TOP 10 PREHISTORIC OCEAN PREDATORS

yeswe_travel

Look how littel I am, next to this massive mountain..

Can you see the beauty around me ✨ .

DE)

Planet: Saturn

Saturn is losing its rings at an accelerated rate. Scientists estimate that the rings will be gone in 100 million years.

“Cassini's own discoveries were its demise.”

– Earl Maize, its project engineer @ JPL

current mood: emotional about a space probe

Cassini is the first spacecraft that was destroyed not from malfunction, or as a necessary end result of its mission… but out of love.

The probe was running out of propulsion fuel, but there’s no reason it couldn’t have been pushed into a stable orbit from where it could collect data and send back pictures for a long while yet.

Except it had detected that one of Saturn’s moons held liquid water and organic compounds: a world that might support life. A world that is, at the least, dreaming of life.

There is no orbit stable enough to be certain that the probe, carrying radioactive batteries and Earth’s bacteria, would never have come into contact with Enceladus. A delicate island of alien life could have been snuffed out or overrun. The sheep could have eaten the rose.

So instead - for the love of this fragile possibility, this potential that might yet never be realized - Cassini was brought into a final, intimate tango with Saturn.

But of course, all space probes are built for the sake of awe, which is nearly love. Science is rational, but scientists are driven to understand the universe just as the religious strive to know the face of God.

The Cassini probe was a 4 billion dollar machine for understanding Saturn. And yesterday, two decades after it launched from our planet, it was destroyed while sending us information about Saturn it never could have gathered from a distant, stable orbit: advancing its purpose, even though it would be consumed.

from Asimov’s ‘Nightfall’

Here’s a great explanation of language usage in sci-fi literature for all those who cannot keep their nit-picking to themselves:

Kalgash is an alien world and it is not our intention to have you think that it is identical to Earth, even though we depict its people as speaking a language that you can understand, and using terms that are familiar to you. Those words should be understood as mere equivalents of alien terms-that is, a conventional set of equivalents of the same sort that a writer of novels uses when he has foreign characters speaking with each other in their own language but nevertheless transcribes their words in the language of the reader. So when the people of Kalgash speak of “miles,” or “hands,” or “cars,” or “computers,” they mean their own units of distance, their own grasping-organs, their own ground-transportation devices, their own information-processing machines, etc. The computers used on Kalgash are not necessarily compatible with the ones used in New York or London or Stockholm, and the “mile” that we use in this book is not necessarily the American unit of 5,280 feet. But it seemed simpler and more desirable to use these familiar terms in describing events on this wholly alien world than it would have been to invent a long series of wholly Kalgashian terms.

In other words, we could have told you that one of our characters paused to strap on his quonglishes before setting out on a walk of seven vorks along the main gleebish of his native znoob, and everything might have seemed ever so much more thoroughly alien. But it would also have been ever so much more difficult to make sense out of what we were saying, and that did not seem useful. The essence of this story doesn’t lie in the quantity of bizarre terms we might have invented; it lies, rather, in the reaction of a group of people somewhat like ourselves, living on a world that is somewhat like ours in all but one highly significant detail, as they react to a challenging situation that is completely different from anything the people of Earth have ever had to deal with. Under the circumstances, it seemed to us better to tell you that someone put on his hiking boots before setting out on a seven-mile walk than to clutter the book with quonglishes, vorks, and gleebishes.

If you prefer, you can imagine that the text reads “vorks” wherever it says “miles,” “gliizbiiz” wherever it says “hours,” and “sleshtraps” where it says “eyes.” Or you can make up your own terms. Vorks or miles, it will make no difference when the Stars come out.

-I.A.

-R.S.

Shout out to all of my awake friends!

So I just discovered that the famous depth chart of Lake Baikal, you know, this one

Is

Uh

Not the whole picture

So this is going to haunt me forever

A giant #ammonite from millions of years ago. One of New Zealand’s largest fossils is on permanent display in Te Papa.

Ultra-Close Orbits of Saturn = Ultra-Cool Science

On Sept. 15, 2017, our Cassini spacecraft ended its epic exploration of Saturn with a planned dive into the planet’s atmosphere–sending back new science to the very last second. The spacecraft is gone, but the science continues!

New research emerging from the final orbits represents a huge leap forward in our understanding of the Saturn system – especially the mysterious, never-before-explored region between the planet and its rings. Some preconceived ideas are turning out to be wrong while new questions are being raised. How did they form? What holds them in place? What are they made of?

