As I have written in my previous post, Edwin Powell Hubble expanded our understanding of the
universe by calculating the distance of Andromeda using Cepheid Variable stars
using 100 inch Hooker telescope at Mount Wilson. It was believed that it’s a nebula
like many others inside our own galaxy but he calculated that its distance is
90,000 light years from earth.
Later Walter Baade
studied the RR Lyrae stars using the same telescope. RR Lyrae are also variable
star similar to Cepheids but less luminous. It was shown before that like
Cepheids, the variability of RR Lyrae stars can be used to measure distances.
The movie shows RR Lyrae stars in a globular cluster. You
can see their brightness changing; they look blue as they become brighter.
astro.princeton.edu |
Walter
Baade wanted to use these stars to measure the distance of Andromeda as it was
done before using Cepheids. But the 100 inch telescope was not good enough to
detect those stars. So he had to wait until the 200 inch (~5 meter) telescope was
ready which was being built by George Hale but sadly he died two years after
the project started. Later the telescope was named after him.
When the new Hale telescope became operational Baade used
the telescope to search the faint variable stars in Andromeda but even after
searching for a long time he was not able to find any sign of these stars.
He concluded that the only possible reason for this can be
the distance of Andromeda previously measured is not correct!
At that time it was becoming evident that stars can be categorized
into two broad types called populations. Older stars fall in Population2 and
younger and brighter stars in Population1.
So Baade assumed that Cepheid variable stars will also have
two different types. Thus he reasoned his argument that the previously measured
distance of Andromeda was wrong using two points,
1.
Population1 Cepheids are brighter than
Population2 Cepheids.
2.
Astronomers only saw the brighter Population1
stars in Andromeda and compared it to the dimmer population2 stars in Milky Way.
That’s what lacked in the calculations made by Hubble. And
that’s why he measured the distance of Andromeda little less.
Baade calculated that Population1 stars are on average 4
times more luminous than Popluations2 stars of same period of variations. So if
a star is moved twice as far away it will appear 4 times fainter. Thus Andromeda
Galaxy should be twice as far away - approximately 2 million light years away!
More accurately,
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