Planet Formation Imager (PFI): Science vision and key requirements

Stefan Kraus; John D. Monnier; Michael J. Ireland; Gaspard Duchêne; Catherine Espaillat; Sebastian Hönig; Attila Juhasz; Chris Mordasini; Johan Olofsson; Claudia Paladini; Keivan Stassun; Neal Turner; Gautam Vasisht; Tim J. Harries; Matthew R. Bate; Jean François Gonzalez; Alexis Matter; Zhaohuan Zhu; Olja Panic; Zsolt Regaly; Alessandro Morbidelli; Farzana Meru; Sebastian Wolf; John Ilee; Jean Philippe Berger; Ming Zhao; Quentin Kral; Andreas Morlok; Amy Bonsor; David Ciardi; Stephen R. Kane; Kaitlin Kratter; Greg Laughlin; Joshua Pepper; Sean Raymond; Lucas Labadie; Richard P. Nelson; Gerd Weigelt; Theo Ten Brummelaar; Arnaud Pierens; Rene Oudmaijer; Wilhelm Kley; Benjamin Pope; Eric L.N. Jensen; Amelia Bayo; Michael Smith; Tabetha Boyajian; Luis Henry Quiroga-Nuñez; Rafael Millan-Gabet; Andrea Chiavassa; Alexandre Gallenne; Mark Reynolds; Willem Jan De Wit; Markus Wittkowski; Florentin Millour; Poshak Gandhi; Cristina Ramos Almeida; Almudena Alonso Herrero; Chris Packham; Makoto Kishimoto; Konrad R.W. Tristram; Jörg Uwe Pott; Jean Surdej; David Buscher; Chris Haniff; Sylvestre Lacour; Romain Petrov; Steve Ridgway; Peter Tuthill; Gerard Van Belle; Phil Armitage; Clement Baruteau; Myriam Benisty; Bertram Bitsch; Sijme Jan Paardekooper; Christophe Pinte; Frederic Masset; Giovanni Rosotti

doi:10.1117/12.2231067

Planet Formation Imager (PFI): Science vision and key requirements

Stefan Kraus, John D. Monnier, Michael J. Ireland, Gaspard Duchêne, Catherine Espaillat, Sebastian Hönig, Attila Juhasz, Chris Mordasini, Johan Olofsson, Claudia Paladini, Keivan Stassun, Neal Turner, Gautam Vasisht, Tim J. Harries, Matthew R. Bate, Jean François Gonzalez, Alexis Matter, Zhaohuan Zhu, Olja Panic, Zsolt RegalyAlessandro Morbidelli, Farzana Meru, Sebastian Wolf, John Ilee, Jean Philippe Berger, Ming Zhao, Quentin Kral, Andreas Morlok, Amy Bonsor, David Ciardi, Stephen R. Kane, Kaitlin Kratter, Greg Laughlin, Joshua Pepper, Sean Raymond, Lucas Labadie, Richard P. Nelson, Gerd Weigelt, Theo Ten Brummelaar, Arnaud Pierens, Rene Oudmaijer, Wilhelm Kley, Benjamin Pope, Eric L.N. Jensen, Amelia Bayo, Michael Smith, Tabetha Boyajian, Luis Henry Quiroga-Nuñez, Rafael Millan-Gabet, Andrea Chiavassa, Alexandre Gallenne, Mark Reynolds, Willem Jan De Wit, Markus Wittkowski, Florentin Millour, Poshak Gandhi, Cristina Ramos Almeida, Almudena Alonso Herrero, Chris Packham, Makoto Kishimoto, Konrad R.W. Tristram, Jörg Uwe Pott, Jean Surdej, David Buscher, Chris Haniff, Sylvestre Lacour, Romain Petrov, Steve Ridgway, Peter Tuthill, Gerard Van Belle, Phil Armitage, Clement Baruteau, Myriam Benisty, Bertram Bitsch, Sijme Jan Paardekooper, Christophe Pinte, Frederic Masset, Giovanni Rosotti

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

8 Scopus citations

Abstract

The Planet Formation Imager (PFI) project aims to provide a strong scientific vision for ground-based optical astronomy beyond the upcoming generation of Extremely Large Telescopes. We make the case that a breakthrough in angular resolution imaging capabilities is required in order to unravel the processes involved in planet formation. PFI will be optimised to provide a complete census of the protoplanet population at all stellocentric radii and over the age range from 0.1 to ∼100 Myr. Within this age period, planetary systems undergo dramatic changes and the final architecture of planetary systems is determined. Our goal is to study the planetary birth on the natural spatial scale where the material is assembled, which is the "Hill Sphere" of the forming planet, and to characterise the protoplanetary cores by measuring their masses and physical properties. Our science working group has investigated the observational characteristics of these young protoplanets as well as the migration mechanisms that might alter the system architecture. We simulated the imprints that the planets leave in the disk and study how PFI could revolutionise areas ranging from exoplanet to extragalactic science. In this contribution we outline the key science drivers of PFI and discuss the requirements that will guide the technology choices, the site selection, and potential science/technology tradeoffs.

