Tag: astronomy

Why interstellar objects like ‘Oumuamua and Borisov may hold clues to exoplanets

On October 17 and 18, 2017, an unusual object sped across the field of view of a large telescope perched near the summit of a volcano on the Hawaiian island of Maui. The Pan-STARRS1 telescope was designed to survey the sky for transient events, like asteroid or comet flybys. But this was different: The object was not gravitationally bound to the Sun or to any other celestial body. It had arrived from somewhere else.

The mysterious object was the first visitor from interstellar space observed passing through the Solar System. Astronomers named it 1I/‘Oumuamua, borrowing a Hawaiian word that roughly translates to “messenger from afar arriving first.” Two years later, in August 2019, amateur astronomer Gennadiy Borisov discovered the only other known interstellar interloper, now called 2I/Borisov, using a self-built telescope at the MARGO observatory in Nauchnij, Crimea.

While typical asteroids and comets in the Solar System orbit the Sun, ‘Oumuamua and Borisov are celestial nomads, spending most of their time wandering interstellar space. The existence of such interlopers in the Solar System had been hypothesized, but scientists expected them to be rare. “I never thought we would see one,” says astrophysicist Susanne Pfalzner of the Jülich Supercomputing Center in Germany. At least not in her lifetime.

With these two discoveries, scientists now suspect that interstellar interlopers are much more common. Right now, within the orbit of Neptune alone, there could be around 10,000 ‘Oumuamua-size interstellar objects, estimates planetary scientist David Jewitt of UCLA, coauthor of an overview of the current understanding of interstellar interlopers in the 2023 Annual Review of Astronomy and Astrophysics.

Researchers are busy trying to answer basic questions about these alien objects, including where they come from and how they end up wandering the galaxy. Interlopers could also provide a new way to probe features of distant planetary systems.

But first, astronomers need to find more of them.

“We’re a little behind at the moment,” Jewitt says. “But we expect to see more.”

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CUTTING-EDGE ANALYSIS OF THE WINCHCOMBE METEORITE CONFIRMS PRESENCE OF LIFE-SUPPORTING ORGANIC COMPOUNDS

German researchers using a cutting-edge, chemical-free detection method have confirmed the presence of organic compounds in the Winchcombe Meteorite, including nitrogen and amino acids. The new findings confirm similar results from a previous analysis of the well-known space rock, although this is the first time such a detection was made without chemical treatments.

“The team of researchers are now the first to demonstrate, to a high degree of precision, the existence of some important nitrogen compounds in this meteorite with amino acids and heterocyclic hydrocarbons – without applying any chemical treatment, and by using a new type of detector design,” a press release announcing the findings explains.

WITNESSES SPOTTED WINCHCOMBE METEORITE FALLING OVER ENGLAND IN 2021

The Winchcombe meteorite gained some level of media attention after it was witnessed by a network of cameras falling from the sky over Winchcombe, England, in February 2021. This allowed researchers to locate it within days, offering those who study space rocks one of the most pristine specimens ever collected.

“Normally, meteorites are tracked down in the cold and hot deserts on Earth, where the dry climate means that they don’t weather very fast, but they do change as a result of humidity,” explained Dr. Christian Vollmer from the Institute of Mineralogy at Münster University. “If a meteorite fall is observed soon after the event and the meteorite is quickly collected, as was the case in Winchcombe, they are important ‘witnesses’ for us regarding the birth of our solar system – which makes them especially interesting for research purposes.”

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SOMETHING IS ORBITING THESE DISTANT EXOPLANETS AFTER ALL, ACCORDING TO RESEARCHERS WHO FIRE BACK OVER EXOMOON CONTROVERSY

The search for exomoons orbiting planets outside our solar system has sparked a significant debate within the astronomical community, involving a pair of contrasting studies that presented divergent viewpoints on the existence of exomoons Kepler-1625b-i and Kepler-1708b-i.

Much like Schrödinger’s oddball cat that is both dead and alive inside a box, we won’t really know until someone goes and looks. But in a new paper recently uploaded to the arXiv preprint server, a team of astronomers led by David Kipping from Columbia University takes issue with the drama surrounding the ongoing exomoon search. 

