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In this video, we explore the perplexing size gap that exists between super-Earths and mini-Neptunes in the exoplanet population. Recent studies from nearby star clusters have revealed that a significant majority of young exoplanets actually fall into this missing middle category, suggesting a shrinkage process occurs over time. The video discusses two main theories for this phenomenon - atmospheric loss due to stellar radiation or core heat - and presents the latest findings that may lean towards the latter. The video concludes by inviting viewers to ponder the implications of these discoveries and to engage in discussion about potential other causes for this exoplanetary gap. Viewers are encouraged to subscribe for more space-related content.