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Multispectral Scanner System (MSS)

The Multispectral Scanner System (MSS) was the first digital remote sensing instrument, revolutionizing Earth observation from space.

An artist rendering of the Multispectral Scanner System. The painting shows the golden components of the MSS, with a chunk out of the middle showing the innerworkings of this scanner.

Overview

The Multispectral Scanner System (MSS) was a line scanning sensor carried on the first five Landsat satellites. It sensed sunlight reflected off the Earth’s surface in four spectral bands: two in the visible and two in the near-infrared portions of the spectrum. Landsat 3 carried an MSS with an additional band that measured thermal-infrared radiation (heat) emitted from the Earth’s surface.

The primary function of the MSS was to provide repetitive daylight observations of the Earth's surface on a global basis to support various disciplines such as agriculture, forestry, geology, and hydrology. After launch, data from the MSS was proven useful for additional applications: mapping sea-ice fields, locating and tracking major ocean currents, monitoring both air and water pollution, determining snow cover, investigating severe storm environments, and more.

The MSS revolutionized Earth observations by introducing digital imaging technology that enabled pixel-level measurements to study land dynamics from space. This groundbreaking sensor served as the foundation for modern digital imaging technologies, including today's digital cameras and high-definition televisions.

The MSS engineering model on the back of a truck with a man standing on the ground to the right.
The Landsat 1 MSS engineering model on the back of its road trip transport truck in May 1972. A Hughes technician stands to the right wearing a maroon shirt and grey jacket. He holds a control box in his right hand.
Hughes / NASA

Requirements

  • return images in four spectral bands: the green, red and two near-infrared bands
  • cover a continuous video strip corresponding to the RBV coverage with a swath width of 185 km (115 miles)
  • imaging swath width of 100 nautical miles
  • ability to resolve details of 80 meters across 
  • no gaps in sampling from the edge of one orbit to the next at the equator
  • acquisition of full Earth surface coverage in less than a month

The mission's coverage needs determined the spacecraft's orbital parameters—an altitude of 917 kilometers and an inclination of 99.2 degrees—which created an 18-day repeat pattern. 

Rigorous radiometric and geometric calibration were required to ensure consistency between subsequent scenes collected over the same location. This requirement was essential for analyzing change over time.

A black and white line drawing showing the MSS Scanner arrangement and its orbit direction and swath above the earth.
Enlarged view of MSS scanning geometry and image projection. The MSS collected data by continually scanning the ground directly beneath the observatory. The width of the strip was 185 kilometers, identical to the coverage of the Return Beam Vidicon (RBV) Camera.
NASA

Design

The Multispectral Scanner System (MSS) sensors were line scanning devices observing the Earth perpendicular to the orbital track. The cross-track scanning was accomplished by an oscillating mirror; six lines were scanned simultaneously in each of the four spectral bands for each mirror sweep. The forward motion of the satellite provided the along-track scan line progression.

The MSS consisted of a 22.86-centimeter double reflector-type telescope, scanning mirror, filters, detectors, and associated electronics. Incoming radiation was collected by the scanning mirror and separated into four spectral bands using optical filters and sensed by an array of detectors. The detectors for bands 4 through 6 used photomultiplier tubes, while band 7 detectors used silicon photodiodes.

Diagram of the four-band MSS, the photomultiplier tubes and silicon photodiodes are tucked in the rear of the sensor.
Diagram of the four-band MSS sensor.
NASA

MSS Enhancements on Landsat 3

Following the recommendation of the National Research Council, Landsat engineers added a thermal band on Landsat 3 and future missions. Landsat 3’s thermal-infrared band was sensitive to temperatures from 260–340 K (-13º–67º C) and represented a major leap forward. It was used for measuring land surface temperature, better monitoring agriculture, detecting fires, and studying urban heat islands.

Data Handling

The MSS used a multiplexer to process the scanner's 24 channels of data. These data were then transmitted (at 2229.5 MHz) directly to an acquisition station or stored on magnetic tape for subsequent playback the next time the spacecraft came within communication range of a ground station.

The NASA Data Processing Facility, at NASA Goddard Space Flight Center (GSFC) converted image data from the magnetic tape to photographic prints and color transparencies. The facility also duplicated and distributed data tapes in addition to transmitting image data to the U.S. Geological Survey’s EROS Data Center.

Landsat 3’s first image features a slice of Northern California on March 7, 1978.   San Jose sits in Santa Clara Valley touching the southernmost portion of San Francisco. The area is shaken by earthquakes once or twice annually as just east of the city lays the Calaveras Fault. The focused imagery showcases the urbanization of the valley, which exploded in the 1970s as Silicon Valley grew.
Landsat 3’s first image features a slice of Northern California on March 7, 1978.
USGS
Landsat 3 data being converted to film transparencies.
NASA
A diagram showing the data flow process of Landsat 1 MSS data.
Downlinked data were recorded on wide band video tapes (WBVT). The bulk data processor performed digital-to-analog conversion of the MSS data. This process also used the ephemeris and telemetry data to create radiometrically and geometrically corrected MSS images. The final image cropped to a scene size, annotated, and written to 70-mm archival film.
L. Rocchio

Spectral Bands

Landsat 1-2
Band
Landsat 3
Band
Landsat 4-5
Band*
Band width (µm)GSD (m)
4 - Green4 - Green1 - Green0.5-0.680
5 - Red5 - Red2 - Red0.6-0.780
6 - Near-infrared (NIR)6 - Near-infrared (NIR)3 - Near-infrared (NIR)0.7-0.880
7 - Near-infrared (NIR)6 - Near-infrared (NIR)4 - Near-infrared (NIR)0.8-1.180
N/A8 - Thermal-infrared (TIR)N/A10.4-12.6240
*Bands 4-7 were renamed for Landsat 4-5 MSS.
A diagram showing all spectral bands from Landsat 1-9, separated by instrument.
The Multispectral Scanner System (MSS) aboard Landsats 1–5 had four bands. The Thematic Mapper (TM) aboard Landsats 4 & 5 had seven bands. Landsat 7’s Enhanced Thematic Mapper Plus (ETM+) has 8 bands and Landsats 8 & 9 have 11 bands. The atmospheric transmission values for this graphic were calculated using MODTRAN for a summertime mid-latitude hazy atmosphere (circa 5 km visibility).  *Bands 4-7 were renamed for Landsat 4-5 MSS.
NASA