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A Cepheid variable (/ˈsɛfi.ɪd, ˈsiːfi-/) is a type of variable star that pulsates radially, varying in both diameter and temperature. It changes in brightness, with a well-defined stable period (typically 1–100 days) and amplitude. Cepheids are important cosmic benchmarks for scaling galactic and extragalactic distances; a strong direct relationship…
History, Classes & Uncertain distances
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cepheids cepheid classical helium variables type ionized stars ii star pulsation period distance variable doubly luminosity hubble known distances delta
| Subject | Predicate | Object | Confidence | Src |
|---|---|---|---|---|
| RS Puppis | instance of | calibrated by direct observation of the parallax distance to the closest Cepheids | 0.80 | text |
| Polaris.Cepheids change brightness due to the κ | instance of | calibrated by direct observation of the parallax distance to the closest Cepheids | 0.80 | text |
| RS Puppis.Delta Cephei is also of particular importance as a calibrator of the Cepheid period-luminosity relation since its distance is among the most precisely established for a Cepheid | instance of | due in part to discoveries | 0.80 | text |
| partly because it is a member of a star cluster | instance of | due in part to discoveries | 0.80 | text |
| the availability of precise parallaxes observed by the Hubble | instance of | due in part to discoveries | 0.80 | text |
| Hipparcos | instance of | due in part to discoveries | 0.80 | text |
| and Gaia space telescopes | instance of | due in part to discoveries | 0.80 | text |
| Cepheid variable | related to Anomalous Cepheids | RR Lyrae | 0.60 | section |
| Cepheid variable | related to Anomalous Cepheids | Anomalous Cepheid | 0.60 | section |
| Cepheid variable | related to Anomalous Cepheids | II Cepheids | 0.60 | section |
| Cepheid variable | related to Anomalous Cepheids | Sun | 0.60 | section |
| Cepheid variable | related to Anomalous Cepheids | It | 0.60 | section |
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