In the past decade, extrasolar planet scientists have been searching for a new world at a brisk pace. But as the increase in the number of planetary institutions in our galactic coefficient, how many of these possible, in fact, problems that are habitable have all reached a climax. The standards of habitability fall into a big discussion. This seems to be necessary on the surface of liquid water, but some researchers are suggesting that underground flow may also be a hotbed of primitive life. In both cases, water is a key component of the metabolic process in carbon-based life.
In addition, planets should have a solid surface, the same as Jupiter's gaseous planet world. Finally, the amount of gas that the planet should have. Gas blankets were found to contain large amounts of oxygen molecules and it is likely that life has spread all over the surface. Other molecules rapidly absorb oxygen, which will need to be supplemented by a biological process, in order to continuously supplement one of the planetary atmospheres with high concentrations.
With these conditions in mind, astronomers have created a formula for calculating the habitable area around stars. Based on the radiant energy of the star, this is directly related to its quality - scientists are able to determine the distance around the star and will be warm enough to maintain the liquid water of the planet, but not so much, the atmosphere is boiling.
Although this seems quite simple, the controversy continues. The specific variables used to perform the calculations are open interpretations, some of the parameter values ​​of the arguments and other broader ranges of narrower ranges proposed in their calculations. Some of the most recent works suggest that certain star types - such as the smallest red dwarf - may be completely poor incubator planets, and that the computational habitability zone will be a fairly close star, and therefore interaction with the solar magnetic field will hinder.
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