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Category - Space Place

Space Place

SPACE PLACE – FEBRUARY 2020

The Sun: More Than An Average Star There is one object in space that is more important to us on Earth than anything else in the universe. It is a bright star that lies at the very center of our solar system. at star is our sun. It is a huge ball of super hot gas, made up mainly of hydrogen and helium. e sun is by far the largest object in our solar system. e Earth orbits around our sun, and so do all the other planets, dwarf planets, moons, asteroids, and comets in our solar system. The sun is really just an average star, like trillions of other stars in the universe. But to us, it looks so big and so bright! How can it be like the tiny points of light that we see in the night sky? It appears so much larger and brighter than other stars because it is much closer to us than any other star. So how close is the sun? The sun is around 93 million miles (150 million km) from Earth. That is so far that it would take about 163 years to get to the sun if you traveled at a speed of 65 miles per hour (104 km per hour)— the speed of a car on the freeway. That at might seem incredibly far away. However, the next closest star to us is about 270,000 times farther away than this! For the sun to appear so bright and feel so warm to us from such a distance, it must be very big and very hot. e sun is actually so big that 109 Earths could t across it, and 1,300,000 Earths could t inside it. The sun has around 333,000 times as much mass as the Earth and contains 99.86 percent of all the mass in the entire solar system. The sun is also incredibly hot, with a surface temperature of about 10,000 degrees Fahrenheit (5,500 degrees Celsius). The temperature at the center of the sun is even higher, where it reaches 27 million degrees Fahrenheit (15 million degrees Celsius). The extremely high temperatures and pressures in the core of the sun force hydrogen atoms to smash together and form helium. Every second, 600 million tons of hydrogen are converted into helium. This creates an enormous amount of energy. is energy powers the sun and creates its light and heat. The heat from the sun powers our weather and keeps us warm. Its light is used by plants to provide food for life on Earth. Plants also use energy from the sun to create the oxygen we breathe. Without the sun, Earth would be a dark and frozen planet where no life could exist. So, the sun may be just an average star, but for us, it is the most important star of all! To learn more about how our sun compares to other stars, visit: The NASA Space Place

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Space Place

SPACE PLACE | MARCH 2018

Sixty Years of Observing Our Earth Satellites are a part of our everyday life. We use global positioning system (GPS) satellites to help us find directions. Satellite television and telephones bring us entertainment, and they connect people all over the world. Weather satellites help us create forecasts, and if there’s a disaster — such as a hurricane or a large fire — they can help track what’s happening. Then, communication satellites can help us warn people in harm’s way. There are many different types of satellites. Some are smaller than a shoebox, while others are bigger than a school bus. In all, there are more than 1,000 satellites orbiting Earth. With that many always around, it can be easy to take them for granted. However, we haven’t always had these helpful eyes in the sky. The United States launched its first satellite on Jan. 31, 1958. It was called Explorer 1, and it weighed in at only about 30 pounds. This little satellite carried America’s first scientific instruments into space: temperature sensors, a microphone, radiation detectors and more. Explorer 1 sent back data for four months, but remained in orbit for more than 10 years. This small, relatively simple satellite kicked off the American space age. Now, just 60 years later, we depend on satellites every day. Through these satellites, scientists have learned all sorts of things about our planet. For example, we can now use satellites to measure the height of the land and sea with instruments called altimeters. Altimeters bounce a microwave or laser pulse off Earth and measure how long it takes to come back. Since the speed of light is known very accurately, scientists can use that measurement to calculate the height of a mountain, for example, or the changing levels of Earth’s seas. Satellites also help us to study Earth’s atmosphere. The atmosphere is made up of layers of gases that surround Earth. Before satellites, we had very little information about these layers. However, with satellites’ view from space, NASA scientists can study how the atmosphere’s layers interact with light. This tells us which gases are in the air and how much of each gas can be found in the atmosphere. Satellites also help us learn about the clouds and small particles in the atmosphere, too. When there’s an earthquake, we can use radar in satellites to figure out how much Earth has moved during a quake. In fact, satellites allow NASA scientists to observe all kinds of changes in Earth over months, years or even decades. Satellites have also allowed us—for the first time in civilization—to have pictures of our home planet from space. Earth is big, so to take a picture of the whole thing, you need to be far away. Apollo 17 astronauts took the first photo of the whole Earth in 1972. Today, we’re able to capture new pictures of our planet many times every day. Many satellites are buzzing around Earth, and each one plays an important part in how we understand our planet and live life here. These satellite explorers are possible because of what we learned from our first voyage into space with Explorer 1 — and the decades of hard work and scientific advances since then. To learn more about satellites, including where they go when they die, check out NASA Space Place: spaceplace.nasa.gov

