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The Sun is the star at the center of the Solar System. It is a massive, hot ball of plasma, inflated and heated by energy produced by nuclear fusion reactions at its core. Part of this energy is emitted from its surface as light, ultraviolet, and infrared radiation, providing most of the energy for life on Earth. The Sun has been an object of veneration in many cultures. It has been a central subject for astronomical research since ancient times.

The Sun is a G-type main-sequence star (G2V), informally called a yellow dwarf, though its light is actually white. 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.

Composition

The Sun consists primarily of the chemical elements hydrogen and helium. At this time in the Sun's life, they account for 74.9% and 23.8%, respectively, of the mass of the Sun in the photosphere.

hydrogen
Hydrogen (H)
Helium
Helium (He)

All heavier elements, called metals in astronomy, account for less than 2% of the mass, with oxygen (roughly 1% of the Sun's mass), carbon (0.3%), neon (0.2%), and iron (0.2%) being the most abundant.

Neon
Neon (Ne)
Iron
Iron (Fe)
carbon
Carbon (C)
Oxygen
Oxygen (O₂)
Log

In solar research it is more common to express the abundance of each element in dex, which is a scaled logarithmic unit.

With 'e' being the element in question and nH as 10¹² hydrogen atoms. By definition :


  • Hydrogen abundance = 12
  • Helium abundance varies = 10.3 and 10.5 approx.
  • Carbon abundance = 8.47
  • Neon abundance = 8.29
  • Oxygen abundance= 7.69
  • Iron abundance = 7.62

Location

a. Location (in the Solar System)

The Sun has eight known planets orbiting it. This includes four terrestrial planets (Mercury, Venus, Earth, and Mars), two gas giants (Jupiter and Saturn), and two ice giants (Uranus and Neptune). The Solar System also has nine bodies generally considered as dwarf planets and some more candidates, an asteroid belt, numerous comets, and a large number of icy bodies which lie beyond the orbit of Neptune. Six of the planets and many smaller bodies also have their own natural satellites: in particular, the satellite systems of Jupiter, Saturn, and Uranus are in some ways like miniature versions of the Sun's system.

Location Pict

b. Location (In relation to the Celestial Neighbourhood)

The Solar System is surrounded by the Local Interstellar Cloud, although it is not clear if it is embedded in the Local Interstellar Cloud or if it lies just outside the cloud's edge. Multiple other interstellar clouds also exist in the region within 300 light-years of the Sun, known as the Local Bubble. The latter feature is an hourglass-shaped cavity or superbubble in the interstellar medium roughly 300 light-years across. The bubble is suffused with high-temperature plasma, suggesting that it may be the product of several recent supernovae.

celestial Pict

Visual Brightness

−26.74 (V)


Absolute Magnitude

4.83


Metallicity

Z = 0.0122


Angular Size

0.527–0.545°


Velocity

- 251 km/s (156 mi/s) orbit Galactic Center
- 20 km/s (12 mi/s) to stellar neighborhood
- 370 km/s (230 mi/s) to cosmic microwave background


Galactic Period

225–250 million years


Age

4.6 billion years


Temperature (approx.)

- 15,700,000 K (center)
- 5,772 K (photosphere)
- 5,000,000 K (corona)


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