Posted on by Brian Koberlein

Neutrinos prove the Sun is doing a second kind of fusion in its core

The central nylon balloon of the Borexino Detector. Credit: The Borexino Collaboration

Like all stars, our Sun is powered by the fusion of hydrogen into heavier elements. Nuclear fusion is not only what makes stars shine, it is also a primary source of the chemical elements that make the world around us. Much of our understanding of stellar fusion comes from theoretical models of atomic nuclei, but for our closest star, we also have another source: neutrinos created in the Sun’s core.

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Posted on by Paul M. Sutter

A third of the stars in the Milky Way came from a single merger 10 billion years ago

This artist’s impression shows how the Milky Way galaxy would look seen from almost edge on and from a very different perspective than we get from the Earth. The central bulge shows up as a peanut shaped glowing ball of stars and the spiral arms and their associated dust clouds form a narrow band. Image Credit: By ESO/NASA/JPL-Caltech/M. Kornmesser/R. Hurt - http://www.eso.org/public/images/eso1339a/, CC BY 4.0, https://commons.wikimedia.org/w/index.php?curid=28256788

Ten billion years ago the young Milky Way survived a titanic merger with a neighboring galaxy, eventually consuming the whole thing. Now, remnants of that fossil galaxy still swim in our galaxy’s core – and astronomers have discovered that almost a third of the Milky Way’s current population came from that dismantled rival.

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Posted on by Andy Tomaswick

ESA Is Going To Spend $102 Million To Remove a Single Piece of Space Junk

How much would you be willing to spend to remove a piece of space debris?  Does $102 million sound like enough?  That is how much a contract between the European Space Agency (ESA) and a Swiss start-up named ClearSpace SA is worth, and the entire contract is to simply remove a single piece of space debris.

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Posted on by Andy Tomaswick

There’s Fabric on the Space Station That Scientists Are Using to “Listen” for Space Dust Impacts

One of the biggest threats to the International Space Station (ISS) comes from micrometeoroid impacts.  A small hole in the wrong place can throw the resident astronauts into a life threatening situation.  Currently, there is no active program to monitor these types of impacts, though scientists think they must be common given the ubiquity of small objects in the ISS’s orbit.  An interdisciplinary team from MIT hopes to provide some data to support that theory by using an extremely unusual impact sensor made almost entirely out of fabric.

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Posted on by Paul M. Sutter

A new way to map out dark matter is 10 times more precise than the previous-best method

Simulation of dark matter and gas. Credit: Illustris Collaboration (CC BY-SA 4.0)

Astronomers have to be extra clever to map out the invisible dark matter in the universe. Recently, a team of researchers have improved an existing technique, making it up to ten times better at seeing in the dark.

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Posted on by Evan Gough

Every Year NASA Simulates Our View of the Moon for the Upcoming 12 Months. Here’s 2021, Hour by Hour

A screenshot from NASA's Moon Phases 2021 video in 4k. This is from the northern hemisphere view. Image Credit: NASA Goddard

There’s no real reason most of us need to know what the Moon will look like on any particular day at any particular hour next year. No reason other than intellectual curiosity, that is. So if you have a healthy supply of that, then you’ll enjoy NASA’s latest contribution to staring at the internet and wondering where the time went.

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Posted on by Andy Tomaswick

Geysers on Europa might come from pockets of water under the ice

Artist's conception of a cryovolcanic eruption on Europa. Credit: Justice Blaine Wainwright

Observations have already confirmed the existence of a sub-surface ocean on Europa, and there has been rampant speculation about whether they could contain life.  While there have been tentative plans to send a submersible spacecraft to this ocean, we are still a long way from uncovering what lies in those depths.

Which is one big reason why the geysers that occasionally shoot out of Europa’s ice sheet have garnered such interest.  Scientists hoped that some of the ejected water could come from that ocean.  It could then be sampled with a simple fly-by mission, such as Europa Clipper, rather than a submersible craft.  However, a new paper published in Geophysical Research Letters suggests a much more mundane source of the geysers – local liquid water buried in the moon’s thick ice shelf.

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Posted on by Matt Williams

The Moon has Resources, but Not Enough to Go Around

A geological map of the Moon showing different formations and mineral deposits. Credit: NASA/GSFC/USGS

It’s no secret that in this decade, NASA and other space agencies will be taking us back to the Moon (to stay, this time!) The key to this plan is developing the necessary infrastructure to support a sustainable program of crewed exploration and research. The commercial space sector also hopes to create lunar tourism and lunar mining, extracting and selling some of the Moon’s vast resources on the open market.

Ah, but there’s a snag! According to an international team of scientists led by the Harvard & Smithsonian Center for Astrophysics (CfA), there may not be enough resources on the Moon to go around. Without some clear international policies and agreements in place to determine who can claim what and where, the Moon could quickly become overcrowded, overburdened, and stripped of its resources.

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Posted on by Evan Gough

Astronomers See a Newly Forming Planetary Disk That’s Continuing to Feed On Material from its Nebula

This false-colour image shows the filaments of accretion around the protostar [BHB2007] 1. The large structures are inflows of molecular gas (CO) nurturing the disk surrounding the protostar. The inset shows the dust emission from the disk, which is seen edge-on. The "holes" in the dust map represent an enormous ringed cavity seen (sideways) in the disk structure. Image Credit: MPE

Over the last few years, astronomers have observed distant solar systems in their early stages of growth. ALMA (Atacama Large Millimeter/submillimeter Array) has captured images of young stars and their disks of material. And in those disks, they’ve spotted the tell-tale gaps that signal the presence of growing young planets.

As they ramped up their efforts, astronomers were eventually able to spot the young planets themselves. All those observations helped confirm our understanding of how young solar systems form.

But more recent research adds another level of detail to the nebular hypothesis, which guides our understanding of solar system formation.

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