Latest news with #Astronomers
Gizmodo
22-05-2025
- Science
- Gizmodo
New Minor Planet Spotted Past Pluto, One of the Largest Distant Objects in the Solar System
There's a new frozen oddball orbiting the Sun, and it's not your average space rock. It's a planet—a minor one, to be fair—but one of the largest yet discovered and with an orbit around the Sun that puts our own planet's orbit to shame. The minor world is dubbed 2017 OF201; the International Astronomical Union's Minor Planet Center added the object to its catalog on May 21. Despite its classification, the planet measures somewhere between 290 and 510 miles (470 and 820 kilometers) across. Its upper size limit would put the minor planet in the same wheelhouse as Ceres, the largest asteroid in the belt between Mars and Jupiter, boasting a diameter of about 592 miles (952 km). Astronomers first spotted 2017 OF201 in archival images, but only now is the object officially recognized as a trans-Neptunian object, or TNO. TNOs are bodies in the solar system that orbit the Sun beyond Neptune, which is 30 times more distant from the Sun than the Earth. But 2017 OF201 is superlative even among the distant TNOs; its orbit takes it as far as 838 astronomical units from the Sun—making it nearly 30 times farther than Neptune, which again, is itself 30 times farther from the Sun than Earth is, on average. At its closest, as reported by EarthSky, 2017 OF201 comes within 45 AU of the Sun. That remarkable orbit earns the minor planet the label of an extreme trans-Neptunian object (ETNO), a subset of distant rocks that fuel theories about mysterious gravitational forces at play in the far reaches of the solar system. Which brings us, inevitably, to Planet Nine, the theorized distant world posited as a gravitational explanation for the strange clustering of objects in the Kuiper Belt. Other ideas have been floated to explain the phenomenon—such as a ring of debris exerting gravitational influence, or even a primordial black hole—but nothing grips our human fascination like a distant planet, so far away from our solar system's other worlds that it's never been observed. Planet Nine, if it exists, would have to be a little over six times Earth's mass, with an orbital period of about 7,400 years. The newly cataloged minor planet is big, but not Planet Nine big. Still, discoveries like this keep astronomers buzzing. Just last month, a different team of astronomers found a different slow-moving object beyond Neptune—a would-be Planet Nine candidate, but it's in the wrong place. Objects like those recently reported add to the growing list of bodies that might eventually help pinpoint the elusive Planet Nine—or at least explain the strange movement of objects on the periphery of our solar neighborhood. 2017 OF201 isn't the planetary heavyweight many have been waiting for, but it's a reminder that the solar system is still full of surprises—especially in its frigid, hard-to-see suburbs.
The Independent
08-04-2025
- Science
- The Independent
Astronomers spot two stars the size of Earth headed toward a violent explosion
Astronomers have discovered a pair of white dwarf stars locked in a tight orbital dance, hurtling towards a spectacular and violent end. Located a mere 160 light-years from Earth within our Milky Way galaxy, these stellar remnants are destined for not one, but four explosive detonations. White dwarfs represent the final stage of evolution for stars up to eight times the mass of our sun. After exhausting their hydrogen fuel, these stars collapse under their own gravity, shedding their outer layers in a dramatic "red giant" phase. What remains is an incredibly dense core, roughly the size of Earth – a white dwarf. The two white dwarfs in this binary system are gravitationally bound, spiraling ever closer. This proximity sets the stage for a cataclysmic event. As they draw nearer, the immense gravitational forces will trigger a series of explosions, culminating in a final, powerful detonation. This discovery offers a glimpse into the dramatic and explosive fates awaiting some of the universe's most fascinating objects. "White dwarfs are the stellar remnants of the vast majority of stars, and from time to time we find systems where two white dwarfs closely orbit each other," said James Munday, a PhD researcher at the University of Warwick in England and lead author of the study published in the journal Nature Astronomy. The researchers used data from four ground-based telescopes to study this binary system. One of the white dwarfs has a mass about 83 per cent that of our sun and the other about 72 per cent. No other known white dwarf binary has a larger combined mass, Munday said. "They are both about as big as the Earth. One has a diameter about 20 per cent larger and the other about 50 per cent larger. That gives you an idea of how dense they are. It's the sun compressed onto the size of Earth. Their masses when they were regular stars were probably around three to four times the mass of the sun," said University of Warwick astrophysicist and study co-author Ingrid Pelisoli. A few hundred binary systems composed of two white dwarf stars are known. These two orbit closest to each other of any of them. They are about 25 times closer to each other than our solar system 's innermost planet Mercury is to the sun, completing an orbit every roughly 14 hours. With the gap between them very gradually narrowing as the binary system loses energy, the fact that they are so massive and so close ensures their demise over a large timescale. When they get closer to each other, the heavier of the two white dwarfs, because of its greater gravitational strength, will begin to draw material from the lighter one's outer layer and increase in mass past the threshold beyond which a white dwarf experiences a thermonuclear explosion. This will set the stage for a complex explosion called a type 1a supernova, in this instance involving a quadruple detonation. "White dwarfs are made up of layers, much like an onion. Their inner layer is a core of carbon and oxygen, surrounded by a helium layer and finally by a hydrogen layer," Pelisoli said. "The less-massive star will transfer mass to the massive one when they start interacting. This will lead the helium layer (of the heavier one) to become too massive, triggering an explosion. This then triggers a second explosion in the carbon-oxygen core. The shock wave from these explosions in turn triggers a third explosion in the remaining helium layer of the companion, which triggers a fourth explosion in its carbon-oxygen core," Pelisoli added. This quadruple detonation is expected to take about four seconds, start to finish. But it will not come anytime soon. The researchers calculate that it will occur approximately 22.6 billion years from now. The universe is about 13.8 billion years old. When the explosion occurs, it would appear from the perspective of Earth about 10 times brighter than the moon in the night sky - if Earth, now about 4.5 billion years old, still exists. This is the first time a binary system apparently headed for such a fate has been identified. If the two white dwarfs were far enough apart that the heavier one would not siphon material from the lighter one, they could survive in perpetual peace. "In a wider orbit, they could indeed live stably without any catastrophic future, but here we know that the explosion will light up our side of the galaxy," Munday said.
