Astronomers Monitor Interstellar Comet 3I/Atlas

3i/Atlas is only the third celestial object ever detected, following the interstellar asteroid 1i/Oumuamua in 2017 and the interstellar comet 2i/Borisov in 2019.



Images of 3i/Atlas captured by the Atlas telescope. Image credit: University of Hawaii.

The 3i/Atlas is currently about 670 million km (420 million miles) from the Sun and is expected to make its closest approach in October 2025, moving just within Mars’ orbit.

It is estimated to be up to 20 km (12 miles) in diameter, traveling at around 60 km (37 miles) per second relative to the Sun.

This comet poses no threat to Earth, remaining within a distance of 240 million km (150 million miles), which is more than 1.5 times the distance between the Earth and the Sun.

3i/Atlas is an active comet. As it approaches the Sun, the heat causes frozen gases to turn into vapor, releasing dust and ice particles into space and initiating the formation of a glowing coma and tail.

However, by the time it reaches its closest point to Earth, it will be obscured by the Sun. It is expected to be visible again by early December 2025, providing astronomers with an opportunity for further research.

“Finding possible interstellar objects is extremely rare, and it’s thrilling to see the Atlas telescope catch this asteroid,” said a representative.

“These interstellar visitors allow us to glimpse something intriguing from solar systems beyond our own.”

“3i/Atlas is the largest ever observed, yet numerous such objects traverse our inner solar system each year.”

“The likelihood of an impact with Earth is minimal, occurring less than once in 10 million years, but Atlas is consistently scanning the sky for potentially hazardous objects.”

https://www.youtube.com/watch?v=4d-nqd1uwvy

Astronomers across Hawaii, Chile, and other nations are tracking the comet’s progression.

They seek to learn more about the composition and behavior of this interstellar visitor.

“It is precisely their foreign nature that makes interstellar objects like 3i/Atlas so remarkable,” an ESA astronomer stated.

“While all planets, moons, asteroids, comets, and life forms in our solar system share a common origin, our interstellar visitors are genuine outsiders.”

“They are remnants from other planetary systems, providing clues about the formation of worlds beyond our own.”

“It may take thousands of years before humans visit planets in another solar system, and interstellar comets give us the chance to stimulate our curiosity as we interact with something from another world.”

“These icy nomads offer a rare, tangible link to the broader galaxy. This material is fundamentally different from our own and is formed in unique environments.”

“Visiting such objects connects humanity with the universe on a grander scale.”

Source: www.sci.news

Astronomers Uncover Third Interstellar Object: 3I/ATLAS

Following the interstellar asteroid 1i/Oumuamua and comet 2i/Borisov, 3i/Atlas is the third identified object and the second comet from outside the solar system.



This image was captured on July 2, 2025, with an Itemescope.net T72 telescope in Riojartad, Chile, depicting the interstellar comet 3i/Atlas. Image credit: Filipp Romanov/CC by-sa 4.0.

3i/Atlas was discovered by a NASA-funded research telescope dedicated to the Atlas (Asteroid Surface Impact Last Altar System) project on July 1, 2025, in Riojartad, Chile.

The interstellar comet approached from the direction of constellations and is currently about 670 million km (420 million miles) away.

“Since the initial report, pre-discovery observations have been gathered from archives of three different Atlas telescopes globally and from Zwicky’s transitional facility at Palomar Observatory in San Diego County, California,” a NASA astronomer wrote in a statement.

“These pre-discovery observations date back to June 14th, 2025.”

Known as 3I/ATLAS, C/2025 N1 (ATLAS), and A11PL3Z, it currently measures approximately 4.5 AU (670 million km, or 416 million miles) away.

Comets pose no threat to Earth, maintaining a safe distance of at least 1.6 AU (240 million km, or 150 million miles).

It is predicted to reach its closest approach to the Sun around October 30th, 2025, at a distance of 1.4 AU (210 million km, or 130 million miles).

Its size and physical characteristics are being studied by astronomers worldwide.



This diagram illustrates the trajectory of 3i/Atlas as it traverses the solar system. Image credit: NASA/JPL-Caltech.

If the brightness of 3i/Atlas is attributed to reflecting sunlight at a typical albedo of 10%, its diameter would be approximately 100-200 times greater than the estimated length of 20 km for Oumuamua and about 50-100 times larger than the estimated size of Borisov.

