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NASA

A Hidden Giant: Scientists Uncover a Massive Exoplanet Hiding in Plain Sight

Astronomers have uncovered a massive, hidden exoplanet nestled in the dusty disc of a young star—MP Mus—by combining cutting-edge data from the ALMA observatory and ESA’s Gaia mission. Initially thought to be planet-free, the star’s surrounding disc appeared deceptively empty. But new observations and a telltale stellar “wobble” pointed to a Jupiter-sized gas giant forming within the disc’s obscured gaps. This marks the first time a planet in such a disc has been detected using these tools, opening the door to finding more young worlds that have so far evaded detection.

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Astronomers have made a groundbreaking discovery by detecting a massive exoplanet hiding in plain sight around a young star. The team, led by researchers from the University of Cambridge, used a combination of observations from the Atacama Large Millimeter/submillimeter Array (ALMA) and the European Space Agency’s Gaia mission to uncover the hidden giant.

The star, called MP Mus, was previously thought to be alone in its protoplanetary disc, with no signs of planet formation. However, further analysis revealed a cavity close to the star and two gaps further out, suggesting that MP Mus may not be as featureless as initially believed.

Using data from Gaia, Miguel Vioque, a researcher at the European Southern Observatory, found that MP Mus was wobbling, which is likely caused by a massive gas giant less than ten times the mass of Jupiter orbiting the star. The team’s computer modeling work confirmed that this is indeed the case, and that the exoplanet is embedded in the protoplanetary disc.

This discovery marks the first time an exoplanet has been indirectly detected in a protoplanetary disc using this method. The research also suggests that many more hidden planets might exist in other discs, just waiting to be found.

The detection of young planets in protoplanetary discs is extremely challenging due to interference from gas and dust. However, the combination of ALMA and Gaia data has provided new insights into how these planets form and how our own Solar System may have evolved.

Dr Álvaro Ribas from Cambridge’s Institute of Astronomy said, “We think this might be one of the reasons why it’s hard to detect young planets in protoplanetary discs, because in this case, we needed the ALMA and Gaia data together.”

The research was supported by the European Union’s Horizon Programme, the European Research Council, and the UK Science and Technology Facilities Council (STFC), part of UK Research and Innovation (UKRI).

Asteroids, Comets and Meteors

Unveiling a Hidden World: Astronomers Discover Distant Object at Solar System’s Edge

Astronomers have uncovered a massive new trans-Neptunian object, 2017 OF201, lurking at the edge of our solar system. With an orbit stretching 25,000 years and a size that may qualify it as a dwarf planet, this mysterious world challenges long-held assumptions about the “empty” space beyond Neptune. Its unusual trajectory sets it apart from other distant bodies and may even cast doubt on the controversial Planet Nine hypothesis.

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As we venture further into the uncharted territories of our solar system, scientists have made a groundbreaking discovery that sheds new light on the mysteries of the outer reaches. A small team led by Sihao Cheng has uncovered an extraordinary trans-Neptunian object (TNO), dubbed 2017 OF201, at the edge of our celestial neighborhood.

This remarkable find is significant not only because it suggests that the Kuiper Belt, a region previously thought to be empty, may harbor more hidden worlds, but also because it challenges our understanding of the solar system’s architecture. The object’s extreme orbit and large size make it comparable to Pluto, a dwarf planet that has captivated astronomers for decades.

The discovery team used advanced computational methods to identify 2017 OF201’s distinctive trajectory pattern on the sky, pinpointing bright spots in an astronomical image database from the Victor M. Blanco Telescope and Canada France Hawaii Telescope (CFHT). The new TNO is estimated to be around 700 km in diameter, making it the second-largest known object in its wide orbit.

Further observations are needed to determine the exact size of 2017 OF201, but this groundbreaking find has significant implications for our understanding of the outer solar system. As Cheng notes, “The presence of this single object suggests that there could be another hundred or so other objects with similar orbit and size; they are just too far away to be detectable now.”

This detection also highlights the power of open science, as the data used to identify and characterize 2017 OF201 are archival and available to anyone, not only professional astronomers. This approach underscores the value of sharing scientific resources and demonstrates that groundbreaking discoveries can be made by researchers, students, or even citizen scientists with the right tools and knowledge.

As we continue to explore the vast expanse of our solar system, discoveries like 2017 OF201 remind us that there is still much to uncover about the celestial world that surrounds us. The detection of this hidden world at the edge of our solar system serves as a poignant reminder of the awe-inspiring mysteries that await us in the uncharted territories of space.

