A dataset provided by the European Space Agency

Name: The X-ray irradiation of the nearest transiting super-Earth
Published: 2017-07-05T22:00:00Z
License: https://creativecommons.org/licenses/by-nc/3.0/igo

Proposal ID	078492
Title	The X-ray irradiation of the nearest transiting super-Earth
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0784920201
DOI	https://doi.org/10.5270/esa-4h6k3g6
Principal Investigator, PI	Dr Peter Wheatley
Abstract	The recent discovery of a super-Earth transiting the bright star HD219134provides an unprecedented opportunity for detailed study of the atmosphere of alow-mass exoplanet. The K3V star is located at a distance of only 6.5pc,enabling sensitive measurements of its X-ray flux and spectrum. This isimportant because X-ray/EUV irradiation is believed to drive the observedevaporation of hot Jupiters (HD209458b, HD189733b) and Neptunes (GJ436b), andHD219134b will extended these studies to the super-Earth regime. Here we proposean XMM-Newton observation that will define the high-energy environment of theplanet and allow estimates of its atmospheric escape rate. This will aid theinterpretation of atmosphere observations with HST, Spitzer, JWST etc.
Publications	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 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 Search for Young Stellar Objects within 4XMM-DR13 Using CatBoost and SPE \|Ma Xiangyao Zhang Yanxia et al. \| AJ \| 168-210 \| 2024 \| 2024AJ....168..210M \| http://ui.adsabs.harvard.edu/#abs/2024AJ....168..210M 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	2016-06-13T21:38:27Z/2016-06-14T08:11:47Z
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	2017-07-05T22:00:00Z
Last Update	2026-07-09
Keywords	"transiting super earth", "HD219134", "XMM-Newton", "XMM", "k3v star", "super earth regime", "super earth transiting", "sensitive measurements", "xray irradiation", "bright star hd219134", "hot jupiters hd209458b", "low mass exoplanet", "HST", "euv irradiation", "atmospheric escape rate", "neptunes gj436b", "xray flux", "jwst etc", "xmm newton"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Peter Wheatley, 2017, 'The X-ray irradiation of the nearest transiting super-Earth', 21.51_20241115_1113, European Space Agency, https://doi.org/10.5270/esa-4h6k3g6
Rights	Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license.