“If all three objects are indeed rocky, the mass of 3i/Atlas is more than 10 million times greater than that of Oumuamua and at least 100,000 times the core mass of Borisov.”

“This is remarkable because we expect high-mass objects to be exceedingly rare.”

“Based on data from the major asteroid belts of the solar system, we would expect millions of objects like Oumuamua for each object with the mass of 3i/Atlas.”

3i/Atlas should remain visible to ground telescopes until September 2025.

It is anticipated to reappear on the opposite side of the Sun by early December, enabling further observations.

“Based on its trajectory, 3i/Atlas seems to enter in a retrograde orbit, inclined at 175 degrees relative to Earth’s orbital plane from the thin disc of stars in the Milky Way,” explains Professor Roeb.

“In the upcoming months, we will gain further insights into the properties of 3i/Atlas based on data from various ground-based telescopes and the NASA/ESA/CSA James Webb Space Telescope, including the NSF/DOE Vera C. Rubin Observatory in Chile.”

Source: www.sci.news

Interstellar Comets Become Only the Third Known Visitors Beyond Our Solar System

Astronomers are laying out welcome mats for newly discovered visitors making their way through our solar system.

This particular object is categorized as a comet and marks only the third confirmed interstellar visitor in recorded history to traverse our cosmic neighborhood.

The comet, named 3i/Atlas, poses no threat to Earth, maintaining a distance of about 150 million miles while it accelerates. As reported by NASA.

This interstellar comet was initially discovered on Tuesday by The final alert system for the asteroid’s terrestrial impact (Atlas) located in Rio Hartado, Chile. The research telescope, funded by NASA, is actually two telescopes from Hawaii and one in Chile, in addition to a fourth in South Africa, all dedicated to scanning the sky multiple times nightly for asteroids that could threaten Earth.

Researchers examined archived data from three different Atlas telescopes and Zwick temporary facilities at the Palomar Observatory in California, uncovering observations that would corroborate the findings. Other telescopes worldwide have also joined the initiative, as stated by NASA.

“ESA’s planetary defenders are currently monitoring an object provisionally known as #A11PL3Z, utilizing telescopes from around the globe,” the European Space Agency announced in a post on X this Wednesday.

Interstellar Comet 3i/Atlas.
David Rankin/Saguaro Observatory

The comet is located around 420 million miles away and is rapidly traveling from the direction of the constellation Sagittarius. NASA commented in a blog post regarding the findings. Sagittarius is a prominent constellation in the Southern Hemisphere and indicates the center of the Milky Way galaxy.

The agency noted that 3i/Atlas will make its closest approach to the sun around October 30th, passing roughly 130 million miles away, close to Mars’ orbit.

NASA indicated that the comet will remain observable from ground-based observatories until September, providing scientists with the opportunity to gather additional details about these cosmic visitors, including their size. After September, 3i/Atlas will be too close to the sun for telescopes to observe, but it is expected to become visible again in early December, as it reemerges on the far side of the sun.

The upcoming months will present a rare chance to study these celestial tourists traveling through the solar system. The first confirmed interstellar object, observed in 2017 by the University of Hawaii’s Pan-Starrs1 telescope, was the rocky body named “Oumuamua” (Hawaiian for first visitor), notable for its reddish hue and elongated cigar-like shape. As noted by NASA.

The only other known interstellar visitor is 2i/Borisov, a comet discovered in 2019 by amateur astronomer Gennady Borisov.

Source: www.nbcnews.com

A11PL3Z: The Interstellar Comet 3i/Atlas Traversing Our Solar System

Comet 3i/Atlas is the third interstellar object detected in the solar system

E. Guido, M. Rocchetto, J. Ferguson

Interstellar objects have been observed speeding through the solar system, prompting both amateur and professional astronomers globally to direct their telescopes toward them, refining their orbital models to confirm their status as visitors from other stars.

The comet was initially designated A11PL3Z and marks the third documented interstellar object. The first, ‘Oumuamua, was identified in October 2017, shortly after its closest approach to Earth. Its bizarre acceleration sparked numerous theories, including the possibility that it might be an alien spacecraft. The second interstellar object, Comet Borisov, was discovered in 2019, allowing for more extensive observations early in its journey through the solar system.

