Ancient shell shows days were half-hour shorter 70M years ago
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That is decidedly not true. At the very least the eccentricity of the Earth's orbit around the Sun is known to change[0]: "The major component of these variations occurs with a period of 413,000 years (eccentricity variation of ±0.012)".
Moreover, I seem to recall reading that over the 4.5 billion year scale the distance of various planets to the Sun has varied as well, though I don't have a reference for that right now.
> The orbital period (the length of a sidereal year) is also invariant, because according to Kepler's third law, it is determined by the semi-major axis.
Which makes sense, because the semi-major axis depends on the energy of the orbit, and there's not really much that would be altering that in the short timeframe of a Milankovitch cycle.
But on galactic time scales, IIUC, no, because the gas giants' gravity does affect the orbits of each other and the smaller planets.
Kepler's law is an approximation, and it most certainly does not hold over large time scales. Heck, it fails on short time frames too - one of the early successes of relativity was to explain the precession of Mercury's perihelion from Kepler style theory to observation.
Heck, even restricting to classical physics, Kepler's law fails as soon as you have three bodies, since the derivation is only for a two body problem. A third (or more) body makes his laws fail. Our solar system has well over thousands of bodies all interacting.
So this is only an argument for the invariance of the (incomplete) model of Kepler, but fails in real life. We have plenty of better models (i.e., that agree better with observation) that are not invariant.
In addition Earth year may have changed during the Great Solar System Reconfiguration Event when Jupiter and the other gaseous planets hypothesized to have migrated outwards from orbits closed to the Sun. This may have happened 3.8 billion years ago causing increase of craters on the terrestrial planets at that time.
https://www.nasa.gov/topics/solarsystem/features/young-jupit...
No, they can't. See my other response just upthread.
https://en.wikipedia.org/wiki/Nice_model
Edit: Basically, the gas giants started really close into the sun but later moved outwards. We see a lot of other systems with gas giants close into their suns right now. In the Nice model, the larger gas giants had their orbits move slowly outwards, causing havoc in our system. This is possibly when the Moon was formed. It's still a lively debate, as we have not yet found Planet X yet.
TLDR: Fund NASA more.
It's not an assumption, it's what our best current data tells us. We have abundant evidence of the length of the Earth's day changing--this article is certainly not news, we have known for decades that the Earth's rotation has been gradually slowing over the past few billion years. We have no evidence of the length of the Earth's year changing significantly, and calculations agree with that (see below).
> The Earth experiences tidal friction from the Sun just like the Moon and Earth affect each other. I am guessing the year lengthening effect slower than month & day lengthening because Suns tidal force is a third of Moons.
The size of the tidal bulge on the Earth due to the Sun is about a third of that due to the Moon. But that is not at all the same as the slowing of the Earth's year due to the Sun's tides being about a third of the slowing of the Earth's day due to the Moon's tides. The situations are very, very different.
In the case of the Earth-Moon system, tidal friction causes angular momentum to be transferred from the Earth to the Moon. This slows the Earth's spin and increases the radius of the Moon's orbit.
In the case of the Earth-Sun system, tidal friction can't transfer angular momentum from the Earth's spin to the angular momentum of the Earth's orbit about the Sun, because the Earth is not orbiting itself; the mechanism that transfers angular momentum from the Earth's spin to the Moon's orbit about the Earth simply does not apply to the Earth's orbit about the Sun.
In fact, while the Sun's tidal friction does make the Earth's spin slow down a little more than it would due to the Moon alone, the result of this is to make the radius of the Moon's orbit increase a little more than it would if the Earth-Moon system were alone in space. In other words, the Sun's tidal friction simply augments the Moon's tidal friction in driving the same mechanism, transferring angular momentum from the Earth's spin to the Moon's orbit about the Earth. There is no transfer of angular momentum from the Earth's spin to the Earth's orbit about the Sun.
This argument cannot be correct. Suppose the sun were a point mass. It would still have tides at Earth, just like the real Sun does, but the interaction would not be able to cause any change to its spin. So, by conservation of angular momentum, if the Earth loses rotational angular momentum, that MUST be transferred to orbital angular momentum.
