The threat to the Sun's astrophere
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Planets such as Earth have atmospheres – stars have astropheres. An astrophere – otherwise termed a heliosphere – is a bubble of solar wind that extends a considerable distance out into space. In the case of our own Sun, this goes to beyond the orbit of Pluto, which used to be the outermost of the Sun’s nine planets before it was decreed that the Sun only had eight!
The astrophere/heliosphere performs a vital function in that it shields all the planets from cosmic radiation that would otherwise damage Earth’s ozone layer and make life extremely difficult if not impossible.
However, we cannot count on the heliosphere being permanent. The Sun is orbited by its planets but it is also in orbit around the heart of the Milky Way, being situated on one of its spiral arms. As it performs this orbit it occasionally encounters dense clouds of dust and gas and these therefore enter the Solar System. When this happens, the solar wind cannot penetrate as far as it once did and the heliosphere contracts as a result.
It has been calculated that when the Sun is proceeding through such a cloud, the limit of the heliosphere could be within Earth’s orbit, thus exposing the planet to external cosmic rays and also dimming the light of the Sun due to the intervening dust, leading to ice ages.
How often does this happen? Estimates vary, but it could be between one and ten times every billion years, meaning that the worst scenario condemns Earth to this hazard once every 100 million years!
However, things would not be so bad if the Sun were smaller and dimmer than it is. Three quarters of all stars in our galaxy are red dwarfs and, in order to be habitable, a planet would need to be a lot closer to its star than is Earth to the Sun. The astrophere of a red dwarf is far more likely to be able to protect its planets from external radiation, whatever the star may encounter, than is a yellow mid-sequence star like the Sun.
So we are all in deadly danger! However, given the immense time sequences involved, the chance of anything of this kind occurring during the lifetime of anyone reading this is extremely remote!
The astrophere/heliosphere performs a vital function in that it shields all the planets from cosmic radiation that would otherwise damage Earth’s ozone layer and make life extremely difficult if not impossible.
However, we cannot count on the heliosphere being permanent. The Sun is orbited by its planets but it is also in orbit around the heart of the Milky Way, being situated on one of its spiral arms. As it performs this orbit it occasionally encounters dense clouds of dust and gas and these therefore enter the Solar System. When this happens, the solar wind cannot penetrate as far as it once did and the heliosphere contracts as a result.
It has been calculated that when the Sun is proceeding through such a cloud, the limit of the heliosphere could be within Earth’s orbit, thus exposing the planet to external cosmic rays and also dimming the light of the Sun due to the intervening dust, leading to ice ages.
How often does this happen? Estimates vary, but it could be between one and ten times every billion years, meaning that the worst scenario condemns Earth to this hazard once every 100 million years!
However, things would not be so bad if the Sun were smaller and dimmer than it is. Three quarters of all stars in our galaxy are red dwarfs and, in order to be habitable, a planet would need to be a lot closer to its star than is Earth to the Sun. The astrophere of a red dwarf is far more likely to be able to protect its planets from external radiation, whatever the star may encounter, than is a yellow mid-sequence star like the Sun.
So we are all in deadly danger! However, given the immense time sequences involved, the chance of anything of this kind occurring during the lifetime of anyone reading this is extremely remote!
soncee › Fantastic sky
indexer › @soncee Not my picture! However, it does show you just how vast the Milky Way is. On the other hand, you have to remember that our view in the Northern Hemisphere is looking outwards - away from the centre - but in the Southern Hemisphere they look inwards towards an even greater accumulation of stars.
