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20260808 17:30 UTC · 00:30:59 · 363 transcript segments · GDELT Visual Explorer · plain-text transcript · Event Map

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Transcript

Google Speech-to-Text API Automatic Transcription (Chirp). Treat it as a searchable index of what was broadcast, not a quotation record.

00:00:00Join the movement, stand for our country, stand
00:00:04for one another, hashtag #unite against
00:00:08terror.
00:00:18At
00:00:18of tv news, wherever the big news stories happening, we're
00:00:22get up to aggregate. News,
00:00:26first with breaking news.
00:00:35in
00:00:57of
00:01:07For thousands of years, humans have been looking to the stars searching for
00:01:11answers. Here in New York, scientists continue that
00:01:13tradition, getting information from galaxies far, far away in hopes that
00:01:17humanity might survive in the future. Gennadi Villavin
00:01:21is head of a special astrophysical observatory home to many unique
00:01:25telescopes, which means we're in for an interesting
00:01:28tour.
00:01:33genia, hello, hello, so this is the
00:01:36BTA, so tell me what is it, how do we get an image from here? it's not
00:01:40like looking into a telescope at
00:01:42of home and seeing the moon, what kind of an image can we get here?
00:01:46uh, this is the large alt ismoth
00:01:48telescope, despite its size, the way
00:01:52we capture images of celestial
00:01:55of objects, stars, galaxies, quasars and so
00:01:58on, with this... telescope is fundamentally the same as
00:02:02with amateur telescopes. The unique feature of this
00:02:06instrument is its alter zimoth mount. This
00:02:10telescope was
00:02:11of pioneered in this regard. Up there was the first
00:02:15platform where our initial observations took
00:02:18place. Collocally, we call it the
00:02:22glass, because it looks like a
00:02:24glass. Observers used to sit there at one
00:02:28time.
00:02:30of Nowadays, of course, everything happens
00:02:33automatically, an observer is no longer
00:02:36needed, but the
00:02:38of observer
00:02:38of her used to sit there would
00:02:40of adjust the coordinates, track stars and so
00:02:44of on.
00:02:58So this is my 20 years
00:02:59of ago so... This is like a time machine in many ways, because the
00:03:03light that we're getting here now is from billions of years
00:03:06ago,
00:03:07what is the furthest back that you've ever been able to capture an image here at this
00:03:11telescope?
00:03:15As of today, we can say yes, it's
00:03:19indeed a time machine, it allows us to look not
00:03:23of only far, but also back in time. This
00:03:27telescope was
00:03:28of prepared specifically for this purpose.
00:03:38can look very, very far and
00:03:41of into very,
00:03:43in of very long ago. what we mean by
00:03:47of that is events that happened in the universe
00:03:48more than 10 billion years ago. it can also look at the
00:03:52distance light has traveled,
00:03:54more than 10 billion years. i can't say exactly right now what
00:03:58the maximum red shifts we have. obtained
00:04:00of for galaxies or quisers are, but it's somewhere around
00:04:04five, so that is, I don't know,
00:04:07approximately 11 to 12 billion years
00:04:11ago, and that means 12 billion light years from here
00:04:14accordingly, so there you go, I see we have some movement here, can you tell
00:04:18me what's happening, like what are we actually seeing here with this telescope, the
00:04:22telescope points a star and rotates its
00:04:26axis, the operator gives the command to aim a specific.
00:04:30point in the celestial sphere and it starts, now
00:04:34it's supposedly aimed at the star, so um, not
00:04:38just asteroids, there are other things that can um be dangerous to us here on earth as
00:04:42well, such as let's say a pulsar or a quasar close to
00:04:45us, um, do you worry about any of that, does any of that keep you up at
00:04:49night? don't worry, asas and kizars are
00:04:53very far away from us. cazars in fact,
00:04:57don't really exist in the present time. Well, maybe
00:05:01some
00:05:01of the closest ones do. The quasars we see are among the
00:05:05most distant objects that existed tens of billions
00:05:09of years ago. They show us the active. process of
00:05:13galactic disc formation, these are
00:05:16young, active galaxy nuclei, that emit
00:05:19enormous amounts of energy, but don't
00:05:23worry about them, there's nothing to fear, neither
00:05:27pulsars nor quazers pose any threat, in
00:05:30general, all events related to the collision of large
00:05:34objects such as earth, or the solar
00:05:37system, while not entirely impossible, are
00:05:41extremely rare. and at least for our solar system,
00:05:45nothing will threaten us for hundreds of millions of billions
00:05:49of years, so I have to ask, you've been studying space your entire
00:05:52life, would you like to personally go up into space and be closer to the
00:05:56action, and do you think think that there might be a benefit for
00:06:00astronomers like yourself to be up there and closer and see
00:06:03things for themselves? personally, I do dream of
00:06:07space, but I see many interesting things to do
00:06:11here as well. Moreover, some things in
00:06:14space are fundamentally impossible to achieve.
