Planet Formation Imager (PFI): Introduction and Technical Considerations
arXiv:1407.7032 · doi:10.1117/12.2057262
Abstract
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, newly-formed 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.
SPIE Astronomical Telescopes and Instrumentation conference, June 2014, Paper ID 9146-35, 10 pages, 2 Figures
References in corpus (7)
- LkCa 15: A Young Exoplanet Caught at Formation?
- Transitional and Pre-Transitional disks: Gap Opening by Multiple Planets?
- Large-Scale Asymmetries in the Transitional Disks of SAO 206462 and SR 21
- Small vs large dust grains in transitional disks: do different cavity sizes indicate a planet?
- DARWIN mission proposal to ESA
- Tests with a Carlina-type diluted telescope; Primary coherencing
- Mid-infrared interferometry with K band fringe-tracking I. The VLTI MIDI+FSU experiment
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- AGILIS: Agile Guided Interferometer for Longbaseline Imaging Synthesis - Demonstration and concepts of reconfigurable optical imaging interferometers
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- Setting the Stage for the Planet Formation Imager
- Planet Formation Imager: Project Update