Newzlab

How MIRI became Webb’s coolest instrument


How MIRI became Webb's coolest instrument
The NASA/ESA/CSA James Webb Space Telescope’s mid-infrared view of the Pillars of Creation strikes a chilling tone. Thousands of stars that exist in this region disappear from view — and seemingly endless layers of gas and dust become the centrepiece. The detection of dust by Webb’s Mid-Infrared Instrument (MIRI) is extremely important — dust is a major ingredient for star formation. Many stars are actively forming in these dense blue-grey pillars. When knots of gas and dust with sufficient mass form in these regions, they begin to collapse under their own gravitational attraction, slowly heat up, and eventually form new stars. Although the stars appear to be missing, they aren’t. Stars typically do not emit much mid-infrared light. Instead, they are easiest to detect in ultraviolet, visible, and near-infrared light. In this MIRI view, two types of stars can be identified. The stars at the end of the thick, dusty pillars have recently eroded most of the more distant material surrounding them but they can be seen in mid-infrared light because they are still surrounded by cloaks of dust. In contrast, blue tones indicate stars that are older and have shed most of their gas and dust. Mid-infrared light also details dense regions of gas and dust. The red region toward the top, which forms a delicate V shape, is where the dust is both diffuse and cooler. And although it may seem like the scene clears toward the bottom left of this view, the darkest grey areas are where densest and coolest regions of dust lie. Notice that there are many fewer stars and no background galaxies popping into view. Webb’s mid-infrared data will help researchers determine exactly how much dust is in this region — and what it’s made of. These details will make models of the Pillars of Creation far more precise. Over time, we will begin to understand more clearly how stars form and burst out of these dusty clouds over millions of years. Credit: NASA, ESA, CSA, STScI, J. DePasquale (STScI), A. Pagan (STScI)

The NASA/ESA/CSA James Webb Space Telescope is widely referred to as the successor to the NASA/ESA Hubble Space Telescope. In reality, it is the successor to a lot more than that. With the inclusion of the Mid-InfraRed Instrument (MIRI), Webb also became a successor to infrared space telescopes such as ESA’s Infrared Space Observatory (ISO) and NASA’s Spitzer Space Telescope.

At mid-infrared wavelengths, the Universe is a very different place from the one we are used to seeing with our eyes. Stretching from 3 to 30 micrometers, mid-infrared reveals celestial objects with temperatures of 30 to 700ºC. In this regime, objects that appear dark in visible light images now shine brightly.

For example, the dust clouds in which stars are forming tend to be at these temperatures. In addition, molecules tend to be easy to see at these wavelengths. “It’s such an exciting wavelength range in terms of the chemistry that you can do, and the way you can understand star formation and what’s happening in the nuclei of galaxies,” says Gillian Wright, the Principal Investigator for the European Consortium behind the MIRI instrument.

Our first real glimpses of the mid-infrared cosmos came from ISO, which was operational between November 1995 and October 1998. Arriving in orbit in 2003, Spitzer made further progress at similar wavelengths. Both ISO and Spitzer’s discoveries highlighted the need for a mid-infrared capability with a larger collecting area for better sensitivity and angular resolution to advance many big questions in astronomy.

Gillian and others began to dream of an instrument that could see the mid-infrared in vivid detail. Unfortunately for them, ESA and NASA saw the shorter wavelengths of the near infrared as the primary goal for Webb. ESA would take the lead on a near infrared spectrometer, which became NIRSpec, and NASA set its sights on an imager that became NIRCam.

Not to be deterred, when ESA issued a call for proposals to study their near infrared spectrometer instrument, Gillian and her colleagues saw a chance.

“I led a team that put in a rather cheeky response. It said we’ll study the near infrared spectrograph but we’ll also have an extra channel doing all of this mid-infrared science too. And we presented the science case for why mid infrared astronomy would be fantastic on Webb,” she says.

Although her team did not win that particular contract, the gutsy move helped raise the profile of mid-infrared astronomy in Europe, and she herself was invited to represent those science interests on another ESA study that surveyed European industry’s ability to build infrared instrumentation. Assisted by academic institutions from across Europe, part of that study looked at mid-infrared instrumentation.

The results were so encouraging, as were those of parallel US-led studies, that the appetite for such an instrument grew even larger. By pulling together in Europe an international collaboration of scientists and engineers willing and able to design and build the instrument—and crucially raise the money to do so—Gillian and her collaborators encouraged and gradually convinced ESA and NASA to include it on Webb.

Large consortia are not an unusual way to build spacecraft instruments in Europe. ESA often builds the spacecraft or telescope and then relies of consortia of academic and industrial institutions to raise funds from their national governments to build the instruments. But it is unusual in the US, where NASA usually funded the instrumentation as well.







Webb’s instruments: meet MIRI. Credit: European Space Agency

Extending European leadership in this method of working into the realm of international collaboration with the US, on a flagship NASA mission where the culture of instrument building is so different, was not a guaranteed recipe for success.

“The biggest fear was that this complexity would be the biggest threat to the instrument,” says Jose Lorenzo Alvarez, MIRI Instrument Manager for ESA.

