Characterization of the Host Binary of the Directly Imaged Exoplanet HD 143811 AB b

Fuente: arXiv
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Hauptverfasser: Peck, Anne E., Roberson, William, Nielsen, Eric L., De Rosa, Robert J., Jones, Nathalie, Wang, Jason, Macintosh, Bruce, Lewis, Bailey L., Duchêne, Gaspard, Metchev, Stanimir, Abbas, Asif, Xuan, Jerry W., Sanghi, Aniket, Panience, Jennifer, Barman, Travis S., Bulger, Joanna, Chilcote, Jeffrey K., Esposito, Thomas M., Fitzgerald, Michael P., Follette, Katherine B., Gallamore, Hannah, Goodsell, Stephen, Graham, James R., Greenbaum, Alexandra Z., Hibon, Pascale, Ingraham, Patrick, Kalas, Paul, Konopacky, Quinn M., Marchis, Franck, Maire, Jérôme, Marois, Christian, Matthews, Brenda, Mawet, Dimitri, Millar-Blanchaer, Maxwell A., Oppenheimer, Rebecca, Palmer, David W., Perrin, Marshall D., Pointer, Lisa, Pueyo, Laurent, Rajan, Abhijith, Rameau, Julien, Rantakyrö, Fredrik T., Ren, Bin, Ruffio, Jean-Baptiste, Savransky, Dmitry, Schneider, Adam C., Sivaramakrishnan, Anand, Smith, Adam J. R. W., Song, Inseok, Summer, Remi, Thomas, Sandrine, Ward-Duong, Kimberly, Wolff, Schuyler G.
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Veröffentlicht: 2025
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author Peck, Anne E.
Roberson, William
Nielsen, Eric L.
De Rosa, Robert J.
Jones, Nathalie
Wang, Jason
Macintosh, Bruce
Lewis, Bailey L.
Duchêne, Gaspard
Metchev, Stanimir
Abbas, Asif
Xuan, Jerry W.
Sanghi, Aniket
Panience, Jennifer
Barman, Travis S.
Bulger, Joanna
Chilcote, Jeffrey K.
Esposito, Thomas M.
Fitzgerald, Michael P.
Follette, Katherine B.
Gallamore, Hannah
Goodsell, Stephen
Graham, James R.
Greenbaum, Alexandra Z.
Hibon, Pascale
Ingraham, Patrick
Kalas, Paul
Konopacky, Quinn M.
Marchis, Franck
Maire, Jérôme
Marois, Christian
Matthews, Brenda
Mawet, Dimitri
Millar-Blanchaer, Maxwell A.
Oppenheimer, Rebecca
Palmer, David W.
Perrin, Marshall D.
Pointer, Lisa
Pueyo, Laurent
Rajan, Abhijith
Rameau, Julien
Rantakyrö, Fredrik T.
Ren, Bin
Ruffio, Jean-Baptiste
Savransky, Dmitry
Schneider, Adam C.
Sivaramakrishnan, Anand
Smith, Adam J. R. W.
Song, Inseok
Summer, Remi
Thomas, Sandrine
Ward-Duong, Kimberly
Wolff, Schuyler G.
author_facet Peck, Anne E.
Roberson, William
Nielsen, Eric L.
De Rosa, Robert J.
Jones, Nathalie
Wang, Jason
Macintosh, Bruce
Lewis, Bailey L.
Duchêne, Gaspard
Metchev, Stanimir
Abbas, Asif
Xuan, Jerry W.
Sanghi, Aniket
Panience, Jennifer
Barman, Travis S.
Bulger, Joanna
Chilcote, Jeffrey K.
Esposito, Thomas M.
Fitzgerald, Michael P.
Follette, Katherine B.
Gallamore, Hannah
Goodsell, Stephen
Graham, James R.
Greenbaum, Alexandra Z.
Hibon, Pascale
Ingraham, Patrick
Kalas, Paul
Konopacky, Quinn M.
Marchis, Franck
Maire, Jérôme
Marois, Christian
Matthews, Brenda
Mawet, Dimitri
Millar-Blanchaer, Maxwell A.
Oppenheimer, Rebecca
Palmer, David W.
Perrin, Marshall D.
Pointer, Lisa
Pueyo, Laurent
Rajan, Abhijith
Rameau, Julien
Rantakyrö, Fredrik T.
Ren, Bin
Ruffio, Jean-Baptiste
Savransky, Dmitry
Schneider, Adam C.
Sivaramakrishnan, Anand
Smith, Adam J. R. W.
