Planetary Launch Window Calculator

Find Hohmann transfer launch windows between any two solar system bodies.

Origin

Destination

Earth period
365 days
Mars period
687 days
Earth from Sun
1.00 AU
Mars from Sun
1.52 AU
Next Earth → Mars Window

Opens Nov 18, 2026 · Optimal Dec 3, 2026

Transfer Details

Next window — Hohmann transfer from Earth to Mars

Window opens
Nov 18, 2026
Optimal departure
Dec 3, 2026
Window closes
Dec 18, 2026
Estimated arrival
Aug 19, 2027
Transit time
~259 days (8.5 months)
Next window after this
~25 months
Estimated ΔV: 5.6 km/s Moderate
Upcoming Launch Windows

Next 10 Earth–Mars transfer opportunities

Optimal Departure Arrival Transit Difficulty
Dec 3, 2026 Next Aug 19, 2027 259 d Moderate
Jan 6, 2029 Sep 22, 2029 259 d Moderate
Feb 8, 2031 Oct 25, 2031 259 d Moderate
Mar 17, 2033 Dec 1, 2033 259 d Moderate
May 8, 2035 Jan 22, 2036 259 d Moderate
Jul 26, 2037 Apr 11, 2038 259 d Moderate
Oct 5, 2039 Jun 20, 2040 259 d Moderate
Nov 19, 2041 Aug 5, 2042 259 d Moderate
Dec 25, 2043 Sep 9, 2044 259 d Moderate
Jan 26, 2046 Oct 12, 2046 259 d Moderate
All Destinations from Earth

Comparison of transfer windows from Earth to each body

Body Next Window Transit Difficulty
Mercury Aug 12, 2026 105 d Hard
Venus Jul 27, 2026 146 d Moderate
Mars Dec 3, 2026 259 d Moderate
Ceres Feb 5, 2027 472 d Hard
Jupiter Oct 29, 2026 998 d Hard
Saturn Jun 12, 2026 2208 d Hard
Uranus Aug 4, 2026 5858 d Hard
Neptune Jun 1, 2027 11182 d Hard

Click a row to switch destination.

How It Works

A Hohmann transfer orbit is the most fuel-efficient two-burn path between two circular orbits. A spacecraft departs the origin body at the correct phase angle, coasts along a half-ellipse, and arrives at the destination. Transit times range from ~100 days (Earth–Venus) to over a decade (Earth–Neptune via Hohmann).

Launch windows only open when the destination is at the right position for the spacecraft to arrive on time. These opportunities recur at the synodic period of the two bodies — the time for them to return to the same relative configuration.

ΔV (delta-v) is the change in velocity required to complete the transfer. It determines how much propellant a mission needs. Easy missions (<5 km/s total) require relatively little fuel; hard missions (>8 km/s) — like Earth–Mercury — demand either very powerful rockets or gravity assists from intermediate bodies.

This calculator uses simplified Keplerian orbital elements (NASA/JPL J2000 model) with a fixed-phase-angle Hohmann approximation. Windows may differ from actual mission dates by several weeks for low-eccentricity bodies or up to 90 days for high-eccentricity bodies like Mercury. Real mission planning uses numerical integration and porkchop-plot C3 analysis.

Frequently Asked Questions

What is a planetary launch window?

A launch window is the period when a spacecraft can depart Earth and arrive at another planet using a Hohmann transfer orbit — the most fuel-efficient two-burn path. The window opens when the planets are at the correct phase angle so the spacecraft arrives at the destination orbit when the target planet is there.

How often do Mars launch windows occur?

Every ~26 months, which is Mars's synodic period (the time for Earth and Mars to return to the same relative positions). This is why Mars missions cluster every two years — NASA's Perseverance (2020), Curiosity (2011), and Opportunity (2003) each launched in different windows.

What is delta-v (ΔV)?

Delta-v is the change in velocity (in km/s) required to complete a maneuver. It determines fuel requirements — the rocket equation means exponential fuel growth with ΔV. Earth-to-Mars requires roughly 3.6–4.0 km/s departure + ~0.9 km/s arrival = ~4.5–5.0 km/s total for a Hohmann transfer.

What is a Hohmann transfer orbit?

An elliptical orbit that connects two circular orbits using exactly two engine burns — one to leave the first orbit, one to enter the second. It is the most fuel-efficient path between two orbits but is not the fastest. Faster transfers (like those used for crewed missions) require more ΔV.