Planetary Radio: Space Exploration, Astronomy and Science - What Do You Need to Make Martian Oxygen? MOXIE!
Episode Date: December 16, 2020Mike Hecht is in charge of the MOXIE experiment on NASA’s Perseverance rover, arriving on Mars in February. The tiny device will test our ability to turn the Red Planet’s plentiful carbon dioxide ...into oxygen. Someday a scaled-up version may make the oxidizer that will get astronauts back to Earth. Mike also helps lead the groundbreaking Event Horizon Telescope Collaboration that captured the first image of a black hole. Want to win a Planetary Society baseball cap? Your opportunity arrives with What’s Up. Discover more at https://www.planetary.org/planetary-radio/1216-2020-mike-hecht-moxieSee omnystudio.com/listener for privacy information.See omnystudio.com/listener for privacy information.
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It takes a lot of moxie to make oxygen on Mars, as you'll hear this week on Planetary Radio.
Welcome, I'm Matt Kaplan of the Planetary Society, with more of the human adventure across our solar system and beyond.
NASA's Perseverance rover is closing in on the Red Planet.
NASA's Perseverance rover is closing in on the Red Planet.
Inside the robotic explorer is an experiment that will move us farther down the road toward putting men and women on Mars.
I think you'll enjoy my conversation with MOXIE Principal Investigator Mike Hecht.
Want to win a Planetary Society baseball cap?
You'll get another opportunity when Bruce Betts visits with another What's Up report. The exploration of our solar system
marches on. You can track it in our weekly newsletter, The Downlink.
A couple of the stories have progressed even since the December 11 edition
appeared. For example, Japan's space agency
has just announced that the sample return capsule from the Hayabusa 2
probe does indeed contain
material from asteroid Ryugu. The spacecraft snapped a beautiful shot of Earth as it sped
by our planet. We've got a link waiting for you at planetary.org slash downlink. And as I record
this, China's sample return spacecraft is nearing Earth. Chang'e 5 is believed to be carrying about 2 kilograms of lunar material.
NASA has selected 18 lucky astronauts for what it calls the Artemis team.
Some number of them may be the next humans to walk on the moon.
We'll talk with one of them, veteran Stephanie Wilson, next week.
MOXIE is the Mars Oxygen In-Situ Resource Utilization Experiment.
If all goes well, it will soon demonstrate that one of the most important consumables
for a human trip to Mars and back can be made right there, in situ.
Michael Hecht serves as principal investigator for MOXIE. He spent 30 years at JPL before moving across the
United States to the Massachusetts Institute of Technology. Mike is also associate director of
MIT's Haystack Observatory and, and, deputy project director for the Event Horizon Telescope
collaboration. Yes, a Mars pioneer also helps to lead that worldwide collaboration
of radio telescopes that revealed a black hole for the first time in 2019. We get to that side
of his life toward the end of the great conversation you're about to hear, but the main
topic was making oxygen on Mars, something Mike hopes to attempt not long after Perseverance lands in February of 2021.
Mike Heck, thank you very much for joining us on Planetary Radio as we speak. Not too many weeks
ahead of MOXIE and the rest of Perseverance. Getting through those seven minutes of terror
and down to the Martian surface is the excitement building? Oh, it absolutely is. And one thing that reminds me every evening, and I encourage the audience
here to follow up on, you walk out the door in the evening as the sun goes down and you see Mars
in the eastern sky glowing bright and red, outshining, almost even outshining Jupiter in the sky. And that's how you always
know there's a mission on its way to Mars. That's how the orbital mechanics work out.
You launch before opposition when Mars is at that peak of brightness in the evening sky,
and you land after opposition. So every night when I go up and look in the sky,
I know we're getting closer. It has been gorgeous lately, hasn't it?
I mean, I had the telescope out a couple of nights ago and we were looking at Mars and some of its neighbors farther out.
But it is spectacular to think that we are about to go there again and that we'll be doing science and preparation for humans on Mars that has never been done before. You know,
everybody talks about how important in situ resource utilization will be for human exploration,
but you and the MOXIE team seem to be among the first to actually hope to demonstrate it.
That's absolutely the case. Yes, certainly what we've done is a source of great satisfaction. But I always go back to the fact that the fact
that NASA created this opportunity is the best proof that they're serious about this enterprise.
You know, when I first got involved in preparing for human exploration to Mars back in the 90s, Dan Golden was saying, we'll have astronauts on Mars as early as 2011,
15 years away, he was saying. And we're still talking about 15 years away. And why do I think
this time is different? Well, that's one of the reasons. The fact that NASA was willing to invest
of order $50 million in actually proving ISRU on Mars.
That's a real commitment.
That is such a good point.
I mean, I know that you beat out a lot of other worthy projects.
This space that Moxie's taken up could have been another mass spectrometer or something
like that.
So I guess it is pretty significant that NASA chose this way to demonstrate that we can make what humans are going to need on Mars when we get there.
Absolutely.
It's the next great adventure after the other one that Perseverance is kicking off, which is sample return.
And I found Perseverance such a wonderful, complex mission in that it's dealing with science
today. It's investing in the future with preparing for sample returns, let's say tomorrow. And it's
also preparing for the best science, in my opinion, which is when we have human scientists
on the ground, let's call it the day after tomorrow. I love that. What inspired that great acronym, which I spelled out when I was introducing you?
