A dataset provided by the European Space Agency

Name: X-Ray Observations of Planetary Transits: Secondary Eclipse
Published: 2010-06-04T00:00:00Z

Proposal ID	060097
Title	X-Ray Observations of Planetary Transits: Secondary Eclipse
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0600970201
DOI	https://doi.org/10.5270/esa-2mqkng5
Principal Investigator, PI	Dr Scott Wolk
Abstract	The effect of stellar X-rays on their nearby gas-giant planets appears to besignificant. The X-rays have been cited at the cause of excess heating of theplanet which can induce mass loss. Further, it has been argued that the magneticfields of the two bodies can interact. Recent statistical analysis of starspossessing hot-Jupiters indicates that their activity could be enhanced by asmuch as a factor of 2 and observations in Ca II HK and X-ray phased to theplanetary orbital periods show that there could be in situ X-ray enhancements ofas much as 50%. This makes it possible to detect when the interacting zone movesbehind the star. We propose to observe the secondary eclipse of two nearby (<20pc.) systems HD 189733 and GJ 436.
Publications	XMM-Newton Observations of HD 189733 During Planetary Transits \|Pillitteri, I., Wolk, S. J., et al. \| ApJ \| 722-1216 \| 2010 \| 2010ApJ...722.1216P \| http://ui.adsabs.harvard.edu/#abs/2010ApJ...722.1216P Coronal properties of planet-bearing stars (Corrigendum) \|Poppenhaeger, K., Robrade, J., \| A&A \| 529-1 \| 2011 \| 2011A&A...529C...1P \| http://ui.adsabs.harvard.edu/#abs/2011A&A...529C...1P An XMM-Newton Survey of the Soft X-Ray Background. II. An All-Sky Catalog of Diffuse O VII and O VIII Emission Intensities \|Henley, David B., Shelton, Robin L., \| ApJS \| 202-14 \| 2012 \| 2012ApJS..202...14H \| http://ui.adsabs.harvard.edu/#abs/2012ApJS..202...14H 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 The Interaction of the Fermi Bubbles with the Milky Way.s Hot Gas Halo \|Miller, Matthew J., Bregman, Joel N., \| ApJ \| 829-9 \| 2016 \| 2016ApJ...829....9M \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...829....9M 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 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 Ly\\u03b1 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 An X-Ray- and SZ-bright Diffuse Source toward M31: A Local Hot Bridge \|Qu, Zhijie, Huang, Rui, et al. \| ApJ \| 907-14 \| 2021 \| 2021ApJ...907...14Q \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...907...14Q Modelling the He I triplet absorption at 10 830 \\u00c5 in the atmospheres of HD 189733 b and GJ 3470 b \|Lamp\\u00f3n, M., L\\u00f3pez-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 Five New Hot Jupiter Transits Investigated with Swift-UVOT \|Corrales, Lia, Ravi, Sasikrishna, et al. \| AJ \| 162-287 \| 2021 \| 2021AJ....162..287C \| http://ui.adsabs.harvard.edu/#abs/2021AJ....162..287C 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 The Solar Cycle Temporal Variation of the Solar Wind Charge Exchange X-Ray Lines \|Qu, Zhijie, Koutroumpa, Dimitra, et al. \| ApJ \| 930-21 \| 2022 \| 2022ApJ...930...21Q \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...930...21Q 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
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2009-05-18T21:15:54Z/2009-05-19T07:37:49Z
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	2010-06-04T00:00:00Z
Keywords	"HD 189733", "magnetic fields", "planetary transits", "statistical analysis", "secondary eclipse", "xray phased", "gj 436", "excess heating", "situ xray enhancements", "induce mass loss", "systems hd 189733", "ca ii hk", "interacting zone moves", "x ray", "planetary orbital periods", "stellar xray"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Scott Wolk, 2010, 'X-Ray Observations of Planetary Transits: Secondary Eclipse', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-2mqkng5