Gemini North Telescope Unveils New Images of 3I/ATLAS

On November 26, 2025, astronomers utilized the Gemini Multi-Object Spectrograph (GMOS) on the Gemini North Telescope located on Mauna Kea, Hawaii, to capture images of the interstellar comet 3I/ATLAS. Recent observations demonstrate how this comet has evolved since its closest approach to the Sun.

This image, taken with GMOS on the Gemini North Telescope, depicts 3I/ATLAS traveling among stars and galaxies. Operating as part of the International Gemini Observatory, it is funded in part by NSF and managed by NSF’s NOIRLab. Image credit: International Gemini Observatory / NOIRLab / NSF / AURA / B. Bolin / J. Miller & M. Rodriguez, International Gemini Observatory & NSF’s NOIRLab / TA Rector, University of Alaska Anchorage & NSF’s NOIRLab / M. Zamani, NSF’s NOIRLab.

3I/ATLAS reached its closest approach to the Sun, termed perihelion, on October 30, 2025.

Having emerged from behind the Sun, this interstellar body was observed near Zania, a triple star system situated in the Virgo constellation.

On November 26, 2025, researcher Bryce Bolin from Eureka Scientific, along with colleagues, obtained new images of the comet as part of a public outreach initiative by NSF NOIRLab in partnership with Shadow the Scientist.

“Providing the public with a viewing experience under optimal conditions allows for a genuine front-row glimpse of interstellar visitors,” Dr. Bolin stated.

“Offering the public insight into our work as astronomers and our methodologies also serves to demystify science and the data collection process, enhancing transparency in the study of this captivating astronomical entity.”

The 3I/ATLAS image, captured using GMOS, highlights the comet’s coma—a cloud of gas and dust that forms around its icy center when approaching the Sun. Image credit: International Gemini Observatory / NOIRLab / NSF / AURA / B. Bolin / J. Miller & M. Rodriguez, International Gemini Observatory & NSF’s NOIRLab / TA Rector, University of Alaska Anchorage & NSF’s NOIRLab / M. Zamani, NSF’s NOIRLab.

The recent GMOS image comprises exposures taken through four different filters: blue, green, orange, and red.

“During the exposure, the comet remains stationary in the center of the telescope’s field of view,” the astronomers explained.

“However, the background stars shift in relation to the comet, creating colorful streaks in the final image.”

“Initial images of the comet from the Shadow the Scientist session at Gemini South, Chile, exhibited a red hue.”

“In contrast, the new images released today display a subtle greenish glow.”

“This phenomenon results from light emitted by gases in the comet’s coma containing diatomic carbon, a reactive molecule made of two carbon atoms that emits light at green wavelengths. This gas evaporates as the comet heats up.”

“What remains uncertain is how comets behave as they move away from the Sun and cool down.”

“Many comets respond slowly to the Sun’s heat, as it takes time for the warmth to penetrate the comet’s interior.”

“Such delays could accelerate the evaporation of new compounds or potentially lead to the comet’s disintegration.”

Source: www.sci.news

Gemini South Telescope Shines Light on the Butterfly Nebula

In celebration of the 25th anniversary of the International Gemini Observatory’s completion, students in Chile chose the Gemini South Telescope to capture an image of NGC 6302, also known as the Bug Nebula or Butterfly Nebula (Caldwell 69).

This image captured by the Gemini South Telescope showcases the planetary nebula NGC 6302. Image credit: International Gemini Observatory / NOIRLab / NSF / AURA / J. Miller & M. Rodriguez, International Gemini Observatory & NSF’s NOIRLab / TA Rector, University of Alaska Anchorage & NSF’s NOIRLab / M. Zamani, NSF’s NOIRLab.

NGC 6302 is a planetary nebula situated 2,417 light-years away in the constellation Scorpius.

“Planetary nebulae are a type of emission nebula formed by a massive star at the end of its lifecycle, shedding material and surrounded by an expanding, glowing shell of ionized gas,” stated astronomers at the International Gemini Observatory.

