ESA Science & Technology11-Jul-2005 09:56:52
 

Space Weather

Sun-Earth Relationship

About the Sun

The Sun as seen by SOHO on 14 September 1997 in extreme ultraviolet light. The solar prominence, bottom left, has a temperature of some 70  000 °C. The solar corona is hotter than a million degrees Celsius

The Sun is our nearest star. Nuclear reactions deep inside the Sun create the light and heat we need for our survival. Scientists think the Sun was born about five billion years ago. Although the Sun is consuming four million tonnes of hydrogen fuel every second, it is so large that it should continue to shine for another five billion years. By that time, it will have swollen into a red giant, causing the oceans to boil away and destroying all life on our planet.

The Sun's activity varies over an 11-year period. The number of sunspots and flares, and the radiation output, change over time. The most recent peak in its cycle of activity occurred in mid-2000 with a second peak at the end of 2001. Scientists are hoping that the two missions in ESA's Solar-Terrestrial Programme, SOHO and Cluster, will be able to tell them more about how the Sun works and how it affects the Earth. While SOHO studies explosions on the Sun and detects solar storms heading our way, Cluster will measure the effects of this activity on near-Earth space as the incoming energetic particles subject the magnetosphere to a buffeting.

Facts about the Sun

Distance From Earth

149  600  000  km

Diameter

1  392  000  km (= 109 Earth diameters)

Rotation Period at Equator

24.6 days

Surface Temperature

5500 oC

Core Temperature

15  million oC

Mass (Earth = 1)

333  000

Volume (Earth=1)

1  300  000

Gravity (Earth = 1)

27.94

How the Sun affects our planet

The Sun affects our world in many ways. A continuous stream of atomic particles - the solar wind - pours out into space from the Sun at speeds ranging from 300 to 1000  kilometres per second (1800 times faster than Concorde!). Sometimes, explosions on the Sun send millions of tonnes of gas towards the Earth. These clouds of high energy particles can cross the 150 million kilometre gulf between the Sun and Earth in a few days. The most energetic particles of all, created by solar flares, can reach Earth in just 30 minutes.

An aurora: a product of charged particles radiated by the Sun interacting with the Earth's atmosphere

A solar Coronal Mass Ejection (CME) event as recorded by SOHO on 2 June 1998

When charged particles from the Sun enter Earth's upper atmosphere, they create shimmering curtains of coloured light, known as auroras, in the polar night sky. Other effects can be much more serious:

  • Solar storms affect Earth's ionosphere, causing disruption of short wave radio communications, navigation systems on ships and aircraft, and military radar systems
  • Surges in long electricity transmission lines may cause power and widespread blackouts, as happened in Quebec, Canada, in March 1989 when 6 million people were left without electricity due to a huge solar-induced magnetic storm
  • Damage to microchips and electrical discharges may cause satellites to stop operating, causing disruption of, for example, telephone, TV and data communication services
  • Radiation levels can become hazardous to astronauts and occupants of high flying aircraft
  • High energy particles hitting Earth's upper atmosphere can destroy the ozone layer, which protects us from harmful ultraviolet radiation
  • Solar storms have even been blamed for increased corrosion in oil pipelines
  • Solar energy output varies over the 11-year sunspot cycle. This may cause climate changes, which can affect vegetation growth and food supplies

 



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