
Pluto's 'extreme cousin' is a dwarf planet found at the far reaches of our solar system
Show Caption
Hide Caption
James Webb captures Jupiter's shimmering aurora
NASA'S James Webb Space Telescope captured new details of auroras on Jupiter.
Earth has a newly-discovered neighbor in the solar system.
But the heavenly body – possibly a dwarf planet à la Pluto – isn't a frequent visitor. Located beyond Neptune, its extreme orbit circumnavigates the sun once every 25,000 years, taking it beyond our solar system.
The new object, named 2017 OF201, was discovered by researchers in an astronomical image database while searching for trans-Neptunian objects (TNOs) and possible new planets in the outer solar system.
Sihao Cheng, an astrophysicist at the Institute for Advanced Study's School of Natural Sciences, led the team that discovered the object, which he described as an "extreme 'cousin' of Pluto," in a comment on his personal website.
2017 OF201 is about one-third the size of Pluto, which was reclassified as a dwarf planet in August 2006, and "is likely large enough to qualify as a dwarf planet, and its orbit is extremely wide," Cheng said.
Jupiter: Our solar system's biggest planet used to be twice as large: Study
New tough-to-detect dwarf planet has an extreme orbit
'The object's aphelion – the farthest point on the orbit from the Sun – is more than 1600 times that of the Earth's orbit,' Cheng said in a synopsis of the findings posted May 22 on the Institute for Advanced Study (IAS) website. "Meanwhile, its perihelion – the closest point on its orbit to the Sun – is 44.5 times that of the Earth's orbit, similar to Pluto's orbit."
The researchers identified 2017 OF201 using 19 different astronomical database exposures, captured over seven years. The International Astronomical Union's Minor Planet Center officially announced the new object's discovery on May 21, the IAS said.
2017 OF201's extreme orbit makes it detectable about 1% of the time, the researchers said. Spotting 2017 OF201 beyond the Kuiper Belt, a donut-shaped section of space past the orbit of Neptune filled with icy debris, suggests the region may not be as empty as previously thought.
"The presence of this single object suggests that there could be another hundred or so other objects with similar orbit and size; they are just too far away to be detectable now,' Cheng said in the synopsis. 'Even though advances in telescopes have enabled us to explore distant parts of the universe, there is still a great deal to discover about our own solar system.'
The extreme orbit of 2017 OF201 also suggests the object "must have experienced close encounters with a giant planet, causing it to be ejected to a wide orbit,' said Eritas Yang, a Princeton University graduate student who assisted in the research, in the study synopsis.
More than one galactic event could have created 2017 OF201's orbit, Cheng added. "It's possible that this object was first ejected to the Oort cloud, the most distant region in our solar system, which is home to many comets, and then sent back," he said.
New dwarf planet could dash Planet X hypothesis
The new object could also challenge the hypothesis that there's a "Planet X" or "Planet Nine" beyond Pluto, with gravity affecting dwarf planets and other objects in the Kuiper Belt. That's because 2017 OF201's orbit is "well outside the clustering observed in extreme (TNOs), which has been proposed as dynamical evidence for a distant, undetected planet," the researchers write in a draft version of their submitted research.
"The existence of 2017 OF201 might suggest that Planet 9 or X doesn't exist," said Jiaxuan Li, another Princeton University astrophysical sciences grad student who collaborated on the research, on his personal website.
But research will continue. "I hope Planet 9 still exists, because that'll be more interesting," Cheng told the New Scientist.
Contributing: Doyle Rice and Elizabeth Weise.
Mike Snider is a reporter on USA TODAY's Trending team. You can follow him on Threads, Bluesky, X and email him at mikegsnider & @mikegsnider.bsky.social & @mikesnider & msnider@usatoday.com
What's everyone talking about? Sign up for our trending newsletter to get the latest news of the day
Hashtags

Try Our AI Features
Explore what Daily8 AI can do for you:
Comments
No comments yet...
