The Sun
Stars come in varying sizes, temperatures, and ages and are basically giant balls of exploding hydrogen and helium. Our Sun is an averaged sized, middled aged yellow Dwarf Star.
A star's surface temperatures usually ranges between 2,500 and 40,000°C. We are able to discover the temperature and age of many distant stars merely by observing their colour with the naked eye. The cooler, older stars appear red whereas the hotter, younger stars look blue.
A star's colour ranges from red to orange, yellow, white, bluish-white, and blue the hottest. However, other stars such as Protostars and brown dwarfs, may emit energy beyond the visible spectrum in the form of infrared radiation.
Betelgeuse in Orion is a fine example of a red supergiant star. Arcturus in Boötes appears orange, Capella in Auriga is a yellow star, Sirius B in Canis Major is white, and Rigel in Orion is a an extremely hot blue supergiant about 100 times bigger than our sun.
The Solar System
Our Solar system consists of 8 planets orbiting a yellow star or to give it its Roman name 'Sol."
The nearer the Sun the planet is the hotter it will be. Therefore, Mercury is the hottest planet in our Solar System and Neptune the coldest
To provide perspective on the size of our Solar Sytem, you can imagine our Sun as a basketball with Pluto a grain of sand located 1000 metres away.
Pluto, discovered in 1930, has now been re-classified a "dwarf' planet" as it failed to dominate its orbit around the Sun in the same way as the other planets.
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