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  • 6 weeks ago
After Northern Lights appeared as far south as Colorado, Live Science discusses how "cannibal" coronal mass ejections (CME) are formed and what impact they have on Earth.
Transcript
00:00There are some beautiful auroras happening in the northwest of America right now.
00:04Yes.
00:05So like no scientists have given this a really, really simple explanation.
00:10And it's it's called like a cannibal coronal mass ejection.
00:14That's.
00:15That's the thing that's causing all of these auroras going on right now.
00:19Cannibal.
00:20Corona mass ejection.
00:22Yeah.
00:22That sounds a little terrifying.
00:24I mean, it's kind of.
00:25So funny, right?
00:25Because like just as soon as we get over one kind of Corona, we get hit by another.
00:28But like this.
00:30This one like a cannibal coronal mass ejection.
00:32Like if I break that down for you, it's called.
00:35Caused by sunspots.
00:36So there's a sunspot on the sun called like AR 297.
00:40Five right now.
00:40Okay.
00:41And what it's been doing over the last, say, like few days is.
00:45It's producing up to 17 solar eruptions, two of which.
00:50Um, were I have headed straight towards us.
00:52Now, one of them was traveling far.
00:55And the other, it was the one just like that came just after the.
01:00First one that was emitted now when those, when that second sun like.
01:05Coronal mass ejection caught up with the first, it cannibalized it.
01:09It's sweat.
01:10And then they wrapped it all up into this one big wave of like these, these charged particles.
01:14And then they all.
01:15Swept towards the earth.
01:16And then when they hit it, they caused a geomagnetic.
01:20Storm, what, where they come from in how sunspots are created is mag.
01:25Magnetic fields are created on the sun.
01:26Like the sun is just a giant ball of plasma.
01:29So like there's loads.
01:30loads of charged particles eddying and moving around on like inside the sun across the.
01:35Sun surface now, when you have charged particles moving, you're going to induce some magnetism there.
01:40But because magnetic field lines can't cross and you've got all these moving particles, let's.
01:45Giant traffic jam of particles moving everywhere, you'll inevitably get these field lines bunched up next.
01:50to each other, they'll form into these tight knots that can't escape anywhere else.
01:54And.
01:55Eventually, they will have to snap and release energy.
01:58Now they release energy either in the form of.
02:00solar flare, like a bright flare of radiation, or they'll release energy in the form of.
02:05like chucking out some of that plasma from the sun.
02:07What's the difference between solar.
02:10solar flares and ronal mass ejections.
02:11So solar flares is just the bright flash that you'll see.
02:15of radiation from that from that field line snapping that energy release across.
02:20solar flares and ronal mass ejection is some of the sun's like plasma soup actually being like burnt.
02:25out of the sun.
02:26I love that phrase plasma soup.
02:28Mm hmm.
02:29Yeah.
02:30Tasty.
02:30Tasty.
02:31It's been a nice.
02:32I mean.
02:33pretty.
02:34But.
02:35I mean.
02:35a little terrifying right i mean does it affect earth
02:39um
02:40so it does but not in like a so not in a
02:45in an always really terrible way most of
02:47the time
02:48the earth has a pretty strong
02:50magnetic field
02:50which is really really good news for us
02:52because it protects us from all of the
02:55these like highly energized particles
02:57that the sun has just spewed out at us
02:59um
03:00in this case at like speeds of like two
03:01million miles per hour which is just i
03:03guess
03:0333
03:05times less than the speed of light
03:06pretty quick
03:07um so what the earth's magnet
03:10field will do is it will absorb all of
03:13these particles the energy will
03:15go into stretching out the magnetic field
03:17in space
03:18so it's like it's kind of
03:20bunched out towards the it gives it a
03:22long tail
03:23um and then
03:25most of those particles will gather
03:27kind of towards the poles
03:29you
03:30where they will like go downwards
03:32and then energize some of the molecules
03:35in the atmosphere
03:35and when these when these um molecules
03:38in the atmosphere then give
03:39out
03:40light
03:40um
03:41to in order to kind of go down to a
03:42lower energy level
03:43that's what why
03:45we see the aurora
03:46now because there's so many of these
03:48like particles coming in
03:50you're getting auroras much lower down
03:52um along the northern hemisphere
03:55than you would normally expect to see
03:56that's that's that's that's a pretty
03:59that's
04:00that's a nice effect there um and i
04:02know that
04:03uh people had already taken video
04:05from it
04:05uh this is from manitoba in canada
04:10yeah beautiful just absolutely beautiful
04:13yeah yeah yeah and like
04:15like i think also you could see the aurora in
04:17the u.s certainly like as far south as
04:19pennsylvania
04:20iowa and oregon over the last two days as well
04:22oh right on uh space
04:25weather.com that you guys were sharing
