Age analysis of extrasolar planets: Insight from stellar isochrone models
C. Swastik, Ravinder K. Banyal, Mayank Narang, Athira Unni, T. Sivarani
arXiv:2404.13398v1 Announce Type: new
Abstract: There is growing evidence from stellar kinematics and galactic chemical evolution (GCE) suggesting that giant planets (M$_{P}geq$0.3$M_{J}$) are relatively young compared to the most commonly occurring population of small planets (M$_{P} $10 days), implying that hot Jupiters could be the youngest systems to emerge in the progression of planet formation.arXiv:2404.13398v1 Announce Type: new
Abstract: There is growing evidence from stellar kinematics and galactic chemical evolution (GCE) suggesting that giant planets (M$_{P}geq$0.3$M_{J}$) are relatively young compared to the most commonly occurring population of small planets (M$_{P} $10 days), implying that hot Jupiters could be the youngest systems to emerge in the progression of planet formation.

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