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The transiting planet has a mean density of 4.85\u22120.74<\/jats:sub>+0.84<\/jats:sup> g cm\u22123<\/jats:sup> and an analysis of its internal structure reveals that it is expected to have a small volatile envelope accounting for 0.35% of the mass at most. The star\u2019s brightness and the proximity of the inner planet to what is know as the radius gap make it an interesting candidate for transmission spectroscopy, which could further constrain the composition and internal structure of TOI 1062b.<\/jats:p>","DOI":"10.1051\/0004-6361\/202040247","type":"journal-article","created":{"date-parts":[[2021,6,7]],"date-time":"2021-06-07T08:14:11Z","timestamp":1623053651000},"page":"A105","source":"Crossref","is-referenced-by-count":7,"title":["TESS and HARPS reveal two sub-Neptunes around TOI 1062"],"prefix":"10.1051","volume":"653","author":[{"given":"J. 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