In 2017, Kipping, alongside Columbia University astronomer Alex Teachey, discovered the first possible exomoon candidate, Kepler-1625b-i, using the Hubble and Kepler telescopes. Years later, in 2022, Kipping, as well as astronomers from NASA, MIT, CalTech, UCLA, and other prominent institutions discovered a second possible exomoon, lovingly called Kepler-1708b-i.

For the astronomers, this was a home run. Not only were astronomers finding exoplanets out there, but finding exoplanets with exomoons. The team focused on known cold gas giants that were far away from their host stars, where the effect of the star’s gravity should not be enough to strip these gas giants of their exomoons. This makes sense. In our solar system, gas giants like Jupiter and Saturn have a lot of moons. It stands to reason that gas giant exoplanets could too.

In December of 2023, a study was published that dashed the exomoon theory against the proverbial lunar rocks. Published in Nature Astronomy, astronomers René Heller and Michael Hippke applied a new algorithm, called Pandora, to the previous exomoon research, and concluded, much like Obi-Wan Kenobi in Star Wars, that those were no moons.

It’s an astronomical roller coaster, and Kipping’s latest paper comes out swinging at Heller and Hippke.

“The reason they didn’t see them [the exomoons] is not because of the data (as they thought),” Kipping told The Debrief. “But it is actually because their algorithm for finding moons didn’t work properly.”

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ASTRONOMERS BAFFLED BY A MYSTERIOUS OBJECT IN THE “MASS GAP” BETWEEN NEUTRON STARS AND BLACK HOLES

Astronomers using a telescope array in South Africa have spotted a mysterious yet massive object within what astronomers term the “mass gap” between neutron stars and black holes, that also shares a binary orbit with a neutron star.

The fact that the mysterious object lies in this mass gap leads them to believe it is either the largest neutron star ever observed, the least massive black hole, or something else entirely. The discovery could have significant applications for understanding the “uncertain physics” underlying a range of massive cosmic objects.

Objects of this size are typically categorized as “astrophysical compact objects,” and they generally come in one of two varieties: black holes or neutron stars. Still, there is an enormous mass gap between the smallest black hole and the largest neutron star. For example, the largest neutron stars range between 2.2 to 2.5 solar masses, while black holes smaller than 5 solar masses are considered extremely rare. The result is a mass gap where these objects simply should not be.

As a result, discovering a compact astronomical object situated within this gap is a major event. Astronomers Ewan Barr and Arunima Dutta from the Max-Planck-Institut für Radioastronomie, who made the discovery, say that previous objects in this mass gap have also been spotted, but “the nature of these objects and the mechanisms through which they formed remain unknown.”

The astronomers made the discovery while scanning a globular cluster known as NGC 1851 using the Karoo Array Telescope (MeerKAT) in South Africa. There, they spotted a pulsar in a binary orbit with an unknown compact object with a mass that landed in the lower range of the mass gap.

“The nature of these mass gap objects is unknown, as is the formation of their host binary systems,” the researchers write in the study detailing their findings. They also point out that the companion’s mass of 2.09 to 2.71 (solar masses) is in the mass gap, “indicating either a very massive NS (Neutron Star) or a low-mass BH (Black Hole).”

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No, the James Webb Space Telescope hasn’t found life out there—at least not yet

The rumors have been out there for a while now, percolating through respectable corners of the astronomy and astrobiological community, that the James Webb Space Telescope has found a planet with strong evidence of life.

Some of this sentiment recently bubbled into the public view when the British news magazine The Spectator published an item titled “Have we just discovered aliens?” In accordance with Betteridge’s law of headlines, the answer to the question posed in this headline is no.

But is it a hard no? That’s a more difficult question. The Spectator featured comments by some serious British scientists, including astrophysicist Rebecca Smethurst, who said, “I think we are going to get a paper that has strong evidence for a biosignature on an exoplanet very, very soon.”

