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The article discusses a potential discovery of a giant planet located within the habitable zone around a very hot star called "HD 156295." This would be the first of its kind to be observed around a "Delta Scuti" type star. The planet, designated "HD 156295 b," is likely a gaseous planet with a mass approximately six times that of Jupiter. It orbits its star at a distance of four astronomical units and completes an orbit roughly every 2,200 days. The planet receives about 60% of the radiation that Earth gets from the Sun. Scientists estimate there is about a 50% chance that the detected signal is from a real planet, but its existence has not yet been confirmed. If confirmed, it would be the first planet observed within the habitable zone around such a star, contributing to our understanding of planet formation around hot stars. Future observations, especially using modern techniques such as "pulsar timing" and the European "Plato" space telescope mission, are expected to either confirm or rule out its existence.
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