Show simple item record

dc.contributor.authorIreland, MJ
dc.contributor.authorMonnier, JD
dc.contributor.authorKraus, S
dc.contributor.authorIsella, A
dc.contributor.authorMinardi, S
dc.contributor.authorPetrov, R
dc.contributor.authorten Brummelaar, T
dc.contributor.authorYoung, J
dc.contributor.authorVasisht, G
dc.contributor.authorMozurkewich, D
dc.contributor.authorRinehart, S
dc.contributor.authorMichael, EA
dc.contributor.authorvan Belle, G
dc.contributor.authorWoillez, J
dc.date.accessioned2018-01-15T14:34:20Z
dc.date.issued2016-08-04
dc.description.abstractThe Planet Formation Imager (PFI) project aims to image the period of planet assembly directly, resolving structures as small as a giant planet’s Hill sphere. These images will be required in order to determine the key mechanisms for planet formation at the time when processes of grain growth, protoplanet assembly, magnetic fields, disk/planet dynamical interactions and complex radiative transfer all interact – making some planetary systems habitable and others inhospitable. We will present the overall vision for the PFI concept, focusing on the key technologies and requirements that are needed to achieve the science goals. Based on these key requirements, we will define a cost envelope range for the design and highlight where the largest uncertainties lie at this conceptual stage.en_GB
dc.identifier.citationVol. 9907, article 99071Len_GB
dc.identifier.doi10.1117/12.2233926
dc.identifier.urihttp://hdl.handle.net/10871/31019
dc.language.isoenen_GB
dc.publisherSociety of Photo-optical Instrumentation Engineers (SPIE)en_GB
dc.rights© (2016) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.en_GB
dc.subjectinterferometryen_GB
dc.subjectmid-infrareden_GB
dc.subjectexoplanetsen_GB
dc.subjectplanet formationen_GB
dc.subjectastronomyen_GB
dc.subjectfacilitiesen_GB
dc.subjectimagingen_GB
dc.subjectinfrareden_GB
dc.titleStatus of the Planet Formation Imager (PFI) concepten_GB
dc.typeArticleen_GB
dc.date.available2018-01-15T14:34:20Z
dc.descriptionThis is the author accepted manuscript. The final version is available from SPIE via the DOI in this record.en_GB
dc.identifier.journalProceedings of SPIEen_GB


Files in this item

This item appears in the following Collection(s)

Show simple item record