April 30 - Walpurgis Night

    Posted on April 30, 2022

This is an update of my post published on April 30, 2011:




It's May Day Eve tonight! Time to eat, drink, and be merry around a roaring bonfire!

Some people dress up like witches and go out into the streets in a sort of wandering carnival.

Some folks watching the bonfires may be dressed like witches, too.


There's dancing, “capping” (wearing special caps  and putting similar hats onto statues), entertainment, speeches...and sometimes pranks, as well.

This holiday is called various names in various countries, including Valborg in Sweden, Vappu in Finland, Hexennacht in Germany, Volbrioo in Estonia, and the čarodejnice in the Czech Republic.


What's it all about? Well, it's another spring festival—another way of celebrating the return of sunshine and warmer temperatures. It seems to me that this holiday is a cross between Halloween and Mardi Gras—but with the added benefit that the next day, May Day, is also celebrated by many!








(Last Saturday)



(Last Saturday in April)



National Sense of Smell Day
(Last Saturday in April)






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April 29 - Happy Birthday, Harold Urey

    Posted on April 29, 2022

This is an update of my post published on April 29, 2011:



Harold Urey, born on this date in 1893, discovered  “heavy hydrogen” and “heavy water”!

Imagine a glass of water saying, “Does this hydrogen make me look heavy?”



Of course, the answer is that certain hydrogen atoms and kinds of water don't look heavy, but they are in fact heavier than “normal.” In other words, they weigh more.

If you want to know why, you need to learn a bit about isotopes.

Each kind of element—like carbon or gold or iron or oxygen—has recognizable characteristics. It's the kind of element that easily combines with other elements—or it isn't very reactive. It's a metal, or it isn't. It's radioactive, or not; brittle, or not. At room temperature, a particular element may be a solid, liquid, or gas. It has a certain color.

The thing that makes an element that element—in other words, what makes gold gold and oxygen oxygen—is the number of protons it has.

Gold always has 79 protons and generally has 79 electrons. Oxygen just has 8 protons (and, generally, 8 electrons). It's really hard to change the number of protons an atom has—that's what happens in the center of the sun and in nuclear reactors—but, if you do change the number of protons, you change the element. For example, take away one of gold's protons, you get platinum. Add a proton, you get mercury.


The Periodic Table of the Elements is
organized in part by atomic number, which
is the number of protons each element has.

There aren't just protons and electrons in an atom; there are also neutrons. These particles are about a large as a proton but have no charge. Neutrons are necessary to help protons hang together despite their like charges.

The thing is, since neutrons have no charge, you can add them to an atom and not change the element. Most gold atoms have 117 or 118 neutrons—but if you add a few more or take a few away, you still have gold. You just have a different isotope of gold. It has the same characteristics (solid, metal, yellow colored), but it is heavier.


Forget about gold...I thought we were talking about hydrogen!

Hydrogen, which is the most common element, by far, in the universe, has a super simple structure: just one proton and one electron.

But some hydrogen atoms have one neutron as well. These hydrogen atoms act just like other hydrogen atoms (super light, super reactive, gaseous), but they are almost twice as heavy as normal hydrogen atoms.
Different "flavors" of hydrogen.
The one labeled "protium" is by
far the most common!

These heavier-than-normal atoms are called deuterium, or heavy hydrogen. About one out of every 6,400 hydrogen atoms in Earth's oceans is deuterium.

Discovery!

Back in the day, scientists didn't know why certain samples of materials were heavier than others, they didn't know the reason for the difference in weight; some theorized that it was caused by different numbers of “nuclear electrons.” (Remember, the difference is actually caused by more neutrons.) Scientists believed that hydrogen couldn't have isotopes. But an American chemist named Harold Urey was able to repeatedly distill liquid hydrogen and then—in 1931—to detect “heavy hydrogen” with a spectroscope.

And so it was that Urey and his coworkers were able to discover deuterium a year before scientists discovered neutrons—the correct explanation for deuterium!—and for his work, Urey won a Nobel Prize.


By the way, people are still making discoveries about heavy water. Like, ice cubes made from heavy water sink rather than float!


And heavy water tastes sweet! WARNING: Heavy water can be toxic. Only taste a tiny bit - and only with adult approval and supervision.



April 28 - Happy Birthday, Francis Baily

    Posted on April 28, 2022

This is an update of my post published on April 28, 2011:



I am lucky enough to have seen a total solar eclipse,
and I think you should try hard to see one if you
possibly can!


Francis Baily was lucky, because he got to see two solar eclipses!

You probably know that a solar eclipse is a rare event when the moon gets in the way of Earth's view of the sun. In other words, those people on Earth in the moon's shadow see an eclipse!

What you may not know is the anatomy of a shadow and how that relates to what kind of eclipse people get to see.


The umbra is the darkest part of the shadow in the diagram. People in the umbra see the moon completely cover the sun—and then they get to see the sun's corona, which is usually washed out by the brightness of the sun itself. This is called a total solar eclipse.


Total solar eclipse

The antumbra extends beyond the tip of the umbra. People in the antumbra see the moon fully in front of the sun, but the moon is too small to completely cover the sun, so there appears to be a ring of fire around a black disc. This is called an annular solar eclipse.


Annular solar eclipse

The penumbra is the lighter gray part of the shadow in the diagram. Obviously, you can see that many more people will be in the wide penumbra than in the narrow umbra. These people will see the sun with a “bite” taken out of it as the moon only partially covers it. This is called a partial solar eclipse.



Back to Baily


Francis Baily, born on this day in 1774, was an English astronomer. On May 18, 1836, he observed an annular solar eclipse in Scotland, and he reported that there were bright “beads” of sunlight bulging on the ring of sun visible during the eclipse. These beads are now called “Baily's beads,” and they are caused by the irregular surface of the moon, which of course has mountains and valleys and craters.


Baily traveled to Italy to see a total solar eclipse on July 8, 1842. Again, he was able to observe the beads just before and just after totality.


By the way, when just one “bead” is left uncovered, we see the “diamond ring effect.”




















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