The chemical inventory of the inner regions of planet-forming disks - the JWST/MINDS program

Inga Kamp; Thomas Henning; Aditya M. Arabhavi; Giulio Bettoni; Valentin Christiaens; Danny Gasman; Sierra L. Grant; Maria Morales-Calderón; Benoit Tabone; Alain Abergel; Olivier Absil; Ioannis Argyriou; David Barrado; Anthony Boccaletti; Jeroen Bouwman; Alessio Caratti o Garatti; Ewine F. van Dishoeck; Vincent Geers; Adrian M. Glauser; Manuel Güdel; Rodrigo Guadarrama; Hyerin Jang; Jayatee Kanwar; Pierre-Olivier Lagage; Fred Lahuis; Michael Mueller; Cyrine Nehmé; Göran Olofsson; Eric Pantin; Nicole Pawellek; Giulia Perotti; Tom P. Ray; Donna Rodgers-Lee; Matthias Samland; Silvia Scheithauer; Jürgen Schreiber; Kamber Schwarz; Milou Temmink; Bart Vandenbussche; Marissa Vlasblom; Christoffel Waelkens; L.~B.~F.~M. Waters; Gillian Wright

doi:10.1039/D3FD00013C

The chemical inventory of the inner regions of planet-forming disks - the JWST/MINDS program

Inga Kamp, Thomas Henning, Aditya M. Arabhavi, Giulio Bettoni, Valentin Christiaens, Danny Gasman, Sierra L. Grant, Maria Morales-Calderón, Benoit Tabone, Alain Abergel, Olivier Absil, Ioannis Argyriou, David Barrado, Anthony Boccaletti, Jeroen Bouwman, Alessio Caratti o Garatti, Ewine F. van Dishoeck, Vincent Geers, Adrian M. Glauser, Manuel GüdelRodrigo Guadarrama, Hyerin Jang, Jayatee Kanwar, Pierre-Olivier Lagage, Fred Lahuis, Michael Mueller, Cyrine Nehmé, Göran Olofsson, Eric Pantin, Nicole Pawellek, Giulia Perotti, Tom P. Ray, Donna Rodgers-Lee, Matthias Samland, Silvia Scheithauer, Jürgen Schreiber, Kamber Schwarz, Milou Temmink, Bart Vandenbussche, Marissa Vlasblom, Christoffel Waelkens, L.~B.~F.~M. Waters, Gillian Wright

Department of Astrophysics

Publications: Contribution to journal › Article › Peer Reviewed

Abstract

The understanding of planet formation has changed recently, embracing the new idea of pebble accretion. This means that the influx of pebbles from the outer regions of planet-forming disks to their inner zones could determine the composition of planets and their atmospheres. The solid and molecular components delivered to the planet-forming region can be best characterized by mid-infrared spectroscopy. With Spitzer low-resolution (R = 100, 600) spectroscopy, this approach was limited to the detection of abundant molecules, such as H ₂O, C ₂H ₂, HCN and CO ₂. This contribution will present the first results of the MINDS (MIRI mid-INfrared Disk Survey, PI:Th Henning) project. Due do the sensitivity and spectral resolution provided by the James Webb Space Telescope (JWST), we now have a unique tool to obtain the full inventory of chemistry in the inner disks of solar-type stars and brown dwarfs, including also less-abundant hydrocarbons and isotopologues. The Integral Field Unit (IFU) capabilities will enable at the same time spatial studies of the continuum and line emission in extended sources such as debris disks, the flying saucer and also the search for mid-IR signatures of forming planets in systems such as PDS 70. These JWST observations are complementary to ALMA and NOEMA observations of outer-disk chemistry; together these datasets will provide an integral view of the processes occurring during the planet-formation phase.

Original language	English
Pages (from-to)	112-137
Number of pages	26
Journal	Faraday Discussions
Volume	245
DOIs	https://doi.org/10.1039/D3FD00013C
Publication status	Published - Sept 2023

Austrian Fields of Science 2012

103004 Astrophysics
103003 Astronomy

Keywords

Astrophysics - Earth and Planetary Astrophysics
Astrophysics - Solar and Stellar Astrophysics

