skip navigation - jump to main content
Dawn partners    + View the NASA Portal
Search
JPL Home Earth Solar System Stars & Galaxies Technology
Dawn Banner: Dawn spacecraft orbiting Ceres and Vesta
 
Mission Science Technology Education People Multimedia Get Involved Dawn Home Page
 

Image of Ceres' Layers

   
 

Feature/Overview
and Objectives
Dawn Dictionary
Why Ceres and Vesta?
Technology

Orbit Visualization Tools:

Ceres
Vesta


 
image of Ceres  
Credit: NASA/JPL
 

GRaND Functional Testing

Reported by Tom Prettyman
"December 20 , we completed functional testing of GRaND following spacecraft (S/C) vibe and pyroshock. GRaND performed nominally and is ready to proceed to the next phase of environmental testing. The spacecraft will undergo some additional testing this week, and will then be packed up and shipped from OSC to the Naval Research Laboratory (NRL). In January, the S/C will continue environmental testing (thermal-vac) and mission scenario testing in NRL's large thermal vacuum chamber ("big blue"). Once testing at NRL is complete, the S/C will be shipped to the cape for integration with the launch vehicle. We'll keep you posted on progress."

Side note: LANL team members (Tom and Bruce) supported the test remotely and were able to monitor instrument telemetry and state-of-health from Los Alamos. While some of the future tests will require travel, the ability to carry out a portion of these remotely reduces cost and increases participation by the GRaND team. A big "thank you" is owed to the Dawn project, Betina Pavri and Jason Kim, for making this happen.

What is GRaND?

The Gamma Ray and Neutron Detector (GRaND) will measure the elemental composition of the surfaces of Vesta and Ceres.  Galactic cosmic rays, consisting primarily of high energy protons, interact with nuclei within the top few meters of the surface, producing showers of secondary particles, including gamma rays and neutrons.  Gamma rays and neutrons produced within the top meter can escape into space, and are measured in orbit by GRaND.  The gamma ray energy spectrum provides a "fingerprint," which can be analyzed to determine the abundance of major rock forming elements such as Fe and Si.  The neutron energy spectrum can be analyzed to determine the abundance of light elements, such as H and C, which are the major constituents of ices.  Gamma rays are also emitted by the decay of radioactive isotopes, such as K and Th.  Elemental abundances determined by GRaND will provide constraints on the formation and evolution of the asteroids.

   
About Us Dawn Mission: Ask a Scientist Contact Us Feedback Links Sitemap
FIRST GOV + Freedom of Information Act
+ The President's Management Agenda
+ FY 2002 Agency Performance and
accountability report

+ NASA Privacy Statement, Disclaimer,
and Accessibility Certification

+ Freedom to Manage
NASA Home Page

Site Manager: Dawn Mission Outreach Office
Webmaster: McREL
CL04-1004


link to California Institute of Technology home page link to Jet Propulsion Laboratory home page link to NASA home page