The A11PL3Z was first detected by NASA’s Asteroid Terrestrial Impact Last Alert System (ATLAS). Earlier images of the object, once overlooked, were identified in data collected on June 14. New observations are underway in Chile and beyond through the Deep Random Survey. The Minor Planet Center—charged with the observation and reporting of such entities—has now officially named it 3I/ATLAS, acknowledging both its classification as the third interstellar object and the discoverers.

The object measures approximately 20 km wide and is estimated to move at around 60 km per second, gradually accelerating due to the sun’s gravitational pull. By October, it will reach its closest point to the Sun, passing within two astronomical units (twice the distance from Earth to the Sun) before swinging away and exiting our solar system.

The anticipated trajectory of 3i/Atlas marks its position as only the third interstellar object to be recorded in the solar system

CSS, D. Rankin

This creates a limited window for studying 3i/Atlas, although its visibility offers more time for observation compared to other interstellar entities. “They move through the solar system at astonishing speeds,” states Mark Norris from the University of Central Lancashire, UK. “It’s a race against time to learn as much as we can about them.”

Unfortunately, the technology needed to launch missions to intercept and investigate these celestial visitors remains out of reach, according to Norris. “Even if we started today, it would be too late,” he concludes. However, this may evolve soon, as the European Space Agency (ESA) aims to deploy a comet interceptor mission into space in 2029, where it will await encounters with newly discovered comets and interstellar bodies.

For now, astronomers must depend on existing telescopes to observe 3i/Atlas from a distance. “As we can track it until the end of the year, we have sufficient time to refine its trajectory, and there’s still time to focus the spectrometer on it,” mentions Richard Moisle. Our team is already eager to pinpoint the earliest possible observations. Everyone is highly enthusiastic and ready for what’s ahead.”

World Capital of Astronomy: Chile

Explore the breathtaking astronomical sites in Chile. Visit advanced observatories and marvel at the breathtaking clear night skies.

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New Horizons Images Enable First Test of Interstellar Navigation

Illustration of NASA’s New Horizons spacecraft navigating the outer solar system.

Joe Olmsted/STScI

After departing from our solar system, NASA’s New Horizons spacecraft finds itself considerably distant from Earth, causing the stars of the Milky Way to appear in notably different positions compared to our terrestrial views. Astronomers are harnessing this altered perspective to determine the location of galaxy probes, marking the first instance of intergalactic navigation.

Launched in 2006, New Horizons initially observed Pluto before continuing beyond, traversing the Kuiper Belt—an immensely expansive region of rocky debris and dust billions of miles from the Sun. Currently, the spacecraft is hurtling through space at tens of thousands of kilometers per hour.

When gazing at the night sky from Earth, stars seem widely spread apart, so unless equipped with a strong telescope, their positions appear constant from various locations. In contrast, the New Horizons perspective reveals a significant shift in star positions due to the parallax effect. This phenomenon was demonstrated in 2020 when the probe captured images of two nearby stars, Proxima Centauri and Wolf 359.

Now, Todd Lauer from the U.S. National Institute of Light Change Astronomy in Arizona and his team have utilized this effect to gain a new perspective. They accomplished this by comparing images of Proxima Centauri and Wolf 359 taken by the probe with measurements from the Gaia Space Telescope.

“There’s a three-dimensional map of the galaxies around us, allowing you to see your position,” says Lauer. “Using your own camera on a spacecraft offers incredible accuracy.”

To determine the spacecraft’s location, Lauer and his team analyzed the star positions detected by the New Horizons camera, tracing their lines back to the closest intersection point. They then referenced the precise locations of both stars from the Gaia star map to ascertain this point’s relation to the solar system.

This two-frame animation illustrates the changing position of Proxima Centauri as observed from Earth and New Horizons.

Nearly every spacecraft utilizes NASA’s Deep Space Network (DSN) to determine its position within a margin of tens of meters through a network of radio transmitters on Earth. In contrast, the parallax method provides a less precise estimation, determining New Horizons’ location within a 6,000-kilometer sphere, roughly half the distance from Earth to the Sun.

“We don’t aim to replace the Deep Space Network; this is merely a proof-of-concept demonstration,” Lauer notes. Yet, advancements in cameras and equipment could enhance accuracy by up to 100 times.

