*This post may contain affiliate links. This means we may make a commission if you purchase an item using one of our links*
A celestial body is considered to be tidally locked when it rotates around an object at the exact same pace that it orbits that body. Essentially, the length of a day and a year is the same for a tidally locked planet, because it takes the same amount of time to fully rotate on its axis as it does to orbit around the sun.
Mars is not tidally locked as it’s quite rare for planets to be as such. It’s a phenomenon that usually is relevant to moons. It is often more likely for moons to become tidally locked to a planet than for the opposite to occur, though it is not impossible.
Why Isn’t Mars Tidally Locked?
Well, simply put, there is no object that Mars orbits that it is tidally locked to. First of all, Mars only orbits around one body, that being the Sun.
Mars does not orbit its moons, its moons orbit Mars. That means that only the moons can be tidally locked to Mars, not vice versa.
What this means is that there are moons that are tidally locked to Mars, such as Deimos and Phobos, but Mars is not tidally locked to the moons, because Mars does not orbit the moons, the moons orbit Mars.
Will Mars Tidally Lock to its Moons and When?
As stated previously, Mars’ moons are tidally locked to it already. Those moons are Phobos and Deimos, which are the only two moons that Mars has. So in truth, this question is moot: the moons of Mars are already tidally locked to the planet. They make one full rotation in the time it takes to orbit Mars.
This means the same side of Phobos and Deimos are facing Mars all the time. It is possible for the moons to break their tidal lock with Mars at some point, but such a thing would take an extremely long time.
As for when the moons became tidally locked to Mars, there’s no way to know.
Could Mars Tidally Lock to the Earth
Keep in mind the definition of “tidally locked.” A celestial object can only be tidally locked to an object that they are orbiting (because by definition, they have to rotate at the same speed that they orbit another body). As you may know, Mars does not orbit the Earth.
Therefore, Mars cannot be tidally locked to the Earth. The only celestial body that Mars orbits is the Sun, so Mars could only be tidally locked to the Sun. However, it is not tidally locked to that either.
What Would Happen if Mars Became Tidally Locked to the Sun?
Over time, it is possible for Mars to become tidally locked to the Sun. But what would happen if Mars did become tidally locked to the Sun at some point? Well, some things would change, but the changes wouldn’t be as significant as you may think.
Naturally, being tidally locked to the Sun would mean that only one side of Mars would face the sun all the time. This wouldn’t actually change as much as you think.
Naturally, the side of the planet facing the Sun would have to put up with a lot more solar radiation, but unlike Earth, there isn’t much that would be damaged on the surface of Mars.
There’s no vegetation or animals to die, no water to be evaporated, or anything like that.
Truthfully, the biggest change would simply be the temperature on that side of the planet, since it would never get to face the relatively cooler side of the depths of space. But there wouldn’t be much harm in this.
Even the side permanently facing the Sun would still have “seasons,” so to speak, since that is determined by the tilt of the planet, not by the speed of its rotation or orbit.
It’s worth noting that Mars is relatively far from the Sun, meaning the effects of tidal locking on it would be partially mitigated.
When a celestial body is tidally locked, it rotates on its axis at the same pace that it orbits the body it is tidally locked to. That means the length of a day and the length of a year for that tidally locked planet are the same.
By the definition of what being tidally locked means, Mars can only theoretically be tidally locked to the Sun, which is the only celestial body that Mars orbits. That said, Mars does orbit the Sun, but it does not orbit it at the same rate that Mars itself rotates, meaning it is not tidally locked to the Sun.
On the other hand, Mars does have two moons, Deimos and Phobos. Those moons are tidally locked to Mars, meaning the same face of both moons is facing Mars all the time.
Most tidally locked celestial bodies tend to be moons, though this is not impossible for planets either, Mars is just not one of those planets.
If Mars were to become tidally locked with the Sun, it wouldn’t actually change too much about Mars as a whole, since it has very little on the surface to be affected by never-ending solar radiation. The temperature on that side of the planet would likely increase, but other effects would be minimal.
The distance from the Sun obviously helps.
Ultimately, Mars could become tidally locked to the Sun one day, but it is unlikely to be anytime soon.