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In astronomy, the main sequence is a classification of stars which appear on plots of stellar color versus brightness as a continuous and distinctive band. Stars spend the majority of their lives on the main sequence, during which core hydrogen burning is dominant. These main-sequence stars, or sometimes interchangeably dwarf stars, are the most numerous…
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stars star sequence mass main energy core hydrogen main-sequence luminosity helium temperature fusion star's convection stellar sun known dwarf nuclear
| Subject | Predicate | Object | Confidence | Src |
|---|---|---|---|---|
| Main sequence | is a | classification of stars which appear on plots of stellar color versus brightness as a continuous and distinctive band | 0.90 | text |
| red dwarfs | instance of | dwarfs | 0.80 | text |
| orange dwarfs | instance of | dwarfs | 0.80 | text |
| and yellow dwarfs are indeed much smaller | instance of | dwarfs | 0.80 | text |
| dimmer than other stars of those colors | instance of | dwarfs | 0.80 | text |
| Sirius may transport energy primarily by radiation | instance of | with little or no convection.Intermediate-mass stars | 0.80 | text |
| with a small core convection region | instance of | with little or no convection.Intermediate-mass stars | 0.80 | text |
| Main sequence | related to Classification | Main | 0.60 | section |
| Main sequence | related to Classification | O-type | 0.60 | section |
| Main sequence | related to Dwarf terminology | Main-sequence | 0.60 | section |
| Main sequence | related to Dwarf terminology | For | 0.60 | section |
| Main sequence | related to Dwarf terminology | However | 0.60 | section |
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