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CrazyGames is a browser game platform that features the best free online games. All of our games run in the browser and can be played instantly without downloads or installs. You can play on CrazyGames on any device, including laptops, smartphones, and tablets. This means that whether you are at home, at school, or at work, it's easy and quick to start playing! Every month over 15 million people play our games, either by themselves in single player mode, with a friend in two player mode, or with people from all over the world in multiplayer mode.

Our Games

We feature over 7000 games in all genres that you can imagine. Our most popular games are:

The most popular game titles are Bullet Force, Krunker, Shell Shockers, Moto X3M, UNO, Minecraft Classic, Surviv.io and Doge Miner 2. Everyone has their own favorite games though, so start exploring and discover your favorites.

About CrazyGames

CrazyGames was founded in 2013 and has been providing free online games since then. Our goal is to provide the best possible gaming experience in the browser. The site is owned and operated by Maxflow BV, a Belgium-based company. You can reach out, check our open job positions, or take a look at our game developer platform. For more information about CrazyGames, you can visit our corporate site.

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Crazy Games - Free Online Games on CrazyGames.com

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CrazyGames is a browser game platform that features the best free online games. All of our games run in the browser and can be played instantly without downloads or installs. You can play on CrazyGames on any device, including laptops, smartphones, and tablets.

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I use this app to write stories. I hope you like it.

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Picturebook - Bear & Bear Make a Story (iPad / iPhone / iPod touch)

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Plz watch this video from Sakina thank you

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Plz watch this video from Sakina thank you

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Plz watch it   :)

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Chrome Music Lab

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How were these built?

All our experiments are all built with freely accessible web technology such as Web Audio API, WebMIDI, Tone.js, and more. These tools make it easier for coders to build new interactive music experiences. You can get the open-source code to lots of these experiments here on Github.

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All our experiments are all built with freely accessible web technology such as Web Audio API, WebMIDI, Tone.js, and more. These tools make it easier for coders to build new interactive music experiences. You can get the open-source code to lots of these experiments here on Github.

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Try playing an online chess game against a top chess computer. You can set the level from 1 to 10, from easy to grandmaster. If you get stuck, use a hint or take back the move. When you are ready to play games with human players, register for a free Chess.com account!

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247 Backgammon offers the best backgammon game online. Play with an artificially intellegent opponent or play with a friend with Pass & Play! 247 Backgammon has games in five difficulites, ranging from easy to expert! You'll be sure to find a difficulty you feel comfortable playing, whether you are a beginner or seasoned backgammon player. Options only on 247 Backgammon include doubling cube, highlights, match points, and chip color! This backgammon site even remembers your preferences every time you come back so you'll be set to play immediately! The gameplay on 247 Backgammon is seamless and you'll quickly become addicted to the beautiful artwork and perfect puzzle game.

Backgammon is a popular ancient board game. It is played with two players (lucky you, we have a computer player to enjoy!). The object of backgammon is to move all your checkers around the board in a clockwise motion and ultimately bear off the checkers from the board. The first player to remove all their checkers is the winner.

Alternate turns with your opponent moving checkers toward your home in the upper right hand quadrant of the backgammon board. Move checkers by rolling the dice. The numbers on the dice refer to how many spaces you may move with one or more checkers. Highlights show you where the checkers can possibly move. If you roll doubles, you get to move each die twice, concluding in four moves for that turn. You may move your checkers onto any Point so long as it is occupied by your checkers, is empty, or has 1 opponent checker. You may not move your checkers onto a Point with two or more opponent checkers. If you land on a Point with one opponent checker, you knock the opponent's checker off the board and send it back to the beginning. The opponent must now roll and move into an empty spot in your home territory to get that checker back into gameplay. They may not move any other checkers until that knocked off checker is returned. Beware though! Leaving your checkers open with only one on a point leaves them open to be knocked off by your opponent as well!

Once you move all your checkers into the upper right quadrant (in the single player backgammon game), you may start bearing off. This means you can place your checkers into the slot on the right, removing them from the board. Whoever manages to do this first wins!

