Getting There
Getting to Mars: Windows, Delta-v, Transit
The standard trajectory is a Hohmann transfer: an ellipse touching Earth's orbit at departure and Mars' at arrival, which is the minimum-energy route between two circular orbits. It takes roughly six to nine months depending on the specific alignment, and it is the reason every mission profile is quoted in years rather than weeks.
The 25.6-month cadence is the synodic period, and it propagates through everything. Cargo must land a full window ahead of crew so that propellant can be manufactured before anyone commits to the trip. A surface stay is either short — about a month, catching an immediate return — or long, roughly 500 days, waiting for the next efficient departure. There is no middle option.
Faster transfers are possible and expensive. Higher-energy trajectories cut months off the crossing at the cost of substantially more propellant on both ends, and nuclear thermal or electric propulsion could shorten it further. Every month removed from the cruise is a month of radiation dose and consumables saved, which is why fast transit keeps attracting attention despite the propellant penalty.
The cruise itself is the most hazardous phase. Radiation dose in transit runs around 1.8 mSv per day — roughly nine times the Martian surface rate — because there is no planet blocking half the sky. Six to nine months each way accounts for the bulk of a mission's total exposure, and it is spent in microgravity, deconditioning the crew before the hardest part of the mission begins.
The case for
It has been done many times
Dozens of spacecraft have made the crossing since the 1960s. The trajectory design, navigation and entry problems are solved for robotic mass.
The windows are perfectly predictable
The 25.6-month cadence is celestial mechanics. Every launch opportunity for the next century is already known to the day, which makes long-horizon planning possible.
Mars has an atmosphere to brake against
Aerocapture and aerobraking remove a large share of the arrival delta-v for free — an advantage the Moon does not offer.
Leaving again is cheap
Escape velocity from Mars is 5.0 km/s against Earth's 11.2, which is what makes locally manufactured propellant sufficient for the return.
The case against
The schedule is not negotiable
Miss a window and the next is 25.6 months away. There is no emergency return, no abort-to-Earth after landing, and no resupply on demand.
Transit is the highest-dose phase
About 1.8 mSv per day in cruise, roughly nine times the surface rate, for six to nine months in each direction — the majority of the mission's radiation exposure.
The crew arrives deconditioned
Months of microgravity precede the most physically demanding phase of the mission, and there is no recovery period on arrival.
Fast transfers cost propellant on both ends
Shortening the crossing means more energy at departure and more to shed on arrival, which cascades through the entire vehicle mass budget.
| Departure cadence | Every 25.6 months | Synodic period |
| Cruise | 6–9 months each way | Hohmann-class transfer |
| Cargo lead | One full window | ISRU runs before crew commits |
| Surface stay | ~30 or ~500 days | No intermediate option |
How long does it take to get to Mars?
Six to nine months on a standard minimum-energy transfer, depending on the specific alignment. Higher-energy trajectories can shorten it at a substantial propellant cost.
Why can you only launch to Mars every two years?
Earth and Mars return to the same relative geometry every 25.6 months — the synodic period. An efficient transfer can only depart in the weeks around that alignment, so opportunities come roughly every 26 months.
Why do Mars missions stay for 500 days?
Because departure is governed by the same alignment cycle. Either the crew leaves almost immediately on a short-stay profile, or they wait roughly 500 days for the next efficient return window. There is no option in between.