sunsʌn
sun (v)
- present
- suns
- past
- sunned
- past participle
- sunned
- present participle
- sunning
sun (n)
- plural
- suns
sun
sun
English Definitions:
sun, Sun (noun)
the star that is the source of light and heat for the planets in the solar system
"the sun contains 99.85% of the mass in the solar system"; "the Earth revolves around the Sun"
sunlight, sunshine, sun (noun)
the rays of the sun
"the shingles were weathered by the sun and wind"
sun (noun)
a person considered as a source of warmth or energy or glory etc
sun (noun)
any star around which a planetary system revolves
Sunday, Lord's Day, Dominicus, Sun (verb)
first day of the week; observed as a day of rest and worship by most Christians
sun, sunbathe (verb)
expose one's body to the sun
sun, insolate, solarize, solarise (verb)
expose to the rays of the sun or affect by exposure to the sun
"insolated paper may turn yellow and crumble"; "These herbs suffer when sunned"
sun (Noun)
A star, especially when seen as the centre of any single solar system.
sun (Noun)
The light and warmth which is received from the sun.
sun (Noun)
Something like the sun in brightness or splendor.
sun (Noun)
Sunrise or sunset.
sun (Verb)
To expose to the warmth and radiation of the sun.
sun (Verb)
To warm or dry in the sunshine.
sun (Verb)
To be exposed to the sun.
sun (ProperNoun)
The star which the Earth revolves around and from which it receives light and warmth.
Sun (ProperNoun)
Sunday
Sun (ProperNoun)
The star at the center of the Solar System, represented in astronomy and astrology by .
Sun (ProperNoun)
An English tabloid newspaper.
Sun
The Sun is the star at the center of the Solar System. It is almost perfectly spherical and consists of hot plasma interwoven with magnetic fields. It has a diameter of about 1,392,684 km, about 109 times that of Earth, and its mass accounts for about 99.86% of the total mass of the Solar System. Chemically, about three quarters of the Sun's mass consists of hydrogen, while the rest is mostly helium. The remainder consists of heavier elements, including oxygen, carbon, neon and iron, among others. The Sun formed about 4.6 billion years ago from the gravitational collapse of a region within a large molecular cloud. Most of the matter gathered in the center, while the rest flattened into an orbiting disk that would become the Solar System. The central mass became increasingly hot and dense, eventually initiating thermonuclear fusion in its core. It is thought that almost all other stars form by this process. The Sun's stellar classification, based on spectral class, is a G-type main-sequence star and is informally designated as a yellow dwarf because its visible radiation is most intense in the yellow-green portion of the spectrum, and although its color is white, from the surface of the Earth it may appear yellow because of atmospheric scattering of blue light. In the spectral class label, G2 indicates its surface temperature of approximately 5778 K, and V indicates that the Sun, like most stars, is a main-sequence star, and thus generates its energy by nuclear fusion of hydrogen nuclei into helium. In its core, the Sun fuses 620 million metric tons of hydrogen each second.
Sun
The Sun is the star at the center of the Solar System. It is a nearly perfect sphere of hot plasma, with internal convective motion that generates a magnetic field via a dynamo process. It is by far the most important source of energy for life on Earth. Its diameter is about 1.39 million kilometers (864,000 miles), or 109 times that of Earth, and its mass is about 330,000 times that of Earth. It accounts for about 99.86% of the total mass of the Solar System. Roughly three quarters of the Sun's mass consists of hydrogen (~73%); the rest is mostly helium (~25%), with much smaller quantities of heavier elements, including oxygen, carbon, neon, and iron.The Sun is a G-type main-sequence star (G2V) based on its spectral class. As such, it is informally and not completely accurately referred to as a yellow dwarf (its light is closer to white than yellow). It formed approximately 4.6 billion years ago from the gravitational collapse of matter within a region of a large molecular cloud. Most of this matter gathered in the center, whereas the rest flattened into an orbiting disk that became the Solar System. The central mass became so hot and dense that it eventually initiated nuclear fusion in its core. It is thought that almost all stars form by this process. The Sun currently fuses about 600 million tons of hydrogen into helium every second, converting 4 million tons of matter into energy every second as a result. This energy, which can take between 10,000 and 170,000 years to escape from its core, is the source of the Sun's light and heat. When hydrogen fusion in its core has diminished to the point at which the Sun is no longer in hydrostatic equilibrium, its core will undergo a marked increase in density and temperature while its outer layers expand, eventually transforming the Sun into a red giant. It is calculated that the Sun will become sufficiently large to engulf the current orbits of Mercury and Venus, and render Earth uninhabitable – but not for about five billion years. After this, it will shed its outer layers and become a dense type of cooling star known as a white dwarf, and no longer produce energy by fusion, but still glow and give off heat from its previous fusion. The enormous effect of the Sun on Earth has been recognized since prehistoric times, and the Sun has been regarded by some cultures as a deity. The synodic rotation of Earth and its orbit around the Sun are the basis of solar calendars, one of which is the predominant calendar in use today.
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