One to three points can be awarded during the backgammon game dependant on where the loser's checkers are on the board when the winner wins. If the losing player has not borne off any of their checkers by the time the winner has won, the winner will achieve 2 points, and is known as losing a gammon. If the losing player has not borne off any of their checkers and has checkers in the opponent's home board (lower right quadrant) or are still knocked off, the winner scores three points, which is known as losing a backgammon. The winner is awarded one point (most common) if the opponent has started to bear off their checkers and/or has all of their checkers out of the winner's home territory.

The doubling cube is a fun option for players who are seasoned backgammon aficionados. Turn this option on or off in the menu at the start of the game. It is a marker, instead of a die. At any time during gameplay a player may before his/her turn propose the game be played for twice the current stake (beginning at 2). The opponent must either accept th doubled stake or resign to defeat immediately (thus ending the game). The option to redouble belongs exclusively to the player who accepted the double. Technically, the game can be doubled up to 64 times the score, but it rarely goes beyond 4. If the "double" is declined, the doubler wins however many points the doubling cube is showing (1 x doubling cube). If the game is played, the resulting score will then be multiplied by the doubling cube number. This little die adds a lot of fun strategy to the game. We recommend trying it on for size!

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247 Backgammon offers the best backgammon game online. Play with an artificially intellegent opponent or play with a friend with Pass & Play! 247 Backgammon has games in five difficulites, ranging from easy to expert! You'll be sure to find a difficulty you feel comfortable playing, whether you are a beginner or seasoned backgammon player.

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The Big Bang

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Sizes of Antares and Sun

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How do natural disasters start?

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This is a great website for kid-friendly videos on lots of different topics! I hope you like it.

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The Kid Should See This: Educational videos for curious kids of all ages, a free resource for parents & teachers. Science, art, nature, animals, & more.

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"Every time a comet goes around the sun some of that ice vaporizes in our star’s terrible heat to form a tail that lights up like the dust that rises from a dusty road."

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Space enthusiast Seán Doran downloaded 550 long-exposure photos taken from the International Space Station and compiled them into a real-time video. The result: Comet NEOWISE from ISS [ 4K ]. You can see the comet rise at around 3 minutes.

C/2020 F3 won't pass Earth again for another 6,800 years, so if you're in the Northern Hemisphere, the comet should now be visible near the northeastern horizon just after sunset. It will appear higher in the sky throughout the month, passing closest to Earth on July 22nd. From How To Share Comet NEOWISE With Your Kids:

Use the maps provided to help you find comet NEOWISE. If you're bringing young children ask them later to make a drawing of what they saw with crayons or colored pencils. What a nice keepsake that would make. Talk to them about comets. People used to be afraid comets were portents of disaster. Now that we know what they are - small asteroid-like objects but made of dirty ice instead of rock - we can appreciate them for their beauty. Every time a comet goes around the sun some of that ice vaporizes in our star's terrible heat to form a tail that lights up like the dust that rises from a dusty road. And it's currently shining from over 80 million miles (129 million km) away. What a big place the solar system is with room for one star, at least eight planets and billions of comets and asteroids!

And from Astronomy Picture of the Day:

Comet NEOWISE was discovered on March 27, 2020 by a space telescope called NEOWISE, the Near-Earth Object Wide-field Infrared Survey Explorer. According to CalTech's NEOWISE Project:

The spacecraft was launched in December 2009 and was originally named the Wide-Field Infrared Survey Explorer (WISE). WISE was not designed to study asteroids and comets and is now long past its expected lifetime of 7 months.

Watch this next: Space Rocks: Comets, asteroids, meteors, and meteorites.

Also: What is a comet made of? Dara Ó Briain's Science Club demonstrates.

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Comet NEOWISE from ISS, a calming real-time view | The Kid Should See This

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Space enthusiast Seán Doran downloaded 550 long-exposure photos taken from the International Space Station and compiled them into a real-time video. The result: Comet NEOWISE from ISS [ 4K ]. You can see the comet rise at around 3 minutes.

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I learned something new that I wanted to share with you all.

