Our star, the Sun, makes up 99% of all the mass in the Solar System. Its core is so dense and hot that normally repellent nuclei fuse together in nuclear reactions that produce vast amounts of energy.
The Sun is mostly hydrogen (its main fuel) and helium, and radiates charged particles called solar wind across the Solar System. Phenomena such as solar flares and sunspots are evidence of the Sun's strong magnetic field, which changes on a roughly 11-year cycle.
Read about eye safety during solar eclipses on the NASA website.
Photo: The Sun taken by the SOHO probe (ESA/NASA)
The Sun's core powers the Solar System.
Sir Patrick Moore gets a guided tour of the Sun probe.
Launched in 1990, the European Ulysses spacecraft became the first probe to fly over the poles of the Sun. The craft returned data about solar activity at high latitudes during a series of flybys. The mission ended in 2009.
Brian Cox experiences a perfect solar eclipse.
Professor Brian Cox travels to Varanasi, India, to watch a total solar eclipse.
Brian Cox travels to Norway to see the Northern Lights.
Professor Brian Cox travels to Norway in search of the Aurora Borealis, or Northern Lights. Astrophysicist Professor Mike Lockwood accompanies him as they wait for the dazzling display brought by the solar wind.
What can a tin of water, a thermometer and an umbrella tell us?
Professor Brian Cox re-creates Sir John Herschel's 1838 experiment, which measured the amount of solar energy that falls on the Earth, with a tin, some water, a thermometer and an umbrella.
The Sun was born from a collapsing cloud of hydrogen.
Professor Brian Cox explains how stars are formed. By looking at the Milky Way we can see vast stellar nurseries in our galaxy.
The Sun[a] is the star at the center of the Solar System and is by far the most important source of energy for life on Earth. It is a nearly perfect spherical ball of hot plasma, with internal convective motion that generates a magnetic field via a dynamo process. Its diameter is about 109 times that of Earth, and it has a mass about 330,000 times that of Earth, accounting for about 99.86% of the total mass of the Solar System. Chemically, about three quarters of the Sun's mass consists of hydrogen; the rest is mostly helium, 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 spectral class and it is informally referred to as a yellow dwarf. It formed approximately 4.567 billion[b] 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 increasingly hot and dense, eventually initiating nuclear fusion in its core. It is thought that almost all stars form by this process. The Sun is roughly middle age and has not changed dramatically for four billion[b] years, and will remain fairly stable for four billion more. However, after hydrogen fusion in its core has stopped, the Sun will undergo severe changes and become a red giant. It is calculated that the Sun will become sufficiently large to engulf the current orbits of Mercury, Venus, and possibly Earth.
The enormous effect of the Sun on the Earth has been recognized since prehistoric times, and the Sun has been regarded by some cultures as a deity. Earth's movement around the Sun is the basis of the solar calendar, which is the predominant calendar in use today.