Sierra Space Inflated a Habitat to Destruction, Testing its Limits Before Going to Orbit

What’s left of Sierra Space’s LIFE Habitat test article after the Ultimate Burst Pressure Test. Credit: Sierra Space.

Normally, it would be a very bad day if your space station habitat module blew up. But it was all smiles and high-fives in mission control when Sierra Space’s LIFE habitat was intentionally over-inflated until it popped spectacularly in an Ultimate Burst Pressure (UBP) test. This video shows the moment of boom from several different viewpoints.

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Rubble Pile Asteroids Might be the Best Places to Build Space Habitats

Illustration: SpaceX Crew Dragon at ISS
An illustration shows SpaceX's Crew Dragon capsule approaching the International Space Station. (Credit: SpaceX)

The stars call to us, as Carl Sagan once said. Given the human drive to explore our world and expand our reach, it is likely only a matter of time before we begin to build our homes in the solar system. The Moon and Mars could be acceptable destinations, but nearby asteroids could also become homes, as a recent study shows.

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Could Life Survive on Frigid Exo-Earths? Maybe Under Ice Sheets

This artist's illustration shows what an icy exo-Earth might look like. A new study says liquid water could persist under ice sheets on planets outside of their habitable zones. Image Credit: NASA

Our understanding of habitability relies entirely on the availability of liquid water. All life on Earth needs it, and there’s every indication that life elsewhere needs it, too.

Can planets with frozen surfaces somehow have enough water to sustain life?

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Perseverance Heard a Dust Devil on Mars, and Now You Can Too

NASA's Perseverance Mars rover used one of its navigation cameras to capture these dust devils swirling across Jezero Crater on July 20, 2021, the 148th Martian day, or sol, of the mission. Credit: NASA/JPL-Caltech/SSI

For years, we’ve seen images from various Mars rovers and landers of dust devils churning across the dusty landscape of the Red Planet. But now, thanks to a microphone on the Perseverance rover and a whirling dust storm that passed directly over the rover, we know what a dust devil on Mars sounds like, too.

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The Oort Cloud Could Have More Rock Than Previously Believed

This artist's concept puts Solar System distances in perspective. The scale bar is in astronomical units, with each set distance beyond 1 AU representing 10 times the previous distance (logarithmic scale.) The image shows Voyager 2's location in 2018. (It also shows where the star Ross 248 will be in 40,000 years, when it will briefly be the closest star to the Sun.) Image Credit: NASA/JPL-Caltech

The Oort Cloud is a collection of icy objects in the furthest reaches of the Solar System. It contains the most distant objects in the Solar System, and instead of orbiting on a plane like the planets or forming a ring like the Kuiper Belt, it’s a vast spherical cloud centred on the Sun. It’s where comets originate, and beyond it is interstellar space.

At least that’s what scientists think; nobody’s ever seen it.

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The Formation of the Southern Ring Nebula was Messier Than the Death of a Single Star

JWST images of the Southern Ring Nebula as seen from the telescope's NIRCam (left) and MIRI (right). Credit: NASA, ESA, CSA, and STScI

Two thousand five hundred years ago, during the height of the bronze age, an old red star died. Its outer layers expanded over time, becoming what is now known as the Southern Ring Nebula, or less romantically, NGC 3132. By the looks of it, this planetary nebula looks like many others. As Sun-like stars die, they swell to become red giants before becoming a white dwarf, and their outer layers typically become a planetary nebula. But a recent study finds that this particular nebula formed in a way quite messier than we had thought.

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Hubble Sees a Glittering Jewel in the Small Magellanic Cloud. But the Jewel is Disappearing

A small portion of the Small Magellanic Cloud (SMC) is pictured in this image from the NASA/ESA Hubble Space Telescope. Image Credit: NASA/ESA

As far as we know, nobody lives in our neighbour, the Small Magellanic Cloud (SMC.) So it’s okay to point our telescope there and gaze at it.

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ESA’s Upcoming Mission Will Tell us if Venus is Still Volcanically Active

Venus Envision mission
EnVision orbiting Venus and studying its surface and atmosphere. The mission will launch in the early 2030s. Courtesy ESA.

When it comes to planetary exploration, particularly of Venus, a big part of the story is under the surface. It’s a story that ESA’s EnVision mission was selected to tell when it gets to the planet in the 2030s. That’s because the spacecraft will include a subsurface radar sounder (SRS) to “peek under the surface” of Venus.

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In Case you Missed it, Here are Some Amazing Pictures of Mars Hiding Behind the Moon

This is the occultation of Mars by the Full Moon on December 7, 2022, in a composite showing the motion of Mars relative to the Moon. The motion here is from left to right. However, while this composite makes it look like Mars was doing the moving, it was really the Moon that was passing in front of Mars. Credit and copyright: Alan Dyer.

Last week gave us a celestial triple header, all in one night. The Moon was full and Mars was at opposition (at its closest point to Earth). But the pièce de résistance was when the Moon occulted or passed in front of Mars on the evening/morning of December 7th/8th. Our astrophotographer friends were out in full force to capture the event.

Our lead image comes from prolific amateur astronomer and photographer Alan Dyer, who observed the occultation from his home in Alberta, Canada, and created this composite view of the night’s activities. “While this composite makes it look like Mars was doing the moving,” Dyer explained on Flickr, “it was really the Moon that was passing in front of Mars. But for this sequence I set the telescope mount to track the Moon at its rate of motion against the background stars and Mars, to keep the Moon more or less stationary on the frame while Mars and the background sky passed behind it.”

Here are some more great views from around the world:

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Astronomers Spot Three Interacting Systems with Twin Discs

Artist's conceptualization of the dusty TYC 8241 2652 system as it might have appeared several years ago when it was emitting large amounts of excess infrared radiation. Credit: Gemini Observatory/AURA artwork by Lynette Cook. https://www.gemini.edu/node/11836

According to the most widely-accepted theory about star formation (Nebular Hypothesis), stars and planets form from huge clouds of dust and gas. These clouds undergo gravitational collapse at their center, leading to the birth of new stars, while the rest of the material forms disks around it. Over time, these disks become ring structures that accrete to form systems of planets, planetoids, asteroid belts, and Kuiper belts. For some time, astronomers have questioned how interactions between early stellar environments may affect their formation and evolution.

For instance, it has been theorized that gravitational interactions with a passing star or shock waves from a supernova might have triggered the core collapse that led to our Sun. To investigate this possibility, an international team of astronomers observed three interacting twin disc systems using the Spectro-Polarimetric High-contrast Exoplanet REsearch (SPHERE) on the ESO’s Very Large Telescope (VLT). Their findings show that due to their dense stellar environments, gravitational encounters between early-stage star systems play a significant role in their evolution.

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