DOAJ Open Access 2025

HD 143811 AB b: A Directly Imaged Planet Orbiting a Spectroscopic Binary in Sco-Cen

Nathalie K. Jones Jason J. Wang Eric L. Nielsen Robert J. De Rosa Anne E. Peck +49 lainnya

Abstrak

We present confirmation of HD 143811 AB b, a substellar companion to spectroscopic binary HD 143811 AB through direct imaging with the Gemini Planet Imager (GPI) and Keck NIRC2. HD 143811 AB was observed as a part of the GPI Exoplanet Survey in 2016 and 2019 and is a member of the Sco-Cen star formation region. The exoplanet is detected ∼430 mas from the host star by GPI. With two GPI epochs and one from Keck/NIRC2 in 2022, we confirm through common proper motion analysis that the object is bound to its host star. We derive an orbit with a semimajor axis of $6{4}_{-14}^{+32}$ au and eccentricity ${0.23}_{-0.16}^{+0.24}$ . Spectral analysis of the GPI H -band spectrum and NIRC2 L′ photometry provides additional proof that this object is a substellar companion. We compare the spectrum of HD 143811 AB b to PHOENIX stellar models and Exo-Radioactive-Convective Equilibrium Model (REM) exoplanet atmosphere models and find that Exo-REM models provide the best fits to the data. From the Exo-REM models, we derive an effective temperature of $104{2}_{-132}^{+178}$ K for the planet and translate the derived luminosity of the planet to a mass of 5.6 ± 1.1 M _Jup assuming hot-start evolutionary models. HD 143811 AB b is the first directly imaged planet around a binary that is not on an ultrawide orbit. Future characterization of this object will shed light on the formation of planets around binary star systems.

Topik & Kata Kunci

Penulis (54)

N

Nathalie K. Jones

J

Jason J. Wang

E

Eric L. Nielsen

R

Robert J. De Rosa

A

Anne E. Peck

W

William Roberson

J

Jean-Baptiste Ruffio

J

Jerry W. Xuan

B

Bruce A. Macintosh

S

S. Mark Ammons

V

Vanessa P. Bailey

T

Travis S. Barman

J

Joanna Bulger

E

Eugene Chiang

J

Jeffrey K. Chilcote

G

Gaspard Duchêne

T

Thomas M. Esposito

M

Michael P. Fitzgerald

K

Katherine B. Follette

S

Stephen Goodsell

J

James R. Graham

A

Alexandra Z. Greenbaum

P

Pascale Hibon

P

Patrick Ingraham

P

Paul Kalas

Q

Quinn M. Konopacky

M

Michael C. Liu

F

Franck Marchis

J

Jérôme Maire

C

Christian Marois

B

Brenda Matthews

D

Dimitri Mawet

S

Stanimir Metchev

M

Maxwell A. Millar-Blanchaer

R

Rebecca Oppenheimer

D

David W. Palmer

J

Jenny Patience

M

Marshall D. Perrin

L

Lisa Poyneer

L

Laurent Pueyo

A

Abhijith Rajan

J

Julien Rameau

F

Fredrik T. Rantakyrö

B

Bin Ren

A

Aniket Sanghi

D

Dmitry Savransky

A

Adam C. Schneider

A

Anand Sivaramakrishnan

A

Adam J. R. W. Smith

I

Inseok Song

R

Remi Soummer

S

Sandrine Thomas

K

Kimberly Ward-Duong

S

Schuyler G. Wolff

Format Sitasi

Jones, N.K., Wang, J.J., Nielsen, E.L., Rosa, R.J.D., Peck, A.E., Roberson, W. et al. (2025). HD 143811 AB b: A Directly Imaged Planet Orbiting a Spectroscopic Binary in Sco-Cen. https://doi.org/10.3847/2041-8213/ae2007

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Informasi Jurnal
Tahun Terbit
2025
Sumber Database
DOAJ
DOI
10.3847/2041-8213/ae2007
Akses
Open Access ✓