A team of researchers has confirmed stars ring loud and clear in a “key” that will harmonize well with the science goals and capabilities of NASA’s upcoming Nancy Grace Roman Space Telescope.
This artist’s concept visualizes the Sun and several red giant stars of varying radii. NASA’s upcoming Nancy Grace Roman Space Telescope will be well suited for studying red giant stars with a method known as asteroseismology. This approach entails studying the changes in stars’ overall brightness, which is caused by their turbulent interiors creating waves and oscillations. With asteroseismic detections, astronomers can learn about stars’ ages, masses, and sizes. Scientists estimate Roman will be able to detect a total of 300,000 red giant stars with this method. This would be the largest sample of its kind ever collected.
Credit: NASA, STScI, Ralf Crawford (STScI)
Stars’ turbulent natures produce waves that cause fluctuations in their overall brightness. By studying these changes — a method called asteroseismology — scientists can glean information about stars’ ages, masses, and sizes. These shifts in brightness were perceptible to NASA’s Kepler space telescope, which provided asteroseismic data on approximately 16,000 stars before its retirement in 2018.
Using Kepler data as a starting point and adapting the dataset to match the expected quality from Roman, astronomers have recently proven the feasibility of asteroseismology with the soon-to-launch telescope and provided an estimated range of detectable stars. It’s an added bonus to Roman’s main science goals: As the telescope conducts observations for its Galactic Bulge Time-Domain Survey — a core community survey that will gather data on hundreds of millions of stars in the bulge of our Milky Way galaxy — it will also provide enough information for astronomers to determine stellar measurements via asteroseismology.
“Asteroseismology with Roman is possible because we don’t need to ask the telescope to do anything it wasn’t already planning to do,” said Marc Pinsonneault of The Ohio State University in Columbus, a co-author of a paper detailing the research. “The strength of the Roman mission is remarkable: It’s designed in part to advance exoplanet science, but we’ll also get really rich data for other scientific areas that extend beyond its main focus.”
Exploring what’s possible
The galactic bulge is densely populated with red giant branch and red clump stars, which are more evolved and puffier than main sequence stars. (Main sequence stars are in a similar life stage as our Sun.) Their high luminosity and oscillating frequency, ranging from hours to days, work in Roman’s favor. As part of its Galactic Bulge Time-Domain Survey, the telescope will observe the Milky Way’s galactic bulge every 12 minutes over six 70.5-day stretches, a cadence that makes it particularly well suited for red giant asteroseismology.
While previous research has explored the potential of asteroseismology with Roman, the team took a more detailed look by considering Roman’s capabilities and mission design. Their investigation consisted of two large efforts:
First, the team members looked at Kepler’s asteroseismic data and applied parameters so the dataset matched the expected quality of Roman data. This included increasing the observation frequency and adjusting the wavelength range of light. The team calculated detection probabilities, which confirmed with a resounding yes that Roman will be able to detect the oscillations of red giants.
The team then applied their detection probabilities to a model of the Milky Way galaxy and considered the suggested fields of view for the galactic bulge survey to get a sense of how many red giants and red clump stars could be investigated with asteroseismology.
This sonification is based on a simulation of data that NASA’s Roman Space Telescope will collect after its launch as soon as fall 2026. The sonification converts the waves moving inside red giant stars into sound. These pressure waves cause tiny changes in brightness that Roman can measure. Bigger stars take longer for the waves to bounce around, which means brightness changes have lower frequencies. Here, those frequencies are turned into sound and sped up so we can hear them. The first sound in the sonification comes from the Sun to give a sense of scale (even though Roman won’t look at the Sun). It then moves on to bigger and bigger red giants, with the pitch changing for each one. Astronomers can calculate a star’s size and other properties by measuring these frequencies. An audio-described version is available for download at the bottom of the page.
“At the time of our study, the core community survey was not fully defined, so we explored a few different models and simulations. Our lower limit estimation was 290,000 objects in total, with 185,000 stars in the bulge,” said Trevor Weiss of California State University, Long Beach, co-first author of the paper. “Now that we know the survey will entail a 12-minute cadence, we find it strengthens our numbers to over 300,000 asteroseismic detections in total. It would be the largest asteroseismic sample ever collected.”
Bolstering science for all
The benefits of asteroseismology with Roman are numerous, including tying into exoplanet science, a major focus for the mission and the galactic bulge survey. Roman will detect exoplanets, or planets outside our solar system, through a method called microlensing, in which the gravity of a foreground star magnifies the light from a background star. The presence of an exoplanet can cause a noticeable “blip” in the resulting brightness change.