Additionally, there was British astronaut Tim Peake fanning the flames with this comment: “Potentially, the James Webb telescope may have already found [alien life]… it’s just that they don’t want to release or confirm those results until they can be entirely sure, but we found a planet that seems to be giving off strong signals of biological life.”

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Newly discovered cosmic megastructure challenges theories of the universe

Astronomers have discovered a ring-shaped cosmic megastructure, the proportions of which challenge existing theories of the universe.

The so-called Big Ring has a diameter of about 1.3bn light years, making it among the largest structures ever observed. At more than 9bn light years from Earth, it is too faint to see directly, but its diameter on the night sky would be equivalent to 15 full moons.

The observations, presented on Thursday at the 243rd meeting of the American Astronomical Society in New Orleans, are significant because the size of the Big Ring appears to defy a fundamental assumption in cosmology called the cosmological principle. This states that above a certain spatial scale, the universe is homogeneous and looks identical in every direction.

“From current cosmological theories we didn’t think structures on this scale were possible,” said Alexia Lopez, a PhD student at the University of Central Lancashire, who led the analysis. “We could expect maybe one exceedingly large structure in all our observable universe.”

Zooming out on the universe should, in theory, reveal a vast, featureless expanse. Yet the Big Ring is one of a growing list of unexpectedly large structures. Others include the Giant Arc, which appears just next to the Big Ring and was also discovered by Lopez in 2021. Cosmologists calculate the current theoretical size limit of structures to be 1.2bn light years, but the Big Ring and the Giant Arc, which spans an estimated 3.3bn light years, breach this limit.

Intriguingly, the two structures are at the same distance from Earth, near the constellations of Boötes the Herdsman, raising the possibility that they are part of a connected cosmological system.

“These oddities keep getting swept under the rug, but the more we find, we’re going to have to come face-to-face with the fact that maybe our standard model needs rethinking,” said Lopez. “As a minimum it’s incomplete. As a maximum we need a completely new theorem of cosmology.”

The Big Ring was discovered by analysing data from the Sloan Digital Sky Survey (SDSS), a catalogue of distant quasars. These objects are so bright that they can be seen from billions of light years away and act like giant, distant lamps, illuminating intervening galaxies that their light passes en route and which otherwise would go unseen.

Lopez and colleagues used several different statistical algorithms to identify potential large-scale structures and the Big Ring emerged. The structure appears as an almost perfect ring on the sky, but further analysis revealed it has more of a coil shape, like a corkscrew, which is aligned face-on with Earth.

Cosmologists are unsure what mechanism could have given rise to the structure. One possibility is a type of acoustic wave in the early universe, known as baryonic acoustic oscillations, that could give rise to spherical shells in the arrangement of galaxies today. Another explanation is the existence of cosmic strings, hypothetical “defects” in the fabric of the universe that could cause matter to clump along large-scale faultlines.

Dr Jenny Wagner, a cosmologist at the Bahamas Advanced Study Institute & Conferences, described the discovery as significant. “It doesn’t seem to be a mere chance alignment,” she said.

Wagner said it was possible to accommodate the Big Ring within the cosmological principle, depending on how its limits are defined, but that the more of these outlier, large-scale structures that are discovered, the less statistically plausible this view becomes. “This is why the search for further giant structures is so valuable,” she said. “Personally, I wouldn’t be surprised if we have to abandon the cosmological principle after future discoveries.”

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A CELESTIAL OBJECT “TOO LARGE TO EXIST” HAS BEEN DETECTED BY ASTRONOMERS, UPENDING PAST THEORIES ON PLANETARY FORMATION

Researchers say the discovery of a planet too large for its nearest star is challenging existing theories about the dynamics of planetary formation, according to recent findings.

The discovery, reported by researchers at Penn State University, involves a massive planet orbiting LHS 3154, a star that is around nine times smaller than our Sun, and thereby also much cooler.

By comparison, the newly named planet, LHS 3154b, which orbits it is more than 13 times the size of Earth, which planetary scientists say should not be possible.

Put into context, the mass ratio of the planet to its host star is greater than 100 times that of Earth and the Sun, making LHS 3154b the largest planet ever discovered orbiting an ultracool dwarf star and, more fundamentally, a planet too large to easily fit within current models about how such celestial objects form.

