# Qatar Exoplanet Survey: Qatar-7b -- A Very Hot Jupiter Orbiting a Metal   Rich F-Star

**Authors:** Khalid Alsubai, Zlatan Tsvetanov, David W. Latham, Allyson Bieryla,, Stylianos Pyrzas, Dimitris Mislis, Gilbert A. Esquerdo, Ali Esamdin, Jinzhong, Liu, Lu Ma, Marc Bretton, Enric Palle, Felipe Murgas, Nicolas P. E. Vilchez,, Timothy D. Morton, Hannu Parviainien, Pilar Montanes-Rodriguez, Norio Narita,, Akihiko Fukui, Nobuhiko Kusakabe, Motohide Tamura

arXiv: 1812.05601 · 2019-02-27

## TL;DR

Qatar-7b is a newly discovered very hot, inflated gas giant orbiting a metal-rich F-star, with extreme temperature and size, making it ideal for atmospheric studies.

## Contribution

This paper reports the discovery and characterization of Qatar-7b, a highly inflated hot Jupiter with unique properties among known exoplanets.

## Key findings

- Planet has a mass of 1.88 Mjup and radius of 1.70 Rjup.
- Orbital period is 2.032 days, with an equilibrium temperature of ~2100 K.
- Qatar-7b is among the top 6% hottest and largest known exoplanets.

## Abstract

We present the discovery of Qatar-7b --- a very hot and inflated giant gas planet orbiting close its parent star. The host star is a relatively massive main sequence F-star with mass and radius Mstar = 1.41 +/- 0.03 Msun and Rstar = 1.56 +/- 0.02 Rsun, respectively, at a distance d = 726 +/- 26 pc, and an estimated age ~1 Gyr. With its orbital period of P = 2.032 days the planet is located less than 5 stellar radii from its host star and is heated to a high temperature Teq ~ 2100 K. From a global solution to the available photometric and radial velocity observations, we calculate the mass and radius of the planet to be Mpl = 1.88 +/- 0.25 Mjup and Rpl = 1.70 +/- 0.03 Rjup, respectively. The planet radius and equilibrium temperature put Qatar-7b in the top 6% of the hottest and largest known exoplanets. With its large radius and high temperature Qatar-7b is a valuable addition to the short list of targets that offer the best opportunity for studying their atmospheres through transmission spectroscopy.

## Full text

_Full body text omitted from this summary view._ Fetch the complete paper as Markdown: https://tomesphere.com/paper/1812.05601/full.md

## Figures

10 figures with captions in the complete paper: https://tomesphere.com/paper/1812.05601/full.md

## References

80 references — full list in the complete paper: https://tomesphere.com/paper/1812.05601/full.md

---
Source: https://tomesphere.com/paper/1812.05601