There is a high probability that Asteroid 2024 YR4 will not collide with Earth in 2032.

Astronomers raced to observe asteroid 2024 YR4

NASA/Magdalena Ridge 2.4M Telescope/New Mexico Institute of Technology/Ryan

The world’s space agency has reduced the chance that asteroid 2024 YR4 will affect Earth by less than 1%. This strongly suggests that potentially catastrophic conflicts will be avoided. However, the asteroid probably passes very extraordinarily close to our planet, giving astronomers a rare opportunity to observe the asteroid in close proximity.

“We don’t expect the impact probability above 1% will exceed 1% in 2032 due to our close approach with the Earth,” he says. Richard Moisle With the European Space Agency (ESA). “The most likely further development is a further reduction in impact probability, perhaps even dropping to zero.”

The alarm last December regarding the asteroid 2024 YR4 was first raised in December last year, when it discovered it could be on Earth’s collision course in 2032. It looks like it’s 40-90 meters wide and can produce a fatal explosion if attacked by a city. Over the next few weeks, global telescopes and space agencies have closely tracked their orbits, honing their future paths more accurately. On February 17th, we reached our highest shock risk with one in 32nd chance, but in the next few days this reduced to a 67th or 1.5% risk.

On February 20th, new observations led to a sudden downgrade of this risk, with NASA having a 0.27% impact chance of 1-in-360, and ESA having a 0.16%, or 1-in-in-in- in-in-in-in-in-in-in-in-in-in-in-in-in-in-in-in-in-in-in-in-in-in-in-in-in-in-in-in-in-in-in-in-in-in-in- in-ine 625. These ratings placed it at 1 on a 10-point Turin scale used to evaluate the hazards brought about by such objects. That score has decreased from 3. So, 2024 YR4 is now considered one of many low-risk asteroids discovered each year, but ultimately misses Earth.

I say this is good news Gareth Collins At Imperial College in London, asteroids still serve as a dry run for planetary defense systems and scientific purposes. “This still makes for an epic, close approach. If the risk of a hit was so high, it must be close to us,” he says.

Space companies that were sketching possible schemes to deflect NASA, ESA and asteroids, say they will likely continue their plans. Niklas Voight At OHB, a German space company. Voigt and his team were beginning to think about the mission to deflect the 2024 YR4, but the new risks won’t change that, he says. “The risk has decreased, but for the time being, we are still working on the topic.”

A close approach could be a good opportunity to test its ability to deflect asteroids, says Voigt – the only previous attempt to do this was NASA’s DART mission, the 160m in 2022 The asteroid-shaped trajectory of the . Satellites can be constructed to send to the 2024 YR4, he says, as well as the ESA’s Ramses satellite, to travel to observe the asteroid Apophis, passing near Earth in 2029. It is set to do so.

The final decision on what to do about YR4 2024 will likely not be made until the planned observation in March using James Webb Space Telescope. Not only does it collect orbital data, it also helps to better assess the size and composition of the asteroid. That information will be provided to the UN Assisted Space Mission Planning Advisory Group, which will determine the best action around the end of April. “These are very useful exercises to find a pinch point to make a decision, as you have time to do something wise in advance,” Collins says. “Absolutely, these committees are still meeting, but they’re probably less stressful.”

The possibility of an Earth shock has plummeted, but the risk of a YR4 collision with the moon in 2024 rose from 0.3% to 1.2%. “There’s a clear possibility that those numbers will rise even further,” says Moissl. “The exact impact of the effects of the moon from objects of this size is still under evaluation.”

The response to this object is also a useful rehearsal for other asteroids of concern, Collins says. “We want to avoid screams in the future, as the public is used to this threat, thinking, ‘Oh, that’s never going to happen.’ ”

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Source: www.newscientist.com

Chances of Asteroid 2024 YR4 Colliding with Earth in 2032 Decrease Once More

The artist's impression of what asteroid 2024 YR4 looks like as they approached Earth in December 2032

NASA

NASA downgraded the risk that the 2024 YR4 would hit the planet by 1.5% in 2032. 1-in-67from the height of a 1-in-32 The chance was the best odds ever.

Astronomers discovered that an asteroid was slamming barrels towards Earth in December, and that has since been the focus of telescopes and space agencies around the world. As they collected more data on the exact orbit of the asteroid, astronomers were able to calculate the likelihood of hitting Earth more accurately. The asteroid is thought to be between 40 and 90 meters wide and can release energy equivalent to TNT's 7.7 megatonnes.

According to NASA, the likelihood of a 2032 collision has increased from a coincidence of one-third since it was first discovered. It then moved to 1/67, 1/53, 1/53, 1/53, 1-in-43, 1-in-38, 1-in-32, and now it's 1/67 I did. The European Space Agency has slightly different odds, Currently giving asteroids a 1.38% chance of collision. These changes reflect an increasing understanding of the asteroid path, meaning they may not necessarily impact Earth.

But we are running out of time to predict the risks of asteroids. One problem is that the 2024 YR4 flies behind the sun in April and goes outside from most Earth-based telescope views. It says it limits the amount that astronomers can narrow down their predictions. Hugh Lewis At the University of Southampton, England. That doesn't necessarily mean it's going down before April. It could continue to rise, but in the end I still miss us. ”

Once the asteroid pops out of sight, it is rare to get any more information before it comes back into view in 2028. However, astronomers can look at past data to reveal previously overlooked asteroid observations. Trajectory. The process is already being carried out by the world's space agencies, Lewis says.

We hope that important information about the size and composition of the asteroid will be collected by James Webb's Space Telescope in the coming months, Lewis says. This helps us understand whether an asteroid can make it intact through Earth's atmosphere and whether it can cause an impact or not.

“It helps us to determine what we need to do about it because if it's a stone asteroid, it's a very different proportion of iron metal asteroids,” Lewis said. I say it. Stone-rich asteroids will be even worse as stone-like asteroids potentially split during impact. “Mass makes a huge difference in terms of whether energy and the atmosphere affects it.”

https://www.youtube.com/watch?v=oczdfwl05tq

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Source: www.newscientist.com

The Grand Canyon was created shortly after a massive asteroid impact.

The view of the two large gorge, the month of the month radly radiated from the Schrodinger basin

Nasasvsernie T. Wright

The vast collision crater near the month of the moon was formed on an asteroid that moved in more than 1 kilometer for 1 second or more, and released 130 times the energy of all existing nuclear weapons. Currently, researchers say that two unusual and straight gorge were formed within 10 minutes by a secondary debris chain of two unusual and straight gorge.

David King In Houston, Texas, and the planetary research institute, we investigated a 312 kilometer Schreading Glator for 15 years. Part of it was to develop a landing site that could have a NASA concertation program. This tried to return people to the moon, but ended in 2009.

“They are basically hidden and in a sense mysterious. [of the moon]King says. “And they are generally overlooked.”

For more information, Kring and his colleagues are using a computer model to investigate the origin of two gorgees or “light rays” extending north from the crater. One is VALLISSCHREDINGER, 270 km long, 2.7 km in depth, 280 km in length and 3.5 km in depth. For comparison, Arizona's Grand Canyon length is 446 km and depth of 1.9 km.

However, it has been engraved in water for millions of years, but the gorge of the moon is a straight and straight groove formed by vast shocking force within 10 minutes. The dramatic asteroid strike not only spread dust and tile BLE throughout the moon, but also spread to space and earth.

Researchers also suggest that the main ones that cause the main crater of the main, faster, to drive the fragments that run through the moon, focusing on narrow areas due to the irregularity of Legoris, which is a loose material that covers the moon. It may have been combined.

Using their models, researchers have calculated that asteroids collide 3811 billion years ago to create the speed and direction of debris to create a gorge. 。

“There is a rock that hits 2 kilometers per second per second, perhaps 2 kilometers per second, and it may be devastating,” says Kring. “I knew that Schrödinger's impact would create these rays, but the related process needed some attention.”

Kring is not deep enough at any of the landing points that Legolis, who was kicked out of Schrölinger, was sued to seriously interfere with geological experiments, so Kring is the moon in the ARTEMIS III mission of NASA. He says that he has a sense of security to put an astronaut in. 。 If they were planning to land north of Schledinger, where much more materials landed, they would have faced a very deep layer that hid the early geology.

The view of the gorge that looks straight at the moon

Nasasvsernie T. Wright

Mark Birchel At Kent University in the UK, this study is done in some way to prove that the gorge is formed by a shock chain, but it is necessary to investigate up close.

“The ultimate evidence is the person who brings back the rocks from one or some rocks in these gorgees,” says Birchel. “Then there is a mineral grain that you just cut out, and was shocked there. [by impacts]And some of them have changed the structure as a result. “

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Source: www.newscientist.com

New Asteroid Discovery Reveals Start of Earth’s Incredible History

Small rocks in the universe revealed that life on earth could have come from asteroids. And life outside of earth suggests that we are one step closer than we thought.

A bold NASA mission known as OSIRIS-REX five years ago The Bennu asteroid is on a course close to colliding with earth, and in the process, it will grab a small sample. A small capsule, containing 120 grams (4 ounces) of asteroid material, landed in the Utah Desert in late 2023.

Since then, scientists have been eagerly waiting to hear the contents of the capsule. Currently, scientists have confirmed that the asteroid contains not only organic matter but also all the components that make up DNA.

Sample return capsules from NASA’s OSIRIS-REX mission are found immediately after landing in the Utah Desert on September 24, 2023. Photo Credit: NASA/Keegan Barber

Bennu, currently orbiting close to the earth, is an ancient fragment of our solar system, with its parent asteroid formed about 4.5 billion years ago.

“We now know from Bennu that the ingredients of life are really interesting and complicated,” said Dr. Tim McCoy, the MET stone curator at the National Natural History Museum in the United States and co-leader of new papers.

“We have found the next step on the road to life.”

The breakthroughs suggest that life was formed on earth after asteroid collisions, but this process also occurs throughout the universe, whether through parent bodies or other asteroid collisions. It suggests a new beginning.

How can Bennu help in forming life?

