A dataset provided by the European Space Agency

Name 020008
Title XMM-NEWTON OBSERVATIONS OF JUPITER AND ITS NEIGHBOURHOOD
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0200080101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0200080201
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https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0200080233
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0200080234
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0200080301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0200080401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0200080501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0200080601
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0200080701
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https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0200080731
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0200080732
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0200080733
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0200080734
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0200080801
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https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0200081001

DOI https://doi.org/10.5270/esa-f2ax0iw
Author European Space Agency
Description Jupiter and its neighbourhood are an exceptionally interesting source of X-rays
within the solar system. We propose to observe the planet and its Galilean moons
over two XMM-Newton orbits. A good signal-to-noise RGS spectrum of Jupiter.s
auroral .hot spots. will resolve the question of their origin: energetic ion
precipitation from entirely inside the magnetosphere, or acceleration of
captured solar wind ions in the outer magnetosphere. With EPIC we will study
oscillations observed by Chandra in the hot spot emissions, and the asymmetries
in Jupiter.s low-latitude X-ray emission first observed with ROSAT; we will
study how Io.s and its Plasma Torus X-ray emissions vary with Io.s orbital phase
about Jupiter, and we will obtain the first secure X-ray detections of all four Galilean satellites.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, RGS1, RGS2
Temporal Coverage 2003-11-25T21:07:53Z/2003-11-29T12:17:22Z
Version PPS_NOT_AVAILABLE
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 2008-05-02T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2008, Xmm-Newton Observations Of Jupiter And Its Neighbourhood, PPS_NOT_AVAILABLE, European Space Agency, https://doi.org/10.5270/esa-f2ax0iw