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Space Place

NASA Space Place

There are many places on Earth where it snows, but did you know it snows on other worlds, too? Here are just a few of the places where you might find snow beyond Earth: Mars The north pole and south pole of Mars have ice caps that grow and shrink with the seasons. These ice caps are made mainly of water ice – the same kind of ice you’d find on Earth. However, the snow that falls there is made of carbon dioxide – the same ingredient used to make dry ice here on Earth. Carbon dioxide is in the Martian atmosphere and it freezes and falls to the surface of the planet as snow. In 2020, NASA’s Mars Reconnaissance Orbiter took photos of the sand dunes around Mars’ north pole. The slopes of these dunes were covered with carbon dioxide snow and ice. There are dozens of moons that orbit Jupiter and one of them, called Io, has snowflakes made out of sulfur. In 2001, NASA’s Galileo spacecraft detected these sulfur snowflakes just above Io’s south pole. The sulfur shoots into space from a volcano on Io’s surface. In space, the sulfur quickly freezes to form snowflakes that fall back down to the surface. A Moon of Saturn: Enceladus Saturn’s moon, Enceladus, has geysers that shoot water vapor out into space. There, it freezes and falls back to the surface as snow. Some of the ice also escapes Enceladus to become part of Saturn’s rings. The water vapor comes from a heated ocean, which lies beneath the moon’s icy surface. (Jupiter’s moon Europa is also an icy world with a liquid ocean below the frozen surface.) All of this ice and snow make Enceladus one of the brightest objects in our solar system.

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Space Place

Studying Storms On Earth

You’ve probably seen some scary storms with very fast winds. But did you know that over the oceans, spinning storms can create even faster winds? ese storms are called tropical cyclones. Depending on where they happen in the world, these storms also go by other names, like hurricanes (in the North Atlantic Ocean) and typhoons (in the Western North Paci c Ocean). In order to study these storms, NASA created the Cyclone Global Navigation Satellite System, or CYGNSS. When the tropical cyclones spin, there is an area in the center called the “eye.” e eye of the storm has less wind and rain than other parts of the storm. What happens on the ocean’s surface in the eye may tell scientists what the storm will do next. However, the eye is surrounded on all sides by high-speed winds. is area is called the eye-wall. If a person were to go to the eye-wall to study the ocean’s surface, it could be very dangerous. But satellites can safely study what happens in the eye and eye- wall of an ocean storm. CYGNSS is launching in November and has eight satellites that will orbit Earth. ey will look at the ocean surface, and measure how fast the wind is going. Although other satellites can measure wind strength, sometimes rain from inside the tropical cyclone can make their measurements less accurate. However, the CYGNSS satellites will be able to accurately measure the strength of the wind, even in rainy weather. When there is a storm, the CYGNSS satellites will be able to watch it get stronger or weaker. ey can see what is happening in the eye and eye-wall of the storm from space. Scientists will use information from CYGNSS to learn more about how storms form. It may help them predict where a storm is going. e satellites may also help us know if a storm is going to get worse. When tropical cyclones move toward land, they can be very dangerous for people who live in the path of the storm. If we know when a hurricane or typhoon will happen, where it will go, and how strong it will be, we can keep people safe. CYGNSS may help us do that. is is just one way NASA is helping us here on Earth, as well as exploring the stars. Want to learn more about how hurricanes form? Visit the NASA Space Place for more information: Hurricanes. Artist’s concept of one of the eight Cyclone Global Navigation Satellite System satellites deployed in space above a hurricane. Image credit: NASA

