1 00:00:02,266 --> 00:00:05,000 JOHN YANG: Itús been an exciting time for astronomers, astrophysicist and other scientists 2 00:00:07,033 --> 00:00:09,766 who specialized in the goings on in the far reaches of space. Since the beginning of the month 3 00:00:09,766 --> 00:00:14,766 observations of some never before seen celestial events have been reported in science journals. 4 00:00:16,433 --> 00:00:19,133 Science correspondent Miles OúBrien is here to explain all. Miles, 5 00:00:19,133 --> 00:00:24,133 thanks for joining us. The first one is a star swallowing up a planet that was orbiting around 6 00:00:26,000 --> 00:00:30,166 it. And as you talk about, weúre going to show some animation from Caltech depicting, 7 00:00:30,166 --> 00:00:35,166 MILES OúBRIEN: Well, John, I donút want to ruin your weekend. But this is in fact a preview of 8 00:00:37,700 --> 00:00:42,666 what lies ahead for our little planet Earth. A team of researchers at Palomar Observatory 9 00:00:44,700 --> 00:00:49,333 outside San Diego, were using a Wide Field Camera called the Zwicky Transient Facility, 10 00:00:51,300 --> 00:00:55,433 which looks at a big swath of the night sky looking for things like comets and asteroids. 11 00:00:56,900 --> 00:01:01,866 Astronomer Kishalay De at MIT, is going through data from 2020. 12 00:01:03,866 --> 00:01:06,933 Thereús so much data that they have a backlog, and he noticed a star about 13 00:01:08,533 --> 00:01:12,400 12,000 light years away that grew 100 times brighter over the course 14 00:01:12,400 --> 00:01:17,400 of a week. He thought maybe that was a binary star, which he studied quite a bit two stars, 15 00:01:19,966 --> 00:01:23,400 which kind of interact with each other. And their brightness changes as the gravity pushes in polls. 16 00:01:23,400 --> 00:01:27,166 But the problem was the total amount of energy that was released by this event 17 00:01:27,166 --> 00:01:32,166 was way less than it would be if it was two stars. And so that meant by virtue of that, 18 00:01:34,233 --> 00:01:38,300 that it was probably a black hole swallowing up a planet, but itús not just any planet 10 times 19 00:01:40,900 --> 00:01:44,633 bigger than Jupiter. And I guess the flash that he saw, I guess it amounts to a Cosmic Belt, John. 20 00:01:48,133 --> 00:01:50,300 JOHN YANG: You say this is going to happen to earth. 21 00:01:50,300 --> 00:01:54,433 Does this happen to all planets? Do they eventually sort of go into their sons? 22 00:01:54,433 --> 00:01:58,466 MILES OúBRIEN: Not all of them I gather planets in our solar system are likely to 23 00:01:58,466 --> 00:02:03,433 be spared. And weúre kind of on the bubble. We know Venus and Mercury theyúre goners 24 00:02:05,100 --> 00:02:07,533 eventually. Thereús some scientific debate as to what will happen to us. 25 00:02:07,533 --> 00:02:11,866 But basically, the star gets bigger and bigger as it gets older, like we all do, 26 00:02:11,866 --> 00:02:16,866 I suppose, and gets hotter, and eventually gobbles up the near planet. So Iúm sorry 27 00:02:19,433 --> 00:02:24,433 to give that piece of news to everybody here this weekend. But we have some time to plan. 28 00:02:26,066 --> 00:02:28,000 JOHN YANG: Youúve given us a lot of lead time. The next thing I want to 29 00:02:28,000 --> 00:02:31,600 ask you about is the largest space explosion ever detected. 30 00:02:31,600 --> 00:02:36,600 MILES OúBRIEN: This one is very far away 8 billion light years away. So that means what 31 00:02:38,533 --> 00:02:42,366 weúre seeing in these images or animations, or data is at about 6 billion years after the 32 00:02:44,366 --> 00:02:48,833 creation of the universe, the Big Bang. This explosion lasted about three years. 