A dataset provided by the European Space Agency

Proposal ID 041498
Title An intensive study of the planetary debris disk around SDSS J1228+1040
Download Data Associated to the proposal

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0414980101

DOI https://doi.org/10.5270/esa-0rf668v
Principal Investigator, PI Dr Boris Gaensicke
Abstract While >200 extra-solar planets orbiting main-sequence stars have beendiscovered, the destiny of planetary systems through the late stages of theevolution of their host stars is very uncertain, and no planet has been foundaround a white dwarf. We have identified a metal-rich gas disk around therelatively young white dwarf SDSS 1228+1040. A dynamical model of thedouble-peaked emission lines constrains the outer disk radius to just 1.2Rs. Thelikely origin of the disk is a tidally disrupted asteroid, which has beendestabilised from its initial orbit at a distance of more than 1000 solar radiiby the interaction with a rather massive planetesimal or planet. We propose aVLT and XMM study of the nature of the planetary debris disk around SDSS 1228+1040 and its interaction with the WD
Publications
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2007-06-10T21:54:07Z/2007-06-11T04:32:46Z
Version 17.56_20190403_1200
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 2008-06-25T00:00:00Z
Keywords "initial orbit", "SDSS", "XMM", "massive planetesimal", "planetary systems", "dynamical model", "sdss 1228", "white dwarf", "late stages", "outer disk radius", "tidally disrupted asteroid", "sdss j1228", "solar radii", "planetary debris disk"
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Dr Boris Gaensicke, 2008, 'An intensive study of the planetary debris disk around SDSS J1228+1040', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-0rf668v