Scientists are exploring and continuing to search for potentially habitable alien worlds
Since the first exoplanet orbiting a Sun-like star was confirmed in 1995, scientists have discovered more than 5,000 such distant worlds. More than half of these discoveries were made by NASA’s Kepler space telescope, launched in 2009 to determine the prevalence of Earth-like planets in the Milky Way galaxy. Kepler was decommissioned in 2018, having discovered more than 2,600 exoplanets.
Scientists are studying the history of collisions between the Milky Way and other galaxies and the possible consequences of future collisions. These collisions, incidentally, are still occurring
The Milky Way’s halo contains a large group of stars with unusual orbits, many of which are believed to have been engulfed by our galaxy during an event astronomers call the “last major merger.” As the name suggests, this was the last time our galaxy experienced a significant collision with another galaxy—presumably a massive dwarf galaxy that flooded the Milky Way with stars passing very close to our galaxy’s center.
Magnetars are neutron stars with the strongest magnetic fields. What is known about them today?
Magnetars are a special class of neutron stars with ultra-strong magnetic fields, the strongest of any object in the observable universe, approximately a trillion times stronger than the most powerful permanent magnets ever created on Earth. Neutron stars are the remnant cores of massive stars formed at the end of their lives, possessing a mass greater than the Sun and compressed to the size of a city, making them natural laboratories for studying extreme physical phenomena. Magnetars, as previously thought, can come in different types. One possibility is an exploding object orbiting a black hole surrounded by a disk of material. Another possibility is a pair of rotating neutron stars whose magnetospheres periodically interact, creating a cavity where eruptions can occur. Magnetars are estimated to be active for about 10,000 years before settling down, so they could be found where a firestorm of star formation is occurring. However, this does not seem to be the case for all magnetars.
Modern technologies and problems of studying the Milky Way
The European Space Agency’s XMM-Newton and NASA’s Chandra space telescopes captured the aftermath of three bright explosions echoing in the Milky Way’s outer spiral arms. NASA’s Nancy Grace Roman Space Telescope will help scientists better understand the fainter components of our Milky Way galaxy—the gas and dust scattered between stars, known as the interstellar medium. Scientists can also gain insight into the ages, masses, and sizes of stars using the Kepler space telescope, which provided asteroseismic data on approximately 16,000 stars before its decommissioning in 2018. A laser star pointer mounted on Cerro Pachón in central Chile points upward across the Gemini South observatory’s field of view, illuminating the Milky Way.
Quasars are among the earliest objects in the Universe. Are they creators or destroyers of galaxies?
Quasars represent a stage in a galaxy’s life during which large volumes of matter spiral toward a central supermassive black hole, releasing enormous amounts of energy. During this stage, the galactic core shines brighter than anything else in the universe, often outshining the rest of its host galaxy by hundreds or thousands of times. Quasars are the extremely bright centers of galaxies, powered by actively fueled supermassive black holes. Studying these objects can help researchers understand how black holes evolve throughout the modern Universe. However, by attracting gas and dust, these black holes release so much energy that they can outshine entire host galaxies, making them difficult to study.
In 2024-2026, a theory of dark matter accumulation in the center of our Galaxy was developed
New models show that stars can exist using only dark matter as fuel, and because there is an extremely large amount of dark matter near the Galactic Center, these stars become immortal.
New discoveries in the field of interactions in stellar systems
Using the Transiting Exoplanet Survey Satellite (TESS), a spacecraft designed to search for exoplanets, astronomers discovered an unusual quadruple star system. During another dedicated observing campaign, XRISM revealed that hot plasma signals follow the orbital motion of an otherwise invisible companion star. And a new study by Japanese scientists has shown that our Sun and numerous similar “solar twins” may have migrated together from the core of the Milky Way galaxy.
First proposed by physicist Freeman Dyson in 1960, the idea of alien spheres remains relevant in the 21st century
In the 1960s, physicist and polymath Freeman Dyson proposed the idea of creating these eponymous spheres. He proposed that a sufficiently advanced society would have an insatiable need for space and energy. If they were industrious enough, they could solve both problems by dismantling a planet and turning it into a massive spherical shell. This sphere would encircle the star, providing a surface area equal to billions of planets and absorbing vast amounts of solar energy. Dyson calculated that a shell made from a Jupiter-mass planet could completely envelop the Sun at approximately the same orbit as Earth. However, gravity within the hollow shell is neutralized, meaning there is nothing binding the shell to the star. They are free to move in independent directions, meaning the star containing the Dyson sphere would soon simply smash into the shell, destroying it.
