How does ground-based astronomical radar expand our understanding of the Universe? By allowing us to study our nearby Solar System, and everything in it, in unprecedented detail. Radar can reveal the surface and ancient geology of planets and their moons, letting us trace their evolution.
In our most basic understanding of our Solar System, planets are drawn into the orbit of our massive star, the Sun. But what happens to planet-sized objects that don’t have a star? A team of astronomers studying Jupiter-mass binary objects (JuMBOs) in the Orion Nebula are gaining a new understanding of these unusual systems.
Though far to the west of the St. Croix antenna, the Owens Valley antenna has some similarities, in particular being in a remote location. The high mountains surrounding the valley mean that access to the region is only possible from the south, or through mountain passes. This also makes for a unique geography. To the south are the dry bed remains of Owens Lake, and further beyond is Death Valley. To the East are the White Mountains, which is home to the great bristlecone pine forest, and some of the oldest living trees in the world. Within the Methuselah Grove of this forest is hidden a particular tree that was seeded nearly 5,000 years ago.
SuperKnova is a project to provide learning opportunities in radio technology for students in a way that is inclusive and equitable. Originally conceived at the Radio Astronomy Imaging and Analysis Lab (RADIAL), SuperKnova is a collaboration between RADIAL, NRAO, and educators and students from across the country.
The Green Bank Telescope has discovered over 250 gaseous clouds being blasted out of the center of the Milky Way into interstellar space. A decade ago, astronomers weren’t aware of this phenomenon. It took years of observations, and some surprising finds, to produce this latest result.
An international team of astronomers have found ring and spiral structures in very young planetary disks, demonstrating that planet formation may begin much earlier than once thought.
The National Science Foundation’s National Radio Astronomy Observatory (NRAO) and the National Astronomical Observatory of Japan (NAOJ) are joining efforts to expand the capabilities of the world’s most powerful millimeter/ submillimeter telescope, the Atacama Large Millimeter/submillimeter Array (ALMA).
This blog post celebrates highlights from the brilliant career of astronomer Paul Vanden Bout, who recently received the Karl G. Jansky Lectureship from NRAO. Vanden Bout's vision for millimeter-wavelength astronomy led to the creation of several major radio telescopes around the world.
Gravity can focus light like a lens, allowing astronomers to see distant galaxies and explore dark matter. Join our host Summer Ash of the National Radio Astronomy Observatory as she talks about how astronomers use gravitational lensing to study the universe..
Many objects in the Universe have magnetic fields. Planets such as Earth and Jupiter, the Sun and other stars, even galaxies billions of light years away.
On August 20, 2023, the National Radio Astronomy Observatory (NRAO) marked 30 years since the National Science Foundation’s Very Long Baseline Array (VLBA) had its inauguration ceremony in the high desert of New Mexico. In the three decades since, the VLBA has become not only one of the world’s most famous radio telescopes, but has also played a key role in radio astronomy across the country and the world.
A study of rare megastorms on Saturn using data from the National Science Foundation’s Karl G. Jansky Very Large Array has revealed disruptions in the distribution of ammonia gas in the planet’s deep atmosphere. The findings raise questions about just how different gas giants can be from each other, and challenge scientists’ understanding of how megastorms may form on planets other than Earth. The results of the study appear in Science Advances.
Although the location of St. Croix is perfect for a VLBA antenna, the island poses significant challenges for using and maintaining a radio antenna. The St. Croix dish is located on the eastern side of the island, almost at sea level. So it is constantly bombarded by salt air, ocean rains, and even the occasional tropical storm.
Fast radio bursts are powerful flashes of light that shine for only milliseconds. Join our host Summer Ash of the National Radio Astronomy Observatory as she talks about how astronomers study these mysterious bursts, and what might be causing them.
Scientists using the Atacama Large Millimeter/submillimeter Array (ALMA) to study the protoplanetary disk around a young star have discovered the most compelling chemical evidence to date of the formation of protoplanets.
While studying classical novae using the National Radio Astronomy Observatory’s Very Long Baseline Array (VLBA), a graduate researcher uncovered evidence the objects may have been erroneously typecast as simple. The new observations, which detected non-thermal emission from a classical nova with a dwarf companion, were presented today at a press conference during the 242nd proceedings of the American Astronomical Society in Albuquerque, New Mexico.
