Talking to Mars: the maths
Earth and Mars on circular orbits around the Sun; radio travels at light speed. Computed live.
Equations
- d(t) = |rM(t) − rE(t)|
- Distance between the planets, each moving round its circle (periods 365.256 and 686.98 days).
- delay = d / c
- One-way light time. A question and its answer take twice that.
Constants
| AU | 1.495978707 × 10¹¹ m | exact, by definition |
| Mars's orbit | 1.5237 AU | mean radius |
| c | 299,792,458 m/s | exact |
Worked examples ✓ checked on every change
| One-way delay at closest approach | 4.36 min | (1.5237 − 1) AU ÷ c |
| One-way delay at farthest | 20.99 min | (1.5237 + 1) AU ÷ c |
What's simplified
- Circular orbits: Mars's real orbit is noticeably elliptical, so real delays range from about 3 to 22 minutes.
- Near conjunction the Sun's glare disrupts the signal; the model shows the geometry only.
Where it breaks
It doesn't — for the geometry. Only the orbits' shapes are simplified.
Sources: NASA/JPL planetary fact sheets; IAU (2012) definition of the astronomical unit.