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Gravity Assist: Mars with Bruce Jakosky and Michael Meyer

The largest canyon in the Solar System cuts a wide swath across the face of Mars. Named Valles Marineris, the grand valley extends over 3,000 kilometers long, spans as much as 600 kilometers across, and delves as much as 8 kilometers deep.
Credits: NASA

 

Gravity Assist: Mars with Bruce Jakosky and Michael Meyer

Transcript:

Jim Green: Our solar system is a wondrous place with a single star, our Sun, and everything that orbits around it – planets, moons, asteroids and comets – what do we know about this beautiful solar system we call home? It’s part of an even larger cosmos with billions of other solar systems.

Hi, I’m Jim Green, Director of Planetary Science at NASA, and this is Gravity Assist.

With me today is the “man about Mars,” Bruce Jakosky from the University of Colorado. He’s our principal investigator of NASA’s MAVEN mission.

Now, MAVEN was launched in 2013 to study the atmosphere of the Red Planet. MAVEN’s been in orbit doing fantastic observations of the solar wind. You know, many in the public don’t realize that the Sun constantly out-gasses in every direction, and we call that solar wind. And it has enormous effects on our environment. That’s what the planets are swimming in.

And MAVEN is designed to study that in its interaction with Mars. So, what have you found out?

Bruce Jakosky: We’ve been looking at the way that the solar wind and the sunlight hits the Mars upper atmosphere and can drive gasses from the atmosphere into space, in effect the way the Sun and the solar wind can strip gasses away from the planet. Over the long term, that has the ability to change the climate by removing so much gas from the atmosphere.

What we’ve discovered is, in fact, that is what’s happening. The bulk of the atmosphere, the large fraction appears to have been removed to space. And that stripping of the atmosphere appears to be responsible for changing the planet from a warm, wet environment early in its history to the cold, dry environment we see today. That’s a major change.

Jim Green: What’s really spectacular about the data that you’re taking and then the visuals that you create globally of what’s happening on Mars is where that escape is coming from and what does it look like from a global perspective. Can you describe that?

Bruce Jakosky: We’re seeing a lot of different processes taking place and all adding up. Hydrogen, for example, comes from water in the atmosphere, and hydrogen, if light enough, it can just escape to space directly. Things like oxygen, which come from water or from CO2 carbon dioxide in the atmosphere, are not light enough that they can just escape on their own. They need the solar wind to grab them and knock them out.

So, we’re seeing a lot of different processes, trying to understand how they play together.

To me, what makes this exciting is that we’re looking at the thin, tenuous part of the upper atmosphere—so thin that we would call that a vacuum if we were doing experiments here on Earth. Yet, that’s where all the action is in affecting the climate at the surface of the planet: the ability of water to flow over the surface and really controlling the degree to which Mars could have been habitable by microbes.

Jim Green: Some of the processes at Mars are unique in the sense that we don’t experience them in and around our Earth because of our strong magnetic field. So, you do have a magnetic field on MAVEN, and you have been measuring magnetic fields. What are you finding out?

Bruce Jakosky: We have a magnetometer in order to measure the properties of the solar wind as it comes in and also the, what I’ll call the morphology of how the solar wind interacts with the planet. It turns out that there are regions of the crust that have a magnetic field. Mars doesn’t have a global magnetic field, but it has localized crustal magnetism, and those create little pockets of protection over the atmosphere where the solar wind can’t hit them.

But, they cover a very small fraction of the surface. And overall, we’re seeing interactions between the solar wind and the ionosphere and the planet that have a significant effect.

MAVEN Principal Investigator Bruce Jakosky, University of Colorado
Credits: Merry Bullock

 

Jim Green: What really intrigues me about that remnant magnetic field, you know, that stuff that’s trapped in the crust that you actually measure is it’s a hint of the past. What do you think happened to the magnetic field?

Bruce Jakosky: Well, you’ve got it exactly right. Mars appears to have had a strong magnetic field, global magnetic field early in its history. And that magnetic field is recorded in the ancient crust. The younger crustal regions don’t have it, so we think the magnetic field disappeared.

The magnetic field on the Earth is formed by motions within the molten iron core. You have an electrically conducting material like metal, and it’s moving, and it creates a magnetic field. Mars would have done the same thing early in its history, but when the magnetic field stopped, that must have indicated that the core froze out, it became solid. The Earth’s core is still molten, is still generating a magnetic field that we see today, but Mars has stopped.

Jim Green: You know, here on Earth, one of the things that everyone knows is that our magnetic field helps organize particles, and we see occasionally aurora when the Sun gets really active and hammers our magnetosphere. So, there’s remnant magnetic fields on Mars, but does Mars have aurora?

