The James Webb Space Telescope has finally arrived at its new home. After a Christmas launch and a month of unfolding and assembling itself in space, the new space observatory reached its final destination, a spot known as L2, on January 24.
But the telescope canâ€™t start doing science yet. There are still several monthsâ€™ worth of tasks on Webbâ€™s to-do list before the telescope is ready to peep at the earliest light in the universe or spy on exoplanetsâ€™ alien atmospheres (SN: 10/6/21).
â€œThat doesnâ€™t mean thereâ€™s anything wrong,â€ says astronomer Scott Friedman of the Space Telescope Science Institute in Baltimore, who is managing this next phase of Webbâ€™s journey. â€œEverything could go perfectly, and it would still take six monthsâ€ from launch for the telescopeâ€™s science instruments to be ready for action, he says.
Hereâ€™s what to expect next.
Life at L2
L2, technically known as the second Earth-sun Lagrange point, is a spot about 1.5 million kilometers from Earth in the direction of Mars, where the sun and Earthâ€™s gravity are of equal strength. Pairs of massive objects in space have five such Lagrange points, where the gravitational pushes and pulls from these celestial bodies essentially cancel each other out. That lets objects at Lagrange points stay put without much effort.
The telescope, also known as JWST, isnâ€™t just sitting tight, though. Itâ€™s orbiting L2, even as L2 orbits the sun. Thatâ€™s because L2 is not precisely stable, Friedman says. Itâ€™s like trying to stay balanced directly on top of a basketball. If you nudged an object sitting exactly at that point, it would be easy to make it wander off. Circling L2 as L2 circles the sun in a â€œhalo orbitâ€ is much more stable â€” itâ€™s harder to fall off the basketball when in constant motion. But it takes some effort to stay there.
â€œJWST and other astronomical satellites, which are said to be at L2 but are really in halo orbits, need propulsion to maintain their positions,â€ Friedman says. â€œFor JWST, we will execute what we call station keeping maneuvers every 21 days. We fire our thrusters to correct our position, thus maintaining our halo orbit.â€
The amount of fuel needed to maintain Webbâ€™s home in space will set the lifetime of the mission. Once the telescope runs out of fuel, the mission is over. Luckily, the spacecraft had a near-perfect launch and didnâ€™t use much fuel in transit to L2. As a result, it might be able to last more than 10 years, team members say, longer than the original five- to 10-year estimate.
Webb has one more feature that helps it stay stable. The telescopeâ€™s gigantic kitelike sunshield, which protects the delicate instruments from the heat and light of the sun, Earth and the moon, could pick up momentum from the stream of charged particles that constantly flows from the sun, like a solar sail. If so, that could push Webb off course. To prevent this, the telescope has a flap that acts as a rudder, said Webb sunshield manager Jim Flynn of Northrup Grumman in a January 4 news conference.
Webb sees in infrared light, wavelengths longer than what the human eye can see. But humans do experience infrared radiation as heat. â€œWeâ€™re essentially looking at the universe in heat vision,â€ says astrophysicist Erin Smith of NASAâ€™s Goddard Space Flight Center in Greenbelt, Md., a project scientist on Webb.
That means that the parts of the telescope that observe the sky have to be at about 40 kelvins (â€“233Â° Celsius), which nearly matches the cold of space. That way, Webb avoids emitting more heat than the distant sources in the universe that the telescope will be observing, preventing it from obscuring them from view.
Most of Webb has been cooling down ever since the telescopeâ€™s sunshield unfurled on January 4. The observatoryâ€™s five-layer sunshield blocks and deflects heat and light, letting the telescopeâ€™s mirrors and scientific instruments cool off from their temperature at launch. The sunshield layer closest to the sun will warm to about 85Â° Celsius, but the cold side will be about â€“233Â° Celsius, said Webbâ€™s commissioning manager Keith Parrish in a January 4 webcast.
â€œYou could boil water on the front side of us, and on the backside of us, youâ€™re almost down to absolute zero,â€ Parrish said.
One of the instruments, MIRI, the Mid-Infrared Instrument, has extra coolant to bring it down to 6.7 kelvins (â€“266Â° Celsius) to enable it to see even dimmer and cooler objects than the rest of the telescope. For MIRI, â€œspace isnâ€™t cold enough,â€ Smith says.
