New Delhi: Utilizing an Artificial Intelligence-based algorithm, Indian Astronomers have devised a new approach for identifying potentially habitable planets with a high probability. As a result, around 60 potentially habitable planets have been found from 5000 total planets known.
According to the study conducted by astronomers from the Indian Institute of Astrophysics, an autonomous institute of the Department of Science & Technology, Government Of India, along with astronomers from BITS Pilani, Goa campus a new approach -- an anomaly detection method -- has been found by which potentially habitable planets with high probability can be identified.
"The method is based on the postulate that Earth is an anomaly, with the possibility of the existence of few other anomalies among thousands of data points...There are 60 potentially habitable planets out of about 5000 confirmed, and nearly 8000 candidate planets proposed. The assessment is based on their close similarity to Earth. These planets can be viewed as candidates for anomalous instances in a huge pool of `non-habitable' exoplanets," stated the official release from the Ministry of Science and Technology. "Earth being the only habitable planet among thousands of planets is defined as an anomaly. We explored whether similar 'anomaly candidates can be found using novel anomaly detection methods,' said Dr Snehanshu Saha of BITS Pilani.
The IIA team explained the fulcrum of the idea that postulates (potentially) habitable exoplanets as anomalies pivots around the well-known anomaly detection problem in predictive maintenance of industrial systems. An anomaly detection technique suitable for industrial systems applies equally well for habitable planet detection since in both cases, the anomaly detector is dealing with "imbalanced" data, where the anomalies (number of habitable exoplanets or anomalous behaviour of industrial components) are outliers. These are far less in number compared to the normal data.
However, with a large number of discovered exoplanets, finding those rare anomalous instances by characterizing them in terms of planetary parameters, types, populations, and, ultimately, the habitability potential requires the knowledge of multiple planetary parameters from observations. This, in turn, demands hours of expensive telescope time.