Tuesday, January 23, 2024

4324 - BLACKHOLE - or neutron star detected?

 

-    4324  -  BLACKHOLE  -  or neutron star detected?  -    The supernova observed is “SN 2022jli”  This occurred when a massive star died in a fiery explosion, leaving behind a compact object which is a neutron star or a black hole.


--------------------  4324 -  BLACKHOLE  -  or neutron star detected?

-    This dying star had a companion which was able to survive this violent event. The periodic interactions between the compact object and its companion left periodic signals in the data, which revealed that the supernova explosion had indeed resulted in a compact object.

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-    The explosive deaths of supermassive stars, supernovae,  lead to the creation of black holes or neutron stars? At least, that’s the evolutionary path that astronomers suggest happens. And, these compact objects exist throughout the Universe. But, no one’s ever seen the actual birth process of a neutron star or black hole in action before.

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-    That changed when supernova “SN 2022jli“  occurred in the nearby galaxy “NGC 157”. This catastrophic star death event was discovered in May 2022.   Observations were made from the European Southern Observatory’s Very Large Telescope and New Technology Telescope provided high-quality light-curve measurements.

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-  The supernova explosion ended up creating a massive compact object.  Until now, no one has observed the process happen in (almost) real-time. That makes the light curve a useful window on the creation of either a neutron star or a black hole.

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-   Astronomers wanted to establish a direct connection between the death of a massive supergiant star and the creation of the object.   In “SN 2022jli”  data there was a repeating sequence of brightening and fading.   This is the first time that repeated periodic oscillations, over many cycles, have been detected in a supernova light curve.

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-    Supernovae occur pretty frequently in the Universe. Astronomers study them and chart how their brightness changes over time. After the initial explosion, the light it generates fades out over some time. Usually, it’s a smooth change in the light curve. But, SN 2022jli didn’t fit the “normal” curve. Instead of fading out smoothly, the brightness of light from the explosion oscillated in a 12-day-long period.

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-     A rapidly spinning neutron star (a pulsar) at its heart, surrounded by material rushing out from the site of the explosion.   SN 2022jli could have either a neutron star or a black hole orbiting with a companion star.

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-    What story does SN 2022jli’s strange light curve tell us about the creation of black holes or neutron stars?    The explosion itself was a fine example of what astronomers call “Type II supernovae”.    At the end of its life, a supermassive star collapses and then explodes outward. The remaining core collapses further to create one of two types of massive objects.

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-    A neutron star is one. It’s what’s left over after the rapidly collapsing core of the star crushes the remaining protons and neutrons of matter into neutrons. It’s essentially a ball of neutrons. Most neutron stars have about the mass of the Sun crushed inside themselves. But, they are small compared to their progenitor stars. Most are 20 kilometers across.

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-   Stellar-mass black holes also come from the deaths of supermassive stars that were at least 20 times the mass of the Sun or more. The core collapses during the event, the same as with a neutron star. But, the mass is so great that the event creates a black hole, crushing all the leftover core material into a pinpoint of dense matter.

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-    Like many massive stars, the progenitor of SN 2022jli appears to have had at least one companion star. It probably survived the supernova explosion. The outburst threw out huge amounts of material, and the companion star interacted with it. That caused its atmosphere to “puff up”.

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-    The newly created compact object passes through the orbit of the star and sucks hydrogen gas away from the star. That material funnels into an accretion disk around the compact object. Those periodic episodes of matter theft from the star release lots of energy, which gets picked up as regular changes of brightness in the light curve measurements as well as the gamma-ray signals.

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-    We can’t see light coming from the compact object itself, whether it’s a neutron star or a black hole. But, we do see radiation from the heated material drawn into the accretion disk around the compact object. And, since astronomers were able to track the changes in the light curve due to activity by the massive object, it amounted to watching its formation.

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-   Exactly what astronomers saw being formed?   Was it a neutron star with tremendously strong magnetic fields and gravity, or a black hole with gravity so strong nothing (not even light) could escape it?  What do you think?

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January 21, 2023     BLACKHOLE  -  or neutron star detected?              4324

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--------------------- ---  Tuesday, January 23, 2024  ---------------------------------

 

 

 

 

 

           

 

 

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