Announcer: This is a Getty podcast.
[Theme music begins]
Hi, I’m Lilit Sadoyan, the host of OMMM, Our Museum
Mindfulness Meditation podcast, Getty’s first video podcast.
Welcome to this Deeper Dive, where we explore the themes
of our weekly episodes with experts in everything
from paintings conservation to the history of sleep.
Marek Slipski: Clouds are ubiquitous across planetary
atmospheres, whether it’s, Earth, Mars’ thin
atmosphere, Venus’ thick atmosphere, or the giant
planets like Jupiter and Saturn.
You see clouds everywhere.
Sadoyan: This week, we did a thought clouds
meditation inspired by Simon Denis’ Study of Clouds
with a Sunset near Rome.
To learn more about clouds and the way they capture our
imaginations, I spoke with Marek Slipski, a scientist at
the Jet Propulsion Laboratories in Pasadena, who researches
clouds and climate on Mars.
Now let’s dive in.
[On video call]
Hi, Marek.
Thank you so much for joining us today.
Slipski: Yeah, thanks for having me.
Really excited to be here.
Sadoyan: Thank you.
So this week we focused on a thought-clouds meditation
inspired by a cloud painting by Simon Denis, and we are
talking today about the significance of clouds both
physically and emotionally.
Personally, I have been looking up at the clouds for a very
long time, since childhood.
We are all just so enamored by clouds, and I’m curious to
hear from you why you think clouds are so appealing.
Slipski: Yeah, it’s a great question.
I don’t have the one answer to that, but, they’re something
we see every day, right?
And I think we’ve all had these experiences as kids
and spending time outside watching the clouds overhead.
But it—they’re not static there, right?
They move across the sky.
What’s there one day isn’t there the next, but there
might be something different.
So they move in real time.
But they’re also ephemeral.
They come and go.
Uh, and there’s something that’s easy to
connect with there and, kind of, is a constant but is also
highly variable that, that makes them really interesting.
Sadoyan: Mm-hmm.
And like you said, they’re ephemeral.
They’re constantly changing.
They also can affect our mood, right?
So what do you think about the emotional
significance of clouds?
Slipski: Yeah.
They, you know, I think you can imagine a storm cloud
and the kind of cartoon image of a rain
cloud following somebody.
So there’s obviously that, like, stereotypical,
kind of connection, rainy day type, sadness association.
But also the being outside on a sunny day with
smaller clouds of different shapes passing overhead and
that being, like, a very relaxing zen-type moment.
Um, I think there’s also maybe a subconscious connection with
what we all read about with respect to climate change.
And even if we’re all not intimately familiar with the,
kind of the physical connections of clouds with climate change,
we see the weather changing every day, and we notice
things like that over time.
And so for some, maybe that’s something that...
it’s not easy to express, but it’s clearly there.
Sadoyan: So what is the connection between clouds
and climate change, or what can clouds tell us
about climate change?
Slipski: Clouds play a really important role in the climate.
They have—they can have two sort of competing effects:
they both reflect incoming solar radiation, so they
reflect sunlight, which acts to cool the atmosphere below.
But they also absorb and emit in the infrared.
They can have that sort of greenhouse effect
and warm the atmosphere.
And so the net effect is dependent on sort of the
details, the very small details of the properties of the
cloud, how big or small the droplets are, the size and
shape of the clouds, right?
We know that things can take up large areas and also
be very vertically extended.
And that might have a quite a different impact than sort
of thin cirrus-type clouds.
And a lot of scientists are really focused on this.
When we run global climate models
to understand how the climate is changing, clouds can be
a big source of uncertainty, not just because they have
this competing effect, but they show up in different
places at different times.
If you look at images of Earth from space, you’ll see
that day-to-day variability.
And, over time, that leads to uncertainty in the
state of the atmosphere.
Sadoyan: And as an atmospheric scientist, I know you care a
lot about clouds in your role.
How did you come to study clouds?
Is this something that you were interested in from
childhood, or do you have any early memories of clouds?
Slipski: I do have those, uh, canonical memories of watching
the clouds pass overhead, but I actually never really
intended to study clouds.
I’ve always been interested in planets.
And I am particularly focused on Mars.
I’ve always been interested in the question of, is
there life out there?
And, and Mars is one of these places that we can kind of
scratch the surface of and try to test whether or not
there is life elsewhere.
And I’ve come at this from the sort of
habitability side of things.
So Mars today, the atmosphere is very cold and thin, and
you can’t have liquid water on the surface.
But we know from the surface that there used
to be liquid water.
