A dataset provided by the European Space Agency

Proposal ID 060273
Title X-Rays, Dust, Ice, and Gas in Time (X-DIGIT)
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DOI https://doi.org/10.5270/esa-t2edvq3
Principal Investigator, PI Dr Manuel Guedel
Abstract We propose an extensive investigation of the impact of stellar X-rays on theplanet-forming molecular environments of T Tauri stars by combining X-ray datafrom XMM-Newton with novel far-infrared spectroscopy from our Herschel OpenTime Key Project and complementary mid-infrared spectroscopy from Spitzer. Theprincipal goals are, i) to identify X-ray tracers in the Herschel spectralrange, ii) to study the potential impact of X-rays on circumstellar disks, andiii) to model physical and chemical conditions in the regions where the X-rayimpact is significant. We wish to understand how X-ray radiation influencesstar- and planet formation through physical and chemical processing of disks.Understanding the distribution of the astrobiologically important water plays a key role.
Publications
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2009-08-24T20:33:10Z/2010-02-20T13:33:57Z
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 2011-03-23T00:00:00Z
Last Update 2026-07-09
Keywords "x rays", "XMM-Newton", "XMM", "stellar xray", "potential impact", "time key project", "tauri stars", "xray data", "xray impact", "infrared spectroscopy", "key role", "xray tracers", "chemical conditions", "water plays", "time x digit", "herschel spectral range", "model physical", "planet formation", "extensive investigation", "chemical processing", "circumstellar dis", "xmm newton"
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Dr Manuel Guedel, 2011, 'X-Rays, Dust, Ice, and Gas in Time (X-DIGIT)', 21.51_20241115_1113, European Space Agency, https://doi.org/10.5270/esa-t2edvq3
Rights Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license.