Showing posts with label astronomers. Show all posts
Showing posts with label astronomers. Show all posts

Webb Telescope's Exoplanet Images Leave Researchers Stunned, NASA Reports

The James Webb Space Telescope Scientists have, for the first time, directly detected the crucial molecule of carbon dioxide in planets beyond our solar system. announced Monday.

According to experts, the gas giants cannot support alien life forms; however, they provide insights into an enduring puzzle concerning the formation of far-off worlds. research published in The Astrophysical Journal .

The HR 8799 star system, located about 130 light-years away from Earth, is merely 30 million years old — quite young when contrasted with our own solar system, which has existed for approximately 4.6 billion years. According to the research findings, a group of scientists based in the U.S., utilizing data from Webb, were able to directly observe carbon dioxide present in the atmospheres of all four recognized planets within this system.

Webb's latest images of two well-known systems, HR 8799 and 51 Eridani and their planets have amazed scientists, providing further insights into the chemical composition of youthful gas giants,” as stated by NASA. statement .

They employed Webb’s coronagraph tools, designed to obstruct light from luminous stars so as to obtain a clearer image of the planets orbiting these stars.

"Imagine holding your thumbnail up against the sun as you gaze into the sky," said lead study author William Balmer, an astrophysicist at Johns Hopkins University, to AFP.

Typically, the Webb telescope identifies exoplanets by observing them as they pass in front of their parent star.

The "transit technique" enabled Webb to indirectly discover CO2 in the atmosphere of the gas giant WASP-39 back in 2022.

However, with this recent finding, "what we’re observing is the actual light emanating from the planet rather than just the signature of that light coming from the host star," explained Balmer.

This isn’t simple—Balmer likened the task to trying to see fireflies with a flashlight next to a lighthouse.

Although these gas giants might not support life themselves, it's conceivable that they could have had moons capable of hosting life, he noted.

Several ongoing missions aim to discover whether life exists within the huge oceans hidden beneath the frozen crusts of multiple Jovian satellites.

"Key piece of proof"

Carbon dioxide (CO2) is crucial for life on our planet, which makes it an important element in the quest to find extraterrestrial life.

Since CO2 turns into tiny ice particles in the extreme chill of space, detecting it can provide insights into how planets form.

According to Balmer, Jupiter and Saturn likely initially formed through a "bottom-up" mechanism where numerous small ice fragments combined to create a solid nucleus. This core subsequently attracted gases to expand into massive planets.

Thus, the recent finding serves as a "crucial piece of evidence" indicating that distant planets may also develop through processes akin to those observed in nearby planetary systems, according to Balmer.

However, how widespread this phenomenon is across the universe remains uncertain.

The aim of this type of research is to gain insight into our solar system, life, and our place within it by comparing them to other exoplanetary systems, thus helping us better understand our position in the universe, Balmer said We aim to capture images of other solar systems and observe their similarities or differences relative to our own. This will help us understand whether our solar system is exceptionally unusual or rather typical among others.

Astronomers have currently identified almost 6,000 exoplanets, most of which are quite large — and so far, none has been found to be inhabitable.

According to Balmer, the "significant advancement we need to achieve" is concentrating our efforts on planets of similar size to Earth.

The NASA Nancy Grace Roman space telescope plans to utilize a coronagraph for this purpose shortly following its anticipated launch in 2027.

The previous year, the Webb telescope discovered carbon dioxide And hydrogen peroxide present on the surface of Charon, which is Pluto's biggest satellite.

Balmer aims to utilize Webb for observing additional four-planet systems, yet he also noted that future funding has become uncertain.

The previous week saw the Trump administration declare that NASA's top scientist had been let go, suggesting that further reductions loom for the American space agency.

Scientists Say Living on the Moon Might Be Easier Than We Thought

It could be simpler for us to explore and reside on the Moon That's more than we initially believed, according to scientists.

According to a recent study, ice might be found beneath the Moon's surface in larger areas of its polar regions than previously thought.