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Kids

The Amazing Universe – December 2016

Hubble Space Telescope image of a small part of the universe filled with galaxies. It would take around 25 million pictures like this to cover the whole sky – space is really big! Image credit: NASA, ESA, H. Teplitz and M. Rafelski (IPAC/ Caltech), A. Koekemoer (STScI), R. Windhorst (Arizona State University), and Z. Levay (STScI) “The cosmos is all that is, or ever was, or ever will be.” is is how astronomer Carl Sagan described the universe. Cosmos is another word for universe. e universe is made up of everything we know of. Earth, the sun, and the moon are part of the universe. In fact, so are all of the planets, stars and galaxies. All of space, time, energy and matter exist inside the universe. e universe is so big that we cannot even see it all, and never will! But where did the universe come from? Scientists who study the universe are called astronomers. Astronomers discovered evidence that the universe was created in an enormous expansion beginning about 13.8 billion years ago called the Big Bang. At that moment, all of the matter and energy in the universe was created. Time and space were also created in the Big Bang. At the time of the Big Bang, everything in the universe was squeezed together in an incredibly hot and compressed state. e heat and pressure caused the universe to expand at extremely high speeds, which created space. As the universe expanded and cooled, stars, planets and galaxies formed out of the matter present at the Big Bang. Today, the universe contains billions of galaxies, each of which contain millions or billions of stars, and possibly millions or billions of planets and moons. But all of the things that we can see in the universe — such as planets, stars and galaxies — make up only about 5 percent of what is in the universe. Most of the universe is made up of mysterious forms of matter and energy that we cannot see. These forms of matter and energy are called dark matter and dark energy. We do not yet understand what dark energy and dark matter are. However, experiments show that they exist. Dark matter is thought to make up about 27 percent of the universe, while about 68 percent of the universe is thought to be dark energy. Dark matter clumps together similar to the way galaxies do. Dark energy is thought to ll all of space, maybe the same everywhere, but maybe different at different places and times. So as you can see, the universe is a huge, amazing place with many exciting mysteries to solve and discoveries to be made! If you want to learn more about the Big Bang, visit the NASA Space Place: http://spaceplace.nasa. gov/big-bang/en/

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Space Place

Earth’s Magnetic Shield

Thousands of miles beneath our feet, flowing electrons create a powerful force that protects life on Earth. This effect is called a magnetic field. But what creates this magnetic field? Deep, deep below the ground lies center of the Earth, also called its core. It is a place of incredibly high temperatures and pressures. Earth’s core is made up mostly of metals, like iron and nickel. When metals are very hot, their atoms move so fast that they can no longer stay solid and they melt into liquid. Although the inner part of the core is very hot, the metals there cannot melt. This is because the pressure there is too high from the weight of the rest of the Earth above it. The high pressure makes it difficult for these metal atoms to move around. But in the outer part of the core, the pressure is lower and the metals there can melt. The molten metal in the outer core flows in high speed currents as the Earth spins. Within this molten metal are electric charges. These flowing electric charges create a strong magnetic field. In fact, Earth’s magnetic field is so powerful that it reaches out into space and surrounds the entire Earth! Earth’s magnetic field is very important because it protects us from harmful radiation from space. It also shields us from the solar wind—a stream of high speed particles that flows from the sun. These particles travel at speeds of about one million miles per hour! Thankfully, most of these particles bounce off Earth’s magnetic field and pass around the Earth. If Earth had no magnetic field, these particles would erode away our atmosphere. This actually happened on our neighbor planet, Mars. When the magnetic field surrounding Mars was weakened, most of its atmosphere was stripped away by the solar wind. Sometimes particles from the solar wind get trapped in Earth’s magnetic field. When too many particles get trapped, some overflow into our atmosphere near Earth’s magnetic poles. Here they collide with atoms and molecules in the atmosphere, creating beautiful displays of lights called auroras. Although our magnetic field can’t block every particle from space, the ones that slip through make for an awesome show! To learn more about auroras, visit the NASA Space Place: http://spaceplace.nasa.gov/aurora/en/

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Space Place

Communicating With Curiousity

With cell phones and the Internet, we’re used to communicating with anyone, anywhere, quickly and easily. But how do scientists communicate with things that aren’t on our planet — such as the Curiosity Rover on Mars? This communication beyond Earth is a bit more complicated. We communicate with spacecraft using radio signals. Radio signals move at the speed of light. However, they have a long way to travel. Even when it is closest to Earth, Mars is still about 35 million miles away. And sometimes it’s much, much farther! If you sent a text message to Mars, it would take, on average, about 14 minutes for it to get there. This long distance makes talking with robots on other planets difficult. Imagine driving in a video game and waiting 28 minutes to see your car make a turn! It would take forever to drive the rover one turn at a time. Instead, we send Curiosity all the instructions for the day at once. Most of the rover’s daily tasks —l ike taking photographs and zapping rocks — are planned out in advance. Some days we can’t directly talk to the rovers. We use antennas to send and receive signals, but Mars and Earth are both constantly spinning. On Earth, the antennas are located around the world so that at least one is always facing Mars. About half of the time, though, Curiosity’s location on Mars is not facing toward Earth. During these times, Curiosity can’t send signals directly to our antennas. So how does the rover send its messages to Earth? Through an orbiter! Orbiters are special spacecraft that spend their time continuously traveling around an object, such as a moon or a planet. There are several orbiters traveling around Mars. When Curiosity isn’t facing Earth, it can send a message to one of these orbiters. Then, once the orbiter reaches the Earth-facing side of Mars, it sends the signal. Each day, Curiosity sends information to at least one Mars orbiter, and the orbiter sends that information to Earth. Hurray for teamwork! Learn more about Curiosity here: http://spaceplace.nasa.gov/mars-curiosity/en/

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Space Place

What’s in Space?

