Tag Archive for 'VLA'

The tidal disruption event AT2024tvd. Image credit: NASA / CXC / University of California, Berkeley / Yao et al. / ESA / STScI / HST / J. DePasquale.

Wandering Supermassive Black Hole Discovered 600 Million Light-Years Away

May 8, 2025 by News Staff

This supermassive black hole was discovered thanks to the newly-identified tidal disruption event AT2024tvd, an astronomical phenomenon in which a star...

Ammonia gas infalling into an accretion disk feeding the protostar HW2. Image credit: NSF / AUI / NSF / NRAO / B. Saxton.

New Observations Shed More Light on Formation of Massive Stars

May 6, 2025 by News Staff

Astronomers using NSF’s Very Large Array (VLA) have spotted the huge flow of gas near HW2 — a massive protostar located 2,283 light-years away...

This composite image shows the quasar H1821+643. Image credit: NASA / CXC / University of Nottingham / Russell et al. / NSF / NRAO / VLA / SAO / N. Wolk.

Astronomers Find Underachieving Quasar in Distant Galaxy Cluster

Mar 22, 2024 by News Staff

Using NASA’s Chandra X-ray Observatory and NSF’s Karl G. Jansky Very Large Array (VLA), astronomers have found that H1821+643 — the nearest quasar...

Yu et al. discovered radio bursts above a sunspot that resemble radio emissions from aurorae on Earth. The pink-purple streaks in this illustration represent the radio emissions, with higher-frequency radio signals in pink, closer to the sunspot, and lower frequencies in purple. The thin lines represent magnetic field lines above the sunspot. The sunspot is the dark region on the Sun at the bottom. Image credit: Sijie Yu, New Jersey Institute of Technology.

Solar Astronomers Detect Aurora-Like Radio Emission above Sunspot

Mar 21, 2024 by News Staff

Astronomers using the Karl G. Jansky Very Large Array have observed long-lasting aurora-like radio bursts above a sunspot. This discovery could help us...

Free-floating binary Jupiter-mass objects are common even when present stellar and planetary theory cannot account for its existence. Image credit: Gemini Observatory / Jon Lomberg.

Astronomers Discover Binary System of Free-Floating Planetary-Mass Objects

Feb 14, 2024 by Enrico de Lazaro

The JuMBO 24 binary system resides in the Orion Nebula, a diffuse nebula located approximately 1,350 light-years away in the constellation of Orion. Free-floating...

Daly et al. found Sagittarius A* is spinning with 60% of the maximum possible rate of spin, a limit set by material not being able to 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 et al.

Milky Way’s Supermassive Black Hole is Spinning Very Rapidly, New Research Shows

Feb 12, 2024 by News Staff

Sagittarius A*, the 4.3-million-solar-mass black hole that resides at the center of the Milky Way Galaxy, is spinning so quickly it is warping the spacetime...

This artist’s impression shows the millisecond pulsar PSR J1023+0038 stealing gas from its companion star. Image credit: ESO / M. Kornmesser.

Matter Ejections Explain Peculiar High-Low Mode Switches in Distant Millisecond Pulsar

Aug 30, 2023 by Enrico de Lazaro

The millisecond pulsar PSR J1023+0038 is known to switch between two brightness modes almost constantly, something that until now has been an enigma. This...

For most of the time, Saturn’s atmosphere looks hazy and featureless to the naked eye in contrast to Jupiter’s colorful and vibrant atmosphere. This picture changes when we look at Saturn using a radio eye. Despite bland looking at the visible wavelengths, different latitudes on Saturn show dramatic contrast in the radio emission. In 2015, Li et al. found substantial brightness temperature variations -- greater than the temperature increase caused by the 2010 storm -- as a function of latitude and radio wavelength based on spatially resolved radio images of Saturn, as obtained from the VLA. Via a spectral inversion study, they created a latitude-altitude map of ammonia concentration anomalies from these images and correlate the anomalies to the occurrences of past giant storms in the northern hemisphere. Image credit: S. Dagnello / NRAO / AUI / NSF / Li et al., doi: 10.1126/sciadv.adg9419.

