According to Kepler observations, the most abundant kind of planets in the Milky Way is the super-Earths. These planets are larger than Earth but smaller than Neptune, and they have been observed in many planetary systems of the galaxy.
Super-earths range in size from 1 to 4 times larger than Earth and exist in many solar systems. They vary in composition from rocky to gaseous, which is important in the study of planets’ formation and potential life. The data about their transit, orbit, and sizes suggest that these planets are among the most frequent results of planet formation.
What are super-Earths and why are they so common
Super-Earths are those planets that have more mass than Earth but much less mass than ice giants such as Neptune.
Although super-Earths do not necessarily share the same composition or atmosphere as Earth, their size seems to be a very popular category among discovered exoplanets.The discovery by the Kepler Mission of NASA revealed the existence of planets in surprising numbers throughout our Galaxy. Planets with radii ranging from one to four times that of Earth are very common throughout the Milky Way.However, these planets are not commonly seen in our solar system.
This is why scientists think that their formation in other systems is natural, since the growth process in a protoplanetary disc can be very effective, but not always large enough for the formation of gas giants.
Insights from kepler mission and exoplanet surveys
The effectiveness of the Kepler Space Telescope has been its capability to find planets via the transit method, detecting fluctuations in the luminosity of a star when the planet crosses its path. The method is responsible for thousands of discoveries of exoplanets, among which super-Earths are particularly abundant.A study called ‘The False Positive Rate of Kepler and the Occurrence of Planets’, for example, states that “small planets are ubiquitous around Sun-like stars”. In other words, super-earths are common occurrences in planetary systems.More precisely, according to another source in the Annual Review of Astronomy and Astrophysics, based on their occurrence rate, “most stars host at least one planet of this size”.In conclusion, it can be safely assumed that the galaxy consists of many different planetary systems than ours.Planetary formation and the role of protoplanetary discsThe prevalence of super-earths correlates significantly with their formation. At the early stage of a star system, a rotating disc made of gas and dust, referred to as a protoplanetary disc, surrounds a nascent star. In such a disc, collisions between particles occur, which results in a growth of their mass.It appears that the development of super-earths involves less stringent parameters compared to the formation of gas giants.
As indicated by an article in Nature, efficient solid accretion will necessarily result in planet formation, specifically super-earths, in the case of moderately massive discs. Besides, migration phenomena that involve the movement of planets inward/outward in a disc may gather those planets in small orbits around stars.
What this means for habitability and future research
The abundance of super-earths also means that they have a lot to say about the chances of finding alien life forms.
Not all super-earths are habitable planets; however, those that contain conditions conducive to life may have liquid water based on their atmospheric composition and the distance between their orbits and the stars around which they orbit.Modern astronomy uses sophisticated instruments to study super-earths’ atmospheres, including the recently launched James Webb Space Telescope. The purpose is to detect chemical indicators in their atmospheres that would prove or refute that life exists on some of them.In conclusion, the findings that super-earths are the most common planets in the universe have altered our perception of planets in the universe. Even though there may be Earth-like planets in the cosmos, they are part of an even more expansive universe that contains planets that may be similar to ours but do not necessarily look like ours.
