Eos: a FUV spectroscopic mission to observe molecular hydrogen in molecular clouds

Eos is a mission concept to be proposed to the expected 2025 NASA Small Explorers Announcement of Opportunity (SMEX AO). Eos observes molecular clouds in our galaxy and nearby planet forming disks to understand the link between star and planet formation and molecular hydrogen in galactic star forming regions. Eos does this using very long-slit, high resolution spectroscopy of far ultraviolet (FUV) emission from fluorescent molecular hydrogen (H<sub>2</sub>), a powerful and underutilized FUV diagnostic. H<sub>2</sub> is the most abundant molecule in the universe, but is typically observed in the infrared (IR) or inferred via proxies such as CO. Eos will directly observe H<sub>2</sub> via fluorescence, which can be stimulated from a range of sources (shocks, interstellar UV radiation, bright stars, etc). Here we briefly describe the science objectives of Eos, as well as the instrument implementation.

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Published
2024-08-21
DOI
https://doi.org/10.1117/12.3017644
Citations
2
Primary Topic
Atmospheric Ozone and Climate
Type
article
Field-Weighted Citation Impact
0.75

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article

Eos: a FUV spectroscopic mission to observe molecular hydrogen in molecular clouds

Tom Haworth, Haeun Chung, Elizabeth Luthman, N. Turner et al.
2 citations
Atmospheric Ozone and Climate
0.75
article

Eos: a FUV spectroscopic mission to observe molecular hydrogen in molecular clouds

Tom Haworth, Haeun Chung, Elizabeth Luthman, N. Turner, Keri Hoadley, Shmuel Bialy, Blakesley Burkhart, T. E. Dharmawardena, Seo Young Kim, Nicole Arulanantham, Karen Willacy, Miles Smith, Erika Hamden, Min-Young Lee, Shuo Kong, David Schiminovich
article en
2 citations

Abstract

Eos is a mission concept to be proposed to the expected 2025 NASA Small Explorers Announcement of Opportunity (SMEX AO). Eos observes molecular clouds in our galaxy and nearby planet forming disks to understand the link between star and planet formation and molecular hydrogen in galactic star forming regions. Eos does this using very long-slit, high resolution spectroscopy of far ultraviolet (FUV) emission from fluorescent molecular hydrogen (H<sub>2</sub>), a powerful and underutilized FUV diagnostic. H<sub>2</sub> is the most abundant molecule in the universe, but is typically observed in the infrared (IR) or inferred via proxies such as CO. Eos will directly observe H<sub>2</sub> via fluorescence, which can be stimulated from a range of sources (shocks, interstellar UV radiation, bright stars, etc). Here we briefly describe the science objectives of Eos, as well as the instrument implementation.

Vol. 534
Rutgers, The State University of New Jersey (US), University of Iowa (US), Space Telescope Science Institute (US), Jet Propulsion Laboratory (US), University of Arizona (US), Queen Mary University of London (GB), Technion – Israel Institute of Technology (IL), Flatiron Health (United States) (US), Flatiron Institute (US), Columbia University (US)
National Aeronautics and Space Administration, California Institute of Technology, Jet Propulsion Laboratory
Openalex Percentile: Top 31%
Atmospheric Ozone and Climate
0.75
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