The most important discovery is that Bennu seems to host “Brinny Bros,” which allows minerals and salts to mix. This compound developed into complex structures that form essential ingredients of life.

Researchers suggest that saltwater outside of earth may be an essential environment for birthing organic compounds throughout the universe, including on earth. In addition to the potential of water, these saltwater environments can facilitate prebiotic organic synthesis processes, where building blocks for life can come together.

Surprisingly, the absence of liquid water plays a vital role here. While liquid water is essential for life, chemical reactions needed to form complex structures require a loss of water in the process.

So what mixture forms this life?

The survey results will be published in the journals Nature and Nature Astronomy. Researchers around the world analyzed a small part of the sample using an electron microscope, enabling inspection at a resolution equal to a human hair.

One paper led by NASA scientists found that Bennu boasts a more extensive collection of organic matter than earth.

“It may seem natural to think that earth, hosting life, has the most widespread collection of organic materials in the solar system,” said Dr. Douglas Vacoc, Research Organization Messaging President of METI (Messaging Extraterrestrial Intelligence), to BBC Science Focus.

The first museum exhibit of a sample from the Bennu Asteroid was announced at the National Natural History Museum of the Smithsonian Institution in the United States. This is a rock-filled fragment with mass. Photo Credit: James di Loret and Philip R. Lee, Smithsonian

The impressive asteroid collection contains 14 of the 20 amino acids found in all living organisms (protein building blocks), including individual non-protein amino acids not known or existing in known biology. The sample also contains all five nucleic bases (adenine, guanine, cytosine, thymine, uracil) that form the code of DNA and RNA.

“There are no signs that Bennu’s amino acids were created by living organisms, but as we know, some essential building blocks for life are abundant on this asteroid,” Vacoch said.

How close are we to “life”?

Researchers have yet to understand the complex structure formed at Bennu’s core upon impact.

“We now have a basic building block moving along this path, but how far along this process can progress is unknown,” they said.

It’s not clear if Bennu’s conditions can advance to the next stage of biological evolution.

“Amino acids alone are not enough for life,” said Professor Lewis Dartnell to BBC Science Focus. “These acids need to bond into long chains to start protein production or bind to DNA. The next step in the origin of life requires not just building blocks but assembling these blocks.”

“To create life, these building blocks must begin the production of molecules like proteins and DNA, forming them into cells,” he added.

What is needed beyond organic molecules and water to reach this point? “The missing elements are energy sources like photosynthesis or chemical energy,” said Dartnell. “Additionally, a long period is required to move from simple amino acids to proteins, DNA, cells, and life spans.”

A scanning electron microscope image of carbonated sodium venous in Bennu’s sample – Photo Credit: Rob Wandel, Tim Gooding, and Tim McCoy, Smithsonian

This discovery represents a significant leap in understanding Bennu’s nature.

“By examining Bennu’s chemical composition, we have found clues to its origins and recent discoveries point to its roots in the outer solar system,” said Vacoch.

Bennu’s contents may set a new baseline for exploring other cosmic bodies. The sample was meticulously preserved before analysis, ensuring the integrity of the salt content.

“There is no substitute for traveling to asteroids, collecting pristine samples, and returning them to an Earth research institute,” Vacoch stated. “OSIRIS-REX serves as proof of profound discoveries from sample return missions.”

If the fragments had fallen to earth on their own, the salt content would have been disrupted in the earth’s atmosphere. But with this knowledge, McCoy and his colleagues may find evidence of this saltwater in existing MET stone collections.

“This is like finding what you were looking for on a mission,” McCoy said. “We have found something unexpected. It’s the best reward for all kinds of exploration.”

About our experts

Dr. Douglas Vacoch, President of the Messaging Extraterrestrial Intelligence (METI), is a research and educational organization that sends signals to nearby stars. He is a member of the International Space Law Research Institute and serves as a general editor for Springer’s Space and Society series.

Professor Lewis Dartnell is a Professor of Science Communication at the University of Westminster, specializing in space biology and the exploration of microbial life on Mars. He is the author of Origin: How Earth Created Us and The Knowledge: How to Rebuild Our World from Scratch.

Read more:

  • 10 future space missions I’m looking forward to
  • What do aliens actually look like?
  • These four signs of alien technology may lead us beyond earth

Source: www.sciencefocus.com

Amino Acids, Salt, and Other Compounds Discovered in Asteroid Bennu Sample by Scientists

The asteroid Benne is believed to be made of tile BLE fragments from the body 4.5 billion years ago, which contains materials generated beyond Saturn, which is a separate object long ago. Destroyed by a collision. In two new papers, scientists include amino acids (including 14 out of 20 used in land biology), polygan aromatic hydrocarbons, ammonia and other compounds, and sodium carbonate, phosphate. It is reported to detect salt such as sulfate, sulfate, sulfate, and sulfate sulfate. Chloride is a Bennu sample delivered to the earth by NASA's OSIRIS-REX spacecraft in 2023.

This mosaic image of the asteroid Benne consists of 12 images collected by 15 miles (24 km) of OSIRIS-REX on December 2, 2018. Image Credit: NASA / NASA Godaddo Space Flight Center / Arizona University.

Dr. Nicky Fox, a semi -manager of the NASA headquarters science mission director, states:

“Asteroids provide time capsules to the history of our hometown planet, and Bennne's sample is extremely important to understand what our solar components exist before life begins on the earth.”

In the Bennu sample, researchers Found Amino Acid -Life on the Earth Used to produce proteins, 14- and all five nuclear foundations used by life on the earth, including a method of placing amino acids amino acids. Used to save and send genetic instructions to molecules. protein.

In addition, the very high existence of ammonia was detected. This is important for biology because it may react with formaldehyde detected in samples, form complex molecules such as amino acids and react in consideration of proper conditions.

When the amino acid is linked to a long chain, protein is created and almost all biological functions supply power.

These building blocks detected by the Bennu sample have previously been found on the outer rocks.

However, it supports the idea that identifying them with an unbalanced sample collected in the universe may be an important cause for the life of the entire solar system. I am.

Dr. Dany Gravin, a senior sample scientist at NASA's Godde Space Flight Center, states:

“That's why some of these new discoveries are not possible without sample return missions, close pollution control measures, and the precious curation and storage of this precious material from Benne.”

OSIRIS-REX View on the outside of sample collector. The asteroid sample material can be seen in the center of the right. Image credit: NASA / ERIKA Blumenfeld / Joseph AeberSold.

scientist It will be identified The traces of 11 salt minerals in the bene sample, which are formed as water containing dissolved salt, evaporate for a long period of time, leaving salt as solid crystals.

Similar salt water is detected or proposed throughout the solar system, including Dwarf Planet Ceres and Saturn's Moon Enkelladus.

“The discovery of these salt was a break -through in space research,” said Dr. Nick Timms, a researcher at Curtin University.

“I was surprised to identify the mineral haright, which is a sodium chloride. It is exactly the same salt as the salt that may be placed in the chip.”

“The mineral we discovered is formed from the evaporation of salt water, which is a bit similar to the salt sediment formed in Australia and the salt lake around the world.”

“By comparing with the mineral sequence of the salt lake on the earth, we can begin to imagine what the asteroid Bennne was, and provide instructions on ancient universe water activities.”

“OSIRIS-REX was a very successful mission,” said Dr. Jason Dworkin, the scientist of OSIRIS-REX, a researcher of NASA's Goddard Space Flight Center.

“OSIRIS-REX data adds a major brush stroke to photos of the solar system that may have life.”

“Why are we so far, not only to see the life on the earth, but it's a really appetite question.”

The survey results are displayed in two journals Natural astronomy And journal Nature

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DP gravin et al。 Asteroid (101955) Sil soluble organic matter with abundant ammonia and nitrogen in Benne sample. Nut asronReleased online on January 29, 2025. Doi: 10.1038/S41550-02472-9

TJ McCoy et al。 2025. An evaporated sequence from ancient salt water recorded in Bennne sample. Nature 637, 1072-1077; DOI: 10.1038/S41586-024-08495-6

Source: www.sci.news

Scientists discover life components in NASA asteroid sample.

summary

  • The NASA spacecraft returned to Earth from the asteroid Bennu in 2023.
  • The first detailed analysis of the material reveals organic molecules, including components of life.
  • This strengthens the theory that asteroids colliding with Earth may have provided life’s ingredients.

Scientists have found many organic molecules, including major building blocks of life, in a sample collected from distant asteroids.

Surprising discoveries suggest that the chemical components required for life may have spread throughout the early solar system.

NASA’s OSIRIS-REX SPACECRAFT was launched in 2016, gathering material from asteroids, dust, soil, and rocks, and returned them to Earth in 2023.

Analysis of the asteroid materials revealed in a sample published in Journal Nature shows that Earth’s life contains key organic compounds and amino acids.

Researchers did not find evidence of life on Bennu, but the results reinforce the theory that asteroids colliding with Earth may have provided life’s necessary ingredients.

Asteroid Bennu seen from Osiris Lex spaceship.NASA

NASA’s Scientific Mission Bureau stated that the OSIRIS-REX mission has already reshaped our understanding of life’s building blocks in the solar system.

The untouched samples collected from asteroids provide unique insights into the early solar system, unlike meteorites that may be contaminated.

The Bennu sample contains surprising concentrations of ammonia, an essential ingredient in biological processes.

NASA scientists have collected data on September 24, 2023, right after a sample return capsule from NASA’s OSIRIS-REX MISSION.Keegan barber / nasa via Getty Images file

Samples from Bennu also contain traces of minerals that are likely remnants of evaporated brine, suggesting complex compositions on the asteroid.

The microscope image of the sample collected from the asteroid Bennu indicates sodium carbonate, also known as soda ash.Rob Wardel, Tim Gooding, Tim McCoy /Smithsonian

These discoveries on Bennu provide valuable insights into the complex composition of minerals and organic compounds that may have influenced the development of life in the solar system.

Further research is needed to fully grasp the implications of the Bennu samples for our understanding of life’s origins on Earth and other celestial bodies.

