Approxiverse

Space

Why is it hard to fly above the solar system?

The planets orbit the Sun in roughly the same plane. Sending a spacecraft steeply out of that plane takes a large change in motion, because it starts with Earth’s orbital speed.

Earth travels around the Sun at about 30 kilometres per second. A spacecraft leaving Earth carries that motion with it. Firing an engine adds to its existing velocity, so the resulting path depends on both the strength and direction of the burn.

Changing the orbital plane

Here, “up” means perpendicular to the plane of Earth’s orbit. A burn directly away from the Sun stays within that plane: it changes the shape of the orbit without tilting it.

A perpendicular burn adds motion above or below the plane. The spacecraft still has its original motion around the Sun, so the two combine to produce a tilted path.

Adding about 5 kilometres per second gives a tilt of roughly 10°. Reaching 45° this way requires adding about 30 kilometres per second, matching the spacecraft’s original orbital speed.

For comparison, adding about 12.5 kilometres per second in the direction Earth is already travelling is enough to escape the Sun’s gravity in this simplified model. A large tilt can therefore require more propulsion than an escape trajectory.

How much propellant does that take?

The propellant requirement grows rapidly with the change in velocity. Carrying more propellant also makes the spacecraft heavier, so some of it is spent accelerating the remaining supply.

The chart below compares chemical and ion propulsion. Notice how quickly the propellant requirement rises as the tilt increases.

Solving…
Propellant per tonne of spacecraft against tilt, on a logarithmic scale.

Ion engines use much less propellant for the same change in velocity, but deliver a small thrust over long periods. The chart compares propellant requirements; it does not show how long each manoeuvre would take.

Explore the orbit

Choose a burn direction and strength to see the resulting path. Compare a burn away from the Sun, one along Earth’s motion, and one perpendicular to the orbital plane.

Real missions can also use a planet’s gravity to redirect their motion. Ulysses flew past Jupiter to enter an orbit that carried it over the Sun’s poles.

This model includes only the Sun’s gravity, so it does not simulate those planetary encounters. It also starts after escape from Earth; the displayed speed changes exclude the launch itself.