Employing this technique for interstellar navigation could yield superior location accuracy compared to the DSN. This not only facilitates the spacecraft’s journey further from Earth but also provides more reliable location tracking, enabling autonomous operations without relying on radio signals from the solar system. Massimiliano Vasile from Strathclyde University in the UK emphasizes this potential.

“When we venture to real stars, we’re talking about light-years,” Vasile explains. “The signal from the Deep Space Network must traverse all the way there, moving at light speed, taking years to reach its destination.”

However, Vasile points out that no agency currently has a mission aimed at deeper exploration of interstellar space, limiting the immediate utility of this technique.

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Source: www.newscientist.com

A11PL3Z: Interstellar Travelers Discovered Racing Through the Solar System

SEI 257609617

The predicted trajectory of A11PL3Z marks it as the third interstellar object observed in the solar system

CSS, D. Rankin

Potential interstellar bodies are now observed zipping through our solar system, and both amateur and professional astronomers globally are racing to direct telescopes towards these phenomena, refine their trajectory models, and ultimately validate their status as visitors from another star.

The object provisionally named A11PL3Z represents the third interstellar entity detected to date. The asteroid ‘Oumuamua was first seen in October 2017, just three days after it passed closest to Earth, and its unusual acceleration sparked a variety of hypotheses, including the possibility of it being an alien spacecraft. The second identified object, Comet Borisov, was observed in 2019, allowing for closer examination given its early passage through the solar system.

A11PL3Z was first identified by the Deep Random Survey in Chile, a group of amateur astronomers. However, a review of earlier observations by other teams revealed that it was initially spotted on June 14 by NASA’s Asteroid Terrestrial-impact Last Alert System (ATLAS). It is estimated to measure approximately 20 km in width and is currently traveling at around 66 km/s, accelerating as it gets pulled in by solar gravity. In October, it will reach its closest point to the Sun, passing within two astronomical units (the Earth is twice the distance from the Sun) before swinging away and exiting the solar system.

This provides a limited window for studying A11PL3Z, though it’s more than that available for previous interstellar objects, which were seen hurtling towards the solar system. “These objects move through the solar system at incredible speeds,” remarks Mark Norris from the University of Central Lancashire. “They are quite transient, which restricts our ability to learn about them.”

Sadly, the prospect of sending missions to intercept and study A11PL3Z is beyond the reach of current technology, notes Norris. “If we were to launch a mission today, it would be too late,” he states. However, the European Space Agency (ESA) is planning a comet interceptor mission set for launch in 2029, which would remain in space to await the arrival of newly discovered comets and possibly interstellar objects.

For the time being, astronomers are relying on existing telescopes to observe A11PL3Z from a distance. “We anticipate we will be observing it by the end of the year, giving us ample time to prepare our spectrometers once we finalize the trajectory,” shares Richard Moisle. When will our observers discern its visibility? There’s a palpable excitement as everyone is prepared and looking forward to this opportunity.

At the time of this writing, over 100 observations of A11PL3Z have already been logged, and the Minor Planet Center—the official body responsible for monitoring and reporting such celestial entities—is expected to confirm its interstellar classification later today.

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Source: www.newscientist.com

Our Solar System passed through a frigid interstellar cloud approximately 2 million years ago, new research reveals.

A cold, dense cloud in the Milky Way’s interstellar medium is about four to five orders of magnitude denser than its diffuse counterparts, and a team of astronomers from Boston University, Harvard University, and Johns Hopkins University has found evidence that two to three million years ago, our solar system encountered one of these dense clouds, which may have been so dense that it disrupted the solar wind.



Offers othersThe interstellar material through which the Sun has traveled over the past few million years indicates the presence of cold, dense clouds that could have had dramatic effects on the heliosphere. Image credit: NASA/JPL-Caltech.

Most stars generate winds that move through the surrounding interstellar medium.

This motion creates a cocoon that protects the planet from interstellar material. The Sun’s cocoon is the heliosphere.

It’s made up of a constant stream of charged particles called the solar wind, which extends far beyond Pluto, enveloping the planet in what astronomers call a “local bubble.”

It protects us from radiation and galactic rays that can alter DNA, and scientists think it’s part of the reason why life on Earth evolved.

A cold interstellar cloud compressed the heliosphere, temporarily placing Earth and other planets in the solar system outside of its influence, according to a new study.