Song, Inseok
Summer, Remi
Thomas, Sandrine
Ward-Duong, Kimberly
Wolff, Schuyler G.
contents HD~143811~AB is the host star to the directly imaged planet HD~143811~AB~b, which was recently discovered using data from the Gemini Planet Imager and Keck NIRC2. A member of the Sco-Cen star-forming region with an age of $13 \pm 4$ Myr, HD~143811~AB is somewhat rare among hosts of directly imaged planets as it is a close stellar binary, with an $\sim$18 day period. Accurate values for the orbital and stellar parameters of this binary are needed to understand the formation and evolutionary history of the planet in orbit. We utilize archival high-resolution spectroscopy from FEROS on the MPG/ESO 2.2-meter telescope to fit the orbit of the binary, and combine with unresolved photometry to derive the basic stellar properties of the system. From the orbit, we derive precise values of orbital period of $18.59098 \pm 0.00007$ days, and mass ratio of $0.885 \pm 0.003$. When combined with stellar evolutionary models, we find masses of both components of $M_A = 1.30^{+0.03}_{-0.05}$ M$_\odot$ and $M_B = 1.15^{+0.03}_{-0.04}$ M$_\odot$. While the current data are consistent with the planet and stellar orbits being coplanar, the 3D orientations of both systems are currently poorly constrained, with additional observations required to more rigorously test for coplanarity.
format Preprint
id arxiv_https___arxiv_org_abs_2509_06727
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Characterization of the Host Binary of the Directly Imaged Exoplanet HD 143811 AB b
Peck, Anne E.
Roberson, William
Nielsen, Eric L.
De Rosa, Robert J.
Jones, Nathalie
Wang, Jason
Macintosh, Bruce
Lewis, Bailey L.
Duchêne, Gaspard
Metchev, Stanimir
Abbas, Asif
Xuan, Jerry W.
Sanghi, Aniket
Panience, Jennifer
Barman, Travis S.
Bulger, Joanna
Chilcote, Jeffrey K.
Esposito, Thomas M.
Fitzgerald, Michael P.
Follette, Katherine B.
Gallamore, Hannah
Goodsell, Stephen
Graham, James R.
Greenbaum, Alexandra Z.
Hibon, Pascale
Ingraham, Patrick
Kalas, Paul
Konopacky, Quinn M.
Marchis, Franck
Maire, Jérôme
Marois, Christian
Matthews, Brenda
Mawet, Dimitri
Millar-Blanchaer, Maxwell A.
Oppenheimer, Rebecca
Palmer, David W.
Perrin, Marshall D.
Pointer, Lisa
Pueyo, Laurent
Rajan, Abhijith
Rameau, Julien
Rantakyrö, Fredrik T.
Ren, Bin
Ruffio, Jean-Baptiste
Savransky, Dmitry
Schneider, Adam C.
Sivaramakrishnan, Anand
Smith, Adam J. R. W.
Song, Inseok
Summer, Remi
Thomas, Sandrine
Ward-Duong, Kimberly
Wolff, Schuyler G.
Earth and Planetary Astrophysics
Solar and Stellar Astrophysics
HD~143811~AB is the host star to the directly imaged planet HD~143811~AB~b, which was recently discovered using data from the Gemini Planet Imager and Keck NIRC2. A member of the Sco-Cen star-forming region with an age of $13 \pm 4$ Myr, HD~143811~AB is somewhat rare among hosts of directly imaged planets as it is a close stellar binary, with an $\sim$18 day period. Accurate values for the orbital and stellar parameters of this binary are needed to understand the formation and evolutionary history of the planet in orbit. We utilize archival high-resolution spectroscopy from FEROS on the MPG/ESO 2.2-meter telescope to fit the orbit of the binary, and combine with unresolved photometry to derive the basic stellar properties of the system. From the orbit, we derive precise values of orbital period of $18.59098 \pm 0.00007$ days, and mass ratio of $0.885 \pm 0.003$. When combined with stellar evolutionary models, we find masses of both components of $M_A = 1.30^{+0.03}_{-0.05}$ M$_\odot$ and $M_B = 1.15^{+0.03}_{-0.04}$ M$_\odot$. While the current data are consistent with the planet and stellar orbits being coplanar, the 3D orientations of both systems are currently poorly constrained, with additional observations required to more rigorously test for coplanarity.
title Characterization of the Host Binary of the Directly Imaged Exoplanet HD 143811 AB b
topic Earth and Planetary Astrophysics
Solar and Stellar Astrophysics
url https://arxiv.org/abs/2509.06727