π•Šπ•¦π•Ÿ’𝕀 ‘π•‹π•¨π•šπ•Ÿ’ ℍ𝕒𝕀 β„™π•π•’π•Ÿπ•–π•₯𝕒𝕣π•ͺ β„‚π• π•‘π•šπ•–π•€ 𝕠𝕗 π•π•¦π•‘π•šπ•₯𝕖𝕣 π•’π•Ÿπ•• ℕ𝕖𝕑π•₯π•¦π•Ÿπ•–, π•Šπ•”π•šπ•–π•Ÿπ•₯π•šπ•€π•₯𝕀 π•Šπ•’π•ͺ

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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