Uh oh, a Recent Study Suggests that Dark Energy’s Strength is Increasing

The concept of accelerating expansion does get you wondering just how much it can accelerate. Theorists think there still might be a chance of a big crunch, a steady-as-she-goes expansion or a big rip. Or maybe just a little rip?

Staring into the Darkness

The expansion of our universe is accelerating. Every single day, the distances between galaxies grows ever greater. And what’s more, that expansion rate is getting faster and faster – that’s what it means to live in a universe with accelerated expansion. This strange phenomenon is called dark energy, and was first spotted in surveys of distant supernova explosions about twenty years ago. Since then, multiple independent lines of evidence have all come to the same morose conclusion: the universe is getting fatter and fatter faster and faster.

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Weekly Space Hangout: Jan 30, 2019: Rod Pyle talks “Space 2.0”

Hosts:
Fraser Cain (universetoday.com / @fcain)
Dr. Morgan Rehnberg (MorganRehnberg.com / @MorganRehnberg & ChartYourWorld.org)

Tonight we welcome author Rod Pyle who will be discussing his new book, Space 2.0: How Private Spaceflight, a resurgent NASA, and International Partners Are Creating a New Space Age (BenBella Books, February 2019), written in collaboration with the National Space Society.

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Crew Dragon Rolls Out to the Launch Pad. Demo-1 Flight Should Happen Shortly

An artist's illustration of the SpaceX Dragon lifting off. Image Credit: SpaceX
An artist's illustration of the SpaceX Dragon lifting off. Image Credit: SpaceX

The long-anticipated first flight of the SpaceX Crew Dragon is almost here. Early in January, the Crew Dragon was rolled out of its hangar at Kennedy Space Center, and on January 24th it performed a brief static firing as part of its testing. The Crew Dragon’s inaugural flight, called Demo-1, is not far off.

Neither NASA nor SpaceX has given us a date for Demo-1, but we’re getting close.

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One of the Oldest Earth Rocks Turned up on the Moon, of all Places

An artist's rendering of the early Moon and Earth, which sustained many asteroid impacts. Many of those asteroids and possibly dark comets contributed their water to the infant Earth. As it cooled, the water outgassed as vapor. Credit: Simone Marchi (SwRI)/SSERVI/NASA
An artist's rendering of the early Moon and Earth, which sustained many asteroid impacts. Many of those asteroids and possibly dark comets contributed their water to the infant Earth. As it cooled, the water outgassed as vapor. Credit: Simone Marchi (SwRI)/SSERVI/NASA

According the Giant Impact Hypothesis, the Earth-Moon system was created roughly 4.5 billion years ago when a Mars-sized object collided with Earth. This impact led to the release of massive amounts of material that eventually coalesced to form the Earth and Moon. Over time, the Moon gradually migrated away from Earth and assumed its current orbit.

Since then, there have been regular exchanges between the Earth and the Moon due to impacts on their surfaces. According to a recent study, an impact that took place during the Hadean Eon (roughly 4 billion years ago) may have been responsible for sending the Earth’s oldest sample of rock to the Moon, where it was retrieved by the Apollo 14 astronauts.

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Tiny Object Found at the Edge of the Solar System for the First Time. A Kuiper Belt Object that’s Only 2.6 km Across

An artist's illustration of the newly-detected object. Image Credit: Ko Arimatsu

The Kuiper Belt, or the Edgeworth-Kuiper Belt, is home to ancient rocks. Kuiper Belt Objects, or KBOs, are remnants of the early planet-formation days of our Solar System. Small KBOs, in the 1 km. diameter range, have been theorized about for decades, but nobody’s every found one.

Until now.

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Astronomers are Continuing to Watch the Shockwaves Expand from Supernova SN1987A, as they Crash Into the Surrounding Interstellar Medium

Composite image showing the effects of a powerful shock wave moving away from the explosion. Credit: X-ray: NASA/CXC/PSU/S.Park & D.Burrows.; Optical: NASA/STScI/CfA/P.Challis)

When stars reach the end of their life cycle, many will blow off their outer layers in an explosive process known as a supernova. While astronomers have learned much about this phenomena, thanks to sophisticated instruments that are able to study them in multiple wavelengths, there is still a great deal that we don’t know about supernovae and their remnants.

For example, there are still unresolved questions about the mechanisms that power the resulting shock waves from a supernova. However, an international team of researchers recently used data obtained by the Chandra X-Ray Observatory of a nearby supernova (SN1987A) and new simulations to measure the temperature of the atoms in the resulting shock wave.

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Without the Impact that Formed the Moon, We Might Not Have Life on Earth

The chemicals that made life possible on Earth may have come from another planet that collided with Earth, forming the Moon. Image Credit: Rice University
The chemicals that made life possible on Earth may have come from another planet that collided with Earth, forming the Moon. Image Credit: Rice University

The Earth wasn’t formed containing the necessary chemicals for life to begin. One well-supported theory, called the “late veneer theory”, suggests that the volatile chemicals needed for life arrived long after the Earth formed, brought here by meteorites. But a new study challenges the late veneer theory.

Evidence shows that the Moon was created when a Mars-sized planet named Theia collided with the Earth. The impact created a debris ring out of which the Moon formed. Now, this new study says that same impact may have delivered the necessary chemicals for life to the young Earth.


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Here it is, the high resolution photo of MU69 we’ve all been waiting for.

High-resolution image of Ultima Thule. Credit: NASA/JHUAPL/SwRI

On December 31st, 2018, NASA’s New Horizons mission made history by being the first spacecraft to rendezvous with a Kuiper Belt Object (KBO) named Ultima Thule (2014 MU69). This came roughly two and a half years after New Horizons became the first mission in history to conduct a flyby of Pluto. Much like the encounter with Pluto, the probe’s rendezvous with Ultima Thule led to a truly stunning encounter image.

And now, thanks to a team of researchers from the John Hopkins University Applied Physics Lab (JHUAPL), this image has been enhanced to provide a more detailed and high-resolution look at Ultima Thule and its surface features. Thanks to these efforts, scientists may be able to learn more about the history of this object and how it was formed, which could tell us a great deal about the early days of the Solar System.

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