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What does Earth sound like from space?

They say space is silent, but turn your ears into radio wave receivers and suddenly it is a symphony of sounds. So what does Earth sound like from space?
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At 1.3 Billion Light-Years Wide, Quipu Is Officially The Biggest Thing in The Universe

Is it possible to understand the Universe without understanding the largest structures that reside in it? In principle, not likely.

In practical terms? Definitely not. Extremely large objects can distort our understanding of the cosmos.

Astronomers have found the largest structure in the Universe so far, named Quipu after an Incan measuring system. It contains a shocking 200 quadrillion solar masses.

The Shape of Mars: Discovering Wind Patterns Through Dune Formation

What can sand dunes on Earth and Mars teach us about the latter’s wind behavior and atmosphere? This is what a recently awarded NASA grant hopes to address as a PhD student at Texas A&M University will be tasked with analyzing what are known as “compound dunes”, which are large sand dunes that possess smaller dunes compounding on the top, giving the appearance they are “growing” on the top of the larger dunes. While compound dunes have been studied extensively on Earth, this will be the first time they are examined on the Red Planet.

Like sand dunes on Earth, Mars sand dunes are formed from wind processes (also called aeolian processes), which is the primary atmospheric behavior occurring on the Red Planet since its atmospheric pressure is far too low to have liquid water on its surface. Because of this, wind patterns drive sandstorms and dust storms, often encircling the entire planet and preventing sunlight from reaching the surface.

“The shape and pattern of these aeolian bedforms—geologic features shaped by wind—can tell us so much about the environment,” said Lauren Berger, who is the recipient of the NASA grant. “By comparing compound dunes on Mars to those on Earth, we can uncover similarities and differences that could help us better understand the Martian surface and atmosphere.”

The Bullseye Galaxy: A Stunning Case of a Galaxy ‘Hit’ by a Dwarf Galaxy

“This was a serendipitous discovery,” said Imad Pasha.


How many rings can galaxies have? This is what a recent study published in The Astrophysical Journal Letters hopes to address as an international team of researchers discovered a unique galaxy with nine rings, possessing six more rings than any known galaxy, that they aptly named the Bullseye Galaxy. This study has the potential to help researchers better understand the formation and evolution of galaxies throughout the universe, potentially resulting in identifying where we could find life.

The Bullseye Galaxy is known as a collisional ring galaxy (CRG) and whose radius is approximately 70 kiloparsecs (228,309 light-years), which is two and a half times larger than our Milky Way Galaxy, which is known as a spiral galaxy. After significant image analysis from NASA’s Hubble Space Telescope and the W. M. Keck Observatory, the researchers estimate the Bullseye Galaxy was created approximately 50 million years ago when a smaller blue dwarf galaxy collided with the center of the former, resulting in nine giant rings like ripples being created when a pebble is dropped in a water.

En route to Jupiter, Europa Clipper captures images of stars

Three months after its launch from NASA’s Kennedy Space Center in Florida, the agency’s Europa Clipper has another 1.6 billion miles (2.6 billion kilometers) to go before it reaches Jupiter’s orbit in 2030 to take close-up images of the icy moon Europa with science cameras.

Meanwhile, a set of cameras serving a different purpose is snapping photos in the space between Earth and Jupiter. Called star trackers, the two imagers look for stars and use them like a compass to help mission controllers know the exact orientation of the spacecraft—information critical for pointing telecommunications antennas toward Earth and sending data back and forth smoothly.

In early December, the pair of star trackers (formally known as the stellar reference units) captured and transmitted Europa Clipper’s first imagery of space. The picture, composed of three shots, shows tiny pinpricks of light from stars 150 to 300 light-years away. The starfield represents only about 0.1% of the full sky around the spacecraft, but by mapping the stars in just that small slice of sky, the orbiter is able to determine where it is pointed and orient itself correctly.

Thermalization and criticality on an analogue–digital quantum simulator

The advent of quantum simulators in various platforms8,9,10,11,12,13,14 has opened a powerful experimental avenue towards answering the theoretical question of thermalization5,6, which seeks to reconcile the unitarity of quantum evolution with the emergence of statistical mechanics in constituent subsystems. A particularly interesting setting is that in which a quantum system is swept through a critical point15,16,17,18, as varying the sweep rate can allow for accessing markedly different paths through phase space and correspondingly distinct coarsening behaviour. Such effects have been theoretically predicted to cause deviations19,20,21,22 from the celebrated Kibble–Zurek (KZ) mechanism, which states that the correlation length ξ of the final state follows a universal power-law scaling with the ramp time tr (refs. 3, 23,24,25).