The great acronym MOXIE?
Yes, I'm sorry. Yes, MOXIE.
Because, of course, it has an embedded acronym in it, and even that is a story.
MOXIE, of course, has the general connotation of audacity.
So there's the rather literal interpretation of the fact that we were a long shot group
when we proposed.
And the fact that we proposed it all, you know, and inspired by my JPL colleagues, was
audacious, was evidence of Moxie.
Of course, the fact that we were selected, even more so. But it also had a real local resonance for me and for my institution. I'm working at Haystack Observatory up in Western Massachusetts, down the road from Lowell, Massachusetts.
was a soft drink everybody knew. And in fact, it goes back to the late 1800s where it was the soft drink. The fact that we have this word moxie that means audacity comes from the advertisements for
the soft drink in those days. It was invented in Lowell, Massachusetts, just down the street from
us. It is even now the state drink of the great state of Maine, just to our north. And embedded in the acronym is another acronym,
ISRU, In-Situ Resource Utilization, which frankly, Matt, means living off the land.
But as I like to say, they couldn't use the acronym LOL. It's already been taken.
Right. It's undoing now.
Embedding an acronym is not normally something I like to do, but the first attempt to do this Right. That's what I'm doing now. Polar Lander in 2000, late 1999. It was put on hold and never really flown, although it did have
a sort of a resurrection with Phoenix, the Phoenix mission. But on the 2001 lander was an attempt to
do a much smaller, more modest version of what MOXIE became. And that was called MIP, which was the Mars ISPP precursor. ISPP was what they used to call ISRU. It was
in situ propellant production. So that had an embedded acronym in it. And I thought,
you know, that's the one thing on Mars 2000, on the 2001 lander that never found another ride to
Mars. And so it's a little bit of a very subtle homage to people on the inside to say,
we're going to embed that same acronym in the middle of MOXIE as a little bit of an homage to
the folks who developed the MIP project. It's a long story. Yeah, but MOXIE is a little bit of
a phoenix in itself, it sounds like. Indeed, indeed it is. And, you know, I've always been of the impression that if you propose
and are selected to fly an experiment to Mars or elsewhere, NASA will eventually find a way to do
it. And I don't know if it's a conscious policy or just the way it works out, but it seems that
all the projects I've been involved in over the years that for one reason or another, like the 2001 mission, haven't made it eventually find another way.
All right.
Well, let's talk about what it does.
I mean, I think I've heard you say and others say, and you can see pictures of it.
We'll put up the link to the MOXIE website on this week's show page at planetary.org slash radio with lots of
other resources. It is only about the size of a car battery. How much O2 are you going to get out
of this little box? That is the key question, Matt. And we're limited not by what we could build.
We could build a full-size MOXIE unit today, probably as easy or easier
than the effort to build this small one. But we have two serious constraints. One constraint is
that we're on a rover that's only so big, and we share it with seven other instruments.
The other constraint that's even more significant is this rover, this big rover, the size of a
even more significant is this rover, this big rover, the size of a Mini Cooper, right,
runs off of 100 watts, 110 watts. You know, back in the day when we had incandescent light bulbs,
a light bulb on your desk lamp would have been brighter than, you know, more power than that.
It's a very, very puny power system. To do what we want to do on Mars to support human exploration, we'll take 25, 30 kilowatts. So just to run on this small power supply, power system, we had to
scale way, way back. Nonetheless, we can demonstrate all the principles, all the technology, all the hardware on a small scale. And so MOXIE will produce about 10 grams
an hour of oxygen. Now, if you and I were sitting having this conversation on my, or in fact,
sitting on having this conversation today, we're probably consuming about 20 grams an hour,
about twice what MOXIE will produce. It's about the amount that if I look out my window at
the trees, that a modest sized tree in my yard will also produce about 10 grams an hour of oxygen
from the CO2 in our atmosphere. I thought that humans needed a lot more O2 per hour. And so a
couple of these little boxes would be able to keep me alive on Mars,
apparently, if it performs as well as you hope it will.
Well, absolutely. Keeping humans alive is easy. And that's really not the main purpose
of the MOXIE technology. The common link, though, to the main purpose is that we,
as human beings, use fuel. We use fuel. We call it food, but if we weren't
appreciating it aesthetically, we call it fuel. And to burn fuel requires oxygen or something
like oxygen, whether you're a human being, whether you're a fireplace, whether you're an automobile,
or in this case, whether you're a rocket ship.
And the more fuel that something uses, the bigger it is, the more oxygen it needs.
The thing that we do not appreciate on earth is that this oxygen that we are burning,
that our car is burning when we drive, weighs much, much more than the fuel. Fuel is light. It's based on hydrogen. It's very light stuff.