04:27information from uh they showed some
04:30pictures purple i mean purple what a what an aura
04:34that earth is giving
04:35giving off of this aurora and you know i uh
04:40when you mentioned polls i'm like that's why
04:42they're always up there towards yeah we got
04:44to get close
04:45citizen polls then yeah but so okay so that's
04:48the good one
04:50but uh how about damage
04:52okay yes
04:55so damage um so they can cause damage so
05:00one of the most recent kind of power outages that
05:02was caused by a storm of this time
05:05fight was um in the was the 1989 quebec power
05:09cut which was called
05:10by a geomagnetic storm
05:11now most of the time especially when it comes to people who provide
05:15like power lines and stuff a lot of them have shielded like their their their like power
05:20cables and things like that with a kind of
05:22faraday cage basically which diverts the
05:24energy
05:25or they also have like other techniques that allow them to kind of siphon off excess energy
05:30that might be given to power lines by storms like this okay but like that hasn't
05:35always been the case like especially back in 1859 there was a really big event called
05:39the court
05:40great carrington event um which was the largest sort of solar storm in modern human
05:45history i'm sure there have been solar storms uh just as large throughout uh
05:57you
05:50our past but like before that point we weren't really documenting it and we didn't have many
05:54electronics
05:55electronics around so we didn't really care um but in this case the great carrington
06:00event fried most of the telegram systems in the u.s and in europe
06:05had been developed at the time and it also led to auroras that could be
06:10seen around like as far south as the as the caribbean um and like there were people waiting
06:15waking up at night thinking that like thinking that it was daytime in the caribbean
06:20because of these enormous auroras from this event i mean we were freaked out about
06:25it now when we see things like that we know more but i can't even imagine you know over 100 years
06:30ago yeah yeah exactly in terms of um more modern sort of phenomena
06:35phenomena that have caused more modern damage other than the quebec event um recently
06:40actually there was another geomagnetic storm that caused the downing of um 40
06:45like 40 of spacex's starlink satellites that was one thing that happened um
06:50um and on top of that as well there's a potential risk um that
06:55that internet like the internet in general especially in the united states
07:00could be cut out by a geomagnetic storm because a lot of these cables run underwater
07:05through like like latitudes that would be affected by it and like
07:10like you would have a geomagnetic storm they're not shielded so they would basically be
07:15probably quite severely affected by this but as is the case with a lot of things and how
07:20they're done with legislation it's like earthquakes it doesn't often get legislated for until
07:25the worst has already happened yeah that's a shame i mean i really like the internet i really i like
07:30i like to keep it around this is how we get to communicate right
07:35um but but you're saying that we have protections now so
07:40so most i think most like power companies have already built in protections into their
07:45grids for these kind of things it's just yeah you're not going to be getting any like um
07:50i guess coronal mass ejection memes in the middle of a coronal mass ejection you have to wait a few
07:54weeks for them to fix
07:55to step out the underwater cables yeah and and luckily earth you know we have
08:00this nice electromagnetic shield right already built in otherwise we'd be you know goners
08:05yeah it would fry us and it would also fry our atmosphere like a big reason why mars doesn't have much
08:10an atmosphere for instance it doesn't really have very active um magnetic fields
08:15so all of those all of the atmosphere when when it gets hit by this these wave of like
08:20hydrogen like particles protons um like the atmosphere gets stripped away quite
08:25quickly poor mars poor mars yeah but that's why we're here right we're not
08:30we're not we're not i mean we are on mars but you know yeah yeah not yet not yet not yet well
08:35so is there a way to know when things like this will happen
08:40i know we watch the sun we have video of the sun it seems more like after the fact
08:45yeah so you get a bit of advanced warning like for instance
08:50great carrington event is named after richard carrington who spotted like intense solar flares
08:55in the sky like a few like a few hours like maybe about 15 hours
09:00before the actual like event hit but the sun is quite a complex
09:05object like there's loads going on in those magnetic fields it's still really really hard for scientists
09:17you
09:10predict what's going on there yeah if only if only if only well
09:15until until until the next major astronomical event thanks so much ben thank you
09:20you
09:25you
09:30you
09:35you
09:40you
09:40you
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