An ESPRESSO view of HD 189733 system. Broadband transmission spectrum, differential rotation, and system architecture
arXiv (Cornell University)(2023)
摘要
The development of state-of-the-art spectrographs has ushered in a new era in
the detection and characterization of exoplanetary systems. Our objective is to
utilize the high-resolution and precision capabilities of the ESPRESSO
instrument to detect and measure the broad-band transmission spectrum of HD
189733b's atmosphere. Additionally, we aim to employ an improved
Rossiter-McLaughlin model to derive properties related to the velocity fields
of the stellar surface and to constrain the orbital architecture.
Our results demonstrate a high degree of precision in fitting the observed
radial velocities during transit using the improved modeling of the
Rossiter-McLaughlin effect. We tentatively detect the effect of differential
rotation with a confidence level of 93.4 % when considering a rotation
period within the photometric literature values, and 99.6% for a broader
range of rotation periods. For the former, the amplitude of differential
rotation ratio suggests an equatorial rotation period of 11.45± 0.09 days
and a polar period of 14.9± 2. The addition of differential rotation breaks
the latitudinal symmetry, enabling us to measure the true spin-orbit angle ψ≈ 13.6 ± 6.9 ^∘ and the stellar inclination axis angle i_⋆≈ 71.87 ^+6.91^∘_-5.55^∘. Moreover, we determine a
sub-solar amplitude of the convective blueshift velocity V_CB ≈
-211 ^+69 _-61 ms^-1, which falls within the expected range for
a K-dwarf host star and is compatible with both runs.
Finally, we successfully retrieved the transmission spectrum of HD 189733b
from the high-resolution ESPRESSO data. We observe a significant decrease in
radius with increasing wavelength, consistent with the phenomenon of
super-Rayleigh scattering.
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关键词
broadband transmission spectrum
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