Showing posts with label galaxy. Show all posts
Showing posts with label galaxy. Show all posts

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:

July 4 – Happy Birthday, Henrietta Swan Leavitt

Posted on July 4, 2015

The American astronomer Henrietta Swan Leavitt was born waaayyy back on this date in 1868, and yet she is the one who discovered an important “measuring stick” that allowed us to better understand the enormity of the universe.

And this “measuring stick” was made of stars!

Did you know that some stars do not shine steadily? Instead, some stars seem to flicker or even to wildly fluctuate with brighter and then dimmer light. The changes in brightness reflect eruptions within the star itself or the in-falling of material from a nearby companion.

They are called variable stars.


Some variable stars are called Cepheid variables. They pulsate at a regular pace, changing in both size and temperature. Their brightness varies along with the size-and-temperature changes. And, it turns out, there is a strong direct relationship between a Cepheid variable's luminosity and pulsation period.

Because of this, we can discover how far away a Cepheid variable star is. We measure its brightness and its pulsation period. Then we figure out how bright it SHOULD be, if we were near it. Voila! We can now compute how far away the Cepheid variable must be to make it appear at the brightness we observe.



It is Leavitt who discovered the relationship between the luminosity and period of Cepheid variables. Her discovery gave astronomers their first way of measuring the distance between the Earth and faraway galaxies, and it was her discovery (and red shifts) that enabled Edwin Hubble to discover that the universe is expanding. And of course, once we discovered the expansion of the universe, we were able to reason that the universe must have started with a Big Bang.

Leavitt was born in Massachusetts. She attended Oberlin and Radcliffe Colleges and then traveled in America and in Europe. During those post-graduate travels, she got ill and lost her hearing. However, she was still able to get a job as a human “computer” working for Edward Pickering at the Harvard College Observatory to measure and catalog the brightness of stars in the observatory's collection of photographic plates.

How did Leavitt make her discovery? She made the assumption that all the Cepheid variable stars in the Magellanic Clouds were roughly the same distance to the Earth. That's sort of like saying that every mountain and crater on the Moon is roughly the same distance from your house. It's not completely true – some of the deepest craters are some tens of thousands of feet “farther away” from your house than some of the mountain tops on the Moon. But compared to the more than one BILLION feet away that the moon is from Earth, that distance is like nothing. (The difference between the lowest and highest spots on the Moon is only about 0.0047% of the distance between the Earth and the Moon.)

Large Magellanic Cloud -
it's really a small, relatively
nearby galaxy.
So, in the same way, we can talk about a group of stars that are very far away from the Earth – such as all the stars in another galaxy – being roughly the same distance away from us. The Large Magellanic Cloud is about 160,000 light years away from us, and the Small Magellanic Cloud is about 200,000 light years away from us. And each light year is about 1,000,000,000,000 miles or kilometers away. So that makes the Magellanic Clouds some 160,000,000,000,000,000 to 200,000,000,000,000,000 miles away!

(Pretty far!)

Interestingly enough, I discovered that recent, more exact studies of the Magellanic Clouds have resulted in fine-tuning Leavitt's assumption. We now think that, based on more exact measurements of the light of Cepheid variables, the Large Magellanic Cloud is tipped 35 degrees, so that the northeast part of the galaxy is slightly closer to our galaxy than the southwest part. That's what I love about science: we just keep getting better and better at discovering and describing reality!

I bet you have already guessed this part: Leavitt got less recognition for her very important discovery than we would like. Someone tried to nominate her for a Nobel Prize, but that prize is never awarded after someone's death, and at that point Leavitt had already died of cancer. Hubble, who enjoyed quite a bit of fame, always said that Leavitt should've gotten a Nobel for her work.

So, not too much fame. Did Leavitt earn fortune? Well, she had money because of her family, so at first she wasn't even paid for her work for the Harvard Observatory; later she earned about 30 cents an hour (woo-hoo!).

Leavitt has gotten SOME credit, now that she is long gone. There is a Leavitt asteroid and a Leavitt crater on the moon. And Leavitt's story has been shared in books and in Neil deGrasse Tyson's Cosmos. I think maybe all of us should spread the word – Henrietta Swan Leavitt made a great contribution to astronomy despite being deaf (AND female, back when that was a hurdle to overcome)!


Also on this date:
























Indivisible Day



























Plan ahead:

Check out my Pinterest boards for:
And here are my Pinterest boards for: