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Facts about Sun

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The Sun does not have a definite boundary as rocky planets do; the density of its gases drops approximately exponentially with increasing distance from the center of the Sun.

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When observing the Sun with appropriate filtration, the most immediately visible features are usually its sunspots, which are well-defined surface areas that appear darker than their surroundings due to lower temperatures.

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The largest sunspots can be tens of thousands of kilometers across.

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The solar interior is not directly observable, and the Sun itself is opaque to electromagnetic radiation.

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All matter in the Sun is in the form of gas and plasma due to its high temperatures.

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Sunlight has approximately a black-body spectrum that indicates its temperature is about 6,000 K(10,340 °F / 5,727 °C), interspersed with atomic absorption lines from the tenuous layers above the photosphere.

image: www.acs.org
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Among the proposals were that the Sun extracted its energy from friction of its gas masses, or that its energy was derived from gravitational potential energy released as it continuously contracted.

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The thermal columns in the convection zone form an imprint on the surface of the Sun, in the form of the solar granulation and supergranulation.

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Each gamma ray in the Sun's core is converted into several million visible light photons before escaping into space.

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The Sun orbits the center of the Milky Way galaxy at a distance of about 25,000 to 28,000 light-years from the galactic center, completing one revolution in about 225–250 million years.

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Within the Sun's core, nuclear fusion reactions take place, with hydrogen nuclei being fused into helium nuclei.

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Nevertheless, the Sun has a well-defined interior structure, described below.

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The solar wind travels outward continuously through the heliosphere, forming the solar magnetic field into a spiral shape, until it impacts the heliopause more than 50 AU from the Sun.

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Above the turbopause (about 100 km), the Earth's atmosphere begins to have a composition that varies with altitude.

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Observed from Earth, the path of the Sun across the sky varies throughout the year.

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The visible surface of the Sun, the photosphere, is the layer below which the Sun becomes opaque to visible light.

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Current theory predicts that in about five billion years, the Sun will evolve into a red giant and then a white dwarf, creating a planetary nebula in the process.

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Sunspots usually exist as pairs with opposite magnetic polarity.

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The Sun is sometimes referred to by its Latin name Sol or its Greek name Helios.

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The solar constant is the amount of power that the Sun deposits per unit area that is directly exposed to sunlight.

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Humanity's most fundamental understanding of the Sun is as the luminous disk in the heavens, whose presence above the horizon creates day and whose absence causes night.

image: i.pinimg.com
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All these satellites have observed the Sun from the plane of the ecliptic, and so have only observed its equatorial regions in detail.

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Another scientist to challenge the accepted view was Nicolaus Copernicus, who in the sixteenth century developed the theory that the Earth orbited the Sun, rather than the other way around.

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The Sun will spend a total of approximately 10 billion years as a main sequence star.

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The Sun does not have enough mass to explode as a supernova.

image: cdn.phys.org
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Nuclear fusion was first proposed as the source of solar energy only in the 1930s, when Hans Bethe calculated the details of the two main energy-producing nuclear reactions that power the Sun.

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Ultraviolet light from the Sun has antiseptic properties and can be used to sterilize tools.

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Neutrinos are also released by the fusion reactions in the core, but unlike photons they very rarely interact with matter, so almost all are able to escape the Sun immediately.

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The energy stored in petroleum and other fossil fuels was originally converted from sunlight by photosynthesis in the distant past.

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The number of sunspots visible on the Sun is not constant, but varies over a 10-12 year cycle known as the Solar cycle.

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The Sun's magnetic field gives rise to many effects that are collectively called solar activity.

image: www.mpg.de
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The Sun will then evolve into a white dwarf, slowly cooling over eons.

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Following the red giant phase, intense thermal pulsations will cause the Sun to throw off its outer layers, forming a planetary nebula.

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The turbulent convection of this outer part of the solar interior gives rise to a "small-scale" dynamo that produces magnetic north and south poles all over the surface of the Sun.

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During partial eclipses most sunlight is blocked by the Moon passing in front of the Sun, but the uncovered parts of the photosphere have the same surface brightness as during a normal day.

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Most of the Sun's mass lies within about 0.7 radii of the center.

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Sunlight is very bright, and looking directly at the Sun with the naked eye for brief periods can be painful, but is generally not hazardous.

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Yohkoh observed an entire solar cycle but went into standby mode when an annular eclipse in 2001 caused it to lose its lock on the Sun.

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The "worship of the five forms" (paсc?yatana p?j?) system, which was popularized by the ninth-century philosopher ?a?kar?c?rya among orthodox Brahmins of the Sm?rta tradition, invokes the five deities Ganesha, Vishnu, Shiva, Dev?, and S?rya.

