Astronomy and Planetary Science Thread

The GeologyHub channel has a video about the potential 2032 impact site location by the 2024 YR4 asteroid:
More about Bennu

on other worlds

Debris

Shielding

Radio silence broken--by airplanes

Spaceflight Propulsion

Jupiter

Supernovae

Black holes--no singularities?

Drake updates

The clouds of Mars

Rings of the Lords

Galacticae
 
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JWST capturing some space motions:


JWST is back with mind-blowing new images that aren’t just beautiful, they’re revealing space in motion! From expanding Wolf-Rayet dust rings to shifting light echoes from an ancient supernova, we’re witnessing cosmic evolution in real-time. Plus, we’re diving into the mystery of the "Little Red Dots", early galaxies that challenged our understanding until JWST uncovered the truth. Let’s break down the latest discoveries and what they mean for our understanding of the universe!
Sources & Further Reading:
Opening music: Space-DNA by KonstantinosP from Pixabay ⏳
Chapters:
0:00 – Intro
0:28 – Wolf-Rayet 140’s Expanding Dust Rings
2:28 – The Mystery of the Little Red Dots
5:06 – The Supernova That’s Still Glowing
7:44 – The Tiny Galaxy That Shouldn’t Exist
 
Anton Petrov has uploaded a video that mentions Dyson Spheres:


0:00 Dyson sphere updates!
0:50 How this was found originally
3:20 Previous announcements
4:02 Followups and analysis
5:05 Contaminated emissions and what this actually is
6:45 Hot dogs and what they are
8:55 Why they are probably not Dyson spheres anyway
10:35 Alternative explanations and conclusions
 
This is a video from Astrum uploaded late last year speculating that Alien isn't as far-fetched as one might think:


Astrum Investigates the Science of the Alien franchise, separating the fact from the fiction.
 
An interesting speculative video about what kind of alien multicellular life could evolve in extraterrestrial environments:


Scientists are uncovering bizarre exoplanets that challenge everything we know about habitability. From super-Earths with crushing gravity to tidally locked planets with scorching hot and frozen hemispheres, these extreme worlds could give rise to lifeforms unlike anything on Earth. In this video, we explore the scientific possibilities of extraterrestrial life—how gravity, atmosphere, and star types could shape truly alien evolution. Could we find snake-like creatures on high-gravity worlds, black-leaved plants around red dwarf stars, or ocean-dwelling bioluminescent life on Europa-like moons? The possibilities are endless, and the science is fascinating!
 
Euclid discovers a stunning Einstein ring

Euclid blasted off on its six-year mission to explore the dark Universe on 1 July 2023. Before the spacecraft could begin its survey, the team of scientists and engineers on Earth had to make sure everything was working properly. During this early testing phase, in September 2023, Euclid sent some images back to Earth. They were deliberately out of focus, but in one fuzzy image Euclid Archive Scientist Bruno Altieri saw a hint of a very special phenomenon and decided to take a closer look.

“I look at the data from Euclid as it comes in,” explains Bruno. “Even from that first observation, I could see it, but after Euclid made more observations of the area, we could see a perfect Einstein ring. For me, with a lifelong interest in gravitational lensing, that was amazing.”


Related paper:

 
NASA CubeSat Finds New Radiation Belts After May 2024 Solar Storm

The largest solar storm in two decades hit Earth in May 2024. For several days, wave after wave of high-energy charged particles from the Sun rocked the planet. Brilliant auroras engulfed the skies, and some GPS communications were temporarily disrupted.

With the help of a serendipitously resurrected small NASA satellite, scientists have discovered that this storm also created two new temporary belts of energetic particles encircling Earth. The findings are important to understanding how future solar storms could impact our technology.


Related paper:

 
NASA Scientists Spot Candidate for Speediest Exoplanet System
Astronomers may have discovered a scrawny star bolting through the middle of our galaxy with a planet in tow. If confirmed, the pair sets a new record for the fastest-moving exoplanet system, nearly double our solar system’s speed through the Milky Way.

The planetary system is thought to move at least 1.2 million miles per hour, or 540 kilometers per second.

