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19 April 2024 |
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NGTS-5b: a highly inflated planet offering insights into the sub-Jovian desert | | Philipp Eigmüller
; Alexander Chaushev
; Edward Gillen
; Alexis Smith
; Louise D. Nielsen
; Oliver Turner
; Szilard Czismadia
; Barry Smalley
; Daniel Bayliss
; Claudia Belardi
; François Bouchy
; Matthew R. Burleigh
; Juan Cabrera
; Sarah L. Casewell
; Bruno Chazelas
; Benjamin F. Cooke
; Anders Erikson
; Boris T. Gänsicke
; Maximilian N. Günther
; Michael R. Goad
; Andrew Grange
; James A. G. Jackman
; James S. Jenkins
; James McCormac
; Maximiliano Moyano
; Don Pollacco
; Katja Poppenhaeger
; Didier Queloz
; Liam Raynard
; Heike Rauer
; Stéphane Udry
; Simon. R. Walker
; Christopher A. Watson
; Richard G. West
; Peter J. Wheatley
; | | Date: |
Tue, 7 May 2019 14:03:01 GMT (11887kb,D) | | Abstract: | Context: Planetary population analysis gives us insight into formation and
evolution processes. For short-period planets, the subJovian desert has been
discussed in recent years with regard to the planet population in the
mass/period and radius/period parameter space without taking stellar parameters
into account. The Next Generation Transit Survey (NGTS) is optimised for
detecting planets in this regime, which allows for further analysis of the
sub-Jovian desert.
Aims: With high-precision photometric surveys (e.g. with NGTS and TESS),
which aim to detect short period planets especially around M/K-type host stars,
stellar parameters need to be accounted for when empirical data are compared to
model predictions. Presenting a newly discovered planet at the boundary of the
sub-Jovian desert, we analyse its bulk properties and use it to show the
properties of exoplanets that border the sub-Jovian desert.
Methods: Using NGTS light curve and spectroscopic follow-up observations, we
confirm the planetary nature of planet NGTS-5b and determine its mass. Using
exoplanet archives, we set the planet in context with other discoveries.
Results: NGTS-5b is a short-period planet with an orbital period of 3.3569866
+- 0.0000026 days. With a mass of 0.229 +- 0.037 MJup and a radius of 1.136 +-
0.023 RJup, it is highly inflated. Its mass places it at the upper boundary of
the sub-Jovian desert. Because the host is a K2 dwarf, we need to account for
the stellar parameters when NGTS-5b is analysed with regard to planet
populations.
Conclusions: With red-sensitive surveys (e.g. with NGTS and TESS), we expect
many more planets around late-type stars to be detected. An empirical analysis
of the sub-Jovian desert should therefore take stellar parameters into account. | | Source: | arXiv, 1905.2593 | | Services: | Forum | Review | PDF | Favorites | |
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