Showing posts with label Hubble. Show all posts
Showing posts with label Hubble. Show all posts

November 20 - Happy Birthday, Edwin Hubble

  Posted on November 20, 2021


This is an update of my post published on November 20, 2010:



Born on this day in 1889 in Missouri, Edwin Hubble soon moved with his family to Illinois. This early move perhaps presaged a varied and movement-filled life.

As a high school student, Hubble was into sports, especially track and field, and he set his state's high-jump record in 1906. In college he studied philosophy and science, and he got a Bachelor of Science degree, but then he went to Oxford University in England to study law and to get a master's degree in Spanish!

Hubble taught Spanish, physics, and math in a high school in Indiana, coached basketball, and passed the Kentucky bar (which would have allowed him to practice law in that state). Instead he entered the U. S. Army during World War I.


Home from the war, Hubble enrolled in a doctorate program in astronomy, and in 1917 he earned his PhD in that subject. Today we know Hubble from his career in astronomy. Still, that career focused on movement.


Hubble's biggest contribution was the demonstration that there were galaxies other than our own Milky Way, and that these galaxies are shooting away from each other at tremendous speeds. In other words, Hubble showed that the universe is huger than most had ever imagined, and that it was expanding.


Most people today are familiar with the name Hubble because of the space telescope that was named after him.

Extra-galactic Astronomy

One reason I am excited about Hubble is that he did some of his most important work pretty much where I grew up, at the Mount Wilson Observatory, which is very, very near my childhood home of Pasadena, California.



The other reason I am excited about Hubble is that he pretty much created an entire science—the study of stuff outside of our galaxy. (“Outside of our galaxy” is what extra-galactic means.)

There is a type of variable star whose behavior is very predictable, and we can deduce the distance of these stars simply by measuring their apparent brightness. (Obviously, if two stars were exactly the same size and temperature, the closer star would appear to be brighter.) In 1923 Hubble identified two of these Cepheid variable stars whose distances proved that they lay far outside our galaxy. They were part of what were then known as spiral nebulae. Hubble showed that these spiral features were not spiral-shaped clouds of gas and dust inside our Milky Way Galaxy, but were instead large, far-away spiral-shaped galaxies made up of billions of stars.

Hubble eagerly collected data from other Cepheid variable stars and discovered that, the farther away they were from our galaxy, the faster they and the galaxies they are a part of seemed to be moving away. This relationship, called Hubble's Law, can be explained by the idea of an expanding universe with a beginning known as the Big Bang.



For information on how we know the speed at which galaxies and other astronomical bodies are moving, check out this earlier post. 

Some links...

Here is a demonstration of the expanding universe that you can try at home. 

And here is a video about cosmology, the Big Bang, and other topics that will expand your head!

Here is a NASA site with some info about the Big Bang and the expanding universe.

There's a lot of Big Bang Theory stuff on the internet, but most of
it is about a popular TV show that ran from 2007 to 2019.





(Third Saturday of November)



(Third Saturday of November)








Family Volunteer Day

(Saturday before Thanksgiving)





December 30 – Another “Island Universe” Is Announced

Posted on December 30, 2014

We Earthlings are not alone in our endless circuits around the Sun – there are seven other planets and vast numbers of other celestial bodies circling our star, making up our Solar System.

We Solar System-ites are not alone in our rush through space – our sun is but one of 100 BILLION stars in a vast, turning pinwheel in space, our Milky Way Galaxy.

Well, on this date in 1924, astronomer Edwin Hubble announced the discovery that a small smudge in our skies – what had been considered a spiral-shaped nebula (cloud of dust and gas in space) inside the Milky Way – was in fact another entirely-separate galaxy!

In other words, the Andromeda Nebula had to be renamed the Andromeda Galaxy.

Because the newly discovered independent galaxy was 2-and-a-half billion light years away from our galaxy, it seemed obvious that it was like another island in an ocean of empty space. Hubble referred to it as another “island universe.” He and other scientists immediately wondered if all the other known spiral nebulae are also separate galaxies, and of course it turns out that the ocean of space is dotted with many island universes.

