I can't find information on which side of mars do probes usually enter.

I suppose that probes do not enter perpendicular to the surface. They are usually represented as entering somewhat tangentially to the surface, and in the same direction as Mars rotation (that would reduce relative speed).

But I do wonder how it is done in reality.


3 Answers 3


There is always a benefit to entering a planet's atmosphere with matching rotation.
In the case of Earth, the difference is a rather huge 920m/s effective airspeed between reentering prograde or retrograde.

With Mars the effect is smaller but still strong, at some 485m/s difference.

Even on the Moon it makes a difference, but so small as to be almost ignored. Merely 9m/s. For the Moon, orbital parameters and communication lines greatly outweigh direction of approach.

There is no law that says each probe must take benefit from this effect, and indeed for some probes heading to the polar regions the effect is completely not relevant. But as a rule of thumb, yes. A Mars lander will always enter its atmosphere prograde to planetary rotation.

  • $\begingroup$ I'm curious if there might be a reason to enter an atmosphere AGAINST the direction of rotation if 1) aerodynamic braking is desired, and 2) the atmosphere is really thin? Maybe in that case matching the rotation direction would not give enough braking? Thanks! $\endgroup$
    – James
    Commented Feb 16, 2021 at 18:02
  • $\begingroup$ @James I think that against the rotation gives more time to be in contact with the probe after the landing, because in favor of the rotation, the probe lands close to the point where Mars rotation hides the machine from Earth. $\endgroup$
    – Raxi Ral
    Commented Feb 16, 2021 at 19:56
  • 4
    $\begingroup$ @james Yes indeed, going counter to the rotation would give an effective higher airspeed, increasing drag. But while drag increases a bit, the heating goes through the roof! Hypersonic reenty heat scales a speed ^ 8 ! It is always better to go with rotation, and dive down to deeper air if you can. bit more heat, bit more drag. Going against the rotation gives bit more drag, and hugely more heat. $\endgroup$ Commented Feb 16, 2021 at 20:02

Space craft will tend to enter orbit counter clockwise as viewed from the northern hemisphere. This is due to the fact that most objects in the solar system orbit and rotate this way with the exceptions of Venus, Uranus and a few asteroids. Moving in the direction of rotation will therefore reduce the required velocity loss where as entering orbit clockwise would increase it.

This is not a definitive rule however, it is entirely possible to enter clockwise if the heat shield is able to withstand the additional velocity loss or even across the poles into a polar orbit with an intermediate velocity change if required and this has advantages from a survey perspective as the entire planet can be viewed from directly above at some point in the orbit.


See also answers to

Answers to What aspects of reentry heating 'scale as the 8th power'? including my unnecessarily downvoted answer there explain that radiative heating from the hot plasma to the spacecraft are an extremely strong function of relative velocity between the spacecraft and the atmosphere, which rotates with the rest of the planet.

A 10% difference in reentry speed could double the radiative heating load on a spacecraft entering Mars' atmosphere ($1.1^8=2.14$).

Mars' standard gravitational parameter $GM$ is 4.2828E+13 m^3/s^2 and a 111 km Mars orbit has a radius of 4000 km. The orbital speed is

$$v = \sqrt{GM/a} = 3272 \ \text{m/s}$$

and the atmosphere's rotational velocity at that altitude is about 241 m/s, so the ratio of radiative heating prograde versus retrograde would be

$$\left( \frac{3272 + 241}{3272 - 241} \right)^8 \approx 3.3$$

and that's a big difference!

Radiative heating is a huge problem and so ablative heat shields continuously vaporize, producing a layer of gas which is somewhat opaque to the thermal infrared light radiated by the plasma so that much of it never reaches the spacecraft, but nothing is 100% effective so you'd still like to keep heating to a minimum by entering the atmosphere at the lowest possible relative velocity.

Note that like the Space Shuttle, the SpaceX Starship planned to land on Mars will use ceramic tiles and not an ablative heat shield, so the outside surfaces of the tiles will be directly exposed to full radiative heating.

The tiles will (hopefully) have high reflectivity for thermal infrared, and low thermal conductivity so that the thermal loading on the ship's structure behind the tiles is low. It will also use aerodynamic fins to somewhat reduce its rate of descent so that it can dump more velocity before reaching denser parts of the atmosphere.

Still, with no ablative heat shield to block radiative heating, it will certainly benefit from the reduced relative velocity of entering with Mars' atmosphere's rotation rather than against it.

slide from Lecture #1: Stagnation Point Heating

Source: Lecture #1: Stagnation Point Heating

  • 1
    $\begingroup$ This is great information, and I appreciate it a lot, but I marked the other as answer, because it closer to answer what most probes actually do. I wish I could mark your own as the answer. $\endgroup$
    – Raxi Ral
    Commented Feb 17, 2021 at 14:47

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