Anonymous ID: 846c47 April 13, 2024, 7:01 a.m. No.20720312   🗄️.is 🔗kun

NASA Astronomy Picture of the Day

April 13, 2024

 

Palm Tree Partial Eclipse

 

Only those along the narrow track of the Moon's shadow on April 8 saw a total solar eclipse. But most of North America still saw a partial eclipse of the Sun. From Clearwater, Florida, USA this single snapshot captured multiple images of that more widely viewed celestial event without observing the Sun directly. In the shade of a palm tree, criss-crossing fronds are projecting recognizable eclipse images on the ground, pinhole camera style. In Clearwater the maximum eclipse phase was about 53 percent.

 

https://apod.nasa.gov/apod/astropix.html?

Anonymous ID: 846c47 April 13, 2024, 7:09 a.m. No.20720333   🗄️.is 🔗kun   >>0353

NASA Invites Media to Mars Sample Return Update

APR 12, 2024

 

NASA will host a media teleconference at 1 p.m. EDT, Monday, April 15, to discuss the agency’s response to a Mars Sample Return Independent Review Board report from September 2023, including next steps for the program.

 

The teleconference will livestream at:

 

https://www.nasa.gov/nasatv

 

Mars Sample Return has been a major long-term goal of international planetary exploration for the past two decades. NASA’s Perseverance rover is collecting compelling science samples that will help scientists understand the geological history of Mars, the evolution of its climate, and prepare for future human explorers. The return of the samples will also help NASA’s search for signs of ancient life.

 

The media teleconference will share the agency’s recommendations regarding a path forward for Mars Sample Return within a balanced overall science program. The speakers include:

 

NASA Administrator Bill Nelson

Nicky Fox, associate administrator, Science Mission Directorate

 

https://www.nasa.gov/news-release/nasa-invites-media-to-mars-sample-return-update/

Anonymous ID: 846c47 April 13, 2024, 7:20 a.m. No.20720374   🗄️.is 🔗kun   >>0650 >>0764

Hubble Spots a Galaxy Hidden in a Dark Cloud

APR 12, 2024

 

The subject of this image taken with the NASA/ESA Hubble Space Telescope is the spiral galaxy IC 4633, located 100 million light-years away from us in the constellation Apus. IC 4633 is a galaxy rich in star-forming activity and also hosts an active galactic nucleus at its core. From our point of view, the galaxy is tilted mostly towards us, giving astronomers a fairly good view of its billions of stars.

 

However, we can’t fully appreciate the features of this galaxy — at least in visible light — because it’s partially concealed by a stretch of dark dust (lower-right third of the image). This dark nebula is part of the Chamaeleon star-forming region, itself located only around 500 light-years from us, in a nearby part of our Milky Way galaxy. The dark clouds in the Chamaeleon region occupy a large area of the southern sky, covering their namesake constellation but also encroaching on nearby constellations, like Apus. The cloud is well-studied for its treasury of young stars, particularly the cloud Cha I, which both Hubble and the NASA/ESA/CSA James Webb Space Telescope have imaged.

 

The cloud overlapping IC 4633 lies east of the well-known Cha I, II, and III, and is also known as MW9 and the South Celestial Serpent. Classified as an integrated flux nebula (IFN) — a cloud of gas and dust in the Milky Way galaxy that’s not near to any single star and is only faintly lit by the total light of all the galaxy’s stars — this vast, narrow trail of faint gas that snakes over the southern celestial pole is much more subdued looking than its neighbors. Hubble has no problem making out the South Celestial Serpent, though this image captures only a tiny part of it.

 

https://science.nasa.gov/missions/hubble/hubble-spots-a-galaxy-hidden-in-a-dark-cloud/

Anonymous ID: 846c47 April 13, 2024, 7:50 a.m. No.20720438   🗄️.is 🔗kun   >>0650 >>0764

NASA’s New Hubble E-Book Spotlights Universe’s Best-Kept Dark Secrets

APR 06, 2024

 

NASA’s Hubble Space Telescope team has released a new downloadable e-book in the Hubble Focus series, called “Hubble Focus: The Dark Universe.” This e-book highlights the mission’s recent discoveries about two mysterious components of our universe, known as dark energy — an unexplained cosmic pressure that’s speeding up the universe’s expansion — and dark matter, an invisible substance detectable only by seeing how it gravitationally influences visible matter.

 

“This new e-book is a wonderful summary of all the work that Hubble, in cooperation with other observatories on the ground and in space, has put into improving our understanding of two of the biggest mysteries in astrophysics today: the true nature and origin of dark matter and dark energy,” said Ken Carpenter, Hubble’s operations project scientist. “Much remains to be done, but this book will give you a front row seat to what’s been happening in this quest!”

 

The trillions of stars, planets, galaxies, and other visible objects strewn throughout the cosmos represent less than 5 percent of what’s truly out there. Visible matter is like the tip of an iceberg, or the foam on top of a latte. All the rest of the universe, dark matter and dark energy, is mired in mystery.

 

Dark matter is a phantom in the machinery of the universe. Though it makes up the vast majority of the universe’s bulk, dark matter would evade even the best “ghost hunters” because it’s invisible, detectable only through its effects on normal matter. Its gravitational pull is the muscle of the cosmos, holding together both individual galaxies and galaxy clusters. Although scientists have long seen evidence of its existence, dark matter’s true nature remains one of the biggest mysteries in modern physics.

 

Hubble’s cosmic detective work offers clues by exploring the way matter, both normal and dark, is structured and distributed throughout space. Some of the mission’s observations have even tested theories about the type of particle that could make up dark matter. But Hubble’s observations haven’t always matched predictions, hinting that our theoretical models still have several missing pieces.

