A dataset provided by the European Space Agency

Proposal ID 088211
Title Juno and XMM-Newtons final search for drivers of Jupiters X-ray aurorae
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DOI https://doi.org/10.57780/esa-kjpxumf
Principal Investigator, PI Ms Affelia Wibisono
Abstract Simultaneous observations with XMM-Newton and Juno over the last 3 years haverevolutionised our understanding of the coupling between Jupiters magnetosphereand ionosphere leading to new theories of how planets can produce X-rays. Forexample, evidence is building from joint XMM-Newton and Juno observations thation cyclotron waves are one of the drivers for the gas giants X-ray aurorae.However, we only have one more opportunity to utilise the unique capabilities ofXMM-Newton and Juno before the jovian explorer is due to finish its mission inJuly 2021. Juno is now in the dusk sector of Jupiters magnetosphere - a regionthat no other spacecraft will visit again for at least another decade.
Publications
Instrument EMOS1, EMOS2, EPN, RGS1, RGS2
Temporal Coverage 2021-05-10T20:10:46Z/2021-06-09T08:27:09Z
Version PPS_NOT_AVAILABLE
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 2022-06-19T00:00:00Z
Last Update 2025-08-04
Keywords "XMM", "ionosphere leading", "XMM-Newton", "final search", "gas giant", "dusk sector", "xmm newton", "jovian explorer", "ion cyclotron waves", "xray aurorae"
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Ms Affelia Wibisono, 2022, 'Juno and XMM-Newton's final search for drivers of Jupiter's X-ray aurorae', PPS_NOT_AVAILABLE, European Space Agency, https://doi.org/10.57780/esa-kjpxumf