Showing posts with label Johannes Kepler. Show all posts
Showing posts with label Johannes Kepler. Show all posts

December 27 - Happy Birthday, Johannes Kepler and Louis Pasteur

  Posted on December 27, 2021


This is an update of my post published on December 27, 2010:




Two giants of science were born on this day (251 years apart!).



On December 27, 1571, Johannes Kepler was born in Germany. His claim to gigantic-ness—he is even called the Father of Modern Astronomy!— is that he figured out that the planets travel in elliptical (oval-shaped) orbits rather than round orbits, and he figured out three major laws of planetary motion. Sir Isaac Newton's law of gravitation had their genesis in Kepler's laws. Kepler also suggested that the tides were caused by the attraction of the moon. All of that is pretty gigantic!





In 1822, Louis Pasteur was born in France.


Pasteur's claim to gigantic-ality—he is considered one of the founders of microbiology!—is that he discovered much about causes and preventions of diseases: he developed the first vaccine for rabies and anthrax, invented pasteurization of milk, and discovered the role of bacteria in fermentation and was therefore able to improve the manufacture of wine.



For more on Kepler's Three Laws, try Carl Sagan's “Cosmos”...

Here is a video on how one of Louis Pasteur's discoveries not only changed science, but also changed the public's knowledge of - and caring about - science!

Kwanzaa (from 12/26/11 to 1/1/12)





March 8 - Kepler's Third Law Makes Its First Debut

Posted on March 8, 2018

You probably know that even ancient peoples knew that the world was spherical, but almost everybody "knew" that we - the Earth, that is - were the center of the universe.

In the 3rd Century BCE, an Ancient Greek astronomer named Aristarchus of Samos suggested that the Earth revolves around the Sun. 





As early as 1514, a German/Polish astronomer named Nicolaus Copernicus began to write and talk about a Sun-centered universe, although he didn't publish his fully worked-out theory until 1543. 

It took a while before the idea was generally accepted - like, a century and a half!

But in all that 150-or-so years, all along the way, various scientists tweaked the model, made more and better observations, suggested alternative explanations for the data, and inched forward in a slow-motion "Copernican Revolution."


One of these contributors was Johannes Kepler. He took Copernicus's model of the solar system, which explained observations better than did earlier models, and he made a few brilliant adjustments, so that the new model explained observations even better!

Kepler's "adjustments" were in the form of three "laws of planetary motion." He published the first two in 1609. He discovered the third on this date in 1618, and he published it in 1619.

Let's check them out:

#1 - The orbit of every planet is an ellipse (basically, an oval) with the Sun as one of the focal points.

Actually, all of the planet's orbits are ALMOST
circular. So this picture is a big-time exaggeration,
making the oval / elliptical orbit look a lot longer
than it is wide.

This exaggeration also makes the Sun look like it is
far to one side instead of, in reality, being pretty
darned close to the center!

We have to exaggerate in these sorts of diagrams,
or everybody would just say, "Oh! The orbit's a circle,
and the Sun is in the center!"

#2 - If there were a line that connected a planet to the Sun (rather like the "hand" of a clock), it would sweep out equal areas during equal intervals of time. This is because the planet moves slower when it is farther from the Sun and quicker when it is closer.



#3 - The square of the orbital period of a planet is directly proportional to the cube of the semi-major axis of the orbit.

Wh- wh- what?

This is a mathematical statement about the relationship between the distance of planets from the Sun and their orbital periods.

Remember, the closer something is to the Sun, the faster it moves. This is because the gravitational pull of the Sun is much stronger on nearby objects.

So not only does a far-away planet like Uranus have to travel a LOT farther to go aaaallllllll the way around the Sun than, say, Earth, it also travels more slowly. You can see how much longer it takes the far-away planets to travel once around the Sun in this chart:


Actually, this chart uses rounded-off measurements

of the years of the planets. To see a more accurate
list, check out this website.

By the way, if you are wondering what the semi-major axis of an orbit is, here is one more exaggerated diagram:



The major axis of an ellipse is a straight line that goes through
the widest part of the ellipse, traveling through both foci.
The semi-major axis is exactly half of that line.

Also on this date:









International Women's Day







Nametag Day

(Thursday of the first full week of March)


Girls Write Now Day











Fiesta of San Juan de Dios



 

Plan ahead:




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October 9 – Supernova!

Posted October 9, 2017


The largest explosions that take place in space are supernovas (also spelled supernovae). 

These are not common events. Even though there are about 100 BILLION stars in the Milky Way Galaxy, a supernova occurs only once every 50 years or so.

There are two reasons for this. First, most stars are pretty long lived - they last (by continuously fusing hydrogen) for a few million years to 10 billion years. Second - even more important! - less than one percent of stars become supernovas!!



Would it surprise you to know that a star explodes into a supernova about once every second? I know you're thinking, "Wait! I thought she said once every 50 years! Now she's saying once a second?"

Well, the first number (once every 50 years, approximately) is for our galaxy alone. But there are a LOT of galaxies - probably about 100 billion galaxies in the observable universe!

So there are probably around 1,000,000,000,000,000,000,000,000 stars in the observable universe! One percent of such a huge number is still huge: 

10,000,000,000,000,000,000,000

No wonder supernovas occur every second!

This is a color-enhanced photo
of the remnant left over from the
1604 supernova.
Why are we talking about such far-away events TODAY? Well, October 9, 1604, was the date of the first appearance of the most recent Milky Way supernova that people could see "with the naked eye."

This stellar eruption appeared in our skies in the constellation Ophiuchus, and it occurred in space only about 20,000 light years away from Earth.



Such a big explosion so nearby meant that this star became the brightest star in the night sky and was even visible during the day, for more than three weeks!

An Italian scholar was the first person to record his observation of the star. His name was Lodovico delle Colombe. The supernova was also recorded by Chinese and Korean astronomers / observers.
About 8 days after the supernova was first spotted, the German astronomer Johannes Kepler began to observe it. He tracked the star for more than a year, and he wrote a book about it. The supernova is often referred to by its date, Supernova 1604, but it is also known as Kepler's Supernova, Kepler's Nova, or even Kepler's Star.

By the way, although this supernova is the last one we are certain was in our galaxy that could be seen with the naked eye, we have been able to see supernovas in other nearby galaxies! (And when I say "nearby" - I mean near compared to most other galaxies! Trust me, these astronomical distances are mind-bogglingly far!)

One supernova that occurred during my lifetime is Supernova 1987A. It appeared in the Large Magellanic Cloud and was "easily visible" to the naked eye.



But the LMC is not visible from where I live in the Northern Hemisphere. Even worse, I live in Southern California, where the cities have conglomerated together into one big mega-city, and where the night sky is pretty darned polluted with light!

There aren't very many galaxies visible to the naked eye, but supernovas are such HUGE explosions, they can outshine their entire galaxy for a short time. A supernova explosion can radiate more energy than our Sun will in its entire 10-billion-year lifetime.

Crucially, supernovas are the main way in which heavy elements are created and spread out through the universe. If there were no supernovas, there would be no me to type these words, there would be no computer for me to type on, and there would be no you to read them!





Also on this date: