An international team of astronomers used ALMA to capture high-resolution images of eight protoplanetary disks in the Sigma Orionis cluster, which is irradiated by intense ultraviolet light from a massive nearby star. To their surprise, they found evidence of gaps and rings in most of the disks—structures commonly associated with the formation of giant planets, like Jupiter.
Recent News
Astronomers Discover New Building Blocks for Complex Organic Matter
There should be a lot of carbon in space, but surprisingly, it’s not always easy to find. While it can be observed in many places, it doesn’t add up to the volume astronomers would expect to see. The discovery of a new, complex molecule (1-cyanopyrene), challenges these expectations, about where the building blocks for carbon are found, and how they evolve.
Massive Stars Born from Violent Cosmic Collapse
An international team of astronomers has observed evidence that massive stars can be born from rapidly collapsing clouds of gas and dust, challenging long-held assumptions about star formation.
Radio Astronomy and Black Holes
How a Telescope Made Mostly of Nothing Became Astronomy’s ‘Killer App’
Astronomers have captured the first direct visual evidence of a black hole at the center of Messier 87 (M87), a giant elliptical galaxy 55 million light-years
from Earth. This unprecedented observation was made possible by the Event Horizon Telescope (EHT), an array of eight individual radio telescopes spread over four continents and linked together to form a new, exceptionally powerful telescope. The newly released image reveals a glowing ring-like structure with a dark central region — a feature known as the “shadow” of a black hole.
As the most sensitive and largest element of the EHT, the Atacama Large Millimeter/submillimeter Array (ALMA) in Chile was instrumental in making this observation possible. With ALMA, the EHT achieved one of the highest resolutions ever in astronomy, 20 microarcseconds. A microarcseconds is about the size of the period at the end of this sentence if you were looking from the Moon. These observations will help scientists understand how the universe behaves under conditions of extreme gravity, forces so strong that they warp the fabric of space and time. This is just the latest step in a journey that began nearly 50 years ago with the National Radio Astronomy Observatory’s (NRAO) Green Bank Interferometer: the first telescope to identify and locate the supermassive black hole at the center of the Milky Way. The EHT is a turbo-powered version of that pioneering telescope.
The full EHT story, including background on black holes and supporting materials can be found at the National Science Foundation’s special section: “Exploring Black Holes.”
NRAO Contacts:
Kazunori Akiyama
The NRAO Jansky fellow at MIT Haystack Observatory who developed new imaging techniques for the EHT and led international efforts to create the first images of the supermassive black hole in M87 as a coordinator of the imaging group.
617-715-5579; [email protected]
Charles E. Blue
Public Information Officer
National Radio Astronomy Observatory
434-296-0314; [email protected]
Recent News
ALMA Reveals Planets Can Form Under Harsh Radiation
An international team of astronomers used ALMA to capture high-resolution images of eight protoplanetary disks in the Sigma Orionis cluster, which is irradiated by intense ultraviolet light from a massive nearby star. To their surprise, they found evidence of gaps and rings in most of the disks—structures commonly associated with the formation of giant planets, like Jupiter.
Astronomers Discover New Building Blocks for Complex Organic Matter
There should be a lot of carbon in space, but surprisingly, it’s not always easy to find. While it can be observed in many places, it doesn’t add up to the volume astronomers would expect to see. The discovery of a new, complex molecule (1-cyanopyrene), challenges these expectations, about where the building blocks for carbon are found, and how they evolve.
Massive Stars Born from Violent Cosmic Collapse
An international team of astronomers has observed evidence that massive stars can be born from rapidly collapsing clouds of gas and dust, challenging long-held assumptions about star formation.