When you look up at the night sky, you see stars and sometimes the moon and the brighter planets. Away from city lights, on a clear night, you might see the beautiful band of the Milky Way stretching across the sky. Is there anything else up there in space? There are many beautiful, strange and mysterious objects in space. We are lucky that we now have large telescopes to help us see far into space. With telescopes, we can get a much better view of the planets and moons in our solar system. By using special telescopes, scientists can get a better view of our sun. We can see that the sun is not smooth and we can see many features on the sun’s surface.Never look at the sun with your eyes or through a telescope. The sun’s intense light can damage your eyes. Looking farther away, we can see other stars. Some are like our sun, while others are much larger or smaller. Stars come in different colors. We do not see the colors of the stars when we look up into the night sky because they are too dim. But telescopes can collect more light and can show us the colors of the stars. Telescopes show us the giant clouds of gas and dust where stars are born. Stars form when parts of these clouds collapse and get hot enough to make their own light. Our own solar system started in one of these clouds. There are many of these clouds in space. When a star runs out of fuel, part or all of the star expands into space. Some of the stars shed their outer layers while the largest stars explode. The material from these stars help form new clouds where new stars will form. Stars, planets and clouds of gas are collected into galaxies where they are held together by gravity. Galaxies are huge, and can have billions of stars in them. We live in a large galaxy called the Milky Way. As we look even farther into space we see more and more galaxies. There are billions of galaxies in space, each holding billions of stars. The universe is a very big place to explore and many of its secrets are yet to be discovered! To learn more about galaxies—including our very own Milky Way—visit: http://spaceplace.nasa.gov/galaxy

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Space Place

Studying the sun is a gas!

If someone asked you to draw the sun, would you make a little yellow circle with lines coming out of it? That’s fun, but what does the sun look like up close? We can see the shapes and outlines of craters and mountains on the moon, but what about the sun? Does it have rocks and dust and hills and valleys? Good question. The sun has been a mystery for thousands of years. In the first place, no human being has ever been to the sun. It’s way too hot for anyone to go near it — even a million miles away would be too close. Also, we didn’t even have telescopes until around 1608. But once they started looking through them, astronomers realized that a lot was happening on our star. Dark spots appeared, moved around and disappeared. And during solar eclipses, astronomers saw that the sun had a big, active atmosphere. Since the space age started, our understanding of what the sun is made of and why it is so dynamic keeps growing. Using powerful space telescopes, scientists have been able to see more details than ever, details that can’t be seen from the ground. In fact, NASA currently has four different missions dedicated to watching the sun. The sun definitely isn’t made of rocks or dust. Or lava. Or even fire. We now believe that the sun is made up of very hot gases called plasma. Why is that important? Well, plasma carries electric currents and magnetic fields as it moves around. That means that the sun is like one giant magnet! We see the surface and atmosphere of the sun moving because magnetism on the sun is constantly changing. Yes, when it comes to the sun, this is a time of exciting discovery. It won’t be long before the star at the center of our solar system is ready for her close-up! We’ve got a whole section of the NASA Space Place website devoted to the sun! Check out http://spaceplace.nasa.gov/menu/sun/

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Kids

Ceres: One Big Rock

Dawn is when the sun rises and a new day begins. You might start thinking about breakfast, too! But Dawn is also the name of an amazing spaceship. NASA named this spacecra Dawn because its purpose is to help understand the beginning of the solar system. You know there are eight planets, right? But there are many other objects in our solar system. ere are moons and asteroids and sometimes a comet! We also share the solar system with dwarf planets. ey’re called dwarf, but they are still pretty huge! One of the ve dwarf planets that we know about is named Ceres (sounds like ‘series’). It’s the biggest object between Mars and Jupiter. Ceres lives in the main asteroid belt. at’s where millions of rocky objects called asteroids hang out and orbit the sun. No one had ever been to Ceres, so NASA had the idea to go and check it out. at idea became the Dawn spacecra — making it the very rst spacecra to visit a dwarf planet. The NASA engineers finished building Dawn in 2007 and launched her into space from Cape Canaveral in Florida. From there, Dawn started flying through space toward Ceres. Ceres is very, very far away—much farther than Mars. Dawn was able to get there thanks to her super-efficient engines. Threy don’t use gasoline or even rocket fuel, they use xenon ions! By going to Ceres in 2015 and studying it for a long time (over a year now), we hope that Dawn will teach us something about the history of our solar system. Then we might learn more about the dawn of Earth, where we live!   The dwarf planet Ceres as seen from the Dawn spacecraft. The bright area is the inside of a large crater.

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