Utilizing that ice and converting it into water will probably play a crucial role in our investigation or potential settlement of the Moon. However, the exact quantity available remains uncertain.

The probability of discovering ice correlates with the surface temperature on the lunar surface.

However, our recordings of the Moon's surface temperatures were conducted during the Apollo missions in the 1970s — which touched down near the equatorial region, quite distant from our planned landing site for future trips to the Moon. Additionally, within these areas of the Moon, the inclination of the terrain has minimal impact on the ambient temperature.

Currently, scientists have utilized data from ChaSTE—a temperature measurement experiment conducted via the Vikram lander aboard India's Chandrayaan-3 mission. This lander reached the southern polar area of the moon in 2023.

They managed to examine both inclined and level sections of the terrain, discovering that areas with inclines facing away from the sun could potentially remain cold enough for frost to form close to the surface. These conditions may occur on the moon—specifically in locations where NASA’s forthcoming manned Artemis missions intend to touch down.

The results are detailed in a recent study titled 'Higher Surface Temperatures Near South Polar Region of the Moon Measured by ChaSTE Experiment on Board Chandrayaan-3,' which has been published in the journal. Communications Earth & Environment .

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Scientists Unveil Tiniest Galaxy Yet Discovered: "A Functional Human Sized Down to a Grain of Rice"

Scientists have identified a group of miniature galaxies situated approximately 3 million light-years distant, which encompasses the tiniest and dimmest galaxy known to date.

This galaxy, named Andromeda XXXV, along with its companions circling around our neighboring galaxy, Andromeda, might alter our perceptions of cosmic evolution.

This is due to dwarf galaxies of such a tiny size typically being obliterated under the hotter and more dense environments. early universe And yet, for some reason, this small galaxy managed to survive without getting destroyed.

Despite their small scale—approximately one-millionth the size of our Milky Way—they function just as well as full-sized galaxies," explained team member and University of Michigan professor Eric Bell in a press release. "Imagine a person with all the capabilities intact, yet shrunk down to the size of a single grain of rice.

Meet Andromeda XXXV

Dwarf galaxies are not unfamiliar to scientists. Our home galaxy, the Milky Way , is orbited by many of these satellite galaxies trapped within the grasp of its larger galactic neighbors.

Nevertheless, many aspects of dwarf galaxies remain mysteries to scientists. Due to their smaller size, these galaxies emit less light compared to larger ones, which makes them more difficult to observe and investigate from far away.

Although astronomers have managed to pinpoint numerous dwarf galaxies revolving around the Milky Way, detecting similar small galaxies circling our luminous neighboring galaxies has proven extremely challenging. Thus, the small galaxies of the Milky Way Have served as our sole source of knowledge regarding tiny galactic entities.

This assignment is relatively easier when concerning the nearest large galaxy to the Milky Way, which is Andromeda. Dwarf galaxies have been observed near Andromeda. Previously, they were big and noticeable, merely reinforcing the data that astronomers had collected regarding dwarf galaxies orbiting the Milky Way.

To uncover these groundbreaking smaller and fainter dwarf galaxies, lead researcher Marcos Arias, an astronomer from the University of Michigan, along with his collaborators examined extensive astronomical databases. They were also granted observing time with major telescopes. Hubble Telescope to aid their search.

This discovery showed that Andromeda XXXV is not just a satellite galaxy, but its size is also significant enough to alter our understanding of galactic evolution theories.

I found this quite astonishing," Bell stated. "Given that it’s the dimmest object detected in the area, it presents an intriguing setup. However, multiple aspects about it were unforeseen.

A cosmic murder mystery

A crucial element of galactic evolution revolves around the duration of their star-forming periods This appeared to be the primary distinction between the Milky Way's dwarf galaxies and the less massive satellite galaxies orbiting Andromeda.

Arias noted that most of the Milky Way’s satellite galaxies possess extremely old stellar communities, ceasing star formation roughly 10 billion years back. In contrast, she pointed out that some analogous satellites orbiting Andromeda were still producing stars until approximately 6 billion years ago,

Stellar creation depends on a continuous supply of gas and dust to collapse and form new stars. Once this fuel runs out, star formation stops, effectively causing the galaxy to “die.”

