DTU delivers star cameras
DTU supplies equipment for the GRACE satellites: a special version of star cameras which help to detect the changes in the gravitational field with very high precision.
For the registration, the Earth’s varying gravitational field is exploited by letting two satellites fly after each other with a distance of about 180 km between them. Variations in the local gravitational field will affect the speed of first one and then the other satellite, resulting in changes in the distance between the two satellites.
It is these changes that can be translated into changes in the mass under the satellites.
The distance between the satellites is measured with a laser, which requires an extremely precise positioning of the two satellites, and this can be carried out with the help of the star cameras.
“We have supplied star cameras for both GRACE missions, and we’re now developing the new star cameras that will be included in the third generation of GRACE. We’re refining the technology all the time to constantly improve the star cameras—typically 10 times per generation,” says Professor John Leif Jørgensen from DTU Space.
In the first GRACE mission, DTU equipment achieved a precision corresponding to 1/100 of the thickness of a hair. In the GRACE satellites in orbit today—GRACE-FO—DTU’s instrument makers achieved a precision of 1/10,000 of a hair.
The third generation of GRACE satellites—GRACE-C—is expected to enter into orbit in 2028.