Astronomers spot rare interstellar comet speeding through solar system
The comet, recently designated 3I/ATLAS, was first observed on July 1 by the NASA-funded Asteroid Terrestrial-impact Last Alert System telescope in Rio Hurtado, Chile.
At the time of its unexpected discovery, the comet was about 420 million miles from Earth, near Jupiter, and closing in on what is considered the inner solar system.
Despite its distance, NASA said the comet poses no threat to Earth or the Moon, as the interstellar object will remain at least 150 million miles away.
A space diagram shows the comet passing between the orbits of Earth and Mars sometime during late fall or early winter, but because of the alignment of planets and the Sun from September through November, it is not expected to be visible.
"The interstellar comet's size and physical properties are being investigated by astronomers around the world," NASA stated. "3I/ATLAS should remain visible to ground-based telescopes through September, after which it will pass too close to the Sun to observe. It is expected to reappear on the other side of the Sun by early December, allowing for renewed observations."
See The Objects Humans Left Behind On The Moon
Since its initial detection, telescopes located in Hawaii, South Africa, California and dozens of other sites have all spotted the comet, which was estimated to be moving through the galaxy at more than 130,000 miles per hour.
Early estimates suggest the comet could have a diameter of at least 10 miles, but that figure remains uncertain due to observational limits.
According to Nasa, a giant complex of dust and ice is usually less than 10 miles across but can eventually stretch millions of miles when the ice turns into gas and forms a tail.
The space agency did not say where astronomers believe the comet originated, though most such objects are thought to come from the Kuiper Belt or the Oort Cloud.
These regions are anywhere from about 3 billion miles to nearly a light-year away from Earth and are known for their icy, rocky debris left over from the formation of the solar system.
Telescope Captures Stunning Images Of Not 1 But 19 Spiral Galaxies
Currently, the comet is said to be observable only through high-powered telescopes, but that could change later in the year as the interstellar object makes its closest approach to Earth.
The agency also did not state if they believe one day the interstellar object will one day enter into any type of orbit around the Sun.
According to astronomers, the closest a recorded comet has ever come to Earth was in 1770, when what became known as Lexell's Comet passed about 1.4 million miles away.Original article source: Astronomers spot rare interstellar comet speeding through solar system
Hashtags

Try Our AI Features
Explore what Daily8 AI can do for you:
Comments
No comments yet...
Related Articles
Yahoo
9 hours ago
- Yahoo
Satellite spies both ISS and China's Tiangong space station
When you buy through links on our articles, Future and its syndication partners may earn a commission. Since 1998, when the International Space Station (ISS) launched, there has been a place for astronauts around the world to run experiments in space, from growing food to learning how low-Earth orbit affects the human body. More recently, the Chinese Tiangong Space Station was fully completed, with its third and final module, the Mengtian, added on Oct. 31, 2022. Tiangong sits at the same height as the ISS. The ISS is a joint venture between NASA, Roscosmos, the European Space Agency (ESA), the Japanese Aerospace Exploration Agency (JAXA) and other organizations. It's been continuously inhabited since 2000 and serves as a microgravity laboratory for research in biology, physics, medicine and earth sciences. The ISS is significantly larger than the Tiangong Space Station, as the ISS has 16 modules while Tiangong only has three. As China was excluded from the ISS program, it created its own space station, Tiangong, which shows the nation's prowess in space exploration. Tiangong, which means "Heavenly Palace" in Chinese, was built by the Chinese Manned Space Agency (CMSA) and provides a platform for scientific research for countries not involved in the ISS program. These two photographs were taken from space, about 250 miles (402 km) from Earth. These two photos were taken by a Maxar WorldView Legion satellite from low-Earth orbit. In a tweet, Maxar Technologies discussed how their satellites could capture these images with crisp clarity as both space stations continue to move in their respective orbits. It's difficult to photograph something moving as quickly as the ISS or the Tiangong Space Station. The ISS orbits Earth every 90 minutes at a speed of about 17,500 mph (28,000 km/h) and the Tiangong moves at a similar rate. Being able to capture the detail on both space stations shows the timing and engineering capabilities of the Maxar satellite. You can read more about the ISS, the Tiangong Space Station, and observation satellites as companies like Maxar continue to study Earth from space.
