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Thematic Mapper (TM)

The Thematic Mapper (TM), carried by Landsats 4 and 5, represented a significant advancement in Earth observation technology. The TM enabled the first-ever natural-color images of the Landsat program, allowing us to observe Earth as we see it.

A diagram of the Thematic Mapper Scanner Schematic detailing all of its components.

Overview

The Thematic Mapper (TM) was an advanced, multispectral scanning, Earth observation sensor designed to achieve higher image resolution, sharper spectral separation, improved geometric fidelity, and greater radiometric accuracy and resolution than the Multispectral Scanner System (MSS) sensor. The Thematic Mapper was so named because of its ability to help scientists create maps tailored to different Earth science disciplines, or “themes.” It was designed to meet the growing needs of university researchers, private industry, government agencies, and international data users. 

TM data are sensed in seven spectral bands, adding more spectral coverage than previous Landsat instruments. Band 1 (visible blue light) enabled the first ever natural-color Landsat images. Band 6 (thermal-infrared energy) sensed heat emitted from the Earth’s surface and provided the first nighttime observations. These new bands unlocked applications including water quality analysis and surface temperature monitoring.

Landsat 4 Thematic Mapper instrument wrapped in gold thermal blankets with a technician in clean room gear working on top.
Landsat 4 Thematic Mapper in clean room.
NASA

These improvements provided distinct advantages for vegetation analysis and land cover mapping applications. The narrower spectral band data in the visible and near-infrared portions of the spectrum, improving the ability to differentiate between conventional crops of wheat, barley, corn, and soybeans. Geological and petroleum exploration scientists benefited from these narrower spectral bands by testing more advanced surveying and exploration procedures and improved geological maps. 

Clean room technician working on Landsat 4 Thematic Mapper instrument covered in gold thermal blankets with visible circular aperture and white panels on red platform.
Clean room technician working on Landsat 4’s Thematic Mapper (TM) instrument.
NASA

Requirements

The TM instrument had to “satisfy requirements for data continuity desired by users, including government agencies, research institutions, and resource enterprises,” according to Landsat’s Enduring Legacy (Goward et al., 2017). The requirements mentioned in the Landsat D Press Kit included:

  • extend the 10 year data set of observations provided by the multispectral scanner 
  • increased spatial resolution for visible, near infrared, and shortwave infrared bands to 30-40m
  • new narrower spectral bands based on results agricultural monitoring experiments (e.g., LACIE, AgRISTARS)  
  • thermal infrared band at 120-m spatial resolution
  • improved radiometric resolution of 0.5% or better reflectance; 0.5°C thermal infrared (TIR) resolution
  • radiance digitized to 8-bits
A video of Landsat 4's Thematic Mapper in a cleanroom.
NASA

Design

The Thematic Mapper (TM) was a seven-band, earth-observing, scanning radiometer. The instrument consisted of primary imaging optics, a scanning mechanism, spectral band discrimination optics, detector arrays, radiative cooler, inflight calibrator, and required operating and processing electronics. 

The TM collected, filtered, and detected radiation in a swath that was 185 km (115 miles) wide. The scanning mechanism provided the cross-track scan while the progress of the spacecraft provided the scan along the track. A TM scene has an Instantaneous Field Of View (IFOV) of 30m x 30m in bands 1-5 and 7 while band 6 has an IFOV of 120m x 120m on the ground.

The instrument works by capturing incoming solar energy (visible and thermal-infrared light) through the Sun-shaded aperture. Filters were used to separate light into spectral bands before reaching the detectors. The visible and near-infrared bands (1, 2, 3, and 4) used four linear arrays of 16 silicon photo diode detectors and the mid-infrared bands (5 and 7) used indium-antimonide photo diode detectors. The thermal infrared band (6) used four mercury-cadium-telluride detectors.

Field team celebrating during Landsat 5 TM mountain expedition with mobile ground station equipment visible in background.
Field team celebrating during Landsat 5 TM mountain expedition with mobile ground station equipment visible in background.
Hughes/NASA

Data collected from the sensor’s detectors were processed in the TM multiplexer for transmission via the Tracking And Data Relay Satellite System (TDRSS) or directly downlinked to ground stations within range. Archival data were made available through the U.S. Geological Survey’s EROS Data Center.

Technical cutaway diagram of the Landsat-D Thematic Mapper instrument showing its internal components and optical system. The illustration displays labeled parts including the scan mirror assembly, secondary mirror, primary mirror, electronics module, thermal louvers, power supply multiplexer, prime focal plane, cooled focal plane, radiative cooler, relay optics assembly, and inchworm mechanism. The diagram shows the complex optical path and mechanical systems within the instrument housing.
Detailed cross-sectional view of the Thematic Mapper instrument used on Landsat-D, illustrating the optical and electronic systems that enable high-resolution multispectral Earth imaging.
NASA

Spectral Bands

The Thematic Mapper's 30-meter spatial resolution (vs. MSS 60-meter) provides approximately seven times more information per scene. The instrument's spectral advancements allow more accurate crop differentiation (e.g., wheat from barley, corn from soybeans) that was previously challenging with MSS technology.

BandWavelength (µm)GSD (m)
1 - Blue0.45-0.5230
2 - Green0.52-0.6030
3 - Red0.63-0.6930
4 - Near-infrared (NIR)0.76-0.9030
5 - Shortwave-infrared (SWIR) 11.55-1.7530
6 - Thermal-infrared (TIR)10.41-12.5120
7 - Shortwave-infrared (SWIR) 22.08-2.3530
The Thematic Mapper provides multi-spectral observations in seven bands including three heritage bands and four new bands. The instrument featured significantly narrower bands in the green (0.52-0.6 microns versus 0.5-0.6 microns), red (0.63-0.69 microns versus 0.6-0.7 microns), and near-infrared (0.76-0.9 microns versus 0.7-1.1 microns) regions compared to the Multispectral Scanner (MSS).
NASA/Ross Walter