A dataset provided by the European Space Agency

Name 078424
Title The future X-ray Sun
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0784240101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0784240201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0784240301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0784240501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0784240701
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0784240901
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0784241101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0784241201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0784241301

DOI https://doi.org/10.5270/esa-193j1m4
Author European Space Agency
Description Magnetic activity is ubiquitous among solar-like stars and coronal X-ray
emission is perhaps the most powerful diagnostic. Stellar X-ray emission decays
during the first Gyr by several orders of magnitude. However, it is currently
unknown if and how this decay continues for older stars, because observational
constraints are sparse due to the X-ray faintness of these systems. We propose
to remedy this situation by obtaining X-ray data of old solar analogs, i.e.,
stars that have essentially the same stellar properties as the Sun so that we
sample only age effects on stellar activity. Our sample of 13 old solar analogs
will clarify the X-ray future of the Sun.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2016-05-10T22:17:48Z/2017-01-05T16:37:42Z
Version 17.56_20190403_1200
Mission Description The European Space Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's 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 Earth's 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 2018-01-24T23:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2018, The Future X-Ray Sun, 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-193j1m4