“Exploring the unique composition of Bennu and its implications for the emergence of life is a fascinating field of study that could shed light on the mysteries of life on Earth and beyond,” said Jason Dworkin, an OSIS-REX project scientist at NASA’s Goddard Space Flight Center.

Source: www.nbcnews.com

A tiny asteroid collides with Earth and disintegrates above Siberia

Webcam images show asteroid burning up in the atmosphere over Siberia

Lensk LR/YouTube

Astronomers discovered the asteroid, about 70 centimeters in diameter, hours before it exploded harmlessly into the atmosphere above Siberia.

european space agency (ESA) issued an alert at 9:27 a.m. GMT, warning that space rocks could illuminate the skies over northern Siberia at around 11:15 p.m. local time (4:15 p.m. GMT).

Speaking before the event, Alan Fitzsimmons from Britain’s Queen’s University Belfast says objects of this size pose no danger to people on the ground, but early warnings are a positive sign that our ability to detect these objects before they hit Earth is increasing.

“It’s small, but it’s still going to be pretty spectacular,” Fitzsimmons said. “The sky above the impact site will darken and a very impressive, very bright fireball will spread across the sky for hundreds of kilometers around it.”

Several objects of this size collide with Earth every year, and we are getting better at detecting them early. The first discovery was in 2008. The next discovery was made six years later, but the pace of observations has picked up. Today’s asteroid, named C0WEPC5, is the fourth predicted to hit Earth this year.

Early warning of small asteroids gives astronomers the opportunity to observe them, collect data, and even try to collect any small pieces that survive. Fitzsimmons said the first such predicted impact in 2008 led to the recovery of a small piece of rock and generated important science. “What was beautiful was that the meteorite’s reflectivity matched exactly what was measured by telescopes before the impact, and it was a perfect match between what we saw in space and what we later found on Earth. It shows a very nice direct connection,” he says.

Detecting larger, more dangerous objects heading toward Earth could provide an opportunity to deflect them or at least evacuate the dangerous area.

A map showing where the asteroid is predicted to hit Siberia’s atmosphere.

ESA

NASA and ESA currently have dedicated programs for asteroid discovery and tracking. This involves a large network of dedicated observatories and amateur astronomers who read the positions of known objects so that their orbits can be better understood and predicted.

This latest asteroid was discovered by NASA’s Asteroid Earth Impact Last Alert System (ATLAS). ATLAS operates four telescopes around the world and is designed to provide up to a week of collision warning.

“This is a victory for science, If you happen to be in Siberia this evening, there will definitely be something to take your mind off the very cold temperatures,” says Fitzsimmons.

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Source: www.newscientist.com

Today, an asteroid will spectacularly burn up in Earth’s atmosphere.

Map showing where asteroid fireballs can be seen in Siberia

ESA

A dramatic but harmless spectacle will take place over Siberia today as an asteroid about 70 centimeters in diameter burns up in the atmosphere.

The space rock will illuminate the sky over northern Siberia at around 11:15 pm local time (4:15 pm Japan time). Warning from the European Space Agency (ESA).

Alan Fitzsimmons Britain's Queen's University Belfast says objects of this size pose no danger to people on the ground, but early warnings are a positive sign that our ability to detect these objects before they hit Earth is increasing. It is said that this is a sign.

“It's small, but it's still going to be pretty spectacular,” Fitzsimmons said. “The sky above the impact site will darken and a very impressive, very bright fireball will spread across the sky for hundreds of kilometers around it.”

Several objects of this size collide with Earth every year, and we are getting better at detecting them early. The first discovery was in 2008. The next discovery was made six years later, but the pace of observations has picked up. Today's asteroid, named C0WEPC5, is the fourth predicted to hit Earth this year.

Early warning of small asteroids gives astronomers the opportunity to observe them, collect data, and even try to collect any small pieces that survive. Fitzsimmons said the first such predicted impact in 2008 led to the recovery of a small piece of rock and generated important science. “What was beautiful was that the meteorite's reflectivity matched exactly what was measured by telescopes before the impact, and it was a perfect match between what we saw in space and what we later found on Earth. “It shows a very nice direct connection,” he says.

Detecting larger, more dangerous objects heading toward Earth could provide an opportunity to deflect them or at least evacuate the dangerous area.

NASA and ESA currently have dedicated programs for asteroid discovery and tracking. This involves a large network of dedicated observatories and amateur astronomers who read the positions of known objects so that their orbits can be better understood and predicted.

This latest asteroid was discovered by NASA's Asteroid Earth Impact Last Alert System (ATLAS). ATLAS operates four telescopes around the world and is designed to provide up to a week of collision warning.

“This is a victory for science, [for] “If you happen to be in Siberia this evening, there will definitely be something to take your mind off the very cold temperatures,” says Fitzsimmons.

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Source: www.newscientist.com

Astronomers reveal new main-belt comet mistaken for active asteroid

456P/Panstars, an active main-belt asteroid first discovered in 2021, is repeatedly active, and its activity is linked to volatile ice formations, according to new observations from the Magellan-Baade and Lowell Discovery telescopes. It is likely that this is caused by sublimation.

456P/PanSTARS image taken on October 3, 2024 with the Magellan Baade Telescope in Chile and with the Lowell Discovery Telescope in Arizona on October 26, 2024. At the center of each image is the comet’s head or nucleus, the tail extends to the right. Image credits: Scott S. Sheppard / Carnegie Institution for Science / Audrey Thirouin, Lowell Observatory / Henry H. Hsieh, Planetary Science Institute.

“Main-belt comets are icy objects found in the asteroid belt between Mars and Jupiter, rather than outside the cold solar system, where icy objects would normally be expected,” said Henry Hsieh, senior scientist at the Planetary Science Institute.

“They have comet-like features, such as tails that extend away from the sun and fuzzy clouds as the sun’s heat evaporates the ice.”

These objects were first discovered in 2006 at the University of Hawaii by Dr. Hsieh and his then-doctoral supervisor, Professor David Jewitt.

“Main-belt comets belong to a larger group of Solar System objects known as active asteroids, which look like comets but have asteroid-like orbits in the warm inner Solar System,” the astronomers said.

“This large group includes not only objects that emit dust from evaporated ice, but also objects that have clouds or tails of ejected dust from collisions or rapid rotation.”

“Both main-belt comets and active asteroids in general are still relatively rare, but scientists are discovering them.”

456P/PANSTARRS was discovered as P/2021 L4 (PANSTARRS) through observations by Pan-STARRS1 on June 9 and 14, 2021, and observations by Canada, France, and Hawaii telescopes on June 14, 2021.

Dr. Hsieh and his co-authors observed the object twice in October 2024 using the Magellan-Baade Telescope and the Lowell Discovery Telescope, establishing its status as a main-belt comet.

“This object is not just an asteroid that experienced a one-off event, but is essentially an active icy object, like other comets in the outer solar system,” Hsieh said.

If 456P/PANSTARRS’s activity is due to something other than ice evaporation, its tail would be expected to appear only once, randomly, and not repeatedly as it approaches the Sun.

On the other hand, icy objects heat up every time they approach the sun, and the evaporated ice is carried away with the dust.

As the object moves away from the sun and cools, it ceases to be active.

Observations of repeated dust ejection activity during their approach to the Sun are currently considered the best and most reliable method of identifying main-belt comets.

“Confirmed main-belt comets are still largely unknown,” Dr. Xie said.

“We want to grow the population so we can understand more clearly what its broader characteristics are, such as its size, active period, and distribution within the asteroid belt. We will be able to better utilize them to track ice within the asteroid belt and across the solar system.”

of findings Published in American Astronomical Society Research Notes.

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Henry H. Shea others. 2024. Recurrence activity of main belt comet 456P/Panstars (P/2021 L4) confirmed. Resolution memo AAS 8,283;doi: 10.3847/2515-5172/ad90a6

This article is a reprint of a press release provided by the Planetary Science Institute.

Source: www.sci.news

Bacteria discovered in asteroid samples, originating from Earth

Bacteria on a sample of asteroid Ryugu observed using an electron microscope

Matthew J. Genge et al. 2024

Rocks brought back to Earth from the asteroid Ryugu appear to be inhabited by microorganisms. But researchers say these microbes almost certainly came from Earth, not space. The contamination is a wake-up call for future sample-return missions, such as NASA’s Mars rover Perseverance, to search for extraterrestrial life.

In 2020, the Japanese space probe Hayabusa2 returned to Earth carrying 5.4 grams of rock collected from the 4.5 billion-year-old asteroid Ryugu. After landing in Australia, the sample capsule was transported to a custom-built facility in Sagamihara, Japan. There, the capsule itself was first opened in a vacuum chamber inside a clean room and then moved to a room filled with pressurized nitrogen for long-term storage. From there, a portion of the sample can be placed in a container filled with nitrogen and sent to researchers.

One of these samples was sent to the UK for research. Matthew Genge Imperial College London and colleagues. Genge and his team initially scanned the samples using X-rays, but found no evidence of bacteria.

Samples from asteroid Ryugu collected by Hayabusa2

JAXA

After 3 weeks, the samples were transferred to resin and further examined using scanning electron microscopy (SEM) after another week. When Genge and his colleagues first looked at the sample and saw what appeared to be thread-like bacteria, his students “almost fell off their chairs” at the prospect of discovering extraterrestrial life. . “It was an exciting moment, but we also had in the back of our minds from previous research that bacteria tend to colonize rocks,” Genge said.

By tracking bacterial growth with follow-up SEM measurements, they found that bacterial populations varied in a manner similar to known microorganisms. Their familiar shape, combined with their absence in the first X-ray scan, makes it very likely that they were terrestrial in origin, Genge says.

He believes the samples may have become contaminated after being embedded in the resin. The experiment was conducted at a facility on Earth that also handles space rocks. Rock specimens often contain bacteria that are adapted to live within them. “All it takes is one bacterium or one bacterial spore for this to happen,” he says. “For example, when we’re preparing meteorite samples, we don’t usually see this kind of colonization happening, and that’s because the probability of it happening is so low. In this case , one bacterium fell onto the sample and started multiplying.”

