This new hypothesis, regarding a habitable environment in Venus’ clouds, has been published today in Proceedings of the National Academy of Sciences by a team of researchers from Cardiff University, MIT and Cambridge University.<\/p>\n
Scientists proposed a new theory which suggests that possible lifeforms in the clouds of Venus could be creating a cascade of chemical reactions that is resulting in the environment being more habitable. The self-sustaining chain of events could also offer an explanation to the many strange anomalies present in the planet\u2019s upper atmosphere that scientists have been debating for decades.<\/p>\n
Ammonia was first detected in the clouds of Venus in the 1970s, and has mystified scientists since, as it should not be produced through any chemical processes known on Venus. In the most recent study, researchers modelled a set of chemical processes to show that if ammonia is truly present, the gas would set off a cascade of chemical reactions that would neutralise surrounding droplets of sulfuric acid.<\/p>\n
This would increase the pH of the clouds from -11 to 0. While this is still acidic, this would be within the range of acidity that life could tolerate. The researchers noted that there are lifeforms on Earth<\/a> that produce ammonia to neutralise and make otherwise acidic environments habitable.<\/p>\n
\u201cWe know that life can grow in acid environments on Earth, but nothing as acid as the clouds of Venus were believed to be. But if something is making ammonia in the clouds, then that will neutralize some of the droplets, making them potentially more habitable,\u201d said Dr William Bains, one co-author of the study, from Cardiff University\u2019s School of Physics and Astronomy.<\/a><\/p>\n
The source of ammonia itself suggests a potentially habitable environment and is speculated that the most plausible explanation is a biological origin, rather than non-biological sources such as, lightning or volcanic eruptions. Past data from past missions to Venus revealed anomalies and chemical signatures that had gone unexplained for decades.<\/p>\n
\u201cAmmonia shouldn\u2019t be on Venus,\u201d said Professor Sara Seager, another co-author on the study, from MIT\u2019s Department of Earth, Atmospheric and Planetary Sciences<\/a> (EAPS). \u201cIt has hydrogen attached to it, and there\u2019s very little hydrogen around. Any gas that doesn\u2019t belong in the context of its environment is automatically suspicious for being made by life.\u201d<\/p>\n