Inactive NASA Satellites Emit Surprisingly Strong Radio Pulses

Illustration of NASA’s Relay 1 satellite, in front of Relay 2

NASA

A long-dormant satellite unexpectedly emitted a powerful radio pulse, momentarily surpassing all other celestial signals. Astronomers speculate that this flash may have resulted from a rare micrometeoroid impact or a spontaneous discharge.

NASA’s Relay 2 satellite was among the earliest operational satellites, launched as an experimental communications tool in 1964. Its use was discontinued the following year, and by 1967, the satellite’s electronic components had ceased functioning, leaving its metal frame orbiting indefinitely.

So Clancy James from Curtin University in Australia and his team were puzzled nearly 60 years later when they detected a burst of short, intense radio waves emanating from the satellite’s suspected location.

Utilizing the Australian Square Kilometer Array Pathfinder (ASKAP), an array of 36 telescopes in Western Australia, James and his colleagues were searching the sky for signs of a mysterious radiation pulse from other galaxies.

On June 13th, they received a signal that seemed to originate from within our galaxy. “If it’s in close proximity, studying it through an optical telescope becomes quite feasible, so I was thrilled at the prospect of discovering a new pulsar or some other object,” Clancy remarks.

However, upon closer examination, the signal appeared to be quite close to Earth, which meant that ASKAP couldn’t focus on everything simultaneously. This indicated the source was likely within 20,000 kilometers of our planet, according to Clancy. The signal was notably short-lived, lasting less than 30 nanoseconds. “It was an exceptionally potent radio pulse that briefly outshone everything else in the sky,” Clancy explains.

When they traced the signal back to its source and compared it to known satellite positions, they concluded the only plausible explanation was Relay 2. Since that satellite is inoperative, Clancy and his team suspect that the signals may result from external events such as electrostatic discharges or micrometeoroids striking the satellite, creating clouds of charged plasma.

“It’s quite challenging to differentiate between these two scenarios,” says Karen Aplin from the University of Bristol in the UK. This difficulty arises because the radio emissions from both phenomena appear comparable. Yet, monitoring future electrostatic discharges from satellites could prove beneficial, she adds. “In an environment filled with space debris and numerous smaller, cost-effective satellites that lack sufficient protection from electrostatic discharges, this radio detection could ultimately lead to innovative technologies for assessing such discharges in space,” she concludes.

Topic:

Source: www.newscientist.com

Scientists worldwide discover a substantial magma reservoir beneath the inactive volcano

The magma reservoir under the cascade range has a different depth, size, and complexity, but the upper magma body is spread, according to the Global Scientist’s team at Cornell University and Cascade Volcano Observatory.

Mountleinia. Image credit: Walter Siegmund / CC by-Sa 3.0.

The visible lava on the surface is an obvious indicator of the activity, but the long-standing beliefs are expelled during the eruption of active volcanoes, and there are large magma body that breaks down over time as the volcano becomes dormant. That is.

But A New study It is published in the journal Natural global science Challenge this assumption.

The study author has identified the magma chamber under the six volcanoes, six volcanoes of various sizes within the cascade range and six volcanoes.

They discovered that all of the volcanoes, including dormant state, have a sustainable and large magma body.

Given that some of these volcanoes, such as Lake Lake in Oregon, have not been active for thousands of years, the results are surprising.

“Regardless of the frequency of eruptions, you can see a large magma under a lot of volcanoes,” said Dr. Guaning Pan, a researcher at Cornel University.

“These magma bodies seem to be not only active, but also under volcanoes for a lifetime.”

The fact that more volcanoes maintain a magma body is an important consideration on how researchers monitor and predict future volcanic activities.

“We thought that if we found a large amount of magma, we thought it would increase the potential of eruptions, but now we change the perception that this is the baseline situation,” said Dr. Pan. Ta.

The result suggests that the eruption does not completely discharge the magma chamber, indicating that it eliminates excessive amounts and pressure instead.

The chamber can gradually solve the crust, so it can be slowly expanded and replenished over time.

“With a general understanding of where the magma is, I was able to do a good job rather than optimizing monitoring,” said Professor Jeffrey Aberters of Cornell University.

“There are many volcanoes that are sparse or not intensive research.”

______

G. bread et al。 Partial melting long life under the volcano in the cascade range. nut. GeosciReleased online on January 23, 2025. Doi: 10.1038/S41561-024-01630-Y

Source: www.sci.news

Webb uncovers massive inactive galaxy with mature stars in the ancient cosmos

The formation of galaxies through the stepwise hierarchical coassembly of baryons and cold dark matter halos is a fundamental paradigm underpinning modern astrophysics and predicts a significant decline in the number of giant galaxies in the early Universe. . Very massive quiescent galaxies have been observed 1 to 2 billion years after the Big Bang. These form between 300 million and 500 million years ago and are very limiting for theoretical models, as only some models can form massive galaxies this early. The spectrum of newly discovered quiescent galaxy ZF-UDS-7329 reveals features typical of much older stellar populations. Detailed modeling shows that the stellar population formed about 1.5 billion years ago, when dark matter halos with sufficient host mass had not yet assembled in the standard scenario. This observation may indicate the existence of an undetected early population of galaxies and potentially large gaps in our understanding of the nature of early stellar populations, galaxy formation, and/or dark matter.



This web image shows ZF-UDS-7329, a rare massive galaxy that formed very early in the universe. Image credit: Glazebrook other., doi: 10.1038/s41586-024-07191-9.

Galaxy formation is a fundamental paradigm underpinning modern astrophysics, and a significant decrease in the number of massive galaxies in the early universe is predicted.

Very large quiescent galaxies have been observed 1 to 2 billion years after the Big Bang, casting doubt on previous theoretical models.

Professor Carl Glazebrook, from Swinburne University of Technology, said: “We have been tracking this galaxy for seven years, observing it for hours with two of the largest telescopes on Earth to find out its age.” Ta.

“But it was too red and too faint to be measured. In the end, we had to go outside Earth and use the web to see its properties.”

“This was truly a team effort, from the infrared sky survey that began in 2010 to identifying this galaxy as an anomaly, and the many hours spent with the Keck Telescope and the Very Large Telescope. But we couldn’t confirm it, and finally, last year, we spent a lot of effort trying to figure out how to process the web data and analyze this spectrum.”

“We are now beyond the realm of possibility to have identified the oldest giant stationary monster deep in the universe,” said Dr Temmiya Nanayakkara, an astronomer at Swinburne University of Technology.

“This pushes the limits of our current understanding of how galaxies form and evolve.”

“The key question now is how do stars form so quickly, so early in the universe, and how do they form at a time when other parts of the universe are forming stars? “What kind of mysterious mechanism could cause it to suddenly stop forming?”

“Galaxy formation is determined primarily by how dark matter is concentrated.”

“The presence of these extremely massive galaxies in the early universe poses significant challenges to our standard model of cosmology.”

“This is because dark matter structures large enough to accommodate these massive galaxies are unlikely to have formed yet.”

“More observations are needed to help us understand how common these galaxies are and how massive they really are.”

“This could open new doors in our understanding of the physics of dark matter,” Professor Glazebrook said.

“Webb continues to discover evidence that massive galaxies form early.”

“This result sets a new record for this phenomenon. It’s very impressive, but it’s just one object. But we want to discover more. If I If we were to do this, it would seriously disrupt our understanding of galaxy formation.”

This finding is reported in the following article: paper Published in this week’s magazine Nature.

_____

K. Glazebrook other. A huge galaxy that formed stars at z ~ 11. Nature, published online on February 14, 2024. doi: 10.1038/s41586-024-07191-9

Source: www.sci.news