But Genge added that this should serve as a warning for future sample return missions. “Finding microbes in samples returned from space should be the gold standard for discovering extraterrestrial life. If we were to do that, we would fly to Mars, collect samples, and bring them back. “If we found microorganisms in it, we would say that was the clincher,” Genge says. “But our findings really show that we have to be very careful in interpreting the samples because they are susceptible to contamination with terrestrial bacteria.”

Javier Martin Torres Researchers at the University of Aberdeen in the UK agree that changes in the microbial filament population suggest a terrestrial origin, but this does not exclude the possibility that they came from elsewhere. . “If you want to be sure that these microorganisms are not of extraterrestrial origin, you need to do DNA sequencing,” he says.

Scientists already knew that bacteria could survive very well in meteorite samples that fell to Earth, but this raises the possibility that bacteria could also survive on materials elsewhere in the solar system. It only strengthens it. “The microorganisms can use organic matter within the meteorite to sustain themselves. They’re feeding on an extraterrestrial snack,” Genge says. “So there may be an ecosystem on Mars. It’s a fairly sparse ecosystem, but it’s an ecosystem that’s supported by manna from the sky and by meteorites that fall on the surface.”

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Source: www.newscientist.com

Can Catastrophe be Prevented if an Asteroid is Approaching Earth?

Hidden somewhere in the dark of space, there is a giant asteroid on a collision course with Earth. If we don’t spot it and somehow stop its arrival, it will hurtle through Earth’s atmosphere at 60,000 kilometers per hour and slam into the ground, vaporizing everything it touches.

With millions of asteroids hurtling through the inner solar system, the threat is inevitable. A conflict will occur sooner or later. But that doesn’t mean the Earth has to be a sitting duck. The global community is obsessed with planetary defense, carefully planning how to repel extraterrestrial invaders should they appear, or at least minimize carnage.

Among other things, this research includes scanning the sky for threats and testing missions to throw asteroids off course. But it also includes a surprising amount of role-playing, with scenarios in which teams impact asteroids in a war game. “Exercises like this are necessary because in the real world, we have not yet reached this point where we need to actually design and build a mission,” NASA said. Paul Chodas do a lot of role-playing. “It makes you think about details that you wouldn’t otherwise think about.”

In the coming paragraphs, you’ll be in the hot seat for a choose-your-own-adventure version of one of these role-playing games. You decide how to react when an asteroid comes towards us. Whether you want to crash your spaceship, use sunlight-absorbing paint to change its course, or just blow it to pieces, you’ll realize we have even more options…

Source: www.newscientist.com

What can preparing for an asteroid impact teach us about climate change?

When it comes to natural disasters, it is often impossible to predict them more than a few months or even days in advance. We cannot say, “Let's prepare because an earthquake will occur within two years.'' But one of the few things we can really prepare for is an asteroid impact.

Although no one has yet discovered a large asteroid on a collision course with Earth, scientists, engineers, and policymakers are working on plans to defend the planet in the event it does. Techniques to avoid disaster are already being tested, such as impacting asteroids to change their orbits, as NASA's Double Asteroid Redirection Test Mission did successfully in 2022.

One of the most surprisingly useful planetary defense tools is running a role-playing game. This reveals roadblocks that can derail even the best-laid plans. Paul Chodas of NASA, who runs some of these exercises, says they reveal problems that would never have been considered otherwise. In our special feature, “If an asteroid is heading towards Earth, can we avoid disaster?”you can try such games yourself.

Compared to other existential threats, the risk from asteroids is relatively small

It goes without saying that factors such as the size of rocks coming from space and how quickly they are discovered have a major impact on whether disasters can be successfully avoided. So is the ability to communicate effectively. different options. These are important lessons that go beyond just protecting yourself from asteroids.

Compared to other existential threats, the risk of an asteroid coming our way is relatively small. Climate change is already happening. Pandemics have occurred regularly throughout human history, and global warming has made them even more likely. We know that these involve technical challenges, such as the development and deployment of green technologies, but the social challenges are equally important.

Only with effective global cooperation and communication can humanity tackle its greatest challenges. That's as true in the Asteroid Roleplaying Game as it is in real life.

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Source: www.newscientist.com

New Hera probe sent to study asteroid target of NASA’s previous experiment

On Monday, a spacecraft was launched to investigate. Space collision site.

The European Space Agency’s Hera spacecraft was rocket-launched on a two-year journey to the small, harmless asteroid it crashed into. Two years ago, NASA During that day’s dress rehearsal, a killer space stone threatens Earth. The experiment, launched by SpaceX from Cape Canaveral, is the second in a series of planetary defense tests that could one day save the planet.

Crash in 2022 NASA dart spacecraft This shortens Dimorphos’ orbit around its larger brethren, indicating that if a dangerous rock is headed in our direction, it can be thrown off course with sufficient advance notice. I did.

Scientists want to study the impact’s aftermath up close to learn exactly how effective Dart was and what changes are needed to protect the planet in the future.

“The more details we can gather, the more details we can gather because it could be important in planning future deflection missions if they are needed,” University of Maryland astronomer Derek Richardson said before the launch. It’s good enough.”

Researchers want to know whether Dart (short for Double Asteroid Redirection Test) left behind a crater or changed the shape of the 500-foot (150-meter) asteroid more dramatically. Richardson, who participates in the dart mission and supports Hera, said that before the dart was shot, it looked like a flying saucer, but now it may resemble a kidney bean.

ESA’s Hera mission lifted off at 10:52 a.m. Monday aboard a SpaceX Falcon 9 rocket from Cape Canaveral Space Force Station in Florida.
S. Korbach / ESA

The flurry of darts sent debris and even rocks flying from Dimorphos, further increasing the force of the impact. The debris trail stretched thousands of miles (more than 10,000 kilometers) into space over several months.

Flight director Ignacio Tanco said rocks and other debris may still be floating around the asteroid, posing a potential threat to Hera.

“We don’t really know what kind of environment we’re going to operate in,” Tanko says. “But the whole point of this mission is to go out there and find out.”

European officials described the $400 million (363 million euro) mission as an “investigation of the accident scene.”

Project manager Ian Carnelli said Hera was “returning to the crime scene and obtaining all the scientific and technical information”.

Hera, which is about the size of a small car and carries more than a dozen scientific instruments, needs to fly past Mars in 2025 to increase its gravity and reach Dimorphos by the end of 2026. This is a satellite of the fast-spinning asteroid Didymos, which means twins in Greek. It’s 5 times bigger. At that point, the asteroid will be 120 million miles (195 million kilometers) from Earth.

Hera, controlled by a flight team in Darmstadt, Germany, will attempt to enter orbit around the pair of rocks as its flight range gradually decreases from 18 miles (30 kilometers) to half a mile (1 kilometer). The spacecraft will study the satellite for at least six months, determining its mass, shape, composition, and orbit around Didymos.

Before impact, Dimorphos circled its larger mate from three-quarters of a mile (1,189 meters) away. Scientists believe the orbit could become tighter and more elliptical, potentially even causing the satellite to fall off.

Source: www.nbcnews.com

2024 RW1: Tiny asteroid strikes Earth and disintegrates above the Philippines

Predicted trajectory of asteroid CAQTDL2 over the Philippines

Catalina Sky Survey/ESA

The asteroid struck Earth and burned up in the atmosphere east of the Philippines. Astronomers spotted it just hours before it streaked across the sky in a bright fireball, but many on the ground couldn’t see it because of cloudy skies caused by Typhoon Enteng.

The asteroid, estimated to be about one meter in diameter, was a NASA-funded Catalina Sky Survey. It was originally designated CAQTDL2 and was later renamed 2024 RW1.

As expected, the asteroid struck the east of the northernmost island of the Philippine archipelago at around 1645 GMT, 1745 London time, 1245 New York time, or 0045 local time. The impact speed was predicted to be 17.6 kilometers per second, or 63,360 kilometers per hour. Alan Fitzsimmons. That’s average for such an object, says a researcher at Queen’s University in Belfast, UK. “Don’t be fooled by Hollywood movies where you see something screaming into the sky and you have time to run out the house, grab your cat, hop in your car and drive somewhere. You don’t have time for that,” he says.

Asteroid CAQTDL2 can be seen moving across the sky in a purple circle.

Catalina Sky Survey

Luckily, no evacuations were necessary: NASA’s Planetary Defense Coordination Office posted on social media that the asteroid “safely impacted Earth’s atmosphere.”

“Something that small wouldn’t do any damage on the ground because the Earth’s atmosphere blocks that,” Fitzsimmons said. Video shared on social media from Cagayan province in the northern tip of the Philippines shows a flickering green fireball appearing behind a cloud, followed by an orange tail, before disappearing a few seconds later.

Fitzsimmons said two to three objects this size hit Earth every year, and early detection is becoming more common – astronomers detected the first near-Earth asteroid before it fell to Earth in 2008. 2024 RW1 will be the ninth asteroid to be accurately predicted to hit Earth.

“The really good thing about this is that our survey telescopes are now good enough to detect these objects as they approach and to provide a warning,” he says. “In other words, if this object was bigger and potentially threatening to people on the ground, it would have appeared brighter and projected farther. So this is a really cool demonstration that our current survey systems work really well. Right now, we’re probably averaging about one asteroid per year that gets detected before it hits the atmosphere, and survey systems are getting better and better.”

Not only is Earth developing and improving its early warning systems, but in 2022 NASA’s Dual Asteroid Reorientation Test (DART) spacecraft proved it could potentially save Earth from a catastrophic impact with a larger object. DART struck the 160-meter-wide moonlet Dimorphos, slowing it slightly, demonstrating that in theory such a disaster could be averted. Next month, the European Space Agency will launch the Hera mission to study the consequences of the impact in detail and further our understanding of planetary defense.