“With asteroseismic data, we’ll be able to get a lot of information about exoplanets’ host stars, and that will give us a lot of insight on exoplanets themselves,” Weiss said.
“It will be difficult to directly infer ages and the abundances of heavy elements like iron for the host stars of exoplanets Roman detects,” Pinsonneault said. “Knowing these things — age and composition — can be important for understanding the exoplanets. Our work will lay out the statistical properties of the whole population — what the typical abundances and ages are — so that the exoplanet scientists can put the Roman measurements in context.”
Additionally, for astronomers who seek to understand the history of the Milky Way galaxy, asteroseismology could reveal information about its formation.
“We actually don’t know a lot about our galaxy’s bulge since you can only see it in infrared light due to all the intervening dust,” Pinsonneault said. “There could be surprising populations or chemical patterns there. What if there are young stars buried there? Roman will open a completely different window into the stellar populations in the Milky Way’s center. I’m prepared to be surprised.”
Since Roman is set to observe the galactic bulge soon after launch, the team is working to build a catalog in advance and provide a target list of observable stars that could help with efforts in validating the telescope’s early performance.
“Outside of all the science, it’s important to remember the amount of people it takes to get these things up and running, and the amount of different people working on Roman,” said co-first author Noah Downing of The Ohio State University. “It’s really exciting to see all of the opportunities Roman is opening up for people before it even launches and then think about how many more opportunities will exist once it’s in space and taking data, which is not very far away.” Roman is slated to launch no later than May 2027, with the team working toward a potential early launch as soon as fall 2026.
The Nancy Grace Roman Space Telescope is managed at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, with participation by NASA’s Jet Propulsion Laboratory in Southern California; Caltech/IPAC in Pasadena, California; the Space Telescope Science Institute in Baltimore; and a science team comprising scientists from various research institutions. The primary industrial partners are BAE Systems, Inc. in Boulder, Colorado; L3Harris Technologies in Melbourne, Florida; and Teledyne Scientific & Imaging in Thousand Oaks, California.
NASA’s Webb Explores Largest Star-Forming Cloud in Milky Way
Stars, gas and cosmic dust in the Sagittarius B2 molecular cloud glow in near-infrared light, captured by Webb’s NIRCam instrument. Full image and caption below.
Credits: Image: NASA, ESA, CSA, STScI, Adam Ginsburg (University of Florida), Nazar Budaiev (University of Florida), Taehwa Yoo (University of Florida); Image Processing: Alyssa Pagan (STScI)
NASA’s James Webb Space Telescope has revealed a colorful array of massive stars and glowing cosmic dust in the Sagittarius B2 molecular cloud, the most massive and active star-forming region in our Milky Way galaxy.
“Webb’s powerful infrared instruments provide detail we’ve never been able to see before, which will help us to understand some of the still-elusive mysteries of massive star formation and why Sagittarius B2 is so much more active than the rest of the galactic center,” said astronomer Adam Ginsburg of the University of Florida, principal investigator of the program.
Image A: Sagittarius B2 (NIRCam Image)
Stars, gas and cosmic dust in the Sagittarius B2 molecular cloud glow in near-infrared light, captured by Webb’s NIRCam instrument. The darkest areas of the image are not empty space but are areas where stars are still forming inside dense clouds that block their light.
Image: NASA, ESA, CSA, STScI, Adam Ginsburg (University of Florida), Nazar Budaiev (University of Florida), Taehwa Yoo (University of Florida); Image Processing: Alyssa Pagan (STScI)
Sagittarius B2 is located only a few hundred light-years from the supermassive black hole at the heart of the galaxy called Sagittarius A*, a region densely packed with stars, star-forming clouds, and complex magnetic fields. The infrared light that Webb detects is able to pass through some of the area’s thick clouds to reveal young stars and the warm dust surrounding them.
However, one of the most notable aspects of Webb’s images of Sagittarius B2 are the portions that remain dark. These ironically empty-looking areas of space are actually so dense with gas and dust that even Webb cannot see through them. These thick clouds are the raw material of future stars and a cocoon for those still too young to shine.
The high resolution and mid-infrared sensitivity of Webb’s MIRI (Mid-Infrared Instrument) revealed this region in unprecedented detail, including glowing cosmic dust heated by very young massive stars. The reddest area on the right half of MIRI’s image, known as Sagittarius B2 North, is one of the most molecularly rich regions known, but astronomers have never seen it with such clarity. (Note: North is to the right in these Webb images.)
