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HD 35843: A Sun-like Star Hosting a Long-period Sub-Neptune and Inner Super-Earth

Abstract:
We report the discovery and confirmation of two planets orbiting the metal-poor Sun-like star HD 35843 (TOI 4189). HD 35843 c is a temperate sub-Neptune transiting planet with an orbital period of 46.96 days that was first identified by Planet Hunters TESS. We combine data from TESS and follow-up observations to rule out false-positive scenarios and validate the planet. We then use ESPRESSO radial velocities (RVs) to confirm the planetary nature and characterize the planet’s mass and orbit. Further analysis of these RVs reveals the presence of an additional planet, HD 35843 b, with a period of 9.90 days and a minimum mass of 5.84 ± 0.84 M⊕. For HD 35843 c, a joint photometric and spectroscopic analysis yields a radius of 2.54 ± 0.08 R⊕, a mass of 11.32 ± 1.60 M⊕, and an orbital eccentricity of e = 0.15 ± 0.07. With a bulk density of 3.80 ± 0.70 g cm−3, the planet might be rocky with a substantial H2 atmosphere or it might be a “water world.” With an equilibrium temperature of ∼480 K, HD 35843 c is among the coolest ∼5% of planets discovered by TESS. Combined with the host star’s relative brightness (V = 9.4), HD 35843 c is a promising target for atmospheric characterization that will probe this sparse population of temperate sub-Neptunes.
Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.3847/1538-3881/add7d7

Authors


Publisher:
American Astronomical Society
Journal:
Astronomical Journal More from this journal
Volume:
170
Issue:
2
Article number:
108
Publication date:
2025-07-22
Acceptance date:
2025-04-14
DOI:
EISSN:
1538-3881
ISSN:
0004-6256


Language:
English
Keywords:
Pubs id:
2267499
Local pid:
pubs:2267499
Source identifiers:
3135314
Deposit date:
2025-07-22
ARK identifier:
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