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The Earth and other matter (including other planets, asteroids, comets, meteoroids, and dust) orbit the Sun, which by itself accounts for more than 99 percent of the solar system's mass.

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Energy from the Sun—in the form of insolation from sunlight—supports almost all life on Earth via photosynthesis, and drives the Earth's climate and weather.

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The low corona, which is very near the surface of the Sun, has a particle density of 1014/m3-1016/m3.

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From about 0.7 solar radii to the Sun's visible surface, the material in the Sun is not dense enough or hot enough to transfer the heat energy of the interior outward via radiation.

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The Sun's radius is measured from its center to the edge of the photosphere.

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The Ulysses probe was launched in 1990 to study the Sun's polar regions.

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The polarity of the leading sunspot alternates every solar cycle, so that it will be a north magnetic pole in one solar cycle and a south magnetic pole in the next.

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The parts of the Sun above the photosphere are referred to collectively as the solar atmosphere.

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Due to logarithmic size distribution, the Sun is actually brighter than 85 percent of the stars in the Galaxy, most of which are red dwarfs.

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The shape described by the Sun's position, considered at the same time each day for a complete year, is called the analemma and resembles a figure 8 aligned along a North/South axis.

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Theoretical models of the sun's development suggest that 3.8 to 2.5 billion years ago, during the Archean period, the Sun was only about 75% as bright as it is today.

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The Sun is thought to be about 4.6 billion years old and about halfway through its main-sequence evolution.

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Computer modeling of the Sun is also used as a theoretical tool to investigate its deeper layers.

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The Sun is placed in a spectral class called G2V.

image: starplot.org
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About 74 percent of the Sun's mass is hydrogen, 25 percent is helium, and the rest is made up of trace quantities of heavier elements.

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The volume of the Sun is 1,303,600 times that of the Earth; 71 percent of hydrogen makes up the mass of the Sun.

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The corona is the extended outer atmosphere of the Sun, which is much larger in volume than the Sun itself.

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Unfiltered binoculars can deliver over 500 times more sunlight to the retina than does the naked eye, killing retinal cells almost instantly.

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One way to view the Sun safely is by projecting an image onto a screen using binoculars or a small telescope.

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Sunlight is the main source of energy near the surface of Earth.

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The Sun is the star at the center of the Earth's solar system.

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Viewing the Sun through light-concentrating optics such as binoculars is very hazardous without an attenuating (ND) filter to dim the sunlight.

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Looking directly at the Sun causes phosphene visual artifacts and temporary partial blindness.

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The Solar system (or solar system) is the home stellar system for human beings and all known forms of life.

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The chromosphere, transition region, and corona are much hotter than the surface of the Sun; the reason why is not yet known.

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The influence of the Sun's rotating magnetic field on the plasma in the interplanetary medium creates the heliospheric current sheet, which separates regions with magnetic fields pointing in different directions.

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The plasma in the interplanetary medium is also responsible for the strength of the Sun's magnetic field at the orbit of the Earth.

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Sunspots are regions of intense magnetic activity where energy transport is inhibited by strong magnetic fields.

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At a typical solar minimum, few sunspots are visible, and occasionally none at all can be seen.

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The Sun is a near-perfect sphere, with an oblateness estimated at about 9 millionths, which means that its polar diameter differs from its equatorial diameter by only 10 km.

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Elemental abundances in the photosphere are well known from spectroscopic studies, but the composition of the interior of the Sun is more poorly understood.

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The first satellites designed to observe the Sun were NASA's Pioneers 5, 6, 7, 8 and 9, which were launched between 1959 and 1968.

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The parts of the Sun above the photosphere are referred to collectively as the solar atmosphere.

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In 1868, Norman Lockyer hypothesized that these absorption lines were due to a new element which he dubbed "helium," after the Greek Sun god Helios.

The mathematician and astronomer Theodosius of Bithynia (ca. 160 BCE-ca. 100 BCE ) is said to have invented a universal sundial that could be used anywhere on Earth. The Romans adopted the Greek sundials, and the first record of a sun-dial in Rome is 293 BC according to Pliny.

Sundials are the oldest known instruments for telling time. The surface of a sundial has markings for each hour of daylight. As the Sun moves across the sky, another part of the sundial casts a shadow on these markings. The position of the shadow shows what time it is.

During their active growing season, Venus Fly Traps should receive a minimum of 12 hours of light (also known as a 12 hour photoperiod) with a minimum of 4 hours of direct sunlight, if you're growing your Venus Flytraps outside. In general, the more direct light the plant receives the healthier the plant will be.

