logo
How a planetarium show discovered a spiral at the edge of our solar system

How a planetarium show discovered a spiral at the edge of our solar system

Fast Company21 hours ago

If you've ever flown through outer space, at least while watching a documentary or a science fiction film, you've seen how artists turn astronomical findings into stunning visuals. But in the process of visualizing data for their latest planetarium show, a production team at New York's American Museum of Natural History made a surprising discovery of their own: a trillion-and-a-half mile long spiral of material drifting along the edge of our solar system.
'So this is a really fun thing that happened,' says Jackie Faherty, the museum's senior scientist.
Last winter, Faherty and her colleagues were beneath the dome of the museum's Hayden Planetarium, fine-tuning a scene that featured the Oort cloud, the big, thick bubble surrounding our Sun and planets that's filled with ice and rock and other remnants from the solar system's infancy. The Oort cloud begins far beyond Neptune, around one and a half light years from the Sun. It has never been directly observed; its existence is inferred from the behavior of long-period comets entering the inner solar system. The cloud is so expansive that the Voyager spacecraft, our most distant probes, would need another 250 years just to reach its inner boundary; to reach the other side, they would need about 30,000 years.
The 30-minute show, Encounters in the Milky Way,

Orange background

Try Our AI Features

Explore what Daily8 AI can do for you:

Comments

No comments yet...

Related Articles

Trump's 2026 budget cuts would force the world's most powerful solar telescope to close
Trump's 2026 budget cuts would force the world's most powerful solar telescope to close

Yahoo

time6 hours ago

  • Yahoo

Trump's 2026 budget cuts would force the world's most powerful solar telescope to close

When you buy through links on our articles, Future and its syndication partners may earn a commission. ANCHORAGE, AK — There was a pindrop silence in the room on Tuesday (June 10), as Christoph Keller, director of the National Solar Observatory, spoke on stage here at the 246th American Astronomical Society meeting. Standing in front of a giant projected bar graph, he solemnly explained the possible fate of the world's most powerful eye on the sun: the Daniel K. Inouye Solar Telescope (DKIST). If Congress enacts President Donald Trump's fiscal year 2026 budget request — allocating just $13 million or so for DKIST — the telescope won't be able to continue on, Keller said. For context, this year alone, the federally funded National Solar Observatory (NSO) expects to spend about $30 million on the facility. "To put it bluntly," Keller said, "for DKIST, at $13 million, we cannot operate. There's no way for us to operate such a complex facility." The graph behind Keller spoke for itself. On the left, a bar represented the actual money the NSO spent in 2024, one in the middle represented what the NSO plans to spend in 2025, and one on the right depicted Trump's FY26 budget request. Each individual bar was divided into two colors: one representing money required for DKIST (a strong majority of each bar) and one representing money required for all other NSO facilities. "If you actually looked at what this means," Keller said. "Between this year and the request for next year, it's a 54% budget cut." The hit to DKIST would be unfortunate, as scientists made clear during the talk, particularly seeing as the telescope only captured its first image in 2020 after over 25 years of effort. Not only is it the world's most powerful solar telescope, it's also the largest. Built with about 150 tons of steel, it sits atop the 10,000-foot-high (3,048-meter) summit of the volcanic mountain. Haleakalā, which translates to "the house of the sun," on the Hawaiian island of Maui. "It's a really nice site," David Boboltz, associate director for DKIST, said during the meeting. "It's got low light scattering; it's got good seeing." "It is literally the greatest leap in humanity's ability to study the sun from the ground since Galileo's time. It's a big deal," Jeff Kuhn, a professor at the University of Hawaii at Mānoa's Institute for Astronomy (IfA) who worked on DKIST, previously said in a statement. Indeed, the details of our sun that DKIST is able to capture are astounding. In the image below, for instance (DKIST's first image of the sun), each cell-like structure is about the size of Texas. This is the highest-resolution image of our star that's ever been captured. What's extra mind-blowing here is how small of a solar region the image actually represents: Another more recent image from DKIST reveals what appear to be magnetic "curtains" on our star's surface, in reference to what are called "photospheric striations" shaped by the sun's magnetic field. In still another, an area above the sun's atmosphere looks like it has the texture of one of those rubber spike balls you can get at Chuck E. Cheese. The list goes on in terms of awesome DKIST data, and that's with only a few years of time online. But DKIST wouldn't be the only at-risk NSO facility, as Keller explained. If Trump's FY26 budget proposal goes through, just $4 million would be available for all other NSO equipment. "We can maybe operate three ground stations," he said, suggesting this would eradicate all of helioseismology. There may only be some room for space weather forecasting initiatives, Keller said. "If something goes wrong; if something really fails, we won't have the money to fix it," he added. "Congress can fix it, and all citizens here, you know what to do."