And so if we had to carry an oxygen tank in our cars, because we couldn't get oxygen for free
in the air around us, it would weigh maybe four times what the gasoline weighs. So if we're
thinking what we need to bring to Mars and what it weighs. The single heaviest thing we would need
to bring is a tank of oxygen, not for the astronauts, that would be a little tank, but for
this rocket that is going to take our crew from the surface of Mars back up into space, lift it
off the ground, climb out of the gravity well of Mars. that uses a tremendous amount of fuel. And of course,
it needs to breathe a tremendous amount of oxygen. So really, the customer for MOXIE
is primarily that ascent vehicle, that Mars ascent vehicle, that rocket that will return our crew
to Mars orbit as the first leg on the return journey, and which I think so many of us read
about and saw in the movies in Andy Weir's The Martian. You know, I was going to bring Andy up.
I'll save that for a moment, but it sounds like, you know, therefore, making the stuff that we need to breathe may just be a side benefit of what will someday be a fairly big plant to create this
oxygen that will be used as the oxidizer in those rockets when we want to come home.
It will definitely be a side benefit. One reason why it's a side benefit is, you know, the astronauts
can't wait till they get to Mars to have oxygen to breathe.
They have to bring it with them just to get to Mars in one piece and healthy and hale and hearty.
While the ascent vehicle can wait.
It doesn't need that oxygen until it's time to leave.
Have you ever talked with Andy Weir, the author of The Martian?
Not substantively.
I've emailed to him. I may have
had one conversation verbally, but haven't gotten to know him, no. I was curious because when he
first came on our show, he's been on a few times, he talked about that big oxygen generator inside
the habitat that played a pretty major part in the book and the movie. I'm just wondering, when you saw the movie, you must have been intrigued.
He told us he had based it on the research he'd done at the time,
but later learned it could have been a simpler and significantly safer device.
Was that right?
Well, first of all, before I saw the movie, I had read the book about three times.
Oh, yeah, me too.
And I've always said I'm indebted to him for making it so easy to explain to people what Moxie does.
I just say the word oxygenator and they say, oh, I get it.
I know how it works.
As for Safer, you know, he didn't say a lot about the technology that the oxygenator was using.
So that's not something I gave a lot of thought to.
Of course, Mark Watney did some things it wasn't designed for that were a lot more dangerous. And
he was dealing with, you know, with hydrogen and explosive constituents. There are different ways
you could do the oxygen generation. There are some that are, I think, arguably much better and simpler than the
way MOXIE is doing it, but just not ready to go, not ready for prime time. So it may well be in
the future that the solid oxide technology we're using for MOXIE is overtaken by, say, what's called a proton exchange membrane technology, which is
what's used, mass produced for hydrogen fuel cells. Because basically, the technology for
MOXIE is the same as a fuel cell. We just run it in the other direction to make an electrolysis
system. I'll be back with MOXIE Principal Investigator Mike Hecht after a break.
Still ahead is our discussion of the Event Horizon Telescope.
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Thank you.
Can you say a little bit more about how MOXIE achieves this?
Absolutely. Absolutely.
The trick, of course, is that you have on Mars very little atmosphere, but it's all CO2.
So when you total it all up, if you were to take a box full of air on Mars and a box full of air on Earth of the same size,
the box full of air on Mars would have 20 or 25 times as much CO2 in it, but very little else.
So you've got a lot of CO2 to work with. And the question then is,
how do you turn CO2 into O2? Well, you don't have to be a chemistry major to understand from that,
that it's already in there. You have to separate some oxygen from the CO2 molecule,
which has one carbon, that's the C, and two oxygen atoms, that's the O2.
There are two ways you could do this that you can imagine. One way is to just pull off the carbon
and be left with the O2, and that's not the way we do it. The other way is to pull off one of the
oxygen atoms and be left with oxygen and CO, which is what we call carbon monoxide. And I think most people are
familiar with that because you go and buy a little carbon monoxide detector to put next to your
furnace in the basement. It's nasty stuff if you breathe it, but it's also a gas. So given those
two choices of making carbon, which is candle soot, are making carbon monoxide, which is a gas
as the byproduct, carbon monoxide wins hands down. And so a lot of the technical difficulty with MOXIE
is just plucking off one oxygen atom without inadvertently plucking off two. Okay. So that's
the chemistry of how it works. And why do I say it's like a fuel cell?
Well, imagine the fuel cell reaction.
What you do in a fuel cell, you know, most people are familiar with hydrogen fuel cells, where you put hydrogen in, you put oxygen in, you get out H2O, which is the stable molecule,
the stable form, and you get out electricity.
If you did the same thing with a carbon-based system, you'd put
in CO, carbon monoxide, you'd put in oxygen, and you'd get out CO2, a nice stable molecule,
and electricity. That would be the fuel cell. Now, if you say you're going to run that backwards,
and literally that involves reversing the voltage, putting a negative instead of a positive voltage on.
If you run it backwards, you start with electricity, you start with CO2, and you get out CO and oxygen.
That's how we do it.
And that's, again, why you could convert it to a fuel cell easily with the same technology.
with the same technology. And it does it by a combination of, well, a very subtle combination of techniques, the first of which actually pull off this oxygen ion, since it's just one.
Then the real heart of it is the membrane that under an applied voltage pulls that oxygen ion
into a separate channel, a separate compartment, without pulling anything
else across. And that involves a very specialized ceramic heated to 800 degrees centigrade
with a very highly controlled voltage across it. And the current that flows in the circuit
is identical to the oxygen current. Oxygen ions produce a current, their charge,
an oxygen current flowing the other way.
And that's the circuit you make.
