Three planets transiting the evolved star EPIC 249893012: a hot 8.8-Mearth super-Earth and two warm 14.7 and 10.2-Mearth sub-Neptunes
Artikel i vetenskaplig tidskrift, 2020

We report the discovery of a new planetary system with three transiting planets, one super-Earth and two sub-Neptunes, that orbit EPIC 249893012, a G8 IV-V evolved star (M⋆ = 1.05 ± 0.05 M☉, R⋆ = 1.71 ± 0.04 R☉, Teff = 5430 ± 85 K). The star is just leaving the main sequence. We combined K2 photometry with IRCS adaptive-optics imaging and HARPS, HARPS-N, and CARMENES high-precision radial velocity measurements to confirm the planetary system, determine the stellar parameters, and measure radii, masses, and densities of the three planets. With an orbital period of 3.5949-0.0007+0.0007days, a mass of 8.75-1.08+1.09 M⊕, and a radius of 1.95-0.08+0.09 R⊕, the inner planet b is compatible with nickel-iron core and a silicate mantle (ρb = 6.39-1.04+1.19 g cm-3). Planets c and d with orbital periods of 15.624-0.001+0.001 and 35.747-0.005+0.005 days, respectively, have masses and radii of 14.67-1.89+1,84 M⊕ and 3.67-0.14+0.17 R⊕ and 10.18-2.42+2.46 M⊕ and 3.94-0.12+0.13 R⊕, respectively, yielding a mean density of 1.62-0.29+0.30 and 0.91-0.23+0.25 g cm-3, respectively. The radius of planet b lies in the transition region between rocky and gaseous planets, but its density is consistent with a rocky composition. Its semimajor axis and the corresponding photoevaporation levels to which the planet has been exposed might explain its measured density today. In contrast, the densities and semimajor axes of planets c and d suggest a very thick atmosphere. The singularity of this system, which orbits a slightly evolved star that is just leaving the main sequence, makes it a good candidate for a deeper study from a dynamical point of view.

planets and satellites: detection

planets and satellites: fundamental parameters

techniques: photometric

planetary systems

techniques: radial velocities

Författare

D. Hidalgo

E. Palle

D. Gandolfi

Malcolm Fridlund

Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik, Galaktisk astrofysik

Grzegorz Nowak

R. Luque

T. Hirano

A. B. Justesen

W. D. Cochran

O. Barragan

L Spina

F. Rodler

S. Albrecht

D. Anderson

P. J. Amado

E. Bryant

J. A. Caballero

Juan Cabrera

Szilard Csizmadia

F. Dai

J. de Leon

Hans Deeg

Ph. Eigmuller

M. Endl

A. Erikson

M. Esposito

P. Figueira

Iskra Georgieva

Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik, Galaktisk astrofysik

S. Grziwa

E. Guenther

Artie P. Hatzes

M. Hjorth

H. J. Hoeijmakers

P. Kabath

J. Korth

M. Kuzuhara

M. Lafarga

M. Lampon

I.C. Leão

J. Livingston

S. Mathur

Pilar Montanes Rodriguez

J. C. Morales

F. Murgas

E. Nagel

N. Narita

L. D. Nielsen

M. Patzold

Carina Persson

Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik, Galaktisk astrofysik

J. Prieto-Arranz

A. Quirrenbach

H. Rauer

S. Redfield

A. Reiners

I Ribas

A. Smith

J. Subjak

V. Van Eylen

P. A. Wilson

Astronomy and Astrophysics

0004-6361 (ISSN) 1432-0746 (eISSN)

Vol. 636 89-

Exoplaneter från rymden - CHEOPS och PLATO

Rymdstyrelsen, 2017-01-01 -- 2022-12-31.

Ämneskategorier

Astronomi, astrofysik och kosmologi

Fundament

Grundläggande vetenskaper

DOI

10.1051/0004-6361/201937080ARXIV: 2002.01755

Mer information

Skapat

2020-05-07