The mechanism of course still exists. The Earth and Moon orbit each other; the Sun and Earth orbit each other. The bulge on the Earth induced by the Moon accelerates the Moon, and the bulge on the Earth induced by the Sun accelerates the Sun.
More precisely, it exerts a torque on the Moon, which is equal and opposite to the torque exerted by the Moon on the bulge. So does the bulge on the Earth induced by the Sun.
> the bulge on the Earth induced by the Sun accelerates the Sun.
This statement is correct in principle (or more precisely, the statement that the bulge on the Earth induced by the Sun exerts a torque on the Sun), and you are right that I left it out of my previous post.
Also, as I noted above, the bulge on the Earth induced by the Sun also exerts a torque on the Moon. And, for that matter, the bulge on the Earth induced by the Moon also exerts a torque on the Sun. I believe the net torque on the Sun is about 20% of the net torque on the Moon.
However, that does not mean the effect on the Earth's orbit is 20% of the effect on the Moon's orbit. The relative magnitudes of the effects depend on how large the torque is compared to the relevant orbital angular momentum. Since we are working in an Earth-centered frame, that means we need to compare the Moon's orbital angular momentum around the Earth with the Sun's orbital angular momentum around the Earth. If you do the math, you find that the latter is about 300 billion times larger than the former. Multiply that by another factor of 5 (for the 20% ratio of torques) and the effect on the Earth's year is about 1.5 trillion times smaller than the effect on the Moon's month.
There's a further point here, though. The torque exerted on the Moon by the bulge is constant over time, because the position of the Moon relative to the bulge is constant (the bulge "leads" the Moon by a constant angle which is the result of a balance between the torque on the bulge exerted by the Moon and the pull on the bulge exerted by the Earth's spin). But the position of the Sun relative to the bulge is not constant: it goes through a complete cycle over the course of a month. So it seems to me that, at least to first order, the net torque of the bulge on the Sun over the course of a month should cancel out, so there will be no net exchange of angular momentum between the Earth's spin and the Sun-Earth orbit.
If you assume the revolution period was same back then as it is now... sure, half an hour difference I get it. Or are we assuming that the rotation is changing faster than the revolution?
Contrast that to the Earth/Moon's rotational period, which we expect to slow over time due to energy consumed by tides "sloshing around".
Not consumed, literally flung out into space via the moon. It’s speeding up, we’re slowing down. No violation of thermodynamics required.
However, the angular rate of the Moon's rotation is staying the same over time (it's tidally locked at one rotation per revolution). It's not exactly speeding up. Instead it's getting further away, which increases the moment of inertia and therefore transfers momentum.
Or, stated another way, anything that could account for that large of time variation in our year over that short of a time period... imagine ocean tides but with the Earth’s mantle instead. Then we’re not here to have this debate.
For all practical purposes, the rotational period of the earth around the sun can be considered a constant.
But there are... The earth orbiting causes tiny tides on the sun. They might only be a few millimeters, but they're non-zero. Over time, tidal drag will tend to make years longer.
Anyone have the time and skill to do a ballpark guess the magnitude of this effect?
Earth spins slower > Moon Speeds Up Less Rotations per Orbit > More Hours per Day
Number of days is changing because the day is going from 23.X hours to 24.X hours due to the Earth rotating slower. Hence, same length year if you measure it in absolute time, just less days in relative time.
>>>>> Wasn't the Earth's revolution on a different period back then too?
>>>> There is no force comparable to lunar tidal forces affecting the period of revolution
>>> But there are... The earth orbiting causes tiny tides on the sun [...] Over time, tidal drag will tend to make years longer.
>> Wouldn't tidal drag make years shorter?
> What's changing isn't that, it's the sidereal day.
https://infiniteundo.com/post/25326999628/falsehoods-program...
The new study found the composition of the shell changed more over the course of a day than over seasons, or with the cycles of ocean tides. The fine-scale resolution of the daily layers shows the shell grew much faster during the day than at night
But Venus and Mercury have lost their rotation, not having a massive moon to keep them rotating, against solar tides slowing them.