Original language	English (US)
Title of host publication	Optical and Infrared Interferometry and Imaging V
Editors	Michelle J. Creech-Eakman, Fabien Malbet, Peter G. Tuthill
Publisher	SPIE
ISBN (Electronic)	9781510601932
DOIs	https://doi.org/10.1117/12.2231067
State	Published - 2016
Event	Optical and Infrared Interferometry and Imaging V - Edinburgh, United Kingdom Duration: Jun 27 2016 → Jul 1 2016

Publication series

Name	Proceedings of SPIE - The International Society for Optical Engineering
Volume	9907

Other

Other	Optical and Infrared Interferometry and Imaging V
Country/Territory	United Kingdom
City	Edinburgh
Period	6/27/16 → 7/1/16

Keywords

Extrasolar Planets
High Angular Resolution Imaging
Interferometry
Planet Formation
Protoplanetary Disks

ASJC Scopus subject areas

Electronic, Optical and Magnetic Materials
Condensed Matter Physics
Computer Science Applications
Applied Mathematics
Electrical and Electronic Engineering

Access to Document

10.1117/12.2231067

Cite this

Kraus, S., Monnier, J. D., Ireland, M. J., Duchêne, G., Espaillat, C., Hönig, S., Juhasz, A., Mordasini, C., Olofsson, J., Paladini, C., Stassun, K., Turner, N., Vasisht, G., Harries, T. J., Bate, M. R., Gonzalez, J. F., Matter, A., Zhu, Z., Panic, O., ... Rosotti, G. (2016). Planet Formation Imager (PFI): Science vision and key requirements. In M. J. Creech-Eakman, F. Malbet, & P. G. Tuthill (Eds.), Optical and Infrared Interferometry and Imaging V Article 99071K (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 9907). SPIE. https://doi.org/10.1117/12.2231067

Planet Formation Imager (PFI): Science vision and key requirements. / Kraus, Stefan; Monnier, John D.; Ireland, Michael J. et al.
Optical and Infrared Interferometry and Imaging V. ed. / Michelle J. Creech-Eakman; Fabien Malbet; Peter G. Tuthill. SPIE, 2016. 99071K (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 9907).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

Kraus, S, Monnier, JD, Ireland, MJ, Duchêne, G, Espaillat, C, Hönig, S, Juhasz, A, Mordasini, C, Olofsson, J, Paladini, C, Stassun, K, Turner, N, Vasisht, G, Harries, TJ, Bate, MR, Gonzalez, JF, Matter, A, Zhu, Z, Panic, O, Regaly, Z, Morbidelli, A, Meru, F, Wolf, S, Ilee, J, Berger, JP, Zhao, M, Kral, Q, Morlok, A, Bonsor, A, Ciardi, D, Kane, SR, Kratter, K, Laughlin, G, Pepper, J, Raymond, S, Labadie, L, Nelson, RP, Weigelt, G, Ten Brummelaar, T, Pierens, A, Oudmaijer, R, Kley, W, Pope, B, Jensen, ELN, Bayo, A, Smith, M, Boyajian, T, Quiroga-Nuñez, LH, Millan-Gabet, R, Chiavassa, A, Gallenne, A, Reynolds, M, De Wit, WJ, Wittkowski, M, Millour, F, Gandhi, P, Ramos Almeida, C, Alonso Herrero, A, Packham, C, Kishimoto, M, Tristram, KRW, Pott, JU, Surdej, J, Buscher, D, Haniff, C, Lacour, S, Petrov, R, Ridgway, S, Tuthill, P, Van Belle, G, Armitage, P, Baruteau, C, Benisty, M, Bitsch, B, Paardekooper, SJ, Pinte, C, Masset, F & Rosotti, G 2016, Planet Formation Imager (PFI): Science vision and key requirements. in MJ Creech-Eakman, F Malbet & PG Tuthill (eds), Optical and Infrared Interferometry and Imaging V., 99071K, Proceedings of SPIE - The International Society for Optical Engineering, vol. 9907, SPIE, Optical and Infrared Interferometry and Imaging V, Edinburgh, United Kingdom, 6/27/16. https://doi.org/10.1117/12.2231067

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title = "Planet Formation Imager (PFI): Science vision and key requirements",

abstract = "The Planet Formation Imager (PFI) project aims to provide a strong scientific vision for ground-based optical astronomy beyond the upcoming generation of Extremely Large Telescopes. We make the case that a breakthrough in angular resolution imaging capabilities is required in order to unravel the processes involved in planet formation. PFI will be optimised to provide a complete census of the protoplanet population at all stellocentric radii and over the age range from 0.1 to ∼100 Myr. Within this age period, planetary systems undergo dramatic changes and the final architecture of planetary systems is determined. Our goal is to study the planetary birth on the natural spatial scale where the material is assembled, which is the {"}Hill Sphere{"} of the forming planet, and to characterise the protoplanetary cores by measuring their masses and physical properties. Our science working group has investigated the observational characteristics of these young protoplanets as well as the migration mechanisms that might alter the system architecture. We simulated the imprints that the planets leave in the disk and study how PFI could revolutionise areas ranging from exoplanet to extragalactic science. In this contribution we outline the key science drivers of PFI and discuss the requirements that will guide the technology choices, the site selection, and potential science/technology tradeoffs.",

keywords = "Extrasolar Planets, High Angular Resolution Imaging, Interferometry, Planet Formation, Protoplanetary Disks",

author = "Stefan Kraus and Monnier, {John D.} and Ireland, {Michael J.} and Gaspard Duch{\^e}ne and Catherine Espaillat and Sebastian H{\"o}nig and Attila Juhasz and Chris Mordasini and Johan Olofsson and Claudia Paladini and Keivan Stassun and Neal Turner and Gautam Vasisht and Harries, {Tim J.} and Bate, {Matthew R.} and Gonzalez, {Jean Fran{\c c}ois} and Alexis Matter and Zhaohuan Zhu and Olja Panic and Zsolt Regaly and Alessandro Morbidelli and Farzana Meru and Sebastian Wolf and John Ilee and Berger, {Jean Philippe} and Ming Zhao and Quentin Kral and Andreas Morlok and Amy Bonsor and David Ciardi and Kane, {Stephen R.} and Kaitlin Kratter and Greg Laughlin and Joshua Pepper and Sean Raymond and Lucas Labadie and Nelson, {Richard P.} and Gerd Weigelt and {Ten Brummelaar}, Theo and Arnaud Pierens and Rene Oudmaijer and Wilhelm Kley and Benjamin Pope and Jensen, {Eric L.N.} and Amelia Bayo and Michael Smith and Tabetha Boyajian and Quiroga-Nu{\~n}ez, {Luis Henry} and Rafael Millan-Gabet and Andrea Chiavassa and Alexandre Gallenne and Mark Reynolds and {De Wit}, {Willem Jan} and Markus Wittkowski and Florentin Millour and Poshak Gandhi and {Ramos Almeida}, Cristina and {Alonso Herrero}, Almudena and Chris Packham and Makoto Kishimoto and Tristram, {Konrad R.W.} and Pott, {J{\"o}rg Uwe} and Jean Surdej and David Buscher and Chris Haniff and Sylvestre Lacour and Romain Petrov and Steve Ridgway and Peter Tuthill and {Van Belle}, Gerard and Phil Armitage and Clement Baruteau and Myriam Benisty and Bertram Bitsch and Paardekooper, {Sijme Jan} and Christophe Pinte and Frederic Masset and Giovanni Rosotti",

note = "Publisher Copyright: {\textcopyright} 2016 SPIE.; Optical and Infrared Interferometry and Imaging V ; Conference date: 27-06-2016 Through 01-07-2016",

year = "2016",

doi = "10.1117/12.2231067",

language = "English (US)",

series = "Proceedings of SPIE - The International Society for Optical Engineering",

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T2 - Optical and Infrared Interferometry and Imaging V

AU - Kraus, Stefan

AU - Monnier, John D.

AU - Ireland, Michael J.

AU - Duchêne, Gaspard

AU - Espaillat, Catherine

AU - Hönig, Sebastian

AU - Juhasz, Attila

AU - Mordasini, Chris

AU - Olofsson, Johan

AU - Paladini, Claudia

AU - Stassun, Keivan

AU - Turner, Neal

AU - Vasisht, Gautam

AU - Harries, Tim J.

