Improved Lyman-Ultraviolet Astronomy Capabilities through Enhanced Coatings

Metadata Updated: November 12, 2020

The  Large Ultraviolet ,Visible, Optical, Infrared (LUVOIR) telescope concept is one of the  NASA mission concept studies for the 2020 decadal study that will merge ultraviolet (UV) astrophysics and visible exoplanet science. This proposal aims at developing broadband reflecting mirror coatings with high performance that could be used on the primiary mirror of LUVOIR in order to enable wavelength coverage from the infrared and down to the Far-Ultraviolet (FUV) spectral regions. Improved reflective coatings for optics, particularly in the FUV region (90-120 nm), could yield dramatically more sensitive instruments and permit more instrument design freedom. The coating performance developed through this work will be evaluated both theoretically and experimentally in the context of meeting requirements for exoplanet research.Pure Aluminum exhibits a high reflectance over the proposed spectral range of the LUVOIR observatory (90-5000 nm). However, the Al has to be protected from the naturally occurring Al2O3 oxide layer (when exposed to oxygen) with a thin film of a transparent material for use below 130 nm. Aluminum protected with fluorides such as LiF or MgF2 have been the most commonly used solutions [4]. But below 102 nm down to 90 nm, no transparent material is available to protect Al and coating mirror reflectance stays well below 30%. But even above 102 nm, the reflectance of protected Al is limited by the residual absorption of the fluoride overcoats and the hygroscopic nature of the LiF overcoat.  The low reflectivity of coatings in the Lyman Ultraviolet (LUV) range of 90-130 nm is one of the biggest constraints on FUV telescope and spectrograph design, and it limits the science return of FUV-sensitive space missions. In fact, to achieve high-reflectance in broadband coatings has been identified as an “Essential Goal” in the technology needs for the LUVOIR) surveyor observatory. Improved reflective coatings for optics, particularly in the LUV spectrum, could yield dramatically more sensitive instruments and permit more instrument design freedom. Furthermore, investigations in improving reflectance performance of coatings in this region has the potential to offer unprecedented return on investment given that the LUV contains the highest density of line observations in the UVVIS-IR spectrum. 

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Public: This dataset is intended for public access and use. License: No license information was provided. If this work was prepared by an officer or employee of the United States government as part of that person's official duties it is considered a U.S. Government Work.

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Metadata Created Date November 12, 2020
Metadata Updated Date November 12, 2020

Metadata Source

Harvested from NASA Data.json

Additional Metadata

Resource Type Dataset
Metadata Created Date November 12, 2020
Metadata Updated Date November 12, 2020
Publisher Space Technology Mission Directorate
Unique Identifier Unknown
Maintainer
Identifier TECHPORT_90773
Data First Published 2017-09-01
Data Last Modified 2020-01-29
Public Access Level public
Bureau Code 026:00
Metadata Context https://project-open-data.cio.gov/v1.1/schema/catalog.jsonld
Metadata Catalog ID https://data.nasa.gov/data.json
Schema Version https://project-open-data.cio.gov/v1.1/schema
Catalog Describedby https://project-open-data.cio.gov/v1.1/schema/catalog.json
Homepage URL https://techport.nasa.gov/view/90773
Program Code 026:027
Source Datajson Identifier True
Source Hash 53f418960e3e73e072aba1b9e272470f99969ac1
Source Schema Version 1.1

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