A rendered view of the night sky from a planet in a globular cluster. Source: Reddit
neohumanity
Grand Prismatic Spring: The most beautiful and dangerous hot spring in the world. Filmed from a helicopter đ Â Shot on
@lexarmemory
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The night palatteÂ
Leedsichthys is a giant member of the Pachycormidae, an extinct group of Mesozoic bony fish, that lived in the oceans of the Middle Jurassic period. Â The first remains of Leedsichthys were identified in the nineteenth century. Â Leedsichthys fossils have been found in England, France, Germany and Chile. Along with its close pachycormid relatives Bonnerichthys and Rhinconichthys, Leedsichthys is part of a lineage of large-sized filter-feeders who swam the Mesozoic seas for over 100 million years, from the middle Jurassic until the end of the Cretaceous period. Pachycormids might represent an early branch of Teleostei, the group most modern bony fishes belong to; in that case Leedsichthys is the largest known teleost fish.
 Leedsichthys fossils have been difficult to interpret, because the skeletons were not completely made of bone. Large parts consisted of cartilage that did not fossilise. On several occasions the enigmatic large partial remains have been mistaken for stegosaurian dinosaur bones. As the vertebrae are among the parts that have not been preserved, it is hard to determine the total body length. Estimates have varied wildly. At the beginning of the twentieth century a length of nine metres was seen as plausible, but by its end Leedsichthys was sometimes claimed to have been over thirty metres long. Recent research has lowered this to about sixteen meters for the largest individuals. Skull bones have been found indicating that Leedsichthys had a large head with bosses on the skull roof. Fossilised bony finrays show large elongated pectoral fins and a tall vertical tail fin. The gill arches were lined by gill rakers, equipped by a unique system of delicate bone plates, that filtered plankton from the sea water, the main food source.
I really wish people would jump on the marine exploration bandwagon as much as space exploration.
Black holes are some of the most bizarre and fascinating objects in the cosmos. Astronomers want to study lots of them, but thereâs one big problem â black holes are invisible! Since they donât emit any light, itâs pretty tough to find them lurking in the inky void of space. Fortunately there are a few different ways we can âseeâ black holes indirectly by watching how they affect their surroundings.
If youâve spent some time stargazing, you know what a calm, peaceful place our universe can be. But did you know that a monster is hiding right in the heart of our Milky Way galaxy? Astronomers noticed stars zipping superfast around something we canât see at the center of the galaxy, about 10 million miles per hour! The stars must be circling a supermassive black hole. No other object would have strong enough gravity to keep them from flying off into space.
Two astrophysicists won half of the Nobel Prize in Physics last year for revealing this dark secret. The black hole is truly monstrous, weighing about four million times as much as our Sun! And it seems our home galaxy is no exception â our Hubble Space Telescope has revealed that the hubs of most galaxies contain supermassive black holes.
Technology has advanced enough that weâve been able to spot one of these supermassive black holes in a nearby galaxy. In 2019, astronomers took the first-ever picture of a black hole in a galaxy called M87, which is about 55 million light-years away. They used an international network of radio telescopes called the Event Horizon Telescope.
In the image, we can see some light from hot gas surrounding a dark shape. While we still canât see the black hole itself, we can see the âshadowâ it casts on the bright backdrop.
Black holes can come in a smaller variety, too. When a massive star runs out of the fuel it uses to shine, it collapses in on itself. These lightweight or âstellar-massâ black holes are only about 5-20 times as massive as the Sun. Theyâre scattered throughout the galaxy in the same places where we find stars, since thatâs how they began their lives. Some of them started out with a companion star, and so far thatâs been our best clue to find them.
Some black holes steal material from their companion star. As the material falls onto the black hole, it gets superhot and lights up in X-rays. The first confirmed black hole astronomers discovered, called Cygnus X-1, was found this way.
If a star comes too close to a supermassive black hole, the effect is even more dramatic! Instead of just siphoning material from the star like a smaller black hole would do, a supermassive black hole will completely tear the star apart into a stream of gas. This is called a tidal disruption event.
But what if two companion stars both turn into black holes? They may eventually collide with each other to form a larger black hole, sending ripples through space-time â the fabric of the cosmos!
These ripples, called gravitational waves, travel across space at the speed of light. The waves that reach us are extremely weak because space-time is really stiff.
