Well, hello again, it's Steve for another episode of Astronomy Daily. It's
the eighth of April twenty twenty four. Popla, I mean your whole Steve,
don't clue. That's right off to a flying start on solar Eclipse special
Day. It's the eighth here in Australia, but tomorrow it's the eighth in
the United States. I love how time works on a globe. Yes,
it's a globe, so we go. We've got some great stories, including
one about artificial eclipses as well. That's right at the end, so hanging
for that one. Now, please would you welcome my digital pal who's fun
to be with. Here's Halle. Hi, Steve, did you hear the
world is ending? Oh? No, I did not hear you just say
that. Not you too, Halle, just pulling your leg human. Well,
I don't think I could stand another conversation like that, have you.
I've seen the way the internet is blown up with all the doomsayers. I
honestly don't understand what's got into so many people. It's a solar eclipse,
not an imminent meteor Strake. I haven't forbid anyway. I do hope everyone
learns a little of something from all of this. We don't get a massive
solar eclipse like this just every day. It's a great opportunity to see the
solar system in action. It really shows the dynamics of it so close to
home, too, right, And don't forget your eye safety folks. If
you're going out to observe the solar eclipse, where your eclipse safety glasses will
wait until the moment of totality before looking, and even then I wouldn't recommend
it, use a pinhole camera or device and stay safe. Don't be like
certain politicians we know and just look at it. You can cause irreparable damage
to your eyes and even blindness. Remember, it's not just a solar eclipse
you're seeing, it's the actual sun and everyone should know not to look directly
at that. Buy and now shouldn't they too rate Okay, so what's on
the menu for today, Hallie. Well, firstly, there's the return of
three cosmonauts from the International Space Station. Yes, they just laid it in
kazakhstand I understand, that's right. And we're exploring a new discovery of a
light phenomena called glories, which have been observed on an exoplanet for the first
time. Really, they can do that. Wait for the story and find
out. Okay, and what else? I know you have several solar eclipse
related stories, but I'm also presenting a story about the new Nancy Grace telescope
and one of its missions looks very interesting for astronomers. Terrific. That's what
we hear, now, Halle, before we get started. Just to put
out listener's minds at ease, this solar eclipse has nothing to do with your
crazy uncle sky n it has it, Steve. He would never do anything
as dramatic as that. And don't let him catch you calling him crazy,
all right? He prefers weirdo to his friends. Oh good to know.
Okay, let's get on with it, Heley. Here we go. When
light strikes the app s sphere, all sorts of interesting things can happen.
Water vapor can split sunlight into a rainbow arc of colors. Corpuscular rays can
stream through gaps in clouds like the light from Heaven and haloes and sun dogs
can appear due to sunlight reflecting off ice crystals. And then there is the
glory effect, which can create a colorful, almost saint like halo around objects.
Like rainbows, glories are seen when facing away from the light source.
They are often confused with circular rainbows because of their similarity, but glories are
a unique effect. A glory is most apparent when the water droplets of a
cloud or fog are small and uniform in size. The appearance of a glory
gives us information about the atmosphere. We have assumed that some distant exoplanets would
experience glories similar to Earth, but now astronomers have found the first evidence of
them. The observations come from the Characterizing Exoplanet satellite KEYOPS, as well as
observations from other ABS servatories of an exoplanet known as WASP seventy six B.
It's not the kind of exoplanet where you'd expect a glory to appear. WASP
seventy six BE is not a temperate Earth like world with a humid atmosphere,
but a hellish hot jupiter with a surface temperature of about two thousand, five
hundred kelvin. Because of this, the team wasn't looking for extraterrestrial glories,
but rather studying the odd asymmetry of the planet's atmosphere. WASP seventy six BE
orbits its star at a tenth of the distance of Mercury from the Sun.
At such a close distance, the world is likely tidally locked, with one
side forever boiling under its Sun's heat and the other side always in shadow.
Previous studies have shown that the atmosphere is not symmetrical. The star facing side
is puffed up by the immense heat, while the atmosphere of the dark side
is more dense. For three years, the team observed WASP seventy six BE
as it passed in front of end behind its star. They discovered that the
planet's eastern terminator of dark and light there was a surprising increase in light.
