Hubble Space Telescope Captures a Mesmerizing Spiral Galaxy Spin

The NASA/ESA Hubble Space Telescope has captured a stunning image of the Barred Spiral Galaxy NGC 3285b.



This Hubble image reveals NGC 3285B, a spiral galaxy approximately 137 million light years away in the Hydra constellation. The color images were generated from separate exposures in the ultraviolet and infrared regions using Hubble’s Wide Field Camera 3 (WFC3), based on data collected through seven filters. Image credits: NASA/ESA/Hubble/RJ Foley, UC Santa Cruz.

NGC 3285b is situated around 137 million light years from the Hydra constellation.

It is also referred to as Leda 31293, ESO 501-18, or IRAS 10322-2723, with a diameter of 100,000 light years.

NGC 3285B boasts a disc and multiple swirling arms, characterized by a large, bright, golden nucleus, while its spiral arms exhibit a light, faint reddish hue.

It is part of the NGC 3312 Galaxy Group (LGG 210) and is a member of the Hydra I Galaxy Cluster.

“NGC 3285B is a component of the Hydra I Cluster, one of the largest galactic clusters in the nearby universe,” stated Hubble astronomers.

“Galactic clusters consist of hundreds to thousands of galaxies held together by gravity.”

“The Hydra I cluster is centered around two massive elliptical galaxies.”

“Each of these galaxies spans about 150,000 light years, roughly 50% larger than our Milky Way.”

NGC 3285B lies on the outskirts of the Hydra I cluster, distanced from the colossal central galaxy.

“This galaxy captured Hubble’s interest as it hosted a Type Ia supernova in 2023,” the astronomer noted.

“Type Ia supernovae produce a condensed star core known as white dwarf explosives, igniting a sudden fusion burst approximately five billion times brighter than the sun.”

The supernova, labeled SN 2023XQM, appears as a blue dot on the far left side of the galaxy’s disc.

“Hubble observed NGC 3285B as part of a campaign focused on Type Ia supernovae.”

“We aim to address the effects of distance and dust by examining each of these supernovae in ultraviolet, optical, and near-infrared light.”

“This initiative will enhance cosmic distance measurements that depend on observations of Type Ia supernovae.”

Source: www.sci.news

VLBA uncovers groundbreaking information on the magnetars with the fastest spin rates

Swift J1818.0-1617 is located about 22,000 light-years away in the constellation Sagittarius.



Artist's impression of magnetar Swift J1818.0-1617. Image courtesy of NSF/AUI/NRAO/S. Dagnello.

Swift J1818.0-1617, discovered in 2020, rotates with a rotation period of 1.36 seconds and is thought to be the fastest rotating magnetar yet discovered.

The star is located on the opposite side of the Milky Way galaxy's bulge, 22,000 light-years away, making it relatively close to Earth.

In fact, it's so close that we can use parallax to pinpoint its 3D location within the galaxy.

The lifespan of magnetars is currently unknown, but astronomers estimate that Swift J1818.0-1617 is only a few hundred years old.

“A magnetar's bright X-ray emission requires a mechanism of extremely high-energy outflow. Only the rapid decay of its powerful magnetic field can explain the force behind these spectral features,” said Dr. Hao Ding, an astronomer at the National Astronomical Observatory of Japan, and his colleagues.

“But again, this is an extreme process: for normal stars on the main sequence, bright blue stars burn through their fuel much faster than yellow stars, and therefore have very short lifetimes.”

“In the case of magnetars, although the physics are different, their lifetimes are also thought to be shorter than those of pulsars.”

“Magnetars are too young to continue releasing energy at this rate for long periods of time,” the researchers added.

“Moreover, magnetars can also exhibit radiation in the lower end of the electromagnetic spectrum, i.e. at radio wavelengths.”

“In these cases, the most likely energy source is synchrotron radiation produced by the magnetar's rapid rotation.”

“In synchrotron radiation, the plasma surrounding the neutron star itself is so tightly attached to the surface of the star that it rotates at very close to the speed of light and produces radiation at radio wavelengths.”