Related Articles
Yahoo
3 hours ago
- Yahoo
Nearby super-Earth K2-18 b may be a water-rich ocean planet: 'This has certainly increased the chances of habitability'
When you buy through links on our articles, Future and its syndication partners may earn a commission. The saga surrounding Neptune-size "super-Earth" exoplanet K2-18 b just got a whole lot more interesting. For a quick recap, this is the world a team of scientists recently suggested could host life — to the dismay of other scientists in the community, who felt the announcement failed to include necessary caution. While signs of life on the world have failed to conclusively present themselves to the James Webb Space Telescope (JWST), the powerful space telescope has discovered that this planet is so rich in liquid water that it could be an ocean, or "Hycean" world. "This has certainly increased the chances of habitability on K2-18 b" Nikku Madhusudhan, the University of Cambridge scientist behind the original K2-18b discovery as well as the new study, told "This is a very important development and further increases the chance of a Hycean environment in K2-18 b. It confirms K2-18 b to be our best chance to study a potential habitable environment beyond the solar system at the present time." The story regarding the habitability of K2-18 b began back in April 2025, when Madhusudhan and fellow researchers from the University of Cambridge announced they had found what they called the "strongest evidence yet" of life beyond the solar system around this distant super-Earth (it's around nine times as massive as our planet). The evidence came from the tentative detection of molecules that, when found in the atmosphere of Earth, are typically the result of biological processes of living things. The pressure was then on to confirm these potential biosignatures: dimethyl sulfide and dimethyl disulfide. The team set about this by observing four separate instances of K2-18 b crossing, or "transiting," the face of its parent red dwarf star, located about 124 light-years away, during its roughly 33-Earth-day orbit. Because chemicals absorb and emit light at characteristic wavelengths, when light from a parent star passes through a planet's atmosphere, the molecules in that atmosphere leave their telltale fingerprints in the spectrum of starlight. "With four additional transit observations using JWST, we have measured the spectrum of K2-18 b's atmosphere with unprecedented precision," Renyu Hu, the new study's team leader and a NASA Jet Propulsion Lab scientist, told "The spectrum allowed us to conclusively detect both methane and carbon dioxide in the planet's atmosphere and to constrain their abundances. This information points to a planet with a water-rich interior." Hu explained that the team searched for signals of dimethyl sulfide and other organic sulfur molecules in the spectrum using several independent models, but did not find conclusive evidence for their presence. "This was not necessarily disappointing," Hu continued. "We're excited about establishing the planet's water-rich nature." Is K2-18 b a ocean world? Saying it's now confirmed that K2-18 b is water-rich, Hu explained that the next step is to discover if the planet possesses a global liquid water ocean. Ironically, one of the most positive signs of such an ocean is the fact that the atmosphere of this super-Earth appears to lack water vapor. "The spectrum we obtained does not show signs of water vapor. If the atmosphere truly lacks water, this suggests that water has been depleted — most likely through condensation," Hu said. "On Earth, this process is known as the 'cold trap,' and geoscientists consider it essential for retaining water over billions of years by preventing it from escaping to space. "Observing a similar process on an exoplanet would be very exciting. Rigorously confirming the absence of water can by itself be a scientifically important goal for future observations," Hu said. However, Hu cautioned that the spectrum detected by the JWST could also be explained by an alternative model in which the atmosphere actually contains abundant water vapor. Establishing whether K2-18 b and other similar temperate, sub-Neptune-sized planets possess liquid water oceans, Hu says, will also require detecting the presence of a broader set of atmospheric gases beyond methane and carbon dioxide. It would also require an absence of molecules like ammonia, carbon monoxide and sulfur dioxide, which, as of yet, have indeed not been detected in the atmosphere of K2-18 b "This conclusion is based on theoretical work by my group and several others," Hu added. "With the new observations providing valuable context, we've summarized these insights into a roadmap to help guide future observations and studies." Meanwhile, the search for the biosignatures, dimethyl sulfide and dimethyl disulfide, is far