Whereas tremendous technical advancements in quantum simulators have enabled the observation of a wealth of thermalization-related phenomena26,27,28,29,30,31,32,33,34,35, the analogue nature of these systems has also imposed constraints on the experimental versatility. Studying thermalization dynamics necessitates state characterization beyond density–density correlations and preparation of initial states across the entire eigenspectrum, both of which are difficult without universal quantum control36. Although digital quantum processors are in principle suitable for such tasks, implementing Hamiltonian evolution requires a high number of digital gates, making large-scale Hamiltonian simulation infeasible under current gate errors.

In this work, we present a hybrid analogue–digital37,38 quantum simulator comprising 69 superconducting transmon qubits connected by tunable couplers in a two-dimensional (2D) lattice (Fig. 1a). The quantum simulator supports universal entangling gates with pairwise interaction between qubits, and high-fidelity analogue simulation of a U symmetric spin Hamiltonian when all couplers are activated at once. The low analogue evolution error, which was previously difficult to achieve with transmon qubits due to correlated cross-talk effects, is enabled by a new scalable calibration scheme (Fig. 1b). Using cross-entropy benchmarking (XEB)39, we demonstrate analogue performance that exceeds the simulation capacity of known classical algorithms at the full system size.

10 Minutes of Violence Gave The Moon Its Very Own ‘Grand Canyons’

Arizona’s magnificent Grand Canyon is painstaking result of the Colorado River’s current wearing away the planet’s surface over millions of years.

Earth, however, isn’t the only body in the Solar System with canyons and gorges. The Moon has structures comparable to Earth’s Grand Canyon; although, in the absence of liquid water, their formation mechanism has been difficult to determine.

Now, scientists believe that they have figured it out. Two huge canyons scored into the surface of the Moon were created in the wake of a giant impact – and, in stark and jaw-dropping contrast to the Grand Canyon, their creation could have taken less than 10 minutes.

Super-Earth vs Sub-Neptune? The Winner is Super-Venus!

New observational data from the James Webb Space Telescope and simulation models have confirmed a new type of planet unlike anything found in the Solar System. This provides another piece of the puzzle to understand how planets and planetary systems form.

To date, more than 5,000 exoplanets have been confirmed around stars other than the Sun.

Many exoplanets are unlike any of the planets in the Solar System, making it difficult to guess their true natures.

Thermal interface material slashes AI data center cooling cost and GPU/CPU power use

With an assist from the NEID spectrograph, a team of astronomers have confirmed the existence of exoplanet Gaia-4b—one of the most massive planets known to orbit a low-mass star. Gaia-4b is also the first planet detected by the European Space Agency’s Gaia spacecraft using the astrometric technique.

NEID is a high-precision radial-velocity spectrograph that is designed to measure the extremely minute wobble of using the radial velocity effect. This effect results from the mutual gravitational force between a planet and its which causes the star’s position to shift very slightly as the planet travels around it. With this powerful capability, one of NEID’s main science goals is to confirm exoplanet candidates found by other exoplanet missions.

NEID is mounted on the WIYN 3.5-meter Telescope at the U.S. National Science Foundation Kitt Peak National Observatory (KPNO), a program of NSF NOIRLab.

Interaction of kinetic waves and suprathermal particles could be key to unlocking biggest mystery in heliophysics

A graduate research assistant at The University of Alabama in Huntsville (UAH), a part of The University of Alabama system, has published a paper in the journal Astronomy & Astrophysics that builds on an earlier study to help understand why the solar corona is so hot compared to the surface of the sun itself.

To shed further light on this age-old mystery, Syed Ayaz, a Ph.D. candidate in the UAH Center for Space Plasma and Aeronomic Research (CSPAR), employed a statistical model known as a Kappa distribution to describe the velocity of particles in space plasmas, while incorporating the interaction of suprathermal particles with kinetic Alfvén waves (KAWs).

KAWs are oscillations of the charged particles and as they move through the , caused by motions in the photosphere, the sun’s outer shell. The waves are a valuable tool for modeling various phenomena in the solar system, including particle acceleration and wave-particle interactions.