Astronomers NSF's Very Long Baseline Array (VLBA) was conducted over a three-year period to collect data on the position and velocity of Swift J1818.0-1617.

“The VLBA provided excellent angular resolution to measure this extremely small disparity, and the spatial resolution is unmatched,” said Dr Ding.

Swift J1818.0-1617's parallax is the smallest of any neutron star, and its so-called transverse velocity is the smallest of any magnetar (a new lower limit).

“Velocity in astronomy can be most simply described as having two components: direction and velocity,” the researchers explained.

“Radial velocity tells us how fast we're moving along the line of sight. In this case, radial velocity means the speed along the radius of the galaxy.”

“For magnetars like Swift J1818.0-1617, which are located on the opposite side of the central bulge, there is too much other material in the way to accurately measure the radial velocity.”

“Transverse velocity, sometimes called proper velocity, describes motion perpendicular to the galactic plane and is more easily identifiable.”

Astronomers are trying to understand the common (and different) formation processes between regular neutron stars, pulsars and magnetars, and hope to use precise measurements of the transverse velocities to analyse the conditions under which stars evolve along one of these three paths.

“This study adds weight to the theory that magnetars are unlikely to form under the same conditions as young pulsars, and suggests that magnetars are born from a more unconventional formation process,” Dr Ding said.

“We need to know how fast magnetars were moving when they were first born. The mechanism by which magnetars form is still a mystery, and we want to find out.”

Source: www.sci.news

Physicists successfully transfer electron spin to photon

A team of physicists led by Dr. Yuan Lu of the Jean Lamour Institute at the University of Lorraine used electrical pulses to manipulate magnetic information into polarized signals. This discovery could revolutionize long-distance optical communications, including between Earth and Mars. This breakthrough involves the field of spintronics, which aims to manipulate the spin of electrons to store and process information.

Structure of SOT Spin LED: Control of emission intensity and charging current is the basis of information transfer and processing. In contrast, robust information storage and magnetic random access memory are implemented using carrier spins and their associated magnetizations in ferromagnets. The missing link between the respective fields of photonics, electronics, and spintronics is modulating the circular polarization of emitted light rather than its intensity through electrically controlled magnetization.Dynon other. demonstrated that this missing link is established in light-emitting diodes at room temperature in the absence of an applied magnetic field through the transfer of angular momentum between photons, electrons, and ferromagnets.Image credit: Dynon other., doi: 10.1038/s41586-024-07125-5.

Spintronics has been successfully used in magnetic computer hard drives, where information is represented by the direction of electron spin and its proxy, magnetization.

Ferromagnetic materials such as iron and cobalt have an unequal number of electrons, with their spins oriented either along or against the magnetization axis.

Electrons with spins aligned with the magnetization move smoothly in a ferromagnetic material, while electrons with spins in the opposite direction bounce. This represents binary information of 0’s and 1’s.

The resulting change in resistance is a key principle in spintronic devices, where magnetic states can be maintained indefinitely, which can be considered stored information.

Just as a refrigerator magnet requires no power to stick to a door, spintronic devices require much less power than traditional electronics.

But like pulling a fish out of water, when an electron is removed from a ferromagnetic material, the spin information is quickly lost and can no longer travel far.

This major limitation can be overcome by utilizing circularly polarized light, also known as helicity, as another spin carrier.

Just as humans used homing pigeons centuries ago to carry written communication farther and faster than on foot, the trick is to transfer the spin of an electron to a photo, a quantum of light. That’s probably true.

Such transfer is possible due to the presence of spin-orbit coupling, which causes spin information loss outside the ferromagnetic material.

The key missing link is to electrically modulate the magnetization and thereby change the helicity of the emitted light.

“The concept of spin LEDs was first proposed at the end of the last century,” Dr. Lu said.

“But to move into practical use, it must meet three important criteria: it must operate at room temperature, it does not require a magnetic field, and it must be able to be electrically controlled.”