Mars has kept its rotation by its distance from the sun. Its tiny moons help only a little.
Mercury is weird. It is tidally locked, but not like our moon. Mercury rotates around its axis three times for every two orbits. (Which I just learned while writing this comment because as a child my books told me it had a permanent sunward side.)
On its face, it is surprising that rotational direction can change, but rotational momentum is conserved not by individual bodies, but by the whole, interacting system, subject also to conservation of energy. So, momentum and energy trade around between bodies in complicated ways.
Somebody double check this please. ;) Also, the Sun will only last for another 4B years.
So we would have had a nice regular calendar back then.
Calendars are silly. "Neat" ones even more so.
I know their mass would be the same but wouldn't a faster spinning earth counter gravity similar to how satellites maintain a stable orbit?
Acceleration due to gravity is 9.8 m/s^2, so you weigh 0.3% less in Singapore than at the North Pole. (There are other factors, like the Earth's bulge, which I won't consider.)
This small enough that people don't notice it. (Presumably dinosaurs wouldn't either.) Plus, most people don't live on the equator, and there's a cos(latitude)^2 factor which reduces the centripetal acceleration. At 45 degree latitude the acceleration is 1/2 that of the equator.
Speed up the Earth's rotation to 23.5 hours and it's 0.0352 m/s^2.
The difference is 0.0015 m/s^2 , which is quite small compared to the normal force of gravity.
Thus, it isn't really important for most things.
Any herbivores would also have to increase in size to not get eaten.
If the Earth slowed 30 minutes 62 times, uh, the days would be less than zero.
Any reason why the slowing of the day would be more dramatic these last 70 million years?
Still, extrapolating back to Earth’s early years would yield a rather short day. Sources from Wikipedia [1] [2] estimate a 5 hour day after the Theia Impact that created the Moon.
[1]: https://en.wikipedia.org/wiki/Earth's_rotation#Origin
[2]: https://www.annualreviews.org/doi/10.1146/annurev.ea.15.0501...
I'm curious, how do they decide that the earth spun faster on it's axis rather than the earth taking longer to orbit the sun?
Oddly enough it's pretty tricky to steer the Earth into the sun as well, but we should be losing minute amounts of energy that will eventually put the Earth closer to the Sun. This probably won't happen before the Sun explodes though.
The entire Earth orbits the Sun at 67,000 mph -- around 67X faster. And note that it is the entire mass of the Earth moving at that speed, not just the equator.
Changing the rotation speed by 1% is a whole lot easier than changing the orbital speed by 1%.
It's both effects really. Celestial bodies' orbits do undergo decay and also their rotation undergoes decay. The question is which happened to which degree, and I think the rotational slow down is the dominant effect in Earth's case.
Orbits decay due to various forms of drag. The long-term rate of decay of orbits in the Solar system is relatively well established.
Rotation also is slowed down due to drag, but in our case there's another major force: the tidal influence from the Moon. Earth's Moon is a relatively large companion (at 1.23%[1] by mass). Both bodies influence each other tidally, and that influence saps away rotational energy and also Moon's orbital energy; the Moon already got tidally locked to Earth. Aside of that there's a (smaller) tidal influence from the Sun, which again saps Earth's rotational energy.
--
[1] https://www.wolframalpha.com/input/?i=mass+of+the+moon+%2F+m...
I can't begin to imagine the forces that made this happen!
That means leap seconds will need to be inserted at ever increasing frequency over time until the Earth becomes tidally locked. Tidally locked means the Earth stops rotation so that the same side always faces the sun.
[1]: A good day for me is more like 27-28 hours, on average. Don't ask. Yes, I'll donate my hypothalamus to science.
Nope! That was just a typo bug in date.c:
int seconds = days * 84600;
See the transposed digits? That makes it exactly 1800 seconds shorter than 86400, or half an hour.Life is old. The time between stegosaurus's day and T. rex's is longer that between T. rex's and today.
AncientShell#> echo day.length