Therefore, Bell characterized the circumstances surrounding these tiny galaxies as a "cold case" puzzle. Was star formation halted within the dwarf galaxies? gas supplies petered out On their own, or when these gases were stripped away by gravitational forces from a massive galactic host?

For the Milky Way, it seems that the supply of gas needed for star formation naturally dwindled over time. In contrast, for the smaller galaxies surrounding Andromeda, it looks like they were essentially “destroyed” by their larger host galaxy.

The lighting is somewhat dim, but it seems these galaxies either fell or were shoved out of place. It appears they were pushed," Bell stated. "This has taught us something fundamentally new regarding how galaxies form.

What is particularly intriguing is the prolonged duration of star formation observed in Andromeda XXXV. To grasp this phenomenon, we must look back to the era when the very first galaxies were formed.

Why doesn’t Andromeda XXXV qualify as a ‘deep-fried’ galaxy?

The initial era of the cosmos was characterized by extremely high temperatures and densities. This inflationary era was initiated by the Big Bang Continuing on, as the universe expanded and cooled, the initial atoms of hydrogen formed, leading to the creation of the first stars that clustered together. first galaxies.

These stars and galaxies emitted energy just like the earliest feeding black holes, which also helped reheat the universe. This event marked the demise of tiny galaxies, with experts suggesting that this heat essentially boiled away the gas required for star formation within these stellar clusters.

Nevertheless, against all odds, Andromeda XXXV endured!

Bell stated, "Initially we believed everything would essentially turn into ash since the whole cosmos transformed into a cauldron of searing hot liquid, resembling boiling oil. We anticipated that it would entirely exhaust its supply of gas; however, that seems not to be the case. This entity has an estimated mass of around 20,000 times that of our sun and continued to form stars without issue for several additional billions of years."

Exactly why Andromeda XXXV managed to avoid being destroyed remains an enigma.

“I don’t have a solution,” Bell stated. “The fact remains that the universe did experience warming; however, we’re now realizing the outcomes are far more complex than previously understood.”

NASA Other agencies are preparing missions that might uncover additional dwarf galaxies orbiting larger galaxies, which could shed light on this enigma. However, it’s likely that these discoveries may raise new queries similar to how the finding of Andromeda XXXV did.

Arias noted, 'We still have much to uncover.' There are numerous aspects we must continue to study — particularly concerning our immediate surroundings when it comes to galactic development, transformation, and organization — before we can deconstruct the chronology of the universe’s past and grasp how we arrived at this point.'

The team's study was released on Tuesday (March 11) in The Astrophysical Journal Letters.

The "Moon Illusion" Has Stumped Scientists for Millennia: Unraveling the Mystery

It's an illusion That has puzzled individuals from the realms of philosophy and science across millennia—but what is the reason behind this? Moon appear bigger when it rises or sets?

Queries about the visual illusion of the moon seeming bigger when it's close to the horizon can be traced back as far as the 4th century BCE.

That's right, even Aristotle He rubbed his chin as he contemplated the cause of this phenomenon. His conclusion was that the Earth’s atmosphere might have some sort of magnification effect that distorts how we perceive the moon.

At the point where the horizon meets the sky, the place where the moon illusion becomes evident, the philosopher surmised that light must travel through a thicker layer of the Earth’s thick atmosphere. This passage acts akin to a magnifying lens, amplifying what we perceive.

According to this theory, Aristotle grasped how the moon illusion deceives the human eye instead of attributing it to the moon or outer space—although not all of his ideas were equally perceptive.

It’s an optical illusion for humans since even though photographs taken of the moon show consistent dimensions every night, our perception makes it seem as if its size changes in the evening sky.

Therefore, we have all acknowledged that this phenomenon is due to an optical illusion, with modern explanations attributing it to our brain’s inability to accurately gauge the Moon’s actual size and distance.