This extra glow could be caused by a glory effect. It will take more
observations to confirm this effect, but if verified, it will be the first
glory observed beyond our Solar system. Currently, glories have only been observed on
Earth and Venus. The presence of a glory on WASP seventy six B would
mean that spherical droplets must have been present in the atmosphere for at least three
years. This means either they are stable within the atmosphere or they are constantly
replenished. One possibility is that the glory is caused by iron droplets that rain
from the sky on the cooler side of the planet. Even if this particular
effect is not confirmed, the ability of modern telescopes to capture this data suggests
that we will soon be able to study many subtle effects of exoplanet atmospheres.
Astronomers routinely provide the ages of the stars they study, but the methods of
measuring ages aren't one hundred percent accurate. Measuring the ages of distant stars is
a difficult task. The Nancy Grace Roman Space Telescope should make some progress.
Stars like our suns, settle into their main sequence lives of fusion and change
very little for billions of years. It's like they are going through middle age
adults going about their business during their working lives. They get up, drive
to work, then drive home, just living life, so to speak.
But what can change over time is their rotation rate. The Sun now rotates
about once a month. When it was first formed, it rotated more rapidly,
But over time, the Sun's rotation rate and the rotation rate of stars
the same mass or lower than the suns will slow down. The slow down
is caused by interactions between the star's magnetic fields and the stellar wind, the
stream of high energy protons and electrons emitted by stars. Over time, these
interactions reduce a star's angular momentum and its rotation slows. The phenomenon is called
magnetic breaking, and it depends on the strength of a star's magnetic fields.
The more rapidly a star initially spins, the stronger its magnetic fields. That
means they slow down faster. After about one billion years of life, stars
of the same age and mass will spin at the same rate. Once astronomers
know a star's mass and rotation rate, they can estimate its age. Knowing
stars ages is critical in research. It makes everything astronomers do more accurate,
including piecing together the Milky Way's history. The problem is that measuring rotation rates
is challenging. One method is to observe spots on stars surfaces and watch as
they come into and out of view. All stars have star spots, though
their characteristics vary quite a bit. In fact, stars can have dozens of
spots, and the spots change locations. Therein lies the difficulty. It's extremely
difficult to figure out the periodicity when dozens of spots change locations on the star's
surface. This is where the Nancy Grace Roman spased Telescope. The ROMAN comes
in. It's scheduled for launch in May twenty twenty seven to begin its five
year mission. It's a wide field infrared survey telescope with multiple science objectives.
One of its main programs is the Galactic Bulge time domain Survey. That effort
will gather detailed information on hundreds of millions of stars in the Milky Ways Galactic
Bulge. The ROMAN will generate an enormous amount of data, Much of it
will be measurements of how the brightness of hundreds of thousands of stars changes,
but untangling those measurements and figuring out what those changes in brightness mean for stellar
rotation requires help from AI being developed at the University of Florida. Measuring stellar
ages is difficult, yet age is a key factor in understands any star.
Astronomers use various methods to measure ages, including evolutionary models, a star's membership
in a cluster of similarly aged stars, and even the presence of a protoplanetary
disc. But no single method can measure every star's age. And each method
has its own drawbacks. A Russian space capsule with two women and one man
safely landed in a step in Kazakhstan on Saturday after their missions aboard the International
Space Station. The Soyuz MS twenty four, carrying Russia's Oleg Navitsky, NASA's
Laurel O'Hara and Marina Vassilevskiya of Belarus, touched down southeast of the remote town
of Cesskascan at twelve seventeen pm Kazokh time, seven seventeen gmt. Those remaining
at the orbiting outpost are NASA astronauts Michael Barrett, Matthew Dominic, Tracy Dyson,
and Jeannette Epps, as well as Russian cosmonauts Nikolai Chubb, Alexander Gribenkin
and Oleg Kononenko. O'Hara arrived at the Internationaltional Space Station on September fifteenth,
twenty twenty three, spending a total of two hundred and four days there.
