What would the world be, once bereft of wet and wildness?
Let them be left, O let them be left, wildness and wet;
Long live the weeds and the wilderness yet.
-- Gerard Manley Hopkins
Wednesday, December 14, 2005
our friend, mr. sun
"Just remember that you're standing on a planet that's evolving
And revolving at nine hundred miles an hour,
That's orbiting at nineteen miles a second, so it's reckoned,
A sun that is the source of all our power.
The sun and you and me and all the stars that we can see
Are moving at a million miles a day
In an outer spiral arm, at forty thousand miles an hour,
Of the galaxy we call the 'Milky Way'.
Our galaxy itself contains a hundred billion stars.
It's a hundred thousand light years side to side.
It bulges in the middle, sixteen thousand light years thick,
But out by us, it's just three thousand light years wide.
We're thirty thousand light years from galactic central point.
We go 'round every two hundred million years,
And our galaxy is only one of millions of billions
In this amazing and expanding universe.
The universe itself keeps on expanding and expanding
In all of the directions it can whizz
As fast as it can go, at the speed of light, you know,
Twelve million miles a minute, and that's the fastest speed there is.
So remember, when you're feeling very small and insecure,
How amazingly unlikely is your birth,
And pray that there's intelligent life somewhere up in space,
'Cause there's bugger all down here on Earth."
Actual information: 'This animation of the sun was created with images from the Solar and Heliospheric Observatory (SOHO). These particular images were gathered by an EIT (Extreme Ultraviolet Imaging Telescope), which takes pictures of the Sun, capturing different wavelengths of the ultraviolet light it emits.
Viewing the Sun at different wavelengths allows scientists to study various parts of the Sun, different elements that the Sun is made of, and the Sun at different temperatures. This particular collection of EIT images was from viewing the Sun at a wavelength of 284 Angstroms. At this wavelength we are seeing ions of iron (Fe XV) in active regions of the Sun, or areas of high temperature and much solar activity. You can see in the animation there are constant explosions happening on the surface of the Sun, and that the space immediately around the Sun is very hot.'