مؤتمر
Planet Formation Imager (PFI): Introduction and technical considerations
| العنوان: | Planet Formation Imager (PFI): Introduction and technical considerations |
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| المؤلفون: | Monnier, J. D., Kraus, S., Buscher, D., Berger, J.-P., Haniff, C., Ireland, M., Labadie, L., Lacour, S., Le Coroller, H., Petrov, R. G., Pott, J.-U., Ridgway, S., Surdej, Jean, Ten Brummelaar, T., Tuthill, P., Van Belle, G., Rajagopal, J. K., Creech, Eakman, M. J., Malbet, F. |
| المصدر: | Proceedings of SPIE: The International Society for Optical Engineering, 9146 (2014); Optical and Infrared Interferometry IV, 23 June 2014 through 27 June 2014 |
| بيانات النشر: | SPIE, 2014. |
| سنة النشر: | 2014 |
| مصطلحات موضوعية: | Planet Formation, Architecture, Image reconstruction, Infrared radiation, High angular resolutions, High-resolution imaging, Long-baseline interferometry, Science requirements, Technical advances, Theoretical framework, Wavelength coverage, Interferometry, Physical, chemical, mathematical & earth Sciences, Space science, astronomy & astrophysics, Physique, chimie, mathématiques & sciences de la terre, Aérospatiale, astronomie & astrophysique |
| الوصف: | Complex non-linear and dynamic processes lie at the heart of the planet formation process. Through numerical simulation and basic observational constraints, the basics of planet formation are now coming into focus. High resolution imaging at a range of wavelengths will give us a glimpse into the past of our own solar system and enable a robust theoretical framework for predicting planetary system architectures around a range of stars surrounded by disks with a diversity of initial conditions. Only long-baseline interferometry can provide the needed angular resolution and wavelength coverage to reach these goals and from here we launch our planning efforts. The aim of the "Planet Formation Imager" (PFI) project is to develop the roadmap for the construction of a new near-/mid-infrared interferometric facility that will be optimized to unmask all the major stages of planet formation, from initial dust coagulation, gap formation, evolution of transition disks, mass accretion onto planetary embryos, and eventual disk dispersal. PFI will be able to detect the emission of the cooling, newlyformed planets themselves over the first 100 Myrs, opening up both spectral investigations and also providing a vibrant look into the early dynamical histories of planetary architectures. Here we introduce the Planet Formation Imager (PFI) Project (www.planetformationimager.org) and give initial thoughts on possible facility architectures and technical advances that will be needed to meet the challenging top-level science requirements. © 2014 SPIE. |
| نوع الوثيقة: | conference paper http://purl.org/coar/resource_type/c_5794 conferenceObject peer reviewed |
| اللغة: | English |
| Relation: | urn:issn:0277-786X; urn:issn:1996-756X |
| DOI: | 10.1117/12.2057262 |
| URL الوصول: | https://orbi.uliege.be/handle/2268/182427 |
| حقوق: | open access http://purl.org/coar/access_right/c_abf2 info:eu-repo/semantics/openAccess |
| رقم الأكسشن: | edsorb.182427 |
| قاعدة البيانات: | ORBi |
| DOI: | 10.1117/12.2057262 |
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