Matt Williams, Author at Universe Today

January 24, 2025January 24, 2025 by Matt Williams

Vera Rubin Completes its Comprehensive System Tests

A drone's view of the Rubin Observatory under construction in 2023. The 8.4-meter telescope is getting closer to completion and first light in 2025. The telescope will create a vast amount of data that will require special resources to manage, including AI. Image Credit: Rubin Observatory/NSF/AURA/A. Pizarro D

The Vera C. Rubin Observatory, previously known as the Large Synoptic Survey Telescope (LSST), will be the first observatory of its kind. Jointly funded by the National Science Foundation (NSF) and the Department of Energy (DOE), Rubin will conduct the Legacy Survey of Space and Time (LSST) – a 10-year survey of the southern hemisphere. The observatory is expected to collect 15 terabytes of data a night, which will be used to create an ultra-wide, ultra-high-definition, time-lapse record of the cosmos, containing tens of billions of stars, galaxies, and astronomical objects.

After ten years of construction, the Vera C. Rubin Observatory is less than one year away from starting this revolutionary observation campaign. In preparation for this, the observatory recently completed a series of full-system tests using an engineering test camera. With this milestone complete, the stage is now set for the installation of the 3200-megapixel LSST Camera (LSSTCam), the world’s largest digital camera. Once mounted on the Simonyi Survey Telescope, the observatory will have finished construction and be ready to collect its first light.

January 22, 2025January 22, 2025 by Matt Williams

Black Hole Jets Seen Forming in Real-Time

Artist's impression of a white dwarf embedded in the disk of a giant black hole. Credit: NASA/Sonoma State University, Aurore Simonnet

A short time ago, astronomers observed a distant supermassive black hole (SMBH) located in a galaxy 270 million light-years away in the constellation Draco. For years, this galaxy (1ES 1927+654) has been the focus of attention because of the Active Galactic Nucleus (AGN) at its core. It all began in 2018 when the SMBH’s X-ray corona mysteriously disappeared, followed by a major outburst in the optical, ultraviolet, and X-ray wavelengths. Astronomers began watching it closely, but what they saw next was completely unexpected!

As we covered in a previous article, much of the excitement was generated by the SMBH’s behavior, which suggested it was consuming a stellar remnant (a white dwarf). In addition, astronomers noted a huge increase in radio emissions and the formation of plasma jets extending from the black hole, which all happened over the course of a year. In a new paper, a team led by the University of Maryland Baltimore County (UMBC) describes how they watched a plasma jet forming in real time, something astronomers have never done before.

January 18, 2025January 18, 2025 by Matt Williams

NASA is Building a Space Telescope to Observe Exoplanet Atmospheres

Artist's impression of the Pandora mission observing a transiting exoplanet. Credit: NASA’s Goddard Space Flight Center/Conceptual Image Lab

The exoplanet census continues to grow. Currently, 5,819 exoplanets have been confirmed in 4,346 star systems, while thousands more await confirmation. The vast majority of these planets were detected in the past twenty years, owing to missions like the Kepler Space Telescope, the Transiting Exoplanet Survey Satellite (TESS), the venerable Hubble, the Convection, Rotation and planetary Transits (CoRoT) mission, and more. Thousands more are expected as the James Webb Space Telescope continues its mission and is joined by the Nancy Grace Roman Space Telescope (RST).

In the meantime, astronomers will soon have another advanced observatory to help search for potentially habitable exoplanets. It’s called Pandora, a small satellite that was selected in 2021 as part of NASA’s call for Pioneer mission concepts. This observatory is designed to study planets detected by other missions by studying these planets’ atmospheres of exoplanets and the activity of their host stars with long-duration multiwavelength observations. The mission is one step closer to launch with the completion of the spacecraft bus, which provides the structure, power, and other systems.

