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.583 as a fraction
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What is .583 as a fraction?
To write .583 as a fraction you have to write .583 as numerator and put 1 as the denominator. Now you multiply numerator and denominator by 10 as long as you get in numerator the whole number..583 = .583/1 = 5.83/10 = 58.3/100 = 583/1000
And finally we have: .583 as a fraction equals 583/1000
0.583 as a fraction – Get Easy Solution – What is 0.583 as a fraction? To write 0.583 as a fraction you have to write 0.583 as numerator and put 1 as the denominator. Now you multiply numerator and denominator by 10 as long as you get in numerator the whole number. 0.583 = 0.583/1 = 5.83/10 = 58.3/100 = 583/1000583 / 1000 is already in the simplest form. It can be written as 0.583 in decimal form (rounded to 6 decimal places). Steps to simplifying fractions. Find the GCD (or HCF) of numerator and denominator GCD of 583 and 1000 is 1; Divide both the numerator and denominator by the GCD 583 ÷ 1 / 1000 ÷ 1; Reduced fraction: 583 / 1000 Therefore, 583/1000 simplified to lowest terms is 583/1000.Here we will show you step-by-step how to convert 9.583 so you can write it as a fraction. You can take any number, such as 9.583, and write a 1 as the denominator to make it a fraction and keep the same value, like this: 9.583 / 1
583/1000 simplified, Reduce 583/1000 to its simplest form – A fraction has a numerator and denominator and is expressed as follows: numerator/denominator. So when you are asking "What is 583 as a fraction?" you are asking "How can I express 583 as numerator/denominator?" To do this, simply set the numerator to 583 and the denominator to 1. Doing this, we find that 583 as a fraction is 583/1. Answer: 583Here we will show you step-by-step how to convert 5.583 so you can write it as a fraction. You can take any number, such as 5.583, and write a 1 as the denominator to make it a fraction and keep the same value, like this: 5.583 / 1You can take any number, such as 2.583, and write a 1 as the denominator to make it a fraction and keep the same value, like this: 2.583 / 1 To get rid of the decimal point in the numerator, we count the numbers after the decimal in 2.583, and multiply the numerator and denominator by 10 if it is 1 number, 100 if it is 2 numbers, 1000 if it is
What is 9.583 as a fraction? – To write .583333 as a fraction you have to write .583333 as numerator and put 1 as the denominator. Now you multiply numerator and denominator by 10 as long as you get in numerator the whole number. .583333 = .583333/1 = 5.83333/10 = 58.3333/100 = 583.333/1000 = 5833.33/10000 = 58333.3/100000 = 583333/10000004.583 as a fraction. Convert from decimal to fraction. Convert 4.583 to Fraction. Here you can find a decimal to fraction chart and also write any decimal number as a fraction. Decimal to Fration Calculator / Converter. Terminating Repeating. Enter a decimal or interger value: Ex.: 0.5, 0.625, 1.75, etc.To write 4/583 as a fraction you have to get to the number where there is a numerator and a denominator written in whole numbers. 4/583 has already a numerator and denominator so it is a fraction already. And finally we have: 4/583 as a fraction equals 4/583. You can always share this solution.
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How fast are you moving when sitting still? – So, you are sitting there comfortably on your armchair while watching your favorite TV show.
Just sitting still and doing nothing… Just relaxing and enjoying your beautiful life… Just sitting still, not moving at all… *sigh* But are you so sure you are not moving at all? I mean, have you ever considered that when you are sitting or standing still you are actually moving? And pretty fast, by the way Yeah! I'm sure you are asking now: how come? Well, any answer will be incomplete unless you know first what's actually the meaning of speed. Speed is equal to the distance traveled over the time taken to travel that distance. For example. When your car is moving at 50 miles per hour it means you cover a distance of 50 miles per each hour you are traveling. So, if you move at that same speed for 3 hours you will cover a total distance of 150 miles. In most countries however, they measure speed in kilometers per hour. So the same example goes like this: If a car is moving at 80 kilometers per hour it means you cover a distance of 80 km per each hour you are traveling. So, if you move at a constant speed for 3 hours you will cover a total distance of 240 kms. However in science we don't measure speed using neither miles nor kilometers, or even hours, but we use meters and seconds. One kilometer is equivalent to 1000 meters, since the kilo prefix means a thousand. This prefix is derived from the Greek word χίλιοι which means "thousand". One hour, on the other hand is equivalent to 3,600 seconds. But to make things easier in this video I'll use both miles and kilometers per hour. But that's not all, another key aspect about how fast things are moving is that you must also ask: "compared to what are they moving?" Without a frame of reference, questions about speed cannot be answered completely. For example, when you measure the speed of a car, a train, a plane or even yourself walking or running the frame of reference is the ground, that means the Earth. If we say a car is moving at a speed of 50 miles per hour (that's 80 kilometers per hour) We compare its speed relative to the ground. So the frame of reference is the ground. That's the Earth. So when you think you are sitting still in your armchair