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Methods of detecting exoplanets usually rely on indirect strategies – that is, they do not directly image the planet but deduce its existence from another signal. Any planet is an extremely faint light source compared to its parent star. For example, a star like the Sun is about a billion times as bright as the reflected light from any of the planets…
Characters, Established detection methods & Other possible methods
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planets star planet method stars light around transit exoplanet mass orbit detect space also using radial velocity planet's telescope first
| Subject | Predicate | Object | Confidence | Src |
|---|---|---|---|---|
| a neutron star or white dwarf | instance of | planets can completely occult a very small star | 0.80 | text |
| an event which would be easily detectable from Earth | instance of | planets can completely occult a very small star | 0.80 | text |
| the Kepler Space Observatory | instance of | such Jupiter-sized planets with an orbital period of a few days are detectable by space telescopes | 0.80 | text |
| the Nancy Grace Roman Space Telescope | instance of | in principle down to Mars mass with future space projects | 0.80 | text |
| the LUVOIR or the HabEx have been proposed.In 2010 | instance of | Concepts | 0.80 | text |
| a team from NASA's Jet Propulsion Laboratory demonstrated that a vortex coronagraph could enable small scopes to directly image planets | instance of | Concepts | 0.80 | text |
| ZIMPOL/CHEOPS | instance of | Groups | 0.80 | text |
| PlanetPol are currently using polarimeters to search for extrasolar planets | instance of | Groups | 0.80 | text |
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