HMS Endurance Visit and Learn Project

Welcome to the Visit and Learn Website

Together we will track HMS Endurance on her 2006/2007 deployment to Antarctica....
Topical Factfiles
Introduction
World Environment Day
A World of Slavery
Volcanoes
Falklands Conflict Remembered
Polar Clothing
Ice, Ice & More Ice
Tourism in Antarctica
Climate Change
Who Owns Antarctica ?
Endurance Obituaries
Ernest Shackleton
Polar Quest
The British Antarctic Survey
History of Antarctic Exploration
Whales & Whaling
Surveying in Antarctica
Discovery & Exploration
Southern Ocean Life
Glaciers and Glaciation
Remembrance Day
Energy and Resources
Latitude and Longitude
Ecosystems
Weather Presentations
Weather
Oceans & Water
About HMS Endurance
The Suns Energy

Did you know that our Sun is actually a star? Because stars vary in size, temperature and colour, Astronomers have catagorised stars so they can distinguish between them. Astronomers call the Sun a dwarf star and in common with other stars, it is actually a huge ball of very hot gas. It has been estimated that the Sun is nearly 1,400,000 km across, with a surface temperature of about 5,500ºC.

The Sun produces its energy from within its centre or core, where the pressure is enormous and the temperature is thought to reach 15 million ºC. Here, atoms of hydrogen gas fuse (join together) to form helium, another gas. This process of fusing together actually creates a nuclear reaction and it is this process that creates the enormous amounts of energy the Sun has. From the core, currents of hot gas carry the energy to the surface of the Sun where it escapes into space as light and heat.

REMINDER: NEVER LOOK DIRECTLY AT THE SUN. IT'S LIGHT IS SO BRIGHT THAT IT WILL DAMAGE YOUR EYES OR POSSIBLY BLIND YOU.
Oceans & Water Navigation
Quick Facts
How Weather Works
The Atmosphere
Day to Day Changes
The Power of the Sun
The Suns Energy <<
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Met Office Velux 5 Oceans Scott Polar Institute
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