New type of Supernova explains ancient mystery
bigthink.com
bigthink.com
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On 2018 March 2.49 (UT dates are used throughout), we dis-covered AT 2018zd13 at an unfiltered optical magnitude of 17.8 in the outskirts of NGC 2146... Combined with our pre-discovery detection at 18.1 mag on 2018 March 1.54, we estimate an explosion epoch of 2018 March 1.4 ± 0.1 (~3 h before the first detection;
I'm not entirely sure I understand the date/time format, but the last part suggests that TFA meant "We pointed our telescope at it when the explosion was already in progress. We think it had been going for about three hours at that point."I think "March 2.49" means ".49 of the way through March 2", so 11:46 AM, but that's just a guess. I've never seen that before. If so, that "first detection" was at 12:58PM on March 1, and they figure it actually started at 9:36AM... about three hours earlier.
Which means there's no such thing as "how much time it takes light to travel from the Sun to Earth". It takes no time at all. Yet we do say "8 minutes 20 seconds". Everyone would claim that's the correct answer. In which case at the point of detecting this light on Earth, if someone asks us "when did the event of it leaving the Sun occur" you'd obviously say "8 minutes 20 seconds ago".
So while there's no true universal "when it happened", we're all here on Earth and we've developed a certain way of expressing ourselves about time and light, and broadly speaking we're all sharing a relative point of view in spacetime, relative to something 31 million light years away.
So to say "we detected it 3 hours after it happened" when it happened 31 million lights away would be poorly written, simply put.
In the reference frame of earth it is 31 mio years. In frames that move faster and faster to the speed of light, relative to ours, this would take less and less time, an effect known as time dilation.
Obviously the article means that 3 hours after the first photons of this event reached earth (and we see it as happened), we managed to aim our sensors towards it and start measuring. It looks a bit clumsy indeed.
This has been an open issue for a while.
I'd think to simulate you basically need to prevent the electrons from going anywhere, and the only place to go is inside the nucleus, where the strict rules of quantum mechanics and particle physics dictate they get merged with protons to form neutrons.
Do we have anything besides tokamaks for smushing things together? Tokamaks seem to peak out at low-energy fusion reactions, but all I read about tokamaks is engineering focused on net-positive fusion.
The core of a star is already very hot and further collapse raises the temperature, so we’re probably talking about photodisintegration of any heavy nuclei into alpha particles, as electron capture process runs.