Even the Outside of Hayabusa 2’s Sample Capsule has Asteroid Debris on it

Hayabusa 2 artwork
An artist's conception shows Hayabusa 2's sample return capsule making its atmospheric re-entry as its mothership flies above. (JAXA Illustration)

On December 5th, 2020, the Japanese Aerospace Exploration Agency’s (JAXA) Hayabusa 2 mission sent a sample capsule home containing debris from the near-Earth asteroid (NEA) 162173 Ryugu. This was the culmination of the probe’s first six years in space, which launched in Dec. 2014 and rendezvoused with Ryugu in June 2018. While the probe sets its sights on its new targets, scientists will be busy analyzing the Ryugu sample.

One thing they noticed immediately after opening the shell on Monday (Dec. 21st) was the black sandy dust that lined the capsule’s outer shell. According to a statement issued by JAXA, the black sand is material taken from the surface of Ryugu. Considering what’s inside sample chamber A, it appears that the amount of material obtained by Hayabusa 2 is more substantial than previously thought.

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One of the Largest, Most Complete Einstein Rings Ever Seen. Astronomers Call it the “Molten Ring”

The "Molten Ring" is one of the most complete Einstein Rings ever discovered. Credit: NASA

A very rare astronomical phenomenon has been in the headlines a lot recently, and for good reason.  It will be hundreds of years until we can see Jupiter and Saturn this close to one another again.  However, there are some even more “truly strange and very rare phenomena” that can currently be observed in our night sky.  The only problem is that in order to observe this phenomena, you’ll need access to Hubble.

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Beyond “Fermi’s Paradox” XV: What is the Percolation Hypothesis?

Artist's impression of the Milky Way Galaxy. Credit: ESO

Welcome back to our Fermi Paradox series, where we take a look at possible resolutions to Enrico Fermi’s famous question, “Where Is Everybody?” Today, we examine the possibility that Earth hasn’t been visited by aliens because interstellar travel is not very practical!

In 1950, Italian-American physicist Enrico Fermi sat down to lunch with some of his colleagues at the Los Alamos National Laboratory, where he had worked five years prior as part of the Manhattan Project. According to various accounts, the conversation turned to aliens and the recent spate of UFOs. Into this, Fermi issued a statement that would go down in the annals of history: “Where is everybody?

This became the basis of the Fermi Paradox, which refers to the disparity between high probability estimates for the existence of extraterrestrial intelligence (ETI) and the apparent lack of evidence. Since Fermi’s time, there have been several proposed resolutions to his question, which includes the very real possibility that interstellar colonization follows the basic rule of Percolation Theory.

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A Single Filament of Gas Has Been Discovered That Stretches 50 Million Light-Years

Minute vibrating strings found in string theory are not the only ones that are of interest to physicists.  The Standard Model of particle physics provides for a theory regarding a different type of string – this one is a string of very sparse gas strung over very long distances.  In fact, the standard model predicts that a large percentage of “baryonic matter” (i.e. the type that makes up everything we can see and interact with) would be contained in these filaments. And now for the first time, scientists led by a team at the University of Bonn in Germany have detected one of these super long strings of gas.

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Astronomy 2021: Top Events for the Coming Year

Comet NEOWISE

Eclipses, meteor showers, occultations and more in store for the next year of astronomy 2021.

Ready for another exciting year of skywatching? 2020 produced several memorable astronomical events, including a surprise naked eye comet C/2020 F3 NEOWISE, the sure-fire Geminid meteors, and a fine, once in a lifetime close pairing of Jupiter and Saturn rounding out the year.

The Sun also awoke from its slumber, as Solar Cycle #25 (finally) got underway in earnest, with the last half of 2020 producing some of the most massive sunspots of recent years. Expect more of the same in 2021, along with increased aurora activity, as we head towards the peak of the 11-year solar maximum in mid-2025.

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A Very Interesting Radio Signal was Just Detected Coming from Proxima Centauri

The Parkes radio telescope at Parkes Observatory in New South Wales, Australia. Astronomers using the telescope detected what appeared to be a radio signal coming from the direction of Proxima Centauri in April and May 2019. Image via Daniel John Reardon/ Wikimedia Commons.