January 17, 2025January 17, 2025 by Matt Williams

New Glenn Reaches Orbit, but Doesn't Recover the Booster

Blue Origin's New Glenn rocket launching on January 16th, 2025. Credit: Blue Origin

On Thursday, January 16th, at 02:03 AM EST, Blue Origin’s New Glenn rocket took off on its maiden flight from Launch Complex 36 at Cape Canaveral Space Force Station. This was a momentous event for the company, as the two-stage heavy-lift rocket has been in development for many years, features a partially reusable design, and is vital to Bezos’ plan of “building a road to space.” While the company failed to retrieve the first-stage booster during the flight test, the rocket made it to orbit and successfully deployed its payload -the Blue Ring Pathfinder – to orbit (which has since begun gathering data).

According to the most recent statement by Blue Origin, the second stage reached its final orbit following two successful burns of its two BE-3U engines. The successful launch of NG-1 means that Blue Origin can now launch payloads to Low Earth Orbit (LEO), a huge milestone for the commercial space company. “I’m incredibly proud New Glenn achieved orbit on its first attempt,” said Blue Origin CEO Dave Limp in a company statement. “We knew landing our booster, So You’re Telling Me There’s a Chance, on the first try was an ambitious goal. We’ll learn a lot from today and try again at our next launch this spring. Thank you to all of Team Blue for this incredible milestone.”

January 16, 2025January 16, 2025 by Matt Williams

Webb and ALMA Team Up to Study Primeval Galaxy

The radio telescope array ALMA has pin-pointed the exact cosmic age of a distant JWST-identified galaxy, GHZ2/GLASS-z12, at 367 million years after the Big Bang. Image Credit: NASA/ESA/CSA/T. Treu, UCLA/NAOJ/T. Bakx, Nagoya U.

One of the most exciting developments in modern astronomy is how astronomers can now observe and study the earliest galaxies in the Universe. This is due to next-generation observatories like the James Webb Space Telescope (JWST), with its sophisticated suite of infrared instruments and spectrometers, and advances in interferometry – a technique that combines multiple sources of light to get a clearer picture of astronomical objects. Thanks to these observations, astronomers can learn more about how the earliest galaxies in the Universe evolved to become what we see today.

Using Webb and the Atacama Large Millimeter/submillimeter Array (ALMA), an international team led by researchers from the National Astronomical Observatory of Japan (NAOJ) successfully detected atomic transitions coming from galaxy GHZ2 (aka. GLASS-z12), located 13.4 billion light-years away. Their study not only set a new record for the farthest detection of these elements This is the first time such emissions have been detected in galaxies more than 13 billion light-years away and offers the first direct insights into the properties of the earliest galaxies in the Universe.

January 15, 2025January 20, 2025 by Matt Williams

Recent Observations Challenge our Understanding of Giant Black Holes

Black holes are among the most mysterious and powerful objects in the Universe. These behemoths form when sufficiently massive stars reach the end of their life cycle and experience gravitational collapse, shedding their outer layers in a supernova. Their existence was illustrated by the work of German astronomer Karl Schwarzschild and Indian-American physicist Subrahmanyan Chandrasekhar as a consequence of Einstein’s Theory of General Relativity. By the 1970s, astronomers confirmed that supermassive black holes (SMBHs) reside at the center of massive galaxies and play a vital role in their evolution.

However, only in recent years were the first images of black holes acquired by the Event Horizon Telescope (EHT). These and other observations have revealed things about black holes that have challenged preconceived notions. In a recent study led by a team from MIT, astronomers observed oscillations that suggested an SMBH in a neighboring galaxy was consuming a white dwarf. But instead of pulling it apart, as astronomical models predict, their observations suggest the white dwarf was slowing down as it descended into the black hole – something astronomers have never seen before!

January 13, 2025January 13, 2025 by Matt Williams

LIGO Fails to Find Continuous Gravitational Waves From Pulsars

Illustration of a pulsar with powerful magnetic fields. Credit: NASA's Goddard Flight Center/Walt Feimer

In February 2016, scientists working for the Laser Interferometer Gravitational-Wave Observatory (LIGO) made history by announcing the first-ever detection of gravitational waves (GW). These waves, predicted by Einstein’s Theory of General Relativity, are created when massive objects collide (neutron stars or black holes), causing ripples in spacetime that can be detected millions or billions of light years away. Since their discovery, astrophysicists have been finding applications for GW astronomy, which include probing the interiors of neutron stars.

