Scientists have discovered conclusive evidence of a rocky exoplanet with a substantial atmosphere circling an ancient star outside our solar system, upending long-held assumptions that extremely small planets can't sustain thick atmospheres.
Located about 280 light-years from Earth, TOI-561 b orbits a 10-billion-year-old G-type star at a scorching distance of less than one million miles. The planet's peculiar composition is marked by an unusually low density, making it difficult to comprehend how such a small world could maintain a substantial atmosphere given the intense radiation emanating from its host star.
Using NASA's Webb Space Telescope, researchers probed TOI-561 b and found conclusive evidence suggesting that it's encircled by a thick atmosphere. This groundbreaking discovery not only dispels the notion of tiny planets unable to support atmospheric gases but also provides valuable insights into the possibility of life on exoplanets with extreme conditions.
Theories had long suggested that such small, tidally locked worlds would be too hot to sustain atmospheres due to their extremely close proximity to their host stars. However, the planet's low density – not akin to a super-puff but rather less dense than expected for an Earth-like composition – appears to defy expectations.
One potential explanation lies in the planet's extremely volatile-rich atmosphere and a hypothetical equilibrium between its magma ocean and atmosphere. It is believed that as gases escape into space due to radiation from the host star, they are simultaneously drawn back into the interior by the magma ocean, allowing the atmosphere to persist.
Scientists now believe that TOI-561 b must be an exceptionally volatile-rich world – "like a wet lava ball" in terms of its atmospheric composition. This remarkable exoplanet serves as a fascinating example of how complex and mysterious planetary atmospheres can be, with its intriguing properties leaving room for further research into the possibility of life on other worlds.
The study's findings have significant implications for our understanding of rocky exoplanets, particularly those orbiting ancient stars. As researchers continue to unravel the mysteries surrounding TOI-561 b and its extraordinary atmosphere, they may uncover more secrets about the nature of life beyond Earth.
Located about 280 light-years from Earth, TOI-561 b orbits a 10-billion-year-old G-type star at a scorching distance of less than one million miles. The planet's peculiar composition is marked by an unusually low density, making it difficult to comprehend how such a small world could maintain a substantial atmosphere given the intense radiation emanating from its host star.
Using NASA's Webb Space Telescope, researchers probed TOI-561 b and found conclusive evidence suggesting that it's encircled by a thick atmosphere. This groundbreaking discovery not only dispels the notion of tiny planets unable to support atmospheric gases but also provides valuable insights into the possibility of life on exoplanets with extreme conditions.
Theories had long suggested that such small, tidally locked worlds would be too hot to sustain atmospheres due to their extremely close proximity to their host stars. However, the planet's low density – not akin to a super-puff but rather less dense than expected for an Earth-like composition – appears to defy expectations.
One potential explanation lies in the planet's extremely volatile-rich atmosphere and a hypothetical equilibrium between its magma ocean and atmosphere. It is believed that as gases escape into space due to radiation from the host star, they are simultaneously drawn back into the interior by the magma ocean, allowing the atmosphere to persist.
Scientists now believe that TOI-561 b must be an exceptionally volatile-rich world – "like a wet lava ball" in terms of its atmospheric composition. This remarkable exoplanet serves as a fascinating example of how complex and mysterious planetary atmospheres can be, with its intriguing properties leaving room for further research into the possibility of life on other worlds.
The study's findings have significant implications for our understanding of rocky exoplanets, particularly those orbiting ancient stars. As researchers continue to unravel the mysteries surrounding TOI-561 b and its extraordinary atmosphere, they may uncover more secrets about the nature of life beyond Earth.