“After more than 15 years of dedicated work in this field, our collaborative team has managed to overcome all obstacles.”

In their research, Dr. Lu and his colleagues succeeded in switching the magnetization of a spin injector using an electric pulse that uses spin-orbit torque.

The electron spin is rapidly converted into information contained in the helicity of the emitted photon, allowing seamless integration of magnetization dynamics and photonic technology.

This electrically controlled spin-to-photon conversion is currently realized with electroluminescence in light-emitting diodes.

In the future, through implementation in semiconductor laser diodes, so-called spin lasers, this highly efficient information encoding will pave the way for high-speed communication across interplanetary distances, since the polarization of light is preserved in spatial propagation. It is possible and could potentially make it possible. The fastest mode of communication between Earth and Mars.

It also has significant benefits for the development of a variety of advanced technologies on Earth, including photonic quantum communications and optical computing, neuromorphic computing for artificial intelligence, and ultra-fast and highly efficient optical transmitters for data centers and light-fidelity applications. will bring about.

“The realization of spin-orbit torque spin injectors is a decisive step in the development of ultrafast and energy-efficient spin lasers for next-generation optical communications and quantum technologies,” said Professor Nils Gerhardt of Ruhr University. ” he said.

team's work It was published in the magazine Nature.

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PA Dynon other. 2024. Optical helicity control by electromagnetic switching. Nature 627, 783-788; doi: 10.1038/s41586-024-07125-5

Source: www.sci.news

New Study Reveals the Superfast Spin of the Milky Way’s Supermassive Black Hole

Sagittarius A*, the 4.3 million solar mass black hole at the center of the Milky Way, spins so fast that space-time around it is warped into the shape of a soccer ball, according to an analysis. Data collected by NASA's Chandra X-ray Observatory and NSF's Carl G. Jansky Very Large Array.



daily other. Sagittarius A* was found to be rotating at 60% of its maximum rotational speed, which is set by matter that cannot travel faster than the speed of light. This image shows Sagittarius A* in X-ray light from NASA's Chandra X-ray Observatory. Image credit: NASA / CXC / University of Wisconsin / Bai other.

Black holes have two fundamental properties: mass (weight) and spin (rotational speed).

Determining either of these two values ​​can tell astrophysicists a lot about black holes and their behavior.

Dr. Ruth Daly of Pennsylvania State University and colleagues applied a new method using X-ray and radio data to predict Sagittarius A*'s rotation rate based on how matter moves toward or away from the black hole. Decided.

They discovered that Sagittarius A* rotates at an angular velocity (rotations per second). Its angular velocity is about 60% of its maximum possible value, a limit set by the inability of matter to travel faster than the speed of light.

In the past, different astronomers have used different techniques to estimate the rate of rotation of Sagittarius A*, ranging from not rotating at all to rotating at near maximum speed, with mixed results.

“Our research may help answer the question of how fast our galaxy's supermassive black holes rotate,” said Dr. Daly.

“Our results show that Sagittarius A* is rotating very rapidly, which is interesting and has far-reaching implications.”

A rotating black hole pulls space-time and nearby matter into its surroundings as it rotates. Spacetime around a rotating black hole is also crushed.

If you look down at a black hole from above and follow the barrel of the jet it produces, spacetime is circular.

However, if you look at a rotating black hole from the side, spacetime looks like a soccer ball. The faster the spin, the flatter the football.

The spin of a black hole acts as an important source of energy. When a supermassive black hole rotates, its spin energy can be extracted to produce a parallel outflow, a thin beam of matter such as a jet, but this requires at least some material near the black hole. must exist.

Because of the limited fuel surrounding Sagittarius A*, the black hole has been relatively quiet for the last several thousand years, with a relatively weak jet stream.

But new research shows that this could change as the amount of material increases near Sagittarius A*.

“A collimated jet powered by a galaxy's rotating central black hole could have a significant impact on the galaxy's entire gas supply,” said Michigan State University astronomer Megan Donahue. “This also influences the rate and uniformity with which stars form.”

