2024年10月24日 · WASP-88 b is a gas giant exoplanet that orbits a F-type star. Its mass is 0.42 Jupiters, it takes 5 days to complete one orbit of its star, and is 0.06431 AU from its star. Its discovery was announced in 2014.

In 2013, one planet, named WASP-88b, was discovered on a tight, circular orbit. [3] The planet is highly inflated, and may be an easy target for atmospheric characterization. Planetary equilibrium temperature is 1775 K. [7] The planetary atmosphere transmission spectrum is gray and featureless, probably indicating a large concentration of hazes ...

The target uncertainty has been defined as the 1/12 of the target's transit duration (in 2029). CAMPAIGN: Planet included in one of the current observing campaings.; TTVs: Planet exhibiting strong Trasit Time Variations due to another planet or orbital decay.; ALERT: Observations in the last 2 years show an O-C greater than 10 minutes.; …

2013年12月6日 · WASP-88 b is a 0.56+-0.08 M_Jup planet orbiting a V=11.4 F6-type star (1.45+-0.05 M_sun, 2.08-0.06+0.12 R_sun, T_eff=6431+-130 K) with a period of 4.954000+-0.000019 days. With a radius of 1.70-0.07+0.13 R_Jup, it joins …

2021年6月28日 · We present ground-based optical transmission spectroscopy of the low-density hot Jupiter WASP-88b covering the wavelength range 4413-8333 Å with the FORS2 spectrograph on the Very Large Telescope.

2021年7月5日 · We present ground-based optical transmission spectroscopy of the low-density hot Jupiter WASP-88b covering the wavelength range of 4413−8333 Å with the FOcal Reducer Spectrograph (FORS2) on the Very Large Telescope.

Abstract: We present ground-based optical transmission spectroscopy of the low-density hot Jupiter WASP-88b covering the wavelength range of 4413−8333 Å with the FOcal Reducer Spectrograph (FORS2) on the Very Large Telescope. The FORS2 white light curves exhibit a significant time-correlated noise that we model using a Gaussian process and ...

High-contrast imaging with VLT/SPHERE. Detailed information about planet WASP-88 b and its parameters.

We present ground-based optical transmission spectroscopy of the low-density hot Jupiter WASP-88b covering the wavelength range 4413 − 8333 Å with the FORS2 spectrograph on the Very Large ...

We present ground-based optical transmission spectroscopy of the low-density hot Jupiter WASP-88b covering the wavelength range 4413 − 8333 Å with the FORS2 spectrograph on the Very Large ...