What’s Being Done to Protect Astronauts From Radiation in Deep Space?

astronauts faced possible radiation dangers on the Moon.
Apollo 17 astronaut Harrison "Jack" Schmitt at Tracy Rock on the lunar surface. If a solar storm had hit the Moon while the astronauts were on the surface exploring, it could have been a disaster. Credit: NASA.

In 1982, author James Michener published his sprawling Space Race novel, Space. In it, he describes a fictional Apollo 18 mission to the Moon. While the astronauts are on the surface, the Sun unleashes a huge storm, trapping them outside of their protective capsule. The two men get blasted by lethal amounts of radiation before they can get to safety.

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Yeast Will Fill in for Humans on Artemis I, Soaking up a Lunar Mission’s Worth of Radiation

SLS and Orion at launch pad
A full Moon looms over NASA's Space Launch System and its Orion capsule containing yeast cells bound for an epic trip. (NASA Photo / Ben Smegelsky)

When Artemis 1 finally takes flight (possibly this Saturday), twelve bags of baker’s yeast will go along for the ride. Millions of these cells of Saccharomyces cerevisiae will experience deep space as it grows and reproduces. The yeast is a stand-in for actual people. The idea is to see what threat the radiation environment in deep space poses to living cells. The data from the experiment will point to how genetic engineering might help reduce damage to astronauts.

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Astronomers Find the Oldest Planetary Nebula

Abell 39 is a good example of a planetary nebula, similar to the one discovered in M37. Credit: WIYN/NOAO/NSF

Planetary nebulae are short-lived “leftovers” of sun-like stars. Most of these “star ghosts” only last—at most—about 25,000 years. Usually, their clouds of debris disperse so broadly that they fade out fairly quickly. However, there’s one that has lasted at least 70,000 years. That makes it a “grande dame” of planetary nebulae.

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A Merger Completely Shut Down Star Formation

star formation stopped by galaxy merger
Scientists observing the newly-dormant galaxy SDSS J1448+1010 found that most of its fuel for star formation had been tossed out of the system as it merged with another galaxy. That gas is not forming new stars for the galaxy but remains nearby in new structures known as tidal tails. This artist’s conception shows the stream of gas and stars that were flung away during the merger. Credit: ALMA (ESO/NAOJ/NRAO), S.Dagnello (NRAO/AUI/NSF)

What’s the recipe for forming stars? Yep, lots of gas and dust. Galaxies rich in these materials get to make a lot of stars. When the supply runs out, star formation stops. That’s what’s happened in the galaxy SDSS J1448+1010, but there’s a twist. The galaxy didn’t stop making stars because it made so many it ran out of material. No, that happened because it merged with another galaxy. That action flung most of the available gas and dust out of the galaxy entirely. Essentially, the galaxy to went “dormant” and ceased star-forming operations.

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Problem Solved! Voyager 1 is no Longer Sending Home Garbled Data!

Voyager 1
Artist's concept of NASA's Voyager spacecraft. Image credit: NASA/JPL-Caltech

Earlier this year, the teams attached to the Voyager 1 mission noticed that the venerable spacecraft was sending weird readouts about its attitude articulation and control system (called AACS, for short). The data it’s providing didn’t really reflect what was actually happening onboard. That was the bad news. The good news was that it didn’t affect science data-gathering and transmission. And, the best news came this week: team engineers have fixed the issue with the AACS and the data are flowing normally again.

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Science Fiction was an Inspiration for Many Professional Astronomers

Science fiction universe for Star Trek
The Star Trek universe occurs in the Milky Way Galaxy; this show and its memorable characters are cited, along with many other SF works as influences for scientists. Courtesy R.H. Hurt.

What do MINBAR, TARDIS, Cardassian Expansion, BoRG, DS9, Tatooines, and ACBAR all have in common? They’re names of astronomical surveys and software created by astronomers who say that science fiction (SF) influenced their careers. Those names are just one indicator of widespread interest in SF in the science community. It’s not surprising considering how many scientists (and science writers) grew up with the genre.

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Carbon Monoxide is Plentiful in Nebulae, but Then Disappears When Planets Form. Now we Know Where it Goes!

carbon monoxide in protoplanetary disk
ALMA image of the protoplanetary disk surrounding the young star HD 163296 as seen in dust. New studies show there may be carbon monoxide ice there. Courtesy NRAO.

Protoplanetary disks—those nurseries around young stars where planets form—are filled with gas and dust. In particular, many show a lot of carbon monoxide gas. It’s a handy “tracer” to estimate the mass of a cloud, its composition, and even its temperature. It’s also easy to observe. However, astronomers think there should be more of it than they’re observing in many disks. And that prompted a question: where’s the rest of it?

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New Horizons Could Still Have More Adventures Ahead

Currently exploring the Kuiper Belt, New Horizons is just one of five spacecraft to reach beyond 50 astronomical units, on its way out of the solar system and, eventually, into interstellar space. (Credit: NASA/Johns Hopkins APL/Southwest Research Institute)

Remember New Horizons? That plucky little spacecraft that gave us our first up-close looks at Pluto and Arrokoth? Of course, we do! Well, it’s still out there, traveling deeper into the Kuiper Belt. Just because it finished its primary mission doesn’t mean we’re done with it yet.

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Samples From Asteroid Ryugu Contain Bits That Came From Outside the Solar System

Asteroid Ryugu, as imaged by the Hayabusa2 spacecraft. The red dot marks the sampling location. Image Credit: JAXA/Hayabusa2
Asteroid Ryugu, as imaged by the Hayabusa2 spacecraft. The red dot marks the sampling location. Image Credit: JAXA/Hayabusa2

Long before our Sun began to form, stars were dying in our part of the galaxy. One of them exploded as a supernova. The catastrophe created minute grains of dust and the force of the explosion blasted through a nearby cloud of gas and dust. That action seeded the cloud with “alien” materials from the dead star. The shock wave from the supernova also caused the cloud to collapse in on itself to create the Sun. The “leftovers” of the cloud became the planets, moons, rings, comets, and asteroids of our solar system.

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Would We Have Continents Without Asteroid Impacts?

continents
An impact between a Mars-sized protoplanet and early Earth is the most widely-accepted origin of the Moon. Did smaller impacts seed the formation of continents? (NASA/JPL-Caltech)

Early Earth was a wild and wooly place. In its first billion years, during a period called the Archean, our planet was still hot from its formation. Essentially, the surface was lava for millions of years. Asteroids bombarded the planet, and the place was still recovering from the impact that formed the Moon. Oceans were beginning to form as the surface solidified and water outgassed from the rock. The earliest atmosphere was actually rock vapor, followed quickly by the growth of a largely hot carbon dioxide and water vapor blanket. Earth was just starting land masses that later became continents. For decades, geologists have asked: what started continental formation?

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