| Name | 041378 |
| Title | X-Ray Observations of Jupiter in Support of the New Horizons Flyby |
| URL | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0413780101 |
| DOI | https://doi.org/10.5270/esa-hcfo9mw |
| Author | European Space Agency |
| Description | On February 28th 2007, the New Horizons (NH) spacecraft will flyby Jupiter for a gravity assist to Pluto. Closest approach (C/A) is 32 Jupiter radii, but the NH instruments will conduct intensive studies from C/A-52d to C/A+100d. Important new studies of auroral and magnetospheric physics are planned that may be well- supported by Chandra observations. Chandra support of the Cassini flyby of Jupiter in 2000 led to a major revision of our understanding of Jupiter.s x-ray aurora. We propose 108ks of Chandra time to support three planned NH investigations; a time-variability study during approach, a multi-spectral morphology study near C/A, and a magnetotail dynamics study as NH heads to Pluto. In addition, we request 72ks of XMM-Newton time to investigate spectral differences at low energy. |
| Publication | No observations found associated with the current proposal |
| Instrument | EMOS1, EMOS2, EPN, RGS1, RGS2 |
| Temporal Coverage | 2007-02-24T20:14:22Z/2007-03-09T02:20:09Z |
| 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 | 2008-03-30T00:00:00Z |
| Publisher And Registrant | European Space Agency |
| Credit Guidelines | European Space Agency, 2008, X-Ray Observations Of Jupiter In Support Of The New Horizons Flyby, 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-hcfo9mw |