Image B: Sagittarius B2 (MIRI Image)
Webb’s MIRI instrument shows the Sagittarius B2 region in mid-infrared light, with warm dust glowing brightly. Only the brightest stars emit strongly enough to appear through the dense clouds as blue pinpoints.
Image: NASA, ESA, CSA, STScI, Adam Ginsburg (University of Florida), Nazar Budaiev (University of Florida), Taehwa Yoo (University of Florida); Image Processing: Alyssa Pagan (STScI)
The difference longer wavelengths of light make, even within the infrared spectrum, are stark when comparing the images from Webb’s MIRI and NIRCam (Near-Infrared Camera) instruments. Glowing gas and dust appear dramatically in mid-infrared light, while all but the brightest stars disappear from view.
In contrast to MIRI, colorful stars steal the show in Webb’s NIRCam image, punctuated occasionally by bright clouds of gas and dust. Further research into these stars will reveal details of their masses and ages, which will help astronomers better understand the process of star formation in this dense, active galactic center region. Has it been going on for millions of years? Or has some unknown process triggered it only recently?
Image C: Compare NIRCam and MIRI Images of Sagittarius B2
NIRCam
MIRI
Stars, gas and cosmic dust in the Sagittarius B2 molecular cloud glow in near-infrared light, captured by Webb’s NIRCam instrument. The darkest areas of the image are not empty space but are areas where stars are still forming inside dense clouds that block their light.
Image: NASA, ESA, CSA, STScI, Adam Ginsburg (University of Florida), Nazar Budaiev (University of Florida), Taehwa Yoo (University of Florida); Image Processing: Alyssa Pagan (STScI)
Stars, gas and cosmic dust in the Sagittarius B2 molecular cloud glow in near-infrared light, captured by Webb’s NIRCam instrument. The darkest areas of the image are not empty space but are areas where stars are still forming inside dense clouds that block their light.
Image: NASA, ESA, CSA, STScI, Adam Ginsburg (University of Florida), Nazar Budaiev (University of Florida), Taehwa Yoo (University of Florida); Image Processing: Alyssa Pagan (STScI)
NIRCam
MIRI
Compare NIRCam and MIRI Images of Sagittarius B2
Slide between these images from Webb to see what different wavelengths of infrared light reveal and conceal. Near-infrared light, which is nearest to visible red, comes from some gas and an abundance of colorful stars. The longer wavelengths of mid-infrared light are emitted by warm dust and only the brightest stars. Credits: Image: NASA, ESA, CSA, STScI, Adam Ginsburg (University of Florida), Nazar Budaiev (University of Florida), Taehwa Yoo (University of Florida); Image Processing: Alyssa Pagan (STScI)
Astronomers hope Webb will shed light on why star formation in the galactic center is so disproportionately low. Though the region is stocked with plenty of gaseous raw material, on the whole it is not nearly as productive as Sagittarius B2. While Sagittarius B2 has only 10 percent of the galactic center’s gas, it produces 50 percent of its stars.
“Humans have been studying the stars for thousands of years, and there is still a lot to understand,” said Nazar Budaiev, a graduate student at the University of Florida and the co-principal investigator of the study. “For everything new Webb is showing us, there are also new mysteries to explore, and it’s exciting to be a part of that ongoing discovery.”
The James Webb Space Telescope is the world’s premier space science observatory. Webb is solving mysteries in our solar system, looking beyond to distant worlds around other stars, and probing the mysterious structures and origins of our universe and our place in it. Webb is an international program led by NASA with its partners, ESA (European Space Agency) and CSA (Canadian Space Agency).
Stars, gas and cosmic dust in the Sagittarius B2 molecular cloud glow in near-infrared light, captured by Webb’s NIRCam instrument. The darkest areas of the image are not empty space but are areas where stars are still forming inside dense clouds that block their light
Sagittarius B2 (MIRI Image)
Webb’s MIRI instrument shows the Sagittarius B2 region in mid-infrared light, with warm dust glowing brightly. Only the brightest stars emit strongly enough to appear through the dense clouds as blue pinpoints.
Sagittarius B2 (NIRCam Compass Image)
This image of the Sagittarius B2 (Sgr B2) molecular cloud, captured by the NIRCam (Near-Infrared Camera) instrument on NASA’s James Webb Space Telescope includes compass arrows, scale bar, and color key for reference.