00:06:18However, I believe that in the future, when space travel
00:06:22becomes less costly, all astronomy will move to
00:06:25space, perhaps to the moon. Observing space
00:06:29from the moon would be very effective. Um, there are some people
00:06:33who think that um, astronomy doesn't help us
00:06:37in our everyday lives, that it's just something that's going to happen in the
00:06:40future. What can you?
00:07:12contributions to
00:07:17provides
00:07:20It technological significant domestic also and global advancements in fields
00:07:24and technologies unrelated to
00:07:27astronomy. In this sense, astronomy,
00:07:31even if it doesn't directly feed us, plays role in
00:07:35this process. All fundamental science is
00:07:39built on this principle. It's very wrong.
00:07:51as a hole, and all technological complexes in the most
00:07:55highly developed countries the world, are
00:07:58interconnected and related each other,
00:08:01so there is a direct practical benefit from
00:08:04astronomy.
00:08:35so looking beyond our solar system uh we have
00:08:38exoplanets uh they exist um
00:08:42tell me about those and are you certain that we're going to find life
00:08:44there? i think so, but that is
00:08:48something that awaits us in the future. life is a
00:08:52stage in the evolution the overall chemistry the
00:08:55universe, its chemical elements, from the moment of
00:08:59birth to the aging of our universe, it becomes more
00:09:03and more complex. initially it was just hydrogen, then
00:09:07other elements were synthesized and so on. then
00:09:11came rock material. organic substances
00:09:15and finally life. We know that this process
00:09:18occurs uniformly throughout the universe. If
00:09:22life exists somewhere, then it exists
00:09:25everywhere. It's just matter of finding
00:09:29it. Personally, I believe that biological life
00:09:33will be discovered on other planets, not
00:09:36civilizations, but biological life, some forms of
00:09:40life or signs of it.
00:10:12hard to believe it would be very similar, it could be some other
00:10:16branch of life, but we can only
00:10:18speculate, so the
00:10:21sun, as it expands, the earth will not survive.
00:10:25this as it gets brighter, how long do we have before this happens
00:10:29and what can we expect
00:10:31to see in this process? don't
00:10:34worry, we still have some 5 billion
00:10:38years to go without any
00:10:40problems.
00:10:43and i'm going to ask this because the dark
00:10:44project,
00:10:48is in essence astronomy the only science that's really going to
00:10:52help us survive in the future, because "we need
00:10:55to be ready for asteroids coming our way, know when they're coming or
00:10:59know how we can manipulate them, you're absolutely right.
00:11:03astronomy in this sense has great meaning for our lives
00:11:07right now, at this time. this has to do
00:11:11with asteroid astronomy as well,
00:11:14mean people underestimated just recently, a
00:11:18couple of years ago, a massive asteroid blew up near
00:11:22Chelabinsk, had it been 10 times bigger. It would have been
00:11:26a tragedy. It was actually quite
00:11:29intense. No one was killed, but windows were
00:11:33shattered, people wounded and so on. And
00:11:36we hadn't noticed it. That's our drama as
00:11:39astronomers. Estimates vary, but these
00:11:43days we only control just few percent of
00:11:47outer space. The rest of
00:11:50it is its own. If
00:11:51an asteroid is far away, we have plenty of time.
00:12:03and
00:12:03they are easy to overlook. Is there a bit of a paradox?
00:12:07I mean, if we can change the course of asteroid, can we be creating more
00:12:11problems in the future? I don't know if
00:12:15there are going to be more problems, but personally, I think
00:12:18what we saw recently, the changing of asteroid's
00:12:22trajectory, that's great progress. Really, it gives
00:12:26us certain hope that in the future, at some point at least,
00:12:30this problem will be solved and will be
00:12:32protected.
