The James Webb Space Telescope survived May meteorite damage and delivered a sweet interstellar miracle in July.

An addition to our #JWSTArt and #UnfoldTheUniverse social media campaigns by Telus Spark, a science center in Calgary, Canada. They created this ice cream treat in tribute to Webb. July 18, 2022. (photo: NASA’s James Webb Space Telescope)
Arianespace’s Ariane 5 rocket launches with NASA’s James Webb Space Telescope onboard, Saturday, Dec. 25, 2021, from the ELA-3 Launch Zone of Europe’s Spaceport at the Guiana Space Centre in Kourou, French Guiana. The James Webb Space Telescope (sometimes called JWST or Webb) is a large infrared telescope with a 21.3 foot (6.5 meter) primary mirror. The observatory will study every phase of cosmic history — from within our solar system to the most distant observable galaxies in the early universe. Photo Credit: (NASA/Bill Ingalls)
NASA James Webb Space Telescope Commissioning Manager John Durning monitors the progress of the Webb observatory as it’s second primary mirror wing is rotated into position, Saturday, Jan. 8, 2022, from NASA’s James Webb Space Telescope Mission Operations Center at the Space Telescope Science Institute in Baltimore. Webb, an infrared telescope with a 21.3-foot (6.5-meter) primary mirror, was folded up for launch and underwent an unprecedented deployment process to unfold in space. As NASA’s next flagship observatory, Webb will study every phase of cosmic history — from within our solar system to the most distant observable galaxies in the early universe. Photo Credit: (NASA/Bill Ingalls)
Engineering teams at NASA’s James Webb Space Telescope Mission Operations Center at the Space Telescope Science Institute in Baltimore monitor progress as the observatory’s second primary mirror wing rotates into position, Saturday, Jan. 8, 2022. Webb, an infrared telescope with a 21.3-foot (6.5-meter) primary mirror, was folded up for launch and underwent an unprecedented deployment process to unfold in space. As NASA’s next flagship observatory, Webb will study every phase of cosmic history — from within our solar system to the most distant observable galaxies in the early universe. Photo Credit: (NASA/Bill Ingalls)
A monitor in the NASA James Webb Space Telescope flight control room of the Space Telescope Science Institute shows the progress of the second primary mirror wing latching on the Webb observatory, Saturday, Jan. 8, 2022, in Baltimore. When fully latched, the infrared observatory will have completed its unprecedented process of unfolding in space to prepare for science operations. Webb will study every phase of cosmic history — from within our solar system to the most distant observable galaxies in the early universe. Photo Credit: (NASA/Bill Ingalls)
NASA’s James Webb Space Telescope mission operations team celebrates, Saturday, Jan. 8, 2022, at the Space Telescope Science Institute in Baltimore, after confirming that the observatory’s final primary mirror wing successfully extended and locked into place. With Webb’s 21.3-foot (6.5-meter) primary mirror fully deployed, the infrared observatory has completed its unprecedented process of unfolding in space to prepare for science operations. The observatory will study every phase of cosmic history — from within our solar system to the most distant observable galaxies in the early universe. Photo Credit: (NASA/Bill Ingalls)
The image is divided horizontally by an undulating line between a cloudscape forming a nebula along the bottom portion and a comparatively clear upper portion. Speckled across both portions is a starfield, showing innumerable stars of many sizes. The smallest of these are small, distant, and faint points of light. The largest of these appear larger, closer, brighter, and more fully resolved with 8-point diffraction spikes. The upper portion of the image is blueish, and has wispy translucent cloud-like streaks rising from the nebula below. The orangish cloudy formation in the bottom half varies in density and ranges from translucent to opaque. The stars vary in color, the majority of which have a blue or orange hue. The cloud-like structure of the nebula contains ridges, peaks, and valleys — an appearance very similar to a mountain range. Three long diffraction spikes from the top right edge of the image suggest the presence of a large star just out of view. (Image Credits: NASA, ESA, CSA, and STScI)
A group of five galaxies that appear close to each other in the sky: two in the middle, one toward the top, one to the upper left, and one toward the bottom. Four of the five appear to be touching. One is somewhat separated. In the image, the galaxies are large relative to the hundreds of much smaller (more distant) galaxies in the background. All five galaxies have bright white cores. Each has a slightly different size, shape, structure, and coloring. Scattered across the image, in front of the galaxies are number of foreground stars with diffraction spikes: bright white points, each with eight bright lines radiating out from the center. (Image Credits: NASA, ESA, CSA, and STScI)
The image is split down the middle, showing two views of the Southern Ring Nebula. Both feature black backgrounds speckled with tiny bright stars and distant galaxies. Both show the planetary nebula as a misshapen oval that is slightly angled from top left to bottom right and takes up the majority of each image. At left, the near-infrared image shows a bright white star at the center with long diffraction spikes. Large, transparent teal and orange ovals, which are shells ejected by the unseen central star, surround it. At right, the mid-infrared image shows two stars at the center very close to one another. The one at left is red, the smaller one at right is light blue. The blue star has tiny triangles around it. A large transparent red oval surrounds the central stars. From that extend shells in a mix of colors, which are red to the left and right and teal to the top and bottom. Overall, the oval shape of the planetary nebula appears slightly smaller than the one seen at left. (Image Credits: NASA, ESA, CSA, and STScI)
Dust lanes of IC533. Processed in much the same way as NGC628. A visible / Hubble view of this galaxy is here: flic.kr/p/2nxgwuB. Red (screen layer mode): MIRI F2100W. Orange: MIRI F1130W. Cyan: MIRI F770W. Extra overall brightness in grayscale: MIRI F1000W. July 24, 2022. (Image Credit: Judy Schmidt)
Squeezing some color out of the various filters showing all the glowing dust in the center of NGC628. (Image Credit: Judy Schmidt)
A combination of NIRCam and MIRI filters to show continuum and emission line dust in NGC7496. A version combining this with HST data is here: flic.kr/p/2nyVKv5. JWST Filter Combination: Cyan: [mathematical operation] NIRCam F335M-(NIRCam F300M+NIRCam F360W). Orange: MIRI F770W. Luminosity (grayscale): MIRI F770W. (Image Credit: Judy Schmidt)
JWST data are overlaid on HST data with a Photoshop screen layer mode. HST Filter Combination: Red: WFC3/UVIS F814W. Green: WFC3/UVIS F555W. Blue: WFC3/UVIS F438W+F336W+F275W. The upper right corner of the HST data was filled with cloned data to get rid of a hard edge where HST data were missing. (Image Credit: Judy Schmidt)