, it means that extraterrestrial life is likely to develop in conditions of high gravity. However, in part this situation may develop due to the fact that the big is seen from a distance. Moreover, at a distance more significant than small one. Then, other stars are very far away and it is just difficult to find Earth-sized or smaller planets near them.
Nevertheless, massive planets have significant advantages in terms of the emergence of habitable conditions on their surface. Even without a large moon, the super-earth will retain seismic activity that feeds the atmosphere and hydrosphere, while the leakage of gases into outer space will be minimal.
The problem of the super-earth, as a habitable planet, is rather that too much water and gases can accumulate on it. A planet several times the mass of the Earth and having, accordingly, a strong gravity, is highly likely to acquire an atmosphere comparable in density to that of Venus. Extra-heavy greenhouse effect can lead to overheating and evaporation of the oceans… Or maybe it won’t, since the boiling point also increases with increasing pressure.
In fact, extraterrestrial life is possible on three types of super-earths: “gas”, “liquid” and “solid” ones. By “gas” a planet is meant, whose habitable atmosphere is very dense. The surface of such a world may (with high probability) be completely covered with superheated, but not boiling water. It is less likely that there will be a place for the land on the surface. The continents and seas of the “gas” planet can also be inhabited, but they will not be the main zone of biomass synthesis. Like at the Venus, a thick gas cover will be able to absorb almost all the light. Thus photosynthesis will move into the atmosphere. Fortunately, it is in conditions when the atmosphere is only ten times less dense than water that an aerostatic method of movement will become convenient and expedient, allowing plants and animals to soar at a height convenient for them.
However, a separate article is already dedicated to the surreal wonders of inhabited worlds with a super-dense atmosphere.
Consequently, on a “liquid” super-earth, the atmosphere has a moderate density, and the photosynthesis zone is the ocean completely covering the surface. However, worlds with an endless sea and floating islands have also already been described. There is also an article on the channel about absolutely crazy “liquid” planets, whose oceans lack not only shores, but also a bottom.
However, the issue of “solid” super-earths, the most Earth-like ones, with a low-density atmosphere, quite ordinary oceans and vast expanses of habitable land, is not over. In fact, a solid super-earth will differ from our planet only in high gravity.
Of course, the increased gravity will not affect the evolution of marine life in any way. But the force that hinders the flapping wing flight and walking will direct the evolution of land creatures in a different way.
Only at first sight, the problem is solved simply — when gravity is doubled, animals will only have to halve their size in order to maintain the force-to-mass ratio. Actually, size is too serious a sacrifice that will not be made. After all, everything is simple in nature: the bigger one to eat.

A characteristic feature of animals of “heavy” worlds may be a vertical mouth.
The blue whale tips over on its side to turn, rather than lift its huge jaw. For
crawling creatures, the mouth opening to the sides is also more convenient.

Extraterrestrial life is subject to the same laws as terrestrial life. The first amphibians on our planet did not yet know how to walk and, resting on the ground with their fin-like paws, dragged their bellies protected by corneous plates over the rocks with difficulty. Only the second generation of land pioneers managed to get up a little on their feet, reducing friction when moving. But if gravity is 2g, moving on four points of support will become an impossible task for primitive vertebrates. No, they will not give up, but simply move to domination on land in a different way, taking up the development of progressive methods of crawling.
The “heavy” planet will turn into a kingdom of serpentine, legless creatures. In some sense, it will even spur evolution, since snakes are a more progressive and adapted form compared to lizards. In other respects, evolution will remain “earth-like”. Crawling animals will occupy all the niches of herbivores and predators, will grow fur in due time and will begin to feed their cubs with milk.
Flying animals, including insects, will most likely not appear at all on a heavy planet, since even for the smallest creatures with sufficient specific power to take off, this method of movement will be associated with excessive energy consumption. It is likely that it simply won’t come even to the appearance of the Hexapoda superclass, which includes winged insects. On a heavy planet, evolution will not follow the path of reducing the number of legs, since the millipede shape will be the most appropriate.

Translated by Pavel Volkov, 2021
The original Russian article is here

Main Neocene
Blue Chimera