Tras estudiar estrellas novas clásicas con el Long Baseline Array (VLBA) del Observatorio Radioastronómico Nacional de Estados Unidos, una estudiante de posgrado descubrió pistas de que estos objetos no son tan simples como se creía. Las nuevas observaciones, en las que se detectaron emisiones no térmicas de una nova clásica con un objeto compañero enano, se presentaron hoy durante la 242 asamblea de la Sociedad Astronómica de Estados Unidos, celebrada en Albuquerque (Nuevo México).
New scientific results from the Very Long Baseline Array (VLBA), the Very Large Array (VLA), and the Green Bank Observatory (GBO) will be revealed at multiple press conferences during the 242nd meeting of the American Astronomical Society (AAS) from June 5-7, in Albuquerque, New Mexico.The AAS meeting includes a series of press conferences based on a range of themes.
Two student researchers from the National Radio Astronomy Observatory’s National Astronomy Consortium (NAC) program were each awarded the prestigious Chambliss Astronomy Achievement Student Awards medal during the 241st proceedings of the American Astronomical Society (AAS).
Scientists studying the supermassive black hole at the heart of the M87 galaxy have revealed the origins of the monster’s powerful jet and imaged the jet and its source together for the first time. What’s more, the observations have revealed that the black hole’s ring is much larger than scientists previously believed.
Un equipo científico que estudió el agujero negro supermasivo presente en el corazón de la galaxia M87 reveló los orígenes de su poderoso chorro y logró obtener las primeras imágenes del chorro y su fuente juntos. Las observaciones también revelaron que el anillo del agujero negro es mucho más grande de lo que la comunidad científica creía.
As a part of its central mission to nurture and inspire the next generation of radio astronomers, the National Science Foundation’s National Radio Astronomy Observatory (NRAO) has selected four outstanding early career professionals for its 2023 Jansky Fellowship.
Artificial lasers on Earth are used for everything from scanning grocery items to delicate surgery. But there are also naturally occurring lasers known as astrophysical masers. Join National Radio Astronomy Observatory as we explore what these “space lasers” tell astronomers about the Universe.
On March 13th, 2023, astronomers around the world will mark the 10th anniversary of the inauguration of the Atacama Large Millimeter/submillimeter Array (ALMA), the world’s largest radio telescope. Over the past decade, the international ALMA collaboration— led by the U.S. National Science Foundation’s National Radio Astronomy Observatory (NRAO), the European Southern Observatory (ESO), and the National Astronomical Observatory of Japan (NAOJ)— has revolutionized our understanding of the Universe and unveiled its secrets, from the formation of planets, stars, and galaxies to deciphering the chemistry of the cosmos, and even taking part in capturing the first images of black holes.
Scientists studying a nearby protostar have detected the presence of water in its circumstellar disk. The new observations made with the Atacama Large Millimeter/submillimeter Array (ALMA) mark the first detection of water being inherited into a protoplanetary disk without significant changes to its composition. These results further suggest that the water in our Solar System formed billions of years before the Sun.
Un equipo científico detectó agua en el disco circumestelar de una protoestrella cercana gracias al Atacama Large Millimeter/submillimeter Array (ALMA). Es la primera vez que se observa agua depositándose en un disco protoplanetario sin que se produzcan cambios significativos en su composición. Este hallazgo permite suponer que el agua presente en nuestro Sistema Solar se formó miles de millones de años antes que el Sol.
While studying galaxies in the early Universe with the Atacama Large Millimeter/submillimeter Array (ALMA), scientists discovered one of the most extreme galaxies ever recorded in the early Universe. What’s more, it was hiding a unique supermassive black hole (SMBH). The observations could unlock clues about the early formation of these violent giants and how to find them.
The Board of the Atacama Large Millimeter/submillimeter Array (ALMA)— an international collaboration in which the National Science Foundation’s National Radio Astronomy Observatory (NRAO) is a partner— has approved multi-million dollar upgrades for the development of a second-generation correlator and a digital transmission system (DTS).