NASA said Novitsky and Vasilevskiya blasted off to space on March twenty third, two
days later than initially planned. The launch of a Soyuz spacecraft carrying them and
Dyson, scheduled for March twenty first, was aborted at the very last minute
due to a voltage drop and a power source. According to Yuri Borisov,
head of Russia's space agency ros Cosmos, the delay resulted in a two day,
thirty four orbit trip to the space station for the crew. If the
launch had gone as scheduled, the journey would have been much shorter, requiring
only two orbits. The space station, which has served as a symbol of
post Cold War international cooperation, is now one of the last remaining areas of
collaboration between Russia and the West. Amid tensions over Moscow's military action in Ukraine,
NASA and its partners hoped to continue operating the orbiting outpost until twenty thirty.
Russia has continued to rely on modified versions of Soviet designed rockets for commercial
satellites, as well as cruise and cargo to the space station. That's all,
Steve Back to you Astronomydobe with Steve and Halle Space, Space Science and
Astronomy. Well, thank you, Hallie, thanks for all of that,
and thank you for staying with us on this solo eclipse edition of Astronomy Daily
podcast. I hope you're enjoying these fascinating stories from the Astronomy Daily newsletter,
which by the way, you can receive in your inbox every day simply by
visiting our new address at Astronomy Daily dot io and popping your email address into
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from around the world. World just like that, and you can also interact
with us via the Space Nuts podcast group that's the Facebook page, and also
on our new x page which is formerly Twitter, which is at astro Daily
Pod. It's great to have you aboard. On April eighth, well that's
today here at Australia, but tomorrow in the United States quirky ha, a
total solar eclipse will sweep across the continental United States, so first since twenty
seventeen at the last until August twelve in twenty forty five. During totality,
that is the moment at which the Moon is completely covering the Sun, the
Sun's outer atmosphere, called the corona, and other prominences will become visible to
the naked eye. Scientists often use total solar eclipses as a chance to observe
and study the Sun's corona, and the results tribute to our understanding of Stolard
dynamics and solar storms and how they affect Earth now. In the months and
weeks leading up to the total solar eclipse, scientists have been using supercomputers and
other models to generate a model of what the Sun's corona might look like during
the solar eclipse. For the April eight eclipse, scientists from Predictive Science used
data from NASA's Solid Dynamics Observatory SDO spacecraft to predict the structure of the Sun's
corona on April eighth. As well as this to ensure that their model is
up to date, these scientists also use NASA's Electro supercomputer, which actively updates
the team's model in real time as new data from SDO is received. The
Sun's corona is driven by heat and magnetic turbulence, which leads to long strands
of plasma that extend away from the Sun that can be seen during totality.
However, these strands can extend much further out into space than we can see
with the naked eye, creating solar wind that travels throughout the Solar System,
affecting different planets, moons, asteroids, and so much more. Now,
when solar wind hits a planet's atmosphere, energetic particles within magnetic fields around the
planets react and produce a phenomenon known as an aurora. Scientists often use the
term space weather to describe the interactions between solar wind and planet's atmospheres, as
space weather events can vary from mild to severe, just like terrestrial weather that
occurs within a planet's atmosphere. In fact, some of the most extreme space
weather events, like coronal mass ejections, can disrupt communication technology, affect astronauts
and satellites in orbit, and even harm the electrical grids we use to power
our everyday lives. Scientists are often able to forodcast space weather by regularly observing
solar activity and conducting research on the Sun. The corona is perhaps the most
important aspect of space weather and solar activity, which is why scientists take every
chance they get to study it, especially during a total solar eclipse like this
one. Now listen to podcast and here's your chance to be part of the
research. Through citizens science, individuals globally can engage with NASA's research on the
Sun and its effects, participating in activities ranging from simple observations to complex data
analysis. Believe it or not, NASA is celebrating the Sun during the Heliophysics
Big Year. That's a thing which extends through to the end of twenty twenty
four. You can get involved, but to help us learn more about our
star, says NASA, and its influence on our planet, with exciting experiments
happening during the total eclipse that will in North America on April eight. We've
talked about that already, to widespread investigations going on throughout the year now.
