The exciting discovery of Gliese 12 b – an exoplanet with potential for life

Exciting discovery of the exoplanet Gliese 12 b with the potential for life at a distance of 40 light years

A team of scientists has discovered the exoplanet Gliese 12b orbiting a stable red dwarf at a distance of 40 light-years, providing hope for the possibility of life and new research.

Exciting discovery of the exoplanet Gliese 12 b with the potential for life at a distance of 40 light years
Photo by: Domagoj Skledar/ arhiva (vlastita)

Exciting discovery of a new planet with potential for life


In a groundbreaking discovery, a team of scientists has confirmed the existence of the exoplanet Gliese 12 b, a planet the size of Earth located just 40 light years away from us, within the so-called "habitable zone." The habitable zone, or "Goldilocks zone," is a region around a star where conditions exist that potentially allow for the presence of liquid water on the planet's surface, which is one of the key elements for life as we know it. This discovery represents a significant step forward in the search for life beyond our solar system and opens up a range of possibilities for further research.


The exoplanet Gliese 12 b, discovered by the team of scientists within the InfraRed Doppler Subaru Strategic Program (IRD-SSP), orbits a red dwarf star, Gliese 12. Red dwarfs are much smaller and cooler than our Sun, making them ideal candidates for the study of exoplanets. Due to their lower mass and reduced radiation, planets orbiting these stars are easier to detect and may have more favorable conditions for developing life forms. Unlike other stars with intense energy outbursts, Gliese 12 has proven to be a remarkably stable red dwarf, which increases the chances of habitability for its planets.


Temperature and the possibility of water on the surface


A particularly interesting aspect of the planet Gliese 12 b is its position in the habitable zone. Specifically, the planet is located very close to the inner edge of this zone, meaning it receives enough light from its star to potentially have liquid water, but not so much that it would evaporate. Although the planet receives a similar amount of radiation as Venus does from the Sun, the stable conditions of its star could provide a more favorable climate. Nevertheless, further observations are crucial to confirm the presence of water, as well as the composition of the atmosphere, which could provide better insights into the potential conditions for life.


One of the methods that will be used for further studying Gliese 12 b is spectral analysis, which will enable the examination of the atmospheric composition. When the planet passes in front of its star (i.e., during a transit), some of the starlight passes through the planet's atmosphere, allowing scientists to identify the gases present, such as oxygen, water, methane, or carbon dioxide. This method has previously been used to identify potential biosignatures on other exoplanets and is a key tool for studying planets like Gliese 12 b.


Accessibility for further research


Another advantage of this planet is its relative proximity to Earth. At a distance of 40 light years, Gliese 12 b allows for detailed investigations using existing and upcoming telescopes like the James Webb Space Telescope and future telescopes on Earth. Scientists will have the opportunity to study not only the planet's atmosphere but also other important elements such as its surface, climate, and the potential existence of a magnetic field that could protect any life from cosmic radiation.


Particularly important for the possibility of life is the study of conditions that make this planet different from other planets in the habitable zone. Comparisons between Gliese 12 b and Venusian conditions will provide answers to questions about what makes a planet suitable for life while others, despite similar positions, have inhospitable conditions. This is an important question that could contribute to a better understanding of the conditions on Earth as well as the evolution of atmospheric and surface conditions necessary for sustaining life.


Opportunity for discoveries that answer the eternal question


The discovery of Gliese 12 b brings new hope in the search for life beyond Earth. Given that red dwarfs are the most common type of stars in the Milky Way, finding a planet like Gliese 12 b suggests that such worlds may be common, further bolstering scientists' optimism. According to current observations, red dwarfs like Gliese 12 emit powerful energy outbursts much less frequently than TRAPPIST-1, increasing the likelihood of stable conditions needed for life.


The James Webb Telescope, along with other upcoming instruments, will become a key tool for further investigation of such planets. The goal of scientists is to study atmospheric composition, uncover potential signs of biological processes, and understand the possibilities of climatic systems that support life. Gliese 12 b represents an important step toward answering the question that humanity has been asking for centuries: Are we alone in the universe?


In a world increasingly turning its gaze to the skies, each such advancement further inspires people worldwide to continue looking to the stars and seeking new discoveries. Gliese 12 b thus becomes a symbol of human curiosity and hope, bringing us a step closer to understanding the universe in which we live.

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