Lesson plan · University · Ages 18 and over · 45 minutes
Getting to Mars: Hohmann transfers and launch windows
The minimum-energy transfer from Earth to Mars: its semi-major axis, its 259-day flight, the 2.9 and 2.6 km/s burns at each end, the 44-degree lead Mars needs at launch, and how the real, eccentric orbits move the window.
The lesson
The class designs a Hohmann transfer to Mars from the vis-viva equation and Kepler's third law: the transfer orbit, the flight time, the two burns and the phase angle at launch. In the viewer at true scale they find when Mars stands 44 degrees ahead of Earth in the 2026 to 2027 cycle, compare it with the mean-motion prediction, and look at where Earth and Mars really were when Curiosity and Perseverance left.
What they take away
In the circular, coplanar model a Hohmann transfer to Mars has a = 1.262 au, takes 259 days, needs 2.95 km/s at Earth and 2.65 km/s at Mars, and starts with Mars 44.3 degrees ahead, a geometry that recurs every synodic period. The real orbits are eccentric, so the window shifts, and real missions are flown on trajectories worked out from where the planets actually are.
Step by step
The caption is what the class reads on screen; the talking points are in your notes drawer (N) when you present. Steps marked Pupils only appear only in the pupil lesson.
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01
Half an ellipse
Presented and for pupilsCaption
The cheapest route from Earth's orbit to Mars's is half an ellipse that touches both: a Hohmann transfer. On 4 December 2026 Mars is 44 degrees ahead of Earth, the angle this model needs at launch.
Talking points
- NASA's Basics of Space Flight (JPL): to reach Mars using the least propellant possible, the spacecraft's solar orbit is adjusted so that its perihelion is at the distance of Earth's orbit and its aphelion at the distance of Mars's. This is a Hohmann transfer orbit. The burn is tangential, in the direction of Earth's motion round the Sun, and the spacecraft then coasts.
- The model here takes both orbits as circles in one plane at NASA's semi-major axes, 149.598 million km for Earth and 227.956 million km for Mars. Mars's real orbit has an eccentricity of 0.0935 and is inclined 1.848 degrees to the ecliptic (NASA Mars Fact Sheet).
- JPL Horizons: Mars is 44.3 degrees ahead of Earth in heliocentric longitude on 4 December 2026 at about 01:23 UT. The viewer's ephemeris (JPL's approximate elements) puts the same moment at 01:16 UT.
- This view is at true scale, from above the ecliptic. Both planets go round anticlockwise, so "ahead" is anticlockwise of Earth.
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02
The transfer orbit and its flight time
Presented and for pupilsCaption
The transfer ellipse has its perihelion at Earth's orbit and its aphelion at Mars's, so a = (r_E + r_M)/2. The flight is half its period.
Talking points
- a_t = (149.598 + 227.956)/2 = 188.777 million km = 1.2619 au.
- The flight from perihelion to aphelion is half an orbit: T = π√(a_t³/GM☉). With JPL's GM☉ = 1.32712440041 × 10²⁰ m³ s⁻² that is 2.2367 × 10⁷ s, 258.9 days.
- The same from Kepler's third law in years and au: T = ½ × 1.2619^1.5 = 0.7088 years = 258.9 days.
Ask the class
With r_E = 149.598 million km, r_M = 227.956 million km and GM☉ = 1.32712 × 10²⁰ m³ s⁻², how many days does the Hohmann transfer to Mars take?
Answer259 days. Answers from 257 to 261 are marked right.
Whya_t = (1.49598 + 2.27956) × 10¹¹ m / 2 = 1.88777 × 10¹¹ m. a_t³ = 6.7274 × 10³³ m³; divided by GM, 5.0691 × 10¹³ s²; the square root is 7.1198 × 10⁶ s, and the half period π × 7.1198 × 10⁶ = 2.2367 × 10⁷ s = 258.9 days. A whole period would be 518 days, but the spacecraft only goes half way round.