“These intriguing structures usually have a circular, planet-like appearance, which is how they earned the name ‘planetary nebulae’ from early astronomers who observed them through telescopes.”

While various dates are associated with the discovery of NGC 6302, a 1907 study by American astronomer Edward E. Barnard is commonly credited, though it could have been discovered earlier in 1826 by Scottish astronomer James Dunlop.

This nebula is characterized by an extremely complex dipolar morphology, highly excited gases, elevated molecular weight, and the presence of crystalline silicate dust.

Its butterfly shape extends over two light-years, roughly half the distance from the Sun to Proxima Centauri.

“In recent images obtained from the Gemini South Telescope, the glowing ‘wings’ of the Butterfly Nebula appear to emerge from the interstellar medium,” the astronomers explained.

“This visually stunning object was chosen by Chilean students for the 8.1-meter telescope as part of the Gemini First Light Anniversary Image Contest.”

“This competition engaged students at the Gemini telescope site, honoring the legacy established by the International Gemini Observatory since its first light in November 2000.”

In 2009, astronomers utilized the Wide Field Camera 3 on the NASA/ESA Hubble Space Telescope to identify the central star of NGC 6302 as a white dwarf. This star shed its outer layers over 2,000 years ago and now possesses about two-thirds the mass of the Sun.

It ranks as one of the hottest known stars, with a surface temperature exceeding 250,000 degrees Celsius (450,000 degrees Fahrenheit), indicating it must have formed from a substantially large star.

Further investigation of NGC 6302 uncovers a dramatic formation history.

Before its transformation into a white dwarf, the star was a red giant approximately 1,000 times the diameter of the Sun.

This massive star expelled its outer gas layer, moving outward from the equator at a relatively slow rate, forming a dark donut-shaped band still observable around the star.

Other gases were expelled perpendicular to this band, restricting outflow and creating the bipolar structure visible today.

As the star evolved, it released strong stellar winds that pierced its “wings” at speeds exceeding 3 million kilometers per hour (1.8 million miles per hour).

This combination of slow and fast-moving gases further sculpted the “wings,” revealing a vast terrain of cloudy ridges and pillars.

Now, as a white dwarf, the star emits intense radiation that elevates the temperature of NGC 6302’s “wings” to over 20,000 degrees Celsius (approximately 35,000 degrees Fahrenheit), causing the gas to glow.

“Dark red areas in the image represent regions of energized hydrogen gas, while deep blue spots indicate regions of energized oxygen gas,” the researchers mentioned.

“These materials, alongside other elements like nitrogen, sulfur, and iron discovered in NGC 6302, are critical for forming the next generation of stars and planets.”

Source: www.sci.news

Google’s Gemini 3 Model Keeps AI Buzz Alive – For the Time Being

Gemini 3 is Google’s latest AI model

VCG (via Getty Images)

Google’s newest chatbot, Gemini 3, has shown remarkable advancement on various benchmarks aimed at evaluating AI progress, according to the company. While these accomplishments may mitigate concerns about a potential AI bubble for the time being, it’s uncertain how effectively these scores reflect real-world performance.

Moreover, the ongoing issues of factual inaccuracies and problematic illusions that are often present in large-scale language models remain unaddressed, particularly in scenarios where accuracy is critical.

In a blog post announcing the new model, Google leaders Sundar Pichai, Demis Hassabis, and Koray Kavukcuoglu stated that Gemini 3 possesses “PhD-level reasoning,” a term also used by competitor OpenAI during the release of its GPT-5 model. They presented scores from several assessments aimed at measuring “graduate-level” knowledge, such as Humanity’s Last Exam, comprising 2500 research-oriented questions from fields like mathematics, science, and humanities. Gemini 3 achieved a score of 37.5 percent on this exam, surpassing the previous record held by OpenAI’s GPT-5, which scored 26.5 percent.

Such improvements could indicate that the model has developed enhanced capabilities in certain areas. However, Luc Rocher suggests caution in interpreting these outcomes. “If a model increases its score from 80 percent to 90 percent on a benchmark, what does that represent? Does it mean the model was 80 percent PhD-level and is now 90 percent? This is quite difficult to ascertain,” he remarks. “It’s challenging to quantify whether an AI model demonstrates inference, as that concept is highly subjective.”

