Astronomer Frank Kiwy uses Astro Data Lab to discover 34 new ultracool dwarf binary systems in the Sun's neighborhood, expanding knowledge of brown dwarfs and their companions. The discovery nearly doubles previously known samples, shedding light on how often brown dwarfs have companions.
A team of astronomers discovered an unusual ultra-faint dwarf galaxy, Pegasus V, on the outer edge of the Andromeda Galaxy using NSF's NOIRLab facilities. The galaxy appears to be extremely deficient in heavier elements, indicating it is very old and likely a fossil of the first galaxies.
Astronomers used the Gemini South telescope to capture high-resolution images of dusty disks around 44 young massive stars. The survey found that smaller star-mass systems have ringed structures, while more massive systems do not.
The Gemini North telescope has helped astronomers understand why Uranus and Neptune have different colors. Excess haze on Uranus builds up in its stagnant atmosphere, making it appear lighter than Neptune's. The team developed a single atmospheric model that matches observations of both planets.
Astronomers have captured detailed images of sinuous stellar jets emanating from young stars, suggesting that their sidewinding appearances are caused by gravitational attraction from companion stars. The observations were made using the Gemini South telescope's adaptive optics system.
Astronomers have discovered a binary system consisting of a rapidly spinning neutron star and the precursor to an extremely-low-mass white dwarf, dubbed a 'cosmic spider'. The system emits powerful gamma-rays and has been observed using the SOAR Telescope in Chile.
Researchers have discovered at least 70 new free-floating planets, each roughly the mass of Jupiter, in a nearby region of the Milky Way. The discovery was made using observations and archival data from several observatories, including NSF's NOIRLab facilities.
A team of astronomers has made the most precise measurements yet of the motions of stars around Sagittarius A*, the supermassive black hole at the center of the Milky Way. The research, using cutting-edge facilities like Gemini Observatory and the European Southern Observatory's Very Large Telescope, shows that nearly all of the mass c...
A new study suggests that most nearby rocky exoplanets are quite unlike anything in our Solar System, with diverse and exotic rock types not found anywhere. The research uses the chemical composition of 'polluted' white dwarfs to estimate the rock types on planets orbiting nearby stars.
Astronomers have discovered a 0.6-second gamma-ray burst caused by the implosion of a massive star, revealing that some short GRBs might be imposters in disguise. The discovery suggests that most collapsing stars fail to produce a GRB jet, making this event an effective fizzle.
Astronomers using Gemini Observatory and WIYN 3.5-meter Telescope found 73 binary star systems among TESS exoplanet hosts, which could be hiding Earth-sized planets. The team discovered that small planets are harder to detect in binary systems due to glare from the companion star.
The Dark Energy Survey has released its most precise look at the universe's evolution, using data from 226 million galaxies observed over nearly one-eighth of the sky. The results confirm the current best model of the Universe, but hint that the Universe today is a few percent less clumpy than predicted.
Three rapidly rotating brown dwarfs were discovered spinning around their axes once every hour, reaching speeds of about 350,000 kilometers per hour. This extreme rotation rate is ten times faster than Jupiter and poses a risk to the stability of these objects.
Two close quasar pairs are found in distant merging galaxies, separated by just over 10,000 light-years. This discovery provides crucial insight into the existence of supermassive black hole pairs and galaxy mergers in the early Universe.
The team has determined the mass of a rocky planet around the nearby star Gliese 486 using MAROON-X's spectrometer. The exoplanet, called Gliese 486 b, is roughly three times the mass of Earth and has a similar density.
Farfarout is the most distant known object in our Solar System, with an orbit taking it 175 au from the Sun at its farthest point. Its discovery provides insights into the history of the outer Solar System and the potential for future interactions with Neptune.
A team of astronomers has created the most complete 3D map of cool brown dwarfs in the Sun's local neighborhood, cataloging over 500 objects including 38 new discoveries. The results provide evidence that the Sun's immediate neighborhood is unusually diverse relative to other parts of the Milky Way Galaxy.
