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The Sun is by far the largest object in the solar system. It contains more than 99.8% of the total mass of the Solar System

It is often said that the Sun is an "ordinary" star. That's true in the sense that there are several others like to it. But there are many more smaller stars than larger ones; the Sun is in the top 10% by mass. The median size of stars in our galaxy is probably less than half the mass of the Sun.

The Sun is, at present, about 70% hydrogen and 28% helium by mass everything else ("metals") amounts to less than 2%. This changes slowly over time as the Sun converts hydrogen to helium in its core.

The outer layers of the Sun exhibit differential rotation: at the equator the surface rotates once every 25.4 days; near the poles it's as much as 36 days. This odd behavior is due to the fact that the Sun is not a solid body like the Earth. Similar effects are seen in the gas planets. The differential rotation extends considerably down into the interior of the Sun but the core of the Sun rotates as a solid body.

Conditions at the Sun's core (approximately the inner 25% of its radius) are extreme. The temperature is 15.6 million Kelvin and the pressure is 250 billion atmospheres. At the center of the core the Sun's density is more than 150 times that of water.

The surface of the Sun, called the photosphere, is at a temperature of about 5800 K.Sunspots are "cool" regions, only 3800 K (they look dark only by comparison with the surrounding regions). Sunspots can be very large, as much as 50,000 km in diameter. Sunspots are caused by complicated and not very well understood interactions with the Sun's magnetic field.

In addition to heat up and glow, the Sun also emits a low density stream of charged particles (mostly electrons and protons) known as the solar wind which propagates throughout the solar system at about 450 km/sec. The solar wind and the much higher energy particles ejected by solar flares can have dramatic effects on the Earth ranging from power line surges to radio interference to the beautiful aurora borealis.

Recent data from the spacecraft Ulysses show that during the minimum of the solar cycle the solar wind emanating from the polar regions flows at nearly double the rate, 750 kilometers per second, than it does at lower latitudes. The composition of the solar wind also appears to differ in the polar regions. During the solar maximum, however, the solar wind moves at an intermediate speed.

Further study of the solar wind will be done by Wind, ACE and SOHO spacecraft from the dynamically stable vantage point directly between the Earth and the Sun about 1.6 million km from Earth.

The solar wind has large effects on the tails of comets and even has measurable effects on the trajectories of spacecraft.

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ppt

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ގޮނޑުދޮށުގައި ދޫނި އުޅޭ

ކަކުނި ފިނަދަނަ ބޮނޑަނަ އުޅޭ
މަކަނަޔާ ބަރަވެއްޔާ

މިފަދަ ދިރޭތަކެތި އުޅޭ

ކަޅުފަހުގައި ބޯށި ކުރެދި
ކާނި މިރިހި މަގޫހުރޭ
އަޅުގަނޑުމެން ބުނެ އުޅޭމާ
ގޮނޑުދޮށްތައް ސާފުކުރޭ f

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ބައްޕަގެ ނަސޭހަތް

ބައްޕަދޭ ހެޔޮހާ ނަސޭހަތް އަޑުއަހާށޭ ދަރިފުޅާ

ބައްޕަ ދުނިޔޭން ވަކިވެ ދިޔަޔަސް ބަސްއަހާށޭ ދަރިފުޅާ

ބައްޕައާއި މަންމަގެ މިއާދޭސް އަޑުއަހާށޭ ދަރިފުޅާ      (2)

ހެޔޮލަފާ އިންސާނަކަށް ވާން  ދަސްކުރާށޭ ދަރިފުޅާ

ހެޔޮކަމެއް ނޫނީ ނުކުރުމަށް އިސްނަގާށޭ ދަރިފުޅާ

ހެޔޮ ނުވާނޭ މާދަމާވެސް  މަރުވެދާނޭ ދަރިފުޅާ

ބައްޕަދޭ ހެޔޮހާ ނަސޭހަތް އަޑުއަހާށޭ ދަރިފުޅާ

މަންމައަށް ހިތްހެޔޮކަމާއެކު  ބަސްބުނާށޭ ދަރިފުޅާ

މަންމަ ރޮއްވާ ދެރަކުރާކަށް ހެޔޮ ނުވާނޭ ދަރިފުޅާ

މަންމައާ އެއްސަފުގަ މީހަކު ުހިމަނާށޭ ދަރިފުޅާ

ބައްޕަދޭ ހެޔޮހާ ނަސޭހަތް އަޑުއަހާށޭ ދަރިފުޅާ

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Mission

To further develop the potential of the individual in a holistic, balanced and integrated manner encompassing the intellectual, spiritual, emotional and physical aspects in order to create a well balanced human being with high Islamic moral standards

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ކިޔާލަމާ