The Gravity Field and Steady-State Ocean Circulation Explorer (GOCE) was the first of ESA's Living Planet Programme heavy satellites intended to map in unprecedented detail the Earth's gravity field. The spacecraft's primary instrumentation was a highly sensitive gravity gradiometer consisting of three pairs of accelerometers which measured gravitational gradients along three orthogonal axes.

Launched on 17 March 2009, GOCE mapped the deep structure of the Earth's mantle and probed hazardous volcanic regions. It brought new insight into ocean behaviour; this in particular, was a major driver for the mission. By combining the gravity data with information about sea surface height gathered by other satellite altimeters, scientists were able to track the direction and speed of geostrophic ocean currents. The low orbit and high accuracy of the system greatly improved the known accuracy and spatial resolution of the geoid (the theoretical surface of equal gravitational potential on the Earth).

Gravity Field and Steady-State Ocean Circulation Explorer

The satellite's unique arrow shape and fins helped keep GOCE stable as it flew through the thermosphere at a comparatively low altitude of . Additionally, an ion propulsion system continuously compensated for the variable deceleration due to air drag without the vibration of a conventional chemically powered rocket engine, thus limiting the errors in gravity gradient measurements caused by non-gravitational forces and restoring the path of the craft as closely as possible to a purely inertial trajectory.

Gravity Field and Steady-State Ocean Circulation Explorer

After running out of propellant, the satellite began dropping out of orbit and made an uncontrolled re-entry on 11 November 2013.

Gravity Field and Steady-State Ocean Circulation Explorer

Discoveries and applications

Mission objectives

To determine gravity-field anomalies with an accuracy of (1 mGal). To increase resolution, the satellite flew in an unusually low orbit. To determine the geoid with an accuracy of 1–2 cm. To achieve the above at a spatial resolution better than 100 km.

Gravity map and model

The final gravity map and model of the geoid will provide users worldwide with well-defined data product that will lead to: A better understanding of the physics of the Earth's interior to gain new insights into the geodynamics associated with the lithosphere, mantle composition and rheology, uplift and subduction processes. A better understanding of the ocean currents and heat transport. A global height-reference system, which can serve as a reference surface for the study of topographic processes and sea-level change. Better estimates of the thickness of polar ice-sheets and their movement.

Findings

The first Earth global gravity model based on GOCE data was presented at ESA's Living Planet Symposium, in June 2010.

Initial results of the GOCE satellite mission were presented at the American Geophysical Union (AGU) 2010 Fall (Autumn) Meeting by Dr Rory Bingham from Newcastle University, UK. The maps produced from the GOCE data show ocean currents in much finer detail than had been available previously. Even very small details like the Mann Eddy in the North Atlantic were visible in the data, as was the effect of Hurricane Igor in 2010. Detailed analysis of GOCE's thruster and accelerometer data serendipitously revealed that it had detected the infrasound waves generated by the 2011 Tōhoku earthquake (whereupon it inadvertently became the first seismograph in orbit).

Later results from the GOCE data exposed details in the Earth's mantle including mantle plumes, ancient subduction zones, and remnants of the Tethys Ocean.

Subsequent analysis of GOCE data has also provided new information about the geological makeup of the Antarctic continent, including the detection of ancient continent remnants and at least three cratons beneath the Antarctic ice.

Operations

Launch

The first launch attempt on 16 March 2009 was aborted due to a malfunction with the launch tower.