L’Ralph: A Visible/Infrared Spectral Imager for the Lucy Mission to the Trojans
The Lucy Mission to the Trojan asteroids in Jupiter’s orbit carries an instrument named L’Ralph, a visible/near infrared multi-spectral imager and a short wavelength infrared hyperspectral imager. It is one of the core instruments on Lucy, NASA’s first mission to the Trojans. L’Ralph’s primary purpo...
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Veröffentlicht in: | Space science reviews 2023-12, Vol.219 (8), p.69, Article 69 |
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creator | Reuter, D. C. Simon, A. A. Lunsford, A. Kaplan, H. Garrison, M. Simpson, J. Casto, G. Dolch, Z. Finneran, P. Grundy, W. Howett, C. Kim, P. Loose, M. Null, T. Parong, F. Rodriguez-ruiz, J. Roming, P. Smith, K. Thompson, P. Tokarcik, B. Veach, T. Wall, S. Ward, J. Weigle, E. Levison, H. |
description | The Lucy Mission to the Trojan asteroids in Jupiter’s orbit carries an instrument named L’Ralph, a visible/near infrared multi-spectral imager and a short wavelength infrared hyperspectral imager. It is one of the core instruments on Lucy, NASA’s first mission to the Trojans. L’Ralph’s primary purpose is to map the surface geology and composition of these objects, but it will also be used to search for possible tenuous exospheres. It is compact, low mass (32.3 kg), power efficient (24.5 W), and robust with high sensitivity and excellent imaging. These characteristics, and its high degree of redundancy, make L’Ralph ideally suited to this long-duration multi-flyby reconnaissance mission. |
doi_str_mv | 10.1007/s11214-023-01009-2 |
format | Article |
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C. ; Simon, A. A. ; Lunsford, A. ; Kaplan, H. ; Garrison, M. ; Simpson, J. ; Casto, G. ; Dolch, Z. ; Finneran, P. ; Grundy, W. ; Howett, C. ; Kim, P. ; Loose, M. ; Null, T. ; Parong, F. ; Rodriguez-ruiz, J. ; Roming, P. ; Smith, K. ; Thompson, P. ; Tokarcik, B. ; Veach, T. ; Wall, S. ; Ward, J. ; Weigle, E. ; Levison, H.</creator><creatorcontrib>Reuter, D. C. ; Simon, A. A. ; Lunsford, A. ; Kaplan, H. ; Garrison, M. ; Simpson, J. ; Casto, G. ; Dolch, Z. ; Finneran, P. ; Grundy, W. ; Howett, C. ; Kim, P. ; Loose, M. ; Null, T. ; Parong, F. ; Rodriguez-ruiz, J. ; Roming, P. ; Smith, K. ; Thompson, P. ; Tokarcik, B. ; Veach, T. ; Wall, S. ; Ward, J. ; Weigle, E. ; Levison, H.</creatorcontrib><description>The Lucy Mission to the Trojan asteroids in Jupiter’s orbit carries an instrument named L’Ralph, a visible/near infrared multi-spectral imager and a short wavelength infrared hyperspectral imager. It is one of the core instruments on Lucy, NASA’s first mission to the Trojans. L’Ralph’s primary purpose is to map the surface geology and composition of these objects, but it will also be used to search for possible tenuous exospheres. It is compact, low mass (32.3 kg), power efficient (24.5 W), and robust with high sensitivity and excellent imaging. 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subjects | Aerospace Technology and Astronautics Asteroid missions Asteroids Astrophysics and Astroparticles Cameras Exosphere Field programmable gate arrays Flyby missions Hyperspectral imaging Jupiter Mercury cadmium telluride Mirrors Near infrared radiation Physics Physics and Astronomy Planetology Redundancy Research centers Sensors Space Exploration and Astronautics Space Sciences (including Extraterrestrial Physics Telescopes Trojan orbits |
title | L’Ralph: A Visible/Infrared Spectral Imager for the Lucy Mission to the Trojans |
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