A dataset provided by the European Space Agency

Name OT1_sdodsonr_1
Title Conditions for Giant Planet Formation: a Herschel Study of Raw Materials in Selected Debris Disks
URL

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DOI 10.5270/esa-qndxa02
Author dodson-robinson, s.
Description Due to the observational difficulties of spatially resolving protostellar disk midplanes near the ice line, where most giant planet formation is thought to take place, most constraints on the possible locations and methods of giant planet formation have come from theory. We propose to use Herschel PACS and SPIRE photometry, and PACS spectroscopy, to observe five debris disks around Solar-type stars, in order to (1) observe young systems where giant planets cannot form, and (2) identify the available raw materials for typical planet formation. We will constrain the range of dust temperatures, and search for crystalline forsterite grains, as well as indirect diagnostics of ice and refractory carbon through deep line scans for [C II] (158 microns) and [O I] 63.2 microns.
Publication Herschel Observations and Updated Spectral Energy Distributions of Five Sunlike Stars with Debris Disks . Dodson-Robinson Sarah E. et al. . The Astrophysical Journal, Volume 833, Issue 2, article id. 183, 11 pp. (2016). . 833 . 10.3847\/1538-4357\/833\/2\/183 . 2016ApJ...833..183D ,
Instrument PACS_PacsPhoto_largeScan, PACS_PacsRangeSpec_point, PACS_PacsLineSpec_point
Temporal Coverage 2011-04-19T22:44:59Z/2013-04-03T10:05:18Z
Version SPG v14.2.0
Mission Description Herschel was launched on 14 May 2009! It is the fourth 'cornerstone' mission in the ESA science programme. With a 3.5 m Cassegrain telescope it is the largest space telescope ever launched. It is performing photometry and spectroscopy in approximately the 55-671 ┬Ám range, bridging the gap between earlier infrared space missions and groundbased facilities.
Creator Contact https://support.cosmos.esa.int/herschel/
Date Published 2013-10-03T09:10:02Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2013-10-03T09:10:02Z, OT1_sdodsonr_1, SPG v14.2.0. https://doi.org/10.5270/esa-qndxa02