Proposal ID | 076410 |
Title | Simultaneous X-ray and ultraviolet observations of exoplanetary evaporation |
Download Data Associated to the proposal | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0764100501 |
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 |
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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 |