Issue |
A&A
Volume 641, September 2020
|
|
---|---|---|
Article Number | A68 | |
Number of page(s) | 15 | |
Section | Planets and planetary systems | |
DOI | https://doi.org/10.1051/0004-6361/202037954 | |
Published online | 10 September 2020 |
The GAPS programme at TNG
XXIV. An eccentric Neptune-mass planet near the inner edge of the BD-11 4672 habitable zone★
1
Dipartimento di Fisica, Università degli Studi di Torino,
Via Pietro Giuria 1,
10125
Torino,
Italy
2
INAF – Osservatorio Astrofisico di Torino,
Via Osservatorio 20,
10025
Pino Torinese,
Italy
e-mail: domenico.barbato@inaf.it
3
Observatoire de Genève, Université de Genève,
51 Chemin des Maillettes,
1290
Sauverny,
Switzerland
4
INAF – Osservatorio Astrofisico di Catania,
Via S. Sofia 78,
95123
Catania,
Italy
5
INAF – Osservatorio Astronomico di Roma,
Via Frascati 33,
00078
Monte Porzio Catone,
Italy
6
INAF – Osservatorio Astronomico di Palermo,
Piazza del Parlamento 1,
90134
Palermo,
Italy
7
INAF – Osservatorio Astronomico di Padova,
Vicolo dell’Osservatorio 5,
35122
Padova,
Italy
8
Dipartimento di Fisica, Università di Roma Tor Vergata,
Via della Ricerca Scientifica 1,
00133
Roma,
Italy
9
Max Planck Institute for Astronomy,
Königstuhl 17,
69117
Heidelberg,
Germany
10
Fundación Galileo Galilei - INAF,
Rambla José Ana Fernandez Pérez 7,
38712
Breña Baja,
TF,
Spain
11
INAF – Osservatorio Astronomico di Trieste,
Via Tiepolo 11,
34143
Trieste,
Italy
12
INAF – Osservatorio Astronomico di Brera,
Via E. Bianchi 46,
23807
Merate (LC),
Italy
13
Astronomy Department and Van Vleck Observatory, Wesleyan University,
Middletown,
CT
06459,
USA
14
INAF – Osservatorio Astronomico di Capodimonte,
Salita Moiariello 16,
80131
Napoli,
Italy
15
Instituto de Astrofísica de Canarias,
C/Vía Láctea s/n,
38205
La Laguna,
Spain
16
INAF – Osservatorio Astronomico di Cagliari,
Via della Scienza 5,
09047
Selargius (CA),
Italy
17
Dipartimento di Fisica e Astronomia “G. Galilei”, Università di Padova,
Vicolo dell’Osservatorio 3,
35122
Padova,
Italy
18
INAF – Osservatorio Astrofisico di Arcetri,
Largo E. Fermi 5,
50125
Firenze,
Italy
Received:
13
March
2020
Accepted:
25
June
2020
Context. With the growth of comparative exoplanetology, it is becoming increasingly clear that investigating the relationships between inner and outer planets plays a key role in discriminating between competing formation and evolution models. To do so, it is important to probe the inner region of systems that host long-period giants in search of undetected lower-mass planetary companions.
Aims. In this work, we present our results on the K-dwarf star BD-11 4672, which is already known to host a long-period giant planet, as the first output of a subsample of the GAPS programme specifically aimed at assessing the impact of inefficient migration of planets formed beyond the snowline by searching for Neptune-mass and super-Earth planetary companions of known longer-period giants.
Methods. We used the high-precision HARPS-N observations of BD-11 4672 in conjunction with time series taken from the literature in order to search for additional inner planetary signals to be fitted using differential evolution Markov chain Monte Carlo. The long-term stability of the new orbital solutions was tested with N-body dynamical simulations.
Results. We report the detection of BD-11 4672 c, a new Neptune-mass planet with an orbital period of 74.20−0.08+0.06 d, eccentricity of 0.40−0.15+0.13, semimajor axis of 0.30 ± 0.01 au, and minimum mass 15.37−2.81+2.97 M⊕, orbiting slightly outside the inner edge of the optimistic circumstellar habitable zone. In order to assess its impact on the dynamical stability of the habitable zone, we computed the angular momentum deficit of the system, showing that planet c has a severe negative impact on the stability of possible additional lower-mass temperate planets. The BD-11 4672 system is notable for its architecture, hosting both a long-period giant planet and an inner lower-mass planet, the latter being one of the most eccentric Neptune-mass planets known at similar periods.
Key words: stars: individual: BD-11 4672 / techniques: radial velocities / planetary systems / planets and satellites: detection / planets and satellites: dynamical evolution and stability
© ESO 2020
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.