Sunshine Photos



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Sunshine Sunshine Sunshine Sunshine Sunshine Sunshine Sunshine - The Sun does not have enough mass to explode as a supernova. Instead when it dies it will first start to swell up to become a red giant and will grow so large that its outer layers will reach the position of the Earth's orbit. After that it will colla Sunshine - The temperature of the Sun varies from 5800K on the surface to 15,600,000K at the core. The outermost layer of the Sun, the corona, is between 1-2,000,000K. Though its temperature is high, its particle density is so low that it releases little heat. If a Sunshine - Akhenaten, the 'heretic' pharoah, changed almost 2,000 years of Ancient Egyptian polytheistic religion when he banned the worship of any God or Goddess other than the Sun disc Aten. He, his wife Nefertiti and his daugheters were depicted worshippi Sunshine - The Sun emits a low density stream of charged particles known as the solar wind which travels 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 Ear Sunshine - Direct viewing of the Sun with the naked eye delivers about 4 milliwatts of sunlight to the retina, heating it up and potentially damaging it. Image courtesy of SOHO (ESA & NASA). Sunshine - The Sun is a second-generation star, perhaps formed from the remains of a previous supernova as there's a high abundance of heavy elements such as iron, gold, and even uranium in the Solar System. The most plausible ways that these elements could be p Sunshine - Sunspot activity isn't constant. 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. I Sunshine - The distance from the Earth to the Sun is 149,570,000 km. Image courtesy of SOHO (ESA & NASA). Sunshine - The Sun is personified in many mythologies: the Greeks called it Helios and the Romans called it Sol. Image courtesy of SOHO (ESA & NASA). Sunshine - The rotation rate of the Sun is 25.4 days at the equator, 36 days at the poles. Image courtesy of SOHO (ESA & NASA). Sunshine - About 74% of the Sun's mass is hydrogen, with 25% helium and the rest made up of trace quantities of heavier elements. Image courtesy of SOHO (ESA & NASA). Sunshine - The Sun contains more than 99.8% of the total mass of the Solar System. Image courtesy of SOHO (ESA & NASA).

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