Precise mass and radius determination for two new and one known Neptune-sized planets around G dwarf hosts
Journal article, 2026

As part of the KESPRINT collaboration, we present the discovery and characterization of three exoplanets in the sub-Neptune to super-Neptune regime, spanning key regions of the exo-Neptunian landscape. TOI-1472 c and TOI-1648 b are newly discovered sub-Neptunes, while TOI-1472 b is a previously known super-Neptune for which we provide an improved mass measurement. These planets have orbital periods of 6–15 d and radii of 2.5–4.1 R(Formula presented), probing regions where planet formation and atmospheric evolution remain poorly understood. We combine Transiting Exoplanet Survey Satellite transit photometry with ground-based radial velocities to determine precise masses, radii, and orbital properties. TOI-1472 b has a mass of (Formula presented)  M(Formula presented) and a radius of (Formula presented)  R(Formula presented), TOI-1472 c has a mass of (Formula presented)  M(Formula presented) and a radius of (Formula presented)  R(Formula presented), and TOI-1648 b has a mass of (Formula presented)  M(Formula presented) and a radius of (Formula presented)  R(Formula presented). The planets exhibit a range of eccentricities (0.041–0.178), indicating diverse evolutionary histories. TOI-1648 b, with a high transmission spectroscopy metric ((Formula presented) ), is a promising target for atmospheric characterization. Together, these three planets provide precise constraints on the structure, composition, and dynamical evolution of small to intermediate-sized exoplanets, enriching our understanding of the exo-Neptunian landscape.

techniques: radial velocities

exoplanets

planets and satellites: detection

techniques: photometric

Author

Ilaria Carleo

Instituto de Astrofísica de Canarias

Istituto nazionale di astrofisica (INAF)

G. Nowak

Nicolaus Copernicus University (SGMK)

F. Murgas

Instituto de Astrofísica de Canarias

University of La Laguna

Enric Palle

Instituto de Astrofísica de Canarias

University of La Laguna

G. Lacedelli

University of La Laguna

Instituto de Astrofísica de Canarias

T. Masseron

University of La Laguna

Instituto de Astrofísica de Canarias

Emily W. Wong

University of Geneva

A. Castro-González

University of Geneva

D. Jankowski

Nicolaus Copernicus University (SGMK)

Patrick Eggenberger

University of Geneva

James S. Jenkins

Diego Portales University

Centro de Astrofísica y Tecnologías Afines (CATA),

K. Goździewski

Nicolaus Copernicus University (SGMK)

V. Bourrier

University of Geneva

Douglas R. Alves

Centro de Astrofísica y Tecnologías Afines (CATA),

University of Chile (UCH)

José I. Vines

Universidad Catolica del Norte

Keivan G. Stassun

Vanderbilt University

M. Brogi

Istituto nazionale di astrofisica (INAF)

University of Turin

Sergio Messina

Istituto nazionale di astrofisica (INAF)

Catherine A. Clark

California Institute of Technology (Caltech)

Karen A. Collins

Harvard-Smithsonian Center for Astrophysics

H. Deeg

Instituto de Astrofísica de Canarias

University of La Laguna

Elise Furlan

California Institute of Technology (Caltech)

D. Gandolfi

University of Turin

Samuel Geraldía González

Instituto de Astrofísica de Canarias

University of La Laguna

Coel Hellier

Keele University

A. Hatzes

Thüringer Landessternwarte Tautenburg

S.B. Howell

National Aeronautics and Space Administration (NASA)

Judith Korth

University of Geneva

Emil Knudstrup

Aarhus University

Chalmers, Space, Earth and Environment, Astronomy and Plasmaphysics

J. Lillo-Box

European Space Agency (ESA)

J.H. Livingston

National Astronomical Observatory of Japan

National Institutes of Natural Sciences

The Graduate University for Advanced Studies (SOKENDAI)

J. Orell-Miquel

University of Texas

Carina Persson

Chalmers, Space, Earth and Environment, Astronomy and Plasmaphysics

S. Redfield

Wesleyan University

B. S. Safonov

Moscow State University

D. Baker

Austin College

William D. Cochran

University of Texas

Rafael Delfin Barrena Delgado

Instituto de Astrofísica de Canarias

University of La Laguna

Allyson Bieryla

Harvard-Smithsonian Center for Astrophysics

A. W. Boyle

California Institute of Technology (Caltech)

The University of North Carolina System

P. Bosch-Cabot

Albanyà Astronomical Observatory

Núria Casasayas Barris

Instituto de Astrofísica de Canarias

University of La Laguna

Stavros Chairetas

Instituto de Astrofísica de Canarias

D. R. Ciardi

California Institute of Technology (Caltech)

A. Fukui

University of Tokyo

Instituto de Astrofísica de Canarias

P. Guerra

Albanyà Astronomical Observatory

Kiyoe Kawauchi

College of Life Sciences

Florence Libotte

Instituto de Astrofísica de Canarias

Sabadell Astronomical Society

Belgian Institute for Space Aeronomy (BIRA-IASB)

M. B. Lund

California Institute of Technology (Caltech)

R. Luque

Spanish National Research Council (CSIC)

Eduardo Lorenzo Martín Guerrero de Escalante

Instituto de Astrofísica de Canarias

Bob Massey

Villa’39 Observatory

Edward J. Michaels

Waffelow Creek Observatory

Giuseppe Morello

Spanish National Research Council (CSIC)

Istituto nazionale di astrofisica (INAF)

Norio Narita

National Institutes of Natural Sciences

University of Tokyo

Instituto de Astrofísica de Canarias

Hannu Parvianien

University of La Laguna

Instituto de Astrofísica de Canarias

R. Schwarz

Harvard-Smithsonian Center for Astrophysics

Avi Shporer

Massachusetts Institute of Technology (MIT)

M. Stangret

Instituto de Astrofísica de Canarias

University of La Laguna

Cristilyn N. Watkins

Montana State University

Monthly Notices of the Royal Astronomical Society

00358711 (ISSN) 13652966 (eISSN)

Vol. 549 3 staf1958

Subject Categories (SSIF 2025)

Astronomy, Astrophysics, and Cosmology

Subatomic Physics

DOI

10.1093/mnras/staf1958

More information

Latest update

6/18/2026