A Colossal Telescope in the Desert Just Captured Galaxies We've Never Seen Before
Here's what you'll learn when you read this story:
After more than a decade under construction, the Vera Rubin Observatory has released its first images, which contain millions of galaxies.
These first images are only the brief, initial glimpse of the observatory's 10-year Legacy Survey of Space and Time (LSST), which will discover new objects in the night sky while also (hopefully) answering questions about dark matter and dark energy.
As a ground-based telescope, the Vera Rubin Observatory will be a perfect companion to space-based telescopes like the James Webb Space Telescope, as its sweeping view will completely scan the night sky every three days.
On August 1, 2014, workers began construction of the Large Synoptic Survey Telescope (LSST) perched atop Cerro Pachón in Chile's Atacama Desert. Fast forward a decade later, and the LSST—now called the Vera C. Rubin Observatory, named for the American astronomer whose groundbreaking work provided evidence for the existence of dark matter—is finally ready to start doing some serious science.
Its main mission will be the Legacy Survey of Space and Time (confusingly also abbreviated LSST), which will ceaselessly scan the night sky continuously for 10 years, noting every visible change along the way. Vera Rubin is particularly well-suited for this task—with a 28-foot-wide primary mirror, and 11-foot-wide secondary mirror, and the largest digital camera ever constructed, this terrestrial telescope can move its 300-ton bulk one full rotation in a half a minute at full speed, according to The New York Times. The amount of data Rubin will collect in the next year alone will be more than all other optical observatories combined. To put it mildly, it's an exciting time.
To celebrate the beginning of its operation, the observatory has released the first images captured by the telescope. A combination of 678 different images, the photo above shows that brilliant Trifid nebula (top right) with the Lagoon nebula (bottom left), which is located more than 4,000 light-years from Earth. The lead image of this article (an in-depth look at the Virgo cluster) is only 2 percent of a full Rubin image, which would actually require 400 ultra high-definition TVs to display. Below is a labeled image of a swath of galaxies and stars—some of which we know, and many of which we've never seen before.
'These images vividly showcase the unprecedented power that Rubin will use to revolutionize astronomy and our understanding of the Universe,' astronomers Manda Banerji and Phil Wiseman from the University of Southampton wrote in The Conversation. 'Rubin is truly transformative, thanks to its unique combination of sensitivity, vast sky area coverage and exceptional image quality.'
It's a big moment for ground-based astronomy, which has often been eclipsed by groundbreaking discoveries made by space-based telescopes like Hubble and JWST. While it's true that these floating telescopes offer a ton of benefits—chief among them being that they circumvent atmospheric interference and the increasing annoyance of satellite disruption (think Starlink)—the benefits of ground-based observatories far outweigh these visual costs.
For one, these telescopes can be easily maintained and—crucially—upgraded with the latest and greatest technologies because... you know... they're on the ground. And without the need for payload restrictions, ground-based telescopes can be absolutely gargantuan (look no further than the adequately named Extremely Large Telescope, also under construction in the Atacama Desert). A quick comparison: JWST's Near Infrared Camera has a field of view of roughly 0.05 square degrees, whereas Vera Rubin has a full 9.6 square degrees. That means it can simply see way more sky than its space-based cousins. Rubin will also be able to produce incredibly high-definition photographs in just a few days, rather than the few years needed by other telescopes.
At the end of its 10-year LSST mission, Rubin will provide invaluable data for investigating dark energy and dark matter, as well as information regarding some 20 billion galaxies. Rubin will also observe billions of objects on more than 800 separate occasions, which will create a kind of astronomical movie detailing the evolution of the night sky over time. Especially excitingly, it will capture asteroids as they move through the Solar System. The Observatory estimates that LSST will discover five million asteroids in the next few years alone—five times more than what humanity has discovered in the last two centuries.
After decades of waiting, it's time for the science to finally commence.
'[Vera Rubin] represents the culmination of about two decades of dedication, innovation, and collaboration by a global team,' Željko Ivezić, Director of Rubin Observatory Construction, said in a press statement. 'With construction now complete, we're turning our eyes fully to the sky—not just to take images, but to begin a whole new era of discovery.'
You Might Also Like
The Do's and Don'ts of Using Painter's Tape
The Best Portable BBQ Grills for Cooking Anywhere
Can a Smart Watch Prolong Your Life?
Hashtags

Try Our AI Features
Explore what Daily8 AI can do for you:
Comments
No comments yet...