from done; while not hitting the significance level required for a confirmation, this research did provide a stronger signal from these molecules than were provided by previous examinations. "The evidence for dimethyl sulfide in the present work is significantly higher than what we had with our previous observations in the same near-infrared wavelength range," Madhusudhan said. "However, this evidence is still not high enough to claim a conclusive detection. "We also need to be able to distinguish dimethyl sulfide from other possible contributors, such as methyl mercaptan, which is also a biosignature on Earth." Related Stories: — The mystery of how strange cosmic objects called 'JuMBOs' went rogue — These mysterious objects born in violent clashes between young star systems aren't stars or planets — James Webb Space Telescope dives into the atmosphere of a mystery rogue planet or failed star It looks certain that K2-18 b will continue to hold the interest of astronomers for some time. "It is great that we are able to infer tentative signs of potential biosignatures with current JWST observations, but significantly more time is needed for conclusive detections. A key question is whether the atmosphere contains one or more biosignatures," Madhusudhan said. "At the same time, extensive theoretical and experimental efforts are needed to robustly identify biological and non-biological pathways for candidate biosignature molecules." One thing the team is sure of, though, is the progress made thus far in the study of K2-18 b wouldn't have been possible without the JWST. And, the $10 billion space telescope is set to play a key role in the future investigation of this super-Earth. "Our observations and analyses add to the growing list of exciting discoveries that highlight the truly transformative science enabled by JWST," Hu concluded. "While we found its Near-Infrared Spectrograph [NIRSpec] particularly well suited to address the goals of our study, other JWST instruments or observational modes could provide complementary and highly valuable information to further enhance our understanding of this planet." The team's research is available as a preprint on the paper repository arXiv. Solve the daily Crossword


The Hill
6 hours ago
- The Hill
How NASA found ‘city killer' asteroid's new potential target: the moon
(KTLA) – Although it won't hit Earth, an asteroid once labeled a ' city killer ' is now back in the spotlight — this time, because it might hit the moon. Nexstar's KTLA spoke with Davide Farnocchia, a navigation engineer at NASA's Jet Propulsion Laboratory who works in the agency's Center for Near-Earth Object Studies. He shared how scientists tracked the 200-foot-long asteroid's shifting path, right up until it slipped out of view — for now. 'You can call it a city killer, but there's no city at risk. The Earth is out of the way,' Farnocchia said. 'But the moon is not.' Asteroid 2024 YR4, first spotted in December 2024, is now being closely monitored as a potential lunar impactor in 2032. 2024 YR4: The 'city killer' that threatened to hit Earth in 2032 Just weeks after its discovery, YR4 made headlines when its odds of hitting Earth spiked to 3.1 percent, making it the most threatening asteroid observed in over two decades. That risk earned it a 3 out of 10 on the Torino scale, a rarely used classification signaling a credible, though uncertain, threat. Farnocchia recalled the moment his team had to alert astronomers of the impact probability. 'We had to notify them and say, 'Look, this object should get higher priority in your schedule for observing asteroids tonight,'' he said. 'We needed more data to hopefully prove that it would move away from the Earth, which is what almost always happens.' But instead of fading from concern, YR4's risk level climbed. By mid-February 2025, the asteroid had a 1 in 32 chance of impacting Earth. An impact of its size could have devastated a metropolitan area if it had struck land. 'YR4 represented the most significant impact risk that we had over the last 20 years,' said Farnocchia. 'However, we communicated early on that the probability would likely drop as we got more data, and that's exactly what happened.' By the end of February, improved measurements helped rule out an Earth impact, but the story didn't end there. Not a threat to Earth. But what about the moon? While Earth was taken off the risk list, the moon quietly took its place. In May, scientists captured one final look at YR4 with NASA's James Webb Space Telescope before it slipped too far from view. That data, released in June, refined its projected path for Dec. 22, 2032, and raised the odds of a lunar impact to 4.3 percent. That's up from 3.8 percent in April, and just 1.7 percent earlier in the year. Even so, Farnocchia emphasized: 'The moon is smaller than the Earth, but it's a large body, so even an asteroid of 200 feet is not going to do much to it.' He noted that it wouldn't alter the motion of the moon. And while a 4.3 percent chance may sound notable, it's still considered low by risk standards. Still, Farnocchia said, it's unusual to see the moon become a potential target at all. 