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  5. The ultra-hot-Jupiter KELT-16 b: dynamical evolution and atmospheric properties
 

The ultra-hot-Jupiter KELT-16 b: dynamical evolution and atmospheric properties

Journal
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY  
Date Issued
2022
Author(s)
Mancini, L.
•
Southworth, J.
•
Naponiello, L.
•
Baştürk, Ö.
•
Barbato, D.
•
Biagiotti, F.
•
BRUNI, IVAN  
•
Cabona, L.
•
D'Ago, G.
•
Damasso, Mario  
•
Erdem, A.
•
Evans, D.
•
Henning, Th
•
Öztürk, O.
•
RICCI, DAVIDE  
•
SOZZETTI, Alessandro  
•
Tregloan-Reed, J.
•
Yalçınkaya, S.
DOI
10.1093/mnras/stab2691
Abstract
We present broad-band photometry of 30 planetary transits of the ultra-hot-Jupiter KELT-16 b, using five medium-class telescopes. The transits were monitored through standard $B,\, V,\, R,\, I$ filters and four were simultaneously observed from different places, for a total of 36 new light curves. We used these new photometric data and those from the TESS space telescope to review the main physical properties of the KELT-16 planetary system. Our results agree with previous measurements but are more precise. We estimated the mid-transit times for each of these transits and combined them with others from the literature to obtain 69 epochs, with a time baseline extending over more than 4 yr, and searched for transit time variations. We found no evidence for a period change, suggesting a lower limit for orbital decay at 8 Myr, with a lower limit on the reduced tidal quality factor of $Q^{\prime }_{\star }\gt (1.9 \pm 0.8) \times 10^5$ with $95{{\ \rm per\ cent}}$ confidence. We built up an observational, low-resolution transmission spectrum of the planet, finding evidence of the presence of optical absorbers, although with a low significance. Using TESS data, we reconstructed the phase curve finding that KELT-16 b has a phase offset of 25.25 ± 14.03 °E, a day- and night-side brightness temperature of 3190 ± 61 K and 2668 ± 56 K, respectively. Finally, we compared the flux ratio of the planet over its star at the TESS and Spitzer wavelengths with theoretical emission spectra, finding evidence of a temperature inversion in the planet's atmosphere, the chemical composition of which is preferably oxygen-rich rather than carbon-rich.
Volume
509
Issue
1
Start page
1447
Uri
http://hdl.handle.net/20.500.12386/32320
Url
https://academic.oup.com/mnras/article/509/1/1447/6373473?login=true
http://arxiv.org/abs/2105.00889v3
Issn Identifier
0035-8711
Ads BibCode
2022MNRAS.509.1447M
Rights
open.access
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