WASP-18b

id: wasp-18b-292-6845723
title: WASP-18b
text: WASP-18b is an exoplanet that is notable for having an orbital period of less than one day. It has a mass equal to 10 Jupiter masses, just below the boundary line between planets and brown dwarfs. Due to tidal deceleration, it is expected to spiral toward and eventually merge with its host star, WASP-18, in less than a million years. The planet is approximately 3.1 million km from its star, which is about 400 light-years from Earth. A team led by Coel Hellier, a professor of astrophysics at Keel
brand slug: wiki
category slug: encyclopedia
description: Extrasolar planet that has an orbital period of less than one day
original url: https://en.wikipedia.org/wiki/WASP-18b
date created:
date modified: 2023-11-27T21:07:32Z
main entity: {"identifier":"Q1061955","url":"https://www.wikidata.org/entity/Q1061955"}
image: {"content_url":"https://upload.wikimedia.org/wikipedia/commons/8/8c/PIA22087-Exoplanet-Wasp18b-COinStratosphere-20171129.jpg","width":2700,"height":2282}
fields total: 13
integrity: 15

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