Benchmark tests come with numerous limitations, including the requirement for single answers or multiple-choice responses that do not necessitate demonstrating how the model operates. “It’s straightforward to evaluate models using multiple-choice questions,” notes Roche. “Yet in real-world scenarios—like visiting a doctor—you are not assessed with multiple-choice questions. Likewise, a lawyer does not provide legal counsel through pick-and-choose answers.” There’s also the risk that responses to such tests could be included in the training data of the AI models being assessed, essentially allowing for cheating.

The ultimate evaluation of whether Gemini 3 and its advanced AI models justify the massive investments being made by companies like Google and OpenAI in AI data centers hinges on user experience and the perceived trustworthiness of these tools, according to Roscher.

Google asserts that enhancements to the model will assist users in developing software, managing emails, and analyzing documents more effectively. The company also emphasizes that it will enhance Google searches, providing AI-generated results alongside graphics and simulations.

Perhaps the most significant advancement, as articulated by Adam Mahdi from Oxford University, is the autonomous coding capabilities facilitated by AI tools, a technique known as agent coding. “We might be approaching the limits of what traditional chatbots can achieve, and it is here that the true advantages of Gemini 3 Pro come into play. [the standard version of Gemini 3] It’s likely that it won’t be used for everyday conversations, but rather for more intricate and potentially agent-based workflows,” he explains.

Here are some initial reactions online: People admire Gemini’s impressive coding and reasoning skills. However, as is typical with new model releases, some users pointed out failures in seemingly simple tasks like drawing an arrow or a straightforward visual reasoning challenge.

Google recognizes in Gemini 3’s technical specifications that the model continues to experience hallucinations at a rate similar to other major AI models and sometimes disseminates inaccuracies. This lack of progress is a significant concern, according to Artur Davila Garces from City St George’s, University of London. “The challenge lies in the fact that AI companies have been striving to minimize hallucinations for over two years, yet even one severely misleading hallucination can irreparably damage trust in the system,” he warns.

topic:

Source: www.newscientist.com

Google Gemini Upgrade Introduces Autonomous AI for Phones and Watches

Google’s newest Gemini AI update aims to forecast how you can obtain essential information to enhance your photography skills or to function as a tailored health and sleep adviser for addressing various concerns.

The newly announced Pixel 10 features a Magic Cue capability for Android devices that enables chatbots to sift through digital content and present relevant information concerning their phones as needed.

When contacting an airline, your reservation details will automatically appear in the phone app via Gmail. Similarly, if a friend texts about Sunday brunch, Gemini will propose the ideal coffee shop and display your calendar alongside the message.

This capability is part of an array of artificial intelligence enhancements for the latest Pixel 10, 10 Pro, and 10 Pro fold Phones. Each device boasts a new Tensor G5 chip that executes magic cues and additional AI functions locally.

Leo Gebbie, a principal analyst at CCS Insight, observed that Google “effectively utilizes AI on-device more than its competitors,” noting that the Magic Cue feature represents “an initial stride towards a much-anticipated agent AI experience that has been long-promised on smartphones.”

He further stated: “Google can leverage the fact that many Android users already have well-populated apps such as Gmail, Calendar, Maps, and others for personal data. This amalgamates the information in a more practical manner than ever before.”




The Pixel 10 is equipped with a Tensor G5 chip that facilitates magical cues and other AI functionalities locally. Photo: Google

The Pixel 10 features an enhanced imaging system with a 6.3-inch OLED display and a 10.8-megapixel 5x telephoto camera for the first time, evolving from the previous models which had two cameras. The Pixel 10 Pro is available in two sizes, with options for a 6.3-inch or 6.8-inch display, and includes three cameras with a 48MP telephoto lens capable of 10x optical zoom.