that's because the frame of reference you use is the Earth. So, you are not moving relative to the Earth, or the ground. But remember, our planet actually is moving, and pretty fast by the way. Now, we'll change our frame of reference in order to find out how fast you are actually moving when sitting still comfortably in your armchair. So first, let's use the Earth axis as a frame of reference And let's ask: "How fast does our planet rotate?", or: "How fast are we spinning?" Which is the same. The earth rotates once every 23 hours, 56 minutes and 4.09053 seconds (23.93 hours) around its own axis. But wait a second Isn’t a day 24 hours? Astronomers calculate a day in two ways. So, they use two different frames of reference. If we take as a frame of reference the background stars located far away, the amount of time it takes for the Earth to complete one full rotation on its own axis is 23 hours, 56 minutes and 4.09053 seconds. Astronomers call this a "sidereal day." However if we use the Sun as a frame of reference our planet makes a complete rotation around its axis in 24 hours with respect to the Sun. So let's see why we rotate in 23 hours, 56 minutes and 4 seconds instead of exactly 24 hours as we use to think. For example, on day 1 the Sun and a certain distant star are both overhead. Then, on day 2, the planet has rotated 360° and the distant star is overhead again but the Sun is not. We need another 3 minutes and 56 seconds to see the Sun overhead. That happens because the Earth doesn't only rotate on its axis but it also obits the Sun. And as we move in our orbital plane, the position of the Sun changes. So we need another 3 minutes and 56 seconds for the Sun to return to the same spot in the sky. Since the Earth is orbiting the Sun we actually need an extra 3 minutes and 56 seconds each day to return the Sun to the same spot in the sky. Astronomers call this a solar day and is the one we use in the Gregorian calendar. However, the Earth has already completed a 360º degree turn 3 minutes and 56 seconds ago. So, to get the actual time it takes our planet to make a full 360º turn we use the distant stars as a frame of reference instead of the Sun. So now that you know the amount of time the Earth requires to complete one full rotation on its axis Let's see how fast does it rotate. Any place on Earth makes a full 360º rotation in 23 hours, 56 minutes and 4 seconds (86,164.090 seconds) so all the places in our planet have the same angular speed. However the speed depends on what latitude you are located at. That's because, the circumference of the Earth at the Equator is the largest with 24,906 miles (or 40,075 km) And as you travel to higher latitudes, the circumference becomes smaller. Since speed is equal to the distance traveled over the time taken to travel that distance and since all the places on Earth have the same angular speed regardless of their latitudes they all complete a full rotation in the same amount of time However due to the difference in size of their circumferences they travel different distances in the same amount of time. So, those places located closer to the Equator travel longer distances and those located in higher latitudes travel shorter distances. While a person positioned at the Equator travels 24,906 miles (40,075 km) in 23 hours, 56 minutes and 4 seconds another at the North Pole needs the same amount of time to spin in place. So if you divide the circumference of the Equator by the length of the day we get a speed at the equator of about 1,040 mph (1,674 km/h). That's about a 60% faster than the average commercial plane. The speed decreases as you move north or south from the Equator but it’s still a good clip throughout North America and Europe. If we move halfway up the globe to 45 degrees in latitude (either north or south) the rotational speed at 45 degrees is around 733 mph (1,180 km/h). That speed decreases more as you go farther north or south. By the time you get to the North or South poles your spin becomes very slow and it takes an entire day to spin in place. But that's not all. In addition to spinning on its axis, the Earth also revolves around the Sun. We are approximately 93 million miles (150 million km) from the Sun and at that distance, it takes us 365 days, 5 hours, 48 minutes and 45 seconds to complete a full orbit around the Sun. The full path of the Earth’s orbit is close to 600 million miles (970 million km). So, if you think you don't travel much enough, think it twice, because you travel 600 million miles or 970 million km around the Sun each year! That's almost the same distance from the Earth to Jupiter. But listen the following numbers. If we divide that distance by the length of the year we get an orbital speed of about 66,616 mph (107,208 km/h) That's 18,51 mi/s (29.78 km/s). At that speed, you could circumnavigate the Earth's equator in just 22.4 minutes and cover the distance to the Moon in 4 hours! That's over three times the speed of the ISS (International Space Station) and 2.5 times the max speed of the Apollo 11! But there is more. Our Sun is just one star among several hundred billion others that together make up the Milky Way Galaxy. Our galaxy, our bigger home. All those stars that make up the Milky Way are also moving, and among them our Sun. Since any planet orbiting a star will share its motion through the Galaxy with it that means the Earth and the entire Solar System are also in motion orbiting the center of the Milky Way. The Milky Way is so big that it is around 100,000 light-years across. That means that something travelling at the speed of light (the speed limit of the Universe) needs 100,000 years to cross the whole galaxy. Our Solar System is about halfway out from the center of the galaxy that's about 25,000 light years. So the speed at which the Solar System moves around the center of the Milky Way is an astounding 483,000 miles per hour (792,000 km/hr). So we are orbiting the center of the Milky Way at a speed of 140 miles per second or 225 km/s. At that speed, an object could circumnavigate the Earth's equator in just 2 minutes and 58 seconds. But the Milky Way is so vast that even at this great speed our Solar System requires about 225 million years to make one complete orbit around the center of the galaxy. This is called a “galactic year” Since the Sun and the Earth first formed about 4.6 billion years ago, about 20 galactic years have passed; that means we have been around the Galaxy just 20 times. Our planet is just 20 galactic years old. And by the way, we live in the same galactic year of dinosaurs. But the universe is filled with billions of galaxies. And they are not sitting still. All of them are moving too And that includes our galaxy, the Milky Way. For the different speeds of our planet mentioned so far, we always used different frames of reference. In your armchair, your speed compared to the walls of your house is zero compared to the Earth axis is over 700 mph (1,126 km/h) compared to the Sun is 66,616 mph (107,208 km/h) and compared to the center of the galaxy it is 483,000 miles per hour (792,000 km/hr). But Compared to what are we measuring the motion of our galaxy, as all the other galaxies are moving too? To answer this question you have to think about the Big Bang and the expansion of the Universe. Since the Big Bang about 13.7 billion years ago, when the Universe was born it has been expanding. And when the universe expands, it is space itself that is stretching. Well, actually space and time, since they are the same thing, but I'll leave that for another video. The whole universe is filled with microwaves and other radio waves. They fill all of space, and as the universe is expanding, these microwaves and radio waves are expanding with it. So they always fill the universe. These waves are known as the cosmic background radiation and as they fill the whole universe, they are everywhere all around you. So that's the frame of reference we use to compare the motion of the Milky Way as well as of the other galaxies. The galaxies in the universe are moving apart because space stretches and creates more distance between them. So, going back to our question about how fast is the Milky Way, (and accordingly all of us), moving through the intergalactic space? Well it turns out to be a blazing 1.3 million miles per hour (2.1 million km/hr)! Which is equivalent to 361 miles/sec (583 km/s). At that speed you could travel from New York City to Chicago in just 2 seconds! Or from New York City to London in 9 seconds! At that speed you can circumnavigate the Earth's equator in 68 seconds! However as fast as this number sounds it is just a little fraction compared to the speed of light, equivalent to 0.19% the light-speed. Thus, each year we travel 11,388,000,000 miles, or 18,323,292,000 km. Our galaxy belongs to a cluster of nearby galaxies called the Local Group comprising about 80 galaxies. Our galaxy together with the rest of the galaxies of the Local Group, are moving toward the Virgo Cluster an enormous group of over 1,300 galaxies located some 59 million light-years away in the direction on the sky that is defined by the constellations of Leo and Virgo. The reasons for this motion are not fully understood Some people think there is a huge concentration of matter in this direction and they call it The Great Attractor. This Great Attractor, has a mass 100 quadrillion times greater than our Sun and a span of 500 million light-years across. And is probably made of both visible matter that we can see along with dark matter that we cannot see. If you ask why we don't feel all this movement that's because these speeds are constant. It means these speeds stay the same all the time so we do not feel any acceleration or deceleration. You can only feel motion if your speed changes. For example, if you are in a car which is moving at a constant speed, you will not feel much motion. However, when the car accelerates or when it slows down, you feel the motion. Another example is that of an airplane flying. When the plane is traveling at a constant speed and constant altitude you can go on and walk down the aisle, but you can't feel the movement of the plane. The reason is simple: you, the plane, and everything else inside is traveling at the same speed. In order to feel the movement, the plane must change its speed or altitude. So the same happens with the Earth, the Solar System and the Galaxy. For example, if the Earth were to change speed, we'd certainly feel that, and it wouldn't be pleasant at all like a sudden acceleration or like applying the brakes at a planetary scale while the atmosphere would keep moving at the same speed and wipe the surface of the planet. Fortunately for us, nothing like that happens and we are moving a blazing 1.3 million miles per hour (2.1 million km/hr) and we don't feel it. So the next time someone asks you why are you sitting there all they long watching TV You can answer: "Although it may look as if I'm just sitting still, I'm actually moving at a great speed through the universe". So, thank you for watching this video and if you liked it and it was useful please subscribe to my channel of Science and Exploration. Good bye folks! .