The Carbon Mapper emissions monitoring system

<p>The Carbon Mapper emissions monitoring system contributes to the broader ecosystem of greenhouse gas observations by locating and quantifying CH<span class="inline-formula">₄</span> and CO<span class="inline-formula">₂</span> super emitters at facility scale across priority regions globally and making the data accessible and actionable. The system includes observing platforms, an operational monitoring strategy optimized for mitigation impact, and a data platform that delivers CH<span class="inline-formula">₄</span> and CO<span class="inline-formula">₂</span> data products for diverse stakeholders. Operational scale-up of the system is centered around a new constellation of hyperspectral satellites. The Carbon Mapper Coalition (hereafter Tanager) satellites are each equipped with an imaging spectrometer instrument designed by NASA's Jet Propulsion Laboratory that are assembled, launched and operated by Planet Labs. The first Tanager satellite (Tanager-1) was launched 16 August 2024 completed commissioning in January 2025 and continued to improve observational efficiency through summer 2025. Planet is currently working to expand the constellation to four Tanagers. Each imaging spectrometer instrument has a spectral range of about 400–2500 nm, 5 nm spectral sampling, a nadir spatial resolution of 30 m, and nadir swath width of about 19 km at the lowest orbital altitude. Each satellite is capable of imaging 250 000 km<span class="inline-formula">²</span> per day on average. By combining the results of independent controlled release testing with empirical evaluation of the radiometric, spectral, spatial, and retrieval noise performance of the Tanager-1 spectrometer, we predict minimum detection limits of about 64–126 kgCH<span class="inline-formula">₄</span> h<span class="inline-formula">⁻¹</span> for CH<span class="inline-formula">₄</span> point sources and about 10 078–18 994 kgCO<span class="inline-formula">₂</span> h<span class="inline-formula">⁻¹</span> for CO<span class="inline-formula">₂</span> point sources for images with 25 % albedo, 45° solar zenith angle, and 3 m s<span class="inline-formula">⁻¹</span> wind speed. A review of the first 11 months of Tanager-1 CH<span class="inline-formula">₄</span> and CO<span class="inline-formula">₂</span> observations including initial validation with coordinated aircraft under-flights and non-blind controlled release testing indicates that the system is meeting performance requirements and, in many cases, surpassing expectations. We also present early evaluations in challenging onshore and offshore observational conditions and summarize the first use of Tanager data to guide the timely mitigation of a CH<span class="inline-formula">₄</span> super emitter.</p>