Q & A with Dr. John Mather on the James Webb Space Telescope

The James Webb Space Telescope (JWST) is the much anticipated, long awaited “next generation” telescope. Planned for launch in 2013 October 2018, fall of 2021, JWST has been touted as the successor to the Hubble Space Telescope. With it, astronomers hope to look back in time to when the universe was just 200 million years old, and see the first stars and galaxies. The lead scientist guiding this project is Dr. John Mather, co-recipient of the 2006 Nobel Prize in Physics for his work with the Cosmic Background Explorer (COBE), which measured the black body form and anisotropy of the cosmic microwave background.

We were understandably honored when Dr. Mather contacted Universe Today, saying he’d like to talk with us about the status of JWST. “I figured it might be time to talk about what we’re doing,” he said, “because exciting things are starting to happen.”

Dr. John Mather. Credit: (NASA/Bill Ingalls)
Dr. John Mather. Credit: (NASA/Bill Ingalls)

Universe Today: Dr. Mather, for over a decade we’ve been hearing about the Next Generation Space Telescope, which later was officially named the James Webb Space Telescope. Can you tell us how the concept for this telescope began?

John Mather: In 1989, even before the Hubble was launched, a conference was held about what the next space telescope should be. They discussed great telescopes of the future and from the proceedings, published a book. But they really didn’t consider that infrared was the great wave of the future. Then, in 1993, there was a committee called HST and Beyond. They published a lovely little report in 1996 that said there were two important things to do. One was to build an infrared telescope, unlike what the previous book had said, and the other was to build a telescope to search for Earth-like planets. At that point, astronomers were just recognizing that searching for extrasolar planets was possible. So in October 1995, NASA Headquarters called me up, gave me a list of scientists and engineers to contact and said to start planning. So we did, and we immediately came to a remarkable convergence of thought and opinion. We quickly agreed on a concept which met the wishes of the scientific community and came within the ambitions of NASA. You’ll find that the telescope we wanted to fly back then is very much like the one we’re going to fly in 2013.

UT: Can you give us an update on the status of the JWST right now?

Mather: The flight instrument hardware will be coming in from all over the world in the summer of 2010. The fine guidance sensor comes from Canada, one and a half instrument packages come from Europe and the rest comes from the US. So, in 18 months the instrument package starts going together, and then it meets up with the telescope around a year later. The four science instruments are a near-infrared camera, a near-infrared multi-object spectrograph, a mid-infrared instrument, and a tunable filter imager.

We just went through the Critical Design review for the instrument module. Last week we had hundreds of people come to look at everything and tell us if we’re doing it right. I think we passed, although I haven’t seen the official paperwork yet. But even I was impressed.

UT: The question many people ask me is, since Hubble has been so successful, why isn’t JWST going to be an optical telescope?

Mather: Why did the committee change from optical to infrared? It was twofold. One was that Hubble was getting so good, they could see it would be hard to beat it, no matter how big you built a telescope. Another thing happening was that people were seeing you could build big optical telescopes on the ground. The Keck Telescope was working really well, and people were starting to talk about adaptive optics, which meant even bigger telescopes on the ground were worthwhile. So those two things pointed us towards an infrared telescope. Also all the scientists of the JWST said we needed infrared. From the little capability we did have at the time, infrared was fascinating, finding that the most distant universe is exciting and is red-shifted from the visible. It starts out in ultraviolet and gets to infrared because of the great distances of these objects and the huge red shift they have. So if you want to do ultraviolet astronomy at the almost-edge of the universe you need an infrared telescope.

A full-scale model of the JWST.  Credit: NASA
A full-scale model of the JWST. Credit: NASA

UT: Now that the infrared Spitzer Space Telescope is up and running so well, has that changed anyone’s mind, or does that make scientists want to go to the next level with infrared?

Mather: Yes, Spitzer has proved this is actually a fascinating territory. Spitzer is actually a little bitty telescope by modern standards; it’s only 3 feet wide, 85 cm. But it has been producing some astonishing surprises. They can see things out to very, very high red shifts, and none of those things were expected. So, that tells us infrared is where the wonderful discoveries will be. We now know we can do the technology, so let’s get a better telescope. The science is way, way exciting, and there’s so much out there waiting to be discovered.

UT: In your opinion, what will set the JWST apart from previous space telescopes?

Mather: Every telescope says, “I’m better than the one before me,” and we say the same. Of course, this telescope will see farther back in time with its infrared capability and its huge aperture; it will see through dust clouds to see where stars are being born; it will see things that are room temperature, like you and me, planets, or young stars being born. All those things can be seen directly with the infrared capability we have on this new telescope. Most of the work will be done in infrared, with some capability in the visible range.