You have electrons flowing one way as electricity,
oxygen ions flowing through the membrane in the other direction.
That's the product that you're making.
You turn it around, you get a fuel cell.
Fascinating technology.
I mean, and when you talk about this needing to
be heated to 800 degrees, you start to understand the energy consumption that you were talking
about. I saw that MOXIE needs about 300 watts to do its work. Is that correct? And where do you
get that? I mean, that's a huge part of the Perseverance Energy Budget. Yes, Matt, that's absolutely right.
And this is why MOXIE will not run very often on Mars.
The expectation or the arrangement, if you will, with NASA is that we are scheduled in to run 10 times in the primary mission, which is one Martian year, so about two Earth years.
So in other words, every couple of Earth months that we'd be expected to run. Now, in practice, when you plan these missions, of course, there
are always opportunities that you take and you seize. And I'd be surprised if we didn't run more
often than that. But that's a primary reason. When Moxie runs, everybody else stands down and steps
back and waits and gets out of the way or takes a rare vacation day.
And an important thing to understand about how these Mars surface missions work is they
have a wimpy power supply, whether it's solar or whether it's the radioisotope version that
Perseverance uses, they're pretty wimpy. And so you never actually run off of the solar
panels or run off of the radioisotope source. You run off of a battery. And the battery charges up
all night long. That's really why they don't like to run these things at night. That's the
best time for charging a battery. And then when you're ready to go, you just drain the battery as fast as you need to.
So Moxie is designed to use the whole day's worth of available energy. I say available because the rover needs some, but everything else the rover isn't using, Moxie is using.
So when we're all done, we leave the battery the same way we found it.
We use a whole day's worth of charge.
same way we found it. We use a whole day's worth of charge. We bring the battery down to where it was when we started, when they started charging it up, and you're ready to go the next day as if
nothing happened. So we're energy neutral. The only thing we impose on our shipmates is a day off
when we run. Probably a well-earned day off. Oh, certainly a welcomed day off, I can tell you
that. How will you know that it's working, that it's creating the oxygen you hope to create?
Yeah, this was a source of, I'd say, creative tension all during the development of MOXIE.
We'd written the first sentence, I believe, or the first paragraph in our
proposal said, we're not just flying MOXIE to Mars to see if it works. We're flying it to Mars to
learn how it works. And we put all emphasis in the proposal on sensor systems, on really transparent ways to diagnose everything that's going on.
Now, you get down to then reality, you get down to the pragmatics, the nuts and bolts of developing
a system like this that is so, so immature when you start. And you're quickly overtaken by just
the need to make it work. Okay. So the sensor systems are maybe not all we hoped for,
but they're adequate. They're adequate. And we'll learn, we'll be able to follow
the gas as it flows through the system to know its pressure, to know its temperature,
to know its composition. We'll know the temperature everywhere in the system.
We'll measure these currents that are flowing through it. We'll measure the voltages flowing through it. A big part of MOXIE that I did not describe,
and a major consumer of power, that 300 watts you mentioned, is actually what we call the compressor.
And it is. It's like any other compressor you might buy to pump up your tires. It's a scroll
pump compressor. It uses a lot of energy. But the Martian atmosphere is very thin and you can't just sit and wait for it to come to you.
You have to pull it in. You have to suck it in and collect it. And we actually pressurize it as we do
that. You know, that's a key part of that energy equation as well. Fascinating. Again, this reminds
me of something else I heard you say.
When you were talking to the Mars Society Conference a few years ago, you said that
vacuum is a scarce resource, which is a pretty entertaining statement in itself.
But what did you mean by that?
I think the point I was making at the time was that the in-situ resource utilization
is maybe not even the right word for what we're doing. And I was suggesting that we should be talking about in situ resource transformation as the special thing that MOXIE and all the other ways of excavating and using resources accomplish.
And whether it's making cement out of Martian soil or growing plants on Mars. That's all a transformation of resources.
Utilization. We utilize resources every time we use a parachute on Mars. We're utilizing the
atmosphere. We're utilizing resources whenever we deploy a solar panel and collect sunlight.
And the point was that on Earth, I spent a good part of my career doing surface science, science of materials in vacuum systems and working very, very hard to find places in chambers on Earth that didn't have any air in it.
That's a very hard job. space shuttle program was to build a wake shield for the shuttle bay because it turns out even the
shuttle generates so much outgas that the vacuum around the shuttle by itself is actually fairly
contaminated with molecules and atoms and particles coming from the shuttle itself.
So they develop kind of a big umbrella that they drag behind them. So the area behind the umbrella is really a good vacuum.
And that could be used for vacuum manufacturing.
It's a scarce resource on Earth.
And to say it's plentiful in space is an understatement.
Talk about getting something from nothing.
Absolutely.
I did not know that about the shuttle.
Here's something else that only just occurred to me.
Where is the oxygen going to go?
The stuff that you create, you just release it or what happens?
Yes, unfortunately, we just release it when one thing we had hoped to be able to do.
And NASA, I think correct NASA correctly said, don't try to do too much, guys.
You know, this is going to be hard enough as it is.
said, don't try to do too much, guys. This is going to be hard enough as it is. But we actually wanted to reuse it. As I mentioned earlier, that MOXIE could be converted to a fuel cell.