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Source: www.newscientist.com

Don’t Panic: Small Asteroid CAQTDL2 is Approaching Earth

Predicted trajectory of asteroid CAQTDL2 over the Philippines

Catalina Sky Survey/ESA

Astronomers have discovered that an asteroid is on its way to collide with Earth at thousands of kilometers per hour, likely somewhere east of the Philippines, over the ocean. Fortunately, this relatively small object won’t pose any harm and will simply burn up in the atmosphere in a fireball.

The asteroid, estimated to be about one meter in diameter, was a NASA-funded Catalina Sky Survey. The asteroid has been named CAQTDL2 and is scheduled to impact Earth at approximately 16:45 GMT, 17:45 London time, 12:45 New York time, and at approximately 00:45 local time at the impact site in the Philippines.

It is currently estimated that CAQTDL2 will impact at a speed of 17.6 kilometers per second, or 63,360 kilometers per hour. Alan Fitzsimmons That’s average for such an object, says a researcher at Queen’s University in Belfast, UK. “Don’t be fooled by Hollywood movies where you see something screaming into the sky and you have time to run out the house, grab your cat, hop in your car and drive somewhere. You don’t have time for that,” he says.

Fortunately, no such evacuation is necessary. Although the impact would be dramatic and could shine as brightly as the moon in the night sky, it poses no danger to people on the ground. “An object this small can’t do any damage on the ground because it’s protected by the Earth’s atmosphere,” Fitzsimmons says. “It would just burn up harmlessly and then explode in a very impressive fireball.”

Asteroid CAQTDL2 can be seen moving across the sky in a purple circle.

Catalina Sky Survey

Fitzsimmons said two to three objects this size hit Earth each year, and early detection is becoming more common – astronomers first spotted a near-Earth asteroid before it fell to Earth in 2008. CAQTDL2 is the ninth asteroid to be accurately predicted to hit Earth.

“The really good thing about this is that our survey telescopes are now good enough to detect these objects as they approach and to provide a warning,” he says. “In other words, if this object was bigger and potentially threatening to people on the ground, it would have appeared brighter and projected farther. So this is a really cool demonstration that our current survey systems work really well. Right now, we’re probably averaging about one asteroid per year that gets detected before it hits the atmosphere, and survey systems are getting better and better.”

Not only is Earth developing and improving its early warning systems, but in 2022 NASA’s Dual Asteroid Reorientation Test (DART) spacecraft proved it could potentially save Earth from a catastrophic impact with a larger object. DART struck the 160-meter-wide moonlet Dimorphos, slowing it slightly, demonstrating that in theory such a disaster could be averted. Next month, the European Space Agency will launch the Hera mission to study the consequences of the impact up close and further our understanding of planetary defense.

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Source: www.newscientist.com

Recent research indicates that a giant asteroid collided with Ganymede 4 billion years ago

Jupiter’s moon Ganymede is home to an ancient impact structure called the Groove System, the largest impact structure in the outer Solar System, whose impact would have had a major impact on Ganymede’s early history.

The distribution of grooves and the location of the center of the groove system are always shown on the hemisphere away from Jupiter (top) and on a cylindrical projection of Ganymede (bottom). Grey areas represent geologically new terrains that are devoid of grooves. Gutters (green lines) are only present in geologically older terrains (black areas). Image courtesy of Naoyuki Hirata, doi: 10.1038/s41598-024-69914-2.

Ganymede is the largest moon in the solar system and has many unique features, including tectonic valleys known as grooves.

The grooves are the oldest surface features identified on Ganymede, as they are crossed by impact craters over 10 km in diameter. The grooves provide clues to the moon’s early history.

The trench is thought to be a fragment of a multi-ring impact basin structure similar to the Valhalla basin on Callisto and the Asgard basin.

The largest trench system lies across the Galileo-Marius region, the so-called Galileo-Marius trench system, which is the remnant of an ancient giant impact that radiates in concentric circles from a single point on Ganymede.

“Jupiter’s moons Io, Europa, Ganymede, and Callisto each have interesting features, but what caught my attention were the grooves on Ganymede,” said planetary scientist from Kobe University. paper Published in the journal Scientific Reports.

“We know that this feature was created by an asteroid impact about 4 billion years ago, but we didn’t know how large that impact was or how it affected the Moon.”

First, Dr. Hirata noticed that the estimated location of the impact was almost exactly on the meridian farthest from Jupiter.

“Similarities with the Pluto impact that shifted the dwarf planet’s rotation axis, as seen through NASA’s New Horizons spacecraft, suggest that Ganymede underwent a similar reorientation,” he said.

The asteroid that struck Ganymede was probably about 300 kilometers (180 miles) in diameter, roughly 20 times larger than the Chicxulub asteroid that smashed into Earth 65 million years ago, ending the age of the dinosaurs, leaving a temporary crater 800 to 1,000 miles (1,400 to 1,600 kilometers) across, according to the study.

Only an impact of this magnitude would be likely to shift the Moon’s rotation axis to its current position due to the change in mass distribution, regardless of where on the surface the impact occurred.

“We want to understand the origin and evolution of Ganymede and other Jupiter moons,” Dr. Hirata said.

“The giant impact must have had a major impact on Ganymede’s early evolution, but the thermal and structural effects of the impact on Ganymede’s interior remain largely unexplored.”

“We think that further research into the application of the internal evolution of icy moons could be done next.”

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N. Hirata. 2024. Giant impact on early Ganymede and subsequent reorientation. Scientific Reports 14, 19982. doi: 10.1038/s41598-024-69914-2

Source: www.sci.news

Study finds that Chicxulub asteroid, which caused dinosaur extinction, originated from beyond Jupiter.

The asteroid, called the Chicxulub impactor, was a carbonaceous asteroid that formed outside the orbit of Jupiter. New Paper Published in the journal Science.

Ankylosaurus magniventrisA Tyrannosaurus, a type of large armored dinosaur, witnessed the impact of an asteroid that fell on the Yucatan Peninsula 66 million years ago. Image by Fabio Manucci.

About 66 million years ago, a 10-kilometer-wide asteroid struck Earth near what is now a small town called Chicxulub in Mexico.

This impact released incredible amounts of climate-changing gases into the atmosphere, setting off a chain of events that led to the extinction of the non-avian dinosaurs and 75% of life on Earth.

Evidence includes the presence of high concentrations of platinum group elements (PGE) in the Cretaceous-Paleogene boundary layer, including iridium, ruthenium, osmium, rhodium, platinum, and palladium, which are rare on Earth but common in meteorites.

These elevated PGE levels have been found worldwide, suggesting that the impact spread debris around the world.

Some have proposed large-scale volcanism in the Deccan Traps igneous province of India as an alternative source of PGEs, but the specific PGE ratios at the Cretaceous-Paleogene boundary are more consistent with an asteroid impact than volcanism.

However, little is known about the nature of the Chicxulub impactor, including its composition and extraterrestrial origin.

To answer these questions, Dr Mario Fischer-Gödde from the University of Cologne and his colleagues measured ruthenium isotopes in samples taken from three sites at the Cretaceous-Palaeogene boundary.

For comparison, the team also analysed samples from five other impacts that occurred between 36 million and 470 million years ago, an ancient impact spherule from 3.5 to 3.2 billion years ago, and two carbonaceous meteorites.

The researchers found that the ruthenium isotope signature of samples taken from the Cretaceous-Paleogene boundary was uniform and matched very closely to that of carbonaceous chondrites rather than those from Earth or other types of meteorites, suggesting that the Chicxulub impactor likely came from a carbonaceous-type asteroid that formed in the outer solar system.

The other five impact structures have isotopic signatures more consistent with silicic asteroids that formed closer to the Sun.

The ancient spherulitic samples are consistent with a carbonaceous asteroid impact during the final stages of Earth's accretion.

“The composition of this asteroid is consistent with that of carbonaceous asteroids that formed outside Jupiter's orbit during the formation of the solar system,” Dr Fischer-Gödde said.

“Asteroid impacts like Chicxulub turn out to be very rare and unique events in geological time,” said Professor Carsten Müncher from the University of Cologne.

“The fate of the dinosaurs and many other species was sealed by this object that came from the outer solar system.”

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Mario Fischer-Gedde others2024. Ruthenium isotopes indicate that the Chicxulub impactor was a carbonaceous asteroid. Science 385 (6710): 752-756; doi: 10.1126/science.adk4868

Source: www.sci.news

Study suggests a remarkably faraway asteroid could have been responsible for dinosaur extinction

Research has shown that the asteroid responsible for the mass extinction that annihilated the dinosaurs 66 million years ago originated from a distant region in the solar system, unlike most asteroids that have collided with Earth.

According to European and American researchers, the dinosaur-killing asteroid formed in a cold area outside Jupiter’s orbit and contained high levels of water and carbon. Survey results The study detailing these findings was published in the journal Science on Thursday.

In their analysis of objects that have struck Earth in the last 500 million years, the researchers noted that only asteroids rich in water have caused mass extinctions like the one that wiped out the dinosaurs. Co-author François Tissot, a professor at the California Institute of Technology, explained that asteroids originating closer to the sun were significantly drier.

Tissot further stated, “All other impacts that occurred were from objects closer to the sun and just happened to hit that specific spot, so the asteroid responsible for the dinosaur extinction is truly unique in both its characteristics and origin.”

This catastrophic asteroid created the Chicxulub crater in Mexico’s Yucatan Peninsula. While direct samples of the asteroid itself were unattainable due to its fragmentation, researchers were able to analyze particles that were dispersed upon impact and settled in Earth’s strata.

The researchers specifically examined ruthenium, a rare element on Earth that can be linked back to the asteroid.

The study confirmed earlier conclusions that classified the asteroid as a carbonaceous, or C-type, asteroid, though some theories proposed it could have been a comet that caused the dinosaur extinction.

Tissot explained, “Comets originate from great distances from the sun and are primarily composed of ice and dust. While the ruthenium levels of a comet have not been measured, based on research indicating other elements, it seems highly improbable that the extinction-causing object was a comet.”

According to Tissot, this study represents progress in understanding the evolution of Earth.

“By delving into Earth’s history, we now have a comprehensive look at its evolution,” he remarked. “This allows us to pose new questions about our planet.”

