A Testbed for Tidal Migration: the 3D Architecture of an Eccentric Hot Jupiter HD 118203 b Accompanied by a Possibly Aligned Outer Giant Planet
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2024
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| author | Zhang, Jingwen Huber, Daniel Weiss, Lauren M. Xuan, Jerry W. Burt, Jennifer A. Dai, Fei Saunders, Nicholas Petigura, Erik A. Rubenzahl, Ryan A. Winn, Joshua N. Wang, Sharon X. Van Zandt, Judah Brodheim, Max Claytor, Zachary R. Crossfield, Ian Deich, William Fulton, Benjamin J. Gibson, Steven R. Hill, Grant M. Holden, Bradford Householder, Aaron Howard, Andrew W. Isaacson, Howard Kaye, Stephen Lanclos, Kyle Laher, Russ R. Lubin, Jack Payne, Joel Roy, Arpita Schwab, Christian Shaum, Abby P. Walawender, Josh Wishnow, Edward Yeh, Sherry |
| author_facet | Zhang, Jingwen Huber, Daniel Weiss, Lauren M. Xuan, Jerry W. Burt, Jennifer A. Dai, Fei Saunders, Nicholas Petigura, Erik A. Rubenzahl, Ryan A. Winn, Joshua N. Wang, Sharon X. Van Zandt, Judah Brodheim, Max Claytor, Zachary R. Crossfield, Ian Deich, William Fulton, Benjamin J. Gibson, Steven R. Hill, Grant M. Holden, Bradford Householder, Aaron Howard, Andrew W. Isaacson, Howard Kaye, Stephen Lanclos, Kyle Laher, Russ R. Lubin, Jack Payne, Joel Roy, Arpita Schwab, Christian Shaum, Abby P. Walawender, Josh Wishnow, Edward Yeh, Sherry |
| contents | Characterizing outer companions to hot Jupiters plays a crucial role in deciphering their origins. We present the discovery of a long-period giant planet, HD 118203 c ($m_{c}=11.79^{+0.69}_{-0.63}\ \mathrm{M_{J}}$, $a_{c}=6.28^{+0.10}_{-0.11}$ AU) exterior to a close-in eccentric hot Jupiter HD 118203 b ($P_{b}=6.135\ \mathrm{days}$, $m_{b}=2.14\pm{0.12}\ \mathrm{M_{J}}$, $r_{b}=1.14\pm{0.029}\ \mathrm{R_{J}}$, $e_{b}=0.31\pm{0.007}$) based on twenty-year radial velocities. Using Rossiter-McLaughlin (RM) observations from the Keck Planet Finder (KPF), we measured a low sky-projected spin-orbit angle $λ_{b}=-11^{\circ}.7^{+7.6}_{-10.0}$ for HD 118203 b and detected stellar oscillations in the host star, confirming its evolved status. Combining the RM observation with the stellar inclination measurement, we constrained the true spin-orbit angle of HD 118203 b as $Ψ_{b}<33^{\circ}.5\ (2σ)$, indicating the orbit normal of the hot Jupiter nearly aligned with the stellar spin axis. Furthermore, by combining radial velocities and Hipparcos-Gaia astrometric acceleration, we constrained the line-of-sight mutual inclination between the hot Jupiter and the outer planet to be $9^{\circ}.8^{+16.2}_{-9.3}$ at $2σ$ level. HD 118203 is one of first hot Jupiter systems where both the true spin-orbit angle of the hot Jupiter and the mutual inclination between inner and outer planets have been determined. Our results are consistent with a system-wide alignment, with low mutual inclinations between the outer giant planet, the inner hot Jupiter, and the host star. This alignment, along with the moderate eccentricity of HD 118203 c, implies that the system may have undergone coplanar high-eccentricity tidal migration. Under this framework, our dynamical analysis suggests an initial semi-major axis of 0.3 to 3.2 AU for the proto-hot Jupiter. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2407_21377 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | A Testbed for Tidal Migration: the 3D Architecture of an Eccentric Hot Jupiter HD 118203 b Accompanied by a Possibly Aligned Outer Giant Planet Zhang, Jingwen Huber, Daniel Weiss, Lauren M. Xuan, Jerry W. Burt, Jennifer A. Dai, Fei Saunders, Nicholas Petigura, Erik A. Rubenzahl, Ryan A. Winn, Joshua N. Wang, Sharon X. Van Zandt, Judah Brodheim, Max Claytor, Zachary R. Crossfield, Ian Deich, William Fulton, Benjamin J. Gibson, Steven R. Hill, Grant M. Holden, Bradford Householder, Aaron Howard, Andrew W. Isaacson, Howard Kaye, Stephen Lanclos, Kyle Laher, Russ R. Lubin, Jack Payne, Joel Roy, Arpita Schwab, Christian Shaum, Abby P. Walawender, Josh Wishnow, Edward Yeh, Sherry Earth and Planetary Astrophysics Solar and Stellar Astrophysics Characterizing outer companions to hot Jupiters plays a crucial role in deciphering their origins. We present the discovery of a long-period giant planet, HD 118203 c ($m_{c}=11.79^{+0.69}_{-0.63}\ \mathrm{M_{J}}$, $a_{c}=6.28^{+0.10}_{-0.11}$ AU) exterior to a close-in eccentric hot Jupiter HD 118203 b ($P_{b}=6.135\ \mathrm{days}$, $m_{b}=2.14\pm{0.12}\ \mathrm{M_{J}}$, $r_{b}=1.14\pm{0.029}\ \mathrm{R_{J}}$, $e_{b}=0.31\pm{0.007}$) based on twenty-year radial velocities. Using Rossiter-McLaughlin (RM) observations from the Keck Planet Finder (KPF), we measured a low sky-projected spin-orbit angle $λ_{b}=-11^{\circ}.7^{+7.6}_{-10.0}$ for HD 118203 b and detected stellar oscillations in the host star, confirming its evolved status. Combining the RM observation with the stellar inclination measurement, we constrained the true spin-orbit angle of HD 118203 b as $Ψ_{b}<33^{\circ}.5\ (2σ)$, indicating the orbit normal of the hot Jupiter nearly aligned with the stellar spin axis. Furthermore, by combining radial velocities and Hipparcos-Gaia astrometric acceleration, we constrained the line-of-sight mutual inclination between the hot Jupiter and the outer planet to be $9^{\circ}.8^{+16.2}_{-9.3}$ at $2σ$ level. HD 118203 is one of first hot Jupiter systems where both the true spin-orbit angle of the hot Jupiter and the mutual inclination between inner and outer planets have been determined. Our results are consistent with a system-wide alignment, with low mutual inclinations between the outer giant planet, the inner hot Jupiter, and the host star. This alignment, along with the moderate eccentricity of HD 118203 c, implies that the system may have undergone coplanar high-eccentricity tidal migration. Under this framework, our dynamical analysis suggests an initial semi-major axis of 0.3 to 3.2 AU for the proto-hot Jupiter. |
| title | A Testbed for Tidal Migration: the 3D Architecture of an Eccentric Hot Jupiter HD 118203 b Accompanied by a Possibly Aligned Outer Giant Planet |
| topic | Earth and Planetary Astrophysics Solar and Stellar Astrophysics |
| url | https://arxiv.org/abs/2407.21377 |