Single Aperture Large Telescope for Universe Studies: science overview

被引:0
|
作者
Chin, Gordon [1 ]
Anderson, Carrie M. [1 ]
Bergner, Jennifer [2 ]
Biver, Nicolas [3 ]
Bjoraker, Gordon L. [1 ]
Cavalie, Thibault [3 ,4 ]
Disanti, Michael [1 ]
Gao, Jian-Rong [5 ]
Hartogh, Paul [6 ]
Harding, Leon K. [7 ]
Hu, Qing [8 ]
Kim, Daewook [9 ]
Kulesa, Craig [9 ]
de Lange, Gert [5 ]
Leisawitz, David T. [1 ]
Levy, Rebecca C. [9 ]
Lichtenberger, Arthur [10 ]
Marrone, Daniel P. [9 ]
Najita, Joan [11 ]
Newswander, Trent [12 ]
Rieke, George H. [9 ]
Rigopoulou, Dimitra [13 ]
Roelfsema, Peter [5 ]
Roth, Nathan X. [1 ]
Schwarz, Kamber [14 ]
Shirley, Yancy [9 ]
Spilker, Justin [15 ]
Stark, Antony A. [16 ]
van der Tak, Floris [5 ]
Takashima, Yuzuru [9 ]
Tielens, Alexander [17 ]
Willner, David J. [16 ]
Wollack, Edward J. [1 ]
Yates, Stephen [5 ]
Young, Erick [18 ]
Walker, Christopher K. [9 ]
机构
[1] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[2] Univ Calif Berkeley, Berkeley, CA USA
[3] Observ Paris, LESIA, CNRS, Meudon, France
[4] Univ Bordeaux, Lab Astrophys Bordeaux, CNRS, Bordeaux, France
[5] Netherlands Inst Space Res SRON, Leiden, Netherlands
[6] Max Planck Inst Solar Syst Res, Gottingen, Germany
[7] Northrop Grumman Space Syst, Dulles, VA USA
[8] MIT, EECS, Cambridge, MA USA
[9] Univ Arizona, Tucson, AZ USA
[10] Univ Virginia, Charlottesville, VA USA
[11] Natl Opt Astron Observ NOAO, Tucson, AZ USA
[12] UTAH STATE UNIV, STEWART RADIANCE LAB SDL, Logan, UT USA
[13] Univ Oxford, Clarendon Lab, Oxford, England
[14] Max Planck Inst Astron, Heidelberg, Germany
[15] Texas A&M Univ, College Stn, TX USA
[16] Harvard Smithsonian, Ctr Astrophys, Cambridge, MA USA
[17] Univ Maryland, College Pk, MD USA
[18] Univ Space Res Assoc, Washington, DC USA
关键词
far-infrared observatory; cooled deployable antenna; cryogenic heterodyne instrument; MKID grating spectrometer; HYDROGEN ISOTOPIC COMPOSITION; WATER; CONFUSION; ABUNDANCE; DISKS; D/H;
D O I
10.1117/1.JATIS.10.4.042310
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
The Single Aperture Large Telescope for Universe Studies (SALTUS) probe mission will provide a powerful far-infrared (far-IR) pointed space observatory to explore our cosmic origins and the possibility of life elsewhere. The observatory employs an innovative deployable 14-m aperture, with a sunshield that will radiatively cool the off-axis primary to <45 K. This cooled primary reflector works in tandem with cryogenic coherent and incoherent instruments that span 34- to 660-mu m far-IR range at both high and moderate spectral resolutions. The mission architecture, using proven Northrop Grumman designs, provides visibility to the entire sky every 6 months with similar to 35% of the sky observable at any one time. SALTUS's spectral range is unavailable to any existing ground or current space observatory. SALTUS will have 16x the collecting area and 4x the angular resolution of Herschel and is designed for a lifetime of >= 5 years. The SALTUS science team has proposed a Guaranteed Time Observations program to demonstrate the observatory's capabilities and, at the same time, address high-priority questions from the Decadal survey that align with NASA's Astrophysics Roadmap. With a large aperture enabling high spatial resolution and sensitive instruments, SALTUS will offer >80% of its available observing time to Guest Observer programs, providing the science community with powerful capabilities to study the local and distant universe with observations of 1000s of diverse targets such as distant and nearby galaxies, star-forming regions, protoplanetary disks, and solar system objects.
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页数:21
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