00:12:53This is the 600. it is the size of 40 football fields and
00:12:57has about a thous mirrored elements. it was designed to
00:13:01capture signals from space listening in to the conversation
00:13:05the
00:13:05cosmos.
00:13:12julia, thank you for taking us to your office, as it were,
00:13:16appreciate the opportunity to show us this radio telescope. what kind
00:13:20of signals do you catch here and what
00:13:24kind of? information can you get from them and also have you ever got any signals that you weren't able
00:13:28to explain? just like a common
00:13:31landbased telescope, raten 600 captures
00:13:35non-thermal synchroton emission mostly from celestial
00:13:39bodies. for example, the sun, the closest star
00:13:43to us emits radio waves, and
00:13:46we can observe it. most other objects are extra galactic
00:13:49sources or radio waves like galaxies and quasars
00:13:53and the signal. from them that the radio telescope
00:13:57captures are the non-thermal synchroton radio emission
00:14:00of electrons. It's called synchroton emission
00:14:04because electrons move along magnetic field lines at
00:14:08close to the speed of light. That's the main type of data that
00:14:12radio telescope captures. What we observe here are
00:14:16hundreds of thousands of space objects that emit radio
00:14:19waves. We receive data on their activity, on their
00:14:23calm state and on. the evolution the synchrotron
00:14:26emission that originates from the central areas of
00:14:30galaxies and quasars, mostly it's galaxies and quasars that we
00:14:34observe here. now i understand that the sun is getting
00:14:38ready for a period of extra
00:14:41activity, and what kind of information can your radio telescope
00:14:45tell us about what's to come and what can we learn from
00:14:49this extra active period
00:14:51in the sun? in our daily observations. with
00:14:55Rayton 600, we study solar activity in the
00:14:59radio frequency band. The key advantage of Rayton
00:15:03600 is that it can work in multiple frequencies. We
00:15:07study space objects from 1 to 30 gigahertz and we
00:15:10receive this data instantly. As the nearest star
00:15:14heated to 6000 degrees Kelvin, the sun is
00:15:18the focus of our studies. As we know, the sun is now in its
00:15:2211 year cycle of activity, now.
00:15:25data
00:15:28now it's at maximum. after many that years
00:15:30the at rain
00:15:32the key minimum, 600 retrieves and where we have massively improved is
00:15:36solar activity for. the
00:15:39radio frequency allows us to predict proton
00:15:43flares on the sun several days in
00:15:45For example, advance. A proton flare is powerful outburst
00:15:49of solar particles with a large share of
00:15:52protons. Radio frequency data retrieved by
00:15:56Rayton 600 allows us to predict such flares
00:16:00two or three days in advance. The data is fed to our
00:16:04observatory's website where automatic forecasts are.
00:16:07least positive or negative? of course, this forecast is
00:16:11not 100% accurate,
00:16:13but in 80% of events, our flare forecasts are
00:16:17confirmed. so these solar flares, these bursts of plasma
00:16:20coming from the sun, they're strong enough to cause disruptions in
00:16:24communication down here on earth, what can we learn from
00:16:28this? what can we do to prepare, and
00:16:32mean is humanity in for some sort of chaos because these solar
00:16:35storms? Solar
00:16:38activity has a significant impact on humans, the atmosphere
00:16:42and all communications. How can we protect ourselves
00:16:46against this? Here, at Rayton 600, we only
00:16:50gather information that helps us understand what's
00:16:52coming. As for the measures that protect us from solar
00:16:56flares, well, sometimes we're told to stay at
00:16:59home.
00:17:02Okay, so the ren 600 can capture
00:17:06signals from.
00:17:37for the benefit of humanity. We all live on earth and it would be
00:17:41foolish not to be curious about what's out there. It's the
00:17:45first question we ask as humans, we are surrounded by
00:17:48colossal energy and enormous energy
00:17:52sources. By studying them, we can explore alternative
00:17:56ways to produce energy, which is a pressing issue
00:17:59given that our planet's resources are
00:18:02limited.
00:18:05So this is incredibly interesting. Can you show us a little bit more of
00:18:09your office, or should I say this
00:18:10telescope?
