Enceladus got life?

Flying Through the Plume on Saturn's Moon Enceladus ...
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Thanks NASA’s Cassini mission, scientists have been able to confirm that underneath the icy crust of one of Saturn’s moons, Enceladus, lies a global ocean. Naturally, that begs the question could there possibly be something living in that ocean. When looking for life in our solar system, the first thing we look for is water (H2O). That is the most important element that has to be present and if we find it, we know we are on the right track.

Now when it comes to Enceladus, not only did we find some water, we essentially found an entire planet full of it. But even though water is a great place to start, it doesn’t guarantee life, especially after you consider that Enceladus is so far away from the sun that sunlight doesn’t reach it making photosynthesis impossible, and there is also no oxygen on Saturn’s moon. After factoring all of that, the whole life on Enceladus thing isn’t looking too good. But what if we can find examples of life thriving is the most exotic and desolate parts of Earth? That’s where there’s hope.

Scientists have discovered microbes in parts of our planet where sunlight doesn’t reach, and oxygen isn’t present because photosynthesis can’t take place. Sound familiar? There are three ecosystem here on Earth that could be the basis for life on Saturn’s moon—two of them are based on methanogens, that belongs to an ancient bacterial group related to the “rugged survivalists” archaea. These are found in volcanic rocks along the Colombian river as well as in Idaho Falls, so they are real! These microbes pull their energy form the chemical interactions of different rocks, while the microbes in third ecosystem located deep within a South African mine, gets energy from radioactive decay in rocks. This is how we know life is feasible on Enceladus, but how would life start.

This is the trickier question to answer because we don’t even know exactly how life started on Earth. But what we do have our theories of how life originated on Earth and we can see which of those theories are applicable to Enchiladas. There are currently two theories that meet this criteria, the Primordial Soup theory and the Deep Sea Vent theory. But there are still more pieces of to this puzzle that we need to have a definitive answer, including analyzing the organic compounds in the plumes released by Enceladus’ aquifers and figuring out what is the energy source powering its aquifers. It looks like we are really close to the answer, and even if we find that life most likely isn’t present on Enceladus, that journey to that answer was definitely a fun one.

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Becoming One with Saturn

Cassini prepares to graze Saturn's rings - SpaceFlight Insider
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On September 17, 2017, NASA’s Cassini’s spacecraft exhausted its fuel supply. This marked the end of a 20 yearlong space exploration and 13 yearlong orbit around The planet Saturn.

The Cassini Mission was monumental in more ways than one. It was the first spacecraft to orbit Saturn, first to land in the outer solar system, and first to sample and extraterrestrial ocean. Because of Cassini, we discovered how Earth-like the moon Titan is and encouraged us to explore it further giving us insight to our own planet. Its long mission let us observer seasonal and weather changes on other planets, its close orbit to Saturn shed light on the complexities of Saturn’s rings.

At the end of its life, Cassini had travelled a total of 4.9 billion miles, captured 645 GB of data along with 453,048 images, and thanks to it, we discovered 6 additional moons.

What the Cassini mission did for science as a whole is endless. To attempt to list them all would be doing a disservice so here is the website dedicated entirely to the Cassini mission as a a beautiful short film about its journey.

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The Cleanest Place on Earth

NASA's MMS Team Assembles Final Observatory | NASA
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While working with or assembling new instruments or components used for space travel , NASA engineers and scientists must make their way to the clean room where they will give satellites and spacecrafts a final inspection before they can be launched into space. As the name suggests this room has to be free of any particles or dust that could disrupt the the sensitive equipment being used or contaminate the spacecraft itself. Clean rooms were first built in 1961 to support to support NASA’s Ranger and Mariner mission to the Moon, Venus, and Mars.

Now, I’m going put you in the shoes a NASA engineer on their way to the clean room. Close your eyes and imag… wait…no don’t close your eyes, you’re reading.

You’re standing in front of a door. You open it and walk in to see the floor covered in with white sticky matts and a shoe cleaner out of the corner of your eye. You stick one foot at a time in the shoe vacuum as it takes 5 seconds to a preliminary dirt removing. Next you start walking on the matts, feeling like someone spilled honey all over the floor, to get rid of even more outside gunk that your shoes are carrying. Congratulations! you made it passed the first set of “lobbies” on your way to the clean room. You have a couple more.

Now you’re standing in front of a phone-booth sized glass box. This is where you will take a quick shower. The walls inside the glass box are lined with jets that starts to blast you with air, “washing” away any debris left in your hair, skin, and clothing. You then notice a green light glowing indicating that you shower is done, allowing you to enter the last station.

