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TOI-849

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TOI-849 is a star system located about 700-741 light-years away from Earth in the constellation Sculptor. It hosts at least one known exoplanet, TOI-849 b.
TOI-849 b


  • Discovery: Discovered in 2020 by NASA's Transiting Exoplanet Survey Satellite (TESS), and confirmed by the HARPS spectrograph.
  • Type: It's considered a candidate chthonian planet, which is the exposed core of a gas giant that has lost most of its atmosphere.
  • Orbit: It orbits very closely to its star with the orbital period of 0.765 days (about 18 hours). The semi-major axis is 0.01598 AU.
  • Size: It has a radius of about 3.4 times that of Earth, similar to Neptune.
  • Mass: It's much more massive than Neptune, at about 39-40 times the mass of Earth.
  • Density: TOI-849 b has a high density of about 5.2-5.5 g/cm³, similar to Earth, and it is the densest Neptune-sized planet discovered.
  • Composition: It's believed to be the remnant core of a gas giant. The gaseous envelope is estimated to compose no more than about 4% of planet's mass.

Significance of TOI-849 bThe discovery of TOI-849 b is significant because:

  • It is the first discovery of its kind.
  • It provides a unique opportunity to study the core of a planet.
  • It offers new insights to the formation of planets.

Theories about TOI-849 b's exposed coreThere are two main theories:

1. It was once a gas giant like Jupiter but lost its outer gas due to factors like tidal disruption (being ripped apart by the star's gravity) or a collision with another planet.

2. It failed to form a substantial atmosphere in the first place.



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