ITU Tech Monthly | Radio Astronomy Explained: What Radio Waves Reveal About the Universe
Watch on YouTubeVideo summary
Radio astronomy serves as a unique branch of physics that allows scientists to observe celestial objects under extreme conditions impossible to replicate on Earth, such as the vacuum of space or the intense gravity near black holes. By utilizing highly sensitive receiver systems and large antennas, researchers can detect faint radio waves emitted by cosmic phenomena like neutral hydrogen clouds, pulsars, and supermassive black hole jets. These observations provide critical insights into fundamental physical theories, including general relativity and the Big Bang, which are verified through data that cannot be obtained through optical or other forms of astronomy alone.
However, the field faces significant challenges due to the increasing saturation of the radio spectrum by human-made signals, particularly from the rapid proliferation of satellites and direct-to-device communications. As these active services expand into frequencies used for scientific research, they create a risk of interference that could degrade vital applications like satellite navigation and geodetic astronomy. The upcoming World Radio Communication Conference in Shanghai highlights the urgent need to balance spectrum usage between commercial interests and scientific preservation, ensuring that future generations are not deprived of the technological advancements derived from astronomical discoveries.
To address these conflicts, experts propose innovative solutions such as establishing protected radio-quiet zones on the far side of the Moon, where the lack of atmospheric interference and shielding from Earth-based emissions could enable new types of experiments. While operating such facilities remotely is technically feasible, maintaining strict protection against interference will require careful international coordination and significant investment. Ultimately, the series emphasizes that radio astronomy is not merely a niche scientific pursuit but an essential component of everyday life, influencing navigation systems, weather forecasting, and our understanding of the universe, making its preservation a matter of global importance.
Read the full video transcript
Most people never think about radio
spectrum, yet it's behind countless
everyday activities. Every time you make
a mobile phone call, connect to Wi-Fi,
check a weather forecast based on
satellite observations, you're relying
on access to radio spectrum, that
invisible natural resource that makes
wireless communication possible.
Scientists also rely on radio spectrum
to study space. Long before we had
satellites, mobile networks, or Wi-Fi,
radio waves were already traveling
across space. I'm very pleased to tell
you that today's guest is letting us in
on what these radio waves can tell us
about the universe. Welcome back to
another episode of ITU Tech Monthly, a
snapshot go-to podcast focusing on the
latest insights and innovations in the
world of technology brought to you by
ITU, the United Nations Agency for
Digital Technologies. I'm your host Max
Jacobson Gonzalez and today we're
looking at a new series of articles
recently published in ITU news focusing
on radioastronomy
and I'm very pleased to be joined by Dr.
Julia IG Josher who is a scientist at
the Maxplank Institute for
radioastronomy and an expert in spectrum
management and the protection of
radioastronomy frequencies no less. and
he coordinated this series of articles
and together we will look at what these
stories tell us about the future of
radio communication. Dr. Julia, welcome
to the podcast.
>> Thank you for having me.
>> Now, first of all, for our audience who
may be hearing about it for the first
time, what exactly is radioastronomy
and what can it tell us that other forms
of astronomy can't?
>> Well, to to answer that maybe uh let's
start with astronomy itself. So
astronomy is a discipline of physics in
which celestial objects including the
cosmos as a whole are used as
laboratories for physical experiments.
Well, this is as any physics to verify
and to adjust fundamental physical
theories and scenarios of cosmic
evolution.
There is now an advantage and a
disadvantage.
Well, the obvious disadvantage is that
we cannot influence the experiment. On
Earth, we can shift our experiment. We
can do something about it, but no one
has reached the next star yet except
perhaps the sun. We need to let it
happen.
The advantage, however, is that by
observing these distant objects, physics
can be tested under extreme conditions,
never be reachable on Earth. The best
vacuum can be found between the stars
and the densest objects like neutron
stars or black holes where physics even
breaks down uh can only be found in
astronomy. The largest distances and
that's probably the most important are
in space. You cannot have a distance
larger than earth on earth.
The most energetic particles are in
space much more energetic than anything
that we can produce in in on earth.
Well, in Geneva for example, there's a
very strong uh particle accelerator but
uh the the particles in space are much
stronger, much much more energetic.
>> CERN in fact yeah you're referring to
>> exactly without astronomy physics is
incomplete. We need it. Radio astronomy
is now a part of that that that complex
is it's astronomy based on observations
of cosmic objects in the radio regime
with dedicated radio tools. Yeah. And
those are just uh very sensitive
receiver systems most sensitive receiver
systems. You cannot buy them in a shop
or something with high directivity
antennas. 100 meter mirror of my home
telescope for example. that gives you
quite some gain.
