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Advancing technology to support science-based action


  • Excessive methane (CH4) and carbon dioxide (CO2) emissions are harmful to our climate and health but invisible to the naked eye. Our science-based algorithms and remote sensing technology offer a unique solution for detecting, pinpointing, and quantifying high-emission methane and CO2 point sources around the globe.

    Making these emissions visible through advanced technology and accessible via our data portal helps put data in the hands of decision makers everywhere. Our science and technology contribute to an ecosystem of observing systems that work together to support mitigation action.

Image Credit: NASA/JPL-Caltech

Group of scientists working on a satellite

  • CO2: Important for long-term impacts

    While reducing methane emissions today can slow the rate of global warming, addressing CO2.  is essential for avoiding the worst impacts of climate change because it traps heat in the atmosphere for hundreds of years.

    Our capability to detect large point sources of CO2 from power plants and refineries and across liquefied natural gas (LNG) supply chains will help independently verify these emissions sources globally.


  • Monitoring emissions from space: A comprehensive approach

    Ultimately, our goal is to provide sustained monitoring of up to 90% of methane and CO2 super-emitters globally via a satellite constellation. It’s ambitious — but critical to slowing global climate change.

Image Credit: Planet Labs

Rendering of a Carbon Mapper coalition Tanager satellite

  • Initial observing regions

    The tasking deck showcases initial regions of global observations for the first two Carbon Mapper Coalition Tanager satellites. As the constellation grows, these efforts will continue to scale.

The tasking deck showcases initial priority regions of global observations for the first two Carbon Mapper coalition Tanager satellites

Imaging spectroscopy: Making invisible emissions visible


  • The satellites and aircraft used by Carbon Mapper each host an imaging spectrometer — a device like a camera, but where every pixel measures hundreds of wavelengths of light reflected by Earth’s surface and absorbed by gases in the planet’s atmosphere. These instruments can see from visible wavelengths into the infrared wavelengths beyond the range of human vision. The instruments gather high-quality data that we use to detect, image, pinpoint, and quantify methane and CO2 super-emitters.

    The instruments being deployed in space on Planet Labs’ Tanager satellites were developed through the Carbon Mapper Coalition. They represent 5th generation imaging spectrometer technology designed by NASA JPL, which builds on previous versions used in our airborne observations and our analysis of EMIT observations from the International Space Station. With the planned launch of the first Tanager satellite in 2024, the new spectrometer technology will begin to scale up global operational monitoring of super-emitters.

Image of imaging spectrometer — a device like a camera but where every pixel measures hundreds of wavelengths of light reflected by Earth’s surface and absorbed by gases in the planet’s atmosphere.

Leading on innovative science

Our science and research team is at the forefront of using remote sensing to detect, pinpoint, and quantify methane and CO2 emissions. Leveraging deep technical expertise and a long history of research, we work to enable science-based action through transparent and credible methods published in peer-reviewed literature.


Image of methane plume over a satellite view basemap

Courtesy Arizona State University Global Airborne Observatory

Arizona State University Global Airborne Observatory airplane on a tarmac