(We now use the word universe to mean everything we can observe in the cosmos. And we use the word galaxy to mean a group of stars that, along with gas and dust and black holes and such, are held together by gravitational attraction.)

It turns out, indeed, that there are at least 100 billion galaxies in the universe! Here are a few of my favorites:


I guess you can say that, on this date in 1924, our known universe got a whole lot bigger!


How did he do that?

I hope you noticed that Hubble was not the first to actually see the Andromeda galaxy; instead, he was just the first to understand what it was: not a cloud of dust and a few stars within the Milky Way Galaxy, but its own separate collection of billions of stars and dust well outside the Milky Way.

The key to Hubble's discovery was figuring out how far away Andromeda really was. An astronomer named Henrietta Leavitt had figured out that a certain kind of variable star – a Cepheid variable – has a set ratio between its maximum brightness and the period of its brightness changes. A Cepheid that is quite close to us looks brighter than a Cepheid that is far (just as a nearby candle seems brighter than a distant candle), so we can use the dependable ratio to compute how far away the Cepheid is.

In other words, Leavitt's careful observations and analysis meant that we now had a measuring stick to use in space! And Hubble had to do some very careful observation and analysis to detect Cepheids as far away as those in Andromeda. But he succeeded in detecting some – hence his discovery we honor today!

This is what happens when
galaxies collide.


Also on this date:













































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November 20, 2010



Happy Birthday, Edwin Hubble

Born on this day in 1889 in Missouri, Hubble's family soon moved with him to Illinois. This early move perhaps presaged a varied and movement-filled life.

As a high school student, Hubble was into sports, especially track and field, and he set his state's high-jump record in 1906. In college he studied philosophy and science, and he got a Bachelor of Science degree, but then he went to Oxford University in England to study law and to get a master's degree in Spanish!

Hubble taught Spanish, physics, and math in a high school in Indiana, coached basketball, and passed the Kentucky bar (which would have allowed him to practice law in that state). Instead he entered the U. S. Army during World War I.

Home from the war, Hubble enrolled in a doctorate program in astronomy, and in 1917 he earned his PhD in that subject. Today we know Hubble from his career in astronomy. Still, that career focused on movement.

Hubble's biggest contribution was the demonstration that there were galaxies other than our own Milky Way, and that these galaxies are shooting away from each other at tremendous speeds. In other words, Hubble showed that the universe is huger than most had ever imagined, and that it was expanding.

Most people today are familiar with the name Hubble because of the space telescope that was named after him.

Extra-galactic Astronomy

One reason I am excited about Hubble is that he did some of his most important work pretty much where I grew up, at the Mount Wilson Observatory, which is very near my childhood home of Pasadena, California.

The other reason I am excited about Hubble is that he pretty much created an entire science—the study of stuff outside of our galaxy. (“Outside of our galaxy” is what extra-galactic means.)

There is a type of variable star whose behavior is very predictable, and we can deduce the distance of these stars simply by measuring their apparent brightness. (Obviously, if two stars were exactly the same size and temperature, the closer star would appear to be brighter.) In 1923 Hubble identified two of these Cepheid variable stars whose distances proved that they lay far outside our galaxy. They were part of what were then known as spiral nebulae. Hubble showed that these spiral features were not spiral-shaped clouds of gas and dust inside our Milky Way Galaxy, but were instead large, far-away spiral-shaped galaxies made up of billions of stars.

Hubble eagerly collected data from other Cepheid variable stars and discovered that, the farther away they were from our galaxy, the faster they and the galaxies they are a part of seemed to be moving away. This relationship, called Hubble's Law, can be explained by the idea of an expanding universe with a beginning known as the Big Bang.

For information on how we know the speed at which galaxies and other astronomical bodies are moving, check out this earlier post. 

Some links...

Here are some demonstrations that speak to some aspects of modern astronomy, including the concept of the expanding universe. 

And here is a T-shirt about the expanding universe. 

Here is a NASA site with a short talk about the expanding universe.