A tiny star gave birth to an absolute giant. Scientists are puzzled.
A tiny star gave birth to an absolute giant. Scientists are puzzled.

Yahoo

time12 hours ago

  • Yahoo

A tiny star gave birth to an absolute giant. Scientists are puzzled.

Astronomers have discovered a world outside the solar system about 240 light-years away in space that is a freak of nature. Somehow, a little red dwarf star only one-fifth the size of the sun gave birth to an enormous baby — an exoplanet that is a little larger than Saturn, although it weighs about half as much as our ringed gas giant. Discovered in a sweeping investigation of NASA's Transiting Exoplanet Survey Satellite data, this world, TOI-6894 b, and its host star have set a new record for their incongruous sizes. Together they are the smallest known star to have an orbiting giant planet. If there were a Guinness Book of Galactic Records, this one would have a landslide victory for the titleholder. The star, TOI-6894, is just 60 percent the size of the next smallest star with such a planet. The pair's existence breaks all the rules of what scientists know about planet formation. "We don't really understand how a star with so little mass can form such a massive planet!" said Vincent Van Eylen, a researcher at the University College London, in a statement. "By finding planetary systems different from our solar system, we can test our models and better understand how our own solar system formed." SEE ALSO: The Webb telescope found something exceedingly rare around a dying star NASA's TESS mission — short for Transiting Exoplanet Survey Satellite — was designed to find new worlds as they pass in front of their host stars. Credit: NASA illustration Edward Bryant, who led the research team, found the behemoth first by poring over TESS space telescope data of over 91,000 small red dwarfs, aka M-type stars. Then he used the European Southern Observatory's Very Large Telescope in Chile to reveal TOI-6894b. According to How to Make a Really Humongous Planet 101, it should be difficult — nearly impossible — for stars this tiny to do this. That's because the disks of gas and dust swirling around young stars are the construction materials for planets. Small stars tend to have smaller and lighter disks. Gas giants like our own Jupiter or Saturn need a lot of stuff to form their cores. They then are able to attract a lot more gas quickly from their surroundings to collect an atmosphere. The mechanics are called "core accretion," and it seems to work best when the building materials are plentiful. But TOI-6894b seems to be playing by a different rulebook. It's about 53 times the weight of Earth and made partly of heavy elements, according to a paper on its discovery published in Nature Astronomy. In fact, the exoplanet is thought to have about 12 Earths'-worth of those chemicals. That's way beyond what most small young stars are thought to have in their midst. Some scientists don't want to throw the baby out with the bathwater: Though the exoplanet doesn't fit neatly into the core-accretion model, it could have formed in a similar way but with a tweak. Perhaps this world started collecting ingredients to form its core very early in its star's life, when the disk was still chock-full of raw material. Or maybe instead of growing a large core quickly to pull in more gas in a runaway process à la Jupiter-like planets, TOI-6894b could have just kept hoarding gas and heavy elements gradually over time. But even that would require a bigger original supply of dust. In a survey sample of 70 disks around small stars, only five had enough material to build a planet on the scale of TOI-6894b, according to the new paper. Another idea, called gravitational instability, suggests the disk could collapse under its own weight to create a planet directly. But the discovery team for TOI-6894 b points out that the process doesn't quite work for something the size of this exoplanet — at least according to computer simulations. Whatever the origin story, TOI-6894b is leading the ranks of other known gas giants orbiting small and faint stars that astronomers want to study. Scientists also have their eyes on LHS 3154 b, GJ 3512 b, and TZ Ari b. Small stars tend to have smaller and lighter protoplanetary disks. Credit: NASA / JPL-Caltech illustration "This discovery will be a cornerstone for understanding the extremes of giant planet formation," Bryant said. The next step for the research team is to use the James Webb Space Telescope to study the exoplanet's atmosphere, which will occur within the next year. By measuring the various materials in the planet, the researchers may be able to determine the size and structure of its core. That could answer the question of whether TOI-6894 b formed through one of the known models. They also have a hunch the exoplanet's atmosphere is rich in methane, something Webb could help confirm. TOI-6894 b is unusually cool for a gas giant, about 300 degrees Fahrenheit. Most of the gas giants known are "hot Jupiters," with temperatures between 1,340 and 3,140 degrees Fahrenheit. Such a discovery of a relatively chilly gas giant would be very rare, the researchers said. "Most stars in our galaxy are actually small stars exactly like this," said Daniel Bayliss, a coauthor from the University of Warwick in the United Kingdom. "The fact that this star hosts a giant planet has big implications for the total number of giant planets we estimate exist in our galaxy."

