Starstruck: The Milky Way rises over Quabbin Reservoir. Possibly one of the darkest sky sites in Massachusetts [2048x2035][OC]

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Starstruck: The Milky Way rises over Quabbin Reservoir. Possibly one of the darkest sky sites in Massachusetts [2048x2035][OC]
Saturn’s diffuse, bright, but icy E-ring, and the ‘bright spot’ of the moon Enceladus, which is responsible for the ring’s existence.
[ 20.04.16 • 1/100 DAYS OF 1 ] first day of posts :) pretty satisfied with how my chem notes turned out (still in the process of vetting and adding stuff) and hopefully i’ll actually make it to 100 days because my exams are really in like 17 days but i’ll try to continue on after that :’)
p.s. if you’ve seen this post before it was from my old blog :)
this is so inspiring o M g
Fluorite with Purple Phantoms
Locality: Okoruso Mine, Otjiwarongo District, Namibia
Cavitation happens when the local pressure in a liquid drops below its vapor pressure. A low-pressure bubble forms, typically very briefly, when this occurs. These bubbles are spherical unless they form near a surface. In that case, the bubbles take on a flatter, oblong shape. As they collapse, the bubbles form a jet, like the one seen inside the bubble above. The jet extends through the bubble and stretches into a funnel shaped protrusion on the bubble’s far side. Eventually, the whole shape becomes unstable and breaks into many smaller bubbles. Shock waves can be generated in the collapse, too; often the jet generates at least two in addition to the ones created when the bubble reaches its minimum size. This is part of why cavitation can be so destructive near a surface. (Image credit: L. Crum)
The Schubert Problem
This is the first in a little two-part sequence about the history of the Schubert calculus. I like this story a lot because it highlights the really human aspect of doing math, and gives lie to the myth that good mathematics only comes from rigorous logical reasoning. Both of these posts are intended to be roughly independent and nontechnical (with the second one, admittedly, a bit more detail-oriented than the first).
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If you study some of the more geometric aspects of math, you at some point start to encounter a lot of objects having the name ‘Schubert’ attached to them: Schubert varieties, Schubert classes, Schubert polynomials. So who was Schubert, anyway?
Hermann Schubert was a German mathematician who worked in the mid-to-late 1800s. Note that he is not Franz Schubert, the famous Classical composer; instead he was a high-school teacher. Although not a member of the university system, he was an active researcher, working in a particularly combinatorial corner of algebraic geometry.
The trouble started when Schubert was trying to answer questions like the following:
Fix four lines in three-dimensional space, no two of which are parallel or intersecting. How many lines intersect all four of them?
If you’re anything like me, you say: there’s no way that’s enough information to give an answer, or even if it is, there’s no way the answer is anything interesting. But in fact, a miracle occurs. Not only is there an answer, but the answer is always the same: there are exactly two such lines!
Schubert was part of a group of people who were interested in answering these questions, and he figured out a brilliant way to do it. You could presumably figure this out by some very long and arduous computations with coordinates, but that’s not what Schubert did. For instance, this is how Schubert solved the problem above:
Let’s solve an easier problem: suppose that there are two pairs of intersecting lines in three-dimensional space, no two of which are parallel. Now, there is one obvious line that meets all four of the others: passing between the two points of intersection. A second line can be constructed as follows: each pair of intersecting lines spans a plane, so take the two planes defined by each pair, and they intersect in a line: that line meets all four of the others.
Now, pick one of the pairs of lines, and pull them apart (slowly?). By continuity considerations, there will still be two lines that intersect all four of them. And then do the same for the other pair and of course there will still be two lines that intersect all four, by conservation of number.
The first time you see this, you may not find this argument very convincing.
Well, turns out nobody else did either.
They said “now, wait just a second here, Schubes. What are these continuity considerations you’re talking about? What’s this whole conservation of number thing?” And Schubert was like “I dunno.”. And the math community said “What do you mean, you don’t know? You don’t have a proof?”. And he was like “Nah man, I don’t have a proof. I have the answer. Deal with it.”.
