Connect with us

Published

on

There are hundreds of millions of asteroids in our solar system, which means new asteroids are discovered quite frequently. It also means close encounters between asteroids and Earth are fairly common. Some of these close encounters end up with the asteroid impacting Earth, occasionally with severe consequences.

A recently discovered asteroid, named 2023 BU, has made the news because today it passed very close to Earth.

Discovered on January 21 by amateur astronomer Gennadiy Borisov in Crimea, 2023 BU passed only about 3,600 km from the surface of Earth (near the southern tip of South America) six days later on January 27.

That distance is just slightly farther than the distance between Perth and Sydney and is only about 1 percent of the distance between Earth and our Moon.

The asteroid also passed through the region of space that contains a significant proportion of the human-made satellites orbiting Earth.

All this makes 2023 BU the fourth-closest known asteroid encounter with Earth, ignoring those that have impacted the planet or our atmosphere.

How does 2023 BU rate as an asteroid and a threat? 2023 BU is unremarkable, other than that it passed so close to Earth. The diameter of the asteroid is estimated to be just 4–8m, which is on the small end of the range of asteroid sizes.

There are likely hundreds of millions of such objects in our solar system, and it is possible 2023 BU has come close to Earth many times before over the millennia. Until now, we have been oblivious to the fact.

In context, on average a 4-metre-diameter asteroid will impact Earth every year and an 8-metre-diameter asteroid every five years or so Asteroids of this size pose little risk to life on Earth when they hit because they largely break up in the atmosphere. They produce spectacular fireballs, and some of the asteroids may make it to the ground as meteorites.

Now that 2023 BU has been discovered, its orbit around the Sun can be estimated and future visits to Earth predicted. It is estimated there is a 1 in 10,000 chance 2023 BU will impact Earth sometime between 2077 and 2123.

So, we have little to fear from 2023 BU or any of the many millions of similar objects in the Solar System.

Asteroids need to be greater than 25m in diameter to pose any significant risk to life in a collision with Earth; to challenge the existence of civilisation, they’d need to be at least a kilometre in diameter.

It is estimated there are fewer than 1,000 such asteroids in the Solar System and could impact Earth every 5,00,000 years. We know about more than 95 per cent of these objects.

Will there be more close asteroid passes? 2023 BU was the fourth closest pass by an asteroid ever recorded. The three closer passes were by very small asteroids discovered in 2020 and 2021 (2021 UA, 2020 QG and 2020 VT).

Asteroid 2023 BU and countless other asteroids have passed very close to Earth during the nearly five billion years of the Solar System’s existence, and this situation will continue into the future.

What has changed in recent years is our ability to detect asteroids of this size, such that any threats can be characterised. That an object roughly 5m in size can be detected many thousands of kilometres away by a very dedicated amateur astronomer shows that the technology for making significant astronomical discoveries is within reach of the general public. This is very exciting.

Amateurs and professionals can together continue to discover and categorise objects, so threat analyses can be done. Another very exciting recent development came last year, by the Double Asteroid Redirection Test (DART) mission, which successfully collided a spacecraft into an asteroid and changed its direction.

DART makes plausible the concept of redirecting an asteroid away from a collision course with Earth if a threat analysis identifies a serious risk with enough warning.


Affiliate links may be automatically generated – see our ethics statement for details.

Continue Reading

Science

Amateur Astronomer Discovers Unexpected Composition of Jupiter’s Clouds

Published

on

By

Amateur Astronomer Discovers Unexpected Composition of Jupiter’s Clouds

Jupiter’s atmospheric composition has been called into question through observations made using an old technique by an amateur astronomer, Steve Hill. The findings have indicated that the planet’s iconic swirling clouds may not be composed of ammonia ice, as previously assumed. This revelation stems from data collected with commercial telescopes and spectral filters, presenting new perspectives on the gas giant’s atmospheric dynamics and chemistry. The observations have sparked further investigation into the structure of Jupiter‘s cloud layers.

Findings from Observational Studies

According to research published in Earth and Space Science, Hill applied a method known as band-depth analysis. This technique measures light absorption at specific wavelengths to map the abundance of gases like ammonia and methane in Jupiter’s atmosphere. As reported by space.com, the data revealed that reflective cloud layers are located at pressure levels of 2-3 bar, far deeper than where ammonia ice was expected to condense at 0.7 bar.

Patrick Irwin, a planetary physicist at the University of Oxford, reviewed Hill’s results and confirmed their accuracy through comparisons with data from instruments such as NASA’s Juno spacecraft and ESO’s Very Large Telescope (VLT). He noted to space.com that the main reflection appears to stem from ammonium hydrosulfide clouds or photochemical products, rather than pure ammonia ice.

Implications and Future Research

Reports indicate that these findings underline the role of photochemistry in shaping Jupiter’s atmosphere, where ammonia is often destroyed faster than it can rise to the upper layers. Similar processes have been observed on Saturn, where cloud layers are also deeper than predicted. Researchers aim to refine models by integrating additional data from the VLT, Juno, and other observatories to better understand ammonia’s vertical distribution.