“We think this is a so-called super-Neptune world orbiting a low-mass star at a distance that would lie between the orbits of Venus and Earth if it were in our solar system,” said Sean Terry, a postdoctoral researcher at the University of Maryland, College Park and NASA’s Goddard Space Flight Center in Greenbelt, Maryland. Since the star is so feeble, that’s well outside its habitable zone. “If so, it will be the first planet ever found orbiting a hypervelocity star.”

Related paper:

 
Scott Manley has uploaded a video about how the 2024YR4 asteroid could be intercepted if it turns out to be on a collision course with Earth:


I did the maths! We can do it, if we want to.
Asteroid effects demonstrated with Nukemap
https://nuclearsecrecy.com/nukemap/
 
Let's wait and see what JWST will discover before making predictions. I can remember that famous asteroid that was supposed to hit Earth a few years back but never did.
 

Ever noticed how the Moon seems HUGE when it’s near the horizon but smaller when it’s overhead? Trick of the eye or something more? Scientists have debated this for 2,000+ years, and we still don’t have a definitive answer! Find out what we do know and learn more about the Moon illusion: https://science.nasa.gov/solar-system...https://www.youtube.com/redirect?ev...the-moon-look-so-big-sometimes/&v=yuxWyIe8TIc
Link to download this video: coming soon
Scott Bednar, Pedro Cota, Jessica Wilde
Editor: James Lucas
Credit: NASA
 
NASA’s Webb Reveals the Ancient Surfaces of Trans-Neptunian Objects

Trans-Neptunian objects (TNOs) are icy bodies ranging in size from Pluto and Eris (dwarf planets with diameters of about 1,500 miles) down to tens of miles (Arrokoth) and even smaller. TNOs are on orbits comparable in size, or even much larger than, that of Neptune. The existence of TNOs was postulated by Kenneth Edgeworth, and later by Gerard Kuiper, in the 1950s; the region of space occupied by TNOs is usually referred to as the Kuiper Belt, and TNOs themselves, sometimes referred to as Kuiper Belt objects (KBOs).

The orbits of TNOs are extremely diverse but fall into groupings that reflect the outward migration of Uranus and Neptune early in the history of the formation of the solar system. As such, TNOs hold the keys to understanding that early history. However, it took NASA’s James Webb Space Telescope and its unparalleled ability to study the materials on the surfaces of TNOs to fully begin to grasp what they can tell us about our origins. Here Bryan Holler and John Stansberry from the Space Telescope Science Institute (STScI) in Baltimore describe how Webb is expanding our knowledge of these objects.

 
Related to the above.

Did LIGO just see its most important gravitational wave ever?

Which brings us to the present, or more accurately, to February 6, 2025. On that date, a gravitational wave event of high significance was detected: an event that definitely contains a neutron star and that either represents a neutron star-neutron star or neutron star-black hole merger, with a combined mass that’s on the relatively low end: no more than five solar masses and possibly as low (or lower than) three solar masses.



And then, only about an hour after that event was automatically reported, complete with sky-localization coordinates, the IceCube Collaboration issued a follow-up alert of their own. They searched for any possible neutrino signatures occurring within 1000 seconds (about 17 minutes) of the gravitational wave event, that were also consistent with the possible locations of the source from gravitational wave observations. A coincidence in space and in time would be very promising, especially considering the estimated distance to this event, from gravitational waves, is fairly large: at about ~1.1 ± 0.3 billion light-years.

Lo and behold, there were two candidates, one of which is an outstanding match: occurring less than five minutes after the gravitational wave event finished.



If there turns out to be an afterglow, or any type of remnant to observe at any wavelength of light, associated with the gravitational wave and neutrino signatures of the event that’s presently called S250206dm, this will mark the greatest gravitational wave detection in history: our first trifecta event in the history of multi-messenger astronomy. It’s worth keeping in mind, however, that the scientists working on this are being slow and careful, and are taking the time they need to get the science right and collect the full suite of relevant data. Only after there’s a completed analysis will we know for sure what happened during this event, and just what its cosmic implications are.