'It should be less likely,' he said. 'In fact, you have a lot more impacts on Earth than on the moon; that checks out. It's much easier to hit the Earth than the moon … but now the moon happens to be in the realm of possibilities.' 2024 YR4 might not dazzle, but Apophis will If 2024 YR4 were to hit the moon, don't expect a light show. 'If it hits the moon, the impact wouldn't be visible to the naked eye,' the NASA engineer said. 'You'd need a pretty big telescope, and even then, it might be hard to detect from Earth.' But skywatchers won't have to wait long for something more dramatic. On April 13, 2029, the asteroid Apophis — about 1,100 feet wide — will fly closer to Earth than many satellites, putting on a rare and safe spectacle. 'It's going to be so close, and given its size, it's going to be bright enough to be visible to the naked eye. It's going to be as bright as the stars in the Little Dipper,' Farnocchia said. Apophis' flyby is one of the closest ever recorded for an object of its size. NASA says it may be the first such event humans have witnessed with modern instruments. 'An asteroid this large passes this close to Earth only every few thousand years on average, so it's likely that an event like this has not happened at any time in recorded human history,' the organization stated. 'Without a doubt this is the first time it's happened when humans have had the technology to observe it.' How good is NASA at predicting impacts? Very good — and getting better. 'We had a few very small objects discovered before reaching Earth. They burn up harmlessly, but predicting their impacts and locations felt like a big accomplishment,' Farnocchia said. New observation tools and modeling techniques are making it possible to predict not only impact locations, but even recover fragments from impacts. 'Recently, we were able to predict impact locations and recover meteorites, which is kind of interesting because that's a final validation that you predicted the right impact point,' he said. 'One colleague was notified of an impact predicted in Canada, so he just went outside and set up a camera to observe it. That was really cool.' Why it matters While the moon isn't in any real danger, 2024 YR4 has become a key case study for NASA's planetary defense systems. It's the first object since Apophis to climb to a 3 on the Torino Scale, and the first ever tracked with the James Webb Space Telescope, which improved impact projections by nearly 20 percent. 'There is so much I could say about YR4 — it was really interesting to see the orbit behave exactly as we expected,' Farnocchia said. 'I like to see how the predictions evolve with each new set of observations. It's a sign that our models are working well.' NASA expects YR4 to reenter view in 2028 for another round of observations — and possibly another plot twist.


Fast Company
11 hours ago
- Fast Company
Light pollution is making it harder for astronomers to study the universe
Outdoor lighting for buildings, roads and advertising can help people see in the dark of night, but many astronomers are growing increasingly concerned that these lights could be blinding us to the rest of the universe. Hot science in the cold, dark night While orbiting telescopes like the Hubble Space Telescope or the James Webb Space Telescope give researchers a unique view of the cosmos—particularly because they can see light blocked by the Earth's atmosphere—ground-based telescopes also continue to drive cutting-edge discovery. Telescopes on the ground capture light with gigantic and precise focusing mirrors that can be 20 to 35 feet wide. Moving all astronomical observations to space to escape light pollution would not be possible, because space missions have a much greater cost and so many large ground-based telescopes are already in operation or under construction. Around the world, there are 17 ground-based telescopes with primary mirrors as big or bigger than Webb's 20-foot mirror, and three more under construction with mirrors planned to span 80 to 130 feet. The newest telescope starting its scientific mission right now, the Vera Rubin Observatory in Chile, has a mirror with a 28-foot diameter and a 3-gigapixel camera. One of its missions is to map the distribution of dark matter in the universe. To do that, it will collect a sample of 2.6 billion galaxies. The typical galaxy in that sample is 100 times fainter than the natural glow in the nighttime air in the Earth's atmosphere, so this Rubin Observatory program depends on near-total natural darkness. Any light scattered at night—road