But the gamble paid off as Jose explains, “It was surprising to see the change in attitudes between people with entirely different working cultures. In the first years, we were on a learning curve. In the end, MIRI, which was organisationally more complex, was the first instrument to be delivered.”

In addition to raising their own money, the consortium had been given another caveat: the instrument could have no impact on the Webb’s operating temperatures and optics. In other words, the telescope would remain optimized for the near-infrared instruments, and MIRI would accept whatever it could get. This would limit the instrument’s performance beyond ten micrometers but it was a small price to pay for Gillian. “I never saw it as a compromise because it would still be better than anything we had ever seen before,” she says.

One of the biggest technological hurdles to overcome was that MIRI needed to operate at a lower temperature than the near-infrared instruments. This was achieved with the cryocooler mechanism provided by NASA’s Jet Propulsion Laboratory. To be sensitive to the mid-infrared wavelengths, MIRI operates at around 6 Kelvin (–267°C).

This is lower than the average surface temperature of Pluto, which is around 40 Kelvin (–233°C). Coincidently, this temperature is where the other instruments and the telescope operate. Both are extremely cold temperatures but because of that difference, heat from the telescope would still leak into MIRI once it was harnessed to the telescope, unless the two were thermally isolated from one another.

“To minimize the thermal leaks we had to choose some quite strange and quite exotic harness materials to minimize the thermal conductance from one side to the other,” says Brian O’Sullivan, MIRI System Engineer for ESA.

Another challenge was the limited space available for the instrument on the telescope. This was made even more difficult since MIRI was to be effectively two instruments in one, an imager and a spectrometer. It called for some clever design work.

“We’ve got a mechanism, and we not only use light shining off one side, but we use the other side of it, too, just to minimize the number of mechanisms we use and the space we take up. It’s a very interesting and very compact optical design,” says Brian.

The instrument uses one light path for its imager, and another for its spectrometer.

Even after the instrument was completed and delivered to NASA for integration with the rest of the telescope, there were more challenges for the team to face.

How MIRI became Webb's coolest instrument
With its powerful, mid-infrared vision, MIRI shows never-before-seen details of Stephan’s Quintet, a visual grouping of five galaxies. MIRI pierced through dust-enshrouded regions to reveal huge shock waves and tidal tails, gas and stars stripped from the outer regions of the galaxies by interactions. It also unveiled hidden areas of star formation. The new information from MIRI provides invaluable insights into how galactic interactions may have driven galaxy evolution in the early universe. Credit: NASA, ESA, CSA, and STScI

The fiercely complicated telescope took longer to complete than anyone had imagined and that meant MIRI and the other instruments would be required to survive on the ground for much longer than originally planned. Designed to remain on Earth for about three years before launch, it took almost a decade more before the spacecraft reached orbit. To ensure the health of the instrument, MIRI was stored in a strictly controlled conditions and periodically tested.

Then on Christmas Day 2021, an ESA Ariane 5 rocket carried the spacecraft into orbit in a picture-perfect launch. In the weeks and months that followed, ground teams readied the telescope and its instruments and handed over to the scientists.

Alongside the other instruments, MIRI is now sending back the kind of data that the scientists had been dreaming about.

“Yeah, those first few months in particular were quite surreal,” says Sarah Kendrew, MIRI Instrument and Calibration Scientist, ESA. “We’d been doing so much preparatory work with simulated data, so in a sense we knew what the data would look like. So you could be looking at it thinking it all looks very familiar, but then at the same time, it’s just like, but it came from space!”

MIRI’s data featured heavily in the very first images released from Webb, including the ‘mountains’ and ‘valleys’ of the Carina nebula, the interacting galaxy group Stephan Quintet, and the Southern Ring Nebula. Subsequent images have continued to raise the bar both in terms of beauty and science.

However, because MIRI is such a large step up from any previous mid-infrared instrument, the bar is also raised in terms of being able to interpret the images. “MIRI is giving us a lot of very new things that are harder to interpret, just because MIRI is such a big difference from what there was before,” says Sarah.

But this is the essence of cutting-edge science and astronomers are already racing to develop more detailed computer models that can tell them more about the various physical processes that give raise to mid-infrared readings.

“There’s a huge potential for new understanding with MIRI, particularly in star formation and the properties of dust and galaxies. It may take a bit longer to interpret but I think the new science that will come out of MIRI is going to be really, really substantial,” says Sarah.

MIRI, together with the other instruments on Webb, has the potential to advance every branch of astronomy. It is the kind of transformative science that comes about only through a large step-up in capability. And it is a remarkable testament to the team-work and international collaboration that went into the telescope in general, and MIRI in particular.

“The thing that made MIRI happen was team spirit. We all wanted the same thing, which was the science. People’s willingness to work together and solve problems together was really what made MIRI happen,” says Gillian.

Citation:
How MIRI became Webb’s coolest instrument (2022, November 8)
retrieved 8 November 2022
from https://phys.org/news/2022-11-miri-webb-coolest-instrument.html

This document is subject to copyright. Apart from any fair dealing for the purpose of private study or research, no
part may be reproduced without the written permission. The content is provided for information purposes only.



Source link