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The Gravity Recovery and Climate Experiment (GRACE) and GRACE Follow-On (GRACE-FO) are satellite missions designed to measure changes in Earth’s gravity field over time.

GRACE was launched in 2002, as a joint partnership between NASA and the German Space Agency (DLR). The key partners were the University of Texas Center for Space Research (CSR), the German Research Centre for Geosciences  (GFZ), and the Jet Propulsion Laboratory (JPL).

GRACE-FO was launched in 2018, as a joint partnership between NASA and the German Research Centre for Geosciences (GFZ) and has continued the essential climate data record of mass change in the Earth system initiated in 2002 by the original GRACE mission (2002–2017).

Type

Earth Observation Satellite

Data Center

PO.DAAC

Launch

GRACE: March 17, 2002 GRACE-FO: May 22, 2018

Objective

Measure Earth's gravity

GRACE-FO successfully completed its five-year prime mission phase in May 2023, and is currently in its extended mission phase.

Together, the GRACE and GRACE-FO multi-decade data records provide foundational observations of monthly to decadal global mass changes and transports in the Earth system, derived from temporal variations in the Earth’s gravity field.

In parallel, a continuity mission called GRACE-Continuity (GRACE-C), scheduled for launch in 2028, is being developed in partnership between NASA (US) and DLR (Germany). While its design heavily leverages heritage elements, one notable departure is that the primary ranging instrument on GRACE-C will be a higher-precision laser interferometer, capitalizing on the successful demonstration of this technology on GRACE-FO.

All GRACE missions consist of two identical satellites that act in unison as a single primary instrument. The two satellites comprising each mission orbit one behind the other in the same orbital plane, maintaining an approximate distance of 220 km (137 miles).

As the pair circles the Earth, areas of varying gravity cause the distance between the two satellites to fluctuate ever so slightly. This variation is continuously measured by precise onboard intersatellite ranging instruments (GRACE: Microwave; GRACE-FO: Microwave and Laser; GRACE-C: Laser). The distance variations are measured with an accuracy of a few micrometers (Microwave), or even nanometers (Laser). Additional instruments measure satellite attitude, non-gravitational forces, and precise orbital position. These observations are then processed on the ground to map Earth’s month-to-month gravity and mass changes.

Remote video URL

The above animation was creating using the Jet Propulsion Laboratory (JPL) Tellus Mascon Release 06.1 v03 product derived from GRACE/GRACE-FO, covering April 2002 to Sept. 2022. Credit: PO.DAAC

A general rule of thumb for choosing which data set to use: most non-expert users interested in hydrology, ice mass, and ocean bottom pressure mass change should look at the MASCON gridded data products (e.g. 10.5067/TEMSC-3MJ634 and 10.5067/TEMSC-3JC634) and the globally averaged Level 4 time series products (10.5067/TEMSC-AT634, 10.5067/TEMSC-GT634, and 10.5067/TEMSC-OT634). These products combine the records from GRACE and GRACE-FO into a longer time series and are added to monthly. 

Advanced users wanting gridded fields based on the traditional spherical harmonic basis functions, or users looking at gravity field analysis, sensitivity studies, and solid Earth processes should consult the Level 2 spherical harmonic gravity field products and Level 3 Tellus products. Note there are different solutions provided from each of the three GRACE project partners.

All GRACE missions are collaborations between NASA and German agencies. For GRACE, NASA partnered with the German Space Agency (DLR). For GRACE-FO, NASA partnered with the German Research Centre for Geosciences (GFZ)

For GRACE-Continuity, NASA is again partnering with the German Space Agency (DLR). For all GRACE missions, key partners are the University of Texas Center for Space Research (CSR), the German Research Centre for Geosciences  (GFZ), and the Jet Propulsion Laboratory (JPL).

 

Instruments Aboard GRACE/GRACE-FO

Instrument Name Operational Date(s) Spectral Resolution Type of Instrument
GRACE Interferometer March 17, 2002 - present Spectrometer/Radiometer
GRACE-FO Laser Ranging Interferometer (GRACE-FO LRI) 2018 - present Positioning/Navigation

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