The topic about the Sub will help the aspirants to know the basic concepts and make their foundation strong while preparing for UPSC IAS Exam.
The sun is the source of heat and light and the midpoint and for the solar system. It is made up of enormously hot gas. It gives the pulling force that binds the solar system.
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Key facts about the Sun
- 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 with only Jupiter having the remaining 1.2%.
- The Sun is personified in many mythologies: the Greeks called it Helios, Ancient Indian called it Surya, Romans called it Sol.
- The Sun is, at present, about 70% hydrogen and 28% helium by mass everything else 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.
- The Sun’s magnetic field is very strong (by terrestrial standards) and very complicated. Its magnetosphere (also known as the heliosphere) extends well beyond Pluto.
- The Sun’s output is not entirely constant. Nor is the amount of sunspot activity. There was a period of very low sunspot activity in the latter half of the 17th century called the Maunder Minimum. It coincides with an abnormally cold period in northern Europe sometimes known as the Little Ice Age. Since the formation of the solar system the Sun’s output has increased by about 40%.
- The Sun is about 4.5 billion years old. Since its birth it has used up about half of the hydrogen in its core. It will continue to radiate “peacefully” for another 5 billion years or so (although its luminosity will approximately double in that time). But eventually it will run out of hydrogen fuel. It will then be forced into radical changes which, though commonplace by stellar standards, will result in the total destruction of the Earth.
Characteristics of the Sun
The various characteristics of the Sun are given in the tables below:
|Mean distance from Earth||1 au ≈ 1.496×108 km
8 min 19 s at light speed
|Visual brightness (V)||-26.74|
|Spectral classification (G)||G2V|
|Metallicity Angular size||Z = 0.0122|
|Angular Size||31.6–32.7 minutes of arc|
The physical characteristics of the Sun is highlighted below:
|Equatorial radius||695,700 km
109 × Earth
|Equatorial circumference||4.379×106 km
109 × Earth
|Flattening Surface area||9×10−6|
1,300,000 × Earth
333,000 × Earth
|Average Density||1.408 g/cm3
0.255 × Earth
|Center Density||162.2 g/cm3
12.4 × Earth
|Temperature||Center (modeled): 1.57×107K
Photosphere (eHoffective): 5,772 K
Corona: ≈ 5×106 K
Corona of the Sun – A Brief Understanding of the Outermost Part of the Sun
What is the corona of the sun?
The Sun’s corona is the outermost part of the Sun’s atmosphere. The corona is usually hidden by the bright light of the Sun’s surface. That makes it difficult to see without using special instruments. However, the corona can be viewed during a total solar eclipse.
What is the sun’s corona made of?
Corona, outermost region of the Sun’s atmosphere, consisting of plasma (hot ionized gas). It has a temperature of approximately two million kelvins and an extremely low density. The corona continually varies in size and shape as it is affected by the Sun’s magnetic field.
Why is the sun’s corona so hot?
Because the coronal material is so thin and tenuous, only a tiny portion of all the sound energy in the photosphere needs to bleed up into the corona and be absorbed in order to heat it to the observed temperatures.
How hot is the corona of the Sun in Fahrenheit?
The outermost atmospheric layer is the corona, which gets really hot, almost 2,000,000 degrees F. This is where the solar wind begins.
What is the diamond ring effect?
A phenomenon, sometimes observed immediately before and after a total eclipse of the sun, in which one of Baily’s beads is much brighter than the others, resembling a diamond ring around the moon.
Which layer of the sun is the hottest?
The hottest part of the Sun is the core, at 28,080,000°F, on average.
Questions related to the Sun
What is the composition of the Sun?
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.
How old is the Sun?
The Sun is one of 100 billion stars in our Milky Way galaxy. Scientists estimate that the Sun is about 4.5 billion years old, or approximately halfway through its life cycle.
What is Inside the Sun?
The sun is a big ball of gas and plasma. Most of the gas — 91 percent — is hydrogen. It is converted into energy in the sun’s core. The energy moves outward through the interior layers, into the sun’s atmosphere, and is released into the solar system as heat and light.
The Sun – UPSC Notes:- Download PDF Here
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