Huge Release of Type 1a Supernovae Data

Nighttime long exposure of the open Samuel Oschin Telescope dome at Palomar Observatory in California. © Palomar/Caltech

Type 1a supernovae are extremely powerful events that occur in binary systems containing at least one white dwarf star – the core remnant of a Sun-like star. Sometimes, the white dwarf’s powerful gravity will siphon material from its companion star until it reaches critical mass and explodes. In another scenario, a binary system of two white dwarfs will merge, producing the critical mass needed for a supernova. Unlike regular supernovae, which occur every fifty years in the Milky Way, Type Ia supernovae happen roughly once every five hundred years.

In addition to being incredible events, Type 1a supernovae are useful astronometric tools. As part of the Cosmic Distance Ladder, these explosions allow astronomers to measure the distances to objects millions or billions of light-years away. This is vital to measuring the rate at which the Universe is expanding, otherwise known as the Hubble Constant. Thanks to an international team of researchers, a catalog of Type 1a Supernovae has just been released that could change what we know of the fundamental physics of supernovae and the expansion history of the Universe.

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Stunning 80 Megapixel Image of a Stellar Nursery

This is an 80-million-pixel picture of the star cluster RCW 38, located 5500 light-years away. Credit: ESO

RCW 38 is a molecular cloud of ionized hydrogen (HII) roughly 5,500 light-years from Earth in the direction of the constellation Vela. Located in this cloud is a massive star-forming cluster populated by young stars, short-lived massive stars, and protostars surrounded by clouds of brightly glowing gas. The European Southern Observatory (ESO) recently released a stunning 80-million-pixel image of the star cluster that features the bright streaks and swirls of RCW 38, the bright pink of its gas clouds, and its many young stars (which appear as multi-colored dots).

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Construction of Roman Continues With the Addition of its Sunshade

Technician Brenda Estavia is installing the innermost layer of the sunshade onto the deployable aperture cover structure of NASA’s Nancy Grace Roman Space Telescope. Credit: NASA/Jolearra Tshiteya

NASA continues to progress with the development of the Nancy Grace Roman Space Telescope (RST), the next-generation observatory with a target launch date of 2027. As the direct successor to the venerable Hubble Space Telescope, Roman will build on the successes of Hubble and the James Webb Space Telescope (JWST). Named after NASA’s first chief astronomer, the “mother of the Hubble,” the Nancy Grace Roman Space Telescope will have a panoramic field of view 200 times greater than Hubble’s infrared view, enabling the first wide-field maps of the Universe.

Combined with observations by the ESA’s Euclid mission, these maps will help astronomers resolve the mystery of Dark Matter and cosmic expansion. The development process reached another milestone as the mission team at NASA’s Goddard Space Flight Center successfully integrated the mission’s sunshade—a visor-like aperture cover—into the outer barrel assembly. This deployable structure will shield the telescope from sunlight and keep it at a stable temperature, allowing it to take high-resolution optical and infrared images of the cosmos.

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To Probe the Interior of Neutron Stars, We Must Study the Gravitational Waves from their Collisions

neutron star merger and gamma ray burst
Artistic representation of two merging neutron stars. Credit: Dana Berry, SkyWorks Digital, Inc.

When massive stars reach the end of their life cycle, they undergo gravitational collapse and shed their outer layers in a massive explosion (a supernova). Whereas particularly massive stars will leave a black hole in their wake, others leave behind a stellar remnant known as a neutron star (or white dwarf). These objects concentrate a mass greater than the entire Solar System into a volume measuring (on average) just 20 km (~12.5 mi) in diameter. Meanwhile, the extreme conditions inside neutron stars are still a mystery to astronomers.

In 2017, the first collision between two neutron stars was detected from the gravitational waves (GWs) it produced. Since then, astronomers have theorized how GWs could be used to probe the interiors of neutron stars and learn more about the extreme physics taking place. According to new research by a team from Goethe University Frankfurt and other institutions, the GWs produced by binary neutron star (BNS) mergers mere milliseconds after they merge could be the best means of probing the interiors of these mysterious objects.

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A New Study Reveals How Dark Matter Dominated the Early Universe

A view of the galaxy GN-z11, which harbors the oldest known black hole in the Universe. Courtesy: NASA, ESA, and P. Oesch (Yale University)
A view of the galaxy GN-z11, which harbors the oldest known black hole in the Universe. Courtesy: NASA, ESA, and P. Oesch (Yale University)

During the 1970s, while probing distant galaxies to determine their mass, size, and other characteristics, astronomers noticed something interesting. When examining the rate at which these galaxies rotated (their rotational curves), they found that the outer parts were rotating faster than expected. In short, their behavior suggested that they were far more massive than they appeared to be. This led to the theory that in addition to stars, gas, and dust, galaxies were surrounded by a “halo” of mysterious, invisible mass – what came to be known as Dark Matter (DM).

It was famed astronomer Vera C. Rubin, for whom the Vera C. Rubin Observatory (formerly the LSST) is named, who first proposed that DM played an important role in galactic evolution. Astronomers have since theorized that DM haloes must have existed shortly after the Big Bang and were integral to the formation of the first galaxies. In a recent study, an international team examined the core regions of two galaxies that existed 13 billion years ago. Their observations confirmed that DM dominated the haloes of these quasars, offering fresh insight into the evolution of galaxies in the very early Universe.