You are surrounded by lockers and benches preparing yourself for the most painstaking step of the process. You spend the next 15 minute meticulously dressing yourself in a white, full body, sterile hazmat-like suit, glove, head covering, boots, and facemask. This is the end of the tunnel, so you don’t want to negate all the cleaning you gone through by rushing this process.

Now you’re all dressed and after giving yourself a pat on the back, you open the door to the clean room where you continue to be a part of history.

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The Iron Catastrophe

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Many believe that under the Earth’s crust, deep within the center of our planet, lies a molten core of iron and nickel responsible for heating up the earth’s and being the source for the lava that flows form our volcanoes. This is an understandable misconception as the temperature of the core of the earth rivals that of the surface of the sun. It’s hard to imagine anything not melting on the sun! Well I’m here to tell you that this is exactly what is happening with the Earth’s core.

YES! the Earth’s core is solid metal ball of iron and nickel.

But there is a story to why our metal core is able to remain solid with temperatures beyond the boiling point of any metal. It all starts 500 million years into the Earth’s lifespan with an event called “The Iron Catastrophe.” Back when the earth was forming, all of the heat and radioactivity from various material colliding and smashing into each other increased. The resulting collisions made the infant Earth so hot that all of the materials melted creating a squishy and gooey sphere. When earth was in this liquid state, due to gravity, all of the iron and nickel began to contract and compact towards the center of the planet where it began to cool.

But this still doesn’t explain why it remains solid despite being around 6,000 degrees Celsius. Well that’s because the pressure at the core of the Earth is so great that it essentially raises the melting point of the iron-nickel core beyond hat it normally should be.

As a result of the Iron Catastrophe, Earth’s magnetosphere formed creating a protective layer that reduces the harm of solar radiation and solar wind here on the surface of the earth.

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What Exactly is a Supernova?

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To put it simply, supernovas are explosions of stars. They are the largest explosions that occur in our universe.

There are actually two ways that supernovas can occur. The first way happens at the end of a star’s lifetime. Stars are able to get their energy through nuclear fusion, which is when two atoms combine to form a new atom. When this energy runs out, there are two different outcomes depending on the mass of the star. The mass that separates these two outcomes is called the Chandrasekhar limit. If the mass of the star is below this limit, the star becomes a white dwarf. If it is above, the core of the star collapses onto itself and releases an extremely large amount of energy, forming either a neutron star or a black hole. Although the majority of this energy is released through invisible particles called neutrinos, the rest of the energy shoots out the outer areas of the star, producing a supernova. The second way only occurs in binary star systems when a white dwarf explodes. When two stars orbit the same point, they are described as binary stars. If the two stars collide or one star takes too much matter from the other, the star can explode and form a supernova.

Stars are mostly composed of hydrogen and helium, but nuclear fusion is able to produce much heavier elements. Supernovas then help distribute these elements from the stars’ cores to the rest of the universe, giving us the life we have today!

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Commercial Space Travel?

Space X Crew Dragon Capsule (Source)

Have you ever thought about traveling to space? While we’re far from intergalactical travel and settlements on other planets, space tourism and commercial space flights are closer to reality than ever before. A year ago, humans were able to access space through a non-government funded space vehicle for the first time in history under Space X, a private corporation with its main goal being affordable space settlement. The Space X Crew Dragon capsule was able to bring two NASA astronauts safely back to Earth from the International Space Station (ISS). Before this feat, the Russian Space Agency was the only company that had offered orbital space flights to the public, with a record of bringing seven tourists to space in the early 2000s before ceasing operations around a decade ago. Now, a few companies have built a solid foundation and are aiming to make the once far-away dream of public space flights a reality. Two private corporations, Virgin Galactic and Blue Origin, have set their eyes on commercial suborbital space flights. These flights travel at speeds slower than those required of orbital flights, but still provide its passengers a few minutes of weightlessness. Space X, most likely the leading corporation in private space exploration, have set its eyes on settling Mars and the Moon, but have also already sold seats on future Crew Dragon flights to wealthy customers. Lastly, an aerospace company named Boeing is right behind Space X in ferrying astronauts to the ISS, and is possibly looking at the ability to fly private passengers into space at a rate of $35,000 per night. While affordable commercial space flights are still not a thing, drastic development have taken place in recent years. With these corporations leading the future of space tourism, who knows? You might soon be able to view the stars and planets from Space!

