Secondary eclipses of WASP-18b – near-infrared observations with the Anglo-Australian Telescope, the Magellan Clay Telescope and the LCOGT network

Kedziora-Chudczer, L. and Zhou, G. ORCID: https://orcid.org/0000-0002-4891-3517 and Bailey, J. and Bayliss, D. D. R. and Tinney, C. G. and Osip, D. and Colon, K. D. and Shporer, A. and Dragomir, D. (2018) Secondary eclipses of WASP-18b – near-infrared observations with the Anglo-Australian Telescope, the Magellan Clay Telescope and the LCOGT network. Monthly Notices of the Royal Astronomical Society, 483 (4). pp. 5110-5122. ISSN 0035-8711

[img]
Preview
Text (Published Version)
sty3381.pdf

Download (8MB) | Preview

Abstract

We present new eclipse observations for one of the hottest 'hot Jupiters', WASP-18b, for which previously published data from HST WFC3 and Spitzer have led to radically conflicting conclusions about the composition of this planet's atmosphere. We measure eclipse depths of 0.15± 0.02 per cent at Ks and 0.07± 0.01 per cent at z′ bands. Using the vstar line-by-line radiative transfer code and both these new observations with previously published data, we derive a new model of the planetary atmosphere. We have varied both the metallicity and C/O ratio in our modelling, and find no need for the extreme metallicity suggested by Sheppard et al. Our best-fitting models slightly underestimate the emission at z′ band and overestimate the observed flux at Ksband. To explain these discrepancies, we examine the impact on the planetary emission spectrum of the presence of several types of hazes which could form on the night side of the planet. Our Ks-band eclipse flux measurement is lower than expected from clear atmosphere models and this could be explained by haze particles larger than 0.2 μm with the optical properties of Al 2 O 3 , CaTiO 3 or MgSiO 3 . We find that z′-band measurements are important for understanding the contribution of photochemical hazes with particles smaller than 0.1 μm at the top of the atmosphere.


Statistics for USQ ePrint 45000
Statistics for this ePrint Item
Item Type: Article (Commonwealth Reporting Category C)
Refereed: Yes
Item Status: Live Archive
Faculty/School / Institute/Centre: No Faculty
Faculty/School / Institute/Centre: No Faculty
Date Deposited: 07 Feb 2022 02:56
Last Modified: 14 Feb 2022 00:44
Uncontrolled Keywords: occultations; planets and satellites: atmospheres; planets and; satellites: individual: WASP-18b; Astrophysics - Earth and Planetary; Astrophysics
Fields of Research (2008): 02 Physical Sciences > 0201 Astronomical and Space Sciences > 020110 Stellar Astronomy and Planetary Systems
Fields of Research (2020): 51 PHYSICAL SCIENCES > 5101 Astronomical sciences > 510109 Stellar astronomy and planetary systems
Socio-Economic Objectives (2008): E Expanding Knowledge > 97 Expanding Knowledge > 970102 Expanding Knowledge in the Physical Sciences
Socio-Economic Objectives (2020): 28 EXPANDING KNOWLEDGE > 2801 Expanding knowledge > 280120 Expanding knowledge in the physical sciences
Identification Number or DOI: https://doi.org/10.1093/mnras/sty3381
URI: http://eprints.usq.edu.au/id/eprint/45000

Actions (login required)

View Item Archive Repository Staff Only