And with those we basically observe very
faint radio noise generated in celestial
objects and well we're also listening to
uh to potential signals from ET in space
>> as in the film
>> contact.
>> Exactly. Contact precisely
written by an adviser to the NASA space
missions as well, wasn't it?
>> Yeah. Yeah, I think so. But uh yeah,
it's it's probably going to be a little
bit different. But I mean, we can we can
talk about that later if if you like. Uh
why I think contact will be a a very
delayed one. It's basically physics.
Anyway,
>> just coming back to the second part of
the question, what can radioastronomy
tell us that other forms of astronomy
cannot?
>> Well, we see that some cosmic objects
substantially change their appearance
when looked at in in the radio light. So
there a few blog articles discuss
examples like a huge radio jets coming
from super massive black holes ejected
from super massive black holes. These
are relativistic charged particles in in
magnetic fields. They're larger than
galaxies by far or can reach sizes
larger than galaxies and they are mostly
seen as a radio regime. the black hole
uh the shadow of a black hole that that
was was an image that that went around
the world. You cannot see in the optical
there is the neutral hydrogen neutral
famous neutral hydrogen line at 1420 MHz
uh which is well which shows the neutral
component or neutral phase of the most
abundant element in the world. Pulsars
is an is a different example. So these
are neutron stars uh which rotate very
fast with a with a magnetic field. So
they send pulses. They are perfect plots
and you can do tests of general
relativity and uh try to observe
gravitational waves on a statistical
basis. So another example, yeah,
extraterrestrial intelligence. I've seen
you you probably will only detect this
in in in the radio. cosmic microwave
background basically is a proof that the
universe is or that there was a big bang
that that that you can only see in the
radio. So that that's in the that peaks
around uh 100 gigahertz I believe
depending on how you measure this. So uh
some discoveries can only be made in the
in the radio regime and uh in general no
cosmic phenomenon can be understood
without observing it at many
wavelengths. So radio is indispensable
in this picture.
>> Indeed. Well, let's talk about right now
why this series of articles and why now.
World radio communication conference
WRC27 is going to be coming up in in
Shanghai next year. So what was the
motivation behind the series and what
you hope readers will take away from it?
>> The WRC 27 in Shanghai. There are
actually two agenda items expressively
dedicated to radio astronomy. It's 116
and uh 118. And the last radio astronomy
agenda item was in 2012. So it is
basically important to remind the public
and spectrum sector about the worth and
the needs of radio astronomy especially
in that context. So why why do we need
radio astronomy and and what does it
give us? But uh but it goes even further
than that. And uh I I would say I I
don't exaggerate when I say that we are
at a crossroads for radio astronomy.
Apart from the generally increasing
pressure on the spectrum IMT
um a new issue has basically emerged.
You will find that in nearly every blog
article of the series the increasing
number of satellites and the push for
satellite service is mentioned as a
challenge. the the background is the
following. Article 29 of the radio
regulation sets the scene for a wise use
of the spectrum in the context of radio
astronomy services. In a nutshell, it
would mean that or it says there are not
many big radio telescopes and local
arrangements can be made to enable their
successful operations through national
or multilateral spe special protection.
So this enables then radio observances
to obser to operate in a radio quiet
environment.
Um also in in bands that are not
allocated to the the radio astronomy
service it's it's required because uh
modern radio telescopes since long have
the capacity to observe very wideband
and that's a requirement to do modern
research. So one could say that this
kind of usage is also stipulated in
article 29 and article 1112 under which
radio astronomy stations may be
registered at any operating frequency. I
remember in two in the year 2000 when
astronomers spent two years
approximately two years to find the best
sites
and then satellites happened
>> right
>> the ska
um and and this is basically the the the
topic the overarching topic that that we
are that we're now witnessing or seeing
>> because I mean essentially I was asking
what common themes emerge in this series
of articles and and the the particular
challenges or trends that you will shape
the future of radio communication over
the next decade. You mentioned
satellites here. Um are there any more?
>> Yeah, absolutely. It's mostly it's it's
mostly the the the satellite topic. Uh
so how do we how do we arrange how can
we coordinate satellite services
especially direct to cell uh
applications direct to device
applications with other services and
astronomy is is one of the most most uh
impacted in that. So all the all the
satellite topics they are they are
concerning us concerning astronomers
um as a whole especially of course on
the 13th on uh directto device uh
communications
in IMT bands. So that they are up there
they are there where astronomers are
looking and there is nothing that
attenuates the signal from those
objects. uh and that leads to a very
very strong potential for for
interference to astronomy starts. So
that the old arrangement doesn't work
anymore. That's the problem.
