Ancient Earth Globe
dinosaurpictures.org
dinosaurpictures.org
https://news.ycombinator.com/item?id=24459997
This one has comments/answers by the author that explain his reasoning behind the design (linked to by the thread above - and so we don't need to ask the same questions all over again ;) ):
Pretty much all of it.
Unless you believe like a couple did in the 70s that there was a coming ice age which we completely stopped and reversed. I would love to hear the steelmanning for that.
However, if the goal was to head off the next Ice Age, all the scientists agree, "Mission Accomplished!"
Probably best to eliminate fossil fuels from the energy mix immediately, don't you think?
Where can I read more?
We've very much curbed out aerosol, but increased our greenhouse-gas pollution. I very much doubt that their analysis was correct to begin with, and I doubt had we not curbed the aerosol pollution, we'd be facing an ice age today - but I'm just some jerk on the internet - I could easily be wrong! Right or wrong, the first paragraph above is how I understand the argument to have been made at the time.
[0] https://arstechnica.com/science/2016/06/that-70s-myth-did-cl...
> The further back we look into the geological past, the more obscured the view, masked by an increasingly fragmentary geological record. This has resulted in a controversy on whether plate tectonics operated the same way, or even at all, during early Earth history.
[1] https://www.gplates.org/ [2] https://www.gplates.org/docs/pygplates/pygplates_introductio... https://github.com/GPlates/gplately [3] https://portal.gplates.org/#apps-anchor [4] https://portal.gplates.org/portal/dt/ (select "Mantle Reference Frame" for a similar layout) [5] https://portal.gplates.org/cesium/?view=PaleoDEM https://www.earthbyte.org/paleodem-resource-scotese-and-wrig...
Consider "today"'s coastline. Earlier today, a mere 15 kya towards Last Glacial Maximum, Florida was twice as thick, and the Boston coast was down past Long Island NY. So how do you non-deceptively show a coastline for "today"? Perhaps use such low resolution that these differences aren't visible? Use an aphysical elevation color scheme which deemphasizes water height? Use timelapse averaging (if a single frame was exposed for 100 ky, then ...)?
Years ago NASA did a global clouds-removed monthly image set. You can see the snow line advancing and retreating with the seasons. See changes in vegetation. Months look very different. What best represents the year? An average of them? The preceding year had different weather. How can the preceding decade be nicely represented? The preceding 100 y, 1 ky, 10 ky?
Clouds are a major visual component our planet. Their patterns change with seasons, with years, with climates, with topographies. How might you show this year's clouds? This decades? This 100 ky? This 1 My?
Climate. Consider the insanely desiccated Pangaean central equatorial desert. In OP, it's colored green based on height. I've seen it shown overlayed with swirls of seemingly cumulus clouds.
Science education graphics have the unfortunate property of combining some aspects done with great care, with many others done with great artistic bogosity, and students left with no way to sort what is which. How might paleoglobe visuals be improved?
Professor Scotese was a great partner and instrumental in putting this visualization together. He's acknowledged on the site, but for those interested here is his website: http://www.scotese.com/. I believe he has a more modern iteration of the paleomap that is not downloadable on the web, but for various reasons I did not get those textures in this visualization (they didn't wrap properly iirc).
He also has a nice writeup of the methods used here: https://drive.google.com/file/d/1-q0WIa7ofISFHyBe4UxvN8DIPs8...
You can see much more cutting edge research here: https://www.science.org/doi/10.1126/science.add2541, which is done within the group that built GPlates. (video of the outputs here: https://youtu.be/QaDt1VQ9WlY )
Like many of these tools it suffers from northern hemisphere bias that hides interesting information about the southern hemisphere.
In looking to correctly simulate axial tilt we get Gondwana and Antarctica hidden from view in the shadow, their sunlit versions only available via options rather than hidden by default.
The southern polar region is the more interesting of the two for the vast majority of geological history and I think as Antarctica thaws we will need more interested geologists in it than our current conversations are generating.
I wish authors would emphasise it more when creating visualisations like this.
I regularly think about what the earth looked like X million years ago and I've been wanting exactly this for a very long time :).
On a related note, I heard both of those coastlines were formed by glaciers in the last ice age. But wouldn't that also have been true during every ice age? Or did they just get more dramatic each time? ;)
Also, the constant spinning is super infuriating and mildly sickening.
Add this somewhere which makes sense in the html;
`<input type="range" min="0" step="1" id="mySlider" max="25">`
Then, add this script in your console;
```js
const slider = document.getElementById('mySlider'); const select = document.getElementById('years-ago');
slider.addEventListener('input', () => { select.selectedIndex = Number(slider.value); select.onchange(); });
```
Earliest humans, Homo Habilis, appeared 2.4-1.4 Mi years ago.