The Dark Energy Survey has released a massive catalog of nearly 700 million astronomical objects, building on the previous data release and improving calibration techniques. The catalog provides unprecedented insights into the distribution of matter in the Universe and may hold clues to how our galaxy was assembled over billions of years.
Astronomers have released the largest-ever map of the sky, comprising over a billion galaxies, to aid in understanding dark energy. The DESI Legacy Imaging Surveys will provide new insights into this mysterious force driving the Universe's accelerating expansion.
The discovery uses a deep residual neural net trained on real data to uncover warped and stretched images of distant galaxies. The new lenses provide astronomers with targets to measure fundamental properties of the Universe, including the Hubble constant.
The most distant quasar known has been discovered, powered by the earliest known supermassive black hole weighing over 1.6 billion times the mass of the Sun. This fully formed distant quasar is also the earliest yet discovered, providing insight into massive galaxy formation in the early Universe.
The Inouye Solar Telescope has released its first image of a sunspot, revealing striking details of the sunspot's structure. The image achieves a spatial resolution about 2.5 times higher than ever previously achieved, showing magnetic fields as small as 20 kilometers on the surface of the Sun.
A team of astronomers using Gemini North's GNIRS instrument discovered that CK Vulpeculae, a bright new star in 1670, is approximately five times farther away and has ejected gas at much higher speeds than previously reported. The new findings suggest the explosion was far more violent, releasing roughly 25 times more energy than a nova.
The NSF's National Solar Observatory has predicted the arrival of a large sunspot on November 18, coinciding with Thanksgiving. The prediction uses helioseismology to detect changes in sound waves from the Sun's interior and is valuable for understanding space weather effects.
A team of astronomers has discovered the first cold brown dwarf using radio observations from the LOFAR telescope and Gemini North. The object, BDR J1750+3809, is a close cousin of Solar System planets like Jupiter and can be used to test theories predicting exoplanet magnetic fields.
For the first time, astronomers have surveyed over 250 million stars in the Milky Way's bulge, measuring their chemical composition and gaining new insights into the galaxy's formation. The data will help scientists understand how the Milky Way formed its central bulge and gain a better understanding of other galaxies.
The team used adaptive optics on the Gemini South telescope to reveal a wealth of detail in the nebula, including unusual structures and evidence for a jet of material ejected from a newly-formed star. The image provides the sharpest view to date of how massive young stars affect their surroundings.
Astronomers have discovered a Jupiter-sized planet, WD 1856b, orbiting close to a white dwarf star, defying previous assumptions about planetary destruction. The planet's unique characteristics suggest it may have originated far from the star and survived its demise, raising hopes for future discoveries.
Astronomers using NSF's NOIRLab facilities and citizen science project Backyard Worlds have discovered approximately 100 cool brown dwarfs near the Sun, with several of these worlds approaching Earth's temperature. These discoveries provide new insights into the formation and atmospheres of planets beyond our Solar System.
Researchers obtained critical data on a special type of exploding star, known as calcium-rich supernovae, which produce vast quantities of calcium. These events account for up to half of the calcium found in the universe and provide insights into how elements are expelled during a supernova explosion.
Astronomers have discovered an exoplanet, K2-25b, that is surprisingly dense for its size and age, defying current planet formation theories. The exoplanet, orbiting a young star in the Hyades cluster, has a mass of 25 Earth-masses and a size slightly smaller than Neptune.
The Gemini Observatory has detected a distant short gamma-ray burst (SGRB) with an optical afterglow, providing new insights into the merger of two neutron stars. The observation, made just hours after the burst's detection, revealed the SGRB's distance and placed it in the epoch of cosmic high noon.
Astronomers have discovered the second most distant quasar, Pōniuāʻena, containing a monster black hole twice the mass of other quasars at the same epoch. The discovery presents significant challenges to current theories on supermassive black hole formation and growth in the early universe.