Sagittarius B2 (MIRI Compass Image)
This image of the Sagittarius B2 (Sgr B2) molecular cloud, captured by MIRI (Mid-Infrared Instrument) on NASA’s James Webb Space Telescope includes compass arrows, scale bar, and color key for reference.
Sagittarius B2 NIRCam to MIRI Fade
See what different wavelengths of infrared light reveal and conceal. Near-infrared light, which is nearest to visible red, comes from some gas and an abundance of colorful stars. The longer wavelengths of mid-infrared light are emitted by warm dust and only the brightest stars….
The Milky Way appears above Earth’s bright atmospheric glow in this Aug. 23, 2025, photograph from the International Space Station as it soared 261 miles above southern Iran at approximately 12:54 a.m. local time. The camera was configured for low light and long duration settings.
This image by NASA’s James Webb Space Telescope’s Near-Infrared Camera (NIRCam) features the central region of the Chamaeleon I dark molecular cloud, which resides 630 light years away. The cold, wispy cloud material (blue, center) is illuminated in the infrared by the glow of the young, outflowing protostar Ced 110 IRS 4 (orange, upper left). The light from numerous background stars, seen as orange dots behind the cloud, can be used to detect ices in the cloud, which absorb the starlight passing through them.
An international team of astronomers has reported the discovery of diverse ices in the darkest regions of a cold molecular cloud measured to date by studying this region. This result allows astronomers to examine the simple icy molecules that will be incorporated into future exoplanets, while opening a new window on the origin of more complex molecules that are the first step in the creation of the building blocks of life.
Hello, folks, and welcome back to your favorite Friday roundup of all the space news fit to print. This week we’ve got experimental rocket engines, a gigantic map, and galaxies galore. The James Webb Space Telescope found hydrogen in a galaxy more than eight billion light years away, and the coldest ice ever, but it’s currently down due to a software glitch.
Closer to home, Rocket Lab launched their Electron rocket from US soil for the first time. NASA came together for a day of remembrance that somehow managed to be both somber and ineffably sweet.
JWST Spots the Coldest Chamaeleon
If you wish to make an apple pie from scratch, you must first invent the universe. And somewhere along the way, you’ll need one of the ancient molecular clouds of dust and ice from which stars and habitable planets like Earth are born. This week, Webb scientists announced that the telescope has spotted just such a place. It’s a stellar nursery called the Chamaeleon I cloud, loaded with these primordial crystals. That’s the tableau you’re seeing in the image above — you can tell it’s from Webb by those iconic six-pointed stars. The ice contains traces of sulfur and ammonia, along with simple organic molecules like methanol. And at just ten degrees above absolute zero, it’s the coldest ice ever found.
“We simply couldn’t have observed these ices without Webb,” said Klaus Pontoppidan, a Webb project scientist involved in the research. “The ices show up as dips against a continuum of background starlight. In regions that are this cold and dense, much of the light from the background star is blocked, and Webb’s exquisite sensitivity was necessary to detect the starlight and therefore identify the ices in the molecular cloud.”
‘Virginia Is for Launch Lovers’: Rocket Lab Launches Electron Rocket From US Soil
Late Wednesday evening, aerospace startup Rocket Lab successfully launched its Electron rocket from NASA’s Wallops Flight Facility in Virginia. This was the 33rd launch of the Electron, but its first launch from American soil.
The Electron isn’t reusable — but in 2021, Rocket Lab announced the Neutron. Designed for reusability, the Neutron will have about a third of the lift capacity of a Falcon 9.
NASA ‘Rotating Detonation Engine’ Aces Hot Fire Tests
Speaking of 3D-printed rocket engines: NASA announced this week that it has successfully validated a next-gen rocket engine it hopes will revolutionize rocket design. The new engine generates thrust “using a supersonic combustion phenomenon known as a detonation.” And this is no experimental error — their full-scale alpha build produced more than 4,000 pounds of thrust at full throttle.
These engines get their name (rotating detonation rocket engine, or RDRE) from the unique way they produce thrust. Detonation waves echo around a circular chamber, wringing out every bit of energy from the rocket fuel. It’s great for efficiency, but it puts the whole system under extreme pressure. Undaunted, NASA turned to an advanced additive manufacturing process, even developing its own bespoke metal alloy for the task.
