Calculator

๐Ÿ›ฐ๏ธ Hohmann Transfer Calculator

You can't point a rocket at Mars and fire. Mars won't be there when you arrive. Spacecraft ride a carefully timed half-ellipse around the Sun, and the timing is set by the planets, not by you.

It's like a quarterback leading a receiver: you throw to where Mars will be. The trip takes a fixed 259 days, so Mars has to start about 44ยฐ ahead of Earth. That lineup only happens once every 26 months, and that's what sets the launch date.

๐Ÿงญ Plan a Transfer

Earth Mars Spacecraft
Travel time
Total delta-v
Fuel mass ratio
Launch alignment
Windows repeat every
the synodic period: how long the two planets take to return to the same alignment
Arrival speed vs. target
Upcoming launch windows
    BurnDelta-vWhat it does

    Model: circular, coplanar planetary orbits and short (impulsive) burns. That's the textbook Hohmann transfer. Real missions use the planets' actual elliptical, slightly tilted orbits, so real launch windows can shift by a few weeks and real delta-v budgets run a bit higher. Getting off the ground and into the parking orbit (about 9.4 km/s from Earth's surface) is not included. Pluto's orbit is far more stretched and tilted (17ยฐ) than the planets', so treat its numbers as rough. The Moon option is worked out around Earth, starting from low Earth orbit.

    ๐Ÿฅš What a Hohmann Transfer Actually Is

    In 1925, German engineer Walter Hohmann worked out the cheapest way to move between two circular orbits: fire your engine once to stretch your orbit into an ellipse that just touches the destination orbit, coast halfway around, then fire again to round the orbit out. The transfer ellipse is tangent to both orbits, so neither burn wastes any effort pushing sideways.

    The catch is that the travel time is fixed by the orbit's size, not by how hard you push. Earth to Mars on a Hohmann transfer always takes about 259 days. You can get there faster by spending more fuel on a steeper path, but you can't get there cheaper.

    โณ Why You Have to Wait for the Planets

    Because the coast takes months, you have to aim where the destination will be when you arrive, not where it is when you leave. For a Hohmann transfer to Mars, the spacecraft sweeps 180ยฐ around the Sun. In those 259 days, Mars moves about 136ยฐ along its own orbit. So at launch, Mars needs to be about 44ยฐ ahead of Earth. Launch any other day, and you get to Mars's orbit while Mars is somewhere else.

    Earth and Mars only line up that way once every 26 months. Miss the window and you wait over two years for the next one, which is why every Mars mission of a given era (rovers, orbiters, landers from several countries) tends to launch within the same few weeks.

    The same logic applies coming home. After a 259-day trip out, the planets are in the wrong places for the return trip, so a crew has to stay at Mars for about 15 months waiting for the return window. Round trip: roughly 2.7 years. The calculator above works out the wait for any pair of planets.

    ๐Ÿงญ Directions in Space: No North, South, East, or West

    North, south, east, and west only mean something because you're standing on a spinning ball with a magnetic field. In orbit there's no ground to point at. Pilots and mission planners use directions defined by your own motion instead, relative to whatever you're orbiting (the Sun, for an interplanetary trip).

    Sun Prograde Retrograde Radial out Radial in Normal (toward you) Anti-normal (away)
    • Prograde: the direction you're already moving. Burning this way raises the opposite side of your orbit.
    • Retrograde: straight backward against your motion. Burning this way lowers the opposite side of your orbit.
    • Radial out / radial in: directly away from, or toward, the body you're orbiting. Pushing this way mostly rotates your orbit rather than growing it.
    • Normal / anti-normal: perpendicular to the plane of your orbit, "up" or "down" out of the page. These tilt your orbit to a new plane, and they're expensive.

    Those six directions are all a spacecraft ever needs, and they lead to some of the least intuitive rules in physics:

    Even "up" is just a convention. For the solar system, astronomers call the plane of Earth's orbit the ecliptic, and by agreement "north" of it is the side from which the planets appear to circle counterclockwise. Nothing out there marks it; it's a choice of which way to hold the map.

    ๐ŸŒ Where Earth's compass directions do sneak in: rockets launch toward the east because Earth spins that way, giving a free boost of up to 0.46 km/s at the equator. Once in orbit, that "east" becomes prograde, and the compass stops mattering.
    ๐Ÿช Hohmann transfers to the outer planets are brutally slow: about 2.7 years to Jupiter, over 30 years to Neptune, and 45 years to Pluto. That's why real missions cheat with gravity assists, stealing a little of a planet's orbital speed on a close flyby. Voyager 2 reached Neptune in 12 years by bouncing off Jupiter, Saturn, and Uranus along the way.