Will Uranus Ever Be Tidal-Locked to the Sun?

In summary: If it ever appears "locked" I'd have to wonder about the coincidence of it. The a^6 term - distance raised to the ^6 of its orbital semi-major axis [a rather large number] is offset only by Radius of it's mass in the denominator, raised to the ^5 - that is such a prodigious number to overcome that time to lock surely won't happen in the remaining Solar lifetime.
  • #1
pixel01
688
1
Will ever Uranus be tidal-locked by the Sun?
 
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  • #2
This offers a good overview:
http://en.wikipedia.org/wiki/Tidal_locking

The formula they show for Time to tidal locking in the case of Uranus would look to be dominated by the a^6 term describing its orbital semi-major axis.

And this does not take into account the tidal locking of the other objects that are tidal locked to Uranus.

I'd say the sun expiry would intervene long before there would be a tidal locking of Uranus to the sun.
 
  • #3
LowlyPion said:
This offers a good overview:
http://en.wikipedia.org/wiki/Tidal_locking

The formula they show for Time to tidal locking in the case of Uranus would look to be dominated by the a^6 term describing its orbital semi-major axis.

And this does not take into account the tidal locking of the other objects that are tidal locked to Uranus.

I'd say the sun expiry would intervene long before there would be a tidal locking of Uranus to the sun.

I did not mention the great distance of Uranus from the Sun, but its eccentric rotation axis. Uranus rotation axis nearly lies on its orbiting plane. So I am not sure whether one day Uranus is locked to the Sun just like Earth-Moon system or it is just free of that.
 
  • #4
pixel01 said:
Uranus rotation axis nearly lies on its orbiting plane. So I am not sure whether one day Uranus is locked to the Sun just like Earth-Moon system or it is just free of that.

If it ever appears "locked" I'd have to wonder about the coincidence of it. The a^6 term - distance raised to the ^6 of its orbital semi-major axis [a rather large number] is offset only by Radius of it's mass in the denominator, raised to the ^5 - that is such a prodigious number to overcome that time to lock surely won't happen in the remaining Solar lifetime.

As I mentioned as an additional perturbating factor, Uranus has several moons (that happen as it turns out to be tidally locked to it) and I would have to think that any anomalies on Uranus would be subjected to greater forces from them than would be exerted by the Sun so far distant.
 

1. What is tidal locking?

Tidal locking is a phenomenon where a celestial body, such as a planet or moon, has one side constantly facing its parent body due to the effects of tidal forces.

2. Is Uranus tidally locked?

No, Uranus is not tidally locked. It rotates on its axis once every 17 hours and 14 minutes, which is much faster than its orbital period around the Sun (84 Earth years).

3. How does tidal locking occur?

Tidal locking occurs due to the gravitational pull of a larger body on a smaller one. As the smaller body rotates, the larger body's gravity pulls on it, causing its rotation to slow down until it becomes tidally locked.

4. Is Uranus affected by tidal forces?

Yes, Uranus is affected by tidal forces from its moons. However, due to its relatively small moons and their distance from the planet, the effect is not as significant as on other planets such as Jupiter or Saturn.

5. What are the implications of tidal locking on a planet?

Tidal locking can lead to a number of effects, such as a planet's rotation and orbit becoming synchronized, changes in its weather patterns, and the formation of tidal bulges on its surface. It can also affect the distribution of heat and potentially impact the planet's habitability.

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