Yahoo
9 hours ago
- Yahoo
Mysterious Leprosy Pathogen Has Lurked in The Americas For 4,000 Years
A new study has found that leprosy was circulating in Chile some 4,000 years ago, meaning the disease arrived in the Americas much earlier than previously thought. That's based on an analysis of ancient bones and teeth by researchers from institutions in Germany, Argentina, and Chile, and it challenges the conventional wisdom that leprosy was a disease introduced by European settlers from the 16th century onwards. Through a comprehensive study of DNA fragments found in two human skeletons, the researchers were able to match the genetic material to the Mycobacterium lepromatosis pathogen – the less common of two bacteria known to cause leprosy. "We were initially suspicious, since leprosy is regarded as a colonial-era disease, but more careful evaluation of the DNA revealed the pathogen to be of the lepromatosis form," says anthropologist Darío Ramirez, from the National University of Córdoba in Argentina. Related: Scientists are still learning about M. lepromatosis, which has only recently been identified. Another bacteria, Mycobacterium leprae, is the dominant strain behind leprosy, and its history and spread has been more clearly mapped to date. While there's a scarcity of samples in the Americas, M. leprae has been tracked back for thousands of years across Eurasia, which is part of the reason why researchers have long thought it traveled from Europe across the Atlantic. Another recent study found traces of M. lepromatosis in remains from Canada and Argentina, stretching back at least a thousand years – again before European settlers showed up. This new find, pushing its arrival back millennia earlier, adds further evidence that we need to rethink the history of leprosy. "Ancient DNA has become a great tool that allows us to dig deeper into diseases that have had a long history in the Americas," says anthropologist Kirsten Bos, from the Max Planck Institute for Evolutionary Anthropology in Germany. "The advanced techniques now used to study ancient pathogen DNA allows us to look beyond the suspects and into other diseases that might not be expected from the context." Trying to pick apart this history of disease isn't easy. Indigenous American peoples would certainly have had afflictions of their own, but they would have also been hit hard by infections imported by colonists – infections their bodies were poorly prepared for. The researchers are confident that there's more to the story, in terms of both modern and ancient forms of the disease – especially in regards to M. lepromatosis. Each archaeological dig and clinical test gives experts more genomes to work with, which then further helps our understanding of disease history, spread, and diversification. Part of the skill needed by researchers is knowing what to look for, which is highlighted by this study – previous work in this area may have missed ancient markers of leprosy, simply because no one thought to look for it. "This disease was present in Chile as early as 4,000 years ago, and now that we know it was there, we can specifically look for it in other contexts," says anthropologist Rodrigo Nores, from the National University of Córdoba. The research has been published in Nature Ecology & Evolution. Massive Review Finds No 'Safe' Level of Processed Meat Consumption Ozempic-Like Drugs Could Treat Chronic Migraines, Trial Finds Gut Bacteria Found to Soak Up Toxic Forever Chemicals
Yahoo
9 hours ago
- Yahoo
Biting the 'Bullet': Amazing new JWST photo shows titanic collision of galaxy clusters
When you buy through links on our articles, Future and its syndication partners may earn a commission. NASA's James Webb Space Telescope (JWST) has produced a new image of the Bullet Cluster, which is a titanic collision between two individual galaxy clusters. The image, produced in conjunction with NASA's Chandra X-ray Observatory, reveals not only the location and mass of dark matter present, but also points the way toward one day figuring out what dark matter is actually made of. In the new image, we see the hot gas within the Bullet Cluster in false-color pink, detected by Chandra. The inferred location of dark matter is represented in blue (also false color), as measured by the JWST. Note that the blue and the pink are separate — what has caused the dark matter and the gas to separate, and how were astronomers able to produce this map of the material within the Bullet Cluster? Located 3.9 billion light-years away, the Bullet Cluster has been an occasionally controversial poster child for dark-matter studies. Back in 2006, the Hubble Space Telescope and the Chandra X-ray Observatory worked together to image the Bullet, showing the presence of its dark matter based on how light from more distant galaxies was being gravitationally lensed by the dark matter's mass. Collisions between galaxy clusters are the perfect laboratories for testing our ideas about dark matter, because they are nature's way of throwing together huge amounts of the stuff. This gives us a chance to test how dark matter particles interact with each other, if at all, and the degree of any interaction would be a huge clue as to the properties of the