4.4 Article

Origins Space Telescope: baseline mission concept

出版社

SPIE-SOC PHOTO-OPTICAL INSTRUMENTATION ENGINEERS
DOI: 10.1117/1.JATIS.7.1.011002

关键词

infrared; space telescope; cryogenic; spectroscopy; galaxy evolution; planet formation; biosignatures

资金

  1. NASA

向作者/读者索取更多资源

The Origins Space Telescope will trace the history of our origins using mid- and far-infrared wavelengths, providing powerful spectroscopic instruments and high sensitivity to answer questions regarding galaxy evolution, habitable planet formation, and the prevalence of life-bearing worlds in the Universe. Origins minimizes complexity in its design, leveraging technology from previous space telescopes and next-generation detector technology to achieve natural background-limited sensitivity.
The Origins Space Telescope will trace the history of our origins from the time dust and heavy elements permanently altered the cosmic landscape to present-day life. How did galaxies evolve from the earliest galactic systems to those found in the Universe today? How do habitable planets form? How common are life-bearing worlds? To answer these alluring questions, Origins will operate atmid- and far-infrared (IR) wavelengths and offer powerful spectroscopic instruments and sensitivity three orders of magnitude better than that of the Herschel Space Observatory, the largest telescope flown in space to date. We describe the baseline concept for Origins recommended to the 2020 US Decadal Survey in Astronomy and Astrophysics. The baseline design includes a 5.9-m diameter telescope cryocooled to 4.5 K and equipped with three scientific instruments. A mid-infrared instrument (Mid-Infrared Spectrometer and Camera Transit spectrometer) will measure the spectra of transiting exoplanets in the 2.8 to 20 mu m wavelength range and offer unprecedented spectrophotometric precision, enabling definitive exoplanet biosignature detections. The far-IR imager polarimeter will be able to survey thousands of square degrees with broadband imaging at 50 and 250 mu m. The Origins Survey Spectrometer will cover wavelengths from 25 to 588 mu m, making wide-area and deep spectroscopic surveys with spectral resolving power R similar to 300, and pointed observations at R similar to 40;000 and 300,000 with selectable instrument modes. Origins was designed to minimize complexity. The architecture is similar to that of the Spitzer Space Telescope and requires very few deployments after launch, while the cryothermal system design leverages James Webb Space Telescope technology and experience. A combination of current-state-of-the-art cryocoolers and next-generation detector technology will enable Origins' natural background-limited sensitivity. (C) The Authors. Published by SPIE under a Creative Commons Attribution 4.0 Unported License.

作者

我是这篇论文的作者
点击您的名字以认领此论文并将其添加到您的个人资料中。

评论

主要评分

4.4
评分不足

次要评分

新颖性
-
重要性
-
科学严谨性
-
评价这篇论文

推荐

暂无数据
暂无数据