The search for dark matter in our Milky Way galaxy is the most challenging task in modern physics
Stars have been observed crawling along the outskirts of the Milky Way more slowly than expected—a slow motion that scientists say can only be explained if our map of galaxies containing dark matter is incorrect. The specific velocities of stars at the edges of these galaxies have historically been irrefutable evidence of the presence of dark matter in galaxies. This is because astronomers can measure a galaxy’s “rotation curve,” which plots the orbital velocities of stars against their distance from the galactic center.
Unique properties of ionic liquids, superalcohols and cosmic radiation indicate the existence of life beyond Earth
Life may exist right under our noses in the Solar System—the moons of Jupiter and Saturn are of great interest. Europa and Enceladus may harbor vast subsurface oceans where at least microbial life could be possible. Thanks to new data obtained with the James Webb Space Telescope, scientists have discovered compelling evidence of extraterrestrial life on one exoplanet. But is water truly a necessary ingredient for life? A new study has determined that ionic liquids can form where liquid water cannot, thanks to their ability to remain liquid over a wide range of temperatures and pressures. These ionic liquids may ultimately support biomolecules such as proteins.
Water is an inevitable consequence of planet formation and is much more common in the galaxy than scientists previously thought
The findings suggest that water may not be a rare cosmic coincidence, but rather an inevitable consequence of planet formation, making it far more common in the galaxy than scientists previously thought. Water is life, at least as we know it. All life on Earth uses liquid water, and researchers studying the origins of life believe that the complex chemistry of life likely originated either in a warm pool on the Earth’s surface or near a deep-ocean hydrothermal vent. Therefore, planetary scientists are particularly interested in extraterrestrial locations where liquid water exists. Based on existing exoplanet data, super-Earths and sub-Neptunes are considered the most common classes of planets in our galaxy, and some of them are likely water worlds. However, these planets are large, and the interactions between the water in their oceans and the rocks in their interiors will determine how habitable they might be.
Science fiction and the official scientific opinion on alien life
Many scientists are searching for extraterrestrial life on planets with conditions similar to Earth. For example, a habitable planet would likely have water. For liquid water, the planet would need to be at the perfect distance from its sun to prevent the water from freezing and turning into gas.
Alien craft or natural object? The most mysterious comet, Atlas, is approaching Earth
Initial estimates placed the comet’s diameter at about 11 kilometers (7 miles). However, subsequent data from the Hubble Space Telescope indicated that 3I/ATLAS is likely closer to the maximum size of 5.6 kilometers (3.5 miles). In any case, it is likely the largest interstellar object ever observed.
New research into astronaut nutrition
Nutrition has been crucial in every era of exploration on Earth, from the days when scurvy plagued sailors to the last century, when polar explorers died from malnutrition or, in some cases, nutrient toxicity. New research sheds light on the risks of inadequate nutrition and food supply, leading to poor health and performance of astronauts during missions, as well as to poor health in the long term (nutrition and food-related risks).
Studies of the cardiovascular and muscular systems under altered gravity conditions
Even intense physical activity by astronauts cannot compensate for the muscle atrophy caused by microgravity. This atrophy occurs, in part, due to the mechanism regulating calcium absorption. Recent studies have shown that spaceflight alters calcium absorption by muscles. However, the molecular mechanisms underlying these changes are poorly understood.
Microbes as part of biodiversity in space flights
Astronauts arriving and returning from space stations carry trillions of microscopic organisms with them. For example, new species of space-adapted bacteria have been discovered on China’s Tiangong space station. Recently, 26 previously unknown species of bacteria were discovered in NASA’s cleanrooms—some of the most sterile environments ever created by humanity. Another study shows that, under stress, strains isolated from the ISS mutated and became genetically and functionally distinct from their terrestrial counterparts.
Dark matter and the cosmic web connect galaxies like city superhighways
Giant filaments crisscross the universe, connecting galaxy clusters like superhighways between cities. Their shape and structure contain vital information about the universe’s contents and history. However, their complex shape makes them extremely difficult to measure. Now, researchers have presented a new method for measuring the mass of these filaments, which could be used to unlock the secrets of dark matter and dark energy.