Bruce Jakosky: It does, and in many ways, it’s more interesting than what we see on Earth–of course I’m gonna say that–because on Mars, we don’t have a magnetic field to stop the solar wind. So, the particles from the solar wind come in and can hit the atmosphere directly. So, we see aurora generated by electrons that are hitting the atmosphere, and they’re spread out over the whole planet rather than concentrated in northern latitudes as on the Earth, northern and southern latitudes.

In addition, we see aurora generated by hydrogen hitting the atmosphere. And occasionally, we see aurora created as these particles from the Sun hit the crustal remnant magnetic fields and get focused into small regions, and that’s the most analogous to aurora on the Earth because it’s connected to the magnetic field. But, most of the aurora on Mars aren’t connected to the magnetic field.

NASA’s Lead Mars Scientist Michael Meyer
Credits: NASA

 

Jim Green: You know, one of the spectacular moments that we had in planetary science was the passage of an Oort cloud comet right in front of our planets. You know, we think about how that may influence our climate, our activity by being hit by objects, but here is a comet, you know, and indeed Siding Spring passed by Mars. What was that like in the MAVEN data?

Bruce Jakosky: Well, let me start by telling you what we thought when we heard about Comet Siding Spring for the first time. It was discovered about a year and a half before MAVEN launched, and when it was initially discovered, they didn’t know the orbit well enough. There was a chance it could hit Mars. And my first reaction is, “Oh, my God, if it hits Mars and we’re in orbit around it, the debris sent up by that impact would destroy our spacecraft.”

Fortunately, as they learned more about the orbit, they knew it would pass close but not hit it (Mars). And the orbital dynamics was such that MAVEN would get there a month before the comet and there was nothing we could do about it.

We were worried about surviving the comet passage because of all this dust that comes off the comet, and we debated: should we put extra shielding on the spacecraft—what should we do? In the end, we did the thing that the engineers were most comfortable with, which was nothing. We took no precautions on the spacecraft, but operationally, we did. When we were in orbit around Mars, we timed where we were in our orbit, so that we were shielded by the planet for about 20 minutes during the time of the peak dust flux to protect the spacecraft. For several hours, we turned edge on to the flow of dust in order to minimize our cross sections so that less dust would hit us, and we survived. We couldn’t even tell that there was a comet there from the spacecraft itself.

Jim Green: Well, you know, that must have been a spectacular event if you were standing on Mars, looking up at night, seeing the material coming in, just like our shooting stars here.

Bruce Jakosky: We see on Earth meteor showers that are pretty spectacular, but they’re left over from dead comets. To have a comet pass this close to Mars, only 140,000 kilometers away, and to have the coma of dust and gas hit the planet directly, it would have been a spectacular event to see.

Jim Green: Well, you know, I was delighted that all our spacecraft survived, you know, that we didn’t have major problems with those. But, you know, there are other objects in orbit around Mars that, as I understand, MAVEN had to avoid. Can you tell us a little bit about your encounter with one of the moons?

Bruce Jakosky: Well, let me start with the difficulty we have in orbit because there are a lot of spacecraft, and their orbits evolve with time. And every now and then, the orbit of MAVEN will cross the orbit of one of the other spacecraft. We call those “COLA” seasons, (short for Collision Avoidance).

We occasionally, maybe once or twice a year, have to do a maneuver to make sure we don’t come too close to another spacecraft. But, recently, we had a collision opportunity–maybe that’s the wrong way to put it, but a possibility that we would collide with the moon Phobos, and in that case, the orbit predictions were such that we were definitely gonna hit it if we didn’t take action. We did a maneuver about five days in advance of that (predicted) collision in order to avoid it. So, instead of hitting it, we missed it by about 200 kilometers. We have to watch constantly every day to make sure we’re not going to hit something.

Jim Green: Yeah, that’s unbelievable. You know, it’s getting crowded at Mars, so to speak, but in a nice way. This is the way I like it.

In this image taken by the Viking 1 orbiter in June 1976, the translucent layer above Mars’ dusty red surface is its atmosphere. Compared to Earth’s atmosphere, the thin Martian atmosphere is a less powerful shield against quick-moving, energetic particles that pelt in from all directions – which means astronauts on Mars will need protection from this harsh radiation environment.
Credits: NASA/Viking 1

 

Bruce Jakosky: Well, today, there are five or six spacecraft in orbit: MAVEN, Mars Reconnaissance Orbiter, Mars Odyssey, the Indian MOM (Mars Orbiter Mission), the European Space Agency Mars Express, and their recent addition, the Trace Gas Orbiter. And these are the ones that are operating today. In addition, there are “dead” spacecraft – Mariner IX, Viking I, Viking II, the Russian Phobos Mission. All of these are in orbit, and it’s getting pretty crowded there.