El directorio del Atacama Large Millimeter/submillimeter Array (ALMA), una colaboración internacional de la que forma parte el Observatorio Radioastronómico Nacional de la Fundación Nacional de Ciencia de Estados Unidos (NRAO, en su sigla en inglés), aprobó un proyecto por varios millones de dólares para desarrollar un correlacionador y un sistema de transmisión digital de segunda generación. Con esta iniciativa, enmarcada en el proyecto de incremento de la sensibilidad de banda amplia de ALMA, se busca duplicar y, eventualmente, cuadruplicar el ancho de banda correlacionado del conjunto de antenas.
The Universe is a dynamic and exciting place, with stars, planets, and galaxies being born, dying, and undergoing dramatic changes. In 2022, the telescopes of the National Science Foundation's National Radio Astronomy Observatory (NRAO) revealed fascinating new details about several of these processes, and we're giving you a taste of the greatest radio astronomy moments of the year.
Radio telescopes are powerful tools that allow astronomers to study the Universe. We often read about the discoveries they make, but we rarely get a glimpse of the engineers and technicians that design and build these telescopes. Join our host Summer Ash as she talks about NRAO’s Central Development Laboratory (CDL) and how CDL helps make modern radio astronomy a reality.
The National Science Foundation (NSF) and SpaceX have finalized a radio spectrum coordination agreement to limit interference from the company’s Starlink satellites to radio astronomy assets operating between 10.6 and 10.7 GHz. The agreement, detailed in a statement released by NSF today, ensures that Starlink satellite network plans will meet international radio astronomy protection standards, and protect NSF-funded radio astronomy facilities, including the National Radio Astronomy Observatory (NRAO) and the Green Bank Observatory (GBO).
While studying a nearby pair of merging galaxies using the Atacama Large Millimeter/submillimeter Array (ALMA)— an international observatory co-operated by the U.S. National Science Foundation’s National Radio Astronomy Observatory (NRAO)— scientists discovered two supermassive black holes growing simultaneously near the center of the newly coalescing galaxy. These super-hungry giants are the closest together that scientists have ever observed in multiple wavelengths. What’s more, the new research reveals that binary black holes and the galaxy mergers that create them may be surprisingly commonplace in the Universe. The results of the new research were published today in The Astrophysical Journal Letters, and presented in a press conference at the 241st meeting of the American Astronomical Society (AAS) in Seattle, Washington.
Mientras usaba el Atacama Large Millimeter/submillimeter Array (ALMA) para estudiar los máseres presentes alrededor de la inusual estrella MWC 349A, un equipo científico descubrió algo inesperado: un desconocido chorro de material emanando del disco de gas de la estrella a velocidades inverosímiles. Se cree, además, que el chorro es generado por intensas fuerzas magnéticas presentes alrededor de la estrella. El hallazgo podría ayudar a la comunidad científica a entender la naturaleza y la evolución de las estrellas masivas, y entender cómo los máseres de hidrógeno se forman en el espacio. Las nuevas observaciones se presentaron hoy durante una conferencia de prensa en la asamblea n.o 241 de la Sociedad Astronómica de Estados Unidos (AAS, en su sigla en inglés) en Seattle (Washington, Estados Unidos).
Mientras estudiaban una dupla de galaxias en colisión cercanas con el Atacama Large Millimeter/submillimeter Array (ALMA) —un observatorio internacional coadministrado por el Observatorio Radioastronómico Nacional (NRAO, en su sigla en inglés) de la Fundación Nacional de Ciencia de Estados Unidos—, un equipo científico descubrió dos agujeros negros supermasivos creciendo juntos cerca del centro de la nueva galaxia en ciernes. Es la primera vez que se observa en longitudes de onda múltiples a dos mastodontes hambrientos como estos tan cerca el uno del otro. El estudio también reveló que los agujeros negros binarios y las galaxias en colisión que los originan pueden ser fenómenos sorprendentemente comunes en el Universo. Los resultados de esta investigación se publicaron hoy en la revista The Astrophysical Journal Letters se presentaron durante una conferencia de prensa en la asamblea n.o 241 de la Sociedad Astronómica de Estados Unidos (AAS, en su sigla en inglés) en Seattle (Washington
While using the Atacama Large Millimeter/submillimeter Array (ALMA) to study the masers around oddball star MWC 349A scientists discovered something unexpected: a previously unseen jet of material launching from the star’s gas disk at impossibly high speeds. What’s more, they believe the jet is caused by strong magnetic forces surrounding the star. The discovery could help researchers to understand the nature and evolution of massive stars and how hydrogen masers are formed in space. The new observations were presented today in a press conference at the 241st meeting of the American Astronomical Society (AAS) in Seattle, Washington.
