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GTO (Geostationary Transfer Orbit)

Also known as: Geostationary Transfer Orbit

📘 Definition
A Geostationary Transfer Orbit (GTO) is a highly elliptical orbit used to carry a satellite from launch towards geostationary orbit (GEO). Its perigee (lowest point) sits near 200–300 km, close to low Earth orbit, while its apogee (highest point) reaches GEO altitude at 35,786 km. A rocket injects the payload into GTO near perigee, after which the satellite coasts roughly five hours out to apogee. There it fires its own engine to raise the perigee and circularise at GEO. GTO is a practical application of the Hohmann transfer: the launcher provides the first burn into the ellipse and the satellite the second at apogee, splitting the work between them. The launch vehicle supplies roughly 2.4 km/s of delta-v from LEO into GTO, and the satellite adds about 1.5 km/s to reach its final orbit.
200–300 km
Perigee
35,786 km
Apogee
~10.5 hours
Orbital period
~1.5 km/s
Delta-v (GTO→GEO)
Equatorial launch; ~1.8 km/s from Cape Canaveral
Surface 9.4 km/s LEO 2.5 km/s GTO 1.5 km/s GEO 3.2 km/s to Moon transfer Lunar orbit

Understanding GTO

How a satellite climbs from GTO to GEO

Once the launch vehicle releases the payload into GTO, the satellite coasts out to apogee at 35,786 km. There it fires its own engine to raise the perigee and circularise the orbit — the burn traditionally delivered by a dedicated apogee kick motor. Because the orbit becomes truly circular only after the apogee burn (and any inclination correction) is complete, operators usually spread the work over several passes. Chemical propulsion can reach GEO within days, but many modern platforms now use electric propulsion for this orbit raising. Ion thrusters take weeks or months to spiral up, yet their high efficiency slashes propellant mass and frees weight for more payload.

Why launch-site latitude drives the fuel bill

A satellite launched due east inherits an orbital inclination equal to its launch site's latitude, so the transfer orbit is tilted relative to the equator. Reaching true GEO means removing that tilt, and the cheapest place to do it is at apogee, where the satellite travels slowest. Launch sites near the equator are therefore prized: from Europe's spaceport at Kourou (about 5°N) the combined circularisation-and-plane-change burn is roughly 1.5 km/s, whereas from Cape Canaveral (28.5°N) it rises to about 1.8 km/s. That difference directly reduces the mass a rocket can send to GEO.

Standard, subsynchronous and supersynchronous GTO

Not every GTO targets exactly GEO altitude. Launch providers tune the apogee to balance the work between the rocket and the satellite, giving three broad variants:

GTO typeApogeeTrade-off
Standard≈35,786 km (GEO)Balanced share of delta-v between launcher and satellite
SubsynchronousBelow GEORocket does less; the satellite must supply more delta-v
SupersynchronousAbove GEOHigher, slower apogee makes the plane change cheaper; the apogee is later lowered back to GEO
🛰️ Watch satellites raise their orbits
Newly launched satellites climb out of GTO by firing at apogee to reach GEO. Our tracker flags these orbit-raising manoeuvres in near real time.
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Frequently Asked Questions

GTO is the elliptical transfer path, while GEO is the circular destination orbit. A geostationary orbit (GEO) is a circular orbit at 35,786 km where a satellite matches Earth's rotation and appears fixed in the sky. GTO is the stepping-stone used to get there: an elongated ellipse whose high point just touches GEO altitude. A satellite occupies GTO only briefly before circularising into GEO.
Splitting the journey through GTO lets a smaller, cheaper rocket loft a heavier satellite. Reaching GEO directly would force the launch vehicle to carry all the propellant for both the climb and the circularisation, cutting deep into payload mass. Instead the rocket does the efficient part — the fast perigee burn — and hands the final delta-v to the satellite's own engine, which can be optimised for that single task.
It ranges from a few days to several months, depending on the propulsion. A satellite with a chemical apogee engine can circularise over a handful of apogee passes and reach GEO within days. One relying on efficient but low-thrust electric propulsion spirals up gradually and may take three to six months, trading time for a large saving in propellant mass.
About 1.5 km/s from an equatorial launch, rising to roughly 1.8 km/s from a mid-latitude site like Cape Canaveral. The extra cost comes from correcting the orbital inclination inherited from the launch latitude, which is folded into the apogee burn. For comparison, the launch vehicle supplies around 2.4 km/s to lift the payload from LEO into GTO in the first place.
An apogee kick motor is the engine that fires at GTO's high point to circularise the orbit at GEO. Historically it was a dedicated solid rocket or bipropellant system built into the satellite, fired in one or more burns at apogee. Many modern satellites instead use their main station-keeping propulsion for the job, blurring the line between the transfer burn and routine operations.
Essentially yes — a GTO is a Hohmann transfer orbit between low Earth orbit and geostationary orbit. A Hohmann transfer is the two-burn, minimum-energy ellipse that connects two circular orbits: one burn to enter the ellipse, one to leave it. GTO applies exactly that geometry to the LEO-to-GEO climb, with the added twist of an inclination change usually merged into the second burn.

Sources & References

Definitions are reviewed against primary sources. Last reviewed: 2026-08-25.