“Fermi bubbles seen in X-rays and gamma rays around the Milky Way's black hole indicate that the black hole was probably active in the past. Measuring the black hole's rotation is important in this scenario. It's a test.”

To determine Sagittarius A*'s spin, astronomers looked at the black hole's spin and its mass, the nature of the matter near the black hole, and its outflow properties.

The parallel outflow produces radio waves, and the disk of gas surrounding the black hole is responsible for emitting X-rays.

Using this method, the researchers combined data from NASA's Chandra X-ray Observatory and NSF's Carl G. Jansky Very Large Array with independent estimates of the black hole's mass from other telescopes. to limit the rotation of the black hole.

“Sagittarius A* offers a special perspective because it is the closest supermassive black hole to us,” said Dr. Anand Lu, an astronomer at McGill University.

“Although it is quiet now, our research shows that in the future it will have an incredibly powerful impact on the matter around it.”

“It could happen in a thousand or million years, or it could happen in our lifetime.”

of study Published in Royal Astronomical Society Monthly Notices.

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Ruth A. Daly et al. 2024. New black hole spin values ​​for Sagittarius A* obtained using the outflow method. MNRAS 527 (1): 428-436; doi: 10.1093/mnras/stad3228

Source: www.sci.news

EthSign Introduces DocuSign-like Features to Line and Telegram with a Web3 Spin

Despite the continued regulatory crackdown on the cryptocurrency industry and the collapse of some of its leading figures, the underlying decentralized technology continues to push internet incumbents into the Web3 realm.

Telegram and Line are two of the world’s most popular messengers with hundreds of millions of monthly users, and both have integrated encryption features in recent months. One of the features being introduced in these apps is electronic signatures provided by a startup called EthSign.

Backed by all three Sequoia divisions: Sequoia Capital, Sequoia Capital India, and Sequoia Capital China (now called HongShan), Singapore-based EthSign promises an additional layer of transparency and trust. We aim to provide the Web3 equivalent of DocuSign. Therefore, its task is to convince the public that signing contracts on the blockchain is better than traditional methods.

“First, it is much easier to authenticate the identity of each signer and see the history of their interaction with the signed document,” said EthSign, who previously worked in the strategic investment department of a centralized exchange. Co-founder and CEO Xin Yan explained. Huobi.

If traditional e-signature service providers shut down, records of users’ signatures would also be lost, but this is an issue unrelated to distributed ledger technology, Yang told TechCrunch. And once signed, the data is immutable. This is one of the most promising features of blockchain.

EthSign will be deployed on the respective blockchain networks running on Telegram and Line, TON and Finschia. Once a user connects his cryptocurrency wallet to Messenger, he can start signing documents through EthSign in the same way he interfaces with DocuSign.

EthSign is one of many Web3 projects built on Telegram’s blockchain partner TON, helping the messenger work towards its vision of becoming a super app like WeChat.

EthSign, which is already running on Line as a web app, has signed a memorandum of understanding with Finschia for further integration in the coming months.

The idea of ​​enabling immutable signatures in messaging apps is not new. Back in 2018, a mini-app called “Little Protocol” was launched on Chinese messaging giant WeChat. The feature, which allows users to enter into contracts using their girlfriend’s WeChat ID and the contents of documents recorded on Ethereum, attracted more than 100,000 hits for her overnight. However, within 48 hours, the app was removed by WeChat.

To date, EthSign has connected approximately 250,000 unique wallet addresses. Although still free to use, its goal is to become an authentication services platform in the future, providing support for authentication, verification, and other user activities, rather than pursuing a traditional SaaS model that monetizes through subscription fees. It’s about charging.

“Certification of on-chain information is about bringing trust to the on-chain world, where the most promising use case is vampire attacks,” Yang explained, adding that users can use established cryptocurrencies to He mentioned the phenomenon of Web3 being directed to forked versions. Projects with enhanced incentives.

Source: techcrunch.com