The answer is that it would take 1.3 million Earths to fill up the Sun. That's a lot of Earths. The Sun makes up 99.86% of the mass of the Solar System. And it's the giant planets like Jupiter and Saturn which make the most of that remaining .14% of the Solar System.May 28, 2010

The answer is that it would take 1.3 million Earths to fill up the Sun. That's a lot of Earths. The Sun makes up 99.86% of the mass of the Solar System. And it's the giant planets like Jupiter and Saturn which make the most of that remaining .14% of the Solar System.May 28, 2010

The Sun is a huge, glowing sphere of hot gas. Most of this gas is hydrogen (about 70%) and helium (about 28%). Carbon, nitrogen and oxygen make up 1.5% and the other 0.5% is made up of small amounts of many other elements such as neon, iron, silicon, magnesium and sulfur.

The Sun plays multiple roles in all of Earth's space missions. The Sun is the gravitational center of the solar system. Its gravitational pull is what keeps the planets in place in their orbits.

The Sun's surface area is 11,990 times that of the Earth's. The Sun contains 99.86% of the mass in the Solar System. The mass of the Sun is approximately 330,000 times greater than that of Earth. It is almost three quarters Hydrogen, whilst most of the remaining mass is Helium.

Facts about the Sun. The Sun accounts for 99.86% of the mass in the solar system. It has a mass of around 330,000 times that of Earth. It is three quarters hydrogen and most of its remaining mass is helium.

The spin caused the cloud to flatten into a disk like a pancake. In the center, the material clumped together to form a protostar that would eventually become the sun. ... The young protostar was a ball of hydrogen and helium not yet powered by fusion.Oct 31, 2017

We definitely need the sun to survive, for many reasons. Without the sun, our planet would get extremely cold, and all living things on it would die. Plants use the sun's energy for photosynthesis, which is the process they use to make nutrients.

Nothing is more important to us on Earth than the Sun. Without the Sun's heat and light, the Earth would be a lifeless ball of ice-coated rock. The Sun warms our seas, stirs our atmosphere, generates our weather patterns, and gives energy to the growing green plants that provide the food and oxygen for life on Earth.

Solar collectors capture the sunlight and turn it into heat. People can heat their houses and their water using the sun's energy. Solar cells can turn solar energy into electricity. ... Today, solar energy provides only a small percentage of the electricity we use, but the amount we use is growing each year.

Human skin can make large amounts of vitamin D when lots of skin is exposed and the sun is high in the sky. Your body is designed to get the vitamin D it needs by producing it when your bare skin is exposed to sunlight. The part of the sun's rays that is important is ultraviolet B (UVB).

The sun provides energy. Plants transform the sun's energy into stored chemical energy during photosynthesis. This is an amazing process in which plants take carbon dioxide, water, and the sun's photons, and produce carbohydrates and oxygen.May 7, 2015

All plants would die and, eventually, all animals that rely on plants for food — including humans — would die, too. While some inventive humans might be able to survive on a Sun-less Earth for several days, months, or even years, life without the Sun would eventually prove to be impossible to maintain on Earth.

Our Sun is actually too small to end up as a black hole. ... If the Sun were somehow compressed enough to become a black hole, it would be less than 6 kilometers (well under 4 miles) across. It would exert no more gravitational force on Earth or the other planets in the solar system than it does now.

If you put a steamy cup of coffee in the refrigerator, it wouldn't immediately turn cold. Likewise, if the sun simply "turned off" (which is actually physically impossible), the Earth would stay warm—at least compared with the space surrounding it—for a few million years.Jul 16, 2013

If The Sun Dies. NASA. If you put a steamy cup of coffee in the refrigerator, it wouldn't immediately turn cold. Likewise, if the sun simply "turned off" (which is actually physically impossible), the Earth would stay warm—at least compared with the space surrounding it—for a few million years.Oct 20, 2008

Snowfall is 5 inches. The average US city gets 26 inches of snow per year. The number of days with any measurable precipitation is 92. On average, there are 152 sunny days per year in Seattle, Washington.

Many scientists think the sun and the rest of the solar system formed from a giant, rotating cloudof 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.

Facts about the SunThe Sun accounts for 99.86% of the mass in the solar system. ... Over one million Earth's could fit inside the Sun. ... One day the Sun will consume the Earth. ... The energy created by the Sun's core is nuclear fusion. ... The Sun is almost a perfect sphere. ... The Sun is travelling at 220 km per second.More items...

Our Sun is not unique in the universe. It is a common middle-sized yellow star which scientists have named Sol, after the ancient Roman name. This is why our system of planets is called the Solar System.

Despite these identifications, Apollo was never actually described by the Greek poets driving the chariot of the sun, although it was common practice among Latin poets. Therefore, Helios is still known as the "sun god" – the one who drives the sun chariot across the sky each day.

The Sun appears so large compared to the other stars because it is so much closer to us than any other star. The Sun is just an average sized star. For example, below is a list of some of the largest stars in our galaxy and how they compare to our Sun: Mu Cephi - about 1500 times the size of our sun.