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Asteroids, Comets and Meteors

Unveiling Ancient Secrets on Mars: A Breakthrough Technique Reveals Hidden Clues

A curious red Martian rock nicknamed Sapphire Canyon has scientists excited, as its spotted appearance hints at possible organic origins. On Earth, researchers tested a powerful laser technique, O-PTIR, on a similar rock found by chance in Arizona, proving it can rapidly and precisely reveal a material’s chemical makeup. This high-resolution method could play a key role in analyzing Mars samples once they arrive, adding to its growing track record in NASA missions like Europa Clipper.

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The discovery of an unusual rock sample, named Sapphire Canyon, by NASA’s Mars rover Perseverance in 2024 has sent shockwaves of excitement through the scientific community. This enigmatic rock features striking white spots with black borders within a red mudstone, sparking hopes that it might hold clues about the presence of organic molecules on Mars.

To unlock the secrets hidden within Sapphire Canyon, researchers from the Jet Propulsion Laboratory and the California Institute of Technology employed an innovative technique called optical photothermal infrared spectroscopy (O-PTIR). This method uses two lasers to study a material’s chemical properties, creating its unique fingerprint by measuring thermal vibrations on its surface.

The team, led by Nicholas Heinz, put O-PTIR to the test on a basalt rock with dark inclusions of similar size to Sapphire Canyon’s. By chance, Heinz stumbled upon this visually similar rock while hiking in Arizona’s Sedona region. The results were astounding – O-PTIR proved to be an extremely effective tool for differentiating between the primary material and its dark inclusions.

One of the key advantages of O-PTIR is its enhanced spatial resolution, allowing scientists to pinpoint specific regions of interest within a sample. Additionally, this technique is remarkably rapid, with each spectrum collection taking mere minutes. This enables researchers to apply more sensitive techniques to study areas containing potential organics in greater detail.

Heinz expressed his hope that the capabilities of O-PTIR will be considered for future Martian samples, as well as those from asteroids and other planetary surfaces. The team’s expertise is currently the only one available at NASA’s Jet Propulsion Laboratory, having previously assisted with confirming the cleanliness of the Europa Clipper mission prior to its launch.

As the scientific community continues to unravel the mysteries hidden within Sapphire Canyon, Heinz and his team are working closely with NASA’s Mars science team to test O-PTIR on algal microfossils typically used as Mars analogs for the rovers. This breakthrough technique is poised to revolutionize our understanding of Martian geology and potentially uncover signs of ancient life on the Red Planet.

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Dark Matter

Clearest Mars Images Yet Reveal Stunning Terrain and Mysterious Rock Formation

Captured at a location called “Falbreen,” this 360-degree view mosaic was stitched together 96 images that were acquired May 26, 2025. In the upper image, the enhanced-color mosaic features deceptively blue skies and the 43rd rock abrasion (the white patch at center-left) of the NASA Perseverance rover’s mission at Mars. Below, in the natural-color version of the “Falbreen” panorama, colors have not been enhanced and the sky appears more reddish. Credit: NASA/JPL-Caltech/ASU/MSSS

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The latest high-resolution panorama captured by NASA’s Perseverance Mars rover has revealed some of the clearest images yet taken on the Red Planet. The stunning mosaic, which was stitched together from 96 individual images, showcases a breathtaking Martian landscape featuring ancient terrain, mysterious rock formations, and vast distances stretching out to the horizon.

The imaging team took advantage of clear skies to capture one of the sharpest panoramas of the mission so far. Visible in the enhanced-color version is a boundary line between two geologic units, with lighter-toned rocks rich in olivine giving way to darker clay-bearing rocks farther away. The transition from one unit to another is marked by a sweeping line that stretches across the image.

One of the most intriguing features of the mosaic is a large rock that appears to sit atop a dark, crescent-shaped sand ripple near the center of the image. Geologists call this type of rock a “float rock” because it was likely formed elsewhere and transported to its current location. The science team suspects that this particular float rock arrived before the sand ripple formed.

The bright white circle just left of center and near the bottom of the image is an abrasion patch, created by the rover’s drill as it prepared for a sample collection mission. This is the 43rd rock Perseverance has abraded since landing on Mars, with two inches (5 centimeters) wide shallow patches enabling the science team to see what lies beneath the weathered surface.

As the rover journeyed towards its current location, it left behind tracks that can be seen winding their way towards the horizon. About 300 feet (90 meters) away, they veer to the left and disappear from sight at a previous geologic stop called “Kenmore.”

The Perseverance rover has been exploring Mars since February 2021, with its Mastcam-Z instrument capturing stunning images of the Martian terrain. The relatively dust-free skies have provided a clear view of the surrounding landscape, accentuating the differences in terrain and sky.

“This is just a glimpse of what we’ll soon witness with our own eyes,” said Sean Duffy, acting NASA administrator, referring to future human space exploration missions that will propel astronauts back to the Moon and eventually to the Martian surface. “NASA’s groundbreaking missions, starting with Artemis, will take human space exploration to new heights.”

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