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The planetary equilibrium temperature is a theoretical temperature that a planet would be if it were in radiative equilibrium, typically under the assumption that it radiates as a black body being heated only by its parent star. In this model, the presence or absence of an atmosphere (and therefore any greenhouse effect) is assumed to be irrelevant; the…
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| Subject | Predicate | Object | Confidence | Src |
|---|---|---|---|---|
| Planetary equilibrium temperature | is a | theoretical temperature that a planet would be if it were in radiative equilibrium | 0.90 | text |
| the orbital distance can be measured through radial velocity | instance of | Orbital properties of the planet | 0.80 | text |
| transit period measurements.Alternatively | instance of | Orbital properties of the planet | 0.80 | text |
| the planetary equilibrium may be written in terms of the temperature | instance of | Orbital properties of the planet | 0.80 | text |
| radius of the star as T e q | instance of | Orbital properties of the planet | 0.80 | text |
| Planetary equilibrium temperature | related to Calculation of equilibrium temperature | Consider | 0.60 | section |
| Planetary equilibrium temperature | related to Calculation of equilibrium temperature | The | 0.60 | section |
| Planetary equilibrium temperature | related to Calculation of equilibrium temperature | One | 0.60 | section |
| Planetary equilibrium temperature | related to Calculation of equilibrium temperature | Stefan | 0.60 | section |
| Planetary equilibrium temperature | related to Calculation of equilibrium temperature | Boltzmann | 0.60 | section |
| Planetary equilibrium temperature | related to Calculation of equilibrium temperature | Radiative | 0.60 | section |
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