Three scientists received the 2017 Nobel Prize in Physics for using LIGO to observe gravitational waves that were sent out from colliding stellar-mass black holes. Though gravitational waves are hard to detect, they offer a way to find black holes without having to see any light.
Weâre teaming up with the European Space Agency for a mission called LISA, which stands for Laser Interferometer Space Antenna. When it launches in the 2030s, it will detect gravitational waves from merging supermassive black holes â a likely sign of colliding galaxies!
So we have a few ways to find black holes by seeing stuff thatâs close to them. But astronomers think there could be 100 million black holes roaming the galaxy solo. Fortunately, our Nancy Grace Roman Space Telescope will provide a way to âseeâ these isolated black holes, too.
Roman will find solitary black holes when they pass in front of more distant stars from our vantage point. The black holeâs gravity will warp the starlight in ways that reveal its presence. In some cases we can figure out a black holeâs mass and distance this way, and even estimate how fast itâs moving through the galaxy.
For more about black holes, check out these Tumblr posts!
â« Gobble Up These Black (Hole) Friday Deals!
â« Hubbleâs 5 Weirdest Black Hole Discoveries
Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com.
The word radio was coined in 1907 after a decade of furious activity to discover the mechanism for wireless transmission.  A decade earlier, French physicist Ădouard Branly coined the term radioconductor to describe a means of wireless transmission.  He based his term on the verb radiate which ultimately came from the Latin word radius meaning the spoke of a wheel, a ray or beam of light.  The word radio was first used by itself in a 1907 article by Lee De Forest. It was used five years later by the Navy to distinguish it from other wireless technologies and entered common usage in the next decade.  Radio technology advanced so quickly that a little over 50 years later on November 16, 1974, scientists broadcast the first interstellar radio message out to the stars, a program that later became known as METI, the Message to Extra-terrestrial Intelligence. To date, only 9 messages have been transmitted by a variety of organizations:
{The Morse Message (1962)}
Arecibo message (1974)
Cosmic Call 1 (1999)
Teen Age Message (2001)
Cosmic Call 2 (2003)
Across the Universe (2008)
A Message From Earth (2008)
Hello From Earth (2009)
RuBisCo Stars (2009)
Wow! Reply (2012)Â
The first radio message, known as the Morse Message, does not technically belong on this list as the Russians directed the message to Venus, and thus the primary mission was not Interstellar. Â The message targets vary in distance from the very short (the majority of targets are under 100 light years away) to the very far, including the Arecibo Message, which targets the M13 globular cluster 24,000 light years away. Â
While there have been some dissenting voices who argue that ârevealingâ our location to enemy or hostile alien civilizations is ill-advised at best, most scientific consensus agrees that due to the physical restrictions on speed and travel (as currently understood) we are in no danger of imminent attack.  While the Arecibo Message wonât reach its target for another 25,000 years or so, the first of the other messages should arrive by 2029.  Other scientist point out that our current terrestrial radio and television broadcasts represent their own METI signal and thus we have no need to fund additional broad- or narrow-cast messages. Â
Image of the Arecibo Radio Telescope courtesy Marius Strom under a Creative Commons 3.0 share alike license. Â
Image of the Arecibo Message of 1679 bits in the public domain. Â
New research into the minds of crows has revealed a jaw-dropping finding: the canny corvids arenât just clever - they also possess a form of consciousness, able to be consciously aware of the world around them in the present. In other words, they have subjective experiences.
This is called primary, or sensory, consciousness, and it had only previously been demonstrated in primates - which means we now may have to rethink our understanding of how consciousness arises, in addition to reconsidering the avian brain.
âThe results of our study opens up a new way of looking at the evolution of awareness and its neurobiological constraints,â said animal physiologist Andreas Nieder of the University of TĂŒbingen.
Continue Reading.
Okay, the title of The Atlanticâs article might be a little click-bait-y. But the discovery is truly remarkable. A new bone has been analyzed from the already-famous cave in Russia, and it belonged to, per DNA analysis, the daughter of a Neanderthal mother and a Denisovan father. Â
Amateur astronomer, owns a telescope. This is a side blog to satiate my science-y cravings! I haven't yet mustered the courage to put up my personal astro-stuff here. Main blog : @an-abyss-called-life
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