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Let's Explore Space! | Astronomy for Kids

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Best Learning Space Videos for Kids, Solar System for Kids and Teach Kids Planets and Science

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How do we fight corona virus when it's not in the air ?

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How should we stop corona?

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This is for our unit.

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How do satellites not  feel the earths gravity and go into earth 🌍

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Why is corona virus here 😭😭😭😭

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why do they move?

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How fast do planets spin?

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We know the Earth spins on its axis once every 24 hours. Well, every 23 hours, 56 minutes and 4 seconds, to be exact. But how does that compare to the rest of the planets and dwarf planets (hey, Pluto) in the Solar System? This nifty visualization from NASA's James O'Donaghue (u/PhysicsJ) puts it all into perspective:

As you can see, Jupiter is absolutely cruising, whirling its bulk around once every 10 hours. To drive home just how fast it's going - the surface of the Earth at the equator is traveling at roughly 1,000 miles per hour as it spins, while Jupiter's fastest point reaches 28,000 miles per hour. Hold on tight.

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This Visualization Of The Relative Rotation Rates Of Every Planet Is Fascinating - Digg

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We know the Earth spins on its axis once every 24 hours. Well, every 23 hours, 56 minutes and 4 seconds, to be exact. But how does that compare to the rest of the planets and dwarf planets (hey, Pluto) in the Solar System?

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Earth's Rotation & Revolution: Crash Course Kids 8.1

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Earth's Rotation & Revolution: Crash Course Kids 8.1

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My favourite video about the planets. Hope you enjoy watching it. From Fatemah

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Anaya Qasmi

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has anyone thought of that

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Can a star Turn into a planet
Does the influence of gravity extend out forever?

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has anyone thought of that

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Did you know that the Moon’s gravity can make a hammer and a feather land at the same time

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Did you know that the Moon’s gravity can make a hammer and a feather land at the same time

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The Moon has gravity

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Anaya Qasmi

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If there is life only on Earth, then why did Allah make all the other planets?

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If there is life only on Earth, then why did Allah make all the other planets?

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Has anyone ever thought about that?

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Sakina

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when the earth is moving why can’t we feel it moving 

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when the earth is moving why can’t we feel it moving 

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If there was no gravity what would happen?

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Did you now Earth's real name scientific name is terra and the sun is sol aka Soler system

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Did you now Earth's real name scientific name is terra and the sun is sol aka Soler system

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Alizeh

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The sun lies at the heart of the solar system, where it is by far the largest object. It holds 99.8 percent of the solar system's mass and is roughly 109 times the diameter of the Earth - about one million Earths could fit inside the sun. [ How Hot Is the Sun?]

The visible part of the sun is about 10,000 degrees Fahrenheit (5,500 degrees Celsius), while temperatures in the core reach more than 27 million F (15 million C), driven by nuclear reactions. One would need to explode 100 billion tons of dynamite every second to match the energy produced by the sun, according to NASA.

The sun is one of more than 100 billion stars in the Milky Way. It orbits some 25,000 light-years from the galactic core, completing a revolution once every 250 million years or so. The sun is relatively young, part of a generation of stars known as Population I, which are relatively rich in elements heavier than helium. An older generation of stars is called Population II, and an earlier generation of Population III may have existed, although no members of this generation are known yet.

Formation & evolution

The sun was born about 4.6 billion years ago. Many scientists think the sun and the rest of the solar system formed from a giant, rotating cloud of gas and dust known as the solar nebula. As the nebula collapsed because of its gravity, it spun faster and flattened into a disk. Most of the material was pulled toward the center to form the sun. [ How Was Earth Formed?]

The sun has enough nuclear fuel to stay much as it is now for another 5 billion years. After that, it will swell to become a red giant. Eventually, it will shed its outer layers, and the remaining core will collapse to become a white dwarf. Slowly, this will fade, to enter its final phase as a dim, cool theoretical object sometimes known as a black dwarf.

(Image credit: NASA)

Internal structure and atmosphere

The sun and its atmosphere are divided into several zones and layers. The solar interior, from the inside out, is made up of the core, radiative zone and the convective zone. The solar atmosphere above that consists of the photosphere, chromosphere, a transition region and the corona. Beyond that is the solar wind, an outflow of gas from the corona.