 
New research to be published in the Planetary Science Journal examines how much material from AC could reach our Solar System and how much might already be here. It’s titled “A Case Study of Interstellar Material Delivery: Alpha Centauri.” The authors are Cole Greg and Paul Wiegert from the Department of Physics and Astronomy and the Institute for Earth and Space Exploration at the University of Western Ontario, Canada.

“Interstellar material has been discovered in our Solar System, yet its origins and details of its transport are unknown,” the authors write. “Here we present Alpha Centauri as a case study of the delivery of interstellar material to our Solar System.” AC likely hosts planets and is moving toward us at a speed of 22 km s?1, or about 79,000 km per hour. In about 28,000 years it will reach its closest point and be about 200,000 astronomical units (AU) of the Sun. According to Greg and Wiegert, material ejected from AC can and will reach us, and some is already here.


Related paper:

 
This is what spooks me

DM 61 366 initially was also thought to make a close approach in about a million years time.
 
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The fly-by is measured in astronomical units now--closer with each update it seems.

Part of me wonders if it is a smaller, but closer object.

If it is a true star, anything orbiting it at a distance might make for a greater collision risk....it is already going be be close enough to where some of our system's objects will wind up in its Hill sphere--and vice versa perhaps.

Let's say Gliese 710 has several objects orbiting it. During closest approach...some of those could be farther out--or worse.... between it and our Sun. If the latter is true--then you must *subtract* it's distance from G 710's position during the fly-by...To date, this is as close to WHEN WORLDS COLLIDE as we can expect.

This coming fly-by may indeed perturb Oort--maybe Kuiper objects --but that will take time.

Now, Scholz's star passed by 70,000 years ago--which may mean that anything it nudged inward during closest approach may only now be headed inbound.

Down the road, WR-104 has us looking down the barrel.
 
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Mystery of 'remarkable' cosmic explosion that lay hidden for years

The "needle in the haystack" discovery of a powerful explosion from a mysterious unknown object outside our galaxy has excited astronomers.

It went unnoticed for years within a vast, two decade-long archive of observations by NASA's Chandra X-ray Observatory, before being unearthed by a new paper published in Monthly Notices of the Royal Astronomical Society.

Astronomers led by Stanford University and Harvard believe the "remarkable" cosmic explosion could either be the first X-ray burster ever discovered in the Large Magellanic Cloud (LMC), a rare flare from a magnetar – one of the most mysterious objects in the universe – or something entirely new and unheard of.


Related paper:

 
On Feb. 7, NASA increased the likelihood that asteroid 2024 YR4 will hit Earth in seven years time from 1.2% to 2.3%. The odds of impact then climbed to 2.6%, and are now at 3.1%, according to the latest data on NASA's Center for Near Earth Object Studies website.


NASA source link:

 
On Wednesday, a team of researchers announced that they got extremely lucky. The team is building a detector on the floor of the Mediterranean Sea that can identify those rare occasions when a neutrino happens to interact with the seawater nearby. And while the detector was only 10 percent of the size it will be on completion, it managed to pick up the most energetic neutrino ever detected.

For context, the most powerful particle accelerator on Earth, the Large Hadron Collider, accelerates protons to an energy of 7 Tera-electronVolts (TeV). The neutrino that was detected had an energy of at least 60 Peta-electronVolts, possibly hitting 230 PeV. That also blew away the previous records, which were in the neighborhood of 10 PeV.

Attempts to trace back the neutrino to a source make it clear that it originated outside our galaxy, although there are a number of candidate sources in the more distant Universe.


Related paper:

 
Anton Petrov has a video out updating the situation in regards to asteroid 2024YR4:


0:00 Updates about 2024 YR4 and the new risks
1:50 How scientists are studying this and the lack of data right now
2:40 New images and what we know
4:00 Properties discovered so far
5:05 What if it collides
6:00 Moon collision?
6:45 What is it made out of and what does it mean?
7:50 Conclusions and what's next?
 
PBS Space Time has put out a video about whether or not there will be another Big Bang:


How did the universe begin? How can something come from nothing? One way to “solve” this most difficult of philosophical conundrums is to avoid it altogether. Maybe the universe didn’t begin. Maybe the Big Bang was just one in an endless cycle.
 

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