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What Is A Quasar?
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The sky that we watch every night is full of thousands stars. But in reality, what we see with our naked eye is just a tiny part of the Universe. In reality, the Universe is so big that most of the distant objects are not visible to us. However, certain objects are so powerful that despite their immense distance from us, we are still able to detect them (although only using telescopes). I’m talking about quasars, or “quasi-stellar radio sources”. Do you want to know what they are? Watch this video and I will tell you more!
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The discovery of quasars dates back to the 1950s, and it’s interesting to look at the history of their first observations.
In the 1950s, astronomers started to look at the sky using radio telescopes for the first time. Radio telescopes, contrary to normal telescopes, detect radio waves instead of visible light. When astronomers first started to “watch” the sky with these instruments, they were surprised to find several objects emitting a large amount of radio waves, but almost no visible light. In fact, most of these sources of radio waves did not correspond to any known visible object.
The first quasar ever discovered was 3C 273, a weird name indicating the 273rd object in the Third Cambridge Catalog of Radio Sources (3C). It was discovered thanks to a “lunar occultation”, an event that occurs when the Moon passes between an object and the Earth, hiding the object to our view. In 1959, a group of astronomers at the Cambridge University identified a radio source in the sky (3C 273), but they couldn’t find an optical counterpart to it. Three years later, in 1962, John Bolton and his Caltech radio astronomy group used the Parkes radio telescope to realize a series of observation of the sky during which the Moon was passing in front of the radio source discovered three years earlier. Thanks to these lunar occultations, Bolton and his group were able to calculate the location of the source with precision. And more importantly, they were able to associate it to a visible counterpart, a faint stellar object.
Later on, new quasars were discovered. Generally, their position in the sky matched with very faint objects, like very distant stars: that’s why they were called quasars, a contraction of “quasi-stellar” (star-like) and “radio source”. However, the chemical composition of these objects observed by looking at their spectral lines was very different from any known star. Also, the amount of radiation emitted by them was too large in order to be normal stars.
The observation of these quasars continued throughout the years. By observing their radiation spectrum, scientists found out that these objects were moving very fast and away from the Earth. This could be inferred thanks to a phenomenon known as “redshift”. What is it?
Every object in the sky emits radiation in a broad range of frequencies – and even in the visible part of the spectrum, which consists of different colours: violet, blue, green, yellow, orange and red. The colour that our eye perceives depends on the frequency of the light that we observe: violet corresponds to the highest frequency, while red corresponds to the lowest one. While the light emitted by an object in the sky contains a mix of different frequencies, it has a peak at a certain colour. If we look at the sky, in fact, we notice that some stars appear red, while others appear blue.
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Credits: Ron Miller
Credits: Nasa/Shutterstock/Storyblocks/Elon Musk/SpaceX/Esa
Credits: Flickr
Video Chapters:
00:00 Introduction
00:43 What is a Quasar?
03:06 Redshift
06:31 Quasars and Black Holes
08:17 Observing Quasars
#insanecuriosity #quasars #howtheuniverseworks
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-------------------------------------------------------------------------------------------
The discovery of quasars dates back to the 1950s, and it’s interesting to look at the history of their first observations.
In the 1950s, astronomers started to look at the sky using radio telescopes for the first time. Radio telescopes, contrary to normal telescopes, detect radio waves instead of visible light. When astronomers first started to “watch” the sky with these instruments, they were surprised to find several objects emitting a large amount of radio waves, but almost no visible light. In fact, most of these sources of radio waves did not correspond to any known visible object.
The first quasar ever discovered was 3C 273, a weird name indicating the 273rd object in the Third Cambridge Catalog of Radio Sources (3C). It was discovered thanks to a “lunar occultation”, an event that occurs when the Moon passes between an object and the Earth, hiding the object to our view. In 1959, a group of astronomers at the Cambridge University identified a radio source in the sky (3C 273), but they couldn’t find an optical counterpart to it. Three years later, in 1962, John Bolton and his Caltech radio astronomy group used the Parkes radio telescope to realize a series of observation of the sky during which the Moon was passing in front of the radio source discovered three years earlier. Thanks to these lunar occultations, Bolton and his group were able to calculate the location of the source with precision. And more importantly, they were able to associate it to a visible counterpart, a faint stellar object.
Later on, new quasars were discovered. Generally, their position in the sky matched with very faint objects, like very distant stars: that’s why they were called quasars, a contraction of “quasi-stellar” (star-like) and “radio source”. However, the chemical composition of these objects observed by looking at their spectral lines was very different from any known star. Also, the amount of radiation emitted by them was too large in order to be normal stars.
The observation of these quasars continued throughout the years. By observing their radiation spectrum, scientists found out that these objects were moving very fast and away from the Earth. This could be inferred thanks to a phenomenon known as “redshift”. What is it?
Every object in the sky emits radiation in a broad range of frequencies – and even in the visible part of the spectrum, which consists of different colours: violet, blue, green, yellow, orange and red. The colour that our eye perceives depends on the frequency of the light that we observe: violet corresponds to the highest frequency, while red corresponds to the lowest one. While the light emitted by an object in the sky contains a mix of different frequencies, it has a peak at a certain colour. If we look at the sky, in fact, we notice that some stars appear red, while others appear blue.
-------------------------------------------------------------------------------------------
Credits: Ron Miller
Credits: Nasa/Shutterstock/Storyblocks/Elon Musk/SpaceX/Esa
Credits: Flickr
Video Chapters:
00:00 Introduction
00:43 What is a Quasar?
03:06 Redshift
06:31 Quasars and Black Holes
08:17 Observing Quasars
#insanecuriosity #quasars #howtheuniverseworks
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