The core extends from the sun's center to about a quarter of the way to its surface. Although it only makes up roughly 2 percent of the sun's volume, it is almost 15 times the density of lead and holds nearly half of the sun's mass. Next is the radiative zone, which extends from the core to 70 percent of the way to the sun's surface, making up 32 percent of the sun's volume and 48 percent of its mass. Light from the core gets scattered in this zone, so that a single photon often may take a million years to pass through.

The convection zone reaches up to the sun's surface, and makes up 66 percent of the sun's volume but only a little more than 2 percent of its mass. Roiling "convection cells" of gas dominate this zone. Two main kinds of solar convection cells exist - granulation cells about 600 miles (1,000 kilometers) wide and supergranulation cells about 20,000 miles (30,000 km) in diameter.

The photosphere is the lowest layer of the sun's atmosphere, and emits the light we see. It is about 300 miles (500 km) thick, although most of the light comes from its lowest third. Temperatures in the photosphere range from 11,000 F (6,125 C) at bottom to 7,460 F (4,125 C) at top. Next up is the chromosphere, which is hotter, up to 35,500 F (19,725 C), and is apparently made up entirely of spiky structures known as spicules typically some 600 miles (1,000 km) across and up to 6,000 miles (10,000 km) high.

After that is the transition region a few hundred to a few thousand miles thick, which is heated by the corona above it and sheds most of its light as ultraviolet rays. At the top is the super-hot corona, which is made of structures such as loops and streams of ionized gas. The corona generally ranges from 900,000 F (500,000 C) to 10.8 million F (6 million C) and can even reach tens of millions of degrees when a solar flare occurs. Matter from the corona is blown off as the solar wind.

Magnetic field

The strength of the sun's magnetic field is typically only about twice as strong as Earth's field. However, it becomes highly concentrated in small areas, reaching up to 3,000 times stronger than usual. These kinks and twists in the magnetic field develop because the sun spins more rapidly at the equator than at the higher latitudes and because the inner parts of the sun rotate more quickly than the surface. These distortions create features ranging from sunspots to spectacular eruptions known as flares and coronal mass ejections. Flares are the most violent eruptions in the solar system, while coronal mass ejections are less violent but involve extraordinary amounts of matter - a single ejection can spout roughly 20 billion tons (18 billion metric tons) of matter into space.

Chemical composition

Just like most other stars, the sun is made up mostly of hydrogen, followed by helium. Nearly all the remaining matter consists of seven other elements - oxygen, carbon, neon, nitrogen, magnesium, iron and silicon. For every 1 million atoms of hydrogen in the sun, there are 98,000 of helium, 850 of oxygen, 360 of carbon, 120 of neon, 110 of nitrogen, 40 of magnesium, 35 of iron and 35 of silicon. Still, hydrogen is the lightest of all elements, so it only accounts for roughly 72 percent of the sun's mass, while helium makes up about 26 percent.

(Image credit: Karl Tate/SPACE.com)

Sunspots and solar cycles

Sunspots are relatively cool, dark features on the sun's surface that are often roughly circular. They emerge where dense bundles of magnetic field lines from the sun's interior break through the surface. [ Related: Largest Sunspot in 24 Years Wows Scientists, But Also Mystifies]

The number of sunspots varies as solar magnetic activity does - the change in this number, from a minimum of none to a maximum of roughly 250 sunspots or clusters of sunspots and then back to a minimum, is known as the solar cycle, and averages about 11 years long. At the end of a cycle, the magnetic field rapidly reverses its polarity.

Observation & history

Ancient cultures often modified natural rock formations or built stone monuments to mark the motions of the sun and moon, charting the seasons, creating calendars and monitoring eclipses. Many believed the sun revolved around the Earth, with ancient Greek scholar Ptolemy formalizing this "geocentric" model in 150 B.C. Then, in 1543, Nicolaus Copernicus described a heliocentric, sun-centered model of the solar system, and in 1610, Galileo Galilei's discovery of Jupiter's moons revealed that not all heavenly bodies circled the Earth.