The composition and structure of dark matter: theories and mysteries
According to the research team, their results also allow them to more accurately determine what proportion of the energy and matter in the Universe is dark energy. They reached their conclusions after analyzing observations of galaxy clusters made by the eROSITA X-ray telescope, which scans the entire sky above Earth in search of detectable galaxy clusters. eROSITA is mounted on Spektr-RG, a Russian-German space telescope launched into Earth orbit in 2019.
Two Theories About the Relationship Between Dark Matter and Black Holes
Tiny black holes that formed seconds after the birth of the universe may be around longer than expected, leading researchers to believe that primordial black holes could be the source of dark matter, the most mysterious substance in the universe.
Dark matter in galaxies may be weakened or absent altogether
The standard view of cosmic evolution may be challenged by the discovery of a huge galaxy that appears to lack dark matter. Dark matter, which makes up about 85% of the matter in the universe, is missing from NGC 1277, a galaxy in the Perseus galaxy cluster. The galaxy, located 240 million light-years from Earth, is the first Milky Way-sized cluster of stars, planets, dust, and gas to be found to lack dark matter.
Evolution of dark matter and the rotation of the Universe
The standard model of cosmology – our leading theory of cosmic evolution – suggests that dark energy is constant throughout the universe and over time, making it a fundamental property of space. If it were constant, the mysterious dark energy, which makes up as much as 70 percent of the universe, would push away all stars and galaxies. However, the most comprehensive survey of the universe’s cosmic history suggests that dark energy, also known as the hypothetical “antigravity” force, may evolve over time rather than remain constant, pointing to a less lonely future for the universe’s inhabitants.
The concept of “Einstein ring” and its connection with dark matte
An Einstein ring is an extremely rare type of gravitationally lensed object, first predicted by Albert Einstein’s theory of relativity. Gravitational lensing occurs when the immense gravity of a massive foreground object, such as a galaxy cluster or a black hole, bends spacetime around it; light emitted by more distant objects, such as galaxies or supernovae, passing through this curved spacetime also appears curved from our perspective on Earth.
Basic principles of the design and operation of the James Webb Space Telescope (JWST)
The James Webb Space Telescope (JWST) is the largest and most powerful space telescope in existence. NASA’s infrared space observatory was launched on December 25, 2021, from ESA’s Kourou Spaceport in French Guiana at 7:20 a.m. ET (12:20 p.m. GMT; 9:20 a.m. local time in Kourou) aboard an Arianespace Ariane 5 launch vehicle. The $10 billion James Webb Telescope will explore the cosmos to uncover the history of the universe, from the Big Bang to the formation of exoplanets and beyond.
Interaction of stars, galaxies and dark matter
The extreme conditions found in neutron stars make them ideal laboratories for studying physics in conditions found nowhere else in the universe. Scientists also suspect that some dead stars made of the densest material in the known universe, called neutron stars, may act as traps for dark matter particles, which collide at high speeds and annihilate each other. New research suggests that brown dwarfs, also known as failed stars, may act as gravitational traps for dark matter, forcing this exotic material to interact with each other.
Planet-Forming Molecules Discovered in Most Extreme Environments
An international team of astronomers has used the NASA/ESA/CSA James Webb Space Telescope to make the first observation of water and other molecules in the inner disk regions that form rocky planets, in one of the most extreme environments in our galaxy.
And asteroids have their own satellites
The European Space Agency’s Gaia star-gazing mission has once again proven its ability to explore asteroids, discovering potential moons around more than 350 asteroids that are not known to have moons.
Analysis of a sample of asteroid Bennu reveals dust rich in carbon, nitrogen and organic compounds needed for life
Early analysis of a sample of the asteroid Bennu returned by NASA’s OSIRIS-REx mission has revealed dust rich in carbon, nitrogen and organic compounds, all of which are essential components for life as we know it. The sample, dominated by clay minerals, particularly serpentine, reflects the type of rock found at mid-ocean ridges on Earth.
Video reports from other planets and systems? Our Sun can provide such an opportunity
Plans to use a solar lens date back to the 1970s. More recently, astronomers have proposed developing a fleet of small, lightweight CubeSats that would deploy solar sails to accelerate them to 542 AU. Once there, they would slow down and coordinate their maneuvers, creating an image and sending data back to Earth for processing.
The Heliosphere – a new object for study
Scientists call the region of space that the Sun influences the heliosphere, but without an interstellar probe, they know little about its shape. The heliosphere, the region of space that the Sun influences, is more than a hundred times the distance from the Sun to Earth.
