ESA’s Earth Cloud Aerosol and Radiation Explorer (EarthCARE) mission is the most complex of all of ESA’s trailblazing Earth Explorer missions – missions that deliver critical information to understand how our world functions and the impact that human activity is having on natural processes.

Equipped with four state-of-the-art instruments, EarthCARE will make a range of different measurements that together will shed new light on the role that clouds and aerosols play in regulating Earth’s delicate temperature balance.

EarthCARE has been developed as a cooperation between ESA and the Japan Aerospace Exploration Agency (JAXA).

Satellite characteristics

Launch Date - End 1716933600 - 1893366000

Status Operational

Orbit type Sun-synchronous orbit

Altitude 393

Orbit inclination 97.05

Equatorial crossing time 10:30:00

Orbit period 92

Satellite family: Earth Explorers

The biggest environmental issue we face is global change, which encompasses not only climate change but also the large-scale impact that a growing global population and continued economic growth are having on the environment.

Earth Explorers provide an important contribution to the global endeavour to further our understanding of Earth. Earth Explorer missions form the science and research element of ESA's Living Planet Programme and focus on the atmosphere, biosphere, hydrosphere, cryosphere and Earth's interior.

However, the emphasis is also on learning more about the interactions between these components and the impact that human activity is having on natural Earth processes.

Earth Explorer missions are divided into two categories: 'core' and 'opportunity'.

Core missions respond directly to specific areas of public concern and are selected through widespread consultation with the science community. Opportunity missions are smaller, low-cost satellites that are relatively quick to implement to address areas of immediate environmental concern.

The user-driven approach is fundamental for both type of mission. The process of mission selection has given the Earth science community an efficient tool for advancing the understanding of the Earth system. The science questions addressed also form the basis for development of new applications of Earth observation.

To date, there have been four core missions and four opportunity missions selected for implementation.

Core missions

  • GOCE: the Gravity field and steady-state Ocean Circulation Explorer was launched on 17 March 2009 and ended on 11 November 2013. GOCE provided high spatial resolution gravity-gradient data to improve global and regional models of Earth's gravity field and geoid.
  • Aeolus: the prime aim of the Atmospheric Dynamics Mission is to demonstrate measurements of vertical wind profiles from space. The mission employs a high-performance Doppler wind lidar based on direct-detection interferometric techniques. ADM-Aeolus was launched on 22 August 2018.
  • EarthCARE: Earth Clouds Aerosols and Radiation Explorer will improve the representation and understanding of Earth's radiative balance in climate and numerical forecast models. 
  • Biomass: The Biomass mission will provide crucial information about the state of our forests and how they are changing. Carrying the first P-band synthetic aperture radar in space, Biomass will provide measurements to determine the amount of biomass and carbon stored in forests, thereby improving our understanding of the carbon cycle. 

Opportunity missions

  • SMOS: the Soil Moisture and Ocean Salinity mission, launched on 2 November 2009, is exploiting an innovative two-dimensional interferometer to acquire brightness temperature observations at L-band (1.4 GHz). These observations translate into information on the moisture held in soil and salinity in the surface layers of the oceans, which are needed to further our understanding of Earth's water cycle.
  • CryoSat: CryoSat, launched on 8 April 2010, is measuring fluctuations in the thickness of ice on both land and sea determine how Earth's ice is changing. This information is leading to a better understanding of the relationship between ice and global climate. CryoSat carries an innovative SAR/interferometric radar altimeter.
  • Swarm: Swarm, launched on 22 November 2013, is providing the best-ever survey of the geomagnetic field and its temporal evolution. The geomagnetic models resulting from the mission will provide new insights into Earth’s interior. This information will lead to a better understanding of atmospheric processes, and also have practical applications in areas such as space weather and radiation hazards.
  • FLEX: the Fluorescence Explorer will map vegetation fluorescence to quantify photosynthetic activity. This information will improve our understanding of the way carbon moves between plants and the atmosphere and how photosynthesis affects the carbon and water cycles. It will also lead to better insight into plant health and stress.

Sensor characteristics

Sensor name ATLID (ATmospheric LIDar)
Sensor short description
Sensor type Lidar
Resolution class Medium (30 - 300 m)
Sensor name CPR (Cloud Profiling Radar) Earthcare
Sensor short description
Sensor type Cloud profile and rain radar
Resolution class Low (300 m - 1 km)
Revisit frequency 25 days
Sensor name MSI (Multispectral Imager) Earthcare
Sensor short description
Sensor type Imaging radiometer (Vis/IR)
Resolution class Low (300 m - 1 km)
Swath width (at nadir) 150 km
Revisit frequency 25 days
Sensor name Broadband Radiometer
Sensor short description

The broadband radiometer plays a crucial role in the mission by measuring the radiative fluxes at the top of Earth's atmosphere. As the satellite travels along its orbit, the radiometer views the atmosphere from three directions, allowing it to accurately quantify the amount of reflected solar radiation and the outgoing thermal radiation emitted by Earth.

This is known as the planet's energy balance. Comparing this to the radiation calculated from the combined observations of the other instruments helps scientists to improve our understanding of the aerosol-cloud-radiation interaction.