Posted on by Mark Thompson

Uranus’s Wobbling Moons Could Point to Oceans Under the Ice

This is an image of the planet Uranus taken by the spacecraft Voyager 2 in 1986.

Subsurface oceans of liquid water are a common feature of the moon’s of Jupiter and Saturn. Researchers are exploring whether the icy moons of Uranus and Neptune might have them as well. Their new paper suggests future missions to the outer Solar System could measure the rotation of the moons and detect any wobbles pointing to liquid oceans. Less wobble means the moons is mostly solid but large wobbles can indicate ice floating on an ocean of liquid. 

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Posted on by Matt Williams

Stem Cells Grown in Space Could Revolutionize Medicine Here on Earth

The International Space Station (ISS) in orbit. Credit: NASA

Extended periods spent in microgravity can take a serious toll on the human body, leading to muscular atrophy, bone density loss, vision problems, and changes to the cardiovascular, endocrine, and nervous systems. At the same time, however, scientists have found that microgravity may play a key role in the future of medicine. This includes bioprinting in space, where cultured cells are printed out to form organic tissues and organs without the need for grafts. Printing in microgravity also ensures that fragile cell structures do not collapse due to pressures caused by Earth’s gravity.

However, space medicine may also have applications for stem cell research, which also benefit from a microgravity environment. Stem cells have countless applications in medicine because of their ability to quickly replicate and differentiate into many different types of cells. Based on experiments carried out aboard the International Space Station (ISS), researchers from the Mayo Clinic in Florida determined that these abilities are enhanced when grown in space. These findings could have significant benefits in the study of disease prevention and treatment on Earth, as well as medical treatments delivered in space.

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Posted on by Mark Thompson

Magnetic Tornado is Stirring up the Haze at Jupiter’s Poles

An artificially colored view of Jupiter as seen in ultraviolet light. In addition to the Great Red Spot, which appears blue, another oval feature can be seen in the brown haze at Jupiter's south pole. The oval, an area of concentrated haze, is possibly the result of mixing generated by a vortex higher up in the planet's ionosphere. These dark UV ovals also appear periodically at the north pole, though less often. Credit Troy Tsubota and Michael Wong, UC Berkeley

Jupiter is a stunning planet to observe. Whether it be visible light or any other wavelength. In a stunning new image released by the University of California -Berkley, Jupiter is seen in ultraviolet light. The familiar Great Red Spot appears as a blue oval as do many of the familiar belt features. Around the polar regions are revealed a brown haze which is thought to be caused by a high altitude vortex mixing up the atmosphere. The jury is still out on the mechanism behind this though but it may be an interaction between Jupiter’s strong magnetic field which pierces the atmosphere near the poles. 

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Posted on by Mark Thompson

Is There Seismic Activity on Venus? Here’s How We Could Find Out

An artist’s depiction of different methods for measuring seismic and acoustic waves on Venus: a seismometer on the ground, pressure sensors on board balloons, and infrared imagers on board orbiters. Credit: Fabio Crameri

Venus is often referred to as Earths twin but size and mass are the only similarities. A visitor to one of our nearest neighbours would experience a very different world at the surface. Unlike other planets in the Solar System, Venus seems to show very little active volcanism. The environmental conditions on the surface are harsh so a researcher has suggested a combination of an orbiter, a balloon and a lander would be able to work together to detect seismic activity under the surface.

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Posted on by Andy Tomaswick

An AI Chemist Made A Catalyst to Make Oxygen On Mars Using Local Materials

Breaking oxygen out of a water molecule is a relatively simple process, at least chemically. Even so, it does require components, one of the most important of which is a catalyst. Catalysts enable reactions and are linearly scalable, so if you want more reactions quickly, you need a bigger catalyst. In space exploration, bigger means heavier, which translates into more expensive. So, when humanity is looking for a catalyst to split water into oxygen and hydrogen on Mars, creating one from local Martian materials would be worthwhile. That is precisely what a team from Hefei, China, did by using what they called an “AI Chemist.”

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Posted on by Brian Koberlein

Asteroid Samples Returned to Earth Were Immediately Colonized by Bacteria

Electron microscope images of sample A0180, showing the presence of life. Credit: Genge, et al

We’ve known for a while that complex chemistry occurs in space. Organic molecules have been detected in cold molecular clouds, and we have even found sugars and amino acids, the so-called “building blocks of life,” within several asteroids. The raw ingredients of terrestrial life are common in the Universe, and meteorites and comets may have even seeded Earth with those ingredients. This idea isn’t controversial. But there is a more radical idea that Earth was seeded not just with the building blocks of life but life itself. It’s known as panspermia, and a recent study has brought the idea back to popular science headlines. But the study is more subtle and interesting than some headlines suggest.

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Posted on by Mark Thompson

An Insanely High-Resolution Image of the Sun

The solar surface in visible light composed of data from Solar Orbiter’s instrument PHI from March 22, 2023

Our local star the Sun has been the source of many studies from ground based telescopes to space based observatories. The ESA Solar Orbiter has been approaching the Sun, capturing images along the way in unprecedented detail. It arrived at its halfway point in March last year and captured a series of 25 images. They have now been stitched together to reveal an astonishingly high resolution image. You can even zoom in to see individual granules in the solar photosphere. 

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Posted on by Matt Williams

Scientists Reveal a New Way to Study Near-Earth Asteroids

A timelapse image of the fireball event from start to finish. Credit: Western Meteor Group

On November 18th, 2022, shortly before midnight, the Catalina Sky Survey (CSS) in Arizona and other observatories worldwide detected a small object (now designated 2022 WJ1) heading toward Earth. For the next three hours, the CSS and the Southern Ontario Meteor Network (SOMN) at the University of Western Ontario monitored the object before it entered Earth’s atmosphere above Southern Ontario. At 03:26 a.m. EST (12:26 a.m. PST) on November 19th, the object appeared as a bright fireball that scattered meteorite fragments across the Niagara region.

This event triggered an international collaboration to hunt down the fragments for analysis, but none have been found yet. In a recent study led by Western University and Lowell Observatory, an international team of scientists described a new approach for studying near-Earth asteroids (NEA) based largely on 2022 WJ1. The study is significant in that the team determined the NEA’s composition—the smallest asteroid characterized to date—and established a new and integrated methodology for studying other NEAs that may impact Earth someday.

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Posted on by Evan Gough

The Hubble and FU Orionis: a New Look at an Old Mystery

This is an artist's concept of the early stages of the young star FU Orionis (FU Ori) outburst, surrounded by a disk of material. A team of astronomers has used the Hubble Space Telescope's ultraviolet capabilities to learn more about the interaction between FU Ori's stellar surface and the accretion disk that has been dumping gas onto the growing star for nearly 90 years. NASA-JPL, Caltech

In 1936 astronomers watched as FU Orionis, a dim star in the Orion constellation, brightened dramatically. The star’s brightness increased by a factor of 100 in a matter of months. When it peaked, it was 100 times more luminous than our Sun.

Astronomers had never observed a young star brightening like this.

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