Table 5
Comparison of WASP-7 b parameters with those of other hot and ultra-hot Jupiters.
Planet | Teq (K) | H(a) (km) | ΔA (10−3) | D2 line contrast (%) | D2 FWHM (Å) | D1 line contrast (%) | D1 FWHM (Å) | Refs.(d) |
---|---|---|---|---|---|---|---|---|
WASP-76 b | 2160 | 1479 | 0.23 | 0.37 ± 0.09 | 0.61 ± 0.17 | 0.50 ± 0.08 | 0.68 ± 0.12 | 1, A |
WASP-121 b | 2358 | 1011 | 0.26 | 0.69 ± 0.12 | 0.73 ± 0.09 | 0.25 ± 0.09 | 0.9 ± 0.1 | 2, B |
WASP-21 b | 1333 | 951 | 0.25 | ![]() |
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0.31 ± 0.05 | 3, C |
WASP-52 b | 1315 | 672 | 0.4 | 1.31 ± 0.13 | 0.42 ± 0.03 | 1.09 ± 0.16 | 0.22 ± 0.03 | 4, D |
WASP-7 b | 1530 | 383 | 0.07 | 0.50 ± 0.06 | 0.13 ± 0.02 | 0.13 ± 0.04 | 0.13 ± 0.02 | 5,E |
WASP-7 b (alt)(c) | 0.49 ± 0.05 | 0.17 ± 0.02 | 0.19 ± 0.03 | 0.17 ± 0.02 | 5,E | |||
MASCARA-2 b | 2260 | 315 | 0.06 | 0.29 ± 0.04 | 0.16 ± 0.02 | 0.29 ± 0.04 | 0.15 ± 0.02 | 6, F |
HD 189733 b | 1140 | 200 | 0.11 | 0.64 ± 0.07 | 0.52 ± 0.08 | 0.40 ± 0.07 | 0.52 ± 0.08 | 7, G |
Notes. (a) Atmospheric scale height. (b) Fraction of the stellar disk covered by an atmospheric annulus with a height of one scale height. (c) For WASP-7 b we show the result of the modeling by considering all spectra and by ignoring ten post-transit spectra (alt). (d) The numerals specify references for Na i D line contrasts and FWHMs, and letters denote references for the planetary effective temperature. We calculated the scale heights based on the references.
References. (1) Seidel et al. (2019); (A) West et al. (2016); (2) Cabot et al. (2020); (B) Delrez et al. (2016); (3) Chen et al. (2020a); (C) Ciceri et al. (2013); (4) Chen et al. (2020b); (D) Hébrard et al. (2013); (5) this work; (E) Southworth (2012); (6) Casasayas-Barris et al. (2019); (F) Talens et al. (2018); (7, G) Wyttenbach et al. (2015).
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