Source: www.nbcnews.com

Study suggests Chicxulub asteroid that caused dinosaur extinction originated beyond Jupiter

The asteroid, called the Chicxulub impactor, was a carbonaceous asteroid that formed outside the orbit of Jupiter. New Paper Published in the journal Science.

Ankylosaurus magniventrisA Tyrannosaurus, a type of large armored dinosaur, witnessed the impact of an asteroid that fell on the Yucatan Peninsula 66 million years ago. Image by Fabio Manucci.

About 66 million years ago, a 10-kilometer-wide asteroid struck Earth near what is now a small town called Chicxulub in Mexico.

This impact released incredible amounts of climate-changing gases into the atmosphere, setting off a chain of events that led to the extinction of the non-avian dinosaurs and 75% of life on Earth.

Evidence includes the presence of high concentrations of platinum group elements (PGE) in the Cretaceous-Paleogene boundary layer, including iridium, ruthenium, osmium, rhodium, platinum, and palladium, which are rare on Earth but common in meteorites.

These elevated PGE levels have been found worldwide, suggesting that the impact spread debris around the world.

Some have proposed large-scale volcanism in the Deccan Traps igneous province of India as an alternative source of PGEs, but the specific PGE ratios at the Cretaceous-Paleogene boundary are more consistent with an asteroid impact than volcanism.

However, little is known about the nature of the Chicxulub impactor, including its composition and extraterrestrial origin.

To answer these questions, Dr Mario Fischer-Gödde from the University of Cologne and his colleagues measured ruthenium isotopes in samples taken from three sites at the Cretaceous-Palaeogene boundary.

For comparison, the team also analysed samples from five other impacts that occurred between 36 million and 470 million years ago, an ancient impact spherule from 3.5 to 3.2 billion years ago, and two carbonaceous meteorites.

The researchers found that the ruthenium isotope signature of samples taken from the Cretaceous-Paleogene boundary was uniform and matched very closely to that of carbonaceous chondrites rather than those from Earth or other types of meteorites, suggesting that the Chicxulub impactor likely came from a carbonaceous-type asteroid that formed in the outer solar system.

The other five impact structures have isotopic signatures more consistent with silicic asteroids that formed closer to the Sun.

The ancient spherulitic samples are consistent with a carbonaceous asteroid impact during the final stages of Earth's accretion.

“The composition of this asteroid is consistent with that of carbonaceous asteroids that formed outside Jupiter's orbit during the formation of the solar system,” Dr Fischer-Gödde said.

“Asteroid impacts like Chicxulub turn out to be very rare and unique events in geological time,” said Professor Carsten Müncher from the University of Cologne.

“The fate of the dinosaurs and many other species was sealed by this object that came from the outer solar system.”

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Mario Fischer-Gedde others2024. Ruthenium isotopes indicate that the Chicxulub impactor was a carbonaceous asteroid. Science 385 (6710): 752-756; doi: 10.1126/science.adk4868

Source: www.sci.news

352 new binary asteroid candidates discovered by ESA’s Gaia mission

Binary asteroid systems have attracted the attention of the scientific community due to their intriguing properties and significant impact on our understanding of the Solar System. Unlike single asteroids, binary systems provide unique insights into many fundamental processes, including planetary formation and evolution, collision dynamics, and gravitational interactions.

Gaia has discovered possible moons around 352 asteroids that are not known to have companion stars. Image courtesy of ESA.

Asteroids are fascinating celestial objects that hold unique insights into the formation and evolution of our solar system.

Binary stars are even more fascinating because they allow astronomers to study how different objects in the universe form, collide, and interact.

With our unique all-sky scanning function, ESA's Gaia satellite Since its launch in 2013, it has made a number of important asteroid discoveries.

In Data Release 3, Gaia pinpointed the positions and movements of more than 150,000 asteroids. That precision has allowed scientists to probe deeper, looking for asteroids that exhibit a characteristic “wobble” caused by the gravitational pull of their orbiting companion stars.

Gaia has also collected data on the asteroid's chemistry, compiling the largest ever collection of asteroid reflectance spectra – light curves that reveal an object's color and composition.

More than 150,000 orbits determined in Gaia's Data Release 3 were refined as part of the mission's Focused Product Release last year, making them 20 times more accurate.

Gaia's upcoming Data Release 4 (due after mid-2026) is expected to reveal the orbits of even more asteroids.

“Binary asteroids are difficult to find because most are very small and far away from Earth,” said Dr Luana Liberato, an astronomer at the Observatory of the Côte d'Azur.

“Although just under one in six asteroids are predicted to have companion stars, only half a billion of the one million known asteroids have been found to be in binary systems.”

“But this discovery shows that there are many more asteroid moons still waiting to be discovered.”

“If confirmed, this new discovery adds 352 potential binary systems, nearly doubling the known number of moon-bearing asteroids.”

“Gaia is proving to be an excellent asteroid explorer, working hard to unlock the secrets of the universe, both within our solar system and beyond,” said Dr Timo Prusti, ESA's Gaia project scientist.

“This discovery highlights the Gaia data release as a major improvement in data quality and demonstrates the incredible new science made possible by this mission.”

a paper A paper describing the results has been published in the journal Astronomy and Astrophysics.

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L. Liberato others2024. Binary asteroid candidate in the Gaia DR3 astronomical measurements. A&A 688, A50;doi: 10.1051/0004-6361/202349122

This article was based on an original release from ESA.

Source: www.sci.news

An Ambitious New Space Mission on a Collision Course with an Approaching Asteroid

To prevent a fate similar to the dinosaurs, The European Space Agency (ESA) has initiated work on a groundbreaking planetary defense mission known as the Rapid Apophis Mission for Space Security (RAMSES).

RAMSES is designed to rendezvous with 99942 Apophis, an asteroid the size of a cruise ship, and accompany it as it approaches Earth in April 2029.

Apophis, with a diameter of about 375 meters, will pass within 32,000 kilometers of Earth’s surface on April 13, 2029. This rare event will be visible to the naked eye in parts of Europe, Africa, and Asia, attracting global attention. An asteroid of this size only comes this close once every 5,000 to 10,000 years.


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Astronomers believe that Apophis is unlikely to collide with Earth in the next 100 years, but the 2029 flyby will provide scientists with a unique opportunity to observe a close encounter.

The ESA’s Ramses spacecraft is set to reach Apophis two months before the closest approach, allowing monitoring of any physical changes to the asteroid caused by Earth’s gravity.

Ramses is scheduled to launch in April 2028 and arrive at Apophis by February 2029. The mission aims to observe and study how Earth’s gravity affects Apophis, potential landslides, and any new material beneath the asteroid’s surface.

Patrick MichelGerry McClellan, CNRS Director of Research at the Observatory of the Côte d’Azur, emphasized the significance of the mission, stating: “There is much we still don’t know about asteroids, but now, nature is bringing one to us to conduct the experiment itself. All we need to do is watch as Apophis is stretched and compressed by powerful tidal forces.”

Ramses will utilize a variety of scientific instruments to comprehensively study Apophis, analyzing its shape, surface, orbit, rotation, and more.

The collected data will be closely examined by scientists to understand the asteroid’s composition, structure, and how to deflect potentially hazardous asteroids in the future.

Experts predict that Earth’s tidal forces could alter the asteroid’s rotation, potentially causing earthquakes and landslides. They hope that Ramses’ flyby will offer detailed observations of how Apophis is affected by the close encounter.

Additionally, NASA is redirecting its OSIRIS-REx spacecraft (now renamed OSIRIS-APEX) towards Apophis, set to arrive about a month after the 2029 flyby.

OSIRIS-REx was the first US mission to collect samples from an asteroid, returning material from Bennu to Earth in September 2023. After successfully delivering the sample, the spacecraft was renamed OSIRIS-APEX for its new mission to explore Apophis.

“Ramses will demonstrate humanity’s capability to deploy a reconnaissance mission to rendezvous with an approaching asteroid in just a few years,” said Richard Moisle, head of ESA’s Planetary Defence Division.

A decision on the full implementation of Ramses will be made at ESA’s Ministerial Council meeting in November 2025. If approved, Ramses will not only enhance knowledge of asteroid deflection but also provide valuable scientific insights into the solar system’s formation and evolution.

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Source: www.sciencefocus.com

Spotting a harmless asteroid passing close to Earth this Saturday: What you need to know.

This weekend, there will be a passing asteroid near Earth, which poses no threat. With the right equipment and timing, you may be able to catch a glimpse of it.

The asteroid, known as 2024 MK, will be at its closest point to Earth on Saturday morning, passing at a distance about three-quarters of the way from Earth to the moon. It was first spotted two weeks ago by an observatory in South Africa and measures approximately 393 to 853 feet (120 to 260 meters) wide.

According to Davide Farnocchia, an asteroid expert at NASA’s Center for Near Earth Object Studies, smaller objects pass by Earth regularly. Asteroids of this size come close to Earth roughly every 25 years.

“We may witness this event a few times in our lifetime, but it’s not a common occurrence,” he noted.

The 7,579-foot (2,310-meter) asteroid made a safe pass near Earth on Thursday, but it was too distant to be visible without specialized telescopes.

To see the asteroid on Saturday, skywatchers will need small telescopes as it won’t be bright enough to be seen with the naked eye. It will move swiftly across the southern sky, making it challenging to spot.

Nick Moskovitz, an astronomer at Lowell Observatory, mentioned, “The asteroid will move rapidly through the star field.”

For the best chance of seeing the asteroid, observers in the Southern Hemisphere should look high overhead. People in the US may have better luck spotting it on Saturday night when it might be less bright, but easier to see without the sun’s glare.

If you miss this event, mark your calendars for April 13, 2029, when the asteroid Apophis will pass close to Earth and be visible to the naked eye from parts of Europe, Africa, and Asia.