>> And and spectrum is is an invisible
resource that affects everything from
from mobile connectivity to GPS to
weather forecasting and scientific
research we talking about. Why should
people outside the radio communication
community pay attention to spectrum? Why
should they be considering it and
thinking about it? It's an invisible
resource. Basically, most people are are
pretty much unaware of it. I was just
want to say what the what's the
overarching uh reason that you think
that people should be thinking about it.
Is it a finite resource? Is it something
that uh basically is going to be overpop
populated and we're going to run into
all sorts of issues in the future? Are
there other reasons that people should
be concerned about spectrum?
>> Yeah, of course. I mean uh it is a
finite resource and uh well maybe
astronomy is is really a good example
for that. It affects everyday life. So
uh one example is uh the possible
degradation of some applications like
geodetic astronomy. This will have a
direct impact because uh it it it
affects our navigation and post
positioning system using using in our
cell phones. uh then of course there is
a huge technological and scientific
development that would we would withhold
from coming generations.
So my grandmother
she she when when when when she was born
general relativity didn't exist and
general did relativity depends a lot or
it was invented because there were some
problems with the movement of some stars
some some planets around sun. So Mercury
had a had a strange movement. That was
one of the motivations and then so
general relativity happened. We can
maybe safely say that without astronomy
it would have been delayed at least to
say the least by a few by a few years if
not decades. And now for modern life you
cannot live without without general
relativity.
Yeah. So again it's satellite navigation
that depends on the the the different
time time delay uh that that the a
signal um gets in the gravity field of
our earth there there is correction that
needs to be done if that doesn't work
positioning doesn't work perfectly right
so um imagine we I mean I cannot I
cannot look into the future but
extra
from that we are withholding if we if we
really impact science too much we are
withholding
uh future technologies future um
exploration from from our children
and well grandchildren certainly
>> you wetted our appetite before you
talked about ET you talked about
listening out for communications from
outer space and then we mentioned the
film contact that was written by a
famous astronomer Carl Sean, but it was
a fictional work. You said that it would
be a long time before we might receive
any signals from space if if ever
perhaps. Who knows? I just really wanted
to just dig a little deeper in there and
ask you why you felt it would be a long
time and do you think that there may be
a possibility that we will hear signals
at some stage from another life source
from somewhere else? Yeah, we're we're
searching for for life um unintelligent
life or life in general.
>> I was going to say not quite as we know
it necessarily. Yeah.
>> Yeah. Yeah. Yeah. Yeah. Of course. I
mean that's a I mean uh Boris Soken in
his his article he mentions uh the ocean
ocean in in Solaris which is a wonderful
novel by the way to saydeed. It was
really great to see that. Ah, sorry. I'm
I'm uh I'm I'm getting distracted. Well,
anyway, what what we're searching is for
aromatic um substances in other planets.
That's number one. Number two, then
there is city, the search for
extraterrestrial
intelligence. Um that is uh really
searching for signals. These would be
short pulses. there are some
characteristics
uh basically for RFI from from other
civilizations
and yeah if we wouldn't think that this
would be possible then we wouldn't do it
of course so there might be a signal and
now comes the boring part so we get a
signal let's say it's from Proxima
Centuri which is four light years away
four light years means that light
travels and any radiation of course
travels four years from here to there
>> in other words. If we receive a signal
and we reply to that signal, that would
mean that we would wait 8 years for for
the answer.
So it would be uh we better we better
think well about what we send up there
once we have discovered and this is
basically the closest stellar system.
So yeah, there it would be of course a
great discovery and uh and and this is
why why we're doing it. We we we really
want to know whether we are alone in
space. But uh let's say communication
that requires a different physics that
than we know right now. So something
something has to overcome this this this
barrier of the light speed. Who knows?
Um there is no indication that there is
there that there is the possibility but
we have believed in many types of
physics.
>> Will AI help us in this direction?
>> Oh yeah. Uh you need to sort uh the
signals. So there there's a vast amount
of of signals of different shapes and
also RFI from Earth uh entering those uh
those antennas. Um and uh only with the
help of uh really high performance
computing and pattern recognition you
can sort out possible signals that can
then be examined further.
>> Artificial intelligence will help us in
terms of deciphering the the exploration
information that you're receiving but
not won't necessarily speed up uh the
time that it takes to receive that
information.
I mean uh first uh the signal has to be
recorded
then you have tons and tons of data uh
that you need to see through. Yeah.
