The space infrared interferometric telescope (SPIRIT): High-resolution imaging and spectroscopy in the far-infrared

David Leisawitz; Charles Baker; Amy Barger; Dominic Benford; Andrew Blain; Rob Boyle; Richard Broderick; Jason Budinoff; John Carpenter; Richard Caverly; Phil Chen; Steve Cooley; Christine Cottingham; Julie Crooke; Dave DiPietro; Mike DiPirro; Michael Femiano; Art Ferrer; Jacqueline Fischer; Jonathan P. Gardner; Lou Hallock; Kenny Harris; Kate Hartman; Martin Harwit; Lynne Hillenbrand; Tupper Hyde; Drew Jones; Jim Kellogg; Alan Kogut; Marc Kuchner; Bill Lawson; Javier Lecha; Maria Lecha; Amy Mainzer; Jim Mannion; Anthony Martino; Paul Mason; John Mather; Gibran McDonald; Rick Mills; Lee Mundy; Stan Ollendorf; Joe Pellicciotti; Dave Quinn; Kirk Rhee; Stephen Rinehart; Tim Sauerwine; Robert Silverberg; Terry Smith; Gordon Stacey; H. Philip Stahl; Johannes Staguhn; Steve Tompkins; June Tveekrem; Sheila Wall; Mark Wilson

doi:10.1016/j.asr.2007.05.081

The space infrared interferometric telescope (SPIRIT): High-resolution imaging and spectroscopy in the far-infrared

David Leisawitz, Charles Baker, Amy Barger, Dominic Benford, Andrew Blain, Rob Boyle, Richard Broderick, Jason Budinoff, John Carpenter, Richard Caverly, Phil Chen, Steve Cooley, Christine Cottingham, Julie Crooke, Dave DiPietro, Mike DiPirro, Michael Femiano, Art Ferrer, Jacqueline Fischer, Jonathan P. GardnerLou Hallock, Kenny Harris, Kate Hartman, Martin Harwit, Lynne Hillenbrand, Tupper Hyde, Drew Jones, Jim Kellogg, Alan Kogut, Marc Kuchner, Bill Lawson, Javier Lecha, Maria Lecha, Amy Mainzer, Jim Mannion, Anthony Martino, Paul Mason, John Mather, Gibran McDonald, Rick Mills, Lee Mundy, Stan Ollendorf, Joe Pellicciotti, Dave Quinn, Kirk Rhee, Stephen Rinehart, Tim Sauerwine, Robert Silverberg, Terry Smith, Gordon Stacey, H. Philip Stahl, Johannes Staguhn, Steve Tompkins, June Tveekrem, Sheila Wall, Mark Wilson

Research output: Contribution to journal › Article › peer-review

19 Scopus citations

Abstract

We report results of a recently-completed pre-formulation phase study of SPIRIT, a candidate NASA Origins Probe mission. SPIRIT is a spatial and spectral interferometer with an operating wavelength range 25-400 μm. SPIRIT will provide sub-arcsecond resolution images and spectra with resolution R = 3000 in a 1′ field of view to accomplish three primary scientific objectives: (1) learn how planetary systems form from protostellar disks, and how they acquire their inhomogeneous composition; (2) characterize the family of extrasolar planetary systems by imaging the structure in debris disks to understand how and where planets of different types form; and (3) learn how high-redshift galaxies formed and merged to form the present-day population of galaxies. Observations with SPIRIT will be complementary to those of the James Webb Space Telescope and the ground-based Atacama Large Millimeter Array. All three observatories could be operational contemporaneously.

Original language	English (US)
Pages (from-to)	689-703
Number of pages	15
Journal	Advances in Space Research
Volume	40
Issue number	5
DOIs	https://doi.org/10.1016/j.asr.2007.05.081
State	Published - 2007
Externally published	Yes

Keywords

Cryogenic optics
Infrared
Infrared detectors
Interferometry
Origins probe
Submillimeter

ASJC Scopus subject areas

Aerospace Engineering
Astronomy and Astrophysics
Geophysics
Atmospheric Science
Space and Planetary Science
Earth and Planetary Sciences(all)

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10.1016/j.asr.2007.05.081

Cite this

Leisawitz, D., Baker, C., Barger, A., Benford, D., Blain, A., Boyle, R., Broderick, R., Budinoff, J., Carpenter, J., Caverly, R., Chen, P., Cooley, S., Cottingham, C., Crooke, J., DiPietro, D., DiPirro, M., Femiano, M., Ferrer, A., Fischer, J., ... Wilson, M. (2007). The space infrared interferometric telescope (SPIRIT): High-resolution imaging and spectroscopy in the far-infrared. Advances in Space Research, 40(5), 689-703. https://doi.org/10.1016/j.asr.2007.05.081