And the original plan was to store a certain amount of the oxygen, then turn MOXIE the other
way and turn it back into CO2 and recapture some of the energy it had burned just to show that we could, in fact,
use this stuff as a fuel and burn it. I'm using burn colloquially in this case, burn it in a fuel
cell to make energy. In the end, we said, all right, this is not what we're focusing on right
now. We're focusing on making it. So we measure it and make sure it's pure and it's sort of a catch and
release, if you will. Release it back into the atmosphere where it gets diluted. There is a tiny
bit of oxygen in the Martian atmosphere as it is, a tenth of a percent. The oxygen we produce
pretty quickly gets diluted back into that background. The CO we produce pretty quickly finds oxygen
atoms to combine with and turns back into CO2. And so we will not leave any footprint on Mars,
but we're not utilizing it either. Like all good campers.
Like all good campers. That's right. Well, I wish we could say we were packing it in and
packing it out, but that will have to wait.
It sounds like there's plenty of room for MOXIE Mark II.
Oh, absolutely. So MOXIE Mark II, the idea follows what's been written about how we should send people to Mars.
Since back in the Wernher von Braun days and the early day of the space program, people thought about this really seriously.
and the early day of the space program, people thought about this really seriously.
I mentioned earlier that we have an opportunity once every cycle of Mars orbit. So all the plans have been designed around that 26-month cycle forever. And it's been a long time. I can't
remember the last time that someone wasn't sending something to Mars in that opportunity.
Boy, I mean, this year we've got United Arab Emirates going. There's been a lot of people taking advantage of
that 26-month cycle. The idea then is that before you send people, it would be really helpful to
have everything in place that they need. You know, I sometimes joke, you want to have your Airbnb all set up and waiting
for them so they just have to travel with a toothbrush. And so the idea you send among these
things you send early is you send an ISRU plant, you send a big moxie, right? That gets there in
seven months or so. The crew doesn't take off for another 18 months or so, 18 or 19 months. So you spend the
next 12, 14 months filling up the oxygen tank for the ascent vehicle. And then you say, we're done,
it's ready to go, and it's okay to launch the crew. That's sort of the synopsis of the strategy
of how you do this. I was in the room, I like to say, I've said to
Bob Zubrin, when he first presented many years ago now, the Mars Express concept, and got a
standing ovation after he had finished. And it has evolved over the years. And this kind of thinking,
this approach that you've just described, this is something that Zubrin had in mind from the
start, isn't it? Well, not just Zubrin. I said that goes all the way back to Wernher von Braun.
It's a colleague of mine, Don Rapp, who's written a number of books on the subject,
and he's a key member of the Moxie team in his 80s. We should all have such a productive
retirement as Don has had. I think he's published seven books since he retired.
such a productive retirement as Don has had. I think he's published seven books since he retired.
Don actually started accumulating plans that people have put together for Mars, for how to send people to Mars. And he counted to a thousand before he gave up.
And he says the vast majority of them, the vast majority of them, not all of them,
take this approach of saying you spread it over two cycles.
Ideally, you sustain it over many cycles.
So when you send the crew, as Andy Weir described, you also establish the infrastructure for the next crew.
journey is to travel from his landing site to the site that was already being prepared for the next crew where there was an alternate ascent vehicle. That's what that's about.
I think a lot of what you have talked about over the last few minutes demonstrates something else
I've heard you say, but I wonder if you could maybe give us another example of what you're
talking about when you say that we need to think like Martians. Yes, that's the hardest thing in the world to do is to think
like a Martian. This is what fascinates me about the study of Mars, the planetary science part of
it, because it makes you aware of just how much we take for granted, just how much is wired in about the way we interact with the
universe. And when you go to a place that's even subtly different, where the ground rules change,
where you have blue clouds and a pink sky, you realize just how much of a foundation your
world experience is imposed on what we see as objective science. It causes you
to rethink so many things. I love that experience. A simple example I love to give has to do with
temperature. Of course, everyone talks about temperature. It's too cold in this room. It's
too warm in this room. I feel a draft. And that is a deeply ingrained concept that is relevant
only in places like Earth that have an atmosphere that's so thick.
You know, to a Martian, we look like fish swimming in an ocean where we are walking around in such a thick atmosphere.
And it is so thick that, in fact, when the atmosphere is cold, we get cold.
And when the atmosphere is warm, we get warm.
And that is a unique characteristic of this kind of thick
atmosphere. And even today, I constantly hear engineering saying, oh, we shouldn't send humans
to the poles because it's too cold, or go to this other place where it's too warm. But I have to
stop them and say, now, wait a minute. Wait a minute. I mean, think about the atmosphere you're
talking about. Talk to an astronaut like my colleague Jeff Hoffman, who's the deputy PI from MOXIE and has flown in a shuttle five times.
You get into space, you're hot.
Now, is space hot?
Is space cold?
Well, neither.
And the reason it's neither is because we use temperature as a proxy for heat because on Earth, in this thick soup, you can use temperature as a proxy for heat.
If you're in space, you're hot if the sun is shining on you.
You're cold if you're in the shadow of the vehicle.
And at the same time, you're in this vacuum bottle and you're generating body heat.
