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![Representative image of the solar system. [Image: Reuters]](https://images.news18.com/ibnlive/uploads/2020/11/1604494522_untitled-design-2020-11-04t182350.117.png?impolicy=website&width=534&height=356 "Representative image of the solar system. [Image: Reuters]")
Representative image of the solar system. [Image: Reuters]
They used data from NASA’s Transiting Exoplanet Survey Satellite (TESS) observatory to present the torch emission analysis process.
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New research based on data procured by a team led by researcher Dimitra Atri of the Center for Space Science at NYU Abu Dhabi (NYUAD) suggests that stars are more likely to be habitable exoplanets than other space bodies. The research is based on the calculated erosion rates of planetary atmospheres.
The study was established in a paper presented by Atri and fellow graduate Shane Carberry Mogan titled “Star Rockets Versus Luminosity: XUV-Induced Atmospheric Escape and Planetary Habitability.”
They used data from NASA’s Transiting Exoplanet Survey Satellite (TESS) observatory to present the torch emission analysis process. It was published in the Royal Astronomical Society’s Monthly Notices: Letters.
The research team noted that the high frequency of lower energy rockets had a greater impact on the exoplanet’s atmosphere than less frequent higher energy rockets. They also noted and determined how different types of stellar atmospheres produce extreme ultraviolet (XUV) radiation through stellar flare and its resulting effects on nearby planets.
Atri said: “Given the proximity of exoplanets to host stars, it is very important to understand how time in space is related to the events of those stars that can affect the extent of the exoplanet’s habitability.” He also pointed out that the next step in the research would be to study stellar flare data from a series of stars to analyze the long-term effects of stellar activity to identify new exoplanets worthy of being habitable.
Atmospheric sustenance is one of the most important requirements of a habitable planet. The new research sheds light on the exoplanet’s habitability as the effects of stellar activity are not yet well understood. The study highlights the need for better numerical modeling of atmospheric escape. It also provides insight into how planets release atmospheric gases into space, as it leads to erosion and decreased habitability of the planet.
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