Related Articles
Yahoo
12 hours ago
- Yahoo
Scientists Merged 3 Human Brains by Thought Alone
"Hearst Magazines and Yahoo may earn commission or revenue on some items through these links." Here's what you'll learn when you read this story: Brain-to-brain verbal communication in humans was first accomplished in 2014 when brain-computer interfaces helped transmit a message from India to France. Since then, some progress has been made on technology that could make so-called mind-reading possible, including a device that would allow at least three people to share thoughts. While communication using only thoughts shows promise in the medical field for patients who are unable to speak, when it comes to other uses, there are still many ethical implications that need to be navigated. Mind reading has long existed in science fiction—Vulcan mind meld, anyone?—and those carnivals where alleged mind readers try to part you from your last $10 bill with a promise that they know exactly what you're thinking. But thanks to some recent scientific developments, it is now no longer the stuff of cyberpunk and magic. Back in 2014, two words were heard halfway around the world. Those words were ciao and hola. The only people who heard them were two subjects, one in India and one in France, both of whom were willing subjects for an experiment that wanted to probe into whether it was possible for one person to find out what another was thinking from 5,000 miles away. The non-invasive research merged brain-computer interfaces and computer-brain interfaces. Brain-computer interfaces allow the brain to control a device or application by analyzing and translating brain signals into digital commands, while computer-brain interfaces use a computer to influence brain activity. Wireless EEG recorded brain activity through electrodes on the subjects' heads. When the subject in India sent the message, the letters of the two words were then converted to binary code. The code was transferred to another computer before being sent to the subject in France via internet. Transmission of thoughts from one brain to another succeeded. Because the computer-brain interface used transcranial magnetic stimulation to prepare the receiver by using magnetic fields to boost electrical signals in neurons, the receiver found out when there was a message on the way. This experiment marked the first brain-to-brain verbal communication in humans and opened up a new frontier. 'We speculate that future research could explore the use of closed mind-loops in which information associated to voluntary activity from a brain area or network is captured and, after adequate external processing, used to control other brain elements in the same subject,' the researchers who ran the experiment said at the time in a study published in PLOS One. How far have we come since then? In 2019, another research team invented BrainNet, a non-invasive system that also uses EEG and transcranial magnetic stimulation and became the first multi-person brain-to-brain interface. Meant for problem-solving applications, it can accommodate three people at a time, decoding the brain signals of the two message senders with EEG before transmitting them to the receiver through an internet connection. BrainNet originally demonstrated how three people could silently work together to tackle a computer game similar to Tetris. The researchers predicted that the system could eventually be scaled to accommodate larger groups. The mechanism behind direct brain-to-brain communication, or neural interfacing, in both humans and animals was elucidated in 2021, when veterinary physiologist Ehsan Hosseini hypothesized that the weak magnetic field in one animal's brain was capable of transmitting information to another. He also suggested that cryptochromes, proteins that act as photoreceptors which help regulate circadian rhythm, can actually perceive these magnetic fields and convert them to action potentials, or ultrafast zaps of voltage across the membrane of a neuron. Other studies even claimed that the ability to pick up on weak magnetic field energy may explain telepathy and other paranormal phenomena. More recently, the neurotechnology startup Neuroba is exploring ways to integrate human consciousness with not only brain-computer interfaces, but AI and even quantum communication. They are currently trying to develop algorithms that will allow messages to be delivered more accurately. This could be a breakthrough in the medical field, with patients who are otherwise unable to speak still having the ability to communicate by using just their brains, whose messages will be analyzed and translated by a computer. Beyond medical use, ethical implications for this technology remain unclear. Neuroba also mentions that a device like an updated version of BrainNet could revolutionize the workplace by connecting thoughts during meetings and other collaborative efforts. While some are convinced that hooking up everyone's brains in a conference room would be revolutionary, there are concerns. Everyone reading each other's thoughts and thinking alike, possibly being pressured to think alike, ventures on the robotic and could possibly (brace for another Star Trek reference incoming) create another Borg. There is also the possibility of misusing neural interfacing to invade others' privacy. Ultimately, much of the field still remains unexplored, and a code of ethics will have to be established if it is to be used regularly in the future. You Might Also Like The Do's and Don'ts of Using Painter's Tape The Best Portable BBQ Grills for Cooking Anywhere Can a Smart Watch Prolong Your Life?