Nonetheless, there isn't a definitive explanation for this phenomenon; one potential cause might be the influence of our environment on how we perceive things — such as trees, mountains, and structures that lead us to believe the moon appears bigger and nearer when it's near the horizon.

When the moon sits high in the sky without anything nearby for scale, it can seem more distant and diminutive.

Does that sound familiar? It should, as the Ponzo illusion works similarly. The pair of converging lines alters how we perceive two lines of identical length.

Even though we might believe the top line appears bigger and more distant, this is incorrect; in reality, both lines are identical in size.

If unsure, we can check with NASA regarding this lunar optical effect.

"Without a full understanding of why we perceive it this way, we can still concur that whether real or an illusion, a large Moon remains a breathtaking spectacle," according to the space agency. IFL Science.

So, until we figure out precisely what our minds are doing, it’s likely for the best to simply appreciate the Moon illusion and the moody, atmospheric, and occasionally eerie scenes it generates.

Consider this the next time you look up at the moon...

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Scientists discover smallest galaxy ever seen: 'It's like having a perfectly functional human being that's the size of a grain of rice'

Astronomers have discovered a collection of tiny galaxies located roughly 3 million light-years away that includes the smallest and faintest galaxy ever seen.

This galaxy, designated Andromeda XXXV, and its compatriots orbiting our neighbor galaxy, Andromeda, could change how we think about cosmic evolution.

That's because dwarf galaxies this small should have been destroyed in the hotter and denser conditions of the early universe . Yet somehow, this tiny galaxy survived without being fried.

"These are fully functional galaxies, but they're about a millionth of the size of the Milky Way," team member and University of Michigan professor Eric Bell said in a statement. "It's like having a perfectly functional human being that's the size of a grain of rice."

Meet Andromeda XXXV

Dwarf galaxies themselves are nothing new to scientists. Our own galaxy, the Milky Way , is orbited by dozens of these satellite galaxies caught in the grip of its more immense galaxies.

There is, however, a great deal about dwarf galaxies that scientists don't know. This is because, being smaller, they are much dimmer than major galaxies, making them harder to spot and tougher to study at large distances.

While astronomers have been able to determine many dwarf galaxies in orbit around the Milky Way, identifying dwarf galaxies around our bright galactic neighbors has been incredibly difficult. This means that the dwarf galaxies of the Milky Way have been our only source of information about small satellite galaxies.

This task is somewhat less challenging around the closest major galaxy to the Milky Way, Andromeda. Other dwarf galaxies have been spotted around Andromeda before, but these have been large and bright, thus simply confirming the information that astronomers had gathered about dwarf galaxies around the Milky Way.

To discover these paradigm-shifting smaller and dimmer dwarf galaxies, team leader Marcos Arias, an astronomer at the University of Michigan, and his colleagues scoured various massive astronomical datasets. The team was also able to obtain time with the Hubble DiwidaTelescope to aid their search.

This revealed that not only is Andromeda XXXV a satellite galaxy, but it is also small enough to change theories of how galaxies evolve.

"It was really surprising," Bell said. "It's the faintest thing you find around, so it's just kind of a neat system. But it's also unexpected in a lot of different ways."

A cosmic murder mystery

One of the key aspects of galactic evolution is how long their star-forming periods last. This seemed to be the main difference between the Milky Way's dwarf galaxies and the smaller satellite galaxies of Andromeda.

"Most of the Milky Way satellites have very ancient star populations. They stopped forming stars about 10 billion years ago," Arias explained. "What we're seeing is that similar satellites in Andromeda can form stars up to a few billion years ago — around 6 billion years."

Star formation requires a steady supply of gas and dust to collapse and birth stellar bodies. When that gas is gone, star formation halts, and the galaxy "dies."

Thus, Bell described the situation around these small galaxies as a "murder mystery." Did star formation end when dwarf galaxies' gas supplies petered out on their own, or when these gases were gravitationally stripped away by a large galactic host?