lighting, building illumination, billboards—would add glare and noise to the scene, greatly reducing the number of galaxies Rubin can reliably measure in the same time, or greatly increasing the total exposure time required to get the same result. The LED revolution Astronomers care specifically about artificial light in the blue-green range of the electromagnetic spectrum, as that used to be the darkest part of the night sky. A decade ago, the most common outdoor lighting was from sodium vapor discharge lamps. They produced an orange-pink glow, which meant that they put out very little blue and green light. Even observatories relatively close to growing urban areas had skies that were naturally dark in the blue and green part of the spectrum, enabling all kinds of new observations. Then came the solid-state LED lighting revolution. Those lights put out a broad rainbow of color with very high efficiency, meaning they produce lots of light per watt of electricity. The earliest versions of LEDs put out a large fraction of their energy in the blue and green, but advancing technology now gets the same efficiency with 'warmer' lights that have much less blue and green. Nevertheless, the formerly pristine darkness of the night sky now has much more light, particularly in the blue and green, from LEDs in cities and towns, lighting roads, public spaces, and advertising. The broad output of color from LEDs affects the whole spectrum, from ultraviolet through deep red. The U.S. Department of Energy commissioned a study in 2019 which predicted that the higher energy efficiency of LEDs would mean that the amount of power used for lights at night would go down, with the amount of light emitted staying roughly the same. But satellites looking down at the Earth reveal that just isn't the case. The amount of light is going steadily up, meaning that cities and businesses were willing to keep their electricity bills about the same as energy efficiency improved, and just get more light. Natural darkness in retreat As human activity spreads out over time, many of the remote areas that host observatories are becoming less remote. Light domes from large urban areas slightly brighten the dark sky at mountaintop observatories up to 200 miles away. When these urban areas are adjacent to an observatory, the addition to the skyglow is much stronger, making detection of the faintest galaxies and stars that much harder. When the Mount Wilson Observatory was constructed in the Angeles National Forest near Pasadena, California, in the early 1900s, it was a very dark site, considerably far from the 500,000 people living in Greater Los Angeles. Today, 18.6 million people live in the L.A. area, and urban sprawl has brought civilization much closer to Mount Wilson. When Kitt Peak National Observatory was first under construction in the late 1950s, it was far from metro Tucson, Arizona, with its population of 230,000. Today, that area houses 1 million people, and Kitt Peak faces much more light pollution. Even telescopes in darker, more secluded regions—like northern Chile or western Texas—experience light pollution from industrial activities like open-pit mining or oil and gas facilities. The case of the European Southern Observatory An interesting modern challenge is facing the European Southern Observatory, which operates four of the world's largest optical telescopes. Their site in northern Chile is very remote, and it is nominally covered by strict national regulations protecting the dark sky. AES Chile, an energy provider with strong U.S. investor backing, announced a plan in December 2024 for the development of a large industrial plant and transport hub close to the observatory. The plant would produce liquid hydrogen and ammonia for green energy. Even though formally compliant with the national lighting norm, the fully built operation could scatter enough artificial light into the night sky to turn the current observatory's pristine darkness into a state similar to some of the legacy observatories now near large urban areas. This light pollution could mean the facility won't have the same ability to detect and measure the faintest galaxies and stars. Light pollution doesn't only affect observatories. Today, around 80% of the world's population cannot see the Milky Way at night. Some Asian cities are so bright that the eyes of people walking outdoors cannot become visually dark-adapted. In 2009, the International Astronomical Union declared that there is a universal right to starlight. The dark night sky belongs to all people—its awe-inspiring beauty is something that you don't have to be an astronomer to appreciate. Richard Green is an astronomer emeritus at Steward Observatory at the University of Arizona. The early-rate deadline for Fast Company's Most Innovative Companies Awards is Friday, September 5, at 11:59 p.m. PT. Apply today.