“Our paper is the first to quantitatively show that there was an encounter between the Sun and something outside our solar system that affected Earth’s climate,” said Professor Merab Auffar of Boston University.

“Stars move, and this paper shows that not only do they move, but they undergo dramatic changes.”

To study this phenomenon, Professor Orpher and his colleagues essentially went back in time and used advanced computer models to visualize where the Sun was located two million years ago, along with the heliosphere and the rest of the solar system.

They also mapped the path of a “localized cold cloud ribbon” system, a series of large, dense and very cold clouds made mainly of hydrogen atoms.

Their simulations showed that one of the clouds near the edge of the ribbon, a “local cold cloud,” may have collided with the heliosphere.

If this had happened, Earth would have been fully exposed to interstellar matter, where gases and dust would have mixed with atomic elements left over from the exploded star, such as iron and plutonium.

Normally, the heliosphere filters out most of these radioactive particles, but without protection they could easily reach Earth.

This is consistent with geological evidence showing increased levels of the isotopes iron-60 and plutonium-244 in the oceans, the moon, Antarctic snow and ice cores from the same period, according to the paper.

This timing also coincides with temperature records indicating a cold period.

“It is rare for our cosmic neighbors outside our solar system to have an impact on life on Earth,” said Harvard University professor Avi Loeb.

“It’s exciting to discover that our passage through dense clouds millions of years ago may have exposed the Earth to much greater amounts of cosmic rays and atomic hydrogen.”

“Our findings open a new window into the evolution of life on Earth and its relationship with our cosmic neighbours.”

“External pressure from localized lynxes of cold clouds could have continuously blocked the heliosphere for hundreds to millions of years, depending on the size of the cloud.”

“But as soon as Earth left the cold cloud, the heliosphere engulfed all the planets, including Earth.”

“It’s impossible to know exactly what effect the cold clouds had on the Earth, such as whether they caused ice ages.”

“But there are other cool clouds in the interstellar medium that the Sun likely encountered in its first few billion years.”

“And we’ll probably encounter many more over the next million years or so.”

The authors are currently working to determine where the Sun was 7 million years ago, and beyond.

Pinpointing the position of the Sun and cold cloud systems millions of years ago is made possible by data collected by ESA’s Gaia mission, which has produced the largest 3D map of the galaxy ever, showing in unprecedented detail how fast stars move.

“This cloud is certainly from our past, and if we passed through something this massive, we would have been exposed to interstellar material,” Prof Auffar said.

“This is just the beginning. We hope this paper opens the door to further exploration of how the solar system was influenced by outside forces in the ancient past, and how these forces may have shaped life on Earth.”

of paper Published in today’s journal Natural Astronomy.

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M. Offer othersIt is possible that Earth was directly exposed to cold, dense interstellar material 2 to 3 million years ago. Nat AstronPublished online June 10, 2024; doi: 10.1038/s41550-024-02279-8

Source: www.sci.news

Three million years ago, a cosmic cloud left Earth exposed to interstellar space

Illustration of a protection bubble around the sun (yellow dot) and the earth (blue dot)

Harvard Radcliffe Institute

Two to three million years ago, the solar system encountered galactic-scale turbulence and collided with dense interstellar clouds, potentially altering both the Earth's climate and evolution.

Only recently have researchers been able to map the Sun's orbit through the Galaxy, particularly in relation to the relatively dense hydrogen clouds that pass through the interstellar medium, the vast expanse of space between star systems.

the current, Merab Offer A research team from Boston University in Massachusetts has found evidence that one of these clouds, a “local cold cloud ribbon” in Lynx, likely intersects with the Sun's heliosphere.

The heliosphere is a protective cocoon or bubble formed by the solar wind pushing out to the edge of the solar system. Within the heliosphere, the planet is protected from the worst gamma radiation in the galaxy.

The new study proposes that as the solar system passed through the interstellar cloud, the heliosphere retreated from it and moved inward toward the Sun. The researchers think that the heliosphere may have shrunk so much that Earth was outside the protective cocoon provided by the solar wind, perhaps for around 10,000 years.

Merab and his colleagues used the European Space Agency's Gaia satellite to map the location of the dense, cold clouds and the sun's past orbit.

