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  Planet formation imager: project update

Monnier, J. D., Ireland, M., Kraus, S., Alonso-Herrero, A., Bonsor, A., Baron, F., Bayo, A., Berger, J.-P., Boyajian, T., Chiavassa, A., Ciardi, D., Creech-Eakman, M., de Wit, W.-J., Defrère, D., Dong, R., Duchêne, G., Espaillat, C., Gallenne, A., Gandhi, P., Gonzalez, J.-F., Haniff, C., Hoenig, S., Ilee, J., Isella, A., Jensen, E., Juhasz, A., Kane, S., Kishimoto, M., Kley, W., Kral, Q., Kratter, K., Labadie, L., Lacour, S., Laughlin, G., Le Bouquin, J.-B., Michael, E., Meru, F., Millan-Gabet, R., Millour, F., Minardi, S., Morbidelli, A., Mordasini, C., Morlok, A., Mozurkewich, D., Nelson, R., Olofsson, J., Oudmaijer, R., Packham, C., Paladini, C., Panic, O., Petrov, R., Pope, B., Pott, J.-U., Quiroga-Nunez, L. H., Ramos Almeida, C., Raymond, S. N., Regaly, Z., Reynolds, M., Ridgway, S., Rinehart, S., Schreiber, M., Smith, M., Stassun, K., Surdej, J., ten Brummelaar, T., Tristram, K., Turner, N., Tuthill, P., van Belle, G., Vasisht, G., Wallace, A., Weigelt, G., Wishnow, E., Wittkowski, M., Wolf, S., Young, J., Zhao, M., Zhu, Z., & Zúñiga-Fernández, S. (2018). Planet formation imager: project update.

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基本情報

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アイテムのパーマリンク: https://hdl.handle.net/21.11116/0000-0005-CC18-B 版のパーマリンク: https://hdl.handle.net/21.11116/0000-0005-CC19-A
資料種別: 会議論文集

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関連URL

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URL:
https://ui.adsabs.harvard.edu/abs/2018SPIE10701E..18M (全文テキスト(全般))
説明:
-
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作成者

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 作成者:
Monnier, John D.1, 著者
Ireland, Michael1, 著者
Kraus, Stefan1, 著者
Alonso-Herrero, Almudena1, 著者
Bonsor, Amy1, 著者
Baron, Fabien1, 著者
Bayo, Amelia1, 著者
Berger, Jean-Philippe1, 著者
Boyajian, Tabetha1, 著者
Chiavassa, Andrea1, 著者
Ciardi, David1, 著者
Creech-Eakman, Michelle1, 著者
de Wit, Willem-Jan1, 著者
Defrère, Denis1, 著者
Dong, Ruobing1, 著者
Duchêne, Gaspard1, 著者
Espaillat, Catherine1, 著者
Gallenne, Alexandre1, 著者
Gandhi, Poshak1, 著者
Gonzalez, Jean-Francois1, 著者
Haniff, Chris1, 著者Hoenig, Sebastian1, 著者Ilee, John1, 著者Isella, Andrea1, 著者Jensen, Eric1, 著者Juhasz, Attila1, 著者Kane, Stephen1, 著者Kishimoto, Makoto1, 著者Kley, Wilhelm1, 著者Kral, Quentin1, 著者Kratter, Kaitlin1, 著者Labadie, Lucas1, 著者Lacour, Sylvestre1, 著者Laughlin, Greg1, 著者Le Bouquin, Jean-Baptiste1, 著者Michael, Ernest1, 著者Meru, Farzana1, 著者Millan-Gabet, Rafael1, 著者Millour, Florentin1, 著者Minardi, Stefano1, 著者Morbidelli, Alessandro1, 著者Mordasini, Chris1, 著者Morlok, Andreas1, 著者Mozurkewich, Dave1, 著者Nelson, Richard1, 著者Olofsson, Johan1, 著者Oudmaijer, Rene1, 著者Packham, Chris1, 著者Paladini, Claudia1, 著者Panic, Olja1, 著者Petrov, Romain1, 著者Pope, Benjamin1, 著者Pott, Joerg-Uwe1, 著者Quiroga-Nunez, Luis Henry1, 著者Ramos Almeida, Cristina1, 著者Raymond, Sean N.1, 著者Regaly, Zsolt1, 著者Reynolds, Mark1, 著者Ridgway, Stephen1, 著者Rinehart, Stephen1, 著者Schreiber, Matthias1, 著者Smith, Michael1, 著者Stassun, Keivan1, 著者Surdej, Jean1, 著者ten Brummelaar, Theo1, 著者Tristram, Konrad1, 著者Turner, Neal1, 著者Tuthill, Peter1, 著者van Belle, Gerard1, 著者Vasisht, Gautum1, 著者Wallace, Alexander1, 著者Weigelt, Gerd1, 著者Wishnow, Edward1, 著者Wittkowski, Markus1, 著者Wolf, Sebastian1, 著者Young, John1, 著者Zhao, Ming1, 著者Zhu, Zhaohuan1, 著者Zúñiga-Fernández, Sebastian1, 著者 全て表示
所属:
1Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners, ou_2421692              

内容説明

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キーワード: Astrophysics - Instrumentation and Methods for Astrophysics Astrophysics - Earth and Planetary Astrophysics
 要旨: The Planet Formation Imager (PFI) is a near- and mid-infrared interferometer project with the driving science goal of imaging directly the key stages of planet formation, including the young proto-planets themselves. Here, we will present an update on the work of the Science Working Group (SWG), including new simulations of dust structures during the assembly phase of planet formation and quantitative detection efficiencies for accreting and non-accreting young exoplanets as a function of mass and age. We use these results to motivate two reference PFI designs consisting of a) twelve 3m telescopes with a maximum baseline of 1.2km focused on young exoplanet imaging and b) twelve 8m telescopes optimized for a wider range of young exoplanets and protoplanetary disk imaging out to the 150K H2O ice line. Armed with 4 x 8m telescopes, the ESO/VLTI can already detect young exoplanets in principle and projects such as MATISSE, Hi-5 and Heimdallr are important PFI pathfinders to make this possible. We also discuss the state of technology development needed to make PFI more affordable, including progress towards new designs for inexpensive, small field-of- view, large aperture telescopes and prospects for Cubesat-based space interferometry.

資料詳細

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 日付: 2018
 出版の状態: 出版
 ページ: -
 出版情報: -
 目次: -
 査読: -
 識別子(DOI, ISBNなど): ISBN: 9781510619555
 学位: -

関連イベント

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イベント名: Optical and Infrared Interferometry and Imaging VI
開催地: -
開始日・終了日: 2018

訴訟

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