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Voyager Mission

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You may have heard of the twin Voyager spacecraft as the two longest-flying spacecraft ever and the only mission to travel to all four outer planets. However, the original purpose of the Voyager mission was to only study Jupiter and Saturn. The two spacecraft were launched over forty years ago in late 1977. Their launch date was timed perfectly to occur during a special alignment of the four outer planets that only happens every 175 years. During this time, they conducted a series of flybys where the spacecraft flew close enough to the planets to use gravity assist but without being captured. By utilizing the planets’ gravity, the spacecraft were able to “slingshot” from one planet to the next. In fact, Voyager 2’s flight time to Neptune decreased from 30 years to only 12 years!

Voyager 1

As of now, Voyager 1 has traveled the farthest out of any spacecraft. During its time observing Jupiter, it discovered a thin ring as well as Thebe and Metis, two new Jovian moons. One of the most interesting discoveries they encountered on Jupiter was that Io, one of Jupiter’s moons, has active volcanoes. It also discovered a new ring on Saturn and five new moons.

Voyager 2

Voyager 2 was the first ever spacecraft to make it past Uranus and is the only one to study all four giants at such a close distance. Its other major discoveries include finding a new moon on Jupiter, ten new moons on Uranus, and five new moons on Neptune. It also found two new rings on Uranus and four new rings on Neptune along with a “Great Dark Spot.”

In August 2012, Voyager 1 became the first spacecraft to enter interstellar space, which is the part of space where the Sun stops having an effect on its surroundings. Voyager 2 later followed in November of 2018. To this day, the Voyager spacecraft are still collecting and sending back data even from over 23 billion kilometers away.

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Blog 3 Falling into Jupiter


What Would You See If You Fell Into Jupiter

Once I got to know about the names of gaseous giants in the outer part of our solar system, I became extremely curious about what the world would look like under their thick atmosphere. The video I shared in this blog provides a perfect fulfillment to my desire of knowing the biggest planet in our solar system: Jupiter. This video vividly simulates the visual feedback during which a person penetrates the atmosphere of Jupiter. As we can discover, the inner Jupiter contains a devastating environment from the perspective of human beings. However, I have to admit that the inner world of Jupiter is not as fascinating as I expected. Although Jupiter is more than 1300 times larger than Earth, the internal environment is relatively simple. In this vast sphere, we cannot see diverse components. Most we can experience if we fell into Jupiter is just endless clouds, winds, increasing pressure and temperatures. Overall, the world of Jupiter reminds me how special the environment of Earth is in the universe.

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Flying by Worlds

Voyager 1 Aircraft (Source)

So how exactly are we able to know so much about the features, terrains, and even atmosphere of the planets and moons of our solar system? Well, one of the main tools used by scientists to explore planets are flybys. In general, flybys are when a spacecraft travel closely past a world for observation and continue on its path. Unlike lander, probes, rovers, or sample return missions, flybys are generally cheaper to fund not only because they are less expensive to launch but also because they can visit multiple planets rather than just one. For example, the Voyager missions, which are probably two of the most famous flybys, observed various worlds beyond their mission scope before exiting our Solar System. Launched just months apart in the summer of 1977, the Voyager aircrafts were created with the goal of exploring Jupiter, Saturn, their rings, and their moons. Nevertheless, the two flybys would go on to explore all Jovian planets, almost 50 of their moons, as well as the rings and magnetic field of the gas giants. Flybys also carry an assortment of tools such as telescopes, cameras, and spectrographs in order to capture the various features of planets during their short period near it. Through the path of flybys and their instruments, we were able to observe many qualities and characteristics of our solar system that would have been close to impossible to observe from Earth; some of these being the ability to capture the highest resolution images of our worlds and the rings of the outer planets from a different view. Flybys are an integral part of our space exploration and will continue to be for years to come.

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Mercury’s Shrinkage

It’s been long thought that of the Fab (Terrestrial) Five, only Earth remains geologically active. However, recent evidence shows that little Mercury, long thought to be tectonically dead, is actually shrinking!

The evidence comes in the form of small troughs (upper arrows in the picture below) and scarps (lower arrows) astronomers were able to photograph on the rocky world’s surface.

Small graben, or narrow linear troughs, have been found associated with small scarps on Mercury
Credits: NASA/JHUAPL/Carnegie Institution of Washington/Smithsonian Institution

But how do scientists know that these markings make for evidence that Mercury is shrinking? Well, they’ve also found similar geological features on the Moon, who also happens to be a metaphorical “twin” of Mercury’s, that show its own shrinkage.

Why are these worlds shrinking though? As the planet cools (yes, cooling! Even despite Mercury being the closest world to the Sun), its interior is condensing, almost as if the planet is crumpling up on itself. That’s why we see these sharp ridges and mountains emerge.

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