The Space Infrared Interferometric Telescope (SPIRIT): High-resolution imaging and spectroscopy in the far-infrared
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 microns. SPIRIT will provide sub-arcsecond resolution images and spectra with resolutio...
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| creator | Leisawitz, David Baker, Charles Barger, Amy Benford, Dominic Blain, Andrew Boyle, Rob Broderick, Richard Budinoff, Jason Carpenter, John Caverly, Richard Chen, Phil Cooley, Steve Cottingham, Christine Crooke, Julie DiPietro, Dave DiPirro, Mike Femiano, Michael Ferrer, Art Fischer, Jacqueline Gardner, Jonathan P Hallock, Lou Harris, Kenny Hartman, Kate Harwit, Martin Hillenbrand, Lynne Hyde, Tupper Jones, Drew Kellogg, Jim Kogut, Alan Kuchner, Marc Lawson, Bill Lecha, Javier Lecha, Maria Mainzer, Amy Mannion, Jim Martino, Anthony Mason, Paul Mather, John McDonald, Gibran Mills, Rick Mundy, Lee Ollendorf, Stan Pellicciotti, Joe Quinn, Dave Rhee, Kirk Rinehart, Stephen Sauerwine, Tim Silverberg, Robert Smith, Terry Gordon, Stacey Stahl, H Philip Staguhn, Johannes Tompkins, Steve Tveekrem, June Wall, Sheila Wilson, Mark |
| description | 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 microns. SPIRIT will provide sub-arcsecond resolution images and spectra with resolution R = 3000 in a 1 arcmin 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. |
| doi_str_mv | 10.48550/arxiv.0707.0883 |
| format | Article |
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All three observatories could be operational contemporaneously.</description><subject>Accretion disks</subject><subject>Extrasolar planets</subject><subject>Far infrared radiation</subject><subject>Field of view</subject><subject>Galactic evolution</subject><subject>Galaxies</subject><subject>Image resolution</subject><subject>Infrared telescopes</subject><subject>Observatories</subject><subject>Physics - Astrophysics of Galaxies</subject><subject>Physics - Cosmology and Nongalactic Astrophysics</subject><subject>Physics - Earth and Planetary Astrophysics</subject><subject>Physics - High Energy Astrophysical Phenomena</subject><subject>Physics - Instrumentation and Methods for Astrophysics</subject><subject>Physics - Solar and Stellar Astrophysics</subject><subject>Planet formation</subject><subject>Planetary systems</subject><subject>Protostars</subject><subject>Radio telescopes</subject><subject>Red shift</subject><subject>Space telescopes</subject><subject>Spectrum 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Harwit, Martin ; Hillenbrand, Lynne ; Hyde, Tupper ; Jones, Drew ; Kellogg, Jim ; Kogut, Alan ; Kuchner, Marc ; Lawson, Bill ; Lecha, Javier ; Lecha, Maria ; Mainzer, Amy ; Mannion, Jim ; Martino, Anthony ; Mason, Paul ; Mather, John ; McDonald, Gibran ; Mills, Rick ; Mundy, Lee ; Ollendorf, Stan ; Pellicciotti, Joe ; Quinn, Dave ; Rhee, Kirk ; Rinehart, Stephen ; Sauerwine, Tim ; Silverberg, Robert ; Smith, Terry ; Gordon, Stacey ; Stahl, H Philip ; Staguhn, Johannes ; Tompkins, Steve ; Tveekrem, June ; Wall, Sheila ; Wilson, Mark</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a516-e0e7e80e5fb7d55471ada0b3ca18667ae5f8fe94a49ddadee00727bed5d53e713</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2007</creationdate><topic>Accretion disks</topic><topic>Extrasolar planets</topic><topic>Far infrared radiation</topic><topic>Field of view</topic><topic>Galactic 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| fulltext | fulltext |
| identifier | EISSN: 2331-8422 |
| ispartof | arXiv.org, 2007-07 |
| issn | 2331-8422 |
| language | eng |
| recordid | cdi_arxiv_primary_0707_0883 |
| source | Freely Accessible Journals; arXiv.org |
| subjects | Accretion disks Extrasolar planets Far infrared radiation Field of view Galactic evolution Galaxies Image resolution Infrared telescopes Observatories Physics - Astrophysics of Galaxies Physics - Cosmology and Nongalactic Astrophysics Physics - Earth and Planetary Astrophysics Physics - High Energy Astrophysical Phenomena Physics - Instrumentation and Methods for Astrophysics Physics - Solar and Stellar Astrophysics Planet formation Planetary systems Protostars Radio telescopes Red shift Space telescopes Spectrum analysis Star & galaxy formation Star formation |
| title | The Space Infrared Interferometric Telescope (SPIRIT): High-resolution imaging and spectroscopy in the far-infrared |
| url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-02-06T04%3A17%3A37IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_arxiv&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=The%20Space%20Infrared%20Interferometric%20Telescope%20(SPIRIT):%20High-resolution%20imaging%20and%20spectroscopy%20in%20the%20far-infrared&rft.jtitle=arXiv.org&rft.au=Leisawitz,%20David&rft.date=2007-07-05&rft.eissn=2331-8422&rft_id=info:doi/10.48550/arxiv.0707.0883&rft_dat=%3Cproquest_arxiv%3E2090279526%3C/proquest_arxiv%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=2090279526&rft_id=info:pmid/&rfr_iscdi=true |