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  "path": "/mission/roman-space-telescope/asteroseismology-using-the-galactic-bulge-time-domain-survey/",
  "publishedAt": "2026-02-10T17:03:49.000Z",
  "site": "https://science.nasa.gov",
  "tags": [
    "Asteroseismology Using The Galactic Bulge Time Domain Survey",
    "NASA Science"
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  "textContent": "Wide-Field Science – RegularMarc Pinsonneault / Ohio State University, PI Overview: Evolved red giant stars are detected as high-amplitude non-radial oscillators in time-domain space missions. Precise, regularly sampled, long-duration photometric observations can be used to characterize their oscillation frequency pattern. Masses, radii, and ages have been measured for tens of thousands of stars observed by […]\n\nThe post Asteroseismology Using The Galactic Bulge Time Domain Survey appeared first on NASA Science.",
  "title": "Asteroseismology Using The Galactic Bulge Time Domain Survey"
}