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AU - Gonzalez, Jean François

AU - Matter, Alexis

AU - Zhu, Zhaohuan

AU - Panic, Olja

AU - Regaly, Zsolt

AU - Morbidelli, Alessandro

AU - Meru, Farzana

AU - Wolf, Sebastian

AU - Ilee, John

AU - Berger, Jean Philippe

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AU - Nelson, Richard P.

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AU - Bayo, Amelia

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AU - Quiroga-Nuñez, Luis Henry

AU - Millan-Gabet, Rafael

AU - Chiavassa, Andrea

AU - Gallenne, Alexandre

AU - Reynolds, Mark

AU - De Wit, Willem Jan

AU - Wittkowski, Markus

AU - Millour, Florentin

AU - Gandhi, Poshak

AU - Ramos Almeida, Cristina

AU - Alonso Herrero, Almudena

AU - Packham, Chris

AU - Kishimoto, Makoto

AU - Tristram, Konrad R.W.

AU - Pott, Jörg Uwe

AU - Surdej, Jean

AU - Buscher, David

AU - Haniff, Chris

AU - Lacour, Sylvestre

AU - Petrov, Romain

AU - Ridgway, Steve

AU - Tuthill, Peter

AU - Van Belle, Gerard

AU - Armitage, Phil

AU - Baruteau, Clement

AU - Benisty, Myriam

AU - Bitsch, Bertram

AU - Paardekooper, Sijme Jan

AU - Pinte, Christophe

AU - Masset, Frederic

AU - Rosotti, Giovanni

PY - 2016

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N2 - The Planet Formation Imager (PFI) project aims to provide a strong scientific vision for ground-based optical astronomy beyond the upcoming generation of Extremely Large Telescopes. We make the case that a breakthrough in angular resolution imaging capabilities is required in order to unravel the processes involved in planet formation. PFI will be optimised to provide a complete census of the protoplanet population at all stellocentric radii and over the age range from 0.1 to ∼100 Myr. Within this age period, planetary systems undergo dramatic changes and the final architecture of planetary systems is determined. Our goal is to study the planetary birth on the natural spatial scale where the material is assembled, which is the "Hill Sphere" of the forming planet, and to characterise the protoplanetary cores by measuring their masses and physical properties. Our science working group has investigated the observational characteristics of these young protoplanets as well as the migration mechanisms that might alter the system architecture. We simulated the imprints that the planets leave in the disk and study how PFI could revolutionise areas ranging from exoplanet to extragalactic science. In this contribution we outline the key science drivers of PFI and discuss the requirements that will guide the technology choices, the site selection, and potential science/technology tradeoffs.

AB - The Planet Formation Imager (PFI) project aims to provide a strong scientific vision for ground-based optical astronomy beyond the upcoming generation of Extremely Large Telescopes. We make the case that a breakthrough in angular resolution imaging capabilities is required in order to unravel the processes involved in planet formation. PFI will be optimised to provide a complete census of the protoplanet population at all stellocentric radii and over the age range from 0.1 to ∼100 Myr. Within this age period, planetary systems undergo dramatic changes and the final architecture of planetary systems is determined. Our goal is to study the planetary birth on the natural spatial scale where the material is assembled, which is the "Hill Sphere" of the forming planet, and to characterise the protoplanetary cores by measuring their masses and physical properties. Our science working group has investigated the observational characteristics of these young protoplanets as well as the migration mechanisms that might alter the system architecture. We simulated the imprints that the planets leave in the disk and study how PFI could revolutionise areas ranging from exoplanet to extragalactic science. In this contribution we outline the key science drivers of PFI and discuss the requirements that will guide the technology choices, the site selection, and potential science/technology tradeoffs.

KW - Extrasolar Planets

KW - High Angular Resolution Imaging

KW - Interferometry

KW - Planet Formation

KW - Protoplanetary Disks

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DO - 10.1117/12.2231067

M3 - Conference contribution

T3 - Proceedings of SPIE - The International Society for Optical Engineering

BT - Optical and Infrared Interferometry and Imaging V

A2 - Creech-Eakman, Michelle J.

A2 - Malbet, Fabien

A2 - Tuthill, Peter G.

PB - SPIE

Y2 - 27 June 2016 through 1 July 2016

ER -

Planet Formation Imager (PFI): Science vision and key requirements

Abstract

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Keywords

ASJC Scopus subject areas

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