Astronomy

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The composition and great density of 'hot Saturn' exoplanet Smertrios are a challenge to planet formation models that the detection of water may help solve.

Novel ways to move on other celestial bodies always draw the attention of the space exploration community. Here at UT, we’ve reported on everything from robots that suspend themselves from the walls of Martian caves to robots that hop using jets of locally mined gas. But we haven’t yet reported on the idea of a balloon that “walks.” But that is the idea behind the BALloon Locomotion for Extreme Terrain, or BALLET, a project from Hari Nayar, a Principal Roboticist at NASA’s Jet Propulsion Laboratory, and his colleagues.

How exactly does a balloon “walk,” you might ask? By picking up and moving one of its six feet. BALLET’s architecture involves a positively buoyant balloon supporting six “feet” attached to adjustable cables. The “feet” are small science packages capable of taking small surface samples or analyzing the chemical composition of the part of the surface it touches.

Each foot is attached to three cables, individually controlled by pulleys. When a foot is done doing its science work at a given location, BALLET retracts the cables for the foot, lifting it off the surface. It then extends the cables using different lengths for the cables to place the foot in a new location.

Balloons have been an integral part of NASA’s explorations, as SciShow describes in this video.
Credit – SciShow

Preliminary research on the concept was done as part of a NASA Institute for Advanced Concepts (NIAC) grant in 2018. That research showed that it was better to lift two opposing feet off the ground at the same time to ensure the balloon’s stability. It also demonstrated where the concept would be most useful—Titan.

Balloon locomotion is typically considered somewhere like Venus, where it could float in the atmosphere in conditions similar to Earth. However, that altitude would make controlling a payload placed on the ground exceedingly tricky. Additionally, the harsh conditions close enough to the ground to be feasible would make the material requirements of the system untenable.

Similarly, a balloon could also work on Mars, but the high wind speeds of the sparse atmosphere would make controlling the balloon difficult. Titan offers the best of both worlds – a relatively stable, thick atmosphere where a negatively buoyant balloon would be feasible and stable environmental conditions that wouldn’t blow BALLET everywhere.

The current plan for exploring Titan – a helicopter named Dragonfly.

It also has many interesting places to explore, including cryovolcanoes and methane lakes. BALLET would allow traversal over even some of the most difficult terrain without accounting for considerations that would dramatically affect the capabilities of either a rover or a helicopter, such as the planned Dragonfly mission. 

There are still plenty of design considerations, though, such as the difficulty of controlling all the different variables, such as balloon orientation, cable length for each of the 18 cables, and pathfinding, simultaneously. After the completion of the Phase I project, the concept appears to be on hold in terms of receiving further funding from NASA at this point.

However, in terms of applications, BALLET also has some obvious ones on Earth. One that immediately sprang to mind is the collection of “nodules” as part of an undersea mining operation. Given the increased need for cobalt and other materials provided in those nodules and the bad image that comes from the destruction of the seabed that comes with traditional mining techniques, this idea might be one of those rare space exploration ideas that sooner sees an application on Earth than off of it.

Learn More:
Nayar et al. – Balloon Locomotion for Extreme Terrain
UT – A Robot With Expandable Appendages Could Explore Martian Caves And Cliffs
UT – A Hopping Robot Could Explore Europa Using Locally Harvested Water
UT – Drones Could Help Map the Lunar Surface with Extreme Precision

Lead Image:
Artist’s conception of the BALLET concept mission architecture, including a “single step” action.
Credit – Nayar et al.

The post A Walking Balloon Could One Day Explore Titan – Or Earth’s Sea Floor appeared first on Universe Today.

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What happens when a spiral and an elliptical galaxy collide? To celebrate the second anniversary of the “first light” for the Webb telescope, NASA released an amazing infrared view of two galaxies locked in a tight dance. They’re called the Penguin and the Egg and their dance will last hundreds of millions of years.

“In just two years, Webb has transformed our view of the universe, enabling the kind of world-class science that drove NASA to make this mission a reality,” said Mark Clampin, director of the Astrophysics Division at NASA Headquarters in Washington. “Webb is providing insights into longstanding mysteries about the early Universe.”

