干旱区生态环境知识资源中心(Arid): Solar System Science with the Orbiting Astronomical Satellite Investigating Stellar Systems (OASIS) Observatory

Arid

DOI	10.1007/s11214-022-00911-5
	Solar System Science with the Orbiting Astronomical Satellite Investigating Stellar Systems (OASIS) Observatory
	Anderson, Carrie M.; Biver, Nicolas; Bjoraker, Gordon L.; Cavalie, Thibault; Chin, Gordon; DiSanti, Michael A.; Hartogh, Paul; Tielens, Alexander; Walker, Christopher K.
通讯作者	Anderson, CM
来源期刊	SPACE SCIENCE REVIEWS
ISSN	0038-6308
EISSN	1572-9672
出版年	2022
卷号	218 期号:5
英文摘要	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.
英文关键词	Solar system science Planetary atmospheres Comets Active icy moons THz spectroscopy Heterodyne spectral resolution Flight mission concept
类型	Review
语种	英语
开放获取类型	hybrid
收录类别	SCI-E
WOS记录号	WOS:000826940200001
WOS关键词	HYDROGEN ISOTOPIC COMPOSITION ; WATER-VAPOR ; VERTICAL-DISTRIBUTION ; PROTOPLANETARY DISKS ; DEUTERIUM ABUNDANCE ; TITANS ATMOSPHERE ; VENUS ATMOSPHERE ; DEUTERATED WATER ; SULFUR-DIOXIDE ; D/H RATIO
WOS类目	Astronomy & Astrophysics
WOS研究方向	Astronomy & Astrophysics
资源类型	期刊论文
条目标识符	http://119.78.100.177/qdio/handle/2XILL650/394525
推荐引用方式 GB/T 7714	Anderson, Carrie M.,Biver, Nicolas,Bjoraker, Gordon L.,et al. Solar System Science with the Orbiting Astronomical Satellite Investigating Stellar Systems (OASIS) Observatory[J],2022,218(5).
APA	Anderson, Carrie M..,Biver, Nicolas.,Bjoraker, Gordon L..,Cavalie, Thibault.,Chin, Gordon.,...&Walker, Christopher K..(2022).Solar System Science with the Orbiting Astronomical Satellite Investigating Stellar Systems (OASIS) Observatory.SPACE SCIENCE REVIEWS,218(5).
MLA	Anderson, Carrie M.,et al."Solar System Science with the Orbiting Astronomical Satellite Investigating Stellar Systems (OASIS) Observatory".SPACE SCIENCE REVIEWS 218.5(2022).