Aligning the mirrors
Webb finished unfolding its 6.5-meter-wide golden mirror on January 8, turning the spacecraft into a true telescope. But itâ€™s not done yet. That mirror, which collects and focuses light from the distant universe, is made up of 18 hexagonal segments. And each of those segments has to line up with a precision of about 10 or 20 nanometers so that the whole apparatus mimics a single, wide mirror.
Starting on January 12, 126 tiny motors on the back of the 18 segments started moving and reshaping them to make sure they all match up. Another six motors went to work on the secondary mirror, which is supported on a boom in front of the primary mirror.
This alignment process will take until at least April to finish. In part, thatâ€™s because the movements are happening while the mirror is cooling. The changing temperature changes the shape of the mirrors, so they canâ€™t be put in their final alignment until after the telescopeâ€™s suite of scientific instruments are fully chilled.
Once the initial alignment is done, light from distant space will first bounce off the primary mirror, then the secondary mirror and finally reach the instruments that will analyze the cosmic signals. But the alignment of the mirror segments is â€œnot just right now, itâ€™s a continuous process, just to make sure that theyâ€™re always perfectly aligned,â€ Scarlin Hernandez, a flight systems engineer at the Space Telescope Science Institute in Baltimore said at a NASA Science Live event on January 24. The process will continue for the telescopeâ€™s lifetime.
Calibrating the science instruments
While the mirrors are aligning, Webbâ€™s science instruments will turn on. Technically, this is when Webb will take its first pictures, says astronomer Klaus Pontoppidan, also of the Space Telescope Science Institute. â€œBut theyâ€™re not going to be pretty,â€ Pontoppidan says. The telescope will first test its focus on a single bright star, bringing 18 separate bright dots into one by tilting the mirrors.
After a few final adjustments, the telescope will be â€œperforming as we want it to and presenting beautiful images of the sky to all the instruments,â€ Friedman says. â€œThen they can start doing their work.â€
These instruments include NIRCam, the primary near-infrared camera that will cover the range of wavelengths from 0.6 to 5 micrometers. NIRCam will be able to image the earliest stars and galaxies as they were when they formed at least 12 billion years ago, as well as young stars in the Milky Way. The camera will also be able to see objects in the Kuiper Belt at the edge of the solar system and is equipped with a coronagraph, which can block light from a star to reveal details of dimmer exoplanets orbiting it.
Next up is NIRSpec, the near-infrared spectrograph, which will cover the same range of light wavelengths as NIRCam. But instead of collecting light and turning it into an image, NIRSpec will split the light into a spectrum to figure out an objectâ€™s properties, such as temperature, mass and composition. The spectrograph is designed to observe 100 objects at the same time.
MIRI, the mid-infrared instrument, is kept the coldest to observe in the longest wavelengths, from 5 to 28 micrometers. MIRI has both a camera and a spectrograph that, like NIRCam and NIRSpec, will still be sensitive to distant galaxies and newborn stars, but it will also be able to spot planets, comets and asteroids.
And the fourth instrument, called the FGS/NIRISS, is a two-parter. FGS is a camera that will help the telescope point precisely. And NIRISS, which stands for near-infrared imager and slitless spectrograph, will be specifically used to detect and characterize exoplanets.
First science targets
It will take at least another five months after arriving at L2 to finish calibrating all of those science instruments, Pontoppidan says. When thatâ€™s all done, the Webb science team has a top secret plan for the first full color images to be released.
â€œThese are images that are meant to demonstrate to the world that the observatory is working and ready for science,â€ Pontoppidan says. â€œExactly what will be in that package, thatâ€™s a secret.â€
Partly the secrecy is because thereâ€™s still some uncertainty in what the telescope will be able to look at when the time comes. If setting up the instruments takes longer than expected, Webb will be in a different part of its orbit and certain parts of the sky will be out of view for a while. The team doesnâ€™t want to promise something specific and then be wrong, Pontoppidan says.
But also, â€œitâ€™s meant to be a surprise,â€ he says. â€œWe donâ€™t want to spoil that surprise.â€
Webbâ€™s first science projects, however, are not under wraps. In the first five months of observations, Webb will begin a series of Early Release Science projects. These will use every feature of every instrument to look at a broad range of space targets, including everything from Jupiter to distant galaxies and from star formation to black holes and exoplanets.
Still, even the scientists are eager for the pretty pictures.
â€œIâ€™m just very excited to get to see those first images, just because they will be spectacular,â€ Smith says. â€œAs much as I love the science, itâ€™s also fun to ooh and ahh.â€Â Â Â