Black Hole Explorer Hopes to Reveal New Details of Supermassive Black Holes

A new agreement between the Center for Astrophysics | Harvard & Smithsonian (CfA) and the U.S. National Science Foundation National Radio Astronomy Observatory (NSF NRAO) will help the Event Horizon Telescope (EHT) take its next steps – into space.

The EHT made headlines around the world in 2019 after it took the first images of a black hole, and then in 2022, imaged the supermassive black hole at the heart of the Milky Way galaxy. The Black Hole Explorer (BHEX) mission would extend this work by combining several of NRAO’s ground-based radio antennas with a space-based telescope to produce the most detailed images in history. BHEX would allow scientists to reveal the light that orbits the edge of a black hole before it escapes, known as a photon ring.

Astronomers Discover Magnetic Loops Around Supermassive Black Hole

NGC 1068 is a well-known, relatively nearby, bright galaxy with a supermassive black hole at its center. Despite its status as a popular target for astronomers, however, its accretion disk is obscured by thick clouds of dust and gas. A few light-years in diameter, the outer accretion disk is dotted by hundreds of distinct water maser sources that hinted for decades at deeper structures. Masers are distinct beacons of electromagnetic radiation that shine in microwave or radio wavelengths; in radio astronomy, water masers observed at a frequency of 22 GHz are particularly useful because they can shine through much of the dust and gas that obscures optical wavelengths.

Led by astronomer Jack Gallimore of Bucknell University, an international team of astronomers and students set out to observe NGC 1068 with twin goals in mind: astrometric mapping of the galaxy’s radio continuum and measurements of polarization for its water masers. “NGC 1068 is a bit of a VIP among active galaxies,”

UC Irvine researchers reveal superconductivity secrets of an iron-based material

Irvine, Calif., Dec. 5, 2024 — Scientists at the University of California, Irvine have uncovered the atomic-scale mechanics that enhance superconductivity in an iron-based material, a finding published recently in Nature. Using advanced spectroscopy instruments housed in the UC Irvine Materials Research Institute, the researchers were able to image atom vibrations and thereby observe new phonons –quasiparticles that carry thermal energy –at the interface of an iron selenide (FeSe) ultrathin film layered on a strontium titanate (STO) substrate.

Scientists prepare for the most ambitious sky survey yet, anticipating new insight on dark matter and dark energy

Argonne scientists are contributing to the success of the Legacy Survey of Space and Time through advanced simulation, analysis and collaborative partnership.

PLANETS BEWARE: NASA UNBURIES DANGER ZONES OF STAR CLUSTER

Most stars form in collections, called clusters or associations, that include very massive stars. These giant stars send out large amounts of high-energy radiation, which can disrupt relatively fragile disks of dust and gas that are in the process of coalescing to form new planets.

A team of astronomers used NASA’s Chandra X-ray Observatory, in combination with ultraviolet, optical, and infrared data, to show where some of the most treacherous places in a star cluster may be, where planets’ chances to form are diminished.

A Cosmic Chemical Breakthrough: Astronomers Discover New Building Blocks for Complex Organic Matter

The element carbon is a building block for life, both on Earth and potentially elsewhere in the vast reaches of space. 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. This research was published today in the journal Science.

NASA’s Hubble, New Horizons Team Up for a Simultaneous Look at Uranus

Uranus, the planet second most distant from our Sun, has been described as mysterious, strange, and fairly unknown to those of us here on Earth. However, in astronomy, these terms are pretty relative. Compared to the remote, dark stretches of the early universe or oddball exoplanets dozens of light-years from our solar system, researchers actually know a lot about Uranus.

Q&A: UW researchers examine link between light pollution and interest in astronomy

Rodolfo Cortes Barragan, research scientist the University of Washington Institute for Learning and Brain Sciences (I-LABS), and Andrew Meltzoff, co-director of I-LABS and professor of psychology, recently co-authored a study in Nature Scientific Reports showing a link between the ability to see the stars unblocked by light pollution and an interest in astronomy.

NSF–DOE Rubin Observatory’s Unparalleled Vision Will Revolutionize Multi-Messenger Astronomy

Photons, neutrinos, cosmic rays and gravitational waves all carry information about the Universe. Multi-messenger astronomy brings together these four signals to investigate astronomical events from multiple cosmic perspectives.

Smithsonian Scientists Help Uncover How The Solar Wind Gets Its Energy

Since the 1960s, astronomers have wondered how the Sun’s supersonic “solar wind,” a stream of energetic particles that flows out into the Solar System, continues to receive energy once it leaves the Sun. Now, thanks to a lucky line up of two spacecraft currently in space studying the Sun, they may have discovered the answer.

UC Irvine astronomers’ simulations support dark matter theory

Computer simulations by astronomers support the idea that dark matter – matter that no one has yet directly detected but which many physicists think must be there to explain several aspects of the observable universe – exists, according to the researchers, who include those at the University of California, Irvine.

SETI institute employs SETI ellipsoid technique for searching for signals from distant civilizations

In a paper published in the Astronomical Journal, a team of researchers from the SETI Institute, Berkeley SETI Research Center and the University of Washington reported an exciting development for the field of astrophysics and the search for extraterrestrial intelligence (SETI), using observations from the Transiting Exoplanet Survey Satellite (TESS) mission to monitor the SETI Ellipsoid, a method for identifying potential signals from advanced civilizations in the cosmos.