33 00:02:50,700 --> 00:02:55,033 So what was it? No oneús really sure. The current thinking is that maybe the black 34 00:02:57,100 --> 00:03:01,566 hole in this case, much more powerful than ours swallowed up a huge gas cloud and in 35 00:03:03,466 --> 00:03:07,866 so doing created this multi-year explosion. So again, the universe is rough place, John. 36 00:03:09,700 --> 00:03:14,633 JOHN YANG: Tough neighborhood. Thereús also a neutron star that is behaving in 37 00:03:16,633 --> 00:03:19,066 a way that scientists didnút think a star could behave. And first of all, 38 00:03:19,066 --> 00:03:21,566 start off by telling us what a neutron star is. 39 00:03:21,566 --> 00:03:26,266 MILES OúBRIEN: Itús like a dead star didnút quite make it to black hole status. But a 40 00:03:26,266 --> 00:03:31,000 neutron star is very, very dense object. There are limits to how bright they can 41 00:03:31,000 --> 00:03:35,333 become. Itús called the Eddington limit, little bit of physics here, but basically, 42 00:03:35,333 --> 00:03:40,333 itús a push and pull between the light photons and gravity. And the physicists would tell you 43 00:03:42,300 --> 00:03:45,500 that given the size of any particular object, thereús a limit to how bright it can be. 44 00:03:47,466 --> 00:03:50,533 But this one turns out is 100 to 500 times brighter beyond this so called Eddington limit. 45 00:03:53,200 --> 00:03:58,200 And they think whatús happening here is that the magnetic field at this particular neutron star is 46 00:04:00,800 --> 00:04:05,600 actually warping the atoms and allowing that star to hold together longer than it would otherwise. 47 00:04:08,100 --> 00:04:12,766 So thatús a little bit mind-bending and actually literally add embedding. But there you have it. 48 00:04:12,766 --> 00:04:17,766 JOHN YANG: This is all mind-bending to me. The closest instance of a black hole tearing apart 49 00:04:19,766 --> 00:04:23,100 a star, remind us or describe what a black hole is. And weúll play some animation from NASA. 50 00:04:25,133 --> 00:04:28,366 MILES OúBRIEN: Yeah, these are huge gravity wells that are at the center of most galaxies 51 00:04:30,300 --> 00:04:33,600 is one of the center of ours. This one, they say close in astronomical terms, 52 00:04:33,600 --> 00:04:38,600 itús 137 million light years away from Earth. And we know about these tidal disruption events, 53 00:04:40,966 --> 00:04:45,966 which create this thing, what my favorite astronomical term spaghettification, 54 00:04:47,866 --> 00:04:51,433 it pulls things in so rapidly that they stretch out spaghetti style. 55 00:04:53,933 --> 00:04:56,900 And this was the closest one weúve seen. But as you look at this animation that NASA made for us, 56 00:04:58,866 --> 00:05:02,100 this is all a reminder of number one, how far science has taken us to even understand all of 57 00:05:04,633 --> 00:05:09,366 this. And the fact that we know this all exists. We have the Webb Space Telescope giving us great 58 00:05:11,333 --> 00:05:15,000 imagery. We have the Vera Rubin Observatory in Chile coming online soon, 59 00:05:15,000 --> 00:05:20,000 all kinds of instruments, which are going to take us even farther and further back in time. 60 00:05:21,933 --> 00:05:25,133 And, you know, to me, John, itús a reminder that we are pretty insignificant in the grand 61 00:05:27,133 --> 00:05:31,200 scheme of things. And yet, weúve gotten pretty smart at figuring some big things out. So, 62 00:05:33,066 --> 00:05:37,266 as we face our problems here on Earth, we do have the capability of understanding big 63 00:05:39,300 --> 00:05:42,833 things. And maybe thatús something we can take in our daily lives to help us understand how 64 00:05:45,300 --> 00:05:47,366 we solve smaller problems right here on Earth. Thatús my philosophical note for the weekend. 65 00:05:47,366 --> 00:05:50,700 JOHN YANG: We appreciate it, Miles. This has been fascinating. Our own -- very 66 00:05:50,700 --> 00:05:53,666 own master the universe, Miles OúBrien. Thank you very much. 67 00:05:53,666 --> 00:05:54,833 MILES OúBRIEN: John, itús a pleasure.