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Europa Clipper Tests its Star Tracker Navigation System

Artist's concept of a Europa Clipper mission. Credit: NASA/JPL

On October 14th, 2024, NASA’s Europa Clipper mission launched atop a Falcon Heavy rocket from Launch Complex 39A at the Kennedy Space Center in Florida. It will spend the next few years traveling 2.9 billion km (1.8 billion mi) to reach Jupiter’s moon Europa, arriving in April 2030. Once it arrives in the system, the probe will establish orbit and conduct 49 close flybys of this “Ocean World” and search for chemical elements that could indicate the presence of life (biosignatures) in the moon’s interior. By July 2031, it will be joined by the ESA’s Jupiter Icy Moon Explorer (JUICE), which will conduct a similar search around Callisto and Ganymede.

As is customary, the mission team has been checking and calibrating the Clipper’s instruments since launch to ensure everything is in working order. The latest test involved the probe’s stellar reference units (or star trackers), which captured and transmitted the Europa Clipper’s first images of space. These two imaging cameras look for stars, which mission controllers use to help orient the spacecraft. This is critical when pointing the probe’s telecommunications antennas toward Earth so it can send and receive critical mission data.

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Space Junk Could Re-Enter the Atmosphere in Busy Flight Areas

Debris and defunct launcher stages in the Geostationary ring. Credit: ESA/ID&Sense/ONiRiXEL

In the more than 60 years since the Space Age began, humans have sent more than 6,740 rockets to space. According to the ESA’s Space Debris Office, this has resulted in 56,450 objects in orbit; about 36,860 of these objects are regularly tracked and maintained in a catalog, while 10,200 are still functioning. The rest is a combination of spent rocket stages, defunct satellites, and pieces of debris caused by unused propellant exploding and orbital collisions. This is leading to a cascade effect known as Kessler Syndrome, where the amount of debris in orbit will lead to more collisions and more debris.

What’s worse, the situation is only projected to get worse since more launches are expected with every passing year. Last year, space agencies and commercial space companies conducted a record-breaking 263 launches, with the U.S. (158) and China (68) leading the way. And with future break-ups occurring at historic rates of 10 to 11 per year, the number of debris objects in orbit will continue to increase. According to a new study by a team from the University of British Columbia (UBC), this also means that debris falling to Earth will have a 1 in 4 chance per year of entering busy airspace.

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Water Arrived in the Final Stages of Earth's Formation

Artist concept of Earth during the Late Heavy Bombardment period. Credit: NASA's Goddard Space Flight Center Conceptual Image Lab.

Roughly 4.6 billion years ago, the Sun was born from the gas and dust of a nebula that underwent gravitational collapse. The remaining gas and dust settled into a protoplanetary disk that slowly accreted to form the planets, including Earth. About 4.5 billion years ago, our planet was impacted by a Mars-sized body (Theia), which led to the formation of the Moon. According to current theories, water was introduced to Earth and the inner planets by asteroids and comets that permeated the early Solar System.

The timing of this event is of major importance since the introduction of water was key to the origin of life on Earth. Exactly when this event occurred has been a mystery for some time, but astronomers generally thought it had arrived early during Earth’s formation. According to a recent study by a team led by scientists from the University of Rutgers-New Brunswick, water may have arrived near “late accretion” – the final stages of Earth’s formation. These findings could seriously affect our understanding of when life first emerged on Earth.

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This Hot Jupiter Probably Formed Close to Its Star

This artist's illustration shows an alien world that is losing magnesium and iron gas from its atmosphere. The observations represent the first time that so-called "heavy metals"—elements more massive than hydrogen and helium—have been detected escaping from a hot Jupiter, a large gaseous exoplanet orbiting very close to its star. The planet, known as WASP-121b, orbits a star brighter and hotter than the Sun. Image Credit: NASA, ESA, and J. Olmsted (STScI)

The current exoplanet census contains 5,832 confirmed candidates, with more than 7,500 still awaiting confirmation. Of those that have been confirmed, most have been gas giants ranging from Neptune-like bodies (1992) to those similar to or many times the size and mass of Jupiter and Saturn (1883). Like the gas giants of the Solar System, astronomers generally theorized that these types of planets form in the outer reaches of their star system, where conditions are cold enough for gases like hydrogen and helium and volatile compounds (water, ammonia, methane, etc.) will condense or freeze solid.

However, astronomers have noted that many of the gas giants they’ve observed orbited close to their stars, known as “Hot Jupiters.” This has raised questions about whether or not gas giants and other planets migrate after formation until they find their long-term, stable orbits. In a new study, a team from Arizona State University’s School Of Earth and Space Exploration (ASU-SESE) examined the atmospheric chemistry of several Hot and Ultra-Hot Jupiters. After examining WASP-121b, the team came to the unexpected conclusion that it likely formed close to its star.

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High-Resolution Imaging of Dyson Sphere Candidate Reveals no Radio Signals

A Type II civilization is one that can directly harvest the energy of its star using a Dyson Sphere or something similar. Credit: Fraser Cain (with Midjourney)

In the more than sixty years where scientists have engaged in the Search for Extraterrestrial Intelligence (SETI), several potential examples of technological activity (“technosignatures”) have been considered. While most SETI surveys to date have focused on potential radio signals from distant sources, scientists have expanded the search to include other possible examples. This includes other forms of communication (directed energy, neutrinos, gravitational waves, etc.) and examples of megastructures (Dyson Spheres, Clarke Bands, Niven Rings, etc.)

Examples of modern searches include Project Hephaistos, the first Swedish Project dedicated to SETI. Named in honor of the Greek god of blacksmiths, this Project is focused on the search for technosignatures in general rather than looking for signals deliberately sent toward Earth. In a recent paper, a team led by the University of Manchester examined a Dyson Sphere candidate identified by Hephaistos. Their results confirmed that at least some of these radio sources are contaminated by a background Active Galactic Nucleus (AGN).

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