The Pixel 10 Pro fold is among the first foldable phones boasting complete IP68 water and dust resistance, akin to standard slab devices, as Google aims to address concerns regarding flexible screen durability. It shares a camera system similar to that of the Pixel 10.

The device also supports multiple AI photography features, including a new camera coach that utilizes Google’s AI server to evaluate the scenes in front of the camera and provide suggestions for improved framing, angles, and lighting.

The Pixel 10 starts at £799 (899 Euros/$799/$1,349), whereas the Pixel 10 Pro begins at £999 (€1,099/$999/$1,699) and will be available from August 28th. The Pixel 10 fold will be priced from £1,749 (€1,899/$1,799/$2,699) and will launch on October 9th.

Pixel Watch 4 and Pixel Bud 2a




The Pixel Watch 4 Smartwatch brings Gemini to your wrist, serving as a personal AI health coach. Photo: Google

Google has also unveiled the Pixel Watch 4 Smartwatch, which integrates Gemini to offer personalized health coaching on your wrist. Utilizing the new Fitbit app, Gemini can devise customized fitness and sleep plans, track training impacts in real-time, and respond to health and fitness inquiries in a chatbot style.

Available in two sizes, the Pixel Watch 4 features a dome-shaped display that is 10% larger than its predecessor. It is the first smartwatch capable of providing SOS satellite-based emergency services in the U.S. when off the grid. This model is also the first designed with maintainability in mind, allowing for easier repair of the battery and screen, aiming to compete with Apple and Samsung in this regard. It starts at £349 (499 Euros/$349/$579).

In addition, the Pixel Buds 2a offers a more affordable option for Google’s compact Bluetooth earphones, priced at £129 (€149/$129/$239). They incorporate the same Tensor A1 chip found in the premium Buds Pro 2, along with noise cancellation and integrated Gemini AI assistants. The Bud 2a charging case is designed with a replaceable battery, although the earphones themselves are not repairable.

Source: www.theguardian.com

Gemini North Telescope Captures Stunning New Images of Interstellar Comet 3I/Atlas

Astronomers utilizing the Gemini North telescope at NSF’s International Gemini Observatory have observed the interstellar comet 3i/Atlas as it passes through our cosmic neighborhood.



This image from the Gemini North Telescope Multi-Object Spectrometer (GMOS-N) showcases the interstellar comet 3i/Atlas. Image credits: International Gemini Observatory/Noirlab/NSF/Aura/K. Meech, Ifa&U. Hawaii / Jen Miller & Mahdi Zamani, Noirlab.

Interstellar objects are those that emerge from and traverse beyond our solar system.

Ranging from several meters to a few kilometers in size, these cosmic fragments are remnants from the formation of the host star’s planetary system.

As they orbit their stars, interactions with the gravitational pull of nearby planets and stars can eject them into interstellar space, allowing them to traverse other solar systems.

Studying interstellar visitors provides critical insights into distant star systems.

They carry valuable information about chemical elements, including their formation timelines and locations, offering scientists glimpses into the formation of planetary systems throughout the history of the Milky Way galaxy.

3i/Atlas marks the third interstellar object discovered, following 1i/Oumuamua in 2017 and 2i/Borisov in 2019.

Astronomers suspect that numerous interstellar objects might regularly pass through our solar system, but capturing them is challenging as they are only visible when telescopes are oriented correctly at the right time.

Multiple teams worldwide utilize various telescopes to monitor 3i/Atlas during its brief visitation, enabling them to collectively assess its key properties.

While many aspects remain unknown, 3i/Atlas is already recognized as distinct in comparison to 1i/Oumuamua and 2i/Borisov.

Previous observations suggest that 3i/Atlas could have a diameter of up to 20 km (12 miles).

New comets typically exhibit highly eccentric orbits, which define how much the object’s path deviates from a perfect circle.

An eccentricity of 0 indicates a circular orbit, while 0.999 signifies a highly elongated ellipse.

Objects with an eccentricity greater than 1 follow paths that do not loop around the Sun and come from, then return to, interstellar space.

The eccentricity of 3i/Atlas is recorded at 6.2, classifying it as a highly hyperbolic interstellar object.