In the case of the Milky Way, it appears that the gas for star formation petered out on its own; however, for the smaller galaxies around Andromeda, it appears they were "killed" by their parent galaxy.

"It's a little dark, but it's either did they fall or did they get pushed? These galaxies appear to have been pushed," Bell said. "With that, we've learned something qualitatively new about galaxy formation from them."

What is even more curious is the extended period of star formation experienced by Andromeda XXXV. To understand why, it is necessary to travel back in time to the the birth of the first galaxies.

Why isn't Andromeda XXXV a 'deep fried' galaxy?

The earliest epoch of the universe was marked by incredibly hot and dense conditions. This inflationary period, begun by the Big Bang , continued, and the universe dispersed and cooled. This allowed the first atoms of hydrogen to take shape, birthing the first stars, which gathered in the first galaxies.

These stars and galaxies blasted out energy as did the first feeding black holes reheating the cosmos. This signaled the death of very small galaxies, and scientists theorize this heat "cooked off" the gas needed for star formation in such collections of stars.

Yet, somehow, Andromeda XXXV survived!

"We thought they were basically all going to be fried because the entire universe turned into a vat of boiling oil," Bell said. "We thought that it would completely lose its gas, but apparently that doesn't happen, because this thing is about 20,000 solar masses and yet it was forming stars just fine for a few extra billion years."

Exactly why Andromeda XXXV managed to avoid being destroyed remains an enigma.

"I don't have an answer," Bell said. "It is also still true that the universe did heat up; we're just learning the consequences are more complicated than we thought."

NASA and other Diwidaagencies are planning missions that could discover further dwarf galaxies around other large galaxies and help solve this mystery. But there's a good chance that the solution will open up new questions just as the discovery of Andromeda XXXV has.

"We still have a lot to discover," Arias said. "There are so many things that we still need to learn — even about what's near to us — in terms of galaxy formation, evolution, and structure before we can reverse engineer the history of the universe and understand how we came to be where we are today."

The team's research was published on Tuesday (March 11) in The Astrophysical Journal Letters.

Mystery Radio Signals Emanate From Uncharted Space Region, Baffling Scientists

For a decade, Earth has been on the receiving end of enigmatic occurrences. radio emissions every two hours.

Following over ten years, the origin of these signals has at last been pinpointed near the constellation of the Big Dipper.

A study published in Nature Astronomy reveals a close pair of stars—a red dwarf and a white dwarf—that orbit each other so closely that their magnetic fields interact with each other every two hours, producing detectable radio emissions during these collisions.

The finding is unexpected for researchers, who until now had solely been able to link radio bursts to neutron stars.

Doctor Iris de Ruiter, who headed the research, said 'We collaborated with specialists from various fields within astronomy.'

'Using various methods and insights, we gradually moved nearer to solving the problem.'

Researchers have managed to capture a particular type of radio signal from a galaxy that’s approximately 9 billion light-years from our planet.

The signal did not originate from aliens; instead, it came from a star-forming galaxy known as 'SDSSJ0826+5630', which existed when the universe was approximately 4.9 billion years old.

The uniqueness of this radio signal lies in its specific wavelength, referred to as the '21 cm line'.

'It's like looking back in time for 8.8 billion years,' explained Arnab Chakraborty, a cosmologist and co-author of the study on this discovery.

This kind of radio signal had never before been observed at such an immense distance.

In 2022, comparable radio signals guided scientists to the detection of a neutron star. a star differing from any discovered before.

Unusual pulses lasting approximately 300 milliseconds each were observed by Manisha Caleb, who is a lecturer at the University of Sydney.

'The flash exhibited traits similar to those of a radio-emitting neutron star. However, this was unlike anything we had encountered previously,' she said. said .

A neutron star represents the condensed remnants of a large supergiant star. Aside from a black hole, they stand as the most compact and dense celestial bodies identified by humans.

When they are particularly dense, these objects can be referred to as pulsars – and frequently are. release pulses of radio waves that we can detect on Earth.

It was discovered that the neutron star emitted pulses never observed before.

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