According to the agency, the RDRE incorporates the agency’s GRCop-42 copper alloy into a powder bed fusion (PBF) additive manufacturing process. PBF uses a laser or particle beam to seamlessly fuse ultra-fine particles. It’s a lot like the sintering process used to make the space shuttle rocket engines — and even they had to be actively cooled by the rockets’ own cryofuel, in order to withstand the unearthly temperatures and pressures of takeoff. If the design holds up, NASA intends to use RDRE in its efforts to establish a long-term presence off-planet.
Dark Energy Detector Plots Largest-Ever Map of Galaxy
Astronomers have created a gargantuan map of the Milky Way, using a telescope built to detect dark energy. Featuring more than three billion stars, it focuses on the galaxy’s orbital plane — a region notoriously difficult to study.
Earth’s atmosphere scatters starlight so that points of light turn into point clouds. So, the astronomers just dove right in. To isolate different stars and celestial objects, the group used some extra-snazzy math to get rid of noise. This allowed them to “paint in” the proper background, letting them tell one star from another.
Astronomers have released a gargantuan survey of the galactic plane of the Milky Way. The new dataset contains a staggering 3.32 billion celestial objects — arguably the largest such catalog so far. The data for this unprecedented survey were taken with the US Department of Energy-fabricated Dark Energy Camera at the NSF’s Cerro Tololo Inter-American Observatory in Chile, a Program of NOIRLab. Credit: Saydjari et al., via NoirLab
“One of the main reasons for the success of DECaPS2 is that we simply pointed at a region with an extraordinarily high density of stars and were careful about identifying sources that appear nearly on top of each other,” said Andrew Saydjari, lead author on the (open-access!) paper accompanying the gigantic map. “Doing so allowed us to produce the largest such catalog ever from a single camera, in terms of the number of objects observed.”
Experts: Milky Way Too Large for Its “Cosmological Wall”
The history of astronomy has been all about recognizing that our place in the universe isn’t all that special. We’ve gone from the center of all existence to just another planet orbiting an average star in one of billions and billions of galaxies. However, a new simulation hints that there might be something special about the Milky Way after all.
Yepun, one of the four Unit Telescopes of the Very Large Telescope (VLT) at the European Southern Observatory, studies the center of the Milky Way. Yepun’s laser beam creates an artificial “guide star” to calibrate the telescope’s adaptive optics. Image: ESO/Yuri Beletsky
The model suggests that the Milky Way is far larger than it should be, based on the scale of the “cosmological wall”: an incomprehensibly huge semi-planar structure occupied by the Milky Way and other galaxies in the Local Group.
Scientists Detect Atomic Hydrogen in Most Distant Galaxy Ever
An international team of astronomers announces the discovery of cold atomic hydrogen, more than eight billion light-years from Earth. Cooler than ionized plasma but warmer than molecular hydrogen gas, atomic hydrogen is the raw fuel of coalescing stars. The researchers used gravitational lensing to spot the telltale — but deeply redshifted — 21cm line.
Webb Spies Centaur Chariklo’s Delicate Rings
Named for the daughter of Apollo, Chariklo is a centaur: a Kuiper belt object that orbits out past Saturn. It’s the first of its kind ever found with a confirmed ring system. The thing really is tiny; it’s about 160 miles in diameter and has less than two percent the mass of Earth. But a new report from Webb shows even that much mass is enough to sustain two slender rings, for a time.
In a remarkable stroke of scientific luck, the telescope was pointed just right to catch Chariklo as it passed in front of a star. When it did, the star’s light fluttered in a way that betrayed the presence of the rings.
Chariklo has two thin rings — the first rings ever detected (in 2013) around a small Solar System object. When Webb observed the occultation, scientists measured dips in the brightness of the star. These dips corresponded exactly as predicted to the shadows of Chariklo’s rings. pic.twitter.com/sqH08v1lOB
Nothing less than delighted, the astronomers report that Chariklo’s rings are two and four miles wide, respectively. But the asteroid actually has something in common with the Chamaeleon I cloud. Chariklo’s surface is covered in exotic phases of water ice that only Webb can see.
Principal investigator Dean Hines added, “Because high-energy particles transform ice from crystalline into amorphous states, detection of crystalline ice indicates that the Chariklo system experiences continuous micro-collisions that either expose pristine material or trigger crystallization processes.” It’ll be up to the JWST to find out more.
Software Glitch Brings JWST Down for Maintenance
Unfortunately, observations of Chariklo and other celestial bodies will have to wait a while. The JWST had a software glitch this week. Per NASA, the telescope’s Near Infrared Imager and Slitless Spectrograph (NIRISS) “experienced a communications delay within the instrument, causing its flight software to time out.” Unfortunately, this led to a software gridlock.
