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A visual binary is a gravitationally bound binary star system that can be visually resolved as two separate stars, as opposed to a singular point source with fluctuating brightness. Like all binaries, a visual binary consists of two stars –usually– of different brightnesses, with the brighter star considered the primary and the fainter star considered…
Mass–luminosity relationship, Distance & Kepler's laws
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stars star mass binary luminosity two visual masses displaystyle system kepler's law orbit distance separation apparent parallax centre primary one
| Subject | Predicate | Object | Confidence | Src |
|---|---|---|---|---|
| Visual binary | is a | gravitationally bound binary star system that can be visually resolved as two separate stars | 0.90 | text |
| Visual binary | related to Determining stellar masses | Binary | 0.60 | section |
| Visual binary | related to Determining stellar masses | Before | 0.60 | section |
| Visual binary | related to Determining stellar masses | Kepler's | 0.60 | section |
| Visual binary | related to Determining stellar masses | Law | 0.60 | section |
| Visual binary | related to Determining stellar masses | Relative | 0.60 | section |
| Visual binary | related to Determining stellar masses | Earth | 0.60 | section |
| Visual binary | related to Determining stellar masses | If | 0.60 | section |
| Visual binary | related to Determining stellar masses | Due | 0.60 | section |
| Visual binary | related to Determining stellar masses | The | 0.60 | section |
| Visual binary | related to Determining stellar masses | Once | 0.60 | section |
| Visual binary | related to Determining stellar masses | Where | 0.60 | section |
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