To learn more about how the sun and other stars work, after early observations using rockets, scientists began studying the sun from Earth orbit. NASA launched a series of eight orbiting observatories known as the Orbiting Solar Observatory between 1962 and 1971. Seven of them were successful, and analyzed the sun at ultraviolet and X-ray wavelengths and photographed the super-hot corona, among other achievements.

In 1990, NASA and the European Space Agency launched the Ulysses probe to make the first observations of its polar regions. In 2004, NASA's Genesis spacecraft returned samples of the solar wind to Earth for study. In 2007, NASA's double-spacecraft Solar Terrestrial Relations Observatory (STEREO) mission returned the first three-dimensional images of the sun. NASA lost contact with STEREO-B in 2014, which is remained out of contact except for a brief period in 2016. STEREO-A remains fully functional.

One of the most important solar missions to date has been the Solar and Heliospheric Observatory (SOHO), which was designed to study the solar wind, as well as the sun's outer layers and interior structure. It has imaged the structure of sunspots below the surface, measured the acceleration of the solar wind, discovered coronal waves and solar tornadoes, found more than 1,000 comets, and revolutionized our ability to forecast space weather. Recently, NASA's Solar Dynamics Observatory (SDO), the most advanced spacecraft yet designed to study the sun, has returned never-before-seen details of material streaming outward and away from sunspots, as well as extreme close-ups of activity on the sun's surface and the first high-resolution measurements of solar flares in a broad range of extreme ultraviolet wavelengths.

There are other missions planned to observe the sun in the next few years. The European Space Agency's Solar Orbiter will launch in 2018, and by 2021 will be in operational orbit around the sun. Its closest approach to the sun will be 26 million miles (43 million km) - about 25 percent closer than Mercury. Solar Orbiter will look at particles, plasma and other items in an environment relatively close to the sun, before these things are modified by being transported across the solar system. The goal is to better understand the solar surface and the solar wind.

The Parker Solar Probe will launch in 2018 to make an extremely close approach to the sun, getting as near as 4 million miles (6.5 million km). The spacecraft will look at the corona - the superheated outer atmosphere of the sun - to learn more about how energy flows through the sun, the structure of the solar wind, and how energetic particles are accelerated and transported.
Additional reporting by Elizabeth Howell and Nola Taylor Redd, Space.com Contributors

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Earth's Sun: Facts About the Sun's Age, Size and History

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The sun lies at the heart of the solar system, where it is by far the largest object. It holds 99.8 percent of the solar system's mass and is roughly 109 times the diameter of the Earth - about one million Earths could fit inside the sun. [ How Hot Is the Sun?]

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Why is this corona vids not going

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What would happen if earth lost its gravity and oxygen

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What would happen if earth lost its gravity and oxygen

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Ilan Haider

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Ilan Haider

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What if we can no longer live on Earth? Where will we go?

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Have people gone to space and seen the Milky Way or any other planets?

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Why can't we live in space?

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If Mercury is close to the Sun, why does it not melt?

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Why is it that sometimes we cannot see our shadow?

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Why is it that sometimes we cannot see our shadow?

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Did you now if you click our little pictures you get an option to follow that person and if you click your own picture you can see how many follower's you have

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Sakina

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Why is there no gravity in space?, Sakina

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I use to live here, I wish I could travel so I could go back

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Did you know the Astronauts jump from space to earth, Sakina

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I wish I could travel to see the stars in space

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Alizeh

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I wonder why space is so big

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Alizeh

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I wonder how so much gravity gets in to the black hole

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The force of gravity

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How are black holes made? - Summaiya Mahmood

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I wish I could travel at all

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The sun is the only object in our solar system to shine with its own light

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So mezmarizing

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I wish I could see the  selesteall fireworks in real life

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I wish I would be a doctor and treat corona

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What will happen to us after a million years?

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If we travel to a planet outside the galaxy, what will we call that planet?

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Oooooooooooo London to

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I wish I could go to Italy to