And they did deal with it. They had to, because he kept solving problems and he kept using these totally wonky methods and he kept getting the right answers. The thing that makes this story really weird is: lots of other people tried to get on this bandwagon, and tons of other people just couldn’t do it. They would do this whole simplifying assumption and try to do this whole “conservation of number” thing and they would just get completely wrong answers.
Eventually, the situation got so ridiculous that in 1900, David Hilbert wrote this as the 15th problem on his famous list:
The problem consists in this: To establish rigorously and with an exact determination of the limits of their validity those geometrical numbers which Schubert especially has determined on the basis of the so-called principle of special position, or conservation of number, by means of the enumerative calculus developed by him.
You can practically feel the frustration seeping out of these words, 117 years later.
Wikipedia lists this question as “partially resolved”. What is meant by this is, to this day, we still don’t really know what “conservation of number” actually means. Phrasing it in Hilbert’s language, we don’t understand the “limits of its validity”. However, in the end, people did figure out a way to do these computations rigorously, and so research interest in figuring out exactly where “number is conserved” has by and large died out.
I’ve already written a [[little]] [[bit]] about the technical tools which make this possible, but in the next post I’d like to talk about a high-level picture, and an “intermediate step” that I’d never really understood before.
[ Next ]
Do you know what this is? A bee? A wasp? Nope. It’s a hoverfly, which looks like a bee or wasp in order to avoid predators. Hoverflies are beneficial insects and can be found everywhere except Antarctica. Glad I just saw one in my garden!
NASA: How to Safely Watch a Solar Eclipse
Physics is my only lover; and no matter how complicated the problem, we always work it out (because I’m quite good at math, and so is he).
Lazulite
Locality: Mt. Seafoam, Rapid Creek, Yukon, Canada
The earth’s movement creates a few cycles. First of all, it rotates on its axis about once every 24 hours, producing sunrises and sunsets. At the same time, it’s making a much slower cycle, orbiting around the sun approximately every 365 days. But there’s a twist. Relative to the plane of its orbit, the Earth doesn’t spin with the North pole pointing straight up. Instead, its axis has a constant tilt of 23.4º. This is known as the Earth’s axial tilt, or obliquity. This seemingly minuscule tilt is the reason…for the seasons.
Another feature of the Earth’s revolution is its orbital eccentricity. The earth’s orbit around the sun is an ellipse, with its distance to the Sun changing at various points. The corresponding change in gravitational force causes the Earth to move fastest in January when it reaches its closest point to the sun – the perihelion – and slowest in July when it reaches its farthest point – the aphelion. The Earth’s eccentricity means that solar noon – the time when the sun is highest in the sky – doesn’t always occur at the same point in the day.
Learn about the Sun’s analemma by watching the TED-Ed Lesson The Sun’s surprising movement across the sky - Gordon Williamson
Animation by TED-Ed
Rare combo of Diopside on Bi-color Tanzanite - Merelani Hills, Tanzania
1,000-Year-Old Colored Glass Beads Discovered in West Africa
A newly discovered treasure trove of more than 10,000 colorful glass beads, as well as evidence of glassmaking tools, suggests that an ancient city in southwestern Nigeria was one of the first places in West Africa to master the complex art of glassmaking, scientists reported.
The finding shows that people who lived in the ancient city of Ile-Ife learned how to make their own glass using local materials and fashion it into colorful beads, said study lead researcher Abidemi Babalola, a fellow at Harvard University’s Hutchins Center for African & African American Research.
“Now we know that, at least from the 11th to 15th centuries [A.D.], there was primary glass production in sub-Saharan Africa,” said Babalola, who specializes in African archaeology.
Ancient city of IIe-Ife
The ancient city of Ile-Ife was the ancestral home of the Yoruba, an ethnic group of people who live in Africa today. The Yoruba people view Ile-Ife as the mythic birthplace of several of their deities, Babalola and his colleagues wrote in the study.
For more posts like these, go to @mypsychology
For more posts like these, go to @mypsychology
Too soon
It’s been 1,937 years