Necrobp

This post needs more creepypastas greentext

>Be OP >Need attention >Idea.gif >Activate ShitUnoriginalGimmick.exe >??? >Profit

[quote]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. 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. Advertisement 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. 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. Advertisement A huge solar filament snakes around the southwestern horizon of the sun in this full disk photo taken by NASA's Solar Dynamics Observatory on Nov. 17, 2010. A huge solar filament snakes around the southwestern horizon of the sun in this full disk photo taken by NASA's Solar Dynamics Observatory on Nov. 17, 2010. 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 leadand 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 kilometers) 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 or kilometers 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. Yup. 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 hydrogenin 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. Still Here? Sunspots & solar cycles See how solar flares, sun storms and huge eruptions from the sun work in this SPACE.com infographic. <a href="http://www.space.com/12047-solar-flares-sun-storms-space-weather-infographic.html">View the full solar storm infographic here</a>. See how solar flares, sun storms and huge eruptions from the sun work in this SPACE.com infographic. View the full solar storm infographic here. Credit: Karl Tate/SPACE.com 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. LENNNYY!!!! 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. - See more at: http://www.space.com/58-the-sun-formation-facts-and-characteristics.html#sthash.YIj9GUek.dpuf[/quote] Wait... Wrong thread

>I was only 9 years old >I loved Bungie so much, I had all the merchandise and movies >I pray to the CoC every night before bed, thanking it for the life I've been given >"Bungie is love" I say; "Bungie is life" >My dad hears me and calls me a -blam!- >I know he was just jealous of my devotion for Bungie >I called him a -blam!- >He slaps me and sends me to go to sleep >I'm crying now, and my face hurts >I lay in bed and it's really cold >Suddenly, a warmth is moving towards me >It's a ninja >I am so happy He whispers into my ear "This is my forum." >He grabs me with his stealthy ninja hands and puts me down onto my hands and knees >I'm ready >I spread my ass-cheeks for the ninja >He penetrates my butt-hole >It hurts so much but I do it for Bungie's CoC >I can feel my butt tearing as my eyes start to water >I push against his force >I want to please Bungie >He roars in a mighty roar as he fills my butt with his love >My dad walks in >The ninja looks him straight in the eyes and says "We're gonna play nice now." >The ninja leaves through my window >Bungie is love. Bungie is life.

>OP post thread >Be Me try to make greenpost >Be me and fails

Bump for later.

This isn't 4chan

>am 12 >Wana make bungie account >Whatsagoodname >thinking.jpg >name my self the great reebok >sign my name after every post >"people will like me!" >noonedoes.jpg