Solar system science with the Single Aperture Large Telescope for Universe Studies space observatory

被引:2
|
作者
Anderson, Carrie M. [1 ]
Biver, Nicolas [2 ]
Bjoraker, Gordon L. [1 ]
Cavalie, Thibault [2 ,3 ]
Chin, Gordon [1 ]
Disanti, Michael A. [1 ]
Hartogh, Paul [4 ]
Roth, Nathan X. [5 ,6 ]
Tielens, Alexander [7 ]
Walker, Christopher K. [8 ]
机构
[1] NASA Goddard Space Flight Ctr, Planetary Syst Lab, Greenbelt, MD 20771 USA
[2] Sorbonne Univ, Univ Paris Cite, Univ PSL, CNRS,LESIA,Observ Paris, Meudon, France
[3] Univ Bordeaux, CNRS, Lab Astrophys Bordeaux, Pessac, France
[4] Max Planck Inst Solar Syst Res, Gottingen, Germany
[5] Amer Univ, Dept Phys, Washington, DC USA
[6] NASA Goddard Space Flight Ctr, Astrochem Lab, Greenbelt, MD USA
[7] Univ Maryland, Astron Dept, College Pk, MD USA
[8] Univ Arizona, Dept Astron, Steward Observ, Tucson, AZ USA
关键词
solar system; astrochemistry; cosmic origins; terahertz spectroscopy; far-infrared; space telescopes; HYDROGEN ISOTOPIC COMPOSITION; WATER-VAPOR; VERTICAL-DISTRIBUTION; PHOTOCHEMICAL MODEL; TITANS ATMOSPHERE; VENUS ATMOSPHERE; INFRARED-SPECTRA; ENCELADUS PLUME; SULFUR-DIOXIDE; D/H RATIO;
D O I
10.1117/1.JATIS.10.4.042302
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
Single Aperture Large Telescope for Universe Studies (SALTUS) is a NASA Astrophysics Probe Explorer (APEX)-class mission concept employing a robust far-infrared pointed space observatory. SALTUS comprises a 14-m inflatable reflector that provides 16x the sensitivity and 4x the angular resolution of Herschel, with a sunshield that radiatively cools the primary to 45 K, along with cryogenic detectors that collectively span the 34 to 660 mu m far-infrared spectral range at high and moderate spectral resolutions. The high sensitivity and high spectral resolving power of the SALTUS heterodyne receivers enable both submillimeter and far-infrared observations of trace compounds comprising water and its isotopologues, hydrogen deuteride (HD), and a plethora of molecular species containing carbon, hydrogen, nitrogen, oxygen, phosphorus, or sulfur (CHNOPS), all of which are obscured by the Earth's atmosphere. The high sensitivity and broadband spectral coverage of the SALTUS far-infrared grating spectrometer enables far-infrared observations of the lattice vibrational spectral signatures of ices and mineral grains contained within a wide variety of solar system targets, including comets, planetary atmospheres, near Enceladus' plumes, and on the surfaces of icy moons, Jupiter trojans, centaurs, and Kuiper Belt objects. A key objective of SALTUS is to measure HDO/H2O in both Jupiter family and Oort cloud comets. Additional observations will allow us to characterize the water torus around Saturn generated by its icy moon Enceladus, determine the source of stratospheric water in the giant planets, ascertain the time evolution of water on Venus, and search for H2O plumes on Europa, Ganymede, and Callisto. SALTUS will measure HD/H-2 in all four giant planets to constrain models of their origin. SALTUS can also measure the abundance of CHNOPS-containing molecules and halides in the atmosphere of Venus and in the comae of comets. We review the extensive amount of solar system science achievable with SALTUS for both the Guaranteed Time Observation and the Guest Observer APEX mission observing programs.
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页数:27
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