Yahoo
17 hours ago
- Yahoo
James Webb Space Telescope uses cosmic archeology to reveal history of the Milky Way galaxy
When you buy through links on our articles, Future and its syndication partners may earn a commission. Astronomers taken on the role of cosmic archeologists, using the James Webb Space Telescope (JWST) to excavate over 100 disk galaxies from up to 11 billion years ago. Just like artifacts excavated here on Earth tell the story of the human race, these galaxies could tell the story of our galaxy, the Milky Way. The aim of this investigation was to discover why galaxies like the Milky Way are constructed of thick disks of stars with embedded thin stellar disks. Each of these disks feature its own distinct stellar population with its own movement. The team behind this research wanted to know how and why this "dual-disk" structure forms, turning to observations of 111 disk galaxies that are oriented "edge-on" from our perspective here on Earth. This represented the first time astronomers had studied thick- and thin-disk structures of galaxies that existed during the infant stages of the cosmos, as early as 2.8 billion years after the Big Bang. "This unique measurement of the thickness of the disks at high redshift, or at times in the early universe, is a benchmark for theoretical study that was only possible with the JWST," team leader Takafumi Tsukui of the Australian National University said in a statement. "Usually, the older, thick disk stars are faint, and the young, thin disk stars outshine the entire galaxy. "But with the JWST's resolution and unique ability to see through dust and highlight faint old stars, we can identify the two-disk structure of galaxies and measure their thickness separately." The first step for the team was to separate the 111 galaxies in the sample into two categories: dual-disked and single-disked. What this seemed to reveal was that galaxies grow their thick stellar disk first, with the thin disk forming at a later point. The team thinks the timing of these disk formation processes hinges on the mass of the galaxy in question. High-mass, single-disk galaxies transformed into dual-disk structures by forming an embedded thin disk around 8 billion years ago in our approximately 14-billion-year-old universe. Lower-mass galaxies only seemed to undergo this transformation when they were around 4 billion years old. "This is the first time it has been possible to resolve thin stellar disks at higher redshift. What's really novel is uncovering when thin stellar disks start to emerge," Emily Wisnioski, study team member and a researcher at the Australian National University, said in the statement. "To see thin stellar disks already in place 8 billion years ago, or even earlier, was surprising." The team then set about determining what caused the transitions for these different types of galaxies. To do this, the researchers went beyond their sample of 111 galaxies to investigate how gas flowed around these subjects. They used gas-motion data from the Atacama Large Millimeter/submillimeter Array (ALMA) — a collection of 66 antennas in northern Chile that work together as a single telescope — and other ground-based observatories. This showed that turbulent gas in the early universe triggers bouts of intense star formation in galaxies, birthing these galaxies' thick stellar disks. As these thick-disk stars form, the gas is stabilized, becoming less turbulent and thinning out. That leads to the formation of the embedded thin stellar disk. This process, the team says, takes a different amount of time in high-mass galaxies and low-mass galaxies because the former convert gas to stars more efficiently than the latter. That means gas is depleted more rapidly in high-mass galaxies, getting them to the point at which their thin stellar disks can form more quickly. This links to our own galaxy as well. The timing of these transitions matched the period at which the Milky Way is theorized to have grown its own thin disk of stars. All in all, the team's research demonstrates the ability of the JWST to peer back in time and find galaxies that match the evolution of our own galaxy, allowing these galaxies to act as proxies that tell the story of the Milky Way. Related Stories: — The Milky Way may not collide with neighboring galaxy Andromeda after all: 'From near-certainty to a coin flip' —Astronomers capture the most intricate picture of a galaxy in a thousand colors ever seen (photo, video) —'The models were right!' Astronomers locate universe's 'missing' matter in the largest cosmic structures The next step for this research will involve the team adding more data to see if the relationships they observed still stand. "There is still much more we would like to explore," Tsukui said. "We want to add the type of information people usually get for nearby galaxies, like stellar motion, age and metallicity [the abundance of elements heavier than hydrogen and helium]. "By doing so, we can bridge the insights from galaxies near and far, and refine our understanding of disk formation."The team's results appear in the July edition of the journal Monthly Notices of the Royal Astronomical Society.
Yahoo
a day ago
- Yahoo
The Rubin Observatory found 2,104 asteroids in just a few days. It could soon find millions more.