And that's going to make you hot most of the time.
So temperature is not this characteristic
of the environment, right? Temperature is a characteristic of you or of your instrument.
And really the characteristic of the environment is all the heat that's flowing in and out and
radiating and convecting and conducting. That's what's characteristic of the environment.
So when I say think like a Martian, and I wrote a little science fiction story about this a long time ago.
When I say think like a Martian, what I mean is start off by imagining you lived on Mars and what would change and what would be different about your experience of the world.
And then ask how you apply that to the instruments or the systems or the processes you're building.
And you'll encounter some surprises if you do that.
That example you gave is exactly the one I was hoping that you would, Mike.
You know, we have spent a lot of time now talking about the red planet. In our last few moments, I want to turn to what easily could be an entire
different life for anybody working in the sciences. And that is this other title that you
have, Deputy Project Director for the Event Horizon Telescope, that made such big news when you and
your team released that first ever image of a black hole, or at least what was happening,
released that first ever image of a black hole, or at least what was happening, you know, what was going on around that particular black hole. So congratulations as well on that magnificent
effort, that tremendous success. I really wonder if there has ever been any kind of collaborative
achievement in science that equaled it. I think you would have to look at, for example, the high energy physics world
and some of the particle physics discoveries are in the astrophysics world. It's something like
the LIGO and the extraordinary detections of black hole collisions by LIGO that was a result of
years of effort of many, many people. It's an extraordinary testimony for who we are as people.
And honestly, the missions that we mount to Mars, if you think of the number of people involved,
that actually probably dwarfs the Event Horizon Telescope. I have been just extraordinarily
fortunate. I don't know how else to describe that. To have the opportunity on working on two such audacious projects in a short span of time as the Perseverance mission to Mars.
You know, talk about audacity and then the Event Horizon Telescope doing something that, you know, that that Einstein was sure was not possible.
And many people have been sure is not possible.
that Einstein was sure was not possible, and many people have been sure is not possible.
And being able to actually image something that is nearly inconceivable to our brains.
And talk about thinking like a Martian.
You know, this is a black hole.
A picture of a black hole causes you to think like someone outside of our universe, I suppose. To some extent, I was given this opportunity
because the two types of adventures have a lot in common, to try to achieve
extraordinary scientific results that requires tremendous coordination of infrastructure.
In the space mission world, it's everything from the people who build,
you know, the tanks for the rockets, to the software people, the software experts programming the, you know, the operations of the instrument. And then, of course, to people like you who are
letting the world know what we're doing. It's an extraordinary communal exercise of hundreds and thousands of people.
And to do what the Event Horizon Telescope has done and to coordinate so many facilities and installations around the world to all look at the same thing with the same equipment at the same time, you know, synchronized to picoseconds is extraordinary. And the fact that I had been involved with the Mars missions was my entree
into becoming involved with the Event Horizon Telescope. Hey, you know how to organize this
sort of big enterprise. Come help us. And I was able to apply a lot of what I had learned about
actually project management, as it turned out, for large scientific enterprises
to the Event Horizon Telescope. And that was my entree as someone who had straddled three worlds,
who had straddled the engineering world, the science world, and the project management world,
which are three different disciplines. And they turn out to be an extraordinarily powerful combination in just this sort of enterprise. Yeah, I can sure see the connection,
but it remains maybe the most interesting juxtaposition of professional duties of anybody
that I've talked to perhaps on this show. And that's 18 years worth of guests. Let me leave you with this. What is the EHT up to now?
Well, the EHT is, first of all, has a big piece of unfinished business. Everybody expected,
you know, back in April of 2019 to see a picture of Sagittarius A star, okay? And Sagittarius A star. And Sagittarius A star is the black hole, the supermassive black hole,
millions of solar masses in the middle of our galaxy, of the Milky Way. That's what everyone
expected to see. What we showed them was not Sagittarius A star. It was a black hole that should be called M87 star. We just tend to call it M87.
There was a Hawaiian name given to it a year ago, Pauahi. That is another galaxy,
not terribly far away as galaxies go, but galaxies are pretty darn far apart.
And it turns out, although that would be ordinarily a thousand
times fainter, it's also a thousand times larger. So it's brighter to begin with. And so it's about
as easy to see as Sagittarius, a star from the earth in that respect. And it also, because it's
so large now, and this is a relativistic issue, things can only change as fast as it takes.
In the amount of time it takes light to go across it.
So when something is as large as billions of solar masses like M87, it changes slowly.
Where Sagittarius A star being a smaller, only millions of solar masses, a smaller source changes rapidly. And that makes it that
much hard to get it to sit still for a picture. It's a squirmy toddler you're trying to take a
picture of. And it's been hard. So we've been working on that and working on that and working
on that. And it's close. That's going to happen. I can't tell you when. I can't tell
you exactly what will be in it. So that's one piece of unfinished business. And of course,
we're still trying to take data every year and have new campaigns. One of the things that
drives the schedule of the Event Horizon Telescope is there's really only one time a year
in March, April, where you get the confluence of circumstances where the sources are visible in
the sky because they move around the sky like any other sky object, and the weather is acceptable
at the different telescopes. There's only that one window every year that allows us to see.
This year, we couldn't observe because the telescopes,
critical telescopes were shut down because of the pandemic.