Webb Witnesses a Galactic Dance

The telescope targeted a collision scene named Arp 142 containing both galaxies—a scene that the Hubble Space Telescope has also explored. They lie about 326 million light-years away. Their first close encounter began somewhere between 25 and 75 million years ago. That’s when two partner galaxies had the first of many passages that will distort their shapes more than they already appear here.

The Hubble Space Telescope captured visible light when observing Arp 142, nicknamed the Penguin and the Egg, in 2013. The Webb view (right) shows the near-infrared view. Courtesy NASA, ESA, CSA, STScI

Webb’s observations, which combine near- and mid-infrared light from Webb’s NIRCam (Near-Infrared Camera) and MIRI (Mid-Infrared Instrument), respectively, clearly show that a hazy cloud of gas and stars (blue) links them together. The close approach also set off tremendous bursts of star birth in the colliding clouds of gas and dust.

Eventually, after several close approaches in their cosmic dance, these two galaxies will merge completely. Observers hundreds of millions of years in the future will look at Arp 142 and see one massive elliptical galaxy.

Interestingly, Webb’s sharp infrared eyes also picked out very distant galaxies. Some lie beyond this cosmic collision, although at least one lies about a hundred million light-years closer to Earth. It bristles with hot, young, newborn stars.

How The Arp 142 Galaxies Experience a Merger

The Penguin and Egg galaxies lie about 100,000 light-years apart but they affect each other. The Egg’s gravitational pull distorts the spiral and that interaction is “sculpting” the Penguin. The core makes up the eye of a penguin. The slowly unwinding spiral arms form a beak, head, backbone, and tail.

Webb’s infrared view reveals otherwise unseen activity between the two. For example, the Penguin is rich in dust. Webb’s view shows us how gravitational interactions pull that dust away from the Penguin. There are also scads of new stars in the galaxy, surrounded by what looks like smoke. Webb’s view shows this hydrogen cloud. It’s rich in carbon-based molecules called polycyclic aromatic hydrocarbons (PAHs). These are incredibly abundant in the Universe and astronomers find them just about everywhere they point a telescope.

Webb’s mid-infrared MIRI image shows the Egg as a small teal oval. Mid-infrared light predominantly shows the oldest stars in the elliptical galaxy, which has lost or used up most of its gas and dust. This is why the view is so different from the combined image, which includes near-infrared light. Courtesy: NASA, ESA, CSA, STScI

By contrast, in Webb’s view, the Egg looks like it’s hardly been touched—it’s still an egg-shaped elliptical. It has much older stars than the Penguin. Past epochs of star birth have pretty much used up the available star-making material. So, even though the two galaxies have about the same mass, the Egg just doesn’t have as much material to get stretched out or turned into stars.

Zeroing in on Webb’s Two Views

If you look at both of Webb’s infrared views of the galaxy collision, you can see marked differences in them. That’s because each one prioritizes a different set of infrared wavelengths. In the mid-infrared view, the egg looks tiny and washed out. That’s because the instrument sees only the old stars in the Egg. By contrast, the Penguin’s distorted core and spiral arms are brimming with young stars embedded in the PAH-rich hydrogen clouds.

The combined near- and mid-infrared view shows more of the gas clouds as the Egg tears them away from the Penguin. These regions will glitter in the future with the light of newly formed stars. For now, however, only cooler, older stars are visible in the combined image. The younger ones are there, but the mid-infrared-sensitive instrument doesn’t spot them.

Here’s a flythrough visualization of Arp 142. NASA, ESA, CSA, Ralf Crawford (STScI), Joseph DePasquale (STScI), Christian Nieves (STScI), Joseph Olmsted (STScI), Alyssa Pagan (STScI), Frank Summers (STScI), Greg Bacon (STScI) Why Does Webb Study Galaxy Collisions?

By studying this galactic collision site, the Webb telescope further probes the activity as galaxies evolve. Collisions are an integral part of this process. Our Milky Way Galaxy will dance with the nearby Andromeda Galaxy, starting in about 5 billion years. Images and data from observations of other galaxies doing the same thing give astronomers a chance to understand the process and forecast the distant future when something called “Milkdromeda” will contain the stars and planets of two spirals that once were close neighbors.

For More Information

Vivid Portrait of Interacting Galaxies Marks Webb’s Second Anniversary
Galaxy Evolution

The post Webb Completes Its Second Year of Operations appeared first on Universe Today.

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