Hill’s approach demonstrates the potential of collaborative efforts between amateur and professional astronomers. These findings not only challenge existing models but also open new pathways for studying atmospheric dynamics on gas giants.

Catch the latest from the Consumer Electronics Show on Gadgets 360, at our CES 2025 hub.

Continue Reading

Science

Blue Origin Delays New Glenn Launch to January 12 Due to Adverse Weather in Atlantic

Published

on

By

Blue Origin Delays New Glenn Launch to January 12 Due to Adverse Weather in Atlantic

The launch of Blue Origin’s highly anticipated New Glenn rocket has been delayed due to adverse weather conditions. Initially planned for Friday, January 10, the liftoff was rescheduled to Sunday, January 12, at 1:00 a.m. EST (0600 GMT). This decision was taken because rough seas in the Atlantic Ocean could jeopardise the landing of the rocket’s reusable first stage. The launch will proceed from the Cape Canaveral Space Force Station in Florida, with the same three-hour launch window.

Weather Challenges Force Delay

According to a statement by Blue Origin, as reported by Space.com, the high sea state in the Atlantic presented risks to the landing operation of the rocket booster, which is designed to return to Earth and land on a barge named Jacklyn. Named after Jeff Bezos’ mother, the barge is critical to the company’s plans to achieve reusability. Blue Origin acknowledged the ambitious nature of attempting a first-time booster landing, emphasising their determination to succeed despite the challenges.

Technical Details of New Glenn

Standing at an impressive height of 320 feet (98 meters), the New Glenn rocket marks Blue Origin’s entry into orbital-class missions. It is equipped with a reusable first stage that is intended to endure at least 25 flights, reducing the cost of space missions. This design mirrors the reusable model successfully employed by rival company SpaceX, which regularly recovers its Falcon 9 and Falcon Heavy boosters for reuse.

Future Missions and Contracts

Blue Origin has already secured several contracts for its New Glenn rocket. Among them are NASA’s ESCAPADE mission to Mars and the deployment of Amazon’s Kuiper internet satellites. If the launch does not proceed on Sunday, notices from the Federal Aviation Administration indicate that the company may attempt additional launches through January 16.

The mission represents a significant step for Blue Origin in advancing reusable space technology, with the industry closely monitoring the outcome of its maiden voyage.

Catch the latest from the Consumer Electronics Show on Gadgets 360, at our CES 2025 hub.

Continue Reading

Science

New Link Found Between Ferroelectric Domain Walls and Superconductivity in 2D Materials

Published

on

By

New Link Found Between Ferroelectric Domain Walls and Superconductivity in 2D Materials

Scientists have discovered a unique link between ferroelectric domain walls and superconductivity in two-dimensional van der Waals materials. This breakthrough, credited to research by Gaurav Chaudhary from the University of Cambridge and Ivar Martin from Argonne National Laboratory, sheds light on how specific structural features in these materials enable strong electron interactions. The findings are expected to pave the way for new superconducting devices and innovative applications in the field of condensed matter physics.

Sliding Ferroelectricity and Polarisation Reversal

According to reports by phys.org, sliding ferroelectricity in certain 2D van der Waals materials, including boron nitride and transition metal dichalcogenides (TMDs), facilitates polarisation reversal under moderate electric fields. This phenomenon allows for large-scale manipulation of layer stacking, significantly impacting the material’s electronic properties. Researchers noted that domain walls—boundaries separating regions with differing orientations of ferroelectric polarisation—exhibit unique characteristics that enhance electron-phonon coupling.

Superconductivity Observed at Domain Walls

The study revealed that in materials like molybdenum ditelluride (MoTe₂), superconductivity is transiently enhanced near ferroelectric reversal transitions. This enhancement occurs within hysteresis loops where domains of varying polarisation coexist. The dynamic fluctuations in domain walls were identified as the driving mechanism for the pairing interactions required for superconductivity. It was highlighted that these conditions are exclusive to 2D TMDs, which support interlayer ferroelectricity while remaining conductive within their planes.

Future Research and Applications

Chaudhary and Martin indicated to phys.org that their findings hold potential for developing highly controllable superconducting devices. Efforts are underway to explore the systematic design of new superconductors by layering polar materials and leveraging domain wall networks in moiré systems. They also emphasised the need for further investigations to validate their theoretical models using advanced microscopic simulations.
The study has generated interest among scientists aiming to uncover unconventional mechanisms of superconductivity, marking an important step forward in understanding and utilising the properties of 2D materials.

Catch the latest from the Consumer Electronics Show on Gadgets 360, at our CES 2025 hub.


Blinkit Announces 10-Minute Delivery of Laptops, Monitors and Printers in These Cities



New Cartilage Type Found: Lipocartilage Resembles Fat, Boosts Elasticity

Related Stories

Continue Reading

Trending