HD 160691 e vs HD 28185 b

HD 160691 e is one of the planets associated with the mu Arae system, which orbits the nearby solar-type star HD 160691 in the constellation Ara. The system became a benchmark for radial-velocity studies because several companions were reported around the same star, including objects with very different orbital periods and inferred masses. HD 160691 e is described as a gas giant and is identified...

HD 28185 b is a giant exoplanet orbiting the Sun-like star HD 28185 in the constellation Eridanus. Its orbit takes about 383 days, giving it a period close to Earth's year, and its orbital distance places it within estimates of the star's habitable zone. The planet itself is not considered Earth-like because it is a gas giant, but its orbit makes the system relevant to studies of planetary formati...