๐•Š๐•ฆ๐•Ÿ’๐•ค ‘๐•‹๐•จ๐•š๐•Ÿ’ โ„๐•’๐•ค โ„™๐•๐•’๐•Ÿ๐•–๐•ฅ๐•’๐•ฃ๐•ช โ„‚๐• ๐•ก๐•š๐•–๐•ค ๐• ๐•— ๐•๐•ฆ๐•ก๐•š๐•ฅ๐•–๐•ฃ ๐•’๐•Ÿ๐•• โ„•๐•–๐•ก๐•ฅ๐•ฆ๐•Ÿ๐•–, ๐•Š๐•”๐•š๐•–๐•Ÿ๐•ฅ๐•š๐•ค๐•ฅ๐•ค ๐•Š๐•’๐•ช

he first of these, HIP 104045 b, weighs about half as much as Jupiter and orbits its star in 6.3 years. The second, HIP 104045 c, is a hot superneptune: it is about 2.5 times the mass of Neptune but moves closer to the star in a 316-day orbit, similar to Earth.

“Small Earth-sized planets are more common than giant planets. These factors open precedents to the search for Earth-like planets around Sun-like stars by primarily looking for Jupiter-like planets,” writes an international team of astronomers led by Thiago Ferreira of the University of Sao Paulo in Brazil.

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