mysterious dark matter particle. Yet despite the dramatic Hubble and Chandra images, the Bullet Cluster — and, indeed, other galaxy cluster collisions — haven't always played ball. For instance, the velocities at which the sub-clusters are colliding seem too high for the standard model of cosmology to explain. Now the JWST has entered into the fray. A team led by Ph.D. student Sangjun Cha of Yonsei University in Seoul, South Korea, and professor of astronomy James Jee at both Yonsei and the University of California, Davis, have used the most powerful space telescope ever built to get a best-ever look at the Bullet Cluster. Hubble and Chandra had previously shown that, as the two individual galaxy clusters in the Bullet Cluster collided, the galaxies and their surrounding dark matter haloes had passed right through each other. This makes sense for the galaxies — the distances between them are so great that the chance of a head-on collision between any two is slim. It also suggests that the degree with which dark matter particles interact with each other — what we refer to as their collisional cross section — is small; otherwise, the interaction would have slowed the clouds of dark matter down, and we would detect it closer to where Chandra sees the hot, X-ray emitting intracluster gas. In contrast to the dark matter, these huge gas clouds can't get out of each other's way, so they slam into each other and don't progress any further. The end result is that the hot gas is found stuck in the middle of the collision, and the galaxies and dark matter belonging to each sub-cluster are found on opposite sides, having glided right through one another. "Our JWST measurements support this," Jee told "The galaxy distribution closely traces the dark matter." JWST was able to produce a better map of the distribution of matter, both ordinary and dark, in the Bullet Cluster by detecting, for the first time, the combined glow from billions of stars that have been thrown out of their galaxies and are now free-floating in the space between the galaxies in each sub-cluster. Cha and Jee's team were then able to use the light from these "intracluster stars" to trace the presence of dark matter and gain a more accurate map of its distribution in the Bullet Cluster. However, this has just raised more mysteries. The more refined map of the dark matter shows that, in the larger sub-cluster, on the left, the dark matter is arranged in an elongated, "hammerhead" shape that, according to Jee, "cannot be easily explained by a single head-on collision." This elongated mass of dark matter is resolved into smaller clumps centered on what we call the brightest cluster galaxies — giant elliptical galaxies that are the brightest galaxies in the sub-cluster located at its gravitational core. In contrast, the dark matter halo around the sub-cluster on the opposite side is smaller and more compact. Cha and Jee's team suspect that the elongated, clumpy mass of dark matter could only have formed when that particular sub-cluster, which was a galaxy cluster in its own right before the Bullet collision, underwent a similar collision and merger with another galaxy cluster billions of years before the formation of the Bullet. "Such an event would have stretched and distorted the dark-matter halo over time, resulting in the elongated morphology that we observe," said Jee. Despite the new discoveries such as this from JWST's more refined observations of the Bullet cluster, it is still not enough to resolve the issue of the collision velocities of the two sub-clusters. "Even with these updates, the required collision velocity remains high relative to expectations from cosmological simulations," said Jee. "The tension persists and remains an active area of research." RELATED STORIES — What is dark matter? — James Webb Space Telescope (JWST) — A complete guide — Astonishing 'halo' of high-energy particles around giant galaxy cluster is a glimpse into the early universe Dark matter makes up over a quarter of all the mass and energy in the universe, and roughly 85% of all matter, so figuring out its secrets, in particular its collisional cross-section and the cause of those high velocities, is going to be essential if we want to better understand this universe in which we live. Alas, the JWST observations of the Bullet Cluster alone are not enough to confirm what the collisional cross-section of dark matter must be. However, they do tighten the estimate of the upper limit for the value of the cross-section, constraining the list of possibilities. Astronomers are already in the process of rigorously measuring as many galaxy cluster collisions as possible, seen from all angles and distances, to try and constrain this value further. Gradually, we'll be able to rule out different models for what dark matter could be, until we're left with just a few. Coupled with experimental data from direct dark matter searches from detectors deep underground, such as the LUX-ZEPLIN experiment at the Sanford Underground Research Facility in South Dakota, we could soon be on the cusp of answering one of science's greatest mysteries: what is dark matter? The JWST observations were reported on June 30 in The Astrophysical Journal Letters.