NASA’s James Webb Space Telescope provided this view of a galactic grouping known as Stephan’s Quintet. Click on the image for a larger version. (NASA / ESA / CSA / STScI)
A day after NASA showed how far the James Webb Space Telescope could dive into the cosmic frontier, scientists released additional pictures demonstrating the observatory’s scientific breadth.
Today’s data release highlighted the $10 billion telescope’s ability to analyze planetary atmospheres and record scenes of stellar birth and death in unprecedented detail.
The infrared images also demonstrated that the Webb Space Telescope’s 21-foot-wide mirror is ready to provide sharp pictures from the very start. That comes in contrast to the Hubble Space Telescope’s debut in 1990, when the initial images were marred by a flaw in its 7.8-foot-wide mirror.
“This telescope is working fantastically well,” Mark McCaughrean, the European Space Agency’s senior adviser for science and exploration, said today during NASA’s Webb webcast.
That raises hopes that the James Webb Space Telescope, also known as JWST, will deliver on its promise to revolutionize the study of phenomena ranging from the origins of the universe to the habitability of alien planets.
One of JWST’s early targets is the TRAPPIST-1 planetary system, which is 34 light-years from Earth. University of Washington astrobiologist Andrew Lincowski hopes to use the telescope to characterize the atmospheres of TRAPPIST-1’s planets.
“All I can say is, Wow!” Lincowski told GeekWire in an email. “JWST will observe deep into the universe. For planets, we look closer, and for rocky exoplanets, this will still be challenging. TRAPPIST-1 remains an excellent target, and in fact, between the observations for the telescope and instrument developers and the first round of proposals, all seven planets will be individually observed this year by JWST.”
Lincowski said this year’s observations are just the beginning.
“These first observations will begin to tease out the possibility of the existence of atmospheres on small planets outside our solar system,” he wrote. “Additional observations will most likely be needed to confirm the presence of an atmosphere or lack thereof, or to confirm the presence of specific gases and attempt to constrain their abundances. With that information, we can assess the possibility of a temperate climate that could harbor life.”
Today’s data release included a spectral analysis focusing on a different sort of planet — WASP-96 b, a “hot Jupiter” that orbits a sunlike star roughly 1,150 light-years from Earth. The spectral signature of near-infrared light filtering through the planet’s atmosphere indicated the presence of water vapor. There was also evidence of obscuring clouds or hazes.
A spectral fingerprint documenting the composition of the atmosphere for a Jupiter-like planet known as WASP-96 b is superimposed over an artist’s conception of the planet. The chart indicates the presence of water vapor. Click on the image for a larger version. (NASA / ESA / CSA / STScI)
“This is just the beginning,” Knicole Colon, an astrophysicist at NASA’s Goddard Space Flight Center, said during today’s webcast. “We’re going to start pushing down to farther, smaller planets.”
In addition to the WASP-96 b data, NASA released four sets of images, including additional data about the deep-field image that was unveiled at the White House the day before. Here’s a roundup:
This mid-infrared JWST image of a galactic grouping known as Stephan’s Quintet highlights activity surrounding a supermassive black hole at the center of the uppermost galaxy. Click on the image for a larger version. (NASA / ESA / CSA / STScI)
Stephan’s Quintet is a picturesque grouping of five galaxies — including four galaxies that are about 290 million light-years away, plus a fifth galaxy that’s a mere 40 million light-years away. The foreground galaxy, known as NGC 7320, is the farthest left galaxy of the grouping.
JWST’s near-infrared and mid-infrared views provide a view of Stephan’s Quintet that’s sharper than Hubble’s version. The mid-infrared picture is particularly striking because it highlights the blast of light coming from the area around the supermassive black hole at the center of the uppermost galaxy, NGC 7319. The energy of the blast is equivalent to 40 billion suns.
Check out how much more you can see in the background of Stephan’s Quintet with the JWST (left) vs the Hubble (right). This is because the IR pierces through dust and captures light that’s redshifted due to the expansion of the Universe. Also, just look at the different views. pic.twitter.com/FjVdwUBeKv
— Sophia Gad-Nasr (@Astropartigirl) July 12, 2022
Southern Ring Nebula
These JWST views show the Southern Ring Nebula in near-infrared wavelengths at left, and in mid-infrared wavelengths at right. The mid-infrared image shows clearly that the dying star at the center of the nebula is actually a binary star system. Click on the image for a larger version. (NASA / ESA / CSA / STScI)
The Southern Ring Nebula is a shell of glowing gas and dust that surrounds a dying star system 2,000 light-years away in the constellation Vela. JWST’s infrared views reveal more of the structure than the Hubble view, and the mid-infrared observations reveal that there’s not just one, but two stars at the center of the nebula. The pictures also feature a faraway edge-on galaxy that’s visible to the left of the nebula.
Hubble’s view of the Southern Ring Nebula vs Webb’s view: pic.twitter.com/QiGYJ3Ah3B
— Jasmine 🌌🔭 (@astro_jaz) July 12, 2022
This JWST image shows a star-forming region in the Carina Nebula known as the “Cosmic Cliffs.” Click on the image for a larger version. (NASA / ESA / CSA / STScI)
JWST’s view of the Carina Nebula, 7,600 light-years from Earth, focuses on the “Cosmic Cliffs” — a dusty region where young stars are being formed. Blistering radiation from the hot blue stars in the upper half of the image is eating away the clouds of dust in the lower half of the image. But the pressure from that radiation is also squeezing still more stars into existence.
The Hubble Space Telescope previously provided images of the same region, but JWST’s infrared views reveal hundreds of previously unseen stars, plus numerous background galaxies.
This really puts things into perspective. On the left, an image of the Carina Nebula captured by Hubble. On the right, the nebula as seen by the James Webb Space Telescope.
Look how far we’ve come ✨#JamesWebbSpaceTelescope pic.twitter.com/tGFrbTf8oV
— Claire Reilly (@reillystyley) July 12, 2022
Webb’s First Deep Field
Two JWST views show a patch of sky around the galaxy cluster SMACS 0723 in mid-infrared wavelengths at left, and in the near-infrared at right. Click on the image for a larger version. (NASA / ESA / CSA / STScI)
The picture known as Webb’s First Deep Field — which made its debut at the White House on Monday — shows a region of sky as small as a grain of sand held at arm’s length. Thanks to the gravitational lensing effect of a galaxy cluster known as SMACS 0723, JWST’s view includes views of thousands of more distant galaxies.
Spectral analysis has shown that light from one of the galaxies traveled for 13.1 billion years before it was captured by the space telescope — and there may be even more distant galaxies in the picture.