Last year, there were other circumstances that kept us from observing
that were a combination of weather and some telescope maintenance issues.
And the year before, 2018, we were somewhat, I won't say crippled,
but the observation was compromised by something as non-natural
as gang activity around the large millimeter telescope in Mexico.
There was armed gangs involved in piracy of gas pipelines,
and they couldn't get the crews to the telescope. So we have to fight everything from pandemics to
gangs to bad weather just to get an opportunity to observe each year.
But we're at the same time building up capability. The next time we observe,
we hope to observe in 2021, if all goes well, that we'll have more and more fidelity, more and more
data. So the next big thing, I think, will be movies of Sagittarius A-star someday.
Wow.
That's what we'd love to see.
Oh, I can't wait to catch that film.
That will be extraordinary. Mike, you have given us at least two very good reasons to invite you back.
Here's to a great successful landing on Mars in February and to clear skies, one might say, representative of all the other factors you have
to deal with to make the EHT do what it's capable of doing. Sounds like we very much might have more
to talk about. I hope you'll come back to the show. Matt, I would really look forward to it.
And I just want to say also, the US government, other governments don't give us all this money.
The U.S. government, other governments don't give us all this money, don't give us, in the case of Mars 2020, a billion and a half dollars or a billion dollars just for a sense that we are extending the human experience where it's never gone before. And it's folks like you and shows like this that actually fulfill that mission.
We're just the guys who do the work.
you're the guys who actually deliver the work to the people who are paying for it and who are receiving it and who are gaining from it.
So thank you for that.
Thank you and all your colleagues for doing what you do.
You are very welcome, Mike.
Thank you for those kind comments. And that's why we do the show because it's certainly why I do it,
That's why we do the show because, certainly why I do it, because it is a thrill to be able to talk to folks like you, leading teams that are doing this work that is expanding what we know of life, the universe, and everything.
Mike, keep up the great work, and I look forward to talking again.
Thanks so much, Matt.
So do I.
Mike Hecht of MIT is the Moxie Principal Investigator and deputy project director for the Event Horizon Telescope Collaboration.
Mars ahead when we join Bruce Betts for What's Up.
Season's greetings. Bill Nye here. The holidays are racing toward us.
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Thank you and happy holidays.
Time for What's Up on Planetary Radio.
So we are joined by Bruce Betts, the chief scientist of the Planetary Society,
who's here with me every week to talk about what's up in the night sky and much, much more.
Fun contest answers this time around.
Hi, welcome.
Hello.
I'm excited, Matt.
Were you excited a couple of nights ago as we speak?
Did you get to see the Geminids?
I got to see some clouds.
They were lovely.
Me too.
I looked a little bit last night after the peak because it was clear.
Didn't get to see that.
How about you?
No, no.
I only checked.
We were up in the mountains.
Nice dark sky,
new moon, as you've told us there would be, because you know, and now it was clouded over.
It was overcast. So no luck. I don't know. I didn't get up again at 2 a.m. to check either.
So what else is up there that we may or may not be able to see? Jupiter and Saturn. It's all about
Jupiter and Saturn for the next couple of weeks. You can ignore the rest of the sky.
It's not important right now.
Well, I mean, it's still fun.
But Jupiter and Saturn will be closer on December 21st than they have been in almost 400 years as they appear in our sky.
They'll be about six or seven arc minutes, so about a tenth of a degree apart.
And that is the equivalent of being closer than a quarter of the moon's diameter.
You should be able to resolve them still separated with decent eyesight.
They'll be looking really cool.
The challenge will be they're low, as you pointed out on a previous show, Matt,
they're already low in the west, not long after sunset.
So you'll want a pretty clear view to the west.
And if you have clouds the night of the 21st, take heart.
They're almost as close on the 20th and the 22nd.
So look in the evening west.
Jupiter, of course, is the really bright object, looking like a really bright star.
Saturn looking like a yellow star.
They should be in the same field of view for binoculars or
most home telescopes, unless you get to a bigger telescope. So it's going to be groovy. Watch them
get closer together coming up on the 21st and getting farther apart after that. We've got an
article coming up on our website with more information at planetary.org. Did you have any
further thoughts upon this, Matt?
Well, you did get this text message, came in moments ago from Mars,
regarding comment, ignore rest of sky, what am I, chopped regolith?
Oh, okay.
Several questions come to mind.
Strangely, the first to pop into my head was not why Mars was contacting us,
but how it got around the light speed limit on communication.
And I didn't know Mars could listen to the show early when we were recording.
I'm sorry, Mars.
We make it available.
Check out bright Mars, still bright in the south when you're done looking at Jupiter and Saturn.
Or if you're an aerophile, just go ahead and check out Mars first and then Jupiter and Saturn, or if you're an aerophile, just go ahead and check out Mars first, and then Jupiter
and Saturn. You know, you know
Mars, you are far more than Chopper
to me. Wait, we just,
there's another text coming in.
Oh, it's a red smiley face. I think
we're good.
Oh, and
before anyone gets angry,
Venus, pre-dawn,
sorry. And there are stars. There are so many stars. But Jupiter and Saturn When before anyone gets angry, Venus, pre-dawn, east. Sorry.
And there are stars.