There’s a powerful scene in the movie “Contact” (one of my favs) where lead character Ellie Arroway is sitting among an array of telescopes and hears the first alien signal – an ominous pulse – received by humanity. She races back to the control center where the array is pointed off target and then back to verify the signal. Contact is made. Shortly after, a message is found in the signal and we’ve confirmed the existence of alien life!

Ellie Arroway was inspired by a real-life pillar of the SETI community, Dr. Jill Tarter. I had the privilege of interviewing Jill Tarter last year and asked about that scene. She laughed saying “There’s not a lot of sitting around with headphones on. It’s not really that simple.” When it comes to analyzing signals from the stars for alien life, distinguishing a potential alien message from the noise of our own planet is quite complicated.

Excitingly, we’re watching that analysis play out right now as a signal which appears to originate from our closest neighbour star, Proxima Centauri, was recently detected by the Breakthrough Listen Project

Simulation of Proxima b, a known planet in the habitable zone of the red dwarf star Proxima Centauri – SpaceEngine Pro by author
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If a Planet Has a Lot of Methane in its Atmosphere, Life is the Most Likely Cause

This artist’s impression shows the planet K2-18b, it’s host star and an accompanying planet in this system. K2-18b is now the only super-Earth exoplanet known to host both water and temperatures that could support life. UCL researchers used archive data from 2016 and 2017 captured by the NASA/ESA Hubble Space Telescope and developed open-source algorithms to analyse the starlight filtered through K2-18b’s atmosphere. The results revealed the molecular signature of water vapour, also indicating the presence of hydrogen and helium in the planet’s atmosphere.

The ultra-powerful James Webb Space Telescope will launch soon. Once it’s deployed, and in position at the Earth-Sun Lagrange Point 2, it’ll begin work. One of its jobs is to examine the atmospheres of exoplanets and look for biosignatures. It should be simple, right? Just scan the atmosphere until you find oxygen, then close your laptop and head to the pub: Fanfare, confetti, Nobel prize.

Of course, Universe Today readers know it’s more complicated than that. Much more complicated.

In fact, the presence of oxygen is not necessarily reliable. It’s methane that can send a stronger signal indicating the presence of life.

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A Proposal for a Neutrino Detection Array Spanning 200,000 Square Kilometers

Sometimes in astronomy the acronym for a project fits it particularly well.  That would absolutely be the case for the Giant Radio Array for Neutrino Detection, who hopes to scale up to a size of 200,000 sq km in an effort to measure ultra-high-energy tau-neutrinos.  Is it ambitious?  Yes, but that doesn’t really stop humanity from exploring when it wants to.

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A Canadian Astronaut Will be on Artemis 2, Making it the Second Nation to Send Humans Into Deep Space (but not Walk on the Moon)

PHOTO DATE: 12-07-17 LOCATION: Ellington Field - Hangar 276 SUBJECT: CSA astronauts NEAR A T-38 PHOTOGRAPHER: BILL STAFFORD AND DAVID DEHOYOS

NASA and the Canadian Space Agency (CSA) recently announced that a Canadian astronaut will fly as part of the crew of Artemis II. This mission, scheduled for May of 2024, will see an Orion space capsule conduct a circumlunar flight where it flies around the Moon without landing. This will be the first of two crew opportunities that NASA will provide for Canadian astronauts on Artemis missions (as per the agreement).

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If Axions Explain Dark Matter, it Could be Possible to Detect Them Nearby Neutron Stars

The Robert C. Byrd Green Bank Telescope. Credit: Green Bank Observatory/NRAO

As we continue to search for dark matter particles, one thing is very clear: they cannot be any of the elementary particles we’ve discovered so far. The particles would need to have mass, but interact with light only weakly. Of the known particles, neutrinos fit that description, but neutrinos have a tiny mass, and aren’t nearly enough to explain dark matter. Some other kind of particle must make up the majority of dark matter.

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