Universe Today

September 12, 2021September 12, 2021 by Brian Koberlein

Researchers Generate an Entire Virtual Universe and Make it Available for Download (if you Have 100 Terabytes of Free Hard Drive Space)

The distribution of dark matter in the Uchuu simulation. Credit: Tomoaki Ishiyama

Astronomy is a bit different from many sciences because you only have a sample size of 1. The cosmos contains everything we can observe, so astronomers can’t study multiple universes to see how our universe ticks. But they can create computer simulations of our universe. By tweaking different aspects of their simulation, astronomers can see how things such as dark matter and dark energy play a role in our universe. Now, if you are willing to spring for a fancy hard drive, you can keep one of these simulations in your pocket.

September 12, 2021September 10, 2021 by Paul M. Sutter

In Addition to Gravitational Waves, is There any way to Detect Merging Black Holes

In February 2016, LIGO detected gravity waves for the first time. As this artist's illustration depicts, the gravitational waves were created by merging black holes. The third detection just announced was also created when two black holes merged. Credit: LIGO/A. Simonnet. — Artist's impression of merging binary black holes. Credit: LIGO/A. Simonnet.

If two black holes merge in the middle of space, and nobody’s around to see it, does it really happen?

September 11, 2021September 10, 2021 by Paul M. Sutter

ALMA’s new Receivers Will let it see Longer Wavelengths, Peering Closer to the Beginning of the Universe

ALMA is an array of dishes located at the Atacama Desert in Chile. Image: ALMA (ESO/NAOJ/NRAO), O. Dessibourg

The ALMA telescope is getting a new set of receivers, enabling it to detect wavelengths down to 8.5 mm. These wavelengths are crucial for observations of the transformative epoch of reionization, when the first stars to appear in the universe unleashed a fury of radiation.

September 11, 2021September 10, 2021 by Paul M. Sutter

Doomed Satellite was Equipped With a Drag Sail to Deorbit it After its Mission was Complete

Drag sails can be used to de-orbit old satellites. Image Credit: Purdue University/David Spencer

A team at Purdue University developed a drag sail to attach to satellites to help them de-orbit to combat space debris. Unfortunately, the rocket carrying the test device, launched by Firefly Aerospace, exploded shortly after launch.

September 10, 2021September 10, 2021 by Evan Gough

Why are Rubble Pile Asteroids Shaped Like Diamonds?

The asteroid Bennu from a distance of 24 km (15) miles captured by the PolyCam on OSIRIS-REx. The spacecraft has detected water on Bennu. On the bottom right in the termination line is the large boulder. The image is a mosaic constructed of 12 images. Image Credit: NASA/Goddard/University of Arizona.

Scientists are fortunate enough to have detailed, close-up views of the near-Earth asteroids Bennu and Ryugu. Both asteroids have a diamond shape, for some reason. Why? Up until now, it’s been a puzzle.

Now a team of scientists has tackled the question and may have come up with the answer.

September 10, 2021September 10, 2021 by Paul M. Sutter

There Should be More Material Left Over From Bombardment Eras. Maybe the Sun Blew it all Away?

This artwork shows a rocky planet being bombarded by comets. Image credit: NASA/JPL-Caltech

The early solar system was an especially violent place. The terrestrial planets (Mercury, Venus, Earth, and Mars) likely formed by suffering countless collisions between planetesimals. But the material left over from all those collisions should have remained in orbit around the sun, where it would’ve eventually found itself in the asteroid belt. But the belt contains no such record of that process.

September 10, 2021September 10, 2021 by Andy Tomaswick

Astronomers Create 3D Printed Nebulae

Visualizations can inspire creative new ways of thinking about an object. But holding that visualization in your hand adds a whole other level of impact to it. That desire for impact has led Dr. Nia Imara, an astrophysicist and artist at UC Santa Cruz, to create the first-ever 3D printed models of stellar nurseries.

September 9, 2021September 9, 2021 by Matt Williams

Perseverance Drills Another Hole, and This Time the Sample is Intact

When it landed on Mars in February of 2021, the Perseverance rover joined a small armada of robotic explorers working hard to characterize Mars’ environment and atmosphere and determine if it ever supported life. But unlike its predecessors, one of the key objectives of the rover is to obtain samples of Martian soil and rock, which it will leave in a cache for later retrieval by a joint NASA-ESA mission.

This will be the first sample return from Mars, and the analysis of these samples will provide new insight into the geological and environmental evolution of Mars. The first attempt to obtain a sample didn’t go so well, with the sample crumbling before it was placed in the cache. Undeterred, the science team moved onto the next site and prepared to try again. A few days ago, NASA confirmed that the rover succeeded in its second attempt and has the pictures to prove it!

September 9, 2021September 8, 2021 by Paul M. Sutter

White Dwarfs can Continue Burning Hydrogen, Even After They’re Dead

White dwarfs are supposed to be dead remnants of stars, doomed to simply fade away into the background. But new observations show that some are able to maintain some semblance of life by wrapping themselves in a layer of fusing hydrogen.

September 9, 2021September 9, 2021 by Evan Gough

Protoplanetary Disks Throw Out More Material Than Gets Turned Into Planets

A protosolar disk is the disk of material around a young stellar object that isn't yet a star. It's called a protoplanetary disk once the star has formed and begun fusion. Planetesimals are the building blocks of planets and are present in both stages of a disk's evolution. Image Credit: NASA/JPL

When a young solar system gets going it’s little more than a young star and a rotating disk of debris. Accepted thinking says that the swirling debris is swept up in planet formation. But a new study says that much of the matter in the disk could face a different fate.

It may not have the honour of becoming part of a nice stable planet, orbiting placidly and reliably around its host star. Instead, it’s simply discarded. It’s ejected out of the young, still-forming solar system to spend its existence as interstellar objects or as rogue planets.