 

Shock waves of surprise rippled through the scientific community in 1998, when Hubble observations of supernovae in more distant galaxies helped show that the universe actually expanded more slowly in the past than it does today. That meant the expansion of the universe was not slowing down due to the attractive force of gravity, as many thought it should — it was speeding up.

 

Today, we still don’t know the exact cause of this mysterious acceleration, but theoretical cosmologists coined the term “dark energy” to describe it. Dark energy is so weak that gravity overpowers it on the scale of humans, planets, and even within the galaxy, which is why it was unobserved for so long.

 

Dark energy is present in the room with you as you read, even within your body, but gravity is much stronger at smaller scales, which is why you don't fly out of your seat. It is only on an intergalactic scale that dark energy becomes noticeable — and since it’s everywhere, it even overwhelms the dark matter! Hubble has helped gather very precise measurements of the universe's expansion rate, but its findings underscore a nagging discrepancy. The universe is expanding faster now than was expected from its trajectory seen shortly after the big bang, and no one yet knows why.

 

The perplexity surrounding dark energy and dark matter indicates that for all we’ve learned about the universe, we still don’t know much about its underpinnings. Studying these mysteries opens the door to discovering exciting new physics.

 

“Hubble’s incredible scientific power continues to drive modern astronomy,” said Jennifer Wiseman, Hubble’s senior project scientist. “Dark matter and dark energy were not in mind when Hubble was first designed, and yet by detecting the impacts of these unseen cosmic phenomena, the Hubble Space Telescope is once again transforming our understanding of the universe.”

 

Scientists will expand upon Hubble’s insights about dark matter and dark energy with complementary observations from the European Space Agency’s Euclid mission, which has NASA contributions; NASA’s upcoming Nancy Grace Roman Space Telescope, and variety of other space and ground-based telescopes. We have far more left to learn among the stars.

 

https://science.nasa.gov/missions/hubble/nasas-new-hubble-e-book-spotlights-universes-best-kept-dark-secrets/

https://science.nasa.gov/mission/hubble/multimedia/e-books.

Anonymous ID: 846c47 April 13, 2024, 8 a.m. No.20720458   🗄️.is 🔗kun

Unraveling The Mysteries Of The Brightest Gamma-Ray Burst: A Supernova Without Heavy Elements

April 12, 2024

 

In October 2022, astronomers observed the brightest gamma-ray burst (GRB) ever recorded, GRB 221009A, also known as the “Brightest of All Time” (B.O.A.T.). This powerful explosion occurred about 2.4 billion light-years away from Earth, lasting just a few hundred seconds.

 

Confirming the Supernova Connection

A Northwestern-led team has now confirmed that the B.O.A.T. was caused by the collapse and explosion of a massive star, a phenomenon called a supernova. Using the James Webb Space Telescope (JWST), the researchers were able to observe the supernova’s signature in the aftermath of the GRB.

 

A “Normal” Supernova

Surprisingly, the supernova associated with the record-breaking GRB was not exceptionally bright. “It looks fairly normal in the context of other supernovae associated with less energetic GRBs,” said lead author Peter Blanchard. “You might expect that the same collapsing star producing a very energetic and bright GRB would also produce a very energetic and bright supernova. But it turns out that’s not the case.”

 

The Missing Heavy Elements

The researchers then searched for evidence of heavy elements, such as platinum and gold, within the supernova. However, they did not find the telltale signatures of these elements. This suggests that extremely energetic GRBs like the B.O.A.T. may not be a significant source of heavy elements in the universe.

 

Solving One Mystery, Raising Another

“When we confirmed that the GRB was generated by the collapse of a massive star, that gave us the opportunity to test a hypothesis for how some of the heaviest elements in the universe are formed,” Blanchard said. “We did not see signatures of these heavy elements, suggesting that extremely energetic GRBs like the B.O.A.T. do not produce these elements.”

 

The Bright Afterglow and the Mysterious Jets

To better understand the B.O.A.T., the researchers combined data from the JWST and the Atacama Large Millimeter/Submillimeter Array (ALMA) in Chile. They found that the bright afterglow of the GRB was still contributing a significant amount of light, even months later. This suggests that the shape and structure of the jets launched by the collapsing star may be responsible for the record-breaking brightness of the B.O.A.T.

 

Clues from the Host Galaxy

The researchers also obtained a spectrum of the galaxy hosting the B.O.A.T., finding that it has the lowest metallicity, or abundance of heavy elements, of all previous GRB host galaxies. This unique aspect of the host galaxy may help explain the properties of the B.O.A.T.

 

Continuing the Search for Answers

While the discovery of the supernova associated with the B.O.A.T. solves one mystery, it raises another. The lack of heavy element signatures in the supernova is a crucial piece of information as scientists continue to investigate the origins of the heaviest elements in the universe. Future observations with the JWST and other powerful telescopes will be crucial in unraveling the remaining secrets of this exceptional cosmic event.

 

https://scienceblog.com/543678/unraveling-the-mysteries-of-the-brightest-gamma-ray-burst-a-supernova-without-heavy-elements/

Anonymous ID: 846c47 April 13, 2024, 8:21 a.m. No.20720542   🗄️.is 🔗kun   >>0650 >>0764

SpaceX Starlink Mission

 

On Friday, April 12 at 9:40 p.m. ET, Falcon 9 launched 23 Starlink satellites to low-Earth orbit from Space Launch Complex 40 (SLC-40) at Cape Canaveral Space Force Station in Florida.

 

This was the 20th flight for the first stage booster supporting this mission, which previously launched GPS III Space Vehicle 04, GPS III Space Vehicle 05, Inspiration4, Ax-1, Nilesat 301, OneWeb Launch 17, ARABSAT BADR-8, and now 13 Starlink missions.

 

https://www.spacex.com/launches/mission/?missionId=sl-6-49