I am definitely not a geologist, and this is probably un-provable... but, to me, it sure seemed like a plausible idea.
Your idea's first hurdle is the length of day vs the length of month. How do you keep the moon over one bulged part of Earth at all times? (it's a very different story for the moon, whose 'day' is as long as its orbit, more at [1]) Additionally, there is a solar tide at work on the oceans that is visible daily, and especially at spring and neap tides. The sun's mass drives a maximum of almost a third of the total ocean tidal bulge.
The second hurdle is viscosity (or if you like, elasticity): tides bulge the most readily-flowing parts of a body the strongest. That means the atmosphere (which is more strongly affected by daily heating <https://en.wikipedia.org/wiki/Atmospheric_tide>), and the oceans are much more strongly affected than the "asthenosphere" (the rocky parts).
In particular, tides bulge the ocean by about a metre. The solid earth tide is closer to 0.2 metres. Thus, the question is: how do you raise a tidal bulge in the rocky part of Earth and keep it from being flooded by ocean tides?
> I am definitely not a geologist
It's more gravitation vs the liquid flow of a stratified (layered) planet than geology that is are the big hurdles.
For experts, tidal Love numbers are the important things for any round stratified body: <https://en.wikipedia.org/wiki/Love_number>, which describe the bumpiness (mass multipole) raised by tidal fores on a spherical body immersed in a tidal gravitational field.
The mantle's rheology (elasticity, viscosity, rigidity), representing about 85% of Earth's total volume, is the primary driver of the Earth's Love numbers. There's more detail on that here: <https://geodesyworld.github.io/SOFTS/solid.htm#link3>.
The crust is quite low-volume by comparison. So a third hurdle is straightforwardly: if there were a persistent bulge in the mantle, why wouldn't a relatively thick part of the crust (a giant continent in your idea) not just "roll downhill", or conversely, how do you get fractions of a round supercontinent to "roll uphill" to some lunar-attraction-induced meeting point?
Finally, with present understanding of continental drift, the continents tend split apart and come together over millions of years, and there's no evidence for anything approaching circularity. The link at the top lets one step through almost a billion years of continental drift, showing this fairly clearly.
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[1] Slide 8 ("Tides (2)") of the lecture notes at <https://websites.pmc.ucsc.edu/~fnimmo/eart162_10/Week8.pdf> is pretty accessible, showing an Earth-centric diagram of tides and a moon-centric diagram of its tides, and throughout the rest of the slide deck there's lots of heavy stuff for people who like to grapple with mathematics.
[0] https://physics.stackexchange.com/questions/31429/how-long-w...
[1] https://www.dummies.com/article/academics-the-arts/science/p...
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[1] You could probably toy with models of Earth-moon as a pair of Jacobi ellipsoids or piriforms (pear-shaped, thin ends inwards) but I don't see that working without a much smaller mass ratio and higher spins. Piriform bodies (at least of homogenous self-gravitating fluid, which is a good representation of the mantle) are generally unstable. Maybe that's good if you can find a path that relaxes back to a Maclaurin (oblate) spheroid for the Earth mass that doesn't also relax the (whole of the) "bump", and relaxes the moon to its weak Jacobi (scalene) spheroid.
Really speculating substantially away from what I know: maybe the "synestia" flavour(s) of the giant impact hypothes(e)s for the origin of the moon might be a path to some test simulation codes: coalesce an ellipsoidal (or as I said, piriform or even oviform) moon first and have that drive some aspects of Earth's planetary differentiation (which happens later in that (family of) model(s): <https://en.wikipedia.org/wiki/Synestia>). In particular, the driving should be away from homogeneity in an attempt to escape eventual hydrostatic equilibrium for the Earth-mass which otherwise leaves you stuck with encoding surface features on the (very) thin crust and then dealing with the Mauna Kea problem above. I don't know how you could approach this idea with realistic chemistry though, which I think melts & dissolves this line of thinking.
ETA: Really wild speculation: with unrealistic chemistry, freeze out a long-term solid hourglass structure with the neck at the Earth's centre of mass, piling lots of rocks on the ends terminating just under the surface (but above the mantle) at the poles, and then have one pole always point to the moon Mass. Doesn't at all fit lots of lines of evidence in very old surface rocks, though. Also very hard to wash out tides raised by the sun.
- the tilt of the earth was substantially different. Where Florida is today, would have been where New York was then. [1]
- the poles (north & south) were in radically different places than today. There’s evidence that dinosuars flourished in what is the artic today because the artic then wasn’t so cold [2]
https://theswaddle.com/earth-had-a-dangerous-axis-tilt-84-mi....
https://www.snexplores.org/article/dinosaur-arctic-bone-foss...
What a completely scitifically illiterate article.