When you buy through links on our articles, Future and its syndication partners may earn a commission. It was weirdly emotional on Monday, June 23, as several grainy white specks streaked across my computer screen while ambient rhythms buzzed in the background. Those specks were part of a film that played during the Vera C. Rubin Observatory's highly anticipated first image release conference — and they each represented an asteroid that had just been discovered. It felt like witnessing something hugely profound, and there are two reasons why. First of all, to put it simply, with just a few nights of data, the Rubin Observatory team was able to identify 2,104 never-before-seen asteroids in our solar system — seven of which are categorized as near-Earth objects. (No, none are expected to strike our planet. Don't worry). For context, there are approximately a million known asteroids in our cosmic neighborhood; over the next few years, Rubin could very well hike that figure up to five million. "This is five times more than all the astronomers in the world discovered during the last 200 years since the discovery of the first asteroid," Željko Ivezić, Deputy Director of Rubin's Legacy Survey of Space and Time, said during the conference. "We can outdo two centuries of effort in just a couple of years." This is astonishing in itself — talk about an exemplary first impression — but there's still that second thing that makes Rubin's new asteroid data incredible. They can be formatted as movies. For some context about Rubin, this observatory is our brilliant new ground-based eye on the universe, and is located at the El Peñón peak of Cerro Pachón in Chile. It has the ability to image giant swaths of the sky using the world's largest digital camera — and when I say giant, I mean giant. Related: 6 incredible objects hidden in Vera C. Rubin Observatory's mind-boggling first image One of its first presented images, for instance, features a bunch of glowing, hazy galaxies of all shapes and sizes. It's difficult not to daydream when looking at a couple of lovely lavender spirals that represent realms comparable to our entire Milky Way. But what you see below in this image is only 2% of the full Rubin view: The plan is for Rubin to capture such massive, high-resolution images of the southern sky once every three nights for at least the next 10 years. You can therefore consider it to be a super-fast, super-efficient and super-thorough cosmic imager. Indeed, those qualities are perfect for spotting some of the smallest details trailing through the space around our planet: asteroids. "We make movies of the night sky to see two things: objects that move and objects that change brightness," Ivezić said. "Objects that move come in two flavors. Stars in our galaxy move, and they move slowly. Much faster objects are asteroids." Zooming into a tiny portion of one of Rubin's images, Ivezić pointed out that there are actually invisible photobombers present. He was talking about the asteroid streaks Rubin's software so kindly removed from the main attraction (I mean, look at that spiral). However, the fact that those asteroids can be removed from an image means they can be precisely isolated to begin with, making it possible to really focus on them if you want to — something that isn't always possible with zippy, fleeting space objects. In fact, it's tremendously difficult to record an asteroid at all. "Asteroids, they disappear after you get one picture of them," Ivezić said, calling Rubin's ability to image small objects orbiting the sun "unprecedented." In the Rubin image Ivezić called out to showcase the observatory's asteroid-tracking capabilities, the asteroid streaks are seen in different colors. This is because each corresponds to one exposure used to create the final image. You can think of it as different images stitched together to create a final view of the asteroids' trajectories. And to take things a step further, if you slap a few of these datasets together, you can indicate asteroid motion against the more static background of stars and galaxies — like a movie. This feature of Rubin should be huge not only because it'd allow scientists to better study asteroid movements and discover new near-Earth objects, but also for humanity's efforts in planetary defense. Over the last couple of years, scientists have really started to question how we can protect our planet if an asteroid were headed our way. NASA's wildly successful DART (Double Asteroid Redirection Test) mission — which sent a spacecraft on a death mission to crash into an asteroid and see if the object's trajectory can be changed — was arguably the feat that brought planetary defense to the public eye. It'd also be remiss not to mention all the recent anxiety surrounding Asteroid 2024 YR4, which was potent enough to even penetrate the jokes of a random comedy show in New York City I went to around the time it was making headlines. 2024 YR4 briefly had a head-turning likelihood of hitting our planet before that likelihood shot down to nil. RELATED STORIES —'City killer' asteroid 2024 YR4 could shower Earth with 'bullet-like' meteors if it hits the moon in 2032 —US Representatives worry Trump's NASA budget plan will make it harder to track dangerous asteroids —NASA's Lucy spacecraft snaps first close-ups of weird peanut-shaped asteroid There was even a hearing about asteroid safety in May, held by the U.S. House Committee on Space, Science and Technology, during which U.S. Representatives expressed their concern that asteroid defense may be impacted by President Trump's major science funding cuts. All of this is to say that I imagine a state-of-the-art asteroid detector is very welcome in the scientific community right now. To really illustrate the ultimate promise of Rubin's asteroid adventures, Ivezić brought up a simulation of all asteroids expected to orbit our sun. "This blue donut is a simulation of all asteroids we expect there," he said. "All of these new discoveries are found in this one narrow slice of this big donut. In two or three years, after we start LSST later this year, we will sweep around and discover all of the millions of asteroids." This article was originally published on