Jim Green: Yeah, and Mars Observer, as I remember.

Bruce Jakosky: No, Mars Observer sailed on by without stopping.

Jim Green: We’re sure of that? (laughs)

Bruce Jakosky: Yes.

Jim Green: Well, you know, Mars is hard. Sometimes, we can’t always pull off what we want at that planet.

I’m here with Bruce Jakosky, my Man about Mars, and we’re talking about that fabulous MAVEN mission. I’m always interested in how we get into this business. You know, this is an exciting thing to do, and everybody I talk to, there’s typically something happens that gives them that “gravity assist” that propels them into the science that we’re doing. What was that like for you?

Bruce Jakosky: You know, I was always interested in space, and I remember being a six-year-old sitting in front of the TV watching the countdown of the first Mercury astronauts in the very early 1960s. But, for me, what really sent me on this path was when I was an undergraduate at UCLA. I was a physics major, and I got bored with the classes because all they were doing was teaching us tools and techniques.

So, I started looking around for something else, and I took a planetary science class from Hugh Kieffer, who was one of the professors there. By the end of the semester, I had changed my major. I was working for him on the Viking Mission, and that really sent me on this path. So, it happened to be one class that happened to be offered when I was looking around for something else to take.

Jim Green: Thanks, Bruce.

Well, we figured out how Mars lost its atmosphere with MAVEN. Now, here to talk about a couple other Mars mysteries is Michael Meyer.

Michael Meyer: Good to be here, Jim.

Jim Green: Michael is our lead Mars scientist at NASA Headquarters.

I’m really intrigued by some of the recent measurements of methane on Mars. Michael, what’s going on?

Michael Meyer: As you might remember, a couple years ago, when we first started doing the methane measurements, we got–all of a sudden, boom, we got this big spike in methane. And then almost as surprising, it disappeared. And you have to kind of go through chemical gymnastics to get methane to show up and get methane to disappear. And so, this–the modelers, you know, atmospheric modelers are just, you know, they’re just in a tizzy over this because, how is this possible?

So, as we go along, we get a low background of methane, which is fine because you can expect, in fact, inputs from comet material to be, you know, just enough to give us some methane. But, then we found another spike, and then it disappeared.

And we’re not getting any correlation with anything else that’s going on as we’re exploring. So, this is a real mystery.

And it is important because, you’re right, it can be a sign of geological processes where rock is interacting with water. If you can pick the right rock, you get methane generated.

And so, there would be an active geologic process going on, which would be really interesting.

Jim Green: Equally exciting, yeah.

Michael Meyer: Yeah.

Jim Green: It’s an active planet.

Michael Meyer: And we know on this planet, most of the methane that we see is biological product. So, of course, that would obviously be very exciting on Mars, too. Either way, it’s a mystery that needs to be solved because we have to figure out what the source is.

Jim Green: One of the more spectacular sets of observations that the Mars Reconnaissance Orbiter has been seeing are these recurring slope lineae, and there’s been some observations in and around Gale Crater that seem to indicate streaks coming down Mount Sharp. What’s our current thinking about those?

Michael Meyer: Yeah, so recurring slope lineae (RSLs)—it’s a mouthful for basically something that shows up seasonally. And, you know, so in the spring when it starts warming up, they appear. Through the summer, they get longer down a slope. In the fall, they start to disappear. In the winter, they’re gone. And the next year, it happens again, and it happens in the same place, and you’re going this looks like water flowing down the slope.

But, it’s hard to explain that being water just because the temperatures are that low, there isn’t that much water on the surface of Mars at all because water’s not stable on the surface. What’s going on?

So, yeah, there have been a couple of candidate recurring slope lineae in Gale Crater, but they’re not very good. I think we only have one or two where the jury’s still out that they might be, right?

But, we’re finding them all around the planet. Mars Reconnaissance Orbiter has been doing a fantastic job of looking at the surface of Mars and seeing change. And it’s only because they’ve been there for a while that you could see the seasonal progression and digression of each of these things.

Jim Green: Well, you know, we needed the Mars Reconnaissance Orbiter’s capability with its high-resolution imager, you know, something that could see a coffee table, you know, if it’s sat down on Mars, to be able to find these because they’re only, you know, a few meters wide. They may be football fields long–.

Michael Meyer: –Right, right.

Jim Green: But, you know, that just gets averaged away with our low-resolution imagers. They never see it.

Michael Meyer: Well, in fact, one of the challenges and why they’re still a mystery is with our spectrometers, when we’re looking at the colors of these things to tell what the mineralogy is and, you know, what rocks are, whether or not there’s water there, they’re really not large enough to get a good spectra.

