Earth ObservationLEOTracked live

TERRA

Terra launched in 1999 as the flagship of NASA's Earth Observing System. Instead of treating the atmosphere, oceans, land, ice and energy budget as isolated subjects, Terra carries five instruments that observe related parts of the Earth system during the same orbital passes. Its long record has supported research on clouds, aerosols, vegetation, fires, pollution, surface temperature, radiation and environmental change. Terra greatly exceeded its original design life, turning a single spacecraft into a multidecade scientific record.

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Object identity

NORAD ID
25994
COSPAR ID
1999-068A
Operator
Not listed
Country
Not listed
Launch date
Not listed

Immediate discovery

Why this satellite matters

Terra carries ASTER, CERES, MISR, MODIS and MOPITT. Together they measure surface features and temperature, Earth's radiation budget, clouds and aerosols from multiple viewing angles, broad spectral imagery, and carbon monoxide in the lower atmosphere.

Understanding the mission

Science and engineering ideas

Terra carries ASTER, CERES, MISR, MODIS and MOPITT. Together they measure surface features and temperature, Earth's radiation budget, clouds and aerosols from multiple viewing angles, broad spectral imagery, and carbon monoxide in the lower atmosphere.

NASA's reference orbit for Terra was approximately 705 km (438 mi) above Earth with a 99-minute period, about 14 orbits per day and a 98.5-degree inclination. Terra's orbit has changed as the mission aged, so live catalog values can differ from those original reference numbers.

A Sun-synchronous orbit was designed to cross locations at nearly the same local solar time, helping scientists compare observations under similar lighting. Terra began drifting away from its original crossing time after maneuvers maintaining that geometry ended.

Repeated measurements are essential to Earth science. A single image records one moment, while a calibrated series collected across years can reveal seasonal cycles, unusual events and persistent change.

Mission

Mission and purpose

These spacecraft use cameras, radiometers, radar, spectrometers, or other instruments to measure features of Earth. Repeated observations make comparisons across seasons and years possible.

  • Terra carries ASTER, CERES, MISR, MODIS and MOPITT. Together they measure surface features and temperature, Earth's radiation budget, clouds and aerosols from multiple viewing angles, broad spectral imagery, and carbon monoxide in the lower atmosphere.
  • NASA's reference orbit for Terra was approximately 705 km (438 mi) above Earth with a 99-minute period, about 14 orbits per day and a 98.5-degree inclination. Terra's orbit has changed as the mission aged, so live catalog values can differ from those original reference numbers.
  • A Sun-synchronous orbit was designed to cross locations at nearly the same local solar time, helping scientists compare observations under similar lighting. Terra began drifting away from its original crossing time after maneuvers maintaining that geometry ended.
  • Repeated measurements are essential to Earth science. A single image records one moment, while a calibrated series collected across years can reveal seasonal cycles, unusual events and persistent change.

Design

Engineering

Terra carries ASTER, CERES, MISR, MODIS and MOPITT. Together they measure surface features and temperature, Earth's radiation budget, clouds and aerosols from multiple viewing angles, broad spectral imagery, and carbon monoxide in the lower atmosphere. NASA's reference orbit for Terra was approximately 705 km (438 mi) above Earth with a 99-minute period, about 14 orbits per day and a 98.5-degree inclination. Terra's orbit has changed as the mission aged, so live catalog values can differ from those original reference numbers. A Sun-synchronous orbit was designed to cross locations at nearly the same local solar time, helping scientists compare observations under similar lighting. Terra began drifting away from its original crossing time after maneuvers maintaining that geometry ended. Repeated measurements are essential to Earth science. A single image records one moment, while a calibrated series collected across years can reveal seasonal cycles, unusual events and persistent change.

Real orbital values

The mathematics

The current two-line element set reports approximately 14.6116 revolutions per day. Dividing 1,440 minutes by that value gives an estimated orbital period of 98.6 minutes.

Period

98.6 min

Representative speed

27,036 km/h

Representative altitude

697 km

Inclination

97.94°

These are representative calculations derived from current orbital elements, not fixed physical specifications. Altitude and speed change around an elliptical orbit, and predictions change as new orbital elements are published.

Launch record

Launch and deployment

Terra, originally called EOS AM-1, launched on 18 December 1999 aboard an Atlas IIAS from Vandenberg Air Force Base in California. The spacecraft entered an initial orbit and was maneuvered toward its planned approximately 705-km (438-mi) Sun-synchronous polar orbit. Its five instruments were then activated and checked before routine science observations began.

TransitSatellite does not estimate historical launch weather. Temperature, clouds, wind, holds, and scrub reasons will appear only when supported by traceable historical sources.

Orbit

LEO orbit explained

Low Earth orbit is the region closest to Earth used by most crewed spacecraft, many science missions, Earth-observation satellites, and large constellations. Objects move quickly and commonly complete an orbit in roughly 90 to 130 minutes.

LEO can provide detailed Earth views, lower communications delay, and easier access than higher orbits, but it covers less area per spacecraft and is more affected by atmospheric drag.

Live TransitSatellite experience

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Open the live tracker to view its current calculated position, trajectory, orbital information, visibility tools, and Save and Share controls.

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Learning

Questions to explore

  • Why are repeated observations valuable?
  • How can satellites observe through clouds or darkness?

Evidence

Sources and data notes

Current identity and orbital elements come from CelesTrak’s public GP data. Calculated orbit values are derived from the current TLE and may change after catalog updates. Mission-history claims are added separately and require authoritative sources.

Catalog updated

Sep 19, 2026, 11:25 PM UTC

Story review

2026-08-30