Shockwaves resulting from the violent collision between an intruder galaxy and Stephan’s Quintet are helping astronomers to understand how turbulence influences gas in the intergalactic medium. New observations with the Atacama Large Millimeter/submillimeter Array (ALMA) and the James Webb Space Telescope (JWST) have revealed that a sonic boom several times the size of the Milky Way has kickstarted a recycling plant for warm and cold molecular hydrogen gas. What’s more, scientists uncovered the break-up of a giant cloud into a fog of warm gas, the possible collision of two clouds forming a splash of warm gas around them, and the formation of a new galaxy. The observations were presented today in a press conference at the 241st meeting of the American Astronomical Society (AAS) in Seattle, Washington.
Las ondas de choque generadas por la violenta colisión entre una galaxia intrusa y el Quinteto de Stephan están ayudando a la comunidad astronómica a entender cómo la turbulencia incide en el gas presente en el medio intergaláctico. Las nuevas observaciones realizadas con el Atacama Large Millimeter/submillimeter Array (ALMA) y el telescopio espacial James Webb revelaron que una explosión sónica varias veces más grande que la Vía Láctea dio origen a un proceso de reciclaje de gas de hidrógeno molecular frío y caliente. También se observó la desintegración de una nube gigante que se convirtió en una niebla de gas caliente, así como la posible colisión de dos nubes que dejaron una mancha de gas caliente a su alrededor y la formación de una nueva galaxia. Los resultados de estas observaciones se presentaron hoy durante una conferencia de prensa en la asamblea n.o 241 de la Sociedad Astronómica de Estados Unidos (AAS, en su sigla en inglés) en Seattle (Washington, Estados Unidos).
Five new scientific results from the Atacama Large Millimeter/submillimeter Array (ALMA), the Very Large Array (VLA), and the Green Bank Observatory (GBO) will be revealed at multiple press conferences during the 241st meeting of the American Astronomical Society (AAS) from January 8 to 12, 2023, in Seattle, Wash.
El diseño del prototipo de antena para el ngVLA pasó por un cuidadoso proceso de revisión por un panel experto y ahora obtuvo el visto bueno para pasar a la etapa de fabricación del prototipo.
The design for the ngVLA prototype antenna has passed a thorough review by a panel of external experts and the project now is cleared to proceed to manufacture the prototype.
Dos artículos científicos publicados recientemente muestran cómo estos telescopios están ayudando a la comunidad científica a conocer mejor el planeta más grande de nuestro sistema solar, Júpiter, y su luna más cercana, Io.
In the center of the Milky Way there is a black hole more massive than 4 million Suns. It’s known as Sagittarius A, or Sgr A*, and it’s hidden behind the dust of our galactic center. So how can astronomers see it? Join our host Summer Ash of the National Radio Astronomy Observatory as she talks about how radio astronomers captured the first direct image of the monster black hole in our backyard.
VLA observations revealed that cosmic rays can play an important role in driving winds that rob galaxies of the gas needed to form new stars. This mechanism may be important in galactic evolution, particularly at earlier times in the history of the universe.
Gracias al Very Large Array, un equipo de astrónomos y astrónomas descubrió una importante pista sobre cómo las galaxias ponen freno a frenéticos episodios de formación estelar.
The European Microwave Association (EuMA) has announced Marian Pospieszalski— a senior research engineer at the National Science Foundation’s National Radio Astronomy Observatory (NRAO)— as the recipient of its 2022 Pioneer Award. The EuMA Pioneer Award recognizes individuals responsible for noteworthy advances in the field of microwaves that have had a lasting and significant impact on the microwave community.
Following a generous grant from the National Science Foundation’s Spectrum Innovation Initiative (SII), NSF’s National Radio Astronomy Observatory (NRAO) will expand efforts to establish and support the co-existence of research and commercial entities across the radio spectrum.