The telescope is unavailable for science observations because NASA and the Canadian Space Agency are doing root-cause analysis to figure out and fix the problem. But NASA emphasizes that the telescope is fine. There’s no damage and no indication of any danger. If it’s a software problem, it may well be a software fix.
Perseverance Files First Weather Report
Now that it’s been on Mars for a while, the Perseverance rover has filed an authoritative report on Martian weather. The number one takeaway: It’s cold on the Red Planet! The average surface temperature is -67C.
It’s also windy on Mars. Since Mars has an atmosphere, it has surface weather. It also has an axial tilt, so it has seasons, just like Earth. Dust storms can envelop Mars’ entire northern hemisphere.
Plumes of darker, subsurface dust waft to the surface when the sun warms Martian sands beneath transparent sheets of ice. Mars’ shifting winds then blow these plumes of dust into V-shaped patterns. Astronomers are using the plumes to learn more about Mars’ weather and surface climate. Image: NASA
Perseverance is covered in a suite of sensors that constantly monitor wind speed and direction, atmospheric pressure, temperature, humidity, and dust. Together, they make the rover’s Mars Environmental Dynamics Analyzer (MEDA).
Here, you can see the MEDA sensors extending from the rover’s mast below the iconic ChemCam.
“The dust devils are more abundant at Jezero than elsewhere on Mars and can be very large, forming whirlwinds more than 100 meters in diameter. With MEDA we have been able to characterize not only their general aspects (size and abundance) but also to unravel how these whirlwinds function,” says Ricardo Hueso, of the MEDA team.
Perseverance has captured numerous dust devils as they sweep through Jezero Crater. However, to get that data, MEDA’s exposed sensors also face damage from the harsh radiation environment, extreme temperature swings, and the ever-present Martian dust. A dust devil in January of last year kicked up enough debris that it damaged one of MEDA’s wind instruments. Still, the rover perseveres.
NASA’s Bittersweet 2023 Day of Remembrance
Every year, NASA holds a memorial for staff, astronauts, and alumni who have died. 2023’s Day of Remembrance holds a somber significance, as Feb. 1 is the 20th anniversary of the Columbia disaster. Unfortunately, this year’s fallen also included Apollo 7 pilot Walt Cunningham, who passed earlier this month. Cunningham was the last surviving member of the Apollo 7 crew.
As in years past, NASA staff gathered this week at space centers and labs around the country, to honor the sacrifices of those who have given their lives in pursuit of exploration and discovery. But they did it in a way only NASA could do. They held nationwide town-hall safety meetings, to reflect on and improve NASA’s aerospace safety culture.
Ask not for whom the safety alarm tolls; it tolls for thee. NASA safety-culture town hall meeting at its Washington headquarters after the Arlington memorial service. Image: NASA/Keegan Barber via NASA HQ Flickr
What a fitting way to honor lives lost, while still reaching for the stars. Town-hall safety culture meetings. We love you guys. Never change.
Psyche Mission Now Targeting October 2023 Launch
Steady as she goes: After a year’s delay and a missed launch window, NASA’s Psyche mission team is getting the spacecraft in shape to launch this year. In a blog post, the agency said, “After a one-year delay to complete critical testing, the Psyche project is targeting an October 2023 launch on a SpaceX Falcon Heavy rocket.”
When it launches, Psyche will carry a technology demo for NASA’s shiny new Deep Space Optical Communications (DSOC) network. DSOC systems will use lasers for high-bandwidth communications between Earth and the Moon, Mars, and beyond. Beyond a deluge of scientific data, NASA expects that the network will be able to handle high-def images and video.
Skywatchers Corner
Comet C/2022 E3 (ZTF) is a long-period comet that last visited Earth in the time of the Neanderthals. Now it’s back for another close approach. And although we didn’t know this when we found it last year, it turns out the comet’s tail glows pale green, like a luna moth under a streetlight.
The robin’s-egg glow of Comet C/2022 E3 (ZTF)’s tail shines against its twin tails. Image: Dan Bartlett/NASA
At first, astronomers thought it might require binoculars to catch a glimpse of the thing. However, as ExtremeTech’s Adrianna Nine writes, the comet is now visible to the naked eye in places across much of the Northern Hemisphere.
Our verdant visitor will continue its brightening trend while it sails toward Earth. It will make its closest approach to us on February 2: perhaps too soon for a Valentine’s Day spectacular, but right on time for Imbolc, Candlemas, and Groundhog Day.
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