JPL Technical Report Server

HabEx Space Telescope Guiding Systems

Show simple item record

dc.contributor.author Martin, Stefan
dc.contributor.author Bottom, Michael
dc.contributor.author Nissen, Joel
dc.contributor.author Shaklan, Stuart
dc.date.accessioned 2020-04-18T04:52:19Z
dc.date.available 2020-04-18T04:52:19Z
dc.date.issued 2018-03-04
dc.identifier.citation 2018 IEEE Aerospace Conference, Big Sky, Montana, March 4-11, 2018 en_US
dc.identifier.clearanceno 18-0141
dc.identifier.uri http://hdl.handle.net/2014/47955
dc.description.abstract The HabEx (Habitable Exoplanet Imaging Mission) study is developing concepts for a next generation space telescope operating from the ultraviolet to the infrared. HabEx is making exoplanet science the primary mission objective and adding two secondary payload instruments for general astrophysics, including ultraviolet spectroscopy. For exoplanet work, two approaches are being developed. The first is a coronagraph with two separate channels to cover a broad spectral range from 450 nm to 1000 nm in two observations. The second is a starshade to cover the band 300 nm to 1000 nm in a single observation. These instruments are complementary; the coronagraph can make rapid survey observations while the starshade can reach closer in to the star and once on target, enables more efficient spectroscopic observations. This paper describes some of the key design considerations necessary to enable coronagraph and starshade observations. en_US
dc.description.sponsorship NASA/JPL en_US
dc.language.iso en_US en_US
dc.publisher Pasadena, CA: Jet Propulsion Laboratory, National Aeronautics and Space Administration, 2018 en_US
dc.title HabEx Space Telescope Guiding Systems en_US
dc.type Preprint en_US


Files in this item

This item appears in the following Collection(s)

Show simple item record

Search


Browse

My Account