Source: www.nbcnews.com

Astronomers report that the moons orbiting asteroid Dinkinesh are in a contact binary configuration

Dinkinesh is a small asteroid orbiting the Sun near the inner edge of the main asteroid belt. NASA’s Lucy spacecraft recently revealed that this asteroid, with an effective diameter of just 720 meters, is unexpectedly complex. The asteroid has a pronounced valley covered by an equatorial ridge and is currently orbited by a contact binary moon, named Seram, which consists of two nearly equal lobes with diameters of 210 meters and 230 meters. The moon orbits at a distance of 3.1 kilometers from Dinkinesh, has an orbital period of about 52.7 hours, and is tidally locked.

Stereo image pair (a-c) taken by the L’LORRI instrument aboard NASA’s Lucy spacecraft on November 1, 2023, shows asteroid Dinkinesh. Yellow and rose dots indicate valley and ridge features, respectively. These images have been sharpened and processed to enhance contrast. Image (d) shows a side-on view of Dinkinesh and its moon Ceram, taken a few minutes after closest approach. Image credit: NASA/GSFC/SwRI/Johns Hopkins APL/NOIRLab.

“We want to understand the strength of small bodies in the solar system because it’s important to understanding how planets like Earth got here,” said Dr. Hal Levison, a research scientist at Southwest Research Institute and Lucy principal investigator.

“Essentially, planets formed when a bunch of tiny objects orbiting the sun, like asteroids, collided with each other.”

“How objects behave when they collide – whether they break or stick together – has a lot to do with the object’s strength and internal structure.”

The researchers believe that how Dinkinesh responded to stress may reveal something about its inner workings.

As it rotated in sunlight for millions of years, tiny forces from thermal radiation radiating from the asteroid’s warm surface created tiny torques that caused Dinkinesh to spin gradually faster, and the accumulated centrifugal forces caused parts of the asteroid to become more elongated.

This event likely sent debris into close orbit, providing the raw material for the formation of the ridge and moons.

If Dinkinesh had been a weaker, more mobile mass of sand, its particles would have gradually migrated toward the equator and then blasted off into orbit as it rotated faster.

But the images suggest that, like rock, the Dinkinesh asteroid was stronger than a fluid and held together longer, until it eventually disintegrated under pressure and broke into larger pieces. Still, the force needed to break up a small asteroid like Dinkinesh is tiny compared to most rocks on Earth.

“This valley suggests a sudden collapse, more like an earthquake, where stress builds up gradually and then is suddenly released, rather than the slow process that creates sand dunes,” said Dr. Keith Noll, a research scientist at NASA’s Goddard Space Flight Center and a Lucy scientist.

“These features show that Dinkinesh has some strength, and we can do a bit of historical reconstruction to see how this asteroid evolved,” Dr Levison said.

“During that collapse, the rocks broke apart and things separated, forming a disk of material, some of which rained down to the surface and formed the ridge.”

“We think that some of the material in the disk formed the moon Ceram, which is actually a structure where two celestial bodies are in contact with each other, known as a contact binary. The details of how this unusual moon formed remain a mystery.”

of Investigation result Published in the journal Nature.

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H.F. Levison others2024. Contact binary moon of asteroid (152830) Dinkinesh. Nature 629, 1015-1020; doi: 10.1038/s41586-024-07378-0

Source: www.sci.news

Berlin witnesses fastest spinning asteroid breakup in recorded history

A long exposure photo showing the trajectory of asteroid 2024 BX1 just before impact. Changes in brightness are caused by the asteroid’s rotation

L. Buzzi, Schiaparelli Observatory, Italy (MPC 204)

The asteroid that entered Earth’s atmosphere this year was spinning at a rate of 2.6 seconds per rotation, faster than any known asteroid.

The object, known as 2024 BX1, was likely less than one meter wide and entered Earth’s atmosphere on January 21. It disintegrated over Berlin, Germany. Some debris survived the fireball and was retrieved. This is a rare instance of a monitored asteroid fall, where the incoming rock was detected before impact, in this case, just three hours prior to impact.

Maxime Devogele and his team at the European Space Agency’s Near-Earth Object Coordination Center in Italy captured images of the asteroid before impact. Despite traveling at around 50,000 kilometers per hour, the elongated shape of the asteroid made changes in brightness due to rotation quite noticeable in these images.

These changes in brightness corresponded to a rotation time of 2.588 seconds, equivalent to approximately 30,000 rotations per day. “This is the fastest rotation we have observed to date,” Devogele remarked.

Asteroids rotate for various reasons, including early-life collisions. In general, a space rock larger than one kilometer cannot rotate more than once every 2.2 hours, as it would disintegrate. However, smaller asteroids like 2024 BX1 are more resilient and can withstand much faster rotations. “They have internal strength, allowing them to rotate at higher speeds,” Devogele explained.

Measuring the rotation of such objects could be beneficial for planetary defense, providing insights into the durability of small asteroids and their likelihood of surviving passage through Earth’s atmosphere. “If you have hard snow, it will react differently than if you have snow with no internal strength,” Devogele stated.

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Source: www.newscientist.com

454 new asteroids discovered in the main asteroid belt by astronomers

632 main-belt asteroids (178 known objects and 454 unknown objects) have been identified in archival images from the NASA/ESA Hubble Space Telescope. Citizen scientists from around the world contributed to the discovery of this asteroid. Professional astronomers identified the asteroid using a combination of volunteer efforts and machine learning algorithms.

This Hubble image of barred spiral galaxy UGC 12158 looks like someone took it with a white marking pen. In reality, this is a combination of long exposures of a foreground asteroid moving within Hubble's field of view, adding light bombardment to observations of the galaxy. The galaxy was photographed several times. The dashed pattern is proof of this. Due to parallax, the asteroid appears as a curved trajectory. Hubble is not stationary, but orbits around the Earth, giving the illusion of a faint asteroid swimming along a curved trajectory. This unknown asteroid is located inside the solar system's asteroid belt, so it is 10 trillion times closer to Hubble than the background galaxy. Image credits: NASA / ESA / Hubble / Pablo García Martín, UAM / Joseph DePasquale, STScI / Alex Filippenko, University of California, Berkeley.

More than 4 billion years ago, the eight major planets around the sun formed by sweeping up debris from the vast disk of dust and gas surrounding the sun.

This is common in the birth process of planets, and the NASA/ESA Hubble Space Telescope has for the first time optically observed a similar disk surrounding a newborn star, providing a glimpse into the solar system's formative years.

Four billion years later, debris still litters the planet's construction yards.

Most of this ancient space debris, or asteroids, lies between the orbits of Mars and Jupiter within the main asteroid belt.

“We are starting to learn more about the presence of a small number of main-belt asteroids,” said Dr. Pablo García Martín, an astronomer at the Autonomous University of Madrid.

“We were surprised to see so many candidate objects.”

“We've had some hints that this population exists, but we're now confirming it with a random asteroid population sample obtained using the entire Hubble archive.”

“This is important for gaining insight into models of the evolution of the solar system.”

Since Hubble orbits around the Earth at high speed, Hubble exposure allows us to follow its trail and capture a wandering asteroid.

When viewed from a telescope on Earth, the asteroid leaves streaks across the photo.

The asteroid appears as an unmistakable curved trajectory in the photo, making the Hubble exposure a “photobomb.”

Hubble observes the asteroid from different perspectives as it moves around Earth, but the asteroid also moves along its own orbit.

By knowing Hubble's position during observations and measuring the curvature of its stripes, scientists can determine the distance to the asteroid and estimate the shape of its orbit.

Most of the asteroids involved are in the main belt between the orbits of Mars and Jupiter.

Their brightness is measured by Hubble's sensitive camera. Then, by comparing its brightness and distance, we can estimate its size.

The faintest asteroid found in the survey is approximately 40 million times less bright than the faintest star visible to the human eye.

“Because the asteroid's position changes over time, you can't find the asteroid's location just by entering the coordinates, because the asteroid may not be there at a different time,” Melin said.

“As astronomers, we don't have time to study images of every asteroid.”

“So we came up with the idea of ​​collaborating with more than 10,000 citizen science volunteers to browse the massive Hubble archive.”

of result appear in the diary astronomy and astrophysics.

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Pablo Garcia-Martin other. 2024. Hubble Asteroid Hunter III. Physical properties of newly discovered asteroids. A&A 683, A122; doi: 10.1051/0004-6361/202346771

Source: www.sci.news

NASA’s DART mission may have reshaped the asteroid moon Dimorphos

On September 26, 2022, NASA’s Double Asteroid Redirection Test (DART) mission successfully impacted Dimorphos, the natural satellite of the near-Earth binary asteroid Didymos. New numerical simulations show that the DART impact triggered global deformation and resurfacing of Dimorphos.

The asteroid moon Dimorphos was seen by NASA’s DART spacecraft 11 seconds before impact. His DRACO imager aboard DART captured this image from a distance of 68 km (42 miles). This image was the last one to include all dimorphos in the field of view. Image credit: NASA/Hopkins Applied Physics Laboratory.

DART was a planetary defense mission that demonstrated the possibility of using kinetic impactors to alter the orbits of asteroids.

The collision was successful and highly effective, resulting in Dimorphos’ orbital period around Didymus being shortened from its original 11 hours and 55 minutes to 33 minutes.

The LICIACube Unit Key Explorer (LUKE) instrument aboard the cubesat took images of the system between 29 seconds and 320 seconds after impact, showing the ejecta stream and other debris that spread for several kilometers from the impact site. revealed a complex pattern.

Furthermore, the dramatic brightening of the Didymos system due to solar illumination of the ejected impact ejecta was observed by ground-based and space-based telescopes for many weeks after the impact.

These three Hubble images capture the breakup of Dimorphos when it was intentionally collided by DART on September 26, 2022. The top panel, taken two hours after impact, shows the ejecta cone (estimated at 1,000 tons of dust). The center frame shows dynamic interactions within the Didymos-Dimorphos binary system that begin to distort the cone of ejecta patterns approximately 17 hours after impact. The most notable structure is a rotating windmill-shaped feature. The windmill is connected to Didymus’s gravitational pull. In the bottom frame, Hubble captures debris being pushed back into the comet-like tail by the pressure of sunlight on tiny dust particles. This spreads out into a column of debris, with the lightest particles traveling fastest and furthest away from the asteroid. The mystery deepens after Hubble recorded the tail splitting into two for several days. Image credit: NASA/ESA/STScI/Jian-Yang Li, PSI/Joseph DePasquale, STScI.