00:18:32So that we know of, we have not heard any
00:18:36signals from aliens.
00:19:38we can receive and process signals within this range, which is
00:19:42why we focus on it. modern instruments such as
00:19:45ground-based and space observatories aim to increase
00:19:49sensitivity to detect very weak signals. it's
00:19:52possible that we're searching for something that doesn't exist. it's
00:19:56also possible that the signal we're looking for is extremely
00:20:00faint, but that is not very likely. it might be
00:20:04that there's no one out there for us to find.
00:21:02so you personally, do you hope to find a alien
00:21:06life out there
00:21:07someday? like
00:21:11everyone else on earth, the thought of us being alone in the universe is
00:21:15frightening to me, on the other hand, it's also scary to
00:21:19think that someone might be close by and could pay us visit.
00:21:23Of course, the theory of probability suggests that a universe with
00:21:27unknown boundaries, we can't be the only form of
00:21:30life. There are most likely other life forms out
00:21:34there, which could be less or more advanced than us. It
00:21:38would be fascinating to meet and understand them, but like most people,
00:21:42I'm also apprehensive about
00:21:43it.
00:21:51kind
00:21:51of goes hand in hand with what you do and what you're studying,
00:21:54what is the next era of space exploration in your mind? what do you think is
00:21:58the next big step for us? are we on the edge of
00:22:01new era in the space race? i
00:22:05believe that the next big step in space development will require a
00:22:09significant technological leap. ground-based telescopes
00:22:13are improving their sensitivity and angular resolution, but
00:22:16we can't do this endlessly. that's why space. telescopes are
00:22:20crucial. There are currently many space telescope
00:22:24missions, including some in our country. They allow us
00:22:28to be unconstrained by the atmosphere and increase
00:22:32sensitivity or angular resolution when a space
00:22:35telescope observes simultaneously with a ground-based
00:22:38telescope. The next step is definitely space
00:22:42observatories, which I think humans have not yet fully
00:22:45mastered. Now
00:22:49what is the one thing? that you just have
00:22:53trouble wrapping your mind around because you're dealing with huge
00:22:56numbers, you're dealing with things that basically people don't
00:23:00understand, is there something in your mind that
00:23:04just really is hard to understand or
00:23:06grasp?
00:23:13the most important reason why we study the universe, why we study
00:23:17outer space is to investigate it.
00:23:20and evolution, this is the main question, we
00:23:24study all kinds of objects and their development can point us to
00:23:27the history the universe and its growth, how and where did
00:23:31everything originate, what was the starting point? there's a
00:23:35theory that everything started with the big bang, but what
00:23:39was before that, and was there a big bang at all? there are
00:23:43many questions, theory and observation do not
00:23:46aligne, in order to explain with theory what? we see
00:23:50and observe, we need to make lot of assumptions, adjustments and
00:23:54introduce various coefficients, which we often do without
00:23:58explanation. our primary goal is to understand how
00:24:02everything happened and how everything evolves. this is the
00:24:06main thing astronomy seeks to answer. if i may
00:24:09ask, what really excites you about your job? why do you do
00:24:13what you do? the most impressive
00:24:17thing about astronomer's work is that: we get to do what we love
00:24:21professionally. when we come here, we are first and
00:24:25foremost free in our choices. we can
00:24:28improvise, and very often we don't have
00:24:31to be told what
00:24:32to do. we are a state of discovery, and that's
00:24:35exciting. as one of our colleagues said, you come
00:24:39here, enjoy yourself and get paid for it. it really is a
00:24:43pleasure, especially when you succeed, when you discover something
00:24:47new or confirm your hypothesis.
00:25:20You also need to be a philosopher, you need comprehensive
00:25:23approaches, sometimes non-trivial ones. In this
00:25:27regard, astronomy is no exception, but it's also
00:25:30global because we study very distant objects that we cannot see
00:25:34directly. We need to figure out how to observe them, how to
00:25:38improve the image and enhance the signal, and this brodens
00:25:42our horizons first of all, but also naturally,
00:25:46our world view. It's a comprehensive approach.
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Data courtesy of The GDELT Project (gdeltproject.org), from the Internet Archive TV News Archive. Film strip and transcript are GDELT's, rehosted here under their terms of use, which permit it with this citation.