But we’ve built a general purpose telescope. After launch, scientists can write proposals as they do for Hubble, for what they would like to observe, so they can observe whatever the hot topic is at that time.

Fully functional, 1/6th scale model of the JWST mirror in optics testbed. Credit: NASA
Fully functional, 1/6th scale model of the JWST mirror in optics testbed. Credit: NASA

UT: With your experience with COBE and the subsequent honors you received, how have you applied that to the JWST?

Mather: It wasn’t so much the honors that affected my life, it was the fact of having been through the process from the very beginning to the very end for a very radically designed observatory, which COBE was, that gave me the nerve to think big things. So when NASA Headquarters said they wanted a successor for Hubble, I thought that would be interesting, and I had enough nerve to say yes, I’d like to try that. COBE was very ambitious for the time, but small enough that I knew the engineers personally and I could talk to them any day about anything. So I thought I could graduate to a bigger project.

UT: And now you’re working with people from all around the world?

Mather: Yes, this is a huge deal. Our science team is about 19 people, from Europe, the US and Canada. The engineering team is over 2,000 people who are spread out all over the world. Clearly, I don’t know all of them. I work with the scientists most closely and talk with them about what we want to accomplish, and make sure we are accomplishing that. So I have a different role now. I don’t have hands-on responsibility for any hardware, but I work with the people who do. We have access to some of the very best people in the world on every topic.

UT: Can you talk about of the problems this telescope has had to overcome, the cost overruns and the delays it has had?

Mather: Number one, the cost overrun is not as big as is being portrayed by some folks that would like the money for their own project ideas. Originally Dan Goldin was the head of NASA when we started, and he said, “We want you to think of a way to do this observatory for a half a billion dollars in 1996 dollars.” We said we’d try. But we quickly realized building this was going to be hard. By the time we got ready to present it to the decadal survey in 2000, the cost was more like one billion dollars. Then, three years ago, we saw that the job was getting harder and we had to replan and rebudget. Now, if you count the entire NASA cost from beginning in 1995 to the end, somewhere after 2019 with inflation and civil servants (which we weren’t counting before) now it is roughly $4.5 billion in actual real dollars, not 1996 dollars. So there is cost growth, but we have had excellent success and we’re on track to launch this wonderful machine, which will be used by thousands of astronomers. And we haven’t had to change our plan or our total budget in three years, thanks to steady leadership from NASA HQ and brilliant technical work by the teams.

UT: That’s good to know. I think people have a general concept that the JWST has had a huge cost overrun.

Mather: Well, it’s not something small, and we wish we could have done better on that. But it’s about a factor of two growth, and not the factor of five that has been advertised by some people who should know better. This telescope will work for a long time. The requirement is five years, but we’re hoping to run it for ten. So, our project spans from 1995 to maybe 2024 when operations would end.

Engineers from Ball Aerospace inspect the first James Webb Space Telescope mirror segment upon its arrival at Marshall Space Flight Center, Huntsville, Al. for cryogenic testing. Credit: NASA
Engineers from Ball Aerospace inspect the first James Webb Space Telescope mirror segment upon its arrival at Marshall Space Flight Center, Huntsville, Al. for cryogenic testing. Credit: NASA

Let me give you some idea of what we needed to do to get ready and what we’ve been up to all this time. We developed a list of ten major technologies that we needed. The hardest thing was to develop the mirrors. That required twelve different contracts just for developing the competitors to where their designs were good enough, so that took quite a few years. The detectors clearly had to be improved over what we have on the Spitzer and Hubble telescopes. So now we have bigger and better detectors, and they are fabulous. One measure astronomers have is how many stray electrons do you get from the detectors. If you close off all the light you should get zero. We now have detectors that give off a few stray electrons per pixel per hour, which is almost perfect. It would be good to be even better, but this is fabulous. I’m impressed.

We needed to improve on the refrigerators in space. We started off saying we need to get a radiatively cooled telescope so that it would be cool enough by itself, and that’s mostly true. But it turns out we still need an active refrigerator to keep the longest wavelength detectors cold, so we had to develop that.
So, those are just some of the things we had to design, and all the technology development was finally finished in 2007 and passed the review board’s approval, who said,”Yes, those things are finally ready now to be built.”

So, just getting to 2007 was a long time, and I don’t think people have really appreciated what it takes to get new technologies ready. On the other hand, we’ve been blessed by not having to “back up.” We put enough planning and effort into these technologies that they work now. That was one of the things we learned from the Hubble project, which was, don’t finish your design until you know what you’re supposed to build.