Sources 1 2 3 4Present from this step
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03
The burn at Earth
Presented and for pupilsCaption
At Earth's distance the transfer orbit is faster than Earth. The difference is the heliocentric speed the spacecraft must add on leaving: about 2.9 km/s.
Talking points
- Earth's circular speed: v_E = √(GM☉/r_E) = 29.78 km/s, NASA's mean orbital velocity for Earth.
- Vis-viva at the transfer's perihelion: v_p = √(GM☉(2/r_E − 1/a_t)) = 32.73 km/s. So Δv₁ = 32.73 − 29.78 = 2.95 km/s. This is the spacecraft's speed relative to Earth once it has climbed out of Earth's gravity, v∞, and the launch energy is C₃ = v∞² = 8.67 km² s⁻².
- From a circular parking orbit 200 km up (r = 6378.137 + 200 km, with JPL's GM of Earth, 398,600.4 km³ s⁻²), the circular speed is 7.784 km/s and the escape speed 11.009 km/s, and the burn that leaves Earth at v∞ is √(v∞² + v_esc²) − v_circ = 11.396 − 7.784 = 3.61 km/s.
- This view is at true scale, 40 Earth radii above Earth's north side.
Ask the class
In the circular model, what heliocentric change in speed (km/s) puts a spacecraft moving with Earth onto the Hohmann transfer to Mars? Use a_t = 188.777 million km.
Answer2.95 km/s. Answers from 2.9 to 3 are marked right.
Whyv_E = √(1.32712 × 10²⁰ / 1.49598 × 10¹¹) = 29.785 km/s. v_p = √(1.32712 × 10²⁰ × (2/1.49598 × 10¹¹ − 1/1.88777 × 10¹¹)) = √(1.32712 × 10²⁰ × 8.0719 × 10⁻¹²) = 32.730 km/s. Δv₁ = 32.730 − 29.785 = 2.945, about 2.95 km/s.
Sources 1 2 4Present from this step
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04
The burn at Mars
Presented and for pupilsCaption
At aphelion the transfer orbit is slower than Mars, so the spacecraft must speed up by about 2.6 km/s to match it. Here it is 259 days after the December departure.
Talking points
- Vis-viva at the transfer's aphelion: v_a = √(GM☉(2/r_M − 1/a_t)) = 21.48 km/s. Mars's circular speed √(GM☉/r_M) = 24.13 km/s, so Δv₂ = 2.65 km/s, and the two burns total 5.59 km/s.
- NASA lists Mars's mean orbital velocity as 24.08 km/s: the average over its eccentric orbit, a little under √(GM/a), as the vis-viva lesson shows for Mercury. Either gives Δv₂ of 2.60 to 2.65 km/s.
- In practice the spacecraft arrives at v∞ = 2.65 km/s relative to Mars and must then slow down relative to Mars to be captured: Basics of Space Flight describes an orbit insertion burn, or aerodynamic braking, a parachute and retro-rockets to land.
- This scene opens on 20 August 2027, 258.9 days after 4 December 2026. With the real, eccentric orbits, Horizons has Mars 162 degrees round the Sun from where Earth was at departure, short of the 180 degrees of the circular model: near aphelion and slow, Mars moves 117.8 degrees in that time against the model's 135.7, at 1.54 to 1.67 au from the Sun against the 1.524 au mean.
Ask the class
In the same model, how much speed (km/s) must the spacecraft gain at the transfer's aphelion to match Mars's circular orbit?
Answer2.65 km/s. Answers from 2.59 to 2.71 are marked right.
Whyv_a = √(1.32712 × 10²⁰ × (2/2.27956 × 10¹¹ − 1/1.88777 × 10¹¹)) = √(1.32712 × 10²⁰ × 3.4764 × 10⁻¹²) = 21.479 km/s. Mars's circular speed √(1.32712 × 10²⁰ / 2.27956 × 10¹¹) = 24.128 km/s. Δv₂ = 24.128 − 21.479 = 2.649, about 2.65 km/s.
Sources 1 3 4 5Present from this step
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05
Leading the target
Presented and for pupilsCaption
The spacecraft goes 180 degrees round the Sun in 259 days, and Mars must be there when it arrives. So at launch Mars has to be ahead of Earth by 180 degrees less the angle Mars moves in 259 days.
