The music of the spheres : $b A nature lover's astronomyGrondal, Florence Armstrong
Science
The music of the spheres : $b A nature lover's astronomy
Grondal, Florence Armstrong
Astronomy
Equally dependent are the seven other planets which, with the earth,
whirl in elliptical orbits about this source of heat and light.
"The Sun the seasons of the year supplies
And bids the evening and the morning rise;
Commands the planets with superior force,
And keeps each wandering light to his appointed course."
--_Lucan's Pharsalia._
The planets are sometimes called the "family" of the sun, although his
family also includes the retinue of each planet, which in the case of
six of them at least, consists of from one to ten moons. Our sun is no
different than thousands of other stars in the sky; is it likely that
our star alone of all the countless millions which shine in our
universe, should be the only one to possess this additional charm of
maturity? One looks far out in the darkness to the hosts of radiant
stars--then wonders--how many stars have flocks of planets--how many
travel alone?
THE SURFACE OF THE SUN
Compared to a point of starlight, the disk of our "day star" looks most
exceedingly huge, and this at a distance of 93,000,000 miles. One is
therefore not quite so surprised to learn that this great sunball, which
rests like the hub of a wheel in the center of the solar system, has a
diameter of 886,000 miles. The 8000 miles which measures across the
earth seems quite inconspicuous when compared with such a diameter as
this.
Completely covering the sun's surface is a mass of intensely hot crimson
gases. These gases are like a turbulent upper atmosphere with a depth of
5000 to 10,000 miles. Raging and seething in long tongues of flame, they
swirl up for thousands of miles above the surface, or are thrown far
above it in titanic explosions. Formerly, these burning gases could only
be seen at the time of total eclipse when the black disc of the
moon passed in front of the glaring face of the sun leaving only the red
flames licking out beyond the dark edge. The invention of the
spectroheliograph now makes it possible to photograph these projections
when the sun is shining. One should never try to see them by looking at
the sun unless the glare is shut off either by the moon or by artificial
means, for the sun is so unbearably brilliant that the eyesight of an
observer would soon be ruined.
[Figure 133: SOLAR PROMINENCES.
Huge flames ejected from the surface of the sun, photographed at
Yerkes Observatory with the Rumford spectroheliograph attached
to the 40-inch refractor.]
Public-domain text, read in full here on John Shaqi.
Reviews
Reviews
No reviews yet
Be the first to share your thoughts on this work.
Elsewhere in the archive
Join the Discussion
Join the discussion
Sign in to leave a comment or review.
Sign InorCreate an account