UT: How about your testing process. Is it pretty rigorous?

Mather: That is another lesson we had to learn from Hubble. If you don’t test it, it’s not going to work. We’ve learned to have a very determined and rigorous process. They did enough testing on the Hubble that they could have known about the mirror focus problems. The mirror manufacturer had two tests that didn’t agree and they decided to ignore one of them instead of tracking down the reason, and that turned out to be foolish and expensive.

We have a generalization that if anything really matters, do it twice. We will actually test the telescope cold in the big vacuum tank down at Johnson Space Center. So it will be a full-scale end-to-end “light-in-at-the-beginning, light-out-at-the end” sort of test, something they could not do for Hubble. But they knew they could go fix Hubble in space, and we know we can’t fix JWST, since the telescope will be at the L-2 point, about 1.5 million kilometers away from Earth, which is about four times further away from the Earth than the Moon.

This is a complicated project, but our approach for doing a complicated project is dramatically different from when I was a young feller. When I got here to Goddard, we used pencils and slide rules, and computers were pretty new and most people didn’t have them. Now we have computers everywhere that keep track of our documents. We can do systems engineering, and even can do very accurate, complete simulations to know if something will fit together and work before we even built it. So the world has changed, and it’s a wonderful thing to see. So this is why we are now able to build this observatory for about the same real cost as it took to get the Hubble launched and working. But JWST is so much bigger and more powerful.

JWST primary mirror. Credit: NASA
JWST primary mirror. Credit: NASA

UT: Can you tell us about the design for the mirror for the JWST?

Mather: The hardest thing to build was the mirror, because we needed something that is way bigger than Hubble. But you can’t possibly lift something that big or fit it into a rocket, so you need something that is lighter weight but nonetheless larger, so it has to have the ability to fold up.
The mirror is made of light-weight beryllium, and has 18 hexagonal segments. The telescope folds up like a butterfly in its chrysalis and will have to completely undo it self. It’s a rather elaborate process that will take many hours. The telescope is huge, at 6.5 meters (21 feet), so it’s pretty impressive.

The sun shield is completely new, and it too will have to deploy. So, what was wrapped up into a small cylinder, relatively speaking becomes a giant shield about as big as a tennis court. It’s huge. All this happens in multiple stages and will take days. We hired a company, Northrop Grumman that had experience unfolding things in space, and they tell us this is definitely not the most complicated thing they’ve unfolded in space, which is reassuring.

Video of the JWST deploying in space:

UT: Has there been any discussion of first light and what the JWST will look at first?

Mather: Yes, a little. That will be the fun part after we get the thing put together.

UT: Do you have any favorite suggestions?

Mather: I think we should start with easy targets that will be pretty, that will enable the public to say, “Oh, I see its working!” Some of the first observations can be done when we’re setting up the telescope, even before it’s fully adjusted. Because it is deployed after launch and the mirror isn’t close to the right shape at first, we’ll be working up to this gradually. There’s a test model at Ball Aerospace in Boulder Colorado, where we get to practice putting the 18 mirror segments into position. Each segment has 7 motors on it to control the position and curvature, so we have to rehearse this one.

This is something they couldn’t do with Hubble. They wished they could, and it did have motors but they couldn’t push hard enough. That’s an interesting story. We learned from Hubble how to correct the optics based on the images we were getting, so we’re doing it on purpose for this telescope.

UT: There has been some controversy about how the JWST will be launched.

Mather: We’ll take the telescope to French Guiana and load it in the rocket down there. The ESA is buying the launch vehicle for us; it’s the Ariane 5 rocket, a commercial product from Europe and they’ve had a good run lately, so it’s very reliable.

Naturally that caused a lot of controversy. Even if Europe was giving us the launch vehicle, so to speak, there were people here who did not want to accept it. It took headquarters two years to accept it. That cost us money. The only reason it was accepted was that we got a new administrator who would accept it. That was Mike Griffin, so I want to say, “thank you very much Mike Griffin!”

Artist concept of the JWST. Credit: NASA
Artist concept of the JWST. Credit: NASA

UT: Your team still has a lot to do before 2013, which will probably be here before you know it!

Mather: Yes, I know. It’s been over 13 years now since NASA contacted me about this, but now the end is coming up fast. We have plenty of technical challenges ahead of us in putting everything together. And we haven’t gotten far enough to along yet find out how many things we broke or how many mistakes we made, but I think we’re pretty good at figuring them out before we make them.