Leisawitz, D, Baker, C, Barger, A, Benford, D, Blain, A, Boyle, R, Broderick, R, Budinoff, J, Carpenter, J, Caverly, R, Chen, P, Cooley, S, Cottingham, C, Crooke, J, DiPietro, D, DiPirro, M, Femiano, M, Ferrer, A, Fischer, J, Gardner, JP, Hallock, L, Harris, K, Hartman, K, Harwit, M, Hillenbrand, L, Hyde, T, Jones, D, Kellogg, J, Kogut, A, Kuchner, M, Lawson, B, Lecha, J, Lecha, M, Mainzer, A, Mannion, J, Martino, A, Mason, P, Mather, J, McDonald, G, Mills, R, Mundy, L, Ollendorf, S, Pellicciotti, J, Quinn, D, Rhee, K, Rinehart, S, Sauerwine, T, Silverberg, R, Smith, T, Stacey, G, Stahl, HP, Staguhn, J, Tompkins, S, Tveekrem, J, Wall, S & Wilson, M 2007, 'The space infrared interferometric telescope (SPIRIT): High-resolution imaging and spectroscopy in the far-infrared', Advances in Space Research, vol. 40, no. 5, pp. 689-703. https://doi.org/10.1016/j.asr.2007.05.081

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title = "The space infrared interferometric telescope (SPIRIT): High-resolution imaging and spectroscopy in the far-infrared",

abstract = "We report results of a recently-completed pre-formulation phase study of SPIRIT, a candidate NASA Origins Probe mission. SPIRIT is a spatial and spectral interferometer with an operating wavelength range 25-400 μm. SPIRIT will provide sub-arcsecond resolution images and spectra with resolution R = 3000 in a 1′ field of view to accomplish three primary scientific objectives: (1) learn how planetary systems form from protostellar disks, and how they acquire their inhomogeneous composition; (2) characterize the family of extrasolar planetary systems by imaging the structure in debris disks to understand how and where planets of different types form; and (3) learn how high-redshift galaxies formed and merged to form the present-day population of galaxies. Observations with SPIRIT will be complementary to those of the James Webb Space Telescope and the ground-based Atacama Large Millimeter Array. All three observatories could be operational contemporaneously.",

keywords = "Cryogenic optics, Infrared, Infrared detectors, Interferometry, Origins probe, Submillimeter",

author = "David Leisawitz and Charles Baker and Amy Barger and Dominic Benford and Andrew Blain and Rob Boyle and Richard Broderick and Jason Budinoff and John Carpenter and Richard Caverly and Phil Chen and Steve Cooley and Christine Cottingham and Julie Crooke and Dave DiPietro and Mike DiPirro and Michael Femiano and Art Ferrer and Jacqueline Fischer and Gardner, {Jonathan P.} and Lou Hallock and Kenny Harris and Kate Hartman and Martin Harwit and Lynne Hillenbrand and Tupper Hyde and Drew Jones and Jim Kellogg and Alan Kogut and Marc Kuchner and Bill Lawson and Javier Lecha and Maria Lecha and Amy Mainzer and Jim Mannion and Anthony Martino and Paul Mason and John Mather and Gibran McDonald and Rick Mills and Lee Mundy and Stan Ollendorf and Joe Pellicciotti and Dave Quinn and Kirk Rhee and Stephen Rinehart and Tim Sauerwine and Robert Silverberg and Terry Smith and Gordon Stacey and Stahl, {H. Philip} and Johannes Staguhn and Steve Tompkins and June Tveekrem and Sheila Wall and Mark Wilson",

note = "Funding Information: Goddard{\textquoteright}s senior management made a generous resource commitment to the SPIRIT study, without which most of the results described here could not have been achieved. We are very grateful for their support. Special thanks to the SPIRIT Advisory Review Panel – Gary Melnick (SAO), Chair, Dave Miller (MIT), Harvey Moseley (GSFC), Gene Serabyn (JPL), Mike Shao (JPL), Wes Traub (SAO), Steve Unwin (JPL), and Ned Wright (UCLA) – for their expert advice. Four industry partners conducted parallel studies on selected topics and contributed their results, enhancing the success of the overall SPIRIT study. In particular, we thank Dave Fischer, Dave Glaister, Paul Hendershott, Vince Kotsubo, Jim Leitch, Jennifer Lock and Charley Noecker of Ball Aerospace, Tracey Espero, Ed Friedman and Mike Kaplan of Boeing, John Miles, Ted Nast, Jeff Olson, Dominick Tenerelli and Bob Woodruff of Lockheed-Martin, and Chuck Lillie and Ron Polidan of Northrop-Grumman. J.F. acknowledges the support of the Naval Research Laboratory 6.1 base funding. We thank our anonymous referees for their many helpful recommendations. NASA sponsored the SPIRIT study under the Origins Science Mission Concept study program.",

year = "2007",

doi = "10.1016/j.asr.2007.05.081",

language = "English (US)",

volume = "40",

pages = "689--703",

journal = "Advances in Space Research",

issn = "0273-1177",

publisher = "Elsevier Limited",

number = "5",

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T1 - The space infrared interferometric telescope (SPIRIT)

T2 - High-resolution imaging and spectroscopy in the far-infrared

AU - Leisawitz, David

AU - Baker, Charles

AU - Barger, Amy

AU - Benford, Dominic

AU - Blain, Andrew

AU - Boyle, Rob

AU - Broderick, Richard

AU - Budinoff, Jason

AU - Carpenter, John

AU - Caverly, Richard

AU - Chen, Phil

AU - Cooley, Steve

AU - Cottingham, Christine

AU - Crooke, Julie

AU - DiPietro, Dave

AU - DiPirro, Mike

AU - Femiano, Michael

AU - Ferrer, Art

AU - Fischer, Jacqueline

AU - Gardner, Jonathan P.

