Solar System Science with the Orbiting Astronomical Satellite Investigating Stellar Systems (OASIS) Observatory

被引：6

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
]}

Tielens, Alexander ^{[5
]}

Walker, Christopher K. ^{[6
]}

机构：

[1] NASA, Planetary Syst Lab, Goddard Space Flight Ctr, 8800 Greenbelt Rd, Greenbelt, MD 20771 USA

[2] Sorbonne Univ, Univ PSL, Univ Paris, Observ Paris,LESIA,CNRS, Meudon, France

[3] Univ Bordeaux, Lab Astrophys Bordeaux, B18N, CNRS, Allee Geoffroy St Hilaire, F-33615 Pessac, France

[4] Max Planck Inst Solar Syst Res, Justus von Liebig Weg 3, Gottingen, Germany

[5] Leiden Observ, POB 9513, Leiden, Netherlands

[6] Univ Arizona, Dept Astron & Steward Observ, Tucson, AZ 85719 USA

来源：

SPACE SCIENCE REVIEWS | 2022年 / 218卷 / 05期

关键词：

Solar system science; Planetary atmospheres; Comets; Active icy moons; THz spectroscopy; Heterodyne spectral resolution; Flight mission concept; HYDROGEN ISOTOPIC COMPOSITION; WATER-VAPOR; VERTICAL-DISTRIBUTION; PROTOPLANETARY DISKS; DEUTERIUM ABUNDANCE; TITANS ATMOSPHERE; VENUS ATMOSPHERE; DEUTERATED WATER; SULFUR-DIOXIDE; D/H RATIO;

D O I：

10.1007/s11214-022-00911-5

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The overarching theme of the Orbiting Astronomical Satellite for Investigating Stellar Systems (OASIS), an Astrophysics MIDEX-class mission concept, is Following water from galaxies, through protostellar systems, to Earth's oceans. The OASIS science objectives address fundamental questions raised in "Pathways to Discovery in Astronomy and Astrophysics for the 2020s (National Academies of Sciences and Medicine, Pathways to Discovery in Astronomy and Astrophysics for the 2020s, 2021, , )" and in "Enduring Quests and Daring Visions" (Kouveliotou et al. in Enduring quests-daring visions (NASA astrophysics in the next three decades), 2014, ), in the areas of: 1) the Interstellar Medium and Planet Formation, 2) Exoplanets, Astrobiology, and the Solar System, and 3) Galaxies. The OASIS science objectives require space-borne observations of galaxies, molecular clouds, protoplanetary disks, and solar system objects utilizing a telescope with a collecting area that is only achievable by large apertures coupled with cryogenic heterodyne receivers. OASIS will deploy an innovative 14-meter inflatable reflector that enables >16x the sensitivity and >4x the angular resolution of Herschel, and complements the short wavelength capabilities of James Webb Space Telescope. The OASIS state-of-the-art cryogenic heterodyne receivers will enable high spectral resolution (resolving power >10(6)) observations at terahertz (THz) frequencies. These frequencies encompass far-IR transitions of water and its isotopologues, HD, and other molecular species, from 660 to 63 mu m that are otherwise obscured by Earth's atmosphere. From observations of the ground state HD line, OASIS will directly measure gas mass in a wide variety of astrophysical objects. Over its one-year baseline mission, OASIS will find water sources as close as the Moon, to galaxies similar to 4 billion light years away. This paper reviews the solar system science achievable and planned with OASIS.

引用

页数：26

共 125 条

[1] Complications in the ALMA Detection of Phosphine at Venus [J].

Akins, Alex B. ;

Lincowski, Andrew P. ;

Meadows, Victoria S. ;

Steffes, Paul G. .

ASTROPHYSICAL JOURNAL LETTERS, 2021, 907 (02)

[2] THE MEASURED COMPOSITIONS OF URANUS AND NEPTUNE FROM THEIR FORMATION ON THE CO ICE LINE [J].

Ali-Dib, Mohamad ;

Mousis, Olivier ;

Petit, Jean-Marc ;

Lunine, Jonathan I. .

ASTROPHYSICAL JOURNAL, 2014, 793 (01)

[3] 67P/Churyumov-Gerasimenko, a Jupiter family comet with a high D/H ratio [J].