VLA Reveals Megastorm-Centric Disruptions in Saturnian Atmosphere

Aug 14, 2023 by News Staff

Planetary-scale giant storms erupt on Saturn periodically. There have been at least six recorded occurrences of past eruptions, and the most recent one...

Akins et al. used microwave observations to spot the first polar cyclone on Uranus, seen here as a light-colored dot to the right of center in each image of the planet. The images use wavelength bands K, Ka, and Q, from left. Image credit: NASA / JPL-Caltech / VLA.

VLA Spots Polar Cyclone on Uranus

May 23, 2023 by News Staff

Astronomers using the Karl G. Jansky Very Large Array in New Mexico have observed a bright, compact spot centered at Uranus’ north pole at several wavelengths....

NSF’s Karl G. Jansky Very Large Array is collecting data that astronomers will analyze for the type of emissions that only artificial transmitters make. Image credit: VLA / SETI.

VLA to Search for Radio Signals from Alien Civilizations

May 4, 2023 by News Staff

NSF’s Karl G. Jansky Very Large Array (VLA), a powerful radio telescope situated about 80.5 km (50 miles) west of Socorro, New Mexico, is joining the...

This artist’s concept shows the brilliant glare of two quasars residing in the cores of two galaxies that are in the chaotic process of merging. Image credit: NASA / ESA / Joseph Olmsted, STScI.

Merger of Two Massive Disk Galaxies Produces Dual Quasar

Apr 5, 2023 by News Staff

Using the NASA/ESA Hubble Space Telescope and other space and ground-based observatories, astronomers have discovered SDSS J0749+2255, a closely bound...

An artist’s conceptual rendering of interactions between a prospective exoplanet and its star. Image credit: NSF / Alice Kitterman.

Astronomers Detect Radio Emission Associated with Magnetic Field of Nearby Exoplanet

Apr 4, 2023 by News Staff

Observing magnetic star-planet interactions offers promise for determining the magnetic fields of exoplanets. Models of star-planet interactions predict...

This image features 3C 297 that is lonelier than expected after it likely pulled in and absorbed its former companion galaxies. In this new composite image, Chandra data is colored purple, VLA data is red and Gemini data is green. Visible light and infrared data from Hubble (blue and orange respectively) have also been included. Image credit: NASA / CXC / University of Torino / Missaglia et al. / ESA / STScI & International Gemini Observatory / NOIRLab / NSF / AURA / NRAO / AUI / NSF.

Chandra Finds Surprisingly Lonely Galaxy in Early Universe

Mar 9, 2023 by News Staff

3C 297 is located about 9.2 billion light-years away in the constellation of Virgo and contains a quasar, a supermassive black hole pulling in gas at the...

This composite image shows at least three galaxy clusters colliding in a jumbled scene. The resulting giant galaxy cluster, known as Abell 2256, resembles a grainy, pixilated, sky blue cloud topped with licks of flaming red hair. The cloud is adorned with red shapes and streaks, and set against a black background heavily dotted with colorful specks. The image combines X-ray, radio, optical, and infrared data. Image credit: NASA / CXC / University of Bolonga / Rajpurohit et al. / ESA / XMM-Newton / LOFAR / ASTRON / NCRA / TIFR / GMRT / NSF / NRAO / VLA / Pan-STARRS.

Astronomers Capture Ongoing Collision of Three Galaxy Clusters

Feb 1, 2023 by News Staff

Using NASA’s Chandra X-ray Observatory, ESA’s XMM-Newton and three radio telescopes (the Giant Metrewave Radio Telescope, the Low Frequency Array,...

