Landsat Lightpath Animations
For nearly half a century, the Landsat mission has shaped our understanding of Earth. Since the launch of the first Landsat satellite in 1972, the mission has gathered and archived more than 8 million images of our home planet’s terrain, including crop fields and sprawling cities, forests and shrinking glaciers. These data-rich images are free and publicly available, leading to scientific discoveries and informed resource management.
Landsat 9 will carry two instruments that largely replicate the instruments on Landsat 8: the Operational Land Imager 2 (OLI-2) and the Thermal Infrared Sensor 2 (TIRS-2). OLI-2 and TIRS-2 are optical sensors that detect 11 wavelengths of visible, near infrared, shortwave infrared, and thermal infrared light as it is reflected or emitted from the planet’s surface. Data from these instruments are processed and stored at the USGS Earth Resources Observation and Science (EROS) Center in Sioux Falls, South Dakota—where decades worth of data from all of the Landsat satellites are stored and made available for free to the public.
The Landsat mission, a partnership between NASA and the U.S. Geological Survey (USGS), has provided the longest continuous record of Earth’s land surfaces from space. The consistency of Landsat’s land-cover data from sensor to sensor and year to year makes it possible to trace land-cover changes from 1972 to the present, and it will continue into the future with Landsat 9. With better technology than ever before, Landsat 9 will enhance and extend the data record to the 50-year mark and beyond.
Data collection of the OLI-2 instrument aboard Landsat 9. OLI-2 will have a 98-foot (30-meter) spatial resolution across most of its spectral bands, meaning each pixel represents an area about the size of a baseball infield. Altogether, the sensors cover a swath 115 miles (185 kilometers) wide. This combination of a wide swath and moderate resolution allows OLI-2 to cover large areas, while still providing fine enough resolution to distinguish individual agricultural fields, forest plots or housing developments—important information for urban planners, land resource managers and commodity analysts.
Light from the sun reflects off Earth's surface and into OLI-2's telescope. In the example in this animation, OLI-2 is colecting data south of Fort Worth, Texas, on July 17, 2020.
Light reflected from Earth's surface shines into OLI-2, bouncing off of five mirrors before shining through a set of wavelength filters covering the focal plane. On the focal plane are thousands of detectors, aligned in rows. These detectors are sensitive to light reflecting off Earth’s surface in nine different wavelengths, including visible, near-infrared and short-wave-infrared light. With data from these bands, either alone or in combination, Earth’s surface is revealed.
Data collection of the TIRS-2 instrument aboard Landsat 9. Whether it’s a cornfield, a parking lot, or an iceberg, a surface emits thermal infrared radiation, or heat. By detecting radiation in two thermal wavelengths, Landsat 9’s TIRS-2 instrument can measure the temperature of our planet’s ground and water.
TIRS-2 works on the same principles as the original TIRS on Landsat 8, but corrects a problem the first instrument had with scattered light inside the telescope. And while TIRS has a three-year design life, TIRS-2 is built with increased robustness and redundancy to last at least five years. TIRS-2, like OLI-2, is a “push-broom” sensor with arrays of detectors that line up to observe a field of view that is 115 miles (185 kilometers) across, with a resolution of 328 feet (100 meters). In this example, TIRS-2 is collecting data south of Fort Worth, Texas, on July 17, 2020.
Lightpath animation of TIRS-2. TIRS-2 uses thermal bands to detect subtle shifts
in temperature—within a tenth of a degree Celsius. Its detectors are called Quantum Well Infrared Photodetectors, or QWIPs, and were developed at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. Thermal infrared radiation in a specific wavelength will excite electrons within the QWIPs, creating an electrical signal that is used to determine surface temperature.
Please give credit for this item to:
NASA's Goddard Space Flight Center Conceptual Image Lab