Webb telescope took a direct image of two exoplanets. See it now.
Webb telescope took a direct image of two exoplanets. See it now.

Yahoo

time12 hours ago

  • Yahoo

Webb telescope took a direct image of two exoplanets. See it now.

Scientists have scored a pristine view of a pair of exotic worlds orbiting a star more than 300 light-years away — one with sand-like clouds and another surrounded in space by moon-making material. The discoveries come from YSES-1, a star system in the deep southern sky. Using the James Webb Space Telescope, a collaboration of NASA and its European and Canadian counterparts, a team of astronomers saw so-called "silicate clouds" directly for the first time on an exoplanet, a world far beyond our own solar system. The team's detection of a dusty disk around the sibling planet is also rare, perhaps just the third time scientists have seen one so clearly. Webb usually observes exoplanets through indirect methods, such as transmission spectroscopy, a technique for studying a planet's atmosphere by analyzing how starlight filters through it. What distinguishes this new research is that the two worlds — YSES-1b and YSES-1c — were directly imaged, meaning the telescope captured light from the planets themselves. Sitting far from their host star, these young planets glow from the leftover heat of their formation. Thanks to their temperature, size, and distance, the result is a clean picture of the exoplanets in thermal infrared, allowing scientists to get much more data. "What's really cool about this system is that unlike most planets, we can actually take a picture of them!" said Evert Nasedkin in a post on the social media platform Bluesky. You can see the image further down in this story. SEE ALSO: A tiny star gave birth to an absolute giant. Scientists are puzzled. The idea for this groundbreaking project began long before Webb was even open for business, said Kielan Hoch, lead author of the research recently published in the journal Nature. Scientists hypothesized the telescope could get both worlds in a single shot, "essentially giving us two for the price of one," Hoch said in a statement. These two gas giant planets weigh five to 15 times the mass of Jupiter and orbit far from their host, a star similar to the sun. What's different is that it's only about 16.7 million years old, a mere whippersnapper compared to our middle-aged, 4.6 billion year-old sun. The planets are also in extremely distant orbits. YSES-1b, the innermost of the two, is still perhaps four times farther from its star than Pluto is from the sun. But given only a handful of known exoplanets can be directly imaged, the study has offered scientists a unique opportunity to see an early stage of a developing star system. From these observations of the YSES-1 system — the letters in its name stand for Young Suns Exoplanet Survey — astronomers can gain insight into how planets and moons form and evolve. SEE ALSO: Webb discovers a distant moon has an intriguing similarity to Earth Few distant worlds meet the criteria for direct imaging because planets are often millions of times fainter than the stars they circle. And if they are orbiting close by, their own light usually gets swamped. The James Webb Space telescope captures a direct image of exoplanets YSES-1b and YSES-1c with its Near-Infrared Spectrograph instrument. Credit: NASA/ ESA / CSA / Hoch et al. / Nature But scientists want these images because there is so much to learn from them. Molecules within a planet's atmosphere absorb certain colors of light, so when astronomers study a planet's spectrum, they can look for what's missing from the rainbow to determine which gases — like water, methane, and carbon dioxide — are present in the planet's air. For the YSES-1 system, scientists not only saw molecules in the direct imaging but detected cloud particles and a dust disk. On YSES-1c, rather than water vapor, the clouds are made of hot, ultra-fine rock grains. While Earth's clouds are often white and pillowy, these are probably hazy and dark, filling the sky with something akin to a glass powder. You can think of these silicate clouds sort of like the plumes of mineral ash that vent out of volcanoes. YSES-1b is even "weirder," said Nasedkin, one of the coauthors. Around it is a so-called circumplanetary dust disk that could serve as a birthplace for moons, similar to those seen around Jupiter. Scientists used computer models to figure out that the dust is hot — about 400 to 600 degrees Fahrenheit. Because this particular disk is much older than two previously found around other unrelated exoplanets, what is creating or sustaining it is a mystery. The original disk of planet-building material around the star is long gone, so the researchers have ruled that out as the source. "It's possible that we're seeing the dust emitted by collisions of moons and other small, rocky bodies left over from the planet's formation!" Nasedkin said.

DOWNLOAD THE APP

Get Started Now: Download the App

Ready to dive into the world of global news and events? Download our app today from your preferred app store and start exploring.
app-storeplay-store