Ofer says the heliosphere's encounter with the cold cloud coincides with deposits of the elements plutonium-244 and radioactive iron-60 in Antarctic ice, deep-sea cores and lunar samples. These elements, which originated from distant supernovae, would have been captured in interstellar clouds and deposited while Earth was outside the heliosphere.

“There are signs of an increase in these elements over the past two years. [million] “The solar cloud record going back 3 million years provides compelling evidence that the Sun did in fact pass through it around 2 million years ago,” Offer says. “The exposure of Earth to a cloud of cold interstellar material and the associated increase in atmospheric hydrogen and radiation almost certainly had a major impact on Earth and its climate.”

Sarah Spitzer The University of Michigan researcher says the paper provides “compelling” evidence that the heliosphere was exposed to a much denser interstellar cloud two to three million years ago. As the solar system passed through that dense, cold cloud, Earth would have been outside the heliosphere and directly exposed to the interstellar environment, she says.

“Understanding this can teach us about the impact interstellar material has had on life on Earth in the past,” Spitzer says, “but it also helps us better understand the impact the heliosphere has on life on Earth today, what would happen if Earth were exposed to interstellar material again in the future, and when that might happen.”

Evan Economo Researchers from Japan's Okinawa Institute of Science and Technology say it's intriguing to consider how encounters in “our nearby space” could have influenced the environment experienced by life on Earth.

“The heliosphere is part of the extended environment experienced by life on the Earth's surface, influencing climate and radiation from space,” he says. “If we had been outside the heliosphere for a period of time, it could have altered the evolutionary trajectory of a wide range of life, including humans. Such connections are highly speculative at this point, but they provide us with new research directions.”

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Source: www.newscientist.com

NASA’s revolutionary new mission using solar sails may pave the way for interstellar travel

Humanity has always dreamed of traveling beyond our solar system to the stars, but the vastness of the universe has kept us grounded. Our closest star, Proxima Centauri, is a staggering 4.24 light years away, which is too far for us to wait patiently.

Recently, on April 23, NASA launched the Advanced Composite Solar Sail System from New Zealand, a system that uses lightweight sails to propel spacecraft instead of traditional rockets. This development has excited both experts and science fiction fans, as it opens up possibilities for long-distance space travel.


How solar sail works

Instead of using thrusters and fuel like traditional spacecraft, solar sail systems use reflective sails to absorb momentum from photons emitted by the sun. This technology enables spacecraft to gain acceleration without the limitations of fuel. In space, where there is no air resistance, a slight push from the sun is all that’s needed for propulsion.

Solar sails operate similar to sailing ships, utilizing the momentum of photons for movement. By harnessing the sun’s energy, spacecraft can travel far distances at manageable speeds.

How fast can an interstellar probe travel with a solar sail?

The speed of a solar sail system depends on factors like the size of the sail, spacecraft mass, and distance from the sun. With creative maneuvers like slingshot maneuvers and potential laser boosts, spacecraft using solar sails can achieve speeds close to 20% of the speed of light.

Future solar sail systems could reach speeds up to 20 percent of the speed of light. – Image credit: NASA/Aero Animation/Ben Schweighart

Will humanity ever be able to sail to another planet?

Potentially, solar sail technology could pave the way for human interstellar travel in the future. However, there are challenges, such as sustaining long-term missions for generations and addressing relativistic effects caused by near-light speed travel.

What exactly is NASA's solar sail mission?

NASA’s Advanced Composite Solar Sail System is a demonstration of solar sail technology that aims to test a new lightweight boom made of flexible materials. The mission involves a CubeSat deploying an 80 square meter sail in orbit to gather data for future solar sail missions.

About our experts

patrick johnson is an associate professor at Georgetown University with expertise in quantum mechanics. He authored the book “Star Wars Physics” and has contributed to scientific journals like Physical Review.

Source: www.sciencefocus.com

Here’s How a spacecraft on the edge of interstellar space is communicating with Earth

NASA stays in touch with its space probes, like Voyager 2, through the Deep Space Network (DSN), which consists of radio receiving antennas located in three different spots globally. These locations include Goldstone in California, Robredo near Madrid, and Tidbinbilla near Canberra.

Voyager 2 can only be observed from the southern hemisphere, making the DSS-43 antenna at the Australian site the sole antenna on Earth that can communicate with the spacecraft.

