Author
Meixner, M.Cooray, A.
Leisawitz, D.T.
Staguhn, J.G.
Armus, L.
Battersby, C.
Bauer, J.
Benford, D.
Bergin, E.
Bradford, C.M.
Burgarella, D.
Carey, S.
De Beck, E.
Ennico-Smith, K.
Fortney, J.J.
Gerin, M.
Helmich, F.P.
Kataria, T.

Mamajek, E.E.
Melnick, G.J.
Milam, S.N.
Moseley, S.H.
Narayanan, D.
Neff, S.G.
Padgett, D.
Pontoppidan, K.
Pope, A.
Roellig, T.L.
Sakon, I.
Sandstrom, K.
Scott, D.

Sheth, K.
Stevenson, K.B.
Su, K.Y.
Vieira, J.
Wiedner, M.C.
Wright, E.
Zmuidzinas, J.
Origins Study Team
Affiliation
University of Arizona, Department of Astronomy and Steward ObservatoryIssue Date
2021
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SPIECitation
Meixner, M., Cooray, A., Leisawitz, D. T., Staguhn, J. G., Armus, L., Battersby, C., ... & Origins Study Team. (2021). Origins Space Telescope science drivers to design traceability. Journal of Astronomical Telescopes, Instruments, and Systems, 7(1), 011012.Rights
Copyright © The Authors. Published by SPIE under a Creative Commons Attribution 4.0 Unported License.Collection Information
This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.Abstract
The Origins Space Telescope (Origins) concept is designed to investigate the creation and dispersal of elements essential to life, the formation of planetary systems, and the transport of water to habitable worlds and the atmospheres of exoplanets around nearby K-and M-dwarfs to identify potentially habitable-and even inhabited-worlds. These science priorities are aligned with NASA's three major astrophysics science goals: How does the Universe work? How did we get here? and Are we alone? We briefly describe the science case that arose from the astronomical community and the science traceability matrix for Origins. The science traceability matrix prescribes the design of Origins and demonstrates that it will address the key science questions motivated by the science case. © The Authors. Published by SPIE under a Creative Commons Attribution 4.0 Unported License. Distribution or reproduction of this work in whole or in part requires full attribution of the original publication, including its DOI.Note
Open access articleISSN
2329-4124Version
Final published versionae974a485f413a2113503eed53cd6c53
10.1117/1.JATIS.7.1.011012
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Except where otherwise noted, this item's license is described as Copyright © The Authors. Published by SPIE under a Creative Commons Attribution 4.0 Unported License.