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  "path": "/articles/the-planet-that-shouldnt-be-there",
  "publishedAt": "2026-03-11T12:55:38.000Z",
  "site": "https://eos.org",
  "tags": [
    "News",
    "astronomy",
    "ESA",
    "exoplanets",
    "NASA",
    "planetary evolution",
    "planets",
    "Space & Planets",
    "telescopes",
    "unsolved mysteries",
    "CC BY-SA 3.0 IGO"
  ],
  "textContent": "LHS 1903 is a small red M dwarf star orbited by a rocky planet and two gaseous planets. In a recent study, scientists used the European Space Agency’s CHEOPS satellite to investigate a fourth planet in this system and discovered that it might be rocky, like Venus. This is surprising because a planet order of rocky-gaseous-gaseous-rocky in a planetary system is rarely observed in the universe. Credit: ESA, CC BY-SA 3.0 IGO",
  "title": "The Planet That Shouldn’t Be There"
}