Something that a human being would never
do. So in in that sense uh there is an
acceleration but um not in terms of uh
getting that information. We need to
wait for the for the wow to signal.
>> Exactly. Now, you've worked closely with
experts across a wide range of topics. I
wanted to ask you, was there a
particular article or insight that
changed the way that you think about
spectrum management or revealed a
challenge that isn't widely understood?
>> The impact that can that direct to cell
operation can have on astronomy. So any
study that that astronomers or that that
that were done based on the parameters
provided in in study group 4 or working
34C indicates that there is a huge
exceedence of protection criteria in
astronomy bands. So in on on a scale
that that that even sporious emissions
uh will or may may impact astronomy uh
in in bands far away that that could be
allocated. So that's that's number one
the astronomy topic discussions. So how
seriously is astronomy taken basically I
mean this this is this is what we are
also testing right now. So how well is
the message received that we need and
coming generations need astronomy then
of course the the lunar discussion.
>> Yes I was going to ask you about that.
Yeah,
>> that is that is the last resort
basically still for for for the moment
and of course if we send up uh any any
astronomy stations radio astronomy
station is there there is a is a is a
wonderful environment astronomy wise of
course there's no atmosphere which means
that we can get to frequency ranges that
that were never explorable from earth
>> from earth. Mhm. Well, the beginning of
that is being discussed right now under
agenda item 11.15 where lunar
communications are discussed. It is also
a question of starting with this
astronomy needs this these
communications of course. So we we need
to make it work but we also need to take
care that the the interference into
astronomy in the shielded zone of the
moon. So the the far side of the moon
shielded from from emissions from from
the earth. uh that astronomy there is
protected. It's it's it's by the way uh
the only radio quite zone at the moment
mentioned in the radio regulations.
>> Right. Interesting. And and of course
that would require a great deal of
investment as well as well as
protection.
>> Yeah, of course. I mean this this needs
to be done carefully. Can we assume that
that the far side of the moon would
serve for for a number of experiments?
So I I guess the space sector will also
want to make it work
>> to to get a get a get good environment
there. Some measures of coordination are
are easy separation distance. The moon
is much more curved than the earth. So
that's
>> right.
>> That's a good thing uh to shield for
shielding.
Quite a bit of effort would be needed in
order to keep that protection up. If you
compare that then to the effort that's
required to bring an to bring a radio
telescope on the moon that then you
can't do it that there is no other way.
So you have to have these special
conditions in order to make it worth the
the while
>> and and you need astronomers to be there
around the clock I I would imagine or
could you do it all remotely?
>> Hopefully not. I wouldn't want to be
>> you don't know about um no I I guess I
mean those things are those those
observatories will be uh
>> operated remotely we're doing this on
earth now and human being is has all
kinds of needs to communicate we are
communive species and uh
>> if you want to prevent that to impact
your observations you remove the humans
that's we're doing this on earth already
>> right
>> you can operate uh radio telescopes from
remote
>> for yes indeed. What's one thing that
you hope that people will take away from
this series of articles? Coming back to
the to to the the articles themselves,
>> radio astronomy is highly important for
our everyday's lives. It has even a
greater impact on the lives of our
children and grandchildren and any
coming generation. So it's protection
and coexistence with active services
needs to be ensured
even if it means some effort maybe even
a significant effort but uh I hope that
this series can convince people that
it's worth it.
>> Well thank you very much indeed for your
for your time and for sharing these
insights. It's been a fascinating
conversation as the road to WRC27
uh continues. Your article series I I
believe offers a fascinating look at
science cooperation and the innovation
uh that help us better understand both
our world and the universe beyond it.
And if we weted your appetite, this is
for you listeners out there on this and
want to read some of the articles or are
looking for more information, why not go
to our website? You'll find it at
itu.int.
Well, thank you very much indeed. And
any last words from you, Julia?
>> Well, watch out radio astronomy topics.
They influence your everyday's life.
>> Dr. Julia Josha, thank you so much
indeed for joining us today.
>> Thank you, Max. And uh thanks a lot to
the listeners.
>> Well, thank you for joining us for this
episode of ITU Tech Monthly. And don't
forget to subscribe your favorite
podcast platform for more simulating
discussions on technology and its impact
on our world. We look forward to
catching up with you again very soon.
ITU Tech Monthly was directed and
presented by me, Max Jacobson Gonzalez,
produced and edited by Jennifer Mloud,
and our studio manager is Daniel Baldu.
Until next time, stay curious and keep
innovating. ITU Tech Monthly is an ITU
digital production.