For instance, scientists believe that probing the continuous gravitational wave (CW) emissions from neutron stars will reveal data on their internal structure and equation of state and can provide tests of General Relativity. In a recent study, members of the LIGO-Virgo-KAGRA (LVK) Collaboration conducted a search for CWs from 45 known pulsars. While their results showed no signs of CWs emanating from their sample of pulsars, their work does establish upper and lower limits on the signal amplitude, potentially aiding future searches.

January 12, 2025January 12, 2025 by Matt Williams

Planets Can Form in Even the Harshest Conditions

Artist concept of planet formation occuring in harsh stellar environments. Credit: NSF/AUI/NSF NRAO/S.Dagnello.

According to the most widely held astronomical model (the Nebular Hypothesis), new stars are born from massive clouds of dust and gas (aka. a nebula) that experience gravitational collapse. The remaining dust and gas form a protoplanetary disk that encircles the new star, which slowly accretes to form systems of planets. For the past decade, astronomers have relied on the Atacama Large Millimeter/submillimeter Array (ALMA) in Chile to study young stars and their disks and learn more about how this process occurs.

In a recent study, an international team of astronomers used ALMA to capture high-resolution images of eight protoplanetary disks in the Sigma Orionis cluster, a group of stars located in the constellation Orion. During their observations, the team found evidence of gaps and rings in most of the disks, which are potential indications that giant planets are forming. This was surprising, seeing as how these disks are irradiated by intense ultraviolet (UV) radiation from a massive star in the cluster. Their findings suggest that planet formation can occur in conditions that were previously thought to be inhospitable.

January 11, 2025January 11, 2025 by Matt Williams

NASA is Sending a Vacuum Cleaner to the Moon

The Lunar Planet Vac, or LPV, is one of 10 payloads set to be carried to the Moon by the Blue Ghost 1 lunar lander in 2025. Credit: Firefly Aerospace

By the end of this decade, NASA, the Chinese National Space Agency (CNSA), Roscosmos, and other space agencies plan to establish a sustained human presence on the Moon. A crucial aspect of these plans is using local resources (particularly water) to lessen dependence on Earth, a process known as in-situ resource utilization (ISRU). Hence why NASA plans to establish a base of operations around the lunar south pole, a heavily cratered region where water ice exists in abundance in permanently shadowed regions (PSRs).

To harvest water ice and other resources successfully, NASA is investing in technologies that will enable cost-effective sample collection, in-situ testing (with or without astronaut oversight), and real-time data transmission to Earth. One such technology is the Lunar PlanetVac (LPV), a sample acquisition and delivery system designed to collect and transfer lunar regolith to sample containers without reliance on gravity. The LPV is one of 10 payloads that will be flown to the lunar surface as part of NASA’s Commercial Lunar Payload Services (CLPS) program.

January 10, 2025January 10, 2025 by Matt Williams

It's Time for Sustainable Development Goal for Space

The destruction of a single satellite could be catastrophic for our orbital endeavours. Image Credit: ESA

In 2015, the United Nations adopted the 2030 Agenda for Sustainable Development—the Sustainable Development Goals (SDGs)—a universal call to action to protect the planet for future generations and ensure that all people will enjoy peace and prosperity. These 17 goals included the elimination of poverty, hunger, and inequalities, the promotion of education, and the promotion of sustainable development worldwide. With the rapid development in Low Earth Orbit (LEO), there are growing concerns that an 18th SDG should be adopted for space.

This goal calls for the sustainable use of Earth’s orbit by space agencies and commercial industry and the prevention of the accumulation of space junk. This has become a growing problem in recent years thanks to the deployment of satellite mega-constellations and the “commercialization of LEO.” In a recent study led by the University of Plymouth, a team of experts outlined how the lessons learned from marine debris mitigation could be applied to space so that future generations can live in a world where space truly is “for all humanity.”