Talking points
- Basics of Space Flight compares this with throwing a dart at a moving target: you have to lead the aim point by just the right amount.
- Mars moves 360 × 258.9/686.980 = 135.7 degrees during the transfer, so it must lead Earth by 180 − 135.7 = 44.3 degrees at launch.
- Earth moves 360 × 258.9/365.256 = 255.2 degrees in the same time, so on arrival Earth is 75.2 degrees ahead of Mars. A Hohmann return needs Earth 75.2 degrees behind Mars; Earth gains on Mars at 0.98561 − 0.52404 = 0.46158 degrees a day, so the crew waits (360 − 2 × 75.2)/0.46158 = 454 days at Mars.
- Earth gains 360 degrees on Mars every 360/0.46158 = 779.9 days, NASA's synodic period, so the same launch geometry comes round every 779.94 days. Basics of Space Flight: the opportunity for a minimum-energy transfer to Mars occurs about every 25 months.
Ask the class
By how many degrees must Mars lead Earth at launch for a Hohmann transfer of 258.9 days? Mars's sidereal period is 686.980 days.
Answer44.3 degrees. Answers from 42.8 to 45.8 are marked right.
WhyMars moves 360 × 258.9/686.980 = 135.7 degrees while the spacecraft goes 180 degrees, so Mars must start 180 − 135.7 = 44.3 degrees ahead. Using 365.256 days instead (Earth's motion) answers a different question.
Sources 1 2 3Present from this step
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06
Predict the window
Presented and for pupilsCaption
Mars is at opposition on 19 February 2027, lined up with Earth. Before that it was ahead of Earth, and Earth gained on it. With the mean rates, when was it 44.3 degrees ahead?
Talking points
- JPL Horizons: opposition on 19 February 2027 at 15:50 UT, when the lead is zero.
- Mean rates from NASA's sidereal periods: Earth 360/365.256 = 0.98561 degrees a day, Mars 360/686.980 = 0.52404, so Earth gains 0.46158 degrees a day.
Ask the class
With the mean angular speeds, how many days before the opposition of 19 February 2027 is Mars 44.3 degrees ahead of Earth?
Answer96 days. Answers from 93 to 99 are marked right.
WhyThe lead shrinks at 0.98561 − 0.52404 = 0.46158 degrees a day and reaches zero at opposition, so 44.3 degrees comes 44.3/0.46158 = 96 days before it: about 15 November 2026. The next step tests that against the real orbits.
Sources 2 3 5Present from this step
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07
Find it in the viewer
Pupils onlyCaption
Your turn. The clock starts on 15 October 2026 at a day a second, with Mars about 71 degrees ahead. Pause it when Mars is 44 degrees ahead of Earth, seen from the Sun.
Talking points
- JPL Horizons: Mars is 44.3 degrees ahead on 4 December 2026 at about 01:23 UT, 77.6 days before the opposition, and 70.9 degrees ahead at the start (the viewer's ephemeris).
- The check reads the date through the Sun's longitude of date: it passes within 6 degrees of 251.9 degrees, its value on 4 December, about six days either side (the Sun moves 1.01 degrees a day then), when the lead is between about 41 and 48 degrees. A pause inside it is 72 to 84 days before the opposition.
Pupil question
How many days before the opposition of 19 February 2027 did you pause?
Answer78 days. Answers from 70 to 86 are marked right.
WhyHorizons puts the 44.3 degree lead on 4 December 2026, 77.6 days before the opposition. The mean rates put it 96 days before, so the real date is about 18 days later than predicted.
Pupil task
Run the clock and watch Earth close on Mars. Pause it when the angle at the Sun between Earth and Mars is 44 degrees, Mars ahead.
Hint44 degrees is just under an eighth of a turn. The mean rates put it in mid-November; watch whether the real orbits agree.
The viewer checks the task as the pupil works and says when it is done.