In a new study, University of Bern scientist Sabina Raducan and colleagues use realistic constraints on the mechanical and compositional properties of dimorphos, informed by DART’s initial results, to create a state-of-the-art impact The DART impact was modeled using physical code.

The simulations that best match observations of the impact suggest that Dimorphos is weakly cohesive, similar to asteroids Bennu and Ryugu, and lacks large rocks on its surface.

The researchers suggest that Dimorphos may be a pile of debris formed by the rotational shedding and re-accumulation of material ejected from Didymos.

Their model also suggests that DART’s impact may not have created an impact crater, but instead may have changed the shape of the moon as a whole, a process known as global deformation, which could have been caused by material from within. It also indicates that it may have caused the resurfacing of Dimorphos.

The discovery provides further insight into the formation and characteristics of binary asteroids and could have implications for future exploration, including ESA’s Hera mission and asteroid deflection efforts.

“ESA’s future Hera mission may discover reformed asteroids rather than well-defined craters,” the authors concluded.

their paper It was published in the magazine natural astronomy.

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SD Raducan other. Physical properties of the asteroid Dimorphos obtained from the DART impact. Nat Astron, published online on February 26, 2024. doi: 10.1038/s41550-024-02200-3

Source: www.sci.news

SOFIA’s discovery of molecular water on a seemingly dry asteroid

Astronomers used the FORCAST instrument on NASA's retired Stratospheric Observatory for Infrared Astronomy (SOFIA) to obtain mid-infrared spectra of four S-type (silicate-rich) asteroids: Iris, Partenope, Melpomene, and Massalia. Did. They detected features on two of her asteroids, Iris and Massalia, that could clearly be attributed to water molecules.

Arredondo other. Using his FORCAST instrument at NASA's SOFIA Observatory, he observed four silicate-rich asteroids and found mid-infrared spectral signatures indicating molecular water on two of them, Iris and Massalia. Separated. Image credit: NASA/Carla Thomas/Southwest Research Institute.

“Asteroids are leftovers from the planet-forming process, so their composition varies depending on where in the solar nebula they form,” said Dr. Anisia Arredondo, a planetary researcher at the Southwest Research Institute.

“Of particular interest is the distribution of water on the asteroid, as it may reveal how water was delivered to Earth.”

Anhydrous, or dry, silicate asteroids form close to the Sun, and icy material coalesces farther away.

Understanding the location of asteroids and their composition can help us understand how material within the solar nebula has been distributed and evolved since its formation.

The distribution of water in our solar system provides insight into the distribution of water in other planetary systems, and because water is necessary for all life on Earth, there is potential both within and outside the solar system. You will decide where to look for natural life.

“We detected features on the asteroids Iris and Massalia that are clearly attributable to water molecules,” Arredondo said.

“We are building on the success of the team that discovered water molecules on the moon's sunlit surface.”

“We thought we could use SOFIA to find this spectral feature in other objects.”

Sofia detected water molecules in one of the largest craters in the moon's southern hemisphere.

Previous observations of both the Moon and the asteroid have detected some types of hydrogen, but have not been able to distinguish between water and its chemical cousin hydroxyl.

Scientists found that in the cubic meters of soil spread across the moon's surface, there is approximately the equivalent of a 12-ounce (355 ml) bottle of water trapped chemically bonded to minerals.

“Based on the band intensities of the spectral features, the water abundance on the asteroid matches the water abundance on the sunlit moon,” Arredondo said.

“Similarly, in asteroids, water not only binds to minerals, but also adsorbs to silicates and can become trapped or dissolved in silicate impact glass.”

Data from two fainter asteroids, Partenope and Melpomene, were too noisy to draw definitive conclusions.

The FORCAST instrument appears not to be sensitive enough to detect the spectral signature of water, if it exists.

But with these discoveries, researchers are calling on NASA/ESA/CSA's James Webb Space Telescope to take advantage of its precise optics and superior signal-to-noise ratio to investigate more targets. I am requesting you to do so.

“We conducted initial measurements of two more asteroids with Mr. Webb during Cycle 2,” said Dr. Arredondo.

“We are making another proposal to consider 30 more goals in the next cycle.”

“These studies will improve our understanding of the distribution of water in the solar system.”

of study Published in Planetary Science Journal.

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Anisia Arredondo other. 2024. Molecular H2O is detected on a nominally anhydrous asteroid. planet. Science. J 5, 37; doi: 10.3847/PSJ/ad18b8

Source: www.sci.news

The Hera mission to revisit an asteroid destroyed by NASA is scheduled for 2024

Hera will soon head to the asteroid Dimorphos with CubeSats

ESA/Science Directorate

The European Space Agency (ESA) is sending a mission to find out what happened to an asteroid that NASA collided with in 2022. The Hera mission, scheduled to launch in October, will head to the asteroid Dimorphos, which NASA collided with during the Double Asteroid Redirection Test (DART). Mission.

The purpose of DART was to see if crashing a spacecraft into an asteroid would be a good way to protect Earth if one were to come our way.we know the impact Change the trajectory of Dimorphos The collisions around parent asteroid Didymos shorten each orbit by about 33 minutes, but details are not known about exactly how the collisions affected the asteroid or what happened next. do not have.

“To determine whether the impact left a crater or completely changed the shape of the asteroid, another spacecraft will need to return to the crime scene, because with the current data, either scenario is possible. That's why,” says Hera Mission Director. patrick michel At the Côte d'Azur Observatory in France. “Hera is a detective who will thoroughly investigate the effects.”

The mission consists of a main spacecraft that will fly up to 1 kilometer to Dimorphos, and two smaller cube-shaped satellites that are intended to land on the surface and see it up close. This research will not only be crucial for simulating potentially dangerous asteroids and how to deflect them in the future, but will also provide important scientific insights.

“Collisions have played an important role in the entire history of the solar system. We started the growth of planets through collisions, and all solid surfaces are full of impact craters,” Michel says. “If we're going to build a complete model of the solar system's collision history, we need to understand how these collisions work.” And it helps clarify how those conflicts work for us.

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Source: www.newscientist.com

National Laboratory Simulates Core Deflection of Armageddon-Type Asteroid

Last year’s successful double asteroid redirection experiment, which involved firing a satellite bomb into an asteroid, has been followed by a detailed simulation of a nuclear deflection scenario, similar to the plot of the 1998 space disaster movie Armageddon.

Researchers at Lawrence Livermore National Laboratory, led by Mary Varkey, have published a paper advancing the active field of research on planetary defense against asteroid threats. They propose that detonating a nuclear explosive device as close as possible to an incoming asteroid may be the best strategy, considering that using satellites as missiles is not always practical.

The challenge, however, lies in precisely deflecting the asteroid’s nucleus to avoid potential impact with Earth, as depicted in the movie Armageddon, or the widespread destruction scenario depicted in the film Deep Impact.

In their paper published in the Planetary Science Journal, Burkey et al. explain the complexities involved in simulating the energy storage and the interaction of X-rays from a nuclear explosion with the asteroid’s surface, emphasizing the high computational cost and the need to break down the problem into stages for accurate modeling.

The team’s efforts have resulted in a comprehensive simulation of the nuclear deflection scenario, offering insight into the potential outcomes of such an event. The team also highlights the need for faster simulations, potentially utilizing machine learning to optimize response times for specific threats.

Image credits: Varkey et al.

By simulating the nuclear deflection scenario, the team aims to further advance the understanding of potential strategies for planetary defense against asteroid threats and minimize response times for future events.

Source: techcrunch.com

Lucy spacecraft makes a new asteroid discovery, finding another one beyond asteroid Dinkinesh

Asteroid Dinkinesh and its orbiting asteroids

NASA/Goddard/SwRI/Johns Hopkins University APL/NOAO

NASA’s Lucy spacecraft passed the first asteroid and discovered a second asteroid at the same time. Lucy passed the small asteroid Dinkinesh on November 1, and images sent back to Earth show that Dinkinesh has an even smaller space rock orbiting it, the smallest main-belt asteroid ever observed up close. It became clear that there was.

This finding was not entirely surprising. As Lucy approached Dinkinesh over the past few weeks, the asteroid’s brightness appeared to oscillate over time, often indicating the presence of some type of satellite. But Dinkinesh’s diameter is only about 790 meters (790 meters), making it impossible to spot the satellite from Earth, and until November 1, even spacecraft were too far away to see it clearly.

During a flyby on November 1, Lucy flew just 430 kilometers (430 kilometers) from Dinkinesh at speeds of about 16,000 kilometers per hour, taking photos as it passed. These photos reveal a second, smaller asteroid in the Dinkinesh binary, this one only about 220 meters in diameter.

“We knew this would be the smallest main-belt asteroid ever seen up close.” Keith Knoll at NASA’s Goddard Space Flight Center in Maryland. statement. “The fact that it’s two makes it even more exciting. In some ways, these asteroids are similar to near-Earth asteroids. Binary Didymus and Dimorpho [NASA’s Double Asteroid Redirection Test mission] However, there are some very interesting differences that we will explore further. ”

The main purpose of the flyby was to test Lucy’s scientific equipment, especially the system that keeps it on target as it passes by at high speed, and the fact that nothing is visible in these first images suggests that the tracking system is not properly aligned. It shows that it is functioning. The remaining data from the encounter will be transmitted to Earth over the next week or so for more thorough examination by the mission’s scientists and engineers.

Now that Lucy has passed Dinkinesh and its partner asteroid, its next target is asteroid 52246 Donald Johansson, where it plans to visit in 2025 before accelerating toward Jupiter’s Trojan asteroids. The Trojan horse travels in front of and behind Jupiter as it orbits around the sun, and because it is likely a remnant left over from the formation of the solar system, it provides valuable insight into how the planet formed and evolved over time. May hold insights. Lucy she will reach the Trojans in 2027.

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Source: www.newscientist.com