So, we don’t see a real change in the spectra over the seasons. So, then you have to wonder what’s causing this.

Jim Green: Yeah.

Michael Meyer: It goes dark, it gets light, what’s going on because you don’t see it with your other instruments. But, we know it’s real. We know that something’s happening, and we don’t have a good explanation yet.

Jim Green: So, I think we’ve got to go see one. You know, I think we’ve got to get up close and personal, really, to understand what’s going on. So, I think that’s in our future. We’ve got to go visit an RSL.

Michael Meyer: Well, certainly, the candidate ones that we’ve been talking about in Gale Crater, we have marked out observation posts. So, there’s spots as the rover goes along. Way in the distance, it could see the candidate RSL (recurring slope lineae) and will image them. And, you know, of course–.

Jim Green: –At high resolution–.

Michael Meyer: –High resolution, plus it has spectrometers, right?

Jim Green: Yeah.

Michael Meyer: And so, it’s one of these things where now we can get a different look at it. It can look at it over better periods of time because MRO (Mars Reconnaissance Orbiter) can only see it when it passes overhead.

Jim Green: Right.

Michael Meyer: And maybe it’s not a good season because it’s the dust season, and so, you know, from orbit, it’s obscured.

Jim Green: Uh-huh.

Michael Meyer: But, from the surface, you may still be able to see it. So, we have high hopes that, as we go along over the next year and we have these observation posts, we can watch it and see whether or not this is, well, is this really real or is this like a shadow that shows up and disappear, or is it really something that’s happening on the surface. And then because we can look at it with multi-colored eyes, we can get a better handle on what actually is the cause of the mechanism.

Jim Green: You know, Curiosity’s been doing fantastic, and it’s really being a pioneer, telling us that there are regions on Mars that could have been habitable in the past. And that means the next mission–right now we call it Mars 2020–is going to have an opportunity to go to those places that Curiosity is uncovering for us that will enable that mission to make even greater progress. So, what’s happening in that area?

Michael Meyer: You said it very well. I mean, 2020 is really standing on the shoulders of Curiosity in a couple different ways. One, it’s using the whole architecture of the mission, of the entry descent and landing, the rover body itself that has worked so well we’re doing it again.

Good news is that we’re adding brand new instruments, we’re updating everything, and it’s gonna cash samples, so that when it finds interesting rocks, we have the opportunity to bring them back.

So, the other thing where 2020 is standing on the shoulders of Curiosity is what Curiosity learns has told us that Mars was habitable during the period of time that Gale Crater was formed or soon after that. Some of the things about the mineralogy, about the rocks that tells us what the environment was like. So now, the instruments that we’re sending on 2020 are informed by that, and then picking the landing site for 2020 to go to is informed by what we’ve learned in Gale Crater and from information we got from orbit so that we’re much more sophisticated on where should we go to get the right rocks that are gonna tell us something about the early history of Mars during the period of time that life started on Earth, that life started in our solar system.

Jim Green: We all get into this field in various ways. It’s just fascinating to me to see how we just turn our attention into space. What was that “gravity assist” that pulled you into this science?

Michael Meyer: You know, it’s a pretty tortuous route from me getting interested in science and actually ending up in the Mars program. But, I would say the first thing that really got me was I’d been a fan of Jacques Cousteau, I liked the oceans, I had an aquarium. You know, I was interested in that. I liked to sail–you know, I liked being on the water. Everybody likes being on the water.

And I got hired as a deckhand with a treasure salvaging operation off the coast of Florida. That, in and of itself, is pretty cool.

But, the big thing was, after I was there for a couple of weeks, the head of the operation fired all the divers because they were, you know, they were just not doing the job. And so, then he asked me if I wanted to dive. Sure, I don’t know how to dive, but I’d be happy to. And so, I got my opportunity to go scuba diving and help with the treasure salvaging.

There it was, my first foray into the subsurface, and like I looked at this world, and despite all the TV shows I’d seen and the occasional book, I looked at this and I went, “My word, I don’t know anything about this world. This is fantastic. Look at all this stuff.” I was just blown away by how fantastic it was, even though I thought I knew a lot about the oceans.

And that set me on the track of, “You know what, I–I could do this for the rest of my life,” type of thing.

Now, how I got to Mars is a whole different story, but that got me interested in the science and looking ahead beyond just going to college, but, you know, graduate school and realizing that I could actually make a living by learning things. It was great.

Jim Green: Thanks, Michael. Join us next time as we continue our virtual tour of the solar system. I’m Jim Green, and this is YOUR gravity assist.

End

source: NASA – Jet Propulsion Laboratory – California Institute of Technology

 

 

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