Venus Over Bioluminescent Algae

Venus Over Bioluminescent Algae

Venus over Bioluminescent Algae

More Posts from Sleepysneezeydopeydoc-blog and Others

Photography By Juh-ku
Photography By Juh-ku

Photography by Juh-ku

I wish I could have been there.

Daytona Beach 1957

Daytona beach 1957

Modified Leaves: Insect Traps
Modified Leaves: Insect Traps
Modified Leaves: Insect Traps

Modified Leaves: Insect Traps

Carnivorous plants are plants that derive some or most of their nutrients (not energy) from trapping and consuming animals, typically insects. Carnivorous plants have adapted to grow in places where the soil is thin or poor in nutrients, especially nitrogen, such as acidic bogs and rock outcroppings. These carnivorous plants have modified leaves that help to trap and digest prey.

The carnivorous plant in the first picture is a Venus flytrap that belongs to the genus Dionaea. The Venus flytrap has small trigger hairs on the inside of its leaf that cause the trap to close around its prey. The carnivorous plant in the middle picture is a sundew that belongs to the Drosera. Sundews have small tentacles, topped with sticky secretions, that cover the leaves.  Sundews are able to move their tentacles towards the center of the leaf to bring the insect into contact with as many stalked glands as possible. The carnivorous plant in the bottom picture is a  species of North American pitcher plants that are commonly called trumpet pitchers. Insects fall into the pitcher plant and cannot climb out. Meanwhile, digestive enzymes in the pitcher leaf break down the prey.

Modified Leaves Part:   1    2     3     4     5     6

Mathematical Spirals
Mathematical Spirals
Mathematical Spirals
Mathematical Spirals

Mathematical Spirals

According to Wikipedia, a spiral is a curve which emanates from a central point, getting progressively farther away as it revolves around the point (similar to helices [plural for helix!] which are three-dimensional). Pictured above are some of the most important spirals of mathematics.

Logarithmic Spiral: Equation: r=ae^bθ. I must admit that these are my favorite! Logarithmic spirals are self-similar, basically meaning that the spiral maintains the same shape even as it grows. There are many examples of approximate logarithmic spirals in nature: the spiral arms of galaxies, the shape of nautilus shells, the approach of an insect to a light source, and more. Additionally, the awesome Mandelbrot set features some logarithmic spirals. Fun fact: the Fibonacci spiral is an approximation of the Golden spiral which is only a special case of the Logarithmic spiral. 

Fermat’s Spiral: Equation: r= ±θ^(½). This is a type of Archimedean spiral and is also known as the parabolic spiral. Fermat’s spiral plays a role in disk phyllotaxis (the arrangement of leaves in a plant system). 

Archimedean Spiral: Equation: r=a+bθ. The Archimedean spiral has the property that the distance between each successive turning of the spiral remains constant. This kind of spiral can have two arms (like in the Fermat’s spiral image), but pictured above is the one-armed version. 

Hyperbolic Spiral: Equation: r=a/θ. It is also know as the reciprocal spiral and is the opposite of an Archimedian spiral. It begins at an infinite distance from the pole in the center (for θ starting from zero r = a/θ starts from infinity), and it winds faster and faster around as it approaches the pole; the distance from any point to the pole, following the curve, is infinite. 

Can You Flatten A Sphere?

Can you flatten a sphere?

The answer is NO, you can not. This is why all map projections are innacurate and distorted, requiring some form of compromise between how accurate the angles, distances and areas in a globe are represented.

This is all due to Gauss’s Theorema Egregium, which dictates that you can only bend surfaces without distortion/stretching if you don’t change their Gaussian curvature.

The Gaussian curvature is an intrinsic and important property of a surface. Planes, cylinders and cones all have zero Gaussian curvature, and this is why you can make a tube or a party hat out of a flat piece of paper. A sphere has a positive Gaussian curvature, and a saddle shape has a negative one, so you cannot make those starting out with something flat.

If you like pizza then you are probably intimately familiar with this theorem. That universal trick of bending a pizza slice so it stiffens up is a direct result of the theorem, as the bend forces the other direction to stay flat as to maintain zero Gaussian curvature on the slice. Here’s a Numberphile video explaining it in more detail.

However, there are several ways to approximate a sphere as a collection of shapes you can flatten. For instance, you can project the surface of the sphere onto an icosahedron, a solid with 20 equal triangular faces, giving you what it is called the Dymaxion projection.

The Dymaxion map projection.

The problem with this technique is that you still have a sphere approximated by flat shapes, and not curved ones.

One of the earliest proofs of the surface area of the sphere (4πr2) came from the great Greek mathematician Archimedes. He realized that he could approximate the surface of the sphere arbitrarily close by stacks of truncated cones. The animation below shows this construction.

The great thing about cones is that not only they are curved surfaces, they also have zero curvature! This means we can flatten each of those conical strips onto a flat sheet of paper, which will then be a good approximation of a sphere.

So what does this flattened sphere approximated by conical strips look like? Check the image below.

But this is not the only way to distribute the strips. We could also align them by a corner, like this:

All of this is not exactly new, of course, but I never saw anyone assembling one of these. I wanted to try it out with paper, and that photo above is the result.

It’s really hard to put together and it doesn’t hold itself up too well, but it’s a nice little reminder that math works after all!

Here’s the PDF to print it out, if you want to try it yourself. Send me a picture if you do!

Get You Best Paper, Cut A Circle And Fold It So That The Circumference Falls On A Fixed Point Inside.

Get you best paper, cut a circle and fold it so that the circumference falls on a fixed point inside. Repeat, using random folds. Now see the creases. This is how you paper-fold an ellipse.

More 1961 - 1969 Lincoln Continentals

More 1961 - 1969 Lincoln Continentals

Hubble Captures Vivid Auroras In Jupiter’s Atmosphere

Hubble captures vivid auroras in Jupiter’s Atmosphere

Via NASA - Full story

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I like to Study Objects In Motion

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