
The discovery of TIC 241249530 b, a high-mass, transiting warm Jupiter with an extreme orbital eccentricity of e = 0.94, provides observational evidence supporting the high-eccentricity tidal-migration pathway for the formation of hot Jupiters.


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The spectroscopic and photometric observations of a high-mass, transiting warm Jupiter, TIC 241249530 b, with an orbital eccentricity of 0.94, provide evidence that hot Jupiters may have formed by means of a high-eccentricity tidal-migration pathway.

A hot-Jupiter progenitor on a super-eccentric retrograde orbit - Nature

discovery-of-a-high-mass-highly-eccentric-warm-jupiter-exoplanet-providing-insights-into-hot-jupiter-formation


Discovery of a High-Mass, Highly Eccentric Warm Jupiter Exoplanet Providing Insights into Hot Jupiter Formation
