I Love Astronomy
Stardate
Feb, 5, 2013
Despite what we see in the movies, there aren't many "Eureka" moments in science -----
moments when a single discovery unlocks a big secret
Yet one such moment came 50 years ago today.
It soon led to the astonishing truth about some of the most powerful objects in the universe.
At the time, astronomers were perplexed by objects known as quasi-stellar radio sources.
But when astronomers looked at such a star's spectrum ---
it's individual wavelengths of light --- it wasn't star like at all.
There were none of the usual "footprints' of chemical elements found in stars.
That left a puzzle.
What could produce so much radio energy,
look like a normal star, but not be a normal star?
In 1962, astronomer Maarten Schmidt looked at one of these objects with the 200-inch telescope Palomar Observatory in California.
And in February of 1963 he realized something astonishing.
The object's spectrum did contain the fingerprints of chemical elements,
but they were shifted to longer wavelengths,
most likely by the object's motion through space.
The shift was so large that the motion was probably caused by the expansion of the universe itself.
That meant that an object that looked like a single star was about two billion light years away -- giving it the power of hundreds of billions of stars.
But it took a bit longer to understand the source of that power -- the power of a quasar.
Feb, 5, 2013
Despite what we see in the movies, there aren't many "Eureka" moments in science -----
moments when a single discovery unlocks a big secret
Yet one such moment came 50 years ago today.
It soon led to the astonishing truth about some of the most powerful ob
At the time, astronomers were perplexed by ob
But when astronomers looked at such a star's spectrum ---
it's individual wavelengths of light --- it wasn't star like at all.
There were none of the usual "footprints' of chemical elements found in stars.
That left a puzzle.
What could produce so much radio energy,
look like a normal star, but not be a normal star?
In 1962, astronomer Maarten Schmidt looked at one of these ob
And in February of 1963 he realized something astonishing.
The ob
but they were shifted to longer wavelengths,
most likely by the ob
The shift was so large that the motion was probably caused by the expansion of the universe itself.
That meant that an ob
But it took a bit longer to understand the source of that power -- the power of a quasar.