Jul 17, 2024, 12:00 AM
Jul 17, 2024, 12:00 AM

Astronomers Identify Unusual Exoplanet with Unique Orbit on Journey to Becoming Hot Jupiter

Highlights
  • Astronomers have discovered a peculiar exoplanet featuring the most elongated and hairpin-like orbit ever recorded.
  • This exoplanet is theorized to be on a trajectory toward potentially transforming into a 'hot Jupiter.'
  • The findings could reshape our understanding of planetary formation and dynamics.
Story

**Astronomers Discover Unique Exoplanet with Eccentric Orbit and Temperature Extremes** Astronomers have identified a remarkable exoplanet, TIC 241249530 b, which features an unusually elongated orbit and experiences significant temperature fluctuations. Located approximately 1,100 light-years from Earth, this exoplanet orbits a primary star in a binary system, raising questions about how such massive planets end up in tight orbits much closer to their stars than Mercury is to the Sun. Lead researcher Arvind Gupta expressed surprise and excitement at the discovery, noting the long-standing search for exoplanets that could serve as precursors to hot Jupiters. The planet's orbit has an eccentricity of 0.94, making it the most oblong transiting exoplanet ever recorded. This extreme orbital shape results in dramatic temperature variations throughout its year, according to co-author Jason Wright. The research team conducted simulations to explore the planet's unusual orbital evolution, suggesting that it likely formed far from its host star in a circular orbit akin to Jupiter's. However, gravitational interactions with a misaligned secondary star have stretched TIC 241249530 b's orbit over time. The findings contribute to the understanding of how high-mass gas giants transition into hot Jupiters as they migrate from eccentric to more circular orbits. The discovery of TIC 241249530 b, alongside another known exoplanet, HD 80606 b, reinforces this theory. Researchers continue to seek additional examples of planets undergoing similar transformations, enhancing the knowledge of planetary evolution in binary star systems.

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