Six teams of researchers are publishing their work Oct. 5 in the journal Science, based on findings from Cassini’s Grand Finale. That’s when, as the spacecraft was running out of fuel, the mission team steered Cassini spectacularly close to Saturn in 22 orbits before deliberately vaporizing it in a final plunge into the atmosphere in September 2017.

Knowing Cassini’s days were numbered, its mission team went for gold. The spacecraft flew where it was never designed to fly. For the first time, it probed Saturn’s magnetized environment, flew through icy, rocky ring particles and sniffed the atmosphere in the 1,200-mile-wide (2,000-kilometer-wide) gap between the rings and the cloud tops. Not only did the engineering push the spacecraft to its limits, the new findings illustrate how powerful and agile the instruments were.

Many more Grand Finale science results are to come, but today’s highlights include:

Complex organic compounds embedded in water nanograins rain down from Saturn’s rings into its upper atmosphere. Scientists saw water and silicates, but they were surprised to see also methane, ammonia, carbon monoxide, nitrogen and carbon dioxide. The composition of organics is different from that found on moon Enceladus – and also different from those on moon Titan, meaning there are at least three distinct reservoirs of organic molecules in the Saturn system.

For the first time, Cassini saw up close how rings interact with the planet and observed inner-ring particles and gases falling directly into the atmosphere. Some particles take on electric charges and spiral along magnetic-field lines, falling into Saturn at higher latitudes – a phenomenon known as “ring rain.” But scientists were surprised to see that others are dragged quickly into Saturn at the equator. And it’s all falling out of the rings faster than scientists thought – as much as 10,000 kg of material per second.

Scientists were surprised to see what the material looks like in the gap between the rings and Saturn’s atmosphere. They knew that the particles throughout the rings ranged from large to small. They thought material in the gap would look the same. But the sampling showed mostly tiny, nanograin- and micron-sized particles, like smoke, telling us that some yet-unknown process is grinding up particles. What could it be? Future research into the final bits of data sent by Cassini may hold the answer.

Saturn and its rings are even more interconnected than scientists thought. Cassini revealed a previously unknown electric current system that connects the rings to the top of Saturn’s atmosphere.

Scientists discovered a new radiation belt around Saturn, close to the planet and composed of energetic particles. They found that while the belt actually intersects with the innermost ring, the ring is so tenuous that it doesn’t block the belt from forming.

Unlike every other planet with a magnetic field in our Solar System, Saturn’s magnetic field is almost completely aligned with its spin axis. Think of the planet and the magnetic field as completely separate things that are both spinning. Both have the same center point, but they each have their own axis about which they spin. But for Saturn the two axes are essentially the same – no other planet does that, and we did not think it was even possible for this to happen. This new data shows a magnetic-field tilt of less than 0.0095 degrees. (Earth’s magnetic field is tilted 11 degrees from its spin axis.) According to everything scientists know about how planetary magnetic fields are generated, Saturn should not have one. It’s a mystery physicists will be working to solve.

Cassini flew above Saturn’s magnetic poles, directly sampling regions where radio emissions are generated. The findings more than doubled the number of reported crossings of radio sources from the planet, one of the few non-terrestrial locations where scientists have been able to study a mechanism believed to operate throughout the universe. How are these signals generated? That’s still a mystery researchers are looking to uncover.

For the Cassini mission, the science rolling out from Grand Finale orbits confirms that the calculated risk of diving into the gap – skimming the upper atmosphere and skirting the edge of the inner rings – was worthwhile.

Almost everything going on in that region turned out to be a surprise, which was the importance of going there, to explore a place we’d never been before. And the expedition really paid off!

Analysis of Cassini data from the spacecraft’s instruments will be ongoing for years to come, helping to paint a clearer picture of Saturn.

To read the papers published in Science, visit: URL to papers

To learn more about the ground-breaking Cassini mission and its 13 years at Saturn, visit: https://www.nasa.gov/mission_pages/cassini/main/index.html

Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com.

Look at the bottom gif! The long tentacles are pushed out and parallel to each other while the jelly is motionless. This behavior is predatory, which means that the Marianas Trench Jelly is set in attack mode! 

Read more about the 2016 discovery of the Marianas Trench Jelly

From the invention of wireless to Radio Broadcast to Space

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 Édouard 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) 

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.  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.  

While there have been some dissenting voices who argue that ‘revealing’ 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 won’t 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.  

Image of the Arecibo Radio Telescope courtesy Marius Strom under a Creative Commons 3.0 share alike license.  

Image of the Arecibo Message of 1679 bits in the public domain.