In contrast, “Oumuamua’s” eccentricity was around 1.2, and Borisov’s was about 3.6.

As of now, 3i/Atlas resides in Jupiter’s orbit, approximately 465 million km (290 million miles) from Earth and 600 million km (370 million miles) from the Sun.

On December 19, 2025, it will come within roughly 270 million km (170 million miles) of Earth, posing no threat to our planet.

The closest approach to the Sun will occur around October 30, 2025, at a distance of 210 million km (130 million miles).

During this close approach, it is expected to travel at about 25,000 km (15,500 miles) per hour.

The latest image of 3i/Atlas was obtained using the Gemini North Telescope Multi-Object Spectrometer (GMOS-N).

“The sensitivity and scheduling precision of the International Gemini Observatory played a critical role in observing this interstellar wanderer,” remarked Martin Still, NSF Program Director at the International Gemini Observatory.

“We eagerly anticipate the wealth of new data and insights as this object warms in sunlight before continuing its cold, dark journey through interstellar space.”

Source: www.sci.news

Google Aims to Introduce Gemini AI Chatbots for Kids Under 13

Google is set to introduce the Gemini AI Chatbot next week for children under 13 who have Google accounts, as tech companies vie for the attention of younger users with their AI offerings.

“The Gemini app will soon be available for your kids,” the company informed an 8-year-old’s parent via email this week. “This means your child can use Gemini to ask questions and get assistance in creating stories for homework.”

Chatbots will be available to children using their parents’ Family Links, Google services designed for families to set up Gmail accounts and access services like YouTube for their children. To create a child account, parents need to provide information such as the child’s name and birth date.

Regarding Gemini, Google has established guardrails for young users, ensuring that chatbots do not generate certain unsafe content. Karl Ryan, a Google spokesperson, noted that data from children with Family Link accounts will not be used to train AI.

The rollout of Gemini for children is expected to help educational institutions, businesses, and others in assessing the efficiency of common generative AI technologies, thus broadening the use of chatbots among at-risk populations. These systems, which are trained on vast amounts of data, can produce human-like text and realistic images and videos.

Google and other developers of AI chatbots are fiercely competing to attract younger users. Recently, President Trump encouraged educational institutions to adopt these tools for learning. Millions of teenagers are already utilizing chatbots for learning support, writing guidance, and virtual companionship. However, a group of children has cautioned that chatbots can pose serious safety risks.

UNICEF and various national children’s advocacy groups point out that AI systems can be misleading, distorted, and manipulated, making it challenging for young children to understand that chatbots are not human.

“Generative AI is producing hazardous content,” noted UNICEF’s Global Research Office in a statement about the risks and opportunities posed by AI for children.

In an email to families this week, Google acknowledged some risks, informing parents that “Gemini can make mistakes,” and advised them to “help children think critically” about chatbots.

The email also suggested that parents educate children on how to fact-check the responses from Gemini. The company urged parents to remind kids that “Gemini is not human” and to “avoid sharing sensitive or personal information with Gemini.”

The email emphasized that, despite Google’s attempts to filter inappropriate content, caution is still advised.

This week’s Google Mail to Parents highlighted the risks associated with Gemini for children.

Over the years, Google has rolled out various products, features, and safety measures for children and teens. In 2015, Google launched YouTube Kids, a dedicated app for children that remains popular among families.

Other initiatives aimed at attracting children online have raised concerns from government officials and child advocates. In 2021, Meta abandoned plans for Instagram Kids after a group of state attorneys general sent a letter criticizing the company for historically failing to ensure the safety of children on its platforms.

Several prominent tech companies, including Google, Amazon, and Microsoft, have faced significant fines for violating the Children’s Online Privacy Protection Act. Federal regulations mandate that children under 13 must obtain parental consent before any personal information is collected online.

With the launch of Gemini, children with family-managed Google accounts will soon be able to access the chatbot on their own. However, the company advised parents that they can modify their children’s chatbot settings to “disable access” if needed.