So that atmosphere four billion years ago was warmer,
thicker, and something happened to change that.
And so I’ve spent a lot of time focused on the
upper atmosphere of Mars above where you see any clouds,
but where you can see the sun interact with particles
in the upper atmosphere and drive them away into space.
And over time, over billions of years, uh, that atmosphere
has been stripped away.
But as I learned about the upper atmosphere of Mars,
and I’ve sort of come down to lower levels and not
too far below that, there are high-altitude clouds on Mars.
We have high-altitude clouds on Earth, noctilucent
clouds, they’re called, polar mesospheric clouds, where
at nighttime, you can see these because of the angle
of the sun, and they’re— they actually—noctilucent
means night-shining clouds.
You may have seen these outside.
But we see similar things on Mars, uh, and I’ve been
studying those a lot recently.
Sadoyan: Sounds so beautiful.
So you’re studying clouds on Mars.
How are these clouds different from the clouds on Earth?
Slipski: Yes.
On Earth, all the clouds are water droplets.
Uh, right, water vapor in the atmosphere condenses
usually onto a seed particle, a condensation nuclei,
and you get liquid water in the atmosphere, and that’s
obviously what rain is.
There are some clouds that have ice mixed in
them as well on Earth.
But on Mars, the atmosphere is very cold and it’s very thin.
And so just like on the surface of Mars, you can’t have liquid
water, you don’t get liquid water in the atmosphere.
That water vapor in the atmosphere, uh, freezes
directly into ice.
So you have a lot of water ice clouds on Mars, especially
over topographical features like the volcanoes.
But interestingly, you also find CO2—carbon dioxide—ice
clouds, dry ice clouds.
Um, and carbon dioxide is the main constituent
of Mars’ atmosphere.
It’s about 95% CO2.
So the main constituent is actually freezing out because
in certain places and at certain times, it gets really cold.
Sadoyan: So can what we’re learning about clouds on
Mars reflect what we know about Earth and vice versa?
Slipski: Absolutely.
I think at a high level, there are, you know, only
a few atmospheres that we can—that we can really study
and learn about clouds, which isn’t to say that clouds
don’t form on other planets.
Clouds are ubiquitous, across planetary atmospheres,
whether it’s, Earth, uh, Mars’ thin atmosphere, Venus’
thick atmosphere, or the giant planets like Jupiter and Saturn.
You see clouds everywhere.
But these questions of the small scale of how different molecules
condense or freeze and, uh, sort of the environments they
need for that to happen, are fundamental physical questions.
So on Mars in particular, we’re trying to learn a lot more
about how these ices form, how you go from water vapor directly
into ice, and how the–how the seed particles that they form on
matter and shape that process.
For instance, these high altitude clouds, we’re not
sure whether the particles they’re forming on are
dust from the surface.
Mars has these incredible dust storms sometimes completely
enveloping the planet.
But we’re not sure if those dust particles make it up to
high altitudes where water vapor can freeze or if it’s
meteor—basically particles from meteors that burn up in
the atmosphere where you get individual small particles,
and maybe those are what these clouds are forming on.
It’s still an open question.
Sadoyan: Well, we’ve talked about cloud watching here
on Earth and looking at clouds from images in space.
Do you have any suggestions for our listeners who
would love to enter this meditative state with clouds?
Slipski: I sure do! [laughs]
So I help lead a project called
Cloud Spotting on Mars.
Um, this is a citizen science project where we use real NASA
data that’s come from the Mars Reconnaissance
Orbiter, which has been at Mars for 20 years now.
I work with an instrument called the Mars Climate Sounder, and we
can identify clouds in our data.
We’re an infrared instrument, so the data we show volunteers
aren’t images of clouds but the clouds have a particular
shape to them where you can find them and mark them.
And we use that data to kind of look at the distribution
of clouds and try to figure out what they’re made of.
Um, it’s really been a lot of fun to do a
citizen science project.
This is my first foray into this.
And we’ve had a lot of great conversations with participants
in our project, and a lot have commented that they use it
to enter a sort of meditative state, something that’s
very different from their normal day-to-day, where they could log
in, start to find these clouds, and enter a kind of flow state
and, and engage with science.
This is, this is data that we use in research.
Sadoyan: What a wonderful way to contribute to science and relax.
Well, thank you so much, Merrick, for joining us on
the OMMM podcast this week.
Slipski: Thank you!
[Theme music plays]
Sadoyan: To find the related meditation and see images,
transcripts, and additional resources, visit our website
at getty dot edu slash ommm.
That’s O-M-M-M.