A dataset provided by the European Space Agency

Name: Planet-Star Interactions in Eccentric Sytems
Published: 2011-09-11T00:00:00Z
License: https://creativecommons.org/licenses/by-nc/3.0/igo

Proposal ID	065303
Title	Planet-Star Interactions in Eccentric Sytems
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0653030501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0653030601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0653030701
DOI	https://doi.org/10.5270/esa-2fdoa92
Principal Investigator, PI	Dr Dennis Bodewits
Abstract	Extrasolar planets orbiting on short orbital distances have violent planet-starinteractions that determine their survival and evolution. We propose to utilizethe unique geometry of giant planets in elliptical orbits to study planet-starinteractions with XMM. Statistical surveys suggest an exponential relationbetween X-ray flux and the orbital distance, and we propose to measure X-rayvariability along the orbits of various planetary systems. Our XMM observationswill determine whether or not the planets have magnetospheres, sample thestellar wind and quantitatively assess planet-star interaction models. Even moreso, these observations might evoke a new way of discovering exoplanets with XMM.
Publications	Estimation of the XUV radiation onto close planets and their evaporation \|Sanz-Forcada J. Micela G. et al. \| A&A \| 532-6 \| 2011 \| 2011A&A...532A...6S \| http://ui.adsabs.harvard.edu/#abs/2011A&A...532A...6S Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift \|Yershov V. N. \| Ap&SS \| 354-97 \| 2014 \| 2014Ap&SS.354...97Y \| http://ui.adsabs.harvard.edu/#abs/2014Ap&SS.354...97Y The Million Optical - Radio/X-ray Associations (MORX) Catalogue \|Flesch Eric W. \| PASA \| 33-52 \| 2016 \| 2016PASA...33...52F \| http://ui.adsabs.harvard.edu/#abs/2016PASA...33...52F Exploring the end states of massive stars using the X-ray emission of neutron stars and supernova remnants \|Prinz Tobias \| PhDT \| 0-305 \| 2013 \| 2013PhDT.......305P \| http://ui.adsabs.harvard.edu/#abs/2013PhDT.......305P Classification of 4XMM-DR9 sources by machine learning \|Zhang Yanxia Zhao Yongheng \| MNRAS \| 503-5263 \| 2021 \| 2021MNRAS.503.5263Z \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.503.5263Z From Active Stars to Black Holes: A Discovery Tool for Galactic X-Ray Sources \|Rodriguez Antonio C. \| PASP \| 136-054201 \| 2024 \| 2024PASP..136e4201R \| http://ui.adsabs.harvard.edu/#abs/2024PASP..136e4201R Robust constraints on feebly interacting particles using XMM-Newton \|Luque Pedro De la Torre Balaji Shyam \| PhRvD \| 109-L101305 \| 2024 \| 2024PhRvD.109j1305L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j1305L Multimessenger search for electrophilic feebly interacting particles from supernovae \|Luque Pedro De la Torre Balaji Shyam \| PhRvD \| 109-103028 \| 2024 \| 2024PhRvD.109j3028L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j3028L Importance of Cosmic-Ray Propagation on Sub-GeV Dark Matter Constraints \|De la Torre Luque Pedro Balaji Shyam \| ApJ \| 968-46 \| 2024 \| 2024ApJ...968...46D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...968...46D New 511 keV Line Data Provide Strongest sub-GeV Dark Matter Constraints \|De la Torre Luque Pedro Balaji Shyam \| ApJ \| 973-L6 \| 2024 \| 2024ApJ...973L...6D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...973L...6D
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2010-08-08T12:35:55Z/2010-08-16T22:42:53Z
Version	21.51_20241115_1113
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	2011-09-11T00:00:00Z
Last Update	2026-07-09
Keywords	"discovering exoplanets", "planetary systems", "statistical surveys", "eccentric sytems", "exponential relation", "orbital distance", "xray flux", "XMM", "elliptical orbits", "planet star interactions", "giant planets", "xray variability", "extrasolar planets orbiting", "stellar wind", "short orbital distances"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Dennis Bodewits, 2011, 'Planet-Star Interactions in Eccentric Sytems', 21.51_20241115_1113, European Space Agency, https://doi.org/10.5270/esa-2fdoa92
Rights	Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license.