Altwegg, K. ;

Balsiger, H. ;

Bar-Nun, A. ;

Berthelier, J. J. ;

Bieler, A. ;

Bochsler, P. ;

Briois, C. ;

Calmonte, U. ;

Combi, M. ;

De Keyser, J. ;

Eberhardt, P. ;

Fiethe, B. ;

Fuselier, S. ;

Gasc, S. ;

Gombosi, T. I. ;

Hansen, K. C. ;

Haessig, M. ;

Jaeckel, A. ;

Kopp, E. ;

Korth, A. ;

Leroy, L. ;

Mall, U. ;

Marty, B. ;

Mousis, O. ;

Neefs, E. ;

Owen, T. ;

Reme, H. ;

Rubin, M. ;

Semon, T. ;

Tzou, C. -Y. ;

Waite, H. ;

Wurz, P. .

SCIENCE, 2015, 347 (6220)

[4] Subsidence-induced methane clouds in Titan's winter polar stratosphere and upper troposphere [J].

Anderson, C. M. ;

Samuelson, R. E. ;

Achterberg, R. K. ;

Barnes, J. W. ;

Flasar, F. M. .

ICARUS, 2014, 243 :129-138

[5] Debiasing the NEOWISE Cryogenic Mission Comet Populations [J].

Bauer, James M. ;

Grav, Tommy ;

Fernandez, Yanga R. ;

Mainzer, A. K. ;

Kramer, Emily A. ;

Masiero, Joseph R. ;

Spahr, Timothy ;

Nugent, C. R. ;

Stevenson, Rachel A. ;

Meech, Karen J. ;

Cutri, Roc M. ;

Lisse, Carey M. ;

Walker, Russell ;

Dailey, John W. ;

Rosser, Joshua ;

Krings, Phillip ;

Ruecker, Kinjal ;

Wright, Edward L. .

ASTRONOMICAL JOURNAL, 2017, 154 (02)

[6] Lunar soil hydration constrained by exospheric water liberated by meteoroid impacts [J].

Benna, M. ;

Hurley, D. M. ;

Stubbs, T. J. ;

Mahaffy, P. R. ;

Elphic, R. C. .

NATURE GEOSCIENCE, 2019, 12 (05) :333-+

[7] SPICAV on Venus Express:: Three spectrometers to study the global structure and composition of the Venus atmosphere [J].

Bertaux, Jean-Loup ;

Nevejans, D. ;

Korablev, O. ;

Villard, E. ;

Quemerais, E. ;

Neefs, E. ;

Montmessin, F. ;

Leblanc, F. ;

Dubois, J. P. ;

Dimarellis, E. ;

Hauchecorne, A. ;

Lefevre, F. ;

Rannou, P. ;

Chaufray, J. Y. ;

Cabane, M. ;

Cernogora, G. ;

Souchon, G. ;

Sernelin, F. ;

Reberac, A. ;

Van Ransbeek, E. ;

Berkenbosch, S. ;

Clairquin, R. ;

Muller, C. ;

Forget, F. ;

Hourdin, F. ;

Talagrand, O. ;

Rodin, A. ;

Fedorova, A. ;

Stepanov, A. ;

Vinogradov, I. ;

Kiselev, A. ;

Kalinnikov, Yu. ;

Durry, Georges ;

Sandel, B. ;

Stern, A. ;

Gerard, J. C. .

PLANETARY AND SPACE SCIENCE, 2007, 55 (12) :1673-1700

[8] Radio wavelength molecular observations of comets C/1999 T1 (McNaught-Hartley), C/2001 A2 (LINEAR), C/2000 WM1 (LINEAR) and 153P/Ikeya-Zhang [J].

Biver, N ;

Bockelée-Morvan, D ;

Crovisier, J ;

Lis, DC ;

Moreno, R ;

Colom, P ;

Henry, F ;

Herpin, F ;

Paubert, G ;

Womack, M .

ASTRONOMY & ASTROPHYSICS, 2006, 449 (03) :1255-U240

[9] Isotopic ratios of H, C, N, O, and S in comets C/2012 F6 (Lemmon) and C/2014 Q2 (Lovejoy) [J].

Biver, N. ;

Moreno, R. ;

Bockelee-Morvan, D. ;

Sandqvist, Aa. ;

Colom, P. ;

Crovisier, J. ;

Lis, D. C. ;

Boissier, J. ;

Debout, V. ;

Paubert, G. ;

Milam, S. ;

Hjalmarson, A. ;

Lundin, S. ;

Karlsson, T. ;

Battelino, M. ;

Frisk, U. ;

Murtagh, D. .

ASTRONOMY & ASTROPHYSICS, 2016, 589

[10]

Biver N., 2022, COMET 46P WIRTANEN A

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