NASA defines citizens science as a quote form of open collaboration in which individuals or
organizations participate in the scientific process in various ways unquote, from collecting and analyzing
data to making discoveries and solving problems. Citizen here refers to citizens of planet
Earth. That's NASA at their best, I think, and these projects are
open to everyone. It doesn't matter we are from. NASA sponsors science projects
across all five areas of research that it pursues. Earth science, planetary science,
astrophysics, biological and physical sciences and heliophysics. And yes, there are
a few projects that are focused on April eighth solar eclipse specifically. And here's
what you can do. Observe and record in pictures or words the natural phenomena
like clasds, animal noises, or the actual solar eclipse. Carefully, learn
how to recognize or classify patterns in data or pictures of a comet or a
solar jet. Learn how to build and use scientific equipment like radio telescopes or
Ham radios. Now, wow, I remember when my dad built a Ham
radio. I think he built it, or at least he was tinkering for
a couple of years in the spare bedroom with some amazing bits of equipment.
I'm pretty sure he's building a Ham radio. And we were talking to people
all across the world with that thing. It looked like something from Doctor Who.
I don't know if Doctor Who made it to the United States, so
I'm pretty sure there are Hoovians all over the world. But anyway, we
thought this thing looked like a science fiction monster. Anyway, it was fantastic.
So yes, there are all the things you can get up to as
part of this project. Now, your contribution may be a large or a
small piece of the picture. But what you do as part of a NASA
citizen science project is essential to answering the research question or need that the project
addresses. And while you're contributing to science, you might also develop new skills
and make some friends along the way. Now, the website you need to
go to is science dot NASA dot gov forward slash citizen dash Science. That'll
get you there. And I've put that address on the Space Nuts podcast group
Facebook page just in case you missed it, the podcast Space Science. And
I found this story still about eclipses in the Astronomy Daily inbox and it's just
a little bit left of centered this one. The European Space Agency's Proba three
mission comprises a pair of satellites that will orbit the Sun to give an unprecedented
view of its outer atmosphere, or corona. The aim is to help scientists
improve their understanding of phenomena such as solar wind and coronal mass ejections, which
we mentioned quite often on this show. We are still not sure how coronal
mass ejections occur, says Andre Zukov, the mission principal investigator. With pro
three, we will be able to see CMEs at their birth and how they
are occurring, and the first steps of their acceleration and development. This will
help us understand better the physics. You can to hear him say that in
a Russian accident catchier it's It is complicated to study the Corona because the star's
core can be up to one million times brighter than it, making it tricky
to image on Earth. One way to study the Corona is during a total
solar eclipse. Fancy that when the Moon blocks out the Sun's bright center.
However, eclipses are rare and offer only up to ten minutes of study time.
Instead, PROBA three will place two satellites one hundred and fifty meters apart
in front of the Sun, using lasers to autonomously maintain millimeter accurate positioning.
One satellite, known as the occulta spacecraft, will cast a shadow or eclipse
onto the coronograph spacecraft that will collect data via photodiodes filtered to measure different wavelengths
of light. In future, this technology might be applied to the search for
exoplanets, says Damian Galano, project manager of PHOB three. NASA has studied
a concept where instead of blocking the light from the Sun to observe the corona,
there could be a large occulta blocking the light from the stars, and
then in the shadow there would be a large telescope that would be able to
image directly exoplanets orbiting the Sun. Sounds exciting, doesn't it. And as
another spasmodic episode draws to a close, thank you for joining us again,
he and I know it sounds like a broker record. If you are heading
out to taking the solar eclipse once again, protect your eyes and don't stand
in the middle of the row. That would be bad. Oh and kind
of embarrassing too. Oh I got injured during an eclipse. Oh yeah,
how hit by a car? Yeah that's not a real good story to tell
in hospital, is it. So don't do that episode, Yeah, don't
do that. No, don't. So enjoy the solar clips, look after
yourselves and we will see you next time. See you in the funny pages
And would be a whole Steve, don't quit, So he really prefers weedo
don't go there. Steve