A dataset provided by the European Space Agency

Proposal ID 076410
Title Simultaneous X-ray and ultraviolet observations of exoplanetary evaporation
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DOI https://doi.org/10.5270/esa-kfkpfl9
Principal Investigator, PI Dr Peter Wheatley
Abstract HST observations show that three of the brightest transiting exoplanets areevaporating (HD209458b, HD189733b and GJ436b) and models suggest that theevolution of close-in low-mass planets may be dominated by this mass loss.Simultaneous X-ray and ultraviolet observations of planetary transits are neededto constrain self-consistent models of the exoplanetary winds. Here we proposetransit observations of four bright exoplanets with XMM in order to determinemass loss rates.
Publications
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2015-05-13T12:24:02Z/2015-11-21T08:30:50Z
Version 17.56_20190403_1200
Mission Description The European Space Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs second cornerstone of the Horizon 2000 Science Programme. It carries 3 high throughput X-ray telescopes with an unprecedented effective area, and an optical monitor, the first flown on a X-ray observatory. The large collecting area and ability to make long uninterrupted exposures provide highly sensitive observations. Since Earths atmosphere blocks out all X-rays, only a telescope in space can detect and study celestial X-ray sources. The XMM-Newton mission is helping scientists to solve a number of cosmic mysteries, ranging from the enigmatic black holes to the origins of the Universe itself. Observing time on XMM-Newton is being made available to the scientific community, applying for observational periods on a competitive basis.
Creator Contact https://www.cosmos.esa.int/web/xmm-newton/xmm-newton-helpdesk
Date Published 2016-12-10T23:00:00Z
Keywords "mass loss rates", "XMM", "low mass planets", "planetary transits", "evaporating hd209458b", "HD209458", "constrain self", "mass loss", "exoplanetary winds", "exoplanetary evaporation", "bright exoplanets", "HST", "brightest transiting exoplanets"
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Dr Peter Wheatley, 2016, 'Simultaneous X-ray and ultraviolet observations of exoplanetary evaporation', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-kfkpfl9