It’s going to be very exciting to put the equipment together for the first time. We’ve got the pieces, we’ve got the picture on the box to show where they go, and pretty soon we get to prove that they work together, or not. By the time we receive all the parts here at Goddard, they will all have been tested individually, so they’re supposed to play together just fine. But nature doesn’t like arrogance, so we have to test the whole thing from beginning to end, just as we’re going to use it in flight. After we put it together here, we take it down to Johnson Spaceflight Center, and put it in the giant vacuum tank there. That will be an extraordinary process.

UT: Thank you so much for talking with us.

Mather: This has been fun. I love telling my story and I’m glad you want to tell it with us. I figured it might be time to talk about what we’re doing because exciting things are starting to happen. Magnificent things are happening. We’ve got the Kepler Observatory up now, and hopefully they’ll find a handful of Earth-like planets to track down and we’ll take a closer look at them.

More information about the JWST.

Additional images and videos can be accessed here.

Could the First Stars Have Been Powered by Dark Matter?


Early stars that began to form about 200 million years after the Big Bang were strange creatures. From observation, the earliest stars (formed from coalescing primordial gas clouds) were not dense enough to support fusion reactions in their cores. Something within the young suns was counteracting the collapsing gas clouds, preventing the core reactions from taking place. Yet, they still produced light, even in absence of nuclear processes. Could dark matter have had a part to play, fueling the stellar bodies and sparking early stars to life?

New research indicates that the energy generated by annihilating dark matter in the early universe may have powered the first stars. How? Well, the violent early universe will have had high concentrations of dark matter. Dark matter has the ability to annihilate when it comes into contact with other dark matter matter, it does not require anti-dark matter to annihilate. When “normal” matter collides with its anti-component (i.e. electron colliding with positron), annihilation occurs. Annihilation is a term often used to describe the energetic destruction of something. While this is true, the annihilation products from dark matter include huge amounts of energy to create neutrinos and “ordinary matter” such as protons, electrons and positrons. Dark matter annihilation energy therefore has the ability to condense and create the matter we see in the Universe today.

Dark matter particles are their own anti. When they meet, one-third of the energy goes into neutrinos, which escape, one-third goes into photons and the last third goes into electrons and positrons.” – Katherine Freese, Theoretical Physicist, University of Michigan.

Katherine Freese (University of Michigan), Douglas Spolyar (University of California, Santa Cruz) and Paolo Gondolo (University of Utah in Salt Lake City) believe the strange physics of the early “dark stars” may be attributed to dark matter. For a star to form from stellar gas cloud to a viable, burning star, it must cool first. This cooling allows the star to collapse so the gas is dense enough to kick-start nuclear reactions in the core. However, early stars appear to have some form of energy acting against the cooling and collapse of early stars, fusion shouldn’t be possible, and yet the stars still shine.

The group believe that early stars may have passed through two stages of development. As the gas clouds collapse, the stars go through a “dark matter phase”, generating energy and producing normal matter. As the phase progresses, dark matter will slowly be used up and converted into matter. As the star becomes sufficiently dense with matter, fusion processes take over, starting the “fusion phase”. Fusion in turn generates heavier elements (such as metals, oxygen, carbon and nitrogen) during the lifetime of the star. When the early stars’ fuel is used up, it will go supernova, exploding and distributing these heavy elements throughout space to form other stars. The “dark matter phase” appears only to have existed in the very first stars (a.k.a. “population three stars”); later stars are supported by fusion processes only.

However, this exciting new theory will have to wait until the James Webb Telescope goes into operation in 2013 before population three stars can be observed with any great accuracy. Light may then be shone on the processes powering the first “dark stars” of our early Universe.

Source: Physorg.com

Grapple Attachment May Be Added to the James Webb Telescope


When the James Webb telescope launches in 2013, it’ll be the most powerful telescope ever deployed in space. To the get the best view, using the least fuel, it’ll sit in a stable orbit about 1.6 million km (1 million miles) from Earth. Unlike Hubble, it was never meant to be repaired. But NASA announced that it’s considering installing a grapple attachment anyway, just to be safe.

Since the new Orion spacecraft will be capable of taking astronauts to the Moon and back, NASA is investigating how feasible it’ll be to send astronauts to the James Webb telescope to perform emergency servicing operations. Although the observatory is meant to never be serviced, it’s good to keep your options open.

Engineers are currently working out what would be the best kind of hardware they could add to the telescope, so that future astronauts or robotic missions could link up with the telescope and perform repairs.

Original Source: NASA News Release