A dataset provided by the European Space Agency

Name: Systematic effects of star-planet interaction
Published: 2012-05-18T00:00:00Z
License: https://creativecommons.org/licenses/by-nc/3.0/igo

Proposal ID	067239
Title	Systematic effects of star-planet interaction
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0672390201
DOI	https://doi.org/10.5270/esa-q6jwxqb
Principal Investigator, PI	Dr Ignazio Pillitteri
Abstract	In 2009 we used XMM-Newton to observe the hot Jupiter HD189733b during asecondary eclipse. Basing on that observation we have published two interestingresults: 1) a distinct softening of the spectrum at mid eclipse and 2) a posteclipse flare coincident with model predictions of the appearance of a magneticfootpoint on the rising limb. That single observation cannot firm evidence of acausal relation with phase and Star-Planet Interaction. We propose to re-observethis system during secondary eclipses four times in order to establish thesystematic nature of these features. We propose to observe also the higheccentricity system GJ 436 at periastron as pathfinder for SPI in hot neptuneplanets.
Publications	X-Ray Activity Phased with Planet Motion in HD 189733? \|Pillitteri I. Gunther H. M. et al. \| ApJ \| 741-18 \| 2011 \| 2011ApJ...741L..18P \| http://ui.adsabs.harvard.edu/#abs/2011ApJ...741L..18P The Corona of HD 189733 and its X-Ray Activity \|Pillitteri I. Wolk S. J. et al. \| ApJ \| 785-145 \| 2014 \| 2014ApJ...785..145P \| http://ui.adsabs.harvard.edu/#abs/2014ApJ...785..145P 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 Comparison of Damped Oscillations in Solar and Stellar X-Ray flares \|Cho I.-H. Cho K.-S. et al. \| ApJ \| 830-110 \| 2016 \| 2016ApJ...830..110C \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...830..110C Ground-based detection of an extended helium atmosphere in the Saturn-mass exoplanet WASP-69b \|Nortmann Lisa Palle Enric et al. \| Sci \| 362-1388 \| 2018 \| 2018Sci...362.1388N \| http://ui.adsabs.harvard.edu/#abs/2018Sci...362.1388N ROME (Radio Observations of Magnetized Exoplanets). II. HD 189733 Does Not Accrete Significant Material from Its Exoplanet Like a T Tauri Star from a Disk \|Route Matthew Looney Leslie W. \| ApJ \| 887-229 \| 2019 \| 2019ApJ...887..229R \| http://ui.adsabs.harvard.edu/#abs/2019ApJ...887..229R Modeling the Lyu03b1 transit absorption of the hot Jupiter HD 189733b \|Odert P. Erkaev N. V. et al. \| A&A \| 638-49 \| 2020 \| 2020A&A...638A..49O \| http://ui.adsabs.harvard.edu/#abs/2020A&A...638A..49O MOVES - IV. Modelling the influence of stellar XUV-flux cosmic rays and stellar energetic particles on the atmospheric composition of the hot Jupiter HD 189733b \|Barth P. Helling Ch et al. \| MNRAS \| 502-6201 \| 2021 \| 2021MNRAS.502.6201B \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.502.6201B Modelling the He I triplet absorption at 10 830 u00c5 in the atmospheres of HD 189733 b and GJ 3470 b \|Lampu00f3n M. Lu00f3pez-Puertas M. et al. \| A&A \| 647-129 \| 2021 \| 2021A&A...647A.129L \| http://ui.adsabs.harvard.edu/#abs/2021A&A...647A.129L 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 X-ray variability of HD 189733 across eight years of XMM-Newton observations \|Pillitteri I. Micela G. et al. \| A&A \| 660-75 \| 2022 \| 2022A&A...660A..75P \| http://ui.adsabs.harvard.edu/#abs/2022A&A...660A..75P The harsh environment where exoplanets live \|Pillitteri Ignazio \| AN \| 343-10099 \| 2022 \| 2022AN....34310099P \| http://ui.adsabs.harvard.edu/#abs/2022AN....34310099P More Evidence for Variable Helium Absorption from HD 189733b \|Zhang Michael Cauley P. Wilson et al. \| AJ \| 164-237 \| 2022 \| 2022AJ....164..237Z \| http://ui.adsabs.harvard.edu/#abs/2022AJ....164..237Z Planetary Parameters XUV Environments and Mass-loss Rates for Nearby Gaseous Planets with X-Ray-detected Host Stars \|Spinelli Riccardo Gallo Elena et al. \| AJ \| 165-200 \| 2023 \| 2023AJ....165..200S \| http://ui.adsabs.harvard.edu/#abs/2023AJ....165..200S 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 Exoplanet Aeronomy: A Case Study of WASP-69 bs Variable Thermosphere \|Levine W. Garrett Vissapragada Shreyas et al. \| AJ \| 168-65 \| 2024 \| 2024AJ....168...65L \| http://ui.adsabs.harvard.edu/#abs/2024AJ....168...65L 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	2011-04-30T23:14:20Z/2011-05-01T10:06:12Z
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	2012-05-18T00:00:00Z
Last Update	2026-07-09
Keywords	"star planet interaction", "rising limb", "model predictions", "XMM-Newton", "mid eclipse", "systematic effects", "'' hot jupiter", "magnetic footpoint", "firm evidence", "XMM", "HD189733", "secondary eclipses", "distinct softening", "hot neptune planets", "causal relation", "secondary eclipse", "xmm newton"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Ignazio Pillitteri, 2012, 'Systematic effects of star-planet interaction', 21.51_20241115_1113, European Space Agency, https://doi.org/10.5270/esa-q6jwxqb
Rights	Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license.