The mechanism by which black holes glow remains an unsolved mystery for scientists
A team of astronomers studied 16 supermassive black holes that shoot powerful beams into space to track where the beams, or jets, are pointing now and where they were pointing in the past. Using NASA’s Chandra X-ray Observatory and the Very Large Baseline Array (VLBA) at the National Science Foundation’s (NSF) National Radio Astronomy Observatory (NRAO), they found that some of the beams had changed direction by a large amount.
James Webb Telescope Reveals Supermassive Black Holes of the Early Universe
Peering deep into space and time, two teams using the NASA/ESA/CSA James Webb Space Telescope have studied an exceptionally bright galaxy called GN-z11, which existed when our 13.8-billion-year-old universe was only about 430 million years old. Also studying JWST data, a team of astronomers led by Lukas Furtak and Adi Zitrin of Ben-Gurion University of the Negev were also able to determine the mass of the supermassive black hole. At about 40 million times the mass of the Sun, it is surprisingly massive compared to the galaxy it hosts.
Several black holes have been discovered in our Milky Way galaxy. At the galaxy’s heart is a dormant one 4.2 million times larger than the Sun
The black holes at the center of the Milky Way (Earth’s home galaxy) and Andromeda (one of our closest galactic neighbors) are among the quietest eaters in the universe. What little light they emit varies subtly in brightness, suggesting that they consume a small but steady stream of matter rather than large clumps. The streams approach the black hole gradually and in a spiral, like water swirling down a drain.
Supermassive black holes protect galaxies from growing too large
Galaxies could live longer if supermassive black holes act as their “hearts and lungs,” keeping them breathing and preventing them from growing too big. That’s the suggestion of a new study, which suggests that the universe would have aged much faster and today be filled with “zombie” galaxies containing dead or dying stars if it weren’t for the supermassive black holes that are thought to reside at the heart of all large galaxies. The astrophysicists behind the discoveries compare the jets of gas and radiation that supermassive black holes blow from their poles into their airways to breathing and lungs.
Black Hole Systems: Gravitational Waves of Space-Time Learned to Catch on Earth
Astronomers have discovered supermassive black holes with masses millions or billions of times that of the Sun in most massive galaxies in the local Universe, including our own Milky Way. Webb’s new observations provide evidence of an ongoing merger of two galaxies and their massive black holes when the Universe was just 740 million years old. The system is known as ZS7. Most black hole binaries are expected to be in what are called “quasi-circular” orbits. The giant black holes are thought to have been created when two smaller black holes collided and merged one day. And now scientists are wondering if we can learn about the black hole family tree by working backwards through the generations.
Anomalous ‘light’ black holes are primordial in the Universe
Black holes are formed either by the collapse of a massive star or by the merger of heavy objects. However, scientists suspect that smaller “primordial” black holes, including some with masses similar to the Earth, may have formed in the chaotic early moments of the universe. When we think of black holes, we tend to picture enormous cosmic monsters, such as stellar-mass black holes with masses tens or hundreds of times that of the Sun. We can even imagine supermassive black holes, with masses millions (or even billions) of times that of the Sun, sitting at the hearts of galaxies and dominating their surroundings. A team of scientists has predicted that NASA’s Nancy Grace Roman Space Telescope could detect a class of “light” black holes that have eluded detection until now.
Latest news on the theory of structure and origin of black holes
Supermassive black holes are thought to be born from successive mergers of smaller black holes, each bringing with it angular momentum that accelerates the spin of the black hole they birth. Measuring the spin of supermassive black holes can therefore provide insight into their history – and a new study suggests a new way to make such inferences based on the effects of spinning black holes on the very fabric of space and time.
The black hole in Omega Centauri is closer to Earth than the black hole at the center of the Milky Way
Most known black holes are either extremely massive, like the supermassive black holes found at the cores of large galaxies, or relatively light, with masses less than 100 solar masses. However, intermediate-mass black holes (IMBHs) are rare and are considered rare “missing links” in black hole evolution.
Magnetic Universe. New discoveries – from everyday use to neutron stars
Scientists smashed atom against atom and unleashed a magnetic monster. A groundbreaking experiment has created a field so strong it could eclipse the grip of a neutron star. Rotating magnets can create levitation that is almost impossible to physics. For the first time, physicists had a clear understanding of how individual atoms behave like waves.
