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| Artist impression of the planetary system around the star LHS 1903 Image Credit: © ESA |
Scientific Frontline: "At a Glance" Summary
- Main Discovery: Identification of LHS 1903 e, a rocky planet located beyond gas giants in the LHS 1903 system, contradicting the standard inner-rocky/outer-gas planetary hierarchy.
- Methodology: Utilized high-precision photometry from the ESA CHEOPS satellite to detect the planet, followed by planetary formation simulations to confirm an "inside-out" formation sequence and exclude migration or collision hypotheses.
- Key Data: Located 116 light-years from Earth around an M-type red dwarf; the fourth planet shares a similar mass with the inner third planet (a gas giant) yet possesses a rocky composition.
- Significance: Provides observational evidence for the inside-out planet formation theory, indicating that planets can form sequentially after the dissipation of protoplanetary disk gas rather than simultaneously.
- Future Application: Refinement of planetary accretion simulations to incorporate asynchronous formation timelines and better characterization of atypical planetary system architectures.
- Branch of Science: Astrophysics and Exoplanetology
- Additional Detail: Analysis indicates LHS 1903 e formed significantly later than its gas giant siblings, occurring only after the protoplanetary disk had been depleted of gas.


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