There are so many stars.
But Jupiter and Saturn doing something kind of special.
That's all I'm saying.
Mars is, of course, always special and near and dear to my heart.
I think we're good.
On to this week in space history.
It was 1968 that Apollo 8 launched and sent the first humans around the moon.
We move on to random space fact. A little trill. I like it.
Almost all Mars landers, and perhaps somewhat coincidentally, all successful Mars landers,
have been targeted to land northwards of about 15 degrees south on Mars. That's because
Mars has this general topographic dichotomy with highlands in the south and lowlands in the north,
at least on average. With Mars's atmosphere already really thin, landers need to get all
the atmosphere they can get to slow down, and hence the targeting of lower elevations.
and hence the targeting of lower elevations.
We move on to the trivia contest, and I asked you how many aluminum panels are or were in the Arecibo radio dish.
How'd we do?
A great response to this.
I don't know if it's because everybody wants to proudly wear that new Planetary Society cap,
which we will once again be giving away this week, or if they just, it was in honor of Arecibo. Here is the answer hidden away in this week's submission from our poet laureate, Dave
Fairchild. Down in a sinkhole, they built Arecibo at 305 meters wide, inverted dome in its Green
Island home with thousands of panels inside, made of aluminum, I'd say by rule of them,
island home with thousands of panels inside, made of aluminum, I'd say by rule of thumb,
seven by three feet across. 38, seven and seven, eight rectangles make this great telescope boss.
Easier to understand? How about from Matt Cotter in Missouri? 38,778 panels and one Bond villain.
They get the number right? They did.
They did indeed.
That's a lot of panels.
Chris Mills in Virginia.
He had the same number.
It took a while to count them, though, from the aerial photo.
I hope I didn't miss one.
Wow.
I mean, they were good on you.
In Illinois is Henry Anderson, who gave us the answer in Spanish,
which I will not read because it would be an insult to all of our Spanish-speaking listeners to hear me attempt that.
You know we love it when we get unique units of measure.
From John Borrelli, total square footage of 814,338 square feet or big enough to fit 101.8 Planetary Society headquarters.
Wow.
That's impressive, isn't it?
I think it would fit 101, but I didn't know about the extra.8.
That's cool.
That's what makes the difference, that.8.
Here's our winner.
Sorry to keep stringing you along.
Corey Schmidt, first-time winner in Missouri.
They are, and then in parentheses, were, PSI, 38,778 panels. They
replaced the original wire mesh that was installed in 1963 when the dish opened. And then he added
this, I luckily got a chance to visit the observatory a few years back while living in
Puerto Rico and still have fond memories of my visit. I bought a commemorative pint glass as a
souvenir, and from now on, every beer I drink from it will be bittersweet. Corey, congratulations.
Nice message, and we hope this sweetens the memory a little bit. Maya Sukup in Newfoundland, Canada,
as a geoscientist learning from your podcast that the dish was built into an extended limestone
valley, that's something that Bill and I mentioned.
And that the contents were then used to construct support materials was very interesting.
I wonder if they'll need geologists to find the next site.
Are you volunteering, Maya?
Just a couple more here.
Fingers crossed, says Darren Ritchie, for a good starship test today.
He wrote this a few days ago.
With that kind of payload capacity, perhaps an Arecibo
2 on the lunar far side would become feasible, would be a worthy successor. I don't know. What
do you think? I think it would be incredibly challenging and expensive. It would be. I mean,
cool results, but economically and feasibility challenged. Probably not a lot of profit in it
either for SpaceX. Finally, this from Gene Lewin
in Washington. A loss to all, though not all know the impact of this tragic blow. A limestone cradle,
a karst was home to this Gregorian inverted dome. This void created by nature's wrath impedes our
travel, but not our path. Rebuild this wonder, return our sight. Reveal the mysteries of distant light. I'm going
to send that one to Francisco Cordova, I think, the director of Arecibo. Yeah, that's nice.
That's it. A lot of stuff there. So I guess we better move on. Returning to Martian topography,
in what feature is the lowest point on Mars? Go to planetary.org slash radio contest. Oh, wait, I got
another text here. It's Mars again.
All is forgiven. Aww.
You have this time until
Wednesday.
That'd be Wednesday, December
23rd at 8 a.m. Pacific
time. Your prize,
should you get it right and be chosen,
is going to be that
Planetary Society baseball cap, which is now
being featured at chopshopstore.com or just go to planetary.org slash store. And you can check out
all our other merch as well. I think we're done. All right, everybody go out there, look up the
night sky and thinking about using light waves to look at ocean waves, making sound waves that you hear.
Thank you and good night. Okay, I got to ask, is this happening? Only in my mind. It sounds
brilliant, though. Maybe some new Earth-observing satellite from NASA. All right, well, they owe you
if they turn this into music. That's Bruce Betts, the chief scientist of the Planetary Society,
who joins us every week here for What's Up.
Planetary Radio is produced by the Planetary Society in Pasadena, California, and it's made possible by its oxygen-loving members.
I promise you that joining them at planetary.org slash membership will be a breath of Fresh Air. Mark Hilverdes and our associate producer, Josh Doyle, composed our theme, which is arranged and performed by Peter Schlosser.
Ad Astra.