Currently positioned more than 20 billion kilometers from Earth, Voyager 2 has a transmitter that outputs approximately 23 watts (around eight times more powerful than a typical cell phone). By the time a radio signal reaches Earth, it has only about one-tenth of this power.


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To detect this extremely faint signal, DSS-43 and Voyager 2’s transmitters use narrowband, high-frequency signals that are highly directional and transmitted at slow bit rates.

Advanced signal processing techniques, minimal interference, and the fact that radio signals can travel through space with little obstruction allow DSS-43 to overcome long distances.

The antenna can transmit a signal to Voyager 2 at a much higher power level (up to about 400,000 watts) than it receives. This strong output can be easily picked up by the spacecraft even at far distances.

This piece (by Elouise Pace) addresses the question, “How can we communicate with Voyager 2, which is billions of miles away?”

If you have inquiries, please contact us at: questions@sciencefocus.comor reach out to us via Facebook, Xor Instagram Page (please include your name and location).

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Webb discovers complex organic compounds in interstellar ice approaching dual protostars

astronomer using Mid-infrared measuring instrument The NASA/ESA/CSA James Webb Space Telescope's (MIRI) detected molecules ranging from relatively simple ones like methane to complex compounds like ethanol (alcohol) and acetic acid. interstellar ice One low-mass protostar and one high-mass protostar: toward NGC 1333 IRAS 2A and IRAS 23385+6053, respectively.



This image taken by Webb's MIRI instrument shows the region near the IRAS 23385+6053 protostar. Image credit: NASA/ESA/CSA/WRM Rocha, LEI.

Complex organic molecules (COM) are molecules with six or more atoms, including at least one carbon atom.

These materials are the raw material for future exoplanetary systems and are therefore of essential importance in understanding the chemical complexity developed in star-forming regions.

If this material becomes available in a primitive planetary system, it could facilitate the planet's habitability.

In a new study, astronomers Will Rocha, Harold Linnaerts and colleagues at Leiden University used Webb's mid-infrared instrument to determine the extent of COM ice in two protostars, NGC 1333 IRAS 2A and IRAS 23385+6053. We investigated the characteristics.

They were able to identify a variety of COMs, including ethanol (alcohol) and perhaps acetic acid (a component of vinegar).

“Our discovery contributes to one of the long-standing questions in astrochemistry,” Dr. Rocha said.

“What is the origin of COM in the Universe?” Are they created in the gas phase or in ice? Detection of COM in ice is based on the solid phase at the surface of cold dust particles It suggests that chemical reactions can build complex types of molecules. ”

“Some COMs, including those detected in the solid phase in our study, were previously detected in the warm gas phase, so they are now thought to originate from ice sublimation.”

“Sublimation is the change from a solid directly to a gas without becoming a liquid.”

“Therefore, we have hope that detecting COM in ice will improve our understanding of the origins of other, larger molecules in the universe.”



This figure shows the spectrum of the NGC 1333 IRAS 2A protostar. Image credit: NASA/ESA/CSA/Leah Hustak, STScI.

The researchers also detected simpler molecules such as formic acid, methane, formaldehyde, and sulfur dioxide.

“Sulfur-containing compounds, such as sulfur dioxide, played an important role in promoting metabolic reactions on early Earth,” the researchers said.

“Of particular interest is that one of the investigated origins, NGC 1333 IRAS 2A, is characterized as a low-mass protostar.”

“NGC 1333 IRAS 2A may resemble the early stages of our solar system.”

“Therefore, the chemicals identified around this protostar may have been present during the earliest stages of the development of the solar system and were later delivered to the proto-Earth.”

“All of these molecules could become part of comets, asteroids, and ultimately new planetary systems as icy material is transported inside planet-forming disks as protostar systems evolve.” '' said Dr. Ewain van Dyschoek, an astronomer at Leiden University.

“We look forward to using more web data in the coming years to follow this astrochemical trajectory step by step.”

of the team paper It was published in the magazine astronomy and astrophysics.

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WRM Rocha other. 2024. JWST Young Protostar Observation (JOYS+): Detection of icy complex organic molecules and ions. I.CH.FourSo2,HCOO,OCN,H2Colorado, Cooh, Switzerland3CH2Oh, CH3Cho, channel3Ocho and CH3Coo. A&A 683, A124; doi: 10.1051/0004-6361/202348427

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