“Your child will soon gain access to the Gemini app,” an email to parents stated. “We will also notify you when your child first uses Gemini.”

Ryan mentioned that Google’s strategy for offering Gemini to younger users adheres to federal regulations concerning children’s online privacy.

Source: www.nytimes.com

Space Flower Spotted by Gemini Telescope in Large Magellan Cloud

Using Gemini South Telescope, NSF's Noirlab astronomers imaged a beautiful nebula around the young open cluster NGC 2040.

The nebula, including the NGC 2040, resembles the vivid roses in this image taken by a Gemini Southeres scope. Image credits: International Gemini Observatory / Neur Love / NSF / Aura / J. Miller & M. Rodriguez, International Gemini Observatory & NSF No Arab/TA Rector, University of Alaska Anchorage & NSF No Arab/NSF No Arab/NSF No Arab, NSF No Arab.

NGC 2040 It is about 160,000 light years away from Earth, the constellation of Dorado.

This cluster, also known as the Cal 60 or ESO 56-164, resides within the large Magellan cloud, a satellite d-star galaxy of the Milky Way.

NGC 2040 is a so-called OB association, usually a stellar group containing stars between 10 and 100 stars O and B.

“O- and B-spectral types of stars live a short life of just millions of years, burning very hot before they explode like supernovae during that time,” Noirlab astronomers said in a statement.

“The energy released by these massive star explosions will be fed into the formation of NGC structures in the 2040s, while the material emitted sowing the growth of the next generation of stars.”

Most of our galaxy stars are thought to have been born in the OB Association, as well as NGC 2040.

“NGC 2040 is part of a large structure of interstellar gas known as LH 88, one of the largest active star-forming regions within the large Magellan cloud,” the astronomer said. Ta.

“Thousands of new stars will be born in the region over the millions of years to come.”

“When stars O and B end their supernovae life, they enrich the clusters with elements like carbon, oxygen and iron,” they said.

“Along with the rich hydrogen in the cluster, these elements provide the components necessary for the formation of new stars, planets, and perhaps life.”

“The bright stars seen in the image are widely separated, but their movements through space are similar, indicating that they have a common origin.”

“The layered ambiguous structure of LH 88 is the remains of an already dead star.”

“The delicate leaves of the rose were formed by both the shock waves of the supernova and the stellar winds of the stars of O and B.”

Source: www.sci.news

Gemini South Telescope zeroes in on unusual lenticular galaxy NGC 4753

NGC 4753’s remarkable and complex network of dust lanes winding around its galactic core defines its “peculiar” classification, and was probably the result of the galaxy’s merger with a nearby dwarf galaxy about 1.3 billion years ago. It is thought that there is.



This image from the Gemini South Telescope, one half of the International Gemini Observatory operated by NSF’s NOIRLab, shows NGC 4753, a lenticular galaxy about 60 million light-years away in the constellation Virgo. Image credits: International Gemini Observatory / NOIRLab / NSF / AURA / J. Miller, International Gemini Observatory and NSF’s NOIRLab / M. Rodriguez, International Gemini Observatory and NSF’s NOIRLab / M. Zamani, NSF’s NOIRLab.

NGC4753 is a lenticular galaxy located approximately 60 million light-years away in the constellation Virgo.

This galaxy, also known as LEDA 43671, UGC 8009, and IRAS 12498-0055, discovered It was proposed by German-born British astronomer William Herschel on February 22, 1784.

NGC 4753 is a member of the NGC 4753 group of galaxies in the Virgo II cloud, a series of at least 100 galaxy clusters and individual galaxies that extend away from the southern edge of the Virgo Supercluster.

“There is an astonishing number of galaxies in the observable universe, with recent estimates putting the number between 100 billion and 2 trillion,” Gemini astronomers said in a statement.

“And just like snowflakes, no two are exactly alike. However, they can be divided into four broad classes based on their appearance and physical characteristics: elliptical, lenticular, irregular, and spiral. , with many subclasses in between.”