Laws formulated by a 17th century scientist are used in modern space technologies
The story of how we understand planetary motion would be impossible to tell if not for the work of the German mathematician Johannes Kepler. Kepler’s Three Laws describe how the planets orbit the Sun. They describe 1 – how planets move in elliptical orbits with the Sun as the focus, 2 – a planet covers the same area of space in the same amount of time, regardless of where it is in its orbit, and 3 – the period revolution is proportional to the size of its orbit.
China outpaces rivals in space exploration
China built its own Tiangong space station, also known as “Tianhe”, located at altitudes of 217 and 280 miles (340 to 450 kilometers) in low Earth orbit in 2021. For the first time in more than four decades, it was China that brought moon rocks to humanity. China launched the Chang’e-6 probe to return soil from the far side of the Moon. The Chinese Academy of Sciences (CAS) Einstein Probe spacecraft was launched on January 9, 2024. China has already begun to lead the world in military launches, sending 45 defense satellites into orbit in 2022.
Heavy hydrogen used in nuclear energy and water turned out to be older than Earth
In protoplanetary disks, water is virtually omnipresent. Recent studies of the water content of early planetary systems like ours show that water is an abundant and ubiquitous molecule, originally synthesized on the surface of tiny grains of interstellar dust by hydrogenation of frozen oxygen, reports the journal Elements. In the molecular cloud from which a new planetary system will emerge, oxygen attaches and freezes to the dust grains it encounters. Once a hydrogen molecule intersects with this frozen oxygen, water ice is formed.
The Voyager 1 spacecraft outside the solar system stopped sending useful data back to Earth
The Voyager 1 space probe is the farthest man-made object in space. It was sent in 1977 with a golden record on board that contained various sounds of our home planet: greetings in different languages, dogs barking and the sounds of two people kissing, to name just a few examples. The idea behind this recording was that Voyager 1 might one day become an emissary of alien life—a sonic time capsule of the creatures of Earth. Since its launch, it has also managed to complete missions to Jupiter and Saturn. In 2012, he crossed interstellar space.
The Hubble telescope discovered water vapor in the atmosphere of an exoplanet located 97 light years from Earth
Astronomers using NASA’s Hubble Space Telescope have observed the smallest exoplanet to have water vapor in its atmosphere. Planet GJ 9827d, which is only about twice the diameter of Earth, could be an example of potential planets with water-rich atmospheres in other parts of our galaxy. GJ 9827d was discovered by NASA’s Kepler space telescope in 2017. It orbits the red dwarf every 6.2 days. The star GJ 9827 is located 97 light years from Earth in the constellation Pisces.
NASA’s DSOC sent video using a laser to Earth from a distance of 31 million kilometers
Following successful testing of DSOC technology in Earth orbit and on the Moon, NASA is now using deep space optical communications technologies to test laser communications over increasingly greater distances. While aboard the agency’s Psyche mission, DSOC has already sent video via laser to Earth from 19 million miles (31 million kilometers) away and is aiming to prove that high-throughput data can be sent even from Mars.
The NASA/JAXA XRISM mission investigates the composition and physical state of space objects by detecting X-ray radiation
Invisible to our eyes, X-rays emitted by the hot gas that fills much of the Universe can shed light on many cosmic mysteries. The first observations of this gas by JAXA’s X-ray Imaging and Spectroscopy Mission (XRISM) are ready and demonstrate that the mission will play a major role in revealing the evolution of the Universe and the structure of spacetime.
Top 12 unusual exoplanets discovered in 2023
In 2023, scientists discovered several stunning exoplanets. Last year, planetary scientists added a number of exciting new worlds to the exoplanet catalog of more than 5,000 objects. Among them are planets that we have never seen before.
The James Webb Space Telescope has proven that complex organic compounds are present even in the most ancient galaxies of the Universe
The James Webb Space Telescope is capable of searching the “carbonaceous” atmospheres of exoplanets to search for alien life. “We have a way to find out if there is liquid water on another planet. And we can achieve this in the next few years.”
NASA demonstrates optical communications for deep space operations
DSOC, an experiment that could change the way spacecraft communicate, has sent data using a laser to and from the Moon for the first time. The transmitted data takes the form of bits (the smallest units of data that a computer can process) encoded in laser photons—quantum particles of light.
ARRAKIHS dark matter satellite will be launched in 2030
The mission is planned to study the dark matter halo of 75 different galaxies – a hypothetical component of galaxies that surrounds the galactic disk and extends far beyond the visible part of the galaxy. The mass of the halo is the main component of the total mass of the galaxy, reports the European Space Agency.