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HD 183579b: a warm sub-Neptune transiting a solar twin detected by TESS

Hellier

HD 183579b: a warm sub-Neptune transiting a solar twin detected by TESS Thumbnail


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Abstract

We report the discovery and characterization of a transiting warm sub-Neptune planet around the nearby bright (V = 8.75 mag, K = 7.15 mag) solar twin HD 183579, delivered by the Transiting Exoplanet Survey Satellite (TESS). The host star is located 56.8 ± 0.1 pc away with a radius of R* = 0.97 ± 0.02?R? and a mass of M* = 1.03 ± 0.05?M?. We confirm the planetary nature by combining space and ground-based photometry, spectroscopy, and imaging. We find that HD 183579b (TOI-1055b) has a radius of Rp = 3.53 ± 0.13?R? on a 17.47 d orbit with a mass of Mp = 11.2 ± 5.4?M? (3s mass upper limit of 27.4?M?). HD 183579b is the fifth brightest known sub-Neptune planet system in the sky, making it an excellent target for future studies of the interior structure and atmospheric properties. By performing a line-by-line differential analysis using the high-resolution and signal-to-noise ratio HARPS spectra, we find that HD 183579 joins the typical solar twin sample, without a statistically significant refractory element depletion.

Acceptance Date Jul 28, 2021
Publication Date Oct 1, 2021
Journal Monthly Notices of the Royal Astronomical Society
Print ISSN 0035-8711
Publisher Oxford University Press
Pages 2220 - 2240
DOI https://doi.org/10.1093/mnras/stab2224
Publisher URL https://academic.oup.com/mnras/article-abstract/507/2/2220/6335490?redirectedFrom=fulltext

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