Skip to main content

James Webb’s MIRI instrument has both a heater and a cooler

The long process of getting the James Webb Space Telescope ready for science operations continues, with the ongoing alignment of three of its instruments.

Webb recently reached the major milestone of aligning its mirrors with its NIRCam instrument, in a successful step that promises great results to come. “Webb’s alignment at the NIRCam field showed some spectacular diffraction-limited images, producing a tantalizing glimpse of the capabilities this observatory will carry for its science program,” wrote two Webb researchers, Michael McElwain, Webb observatory project scientist, and Charles Bowers, Webb deputy observatory project scientist, both at NASA Goddard, in a recent blog post. “This was a major milestone because it required nearly all of the observatory systems to be functioning as designed. It all worked as well as we dared to hope, and it was certainly a moment to celebrate.”

Recommended Videos

Now, the Webb team is working on aligning two more of the instruments — the Near-Infrared Slitless Spectrograph (NIRISS) and Near-Infrared Spectrometer (NIRSpec) — as well as the guider, called the Fine Guidance Sensor (FGS). This process is expected to take around six weeks and will ensure that all of the instruments can work together. Along with NIRCam, these comprise Webb’s near-infrared instruments.

While the three near-infrared instruments are passively cooled — meaning that heat is dispersed from the telescope and into space using design elements like heat sinks which require no power — the fourth instrument, MIRI, works in the mid-infrared wavelength and requires active cooling. Because MIRI uses a different type of detector than the other instruments, and these detectors need to be at an extremely low temperature of less than 7 kelvin to work properly, the instrument needs to be fitted with a cryocooler. This refrigeration system uses helium gas and includes pumps that require power but must produce very little vibration to avoid interfering with instrument readings.

In addition to this cooling system, MIRI is also fitted with heaters so that the cooldown process can be carefully managed to prevent ice from forming on the components. The heaters will shortly be turned off, allowing the cooling system to bring the instrument down to its operating temperature.

With the cooling of MIRI underway, it will take a few weeks until the final instrument gets cool enough to be ready for alignment. Then, with all four of the instruments aligned, the Webb team can move onto the next phase of commissioning — optical stability tests and instrument performance measurement — to get the telescope ready for science operations this summer.

Georgina Torbet
Georgina has been the space writer at Digital Trends space writer for six years, covering human space exploration, planetary…
James Webb is explaining the puzzle of some of the earliest galaxies
This image shows a small portion of the field observed by NASA’s James Webb Space Telescope’s NIRCam (Near-Infrared Camera) for the Cosmic Evolution Early Release Science (CEERS) survey. It is filled with galaxies. The light from some of them has traveled for over 13 billion years to reach the telescope.

From practically the moment it was turned on, the James Webb Space Telescope has been shaking cosmology. In some of its very earliest observations, the telescope was able to look back at some of the earliest galaxies ever observed, and it found something odd: These galaxies were much brighter than anyone had predicted. Even when the telescope's instruments were carefully calibrated over the few weeks after beginning operations, the discrepancy remained. It seemed like the early universe was a much busier, brighter place than expected, and no one knew why.

This wasn't a minor issue. The fact early galaxies appeared to be bigger or brighter than model predicted meant that something was off about the way we understood the early universe. The findings were even considered "universe breaking." Now, though, new research suggests that the universe isn't broken -- it's just that there were early black holes playing tricks.

Read more
James Webb Telescope captures gorgeous galaxy with a hungry monster at its heart
Featured in this new image from the NASA/ESA/CSA James Webb Space Telescope is Messier 106, also known as NGC 4258. This is a nearby spiral galaxy that resides roughly 23 million light-years away in the constellation Canes Venatici, practically a neighbour by cosmic standards. Messier 106 is one of the brightest and nearest spiral galaxies to our own and two supernovae have been observed in this galaxy in 1981 and 2014.

A new image from the James Webb Space Telescope shows off a nearby galaxy called Messier 106 -- a spiral galaxy that is particularly bright. At just 23 million light-years away (that's relatively close by galactic standards), this galaxy is of particular interest to astronomers due to its bustling central region, called an active galactic nucleus.

The high level of activity in this central region is thought to be due to the monster that lurks at the galaxy's heart. Like most galaxies including our own, Messier 106 has an enormous black hole called a supermassive black hole at its center. However, the supermassive black hole in Messier 106 is particularly active, gobbling up material like dust and gas from the surrounding area. In fact, this black hole eats so much matter that as it spins, it warps the disk of gas around it, which creates streamers of gas flying out from this central region.

Read more
James Webb takes rare direct image of a nearby super-Jupiter
Artist’s impression of a cold gas giant orbiting a red dwarf. Only a point of light is visible on the JWST/MIRI images. Nevertheless, the initial analysis suggests the presence of a gaseous planet that may have properties similar to Jupiter.

Even with huge ground-based observatories and the latest technology in space-based telescopes, it's still relatively rare for astronomers to take an image of an exoplanet. Planets outside our solar system are so far away and so small and dim compared to the stars they orbit that it's extremely difficult to study them directly. That's why most observations of exoplanets are made by studying their host stars. Now, though, the James Webb Space Telescope has directly imaged a gas giant -- and it's one of the coldest exoplanets observed so far.

The planet, named Epsilon Indi Ab, is located 12 light-years away and has an estimated temperature of just 35 degrees Fahrenheit (2 degrees Celsius). The fact it is so cool compared to most exoplanets meant that Webb's sensitive instruments were needed to study it.

Read more