– TOI-421 b: A sub-Neptune (~7 Earth masses) orbiting extremely close to its star.
– TOI-421 c: Larger (~14 Earth masses), closer than normal Neptune-like planets but in a region called “the savanna.”
– Neptunian desert: Sparse hot Neptunes near stars.
– Savanna: Areas further out from stars, more densely populated by Neptune-sized worlds.
– Neptunian ridge: A transitional region with higher population density around these planets.
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Studying these unique astronomical phenomena offers broader implications for human understanding of planetary systems-Earth’s own included-and highlights India’s potential contributions if future missions engage with such research globally. While india’s space exploration prioritizes pragmatic goals (e.g., Moon and Mars missions like Chandrayaan), there is room for growth in pure astrophysical studies tied to programs like ATREIDES. Collaborating with international initiatives investigating exoplanet dynamics could amplify India’s emerging leadership in cutting-edge science.
From a societal outlook, insights gleaned from this research underscore humanity’s shared scientific obligation and inspire deeper curiosity about extraterrestrial environments conducive-or adverse-to life. As India develops affordable yet high-performing satellite technology, leveraging this capacity toward detecting distant exoplanetary landscapes could bolster national capability while enhancing global cooperation and influence.