AU - Hallock, Lou

AU - Harris, Kenny

AU - Hartman, Kate

AU - Harwit, Martin

AU - Hillenbrand, Lynne

AU - Hyde, Tupper

AU - Jones, Drew

AU - Kellogg, Jim

AU - Kogut, Alan

AU - Kuchner, Marc

AU - Lawson, Bill

AU - Lecha, Javier

AU - Lecha, Maria

AU - Mainzer, Amy

AU - Mannion, Jim

AU - Martino, Anthony

AU - Mason, Paul

AU - Mather, John

AU - McDonald, Gibran

AU - Mills, Rick

AU - Mundy, Lee

AU - Ollendorf, Stan

AU - Pellicciotti, Joe

AU - Quinn, Dave

AU - Rhee, Kirk

AU - Rinehart, Stephen

AU - Sauerwine, Tim

AU - Silverberg, Robert

AU - Smith, Terry

AU - Stacey, Gordon

AU - Stahl, H. Philip

AU - Staguhn, Johannes

AU - Tompkins, Steve

AU - Tveekrem, June

AU - Wall, Sheila

AU - Wilson, Mark

N1 - Funding Information: Goddard’s senior management made a generous resource commitment to the SPIRIT study, without which most of the results described here could not have been achieved. We are very grateful for their support. Special thanks to the SPIRIT Advisory Review Panel – Gary Melnick (SAO), Chair, Dave Miller (MIT), Harvey Moseley (GSFC), Gene Serabyn (JPL), Mike Shao (JPL), Wes Traub (SAO), Steve Unwin (JPL), and Ned Wright (UCLA) – for their expert advice. Four industry partners conducted parallel studies on selected topics and contributed their results, enhancing the success of the overall SPIRIT study. In particular, we thank Dave Fischer, Dave Glaister, Paul Hendershott, Vince Kotsubo, Jim Leitch, Jennifer Lock and Charley Noecker of Ball Aerospace, Tracey Espero, Ed Friedman and Mike Kaplan of Boeing, John Miles, Ted Nast, Jeff Olson, Dominick Tenerelli and Bob Woodruff of Lockheed-Martin, and Chuck Lillie and Ron Polidan of Northrop-Grumman. J.F. acknowledges the support of the Naval Research Laboratory 6.1 base funding. We thank our anonymous referees for their many helpful recommendations. NASA sponsored the SPIRIT study under the Origins Science Mission Concept study program.

PY - 2007

Y1 - 2007

N2 - We report results of a recently-completed pre-formulation phase study of SPIRIT, a candidate NASA Origins Probe mission. SPIRIT is a spatial and spectral interferometer with an operating wavelength range 25-400 μm. SPIRIT will provide sub-arcsecond resolution images and spectra with resolution R = 3000 in a 1′ field of view to accomplish three primary scientific objectives: (1) learn how planetary systems form from protostellar disks, and how they acquire their inhomogeneous composition; (2) characterize the family of extrasolar planetary systems by imaging the structure in debris disks to understand how and where planets of different types form; and (3) learn how high-redshift galaxies formed and merged to form the present-day population of galaxies. Observations with SPIRIT will be complementary to those of the James Webb Space Telescope and the ground-based Atacama Large Millimeter Array. All three observatories could be operational contemporaneously.

AB - We report results of a recently-completed pre-formulation phase study of SPIRIT, a candidate NASA Origins Probe mission. SPIRIT is a spatial and spectral interferometer with an operating wavelength range 25-400 μm. SPIRIT will provide sub-arcsecond resolution images and spectra with resolution R = 3000 in a 1′ field of view to accomplish three primary scientific objectives: (1) learn how planetary systems form from protostellar disks, and how they acquire their inhomogeneous composition; (2) characterize the family of extrasolar planetary systems by imaging the structure in debris disks to understand how and where planets of different types form; and (3) learn how high-redshift galaxies formed and merged to form the present-day population of galaxies. Observations with SPIRIT will be complementary to those of the James Webb Space Telescope and the ground-based Atacama Large Millimeter Array. All three observatories could be operational contemporaneously.

KW - Cryogenic optics

KW - Infrared

KW - Infrared detectors

KW - Interferometry

KW - Origins probe

KW - Submillimeter

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JO - Advances in Space Research

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ER -

The space infrared interferometric telescope (SPIRIT): High-resolution imaging and spectroscopy in the far-infrared

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ASJC Scopus subject areas

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