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10.1039/D3FD00013CLicence: CC BY 4.0

https://arxiv.org/pdf/2307.16729.pdf

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Kamp, I., Henning, T., Arabhavi, A. M., Bettoni, G., Christiaens, V., Gasman, D., Grant, S. L., Morales-Calderón, M., Tabone, B., Abergel, A., Absil, O., Argyriou, I., Barrado, D., Boccaletti, A., Bouwman, J., Caratti o Garatti, A., van Dishoeck, E. F., Geers, V., Glauser, A. M., ... Wright, G. (2023). The chemical inventory of the inner regions of planet-forming disks - the JWST/MINDS program. Faraday Discussions, 245, 112-137. https://doi.org/10.1039/D3FD00013C

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abstract = "The understanding of planet formation has changed recently, embracing the new idea of pebble accretion. This means that the influx of pebbles from the outer regions of planet-forming disks to their inner zones could determine the composition of planets and their atmospheres. The solid and molecular components delivered to the planet-forming region can be best characterized by mid-infrared spectroscopy. With Spitzer low-resolution (R = 100, 600) spectroscopy, this approach was limited to the detection of abundant molecules, such as H 2O, C 2H 2, HCN and CO 2. This contribution will present the first results of the MINDS (MIRI mid-INfrared Disk Survey, PI:Th Henning) project. Due do the sensitivity and spectral resolution provided by the James Webb Space Telescope (JWST), we now have a unique tool to obtain the full inventory of chemistry in the inner disks of solar-type stars and brown dwarfs, including also less-abundant hydrocarbons and isotopologues. The Integral Field Unit (IFU) capabilities will enable at the same time spatial studies of the continuum and line emission in extended sources such as debris disks, the flying saucer and also the search for mid-IR signatures of forming planets in systems such as PDS 70. These JWST observations are complementary to ALMA and NOEMA observations of outer-disk chemistry; together these datasets will provide an integral view of the processes occurring during the planet-formation phase.",

keywords = "Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics",

author = "Inga Kamp and Thomas Henning and Arabhavi, {Aditya M.} and Giulio Bettoni and Valentin Christiaens and Danny Gasman and Grant, {Sierra L.} and Maria Morales-Calder{\'o}n and Benoit Tabone and Alain Abergel and Olivier Absil and Ioannis Argyriou and David Barrado and Anthony Boccaletti and Jeroen Bouwman and {Caratti o Garatti}, Alessio and {van Dishoeck}, {Ewine F.} and Vincent Geers and Glauser, {Adrian M.} and Manuel G{\"u}del and Rodrigo Guadarrama and Hyerin Jang and Jayatee Kanwar and Pierre-Olivier Lagage and Fred Lahuis and Michael Mueller and Cyrine Nehm{\'e} and G{\"o}ran Olofsson and Eric Pantin and Nicole Pawellek and Giulia Perotti and Ray, {Tom P.} and Donna Rodgers-Lee and Matthias Samland and Silvia Scheithauer and J{\"u}rgen Schreiber and Kamber Schwarz and Milou Temmink and Bart Vandenbussche and Marissa Vlasblom and Christoffel Waelkens and L.~B.~F.~M. Waters and Gillian Wright",

year = "2023",

month = sep,

doi = "10.1039/D3FD00013C",

language = "English",

volume = "245",

pages = "112--137",

journal = "Faraday Discussions",

issn = "1359-6640",

publisher = "ROYAL SOC CHEMISTRY",

}

Kamp, I, Henning, T, Arabhavi, AM, Bettoni, G, Christiaens, V, Gasman, D, Grant, SL, Morales-Calderón, M, Tabone, B, Abergel, A, Absil, O, Argyriou, I, Barrado, D, Boccaletti, A, Bouwman, J, Caratti o Garatti, A, van Dishoeck, EF, Geers, V, Glauser, AM, Güdel, M, Guadarrama, R, Jang, H, Kanwar, J, Lagage, P-O, Lahuis, F, Mueller, M, Nehmé, C, Olofsson, G, Pantin, E, Pawellek, N, Perotti, G, Ray, TP, Rodgers-Lee, D, Samland, M, Scheithauer, S, Schreiber, J, Schwarz, K, Temmink, M, Vandenbussche, B, Vlasblom, M, Waelkens, C, Waters, LBFM & Wright, G 2023, 'The chemical inventory of the inner regions of planet-forming disks - the JWST/MINDS program', Faraday Discussions, vol. 245, pp. 112-137. https://doi.org/10.1039/D3FD00013C

TY - JOUR

T1 - The chemical inventory of the inner regions of planet-forming disks - the JWST/MINDS program

AU - Kamp, Inga

AU - Henning, Thomas

AU - Arabhavi, Aditya M.

