Title: Powers of 10
1Powers of 10
2(No Transcript)
3We see 1/100 of a proton, a representation of a
the quark.
4An even closer look at the array of dots that
comprise the inside of a proton in a carbon atom.
5The inner structure of the proton appears as an
abstract pattern of dots.
6We see individual neutrons and protons that make
up the structure of the carbon atom.
7We see the kernel of a carbon atom, bound by six
neutrons and six protons. This nucleus is dubbed
carbon-12
8We see the atomic nucleus. atom
9We see the innermost electrons of the carbon
atom.
10We see the cloud of electrical charge emitted by
electrons.
11We see our molecular building blocks, a central
carbon atom bonded to three visible hydrogen
atoms.
12In close-up we see the double helix shape of the
DNA strand.
13We see the coiled DNA strands within the cell
nucleus.
14We see the protective membrane inside the
lymphocyte, which encases the cell's nucleus.
15We see inside the capillary vessel to a
lymphocyte.
16We see the thin layers of skin just above the
capillaries.
17We see just below the skin of the man's hand.
18We see the crevices in the skin of the hand.
19A closer look at the hand of the man sleeping at
the picnic.
20We see the picnic at the scale we know best, the
scale of human companionship.
21We see the picnickers from 10 meters away, framed
by the park grass.
22We see the picnic in the park that is the
starting point for the Powers of Ten film. The
picnickers are seen between the highway on the
left and boats on the right.
23From 5/8 mile away, we see more details of
Chicago - boats in their dock, museums, Soldier
Field and Lake Shore Drive.
24The city of Chicago is clearly seen now. We can
make out individual houses, streets and parks
from this distance.
25We see the city of Chicago at the south end of
Lake Michigan
26We can see all of Lake Michigan, formed by
continental glaciers a few tens of thousands of
years ago.
27Measuring in meters, this power of ten is equal
to 10 thousand kilometers. We see the earth in
detail -- sky, clouds, seas and land masses.
28Measuring in meters, this power of ten is equal
to 100 thousand kilometers. The whole earth is
seen from this distance, floating in a sea of
stars.
29Measuring in meters, this power of ten is equal
to 1 million kilometers. This is the length of
the moon's orbit, seen in this image.
30Measuring in meters, this power of ten is equal
to 10 million kilometers. This portion of the
green band we see is the earth's path for four
days in October.
31Measuring in meters, this power of ten is equal
to 100 million kilometers. The portion of the
green arc we see is the Earth's path for about
six weeks each September and October.
32Measuring in meters, this power of ten is equal
to 1 billion kilometers. Within Jupiter's orbit
we see the smaller planets Mars, Earth, Venus
and Mercury.
33Measuring in meters, this power of ten is equal
to 10 billion kilometers. We see the outer
planets as they circulate counterclockwise, all
in nearly the same plane.
34Measuring in meters, this power of ten is equal
to 100 billion kilometers. All of our sun's
planets move in their elliptical orbits marked by
the colored lines in this image.
35Measuring in meters, this power of ten is equal
to 1 trillion kilometers. Our sun is seen clearly
against a background of fainter stars.
36Measuring in meters, this power of ten is equal
to 1 light year. A sky filled with stars, much
like the night sky we view from earth.
37Measuring in meters, this power of ten is equal
to 10 light years. A sky filled with stars, much
like the night sky we view from earth
38Measuring in meters, this power of ten is equal
to 100 light years. We see the bright star
Arcturus and less luminous in the center, our own
sun. The sky is now filled with distinct stars.
39Measuring in meters, this power of ten is equal
to 1,000 light years. We are now looking at the
stars the first astronomers were able to group
into constellations, those within our own galaxy.
40measuring in meters, this power of ten is equal
to 10,000 light years. We see clouