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📡 Tracking & Space Surveillance

TLE (Two-Line Element Set)

Also known as: Two-Line Element Set, Two-Line Element

📘 Definition
A TLE, or two-line element set, is a compact, fixed-width text format that encodes an Earth-orbiting object's entire orbit in just two 69-character lines. Each set captures six mean orbital elements — inclination, eccentricity, RAAN, argument of perigee, mean anomaly and mean motion (which fixes the orbit's size in place of the semi-major axis) — plus an atmospheric-drag term, all referenced to a single instant called the epoch. Devised by NORAD in the punch-card era of the 1960s and still in daily use, TLEs are the backbone of public satellite tracking. Crucially, they are never used on their own: each set is fed into the SGP4 propagator, which accounts for drag and Earth's equatorial bulge to predict where an object will be at any future moment. Orbital Radar propagates fresh TLEs through SGP4 to place every tracked object on the live globe.
2 (+ optional name)
Data lines
69 characters
Line width
SGP4 / SDP4
Propagator
29,132
Catalogued objects
with public TLEs
Line 0 — Name ISS (ZARYA) Line 1 — Identification & Epoch 25544 NORAD ID 25014.51253411 Epoch (YY+day.frac) Line 2 — Orbital Elements 51.6416 Incl ° 247.4627 RAAN ° 0001411 Ecc 15.54227985 Mean Motion (rev/day)

Understanding TLE

Anatomy of the two lines

Despite the name, a TLE usually spans three lines: an optional 'line 0' holding the object's name, followed by two 69-character data lines. Line 1 carries the object's identity and housekeeping information; line 2 carries the pure geometry of the orbit. Every character position is fixed, and each line ends in a modulo-10 checksum digit so software can detect corruption.

FieldLineWhat it describes
Catalogue number (NORAD ID)1 & 2Unique object identifier
Int'l designator (COSPAR ID)1Launch year, number and piece
Epoch1Reference time (year + fractional day)
BSTAR drag term1Models atmospheric drag on the orbit
Inclination2Tilt of the orbital plane (°)
RAAN2Swivel of the plane around Earth (°)
Eccentricity2Orbit shape (0 = circle); decimal implied
Argument of perigee2Orientation of the ellipse (°)
Mean anomaly2Position along the orbit at epoch (°)
Mean motion2Revolutions per day (sets the orbit size)

Why a TLE only works with SGP4

A common mistake is to plug TLE numbers into a textbook two-body orbit calculator. That fails, because TLE values are 'mean' elements deliberately fitted to work with the SGP4 model — they are averaged so that SGP4's own corrections for drag and Earth's oblateness reproduce the real orbit, and they are not the instantaneous (osculating) elements of classical mechanics. SGP4 handles near-Earth orbits with periods under 225 minutes; its sibling SDP4 takes over above that threshold, adding lunar and solar gravitational effects for deep-space orbits. Pair a TLE with the matching propagator and you get accurate position and velocity; use it any other way and the answer can drift by hundreds of kilometres.

How accurate is a TLE, and how long does it last?

A fresh TLE typically places an object within about a kilometre of its true position at the epoch, but that error grows as the prediction runs forward — very roughly one to three kilometres per day for a low-orbit satellite, and faster during periods of high solar activity that puff up the upper atmosphere and increase drag. For this reason TLEs carry a limited shelf life: operators refresh them every few days, and Orbital Radar re-fetches the latest sets from Space-Track so the globe never propagates a stale orbit too far past its epoch. The data is freely published by the US Space Force and mirrored by CelesTrak.

A 1960s format meets modern traffic

The TLE's fixed 69-character layout dates from the era of punch cards, and it is beginning to show its age. The satellite catalogue number is only five digits, capping the scheme at 99,999 objects — a ceiling the fast-growing catalogue is approaching. As a stopgap, the 'Alpha-5' convention lets the first character become a letter to stretch capacity, while the community increasingly favours the modern Orbit Mean-Elements Message (OMM), which carries the same SGP4-compatible data in JSON, XML or KVN without the rigid column limits. For now, though, the humble TLE remains the lingua franca of satellite tracking.

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Frequently Asked Questions

The name refers to the two lines of orbital data; the optional third line — technically 'line 0' — simply holds the satellite's name and is not part of the element set itself. A file that includes those name lines is sometimes called a 3LE or 'three-line' set. Both formats carry identical orbital information across the two 69-character data lines; only the human-readable label differs.
A fresh TLE is typically accurate to roughly one kilometre at its epoch, but that error grows the further you propagate it forward — often one to three kilometres per day in low orbit, and faster during solar storms that thicken the upper atmosphere. This is why TLEs are refreshed every few days, and why precise operations such as collision avoidance rely on higher-fidelity data instead.
No — a TLE only produces accurate results when run through the SGP4/SDP4 propagator it was designed for. Its elements are averaged 'mean' values, not the instantaneous ones used in textbook two-body physics, so a generic Keplerian calculator will give positions that are wrong by hundreds of kilometres. Established libraries such as python-sgp4 and Skyfield implement the correct model.
The authoritative source is Space-Track.org, run by the US Space Force, which requires a free account; CelesTrak.org offers a convenient public mirror with no login. Both publish the same underlying government data. Orbital Radar ingests these feeds automatically — see our data sources page for the full pipeline.
A 3LE is simply a TLE with an extra name line added on top. The 'three-line' format prepends a 'line 0' containing the object's common name, which makes files easier to read but adds no orbital information. The two data lines are byte-for-byte identical in both formats, so any SGP4 tool can read either one.
The epoch is the exact moment the orbital elements were measured, written as a two-digit year plus the fractional day of the year — so 24001.5 means midday on 1 January 2024. Every prediction is calculated relative to this timestamp, and accuracy is highest at the epoch, decaying on either side of it. Always check the epoch before trusting a propagated position.

Sources & References

Definitions are reviewed against primary sources. Last reviewed: 2026-08-04.