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Possible signs of water and differentiation in a rocky exoplanetary body

Farihi, J; Brinkworth, CS; Gänsicke, BT; Marsh, TR; Girven, J; Hoard, DW; Klein, B; (2011) Possible signs of water and differentiation in a rocky exoplanetary body. Astrophysical Journal Letters , 728 (1) , Article L8. 10.1088/2041-8205/728/1/L8. Green open access

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Abstract

Spitzer observations reveal the presence of warm debris from a tidally destroyed rocky and possibly icy planetary body orbiting the white dwarf GD 61. Ultraviolet and optical spectroscopy of the metal-contaminated stellar photosphere reveal traces of hydrogen, oxygen, magnesium, silicon, iron, and calcium. The nominal ratios of these elements indicate an excess of oxygen relative to that expected from rock-forming metal oxides, and thus it is possible that water was accreted together with the terrestrial-like debris. Iron is found to be deficient relative to magnesium and silicon, suggesting the material may have originated as the outer layers of a differentiated parent body, as is widely accepted for the Moon.

Type: Article
Title: Possible signs of water and differentiation in a rocky exoplanetary body
Open access status: An open access version is available from UCL Discovery
DOI: 10.1088/2041-8205/728/1/L8
Publisher version: http://dx.doi.org/10.1088/2041-8205/728/1/L8
Language: English
Additional information: Copyright © 2011. The American Astronomical Society. All rights reserved.
Keywords: circumstellar matter; minor planets, asteroids: general; planetary systems; stars: abundances; white dwarfs
UCL classification: UCL
UCL > Provost and Vice Provost Offices > UCL BEAMS
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Physics and Astronomy
URI: https://discovery-pp.ucl.ac.uk/id/eprint/1477427
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