Sources 5 6Open this step as a pupil
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08
Why the real window is later
Presented and for pupilsCaption
In this cycle Mars is near aphelion, its slowest, and Earth passes perihelion, its fastest, so Earth closes the last 44 degrees in 78 days, against 96 at the mean rates.
Talking points
- JPL Horizons: Mars reaches aphelion, 249.2 million km from the Sun, around 5 March 2027 (NASA's aphelion distance: 249.261 million km). USNO: Earth is at perihelion on 3 January 2027 at 02:33 UTC.
- Horizons' daily rates: on 4 December 2026 Earth moves 1.015 degrees a day and Mars 0.458; on 3 January 2027, 1.019 and 0.446; on 19 February, 1.008 and 0.437. Earth gains 0.56 to 0.57 degrees a day, against the mean 0.462: Kepler's second law at work on both planets.
- Mars is also farther out than the model assumes: 1.626 au on 4 December 2026 against the 1.524 au mean. A transfer whose aphelion is at the mean distance would not even reach it. Real trajectories are worked out from where the planets actually are on the launch and arrival dates.
- The clock runs at a day a second from the 44.3 degree moment.
Ask the class
The mean rates put the 44.3 degree lead 96 days before opposition, the real orbits 78 days. Why?
- Mars is near aphelion and Earth near perihelion, so Earth gains on Mars faster than the mean rateRight answer
- Mars's orbit is inclined 1.85 degrees to the ecliptic
- Earth's day is getting longer
WhyNear aphelion Mars moves at about 0.44 degrees a day, under its mean of 0.524, and near perihelion Earth moves at about 1.02, over its mean of 0.986. Earth gains about 0.57 degrees a day, so the last 44.3 degrees take about 78 days.
Sources 3 5 7Present from this step
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09
Curiosity and Perseverance
Presented and for pupilsCaption
Curiosity launched on 26 November 2011, with Mars 56 degrees ahead, and landed 254 days later. Perseverance launched on 30 July 2020, with Mars 26 degrees ahead, and landed after 203 days.
Talking points
- NASA: Curiosity launched on 26 November 2011 and landed on 6 August 2012; Perseverance launched on 30 July 2020 and landed on 18 February 2021. By the calendar those flights took 254 and 203 days.
- JPL Horizons, heliocentric longitudes at 12:00 UTC on each date: for Curiosity Earth was at 64 and Mars at 120 degrees at launch, a lead of 56 degrees, and Mars at 236 degrees on landing day, so the spacecraft went 172 degrees round the Sun. For Perseverance Earth was at 308 and Mars at 334 degrees, a lead of 26 degrees, and Mars at 90 degrees on landing day: 143 degrees round.
- Basics of Space Flight: a trajectory that carries the spacecraft less than 180 degrees round the Sun is Type I, 180 degrees or more Type II. Both rovers flew Type I trajectories, neither of them the 180-degree, 259-day textbook transfer.
- The scene opens at 12:00 UTC on Curiosity's launch date, when the viewer's ephemeris and Horizons both give a lead of 56.4 degrees.
Ask the class
Curiosity went about 172 degrees round the Sun from launch to landing. In Basics of Space Flight's terms, what kind of trajectory was that?
- Type IRight answer
- Type II
- An exact Hohmann transfer
WhyLess than 180 degrees round the Sun is Type I. A Hohmann transfer goes exactly 180 degrees, and Type II is 180 degrees or more.
Sources 1 5 8 9Present from this step
Sources
Every fact in this lesson comes from these sources, and each step lists the ones it uses.
- Basics of Space Flight, chapter 4: Trajectories, NASA Science (JPL)
- Earth Fact Sheet, NASA NSSDCA
- Mars Fact Sheet, NASA NSSDCA
- Astrodynamic Parameters, JPL Solar System Dynamics
- Horizons System (DE441 ephemeris), JPL Solar System Dynamics
- Approximate Positions of the Planets, JPL Solar System Dynamics
- Earth's Seasons and Apsides, 2027, US Naval Observatory
- Mars Science Laboratory: Curiosity Rover, NASA Science
- Mars 2020: Perseverance Rover, NASA Science