AU - Bettoni, Giulio

AU - Christiaens, Valentin

AU - Gasman, Danny

AU - Grant, Sierra L.

AU - Morales-Calderón, Maria

AU - Tabone, Benoit

AU - Abergel, Alain

AU - Absil, Olivier

AU - Argyriou, Ioannis

AU - Barrado, David

AU - Boccaletti, Anthony

AU - Bouwman, Jeroen

AU - Caratti o Garatti, Alessio

AU - van Dishoeck, Ewine F.

AU - Geers, Vincent

AU - Glauser, Adrian M.

AU - Güdel, Manuel

AU - Guadarrama, Rodrigo

AU - Jang, Hyerin

AU - Kanwar, Jayatee

AU - Lagage, Pierre-Olivier

AU - Lahuis, Fred

AU - Mueller, Michael

AU - Nehmé, Cyrine

AU - Olofsson, Göran

AU - Pantin, Eric

AU - Pawellek, Nicole

AU - Perotti, Giulia

AU - Ray, Tom P.

AU - Rodgers-Lee, Donna

AU - Samland, Matthias

AU - Scheithauer, Silvia

AU - Schreiber, Jürgen

AU - Schwarz, Kamber

AU - Temmink, Milou

AU - Vandenbussche, Bart

AU - Vlasblom, Marissa

AU - Waelkens, Christoffel

AU - Waters, L.~B.~F.~M.

AU - Wright, Gillian

PY - 2023/9

Y1 - 2023/9

N2 - The understanding of planet formation has changed recently, embracing the new idea of pebble accretion. This means that the influx of pebbles from the outer regions of planet-forming disks to their inner zones could determine the composition of planets and their atmospheres. The solid and molecular components delivered to the planet-forming region can be best characterized by mid-infrared spectroscopy. With Spitzer low-resolution (R = 100, 600) spectroscopy, this approach was limited to the detection of abundant molecules, such as H 2O, C 2H 2, HCN and CO 2. This contribution will present the first results of the MINDS (MIRI mid-INfrared Disk Survey, PI:Th Henning) project. Due do the sensitivity and spectral resolution provided by the James Webb Space Telescope (JWST), we now have a unique tool to obtain the full inventory of chemistry in the inner disks of solar-type stars and brown dwarfs, including also less-abundant hydrocarbons and isotopologues. The Integral Field Unit (IFU) capabilities will enable at the same time spatial studies of the continuum and line emission in extended sources such as debris disks, the flying saucer and also the search for mid-IR signatures of forming planets in systems such as PDS 70. These JWST observations are complementary to ALMA and NOEMA observations of outer-disk chemistry; together these datasets will provide an integral view of the processes occurring during the planet-formation phase.

AB - The understanding of planet formation has changed recently, embracing the new idea of pebble accretion. This means that the influx of pebbles from the outer regions of planet-forming disks to their inner zones could determine the composition of planets and their atmospheres. The solid and molecular components delivered to the planet-forming region can be best characterized by mid-infrared spectroscopy. With Spitzer low-resolution (R = 100, 600) spectroscopy, this approach was limited to the detection of abundant molecules, such as H 2O, C 2H 2, HCN and CO 2. This contribution will present the first results of the MINDS (MIRI mid-INfrared Disk Survey, PI:Th Henning) project. Due do the sensitivity and spectral resolution provided by the James Webb Space Telescope (JWST), we now have a unique tool to obtain the full inventory of chemistry in the inner disks of solar-type stars and brown dwarfs, including also less-abundant hydrocarbons and isotopologues. The Integral Field Unit (IFU) capabilities will enable at the same time spatial studies of the continuum and line emission in extended sources such as debris disks, the flying saucer and also the search for mid-IR signatures of forming planets in systems such as PDS 70. These JWST observations are complementary to ALMA and NOEMA observations of outer-disk chemistry; together these datasets will provide an integral view of the processes occurring during the planet-formation phase.

KW - Astrophysics - Earth and Planetary Astrophysics

KW - Astrophysics - Solar and Stellar Astrophysics

UR - http://www.scopus.com/inward/record.url?scp=85164314932&partnerID=8YFLogxK

U2 - 10.1039/D3FD00013C

DO - 10.1039/D3FD00013C

M3 - Article

SN - 1359-6640

VL - 245

SP - 112

EP - 137

JO - Faraday Discussions

JF - Faraday Discussions

ER -

The chemical inventory of the inner regions of planet-forming disks - the JWST/MINDS program

Abstract

Austrian Fields of Science 2012

Keywords

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