Suvrath Mahadevan, the Verne M. Willaman Professor of Astronomy and Astrophysics at Penn State, said he and his colleagues were surprised by the discovery.

“We wouldn’t expect a planet this heavy around such a low-mass star to exist,” Mahadevan said in a press release describing the new findings.

Generally, once a star is formed, gas and dust surrounding it will form a protoplanetary disk, which will eventually form planets over long periods. However, the disk around LHS 3154 does not have enough solid mass to facilitate planetary formation in the case of an object like LHS 3154b, Mahadevan says.

“But it’s out there,” he adds, “so now we need to reexamine our understanding of how planets and stars form.”

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Astronomer Have Discovered A Mysterious Object, Which Is 570 Billion Times Brighter Than The Sun

Billions of light years away, there is a giant ball of hot gas that is brighter than hundreds of billions of suns. It is hard to imagine something so bright. So what is it? Astronomers are not really sure, but they have a couple theories.

They think it may be a very rare type of supernova — called a magnetar — but one so powerful that it pushes the energy limits of physics, or in other words, the most powerful supernova ever seen as of today.

This object is so luminous that astronomers are having a really difficult time finding a way to describe it. “If it really is a magnetar, it’s as if nature took everything we know about magnetars and turned it up to 11,” said Krzysztof Stanek, professor of astronomy at Ohio State University and the team’s co-principal investigator, comedically implying it is off the charts on a scale of 1 to 10.The object was first spotted by the All Sky Automated Survey of Supernovae (ASAS-SN or “assassin”), which is a small network of telescopes used to detect bright objects in the universe. Although this object is ridiculously bright, it still can’t be seen by the naked eye because it is 3.8 billion light years away.

ASAS-SN, since it began in 2014, has discovered nearly 250 supernovae, however this discovery, ASASSN-15lh, stands out because of its sheer magnitude. It is 200 times more powerful than the average supernova, 570 billion times brighter than the sun, and 20 times brighter than all the stars in the Milky Way Galaxy combined.

“We have to ask, how is that even possible?” said Stanek. “It takes a lot of energy to shine that bright, and that energy has to come from somewhere.”

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A comet not seen in 50,000 years is coming. Here’s what you need to know

Typically, during the course of a year about a dozen comets will come within the range of amateur telescopes. Most quietly come and go with little fanfare, but some are particularly noteworthy. 

During the upcoming weeks, a newly-discovered comet will be making a relatively close approach to the Earth. On Feb. 1, comet C/2022 E3 (ZTF) will pass to within 28 million miles (42 million km) of our planet, its first approach in 50,000 years. While this will no doubt entice many skywatchers to attempt to view the comet, whether or not one will actually be able to see it will depend on a variety of factors including location and light pollution from both natural and artificial sources.

But don’t be dismayed! Even if you don’t have the right gear or conditions to see comet C/2022 E3 (ZTF), the Virtual Telescope Project will be hosting a free livestream of the comet beginning at 11:00 p.m. EST on Jan. 12 (0400 GMT on Jan. 13). You can watch the live webcast courtesy of the project’s website(opens in new tab) or on its YouTube channel(opens in new tab).

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Comet Not Seen Since The Stone Age Will Fly Through The Sky In ‘Once-In-A-Civilization’ Event

A comet not seen since the Stone Age will streak across the night sky this month in a “once-in-a-civilization” sight, providing observers are lucky enough to catch a glimpse.

Initially believed to be an asteroid, the comet was first detected by astronomers Frank Masci and Bryce Bolin at the Palomar Observatory in Southern California in March 2022, according to Space.com.  Later observations however showed the “asteroid” had a “very tightly condensed coma” – an indicator of a comet –  traveling approximately 399 million miles away from the sun, near the orbit of Jupiter, the outlet reported.

After further observation, astronomers were able to determine that the comet, dubbed C/2022 E3, had an orbit that lasted approximately 50,000 years, placing its previous journey through our solar system during the Old Stone Age, Space.com reported.

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