The Moon is 40 Million Years Older Than We Thought

Apollo 17 astronaut Harrison Schmitt collecting a soil sample, his spacesuit coated with dust. Credit: NASA

An object the size of Mars crashed into the Earth over 4 billion years ago, creating a cloud of debris that formed the Moon. When the Apollo astronauts landed on the lunar surface, they found and brought back Moon rocks that helped pinpoint when this event happened. Now, a new study of crystals in the lunar samples pushed that event back even further –about 40 million years earlier than previous estimates — setting the Moon’s formation to about 4.46 billion years old – not long after the Earth formed.

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“The Big One”: The Most Powerful Marsquake Ever Detected

Artist illustration of Mars Insight Lander. Credit: NASA/JPL
Artist illustration of Mars Insight Lander. Credit: NASA/JPL

The ground shakes. Paintings tilt. Walls crack. Rubble may fall. On Earth, we understand how and where these events happen due to the discovery of plate tectonics – the continental crust’s creation, movement, and destruction. However, when astronauts placed seismometers on the lunar surface during NASA’s Apollo mission era, those instruments recorded quakes on the Moon. In the 1970s, the Viking landers also recorded quakes on the surface of Mars. Since neither of these worlds has plate tectonics, scientists set about collecting more data to understand the phenomena, which led to the recent NASA InSight lander. Now, a new paper in Geophysical Research Letters explains how the largest recorded seismic event on Mars provided evidence for a different sort of tectonic origin — the release of stress within the Martian crust.

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How Close is Too Close to a Kilonova?

Artist’s impression of merging neutron stars creating a kilonova. Credit: NOIRLab/NSF/AURA/J. da Silva/Spaceengine

Cataclysmic events happen in the Universe all the time. Black hole mergers, supernovae, gamma-ray bursts, and a whole host of others. Most of them happen in distant galaxies, so they pose no threat to us. But there are a few that could affect life on Earth, and a couple could even pose an existential threat. One of these threats is known as a kilonova.

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A Kilonova Simulated in 3D

An artists impression of a kilonova, the moment where two neutron stars merge. Credit: Dana Berry, Skyworks Digital, Inc.

In 2017, astronomers detected gravitational waves from colliding neutron stars for the first time: a kilonova. Enormous amounts of heavy metals were detected in the light from the explosion, and astronomers continued to watch the expanding debris cloud.

Researchers have continued to study this event. Now, using a three-dimensional computer simulation, they have created a new recreation of this merger — second by second, as it happened — giving insights into all the high-energy mayhem and heavy elements formation in this catastrophic event.

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An Unusual Crater on Pluto Might be a Supervolcano

Two features that could be cryovolcanoes exist on Pluto. They lay on either side of heart-shaped Sputnik Planitia in this color-enhanced image of Pluto from NASA’s New Horizons spacecraft taken in July 2015. (Credit: NASA / Johns Hopkins University Applied Physics Laboratory (JHUAPL) / Southwest Research Institute (SwRI))
Two features that could be cryovolcanoes exist on Pluto. They lay on either side of heart-shaped Sputnik Planitia in this color-enhanced image of Pluto from NASA’s New Horizons spacecraft taken in July 2015. (Credit: NASA / Johns Hopkins University Applied Physics Laboratory (JHUAPL) / Southwest Research Institute (SwRI))

Pluto with a super-cryovolcano? Why not! All the elements are there, just not in the way we normally think of volcanoes. And, cryovolcanoes are the reason why Pluto’s surface looks the way it does. A recent research paper explains why Pluto could be the home of the latest supervolcano discovery in the Solar System.

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JWST Looks at the Debris Disc Around a White Dwarf

Illustration of a debris disk around a white dwarf star. Credit: NASA’s Goddard Space Flight Center/Scott Wiessinger

Debris disks are quite common in the Universe. Young stars have protoplanetary disks from which planets form. Black holes have accretion disks that are the source of the galactic jets. Supernova remnants can form a disk around neutron stars. So what about white dwarfs?

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Now Astronomers have Discovered “Ultra-Fast Radio Bursts” Lasting Millionths of a Second

Artist rendition of a radio telescope discovering ultra-fast radio bursts that were recently discovered and the focus of this recent study. (Credit: Daniëlle Futselaar/www.artsource.nl)

A recent study published in Nature Astronomy examines the discovery of what astronomers are dubbing “ultra-fast radio bursts”, a new type of fast radio bursts (FRBs) that the team determined lasts for a mind-boggling ten millionths of a second or less. Traditionally, FRBs have been found to last only thousandths of a second, but this study builds on a 2021 study that hypothesized FRBs could possibly last for millionths of a second. This also comes after astronomers recently announced the discovery of the oldest and farthest FRB ever observed, approximately 8 billion light-years from Earth.

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NASA Tests a 3D Printed Aluminum Rocket Nozzle

The RAMFIRE nozzle performs a hot fire test at Marshall’s East test area stand 115. Credit: NASA

When it comes to the current era of space exploration, one of the most important trends is the way new technologies and processes are lowering the cost of sending crews and payloads to space. Beyond the commercial space sector and the development of retrievable and reusable rockets, space agencies are also finding new ways to make space more accessible and affordable. This includes NASA, which recently built and tested an aluminum rocket engine nozzle manufactured using their new Reactive Additive Manufacturing for the Fourth Industrial Revolution (RAMFIRE) process.

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A Russian Satellite Has Shifted Within 60 km of Another Spacecraft

Geostationary orbits are where telecommunication satellites and other monitoring satellites operate. This image shows one of the NOAA's Geostationary Operational Environmental Satellites. Image Credit: NOAA.

When it comes to saber-rattling, few countries employ it as much as Russia does. During their ongoing invasion and occupation of Ukraine, the country’s leadership has repeatedly threatened to use atomic weapons. But the threats don’t stop there.

A private company called Slingshot Aerospace says Russia has maneuvered one of their Luch satellites uncomfortably close to Western spacecraft in GEO (geostationary orbit.)

And it’s not the first time.

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The Solar Wind Whistles as it Passes Mercury

Image of chorus wave generation on Mercury. Credit: NASA/JHUAPL/Carnegie Institution of Washington

Mercury is the closest planet to our Sun, ranging from 46 million km (28.58 million mi) at perihelion to 69.82 million km (43.38 million mi) at aphelion. Because of its proximity, Mercury is strongly influenced by the steam of plasma constantly flowing from the Sun to the edge of the Solar System (aka. solar wind). Beginning with the Mariner 10 mission in 1974, robotic explorers have been sent to Mercury to measure how solar wind interacts with Mercury’s magnetic field to produce whistler-mode chorus waves – natural radio emissions that play a key role in electron acceleration in planetary magnetospheres.

In addition to being the cause of geomagnetic storms and auroras in planetary atmospheres, these waves also lead to electromagnetic vibrations at the same frequencies as sound, producing chirps and whistles. In a recent study, an international research team consulted data from the BepiColombo International Mercury Exploration Project, which gathered data on Mercury’s magnetosphere during its first and second flyby. Their results are the first direct probing of chorus waves in Mercury’s dawn sector, which showed evidence of possible background variations in magnetic field.

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