The volcano-laced surface of Jupiter’s moon Io was captured in infrared by the Jovian Infrared Auroral Mapper (JIRAM) imager aboard NASA’s Juno spacecraft as it flew by at a distance of was about 80,000 km (50,000 miles) on July 5, 2022. Brighter spots indicate higher temperatures in this image. Image credit: NASA / JPL-Caltech / SwRI / ASI / INAF / JIRAM.

Trace Gas Detection Sheds New Light on Atmospheres of Jupiter and Its Volcanic Moon Io

Dec 28, 2022 by Natali Anderson

Using data from NSF’s Karl G. Jansky Very Large Array (VLA), the Atacama Large Millimeter/submillimeter Array (ALMA) and NASA’s Juno spacecraft, two...

An artist’s impression of a tidal disruption event. Image credit: Carl Knox / OzGrav, ARC Centre of Excellence for Gravitational Wave Discovery, Swinburne University of Technology.

Astronomers Detect Very Luminous Jet from Star-Eating Supermassive Black Hole

Dec 1, 2022 by News Staff

A supermassive black hole devours a star that has come too close. In extremely rare instances — only about 1% of the time — these so-called...

This Hubble image shows a blue stellar system. Image credit: Michael Jones.

New Type of Stellar System Discovered

Jun 17, 2022 by News Staff

Astronomers have spotted five blue stellar systems — which they say appear through a telescope as blue blobs and are about the size of dwarf galaxies...

Top left: a giant blue star, much more massive than our Sun, has consumed, through nuclear fusion at its center, all its hydrogen, helium, and heavier elements up to iron. It now has a small iron core (red dot) at its center. Unlike the earlier stages of fusion, the fusion of iron atoms absorbs, rather than releases, energy. The fusion-released energy that has held up the star against its own weight now is gone, and the star will quickly collapse, triggering a supernova explosion. Top right: the collapse has begun, producing a superdense neutron star with a strong magnetic field at its center (inset). The neutron star, though containing about 1.5 times the mass of the Sun, is only about the size of Manhattan. Bottom left: the supernova explosion has ejected a fast-moving shell of debris outward into interstellar space. At this stage, the debris shell is dense enough to shroud from view any radio waves coming from the region of the neutron star. Bottom right: As the shell of explosion debris expands over a few decades, it becomes less dense and eventually becomes thin enough that radio waves from inside can escape. This allowed observations by the VLA Sky Survey to detect bright radio emission created as the rapidly spinning neutron star’s powerful magnetic field sweeps through the surrounding space, accelerating charged particles. This phenomenon is called a pulsar wind nebula. Image credit: Melissa Weiss, NRAO / AUI / NSF.

Astronomers Spot Pulsar Wind Nebula in Distant Dwarf Galaxy

Jun 15, 2022 by News Staff

A pulsar wind nebula is created when the powerful magnetic field of a rapidly spinning neutron star accelerates surrounding charged particles to nearly...

This image shows the Orion Molecular Clouds, the target of the VANDAM survey; yellow dots are the locations of the observed protostars on a blue background image made by Herschel; side panels show six young protostars imaged by ALMA (blue) and the VLA (orange). Image credit: NRAO / AUI / NSF.

Astronomers Find Protoplanetary Disks in Orion Molecular Clouds

Mar 25, 2022 by Enrico de Lazaro

Astronomers using NSF’s Karl G. Jansky Very Large Array and the Atacama Large Millimeter/submillimeter Array have detected 97 disks of gas and dust around...

Four enormous cavities have been found at the center of the RBS 797 galaxy cluster using Chandra. Image credit: NASA / CXC / University of Bologna / F. Ubertosi / STScl / M. Calzadilla / NSF / NRAO / ALMA.

Chandra Spots Four Cavities in Center of Galaxy Cluster

Dec 29, 2021 by News Staff

Astronomers using NASA’s Chandra X-ray Observatory have found a quartet of pronounced X-ray cavities in RBS 797, a cluster of galaxies located about...

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