A dataset provided by the European Space Agency

Name: Assessing the high-energy environment of the habitable zone planet LHS 1140b
Published: 2020-01-14T23:00:00Z

Proposal ID	082260
Title	Assessing the high-energy environment of the habitable zone planet LHS 1140b
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0822600101
DOI	https://doi.org/10.5270/esa-8q1yeks
Principal Investigator, PI	Dr Jason Dittmann
Abstract	Exoplanets around nearby small stars present the best opportunity for futureatmospheric studies with the James Webb Space Telescope and the ground basedELTs under construction. The MEarth Project has discovered a rocky planet with aperiod of 24.73 days residing in the habitable zone of the nearby, spun- downstar LHS 1140. We seek to detect the high energy emission from LHS 1140 in orderto constrain atmospheric escape and aid future studies of LHS 1140b.satmosphere, which are already planned in the JWST GTO program. In addition, LHS1140 is representative of the low mass, slowly rotating population of M dwarfsin the Milky Way. A deep X-ray exposure on this extremum of the stellarpopulation will shed insight into the magnetic dynamo and high energy processes ongoing in these stars.
Publications	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
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2018-12-21T12:20:03Z/2018-12-22T06:06:43Z
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	2020-01-14T23:00:00Z
Keywords	"magnetic dynamo", "energy emission", "shed insight", "jwst gto program", "star lhs 1140", "mearth project", "low mass", "lhs 1140b", "stellar population", "future atmospheric", "deep xray exposure", "energy processes", "rocky planet", "lhs 1140", "constrain atmospheric escape", "slowly rotating population", "aid future", "habitable zone"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Jason Dittmann, 2020, 'Assessing the high-energy environment of the habitable zone planet LHS 1140b', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-8q1yeks