The Gemini North telescope has collected some of the highest resolution images of Jupiter ever obtained from the ground, complementing Hubble observations to reveal details about Jovian weather. The images show that lightning strikes and giant storm systems are formed in large convective cells over deep clouds of water ice and liquid.
The Gemini Observatory has captured an exquisite image of the planetary nebula CVMP 1, also known as a celestial hourglass. This object is formed when a massive star undergoes a catastrophic explosion, leaving behind a hot core that energizes the ejected gases, causing them to glow and form the striking hourglass shape.
The NEID instrument has made its first observations, detecting the subtle effect of exoplanets on their parent stars. With a precision three times better than previous instruments, NEID aims to determine the masses of exoplanets as small as Earth and characterize their atmospheres.
Researchers have identified a repeating Fast Radio Burst source in a nearby spiral galaxy, which is radically different from previous studies. The discovery challenges assumptions about the origin of these mysterious radio pulses and may indicate that FRBs are produced in a large zoo of locations across the Universe.
The NSF Vera C. Rubin Observatory will conduct a vast astronomical survey, mapping the Milky Way and probing dark energy and dark matter. Vera Rubin's groundbreaking work uncovered the existence of dark matter, making this observatory a fitting tribute to her legacy.
Astronomers have identified overlapping bubbles of hydrogen gas ionized by the stars in early galaxies, providing direct evidence for the reionization of the universe. The earliest detected stars formed around 680 million years after the Big Bang and began to light up the cosmic dark ages.
The NGC 5394/5 galaxies are engaging in a slow and intimate dance, fueled by their gravitational interactions. This process has already led to the coalescence of hydrogen gas into regions of star formation, resulting in the sparkling of new stars.
Teams from Cerro Tololo and Kitt Peak Observatories imaged Mercury's transit with different telescopes and cameras. The goal is to measure the parallax shift caused by Mercury's apparent position on the Sun to calculate the distance to the Sun.
The Dark Energy Spectroscopic Instrument (DESI) has begun testing its capabilities, capturing light from distant galaxies and preparing to map 35 million galaxies across 1/3 of the sky. DESI aims to study 10 million stars in our galaxy, the Milky Way, tackling one of physics' most profound problems: the nature of dark energy.
Astronomers have uncovered two historic events in the Andromeda Galaxy, with evidence suggesting major changes to its structure occurred a few billion years ago and much earlier. The findings provide insights into the evolution and formation of both the Andromeda Galaxy and our own Milky Way.
The new laboratory combines existing and new facilities, fostering innovative scientific programs, idea exchange, and creative development in ground-based optical-infrared astronomy. The lab enables breakthrough discoveries in astrophysics by developing state-of-the-art observatories and providing data products for a diverse community.
The Gemini Observatory has captured the first-ever image of an interstellar comet, C/2019 Q4 (Borisov), in multiple colors. The object exhibits a pronounced tail indicative of outgassing, a characteristic that defines cometary objects.
Astronomers can now automatically follow up on variable astronomical objects with a range of 0.4-meter to 8-meter telescopes, observing in UV light to infrared. The network uses automated software and generates dynamic observing schedules every 15 minutes.
The discovery of ZTF J1539+5027 is the fastest known eclipsing white dwarf binary, with an orbit period of only 6.91 minutes, making it a valuable target for gravitational wave studies. The system is expected to be one of the strongest sources of gravitational waves detectable by LISA, the future space-based gravitational wave detector.
A team of astronomers successfully confirmed the distance to a galaxy hosting an intense radio burst that flashed only once, lasting a thousandth of a second. The Gemini South telescope played a crucial role in verifying that the burst occurred 4 billion years ago.
The study suggests that massive planets form through slow material accumulation, while brown dwarfs come about due to rapid gravitational collapse. The discovery advances the idea of bottom-up planet formation and highlights the differences in planetary systems beyond our own.
Astronomers discover unique infrared signature on Triton, suggesting a mix of carbon monoxide and nitrogen ices. This finding sheds light on conditions on other distant, icy worlds and could provide insights into the origins of life.