“However, galaxies are dynamic objects that evolve over time while interacting with their surrounding environment, meaning that an individual galaxy can fall into multiple classifications over its lifetime. ”

In 1992, Indiana University astronomer Tom Steiman-Cameron and colleagues published A detailed study of NGC 4753 reveals that its complex shape is likely the result of a merger with a small companion galaxy.

“Galaxies that swallow other galaxies often look like train wrecks, but this is a train wreck galaxy,” said Dr. Steiman-Cameron.

Galactic mergers occur when two or more galaxies collide, mixing their material and significantly changing the shape and behavior of each galaxy involved.

In the case of NGC 4753, the once-standard lenticular galaxy is thought to have merged with a nearby gas-rich dwarf galaxy about 1.3 billion years ago.

The dwarf galaxy’s gas, combined with the burst of star formation caused by this galactic collision, injected large amounts of dust into the system.

The galaxy’s gravitational inward spiral spread out the accumulated dust into a disk. And this is where the story gets interesting.

Astronomers have discovered that a phenomenon known as differential precession is responsible for NGC 4753’s tangled dust lanes.

Precession occurs when a rotating object changes its axis of rotation, like a spinning top that loses momentum and wobbles. And differential means that the speed of precession is different depending on the radius.

For a dusty accretion disk orbiting around a galactic nucleus, the rate of precession is faster toward the center and slower near the edges.

This fluctuating wobble-like motion is due to the angle at which NGC 4753 and its former dwarf companion collided, and is responsible for the strongly twisted dust lanes that we see today wrapping around the galaxy’s luminescent core. It becomes.

“For a long time, no one knew what to make of this strange galaxy,” said Dr. Steiman-Cameron.

“But by starting with the idea that the accreted material fills the disk and analyzing the three-dimensional geometry, the mystery was solved.”

“Thirty years later, we are now incredibly excited to be able to see this highly detailed image with the Gemini South Telescope.”

Source: www.sci.news

Everything you should know about the new ChatGPT AI competitor, Google Gemini

The emergence of ChatGPT in 2023 has been so significant that even those who are not typically online or technologically savvy are familiar with its existence. However, as OpenAI continued to develop its AI tool, competitors also began to emerge.

Shortly after launching ChatGPT, Google announced its own competitor called Bard. Bard is capable of doing everything that ChatGPT can, but with the backing of the world’s largest search engine.

Now, Google is taking another step forward with a new project called Google Gemini, which appears to have already surpassed ChatGPT. However, the question on everyone’s mind is whether Google will surpass ChatGPT to become the top AI in 2024?

What is Google Gemini and how does it work?

OpenAI’s well-known tool is ChatGPT, which is powered by GPT-4, a large-scale language model that uses images, text, context, and other factors. For Google, Gemini serves a similar role to GPT-4, functioning as an engine that runs AI programs.



Gemini was built from the ground up and leverages teams across Google to generalize and understand various forms of content. It was trained on a large dataset that includes books, articles, code repositories, music, audio recordings, and other media. This data is processed into a format that is efficiently understood by Gemini, enabling the model to learn relationships between different terms and media, and how to respond to prompts, questions, and suggestions.

How to try Google Gemini for free

There are currently two ways to test Google Gemini, with the most accessible option being through Google Bard, which has been built on a test version of Gemini. An alternative way is to access Gemini through features integrated with Google Keyboard and the Recorder app on a Google Pixel 8 Pro.

What can Gemini do?

Google has been showcasing Gemini’s capabilities, demonstrating its ability to understand, answer questions, and perform various tasks. While impressive, some of these demonstrations are curated, making it difficult to gauge their real-world performance. Gemini can interact with different forms of digital content, from images to videos, and is capable of making connections between different words and images.

Google Gemini vs. GPT-4: Which is better?

Gemini has been touted as outperforming GPT-4 in various categories used to test model knowledge and reasoning. However, these impressive statistics have been verified by Google itself, leaving room for questions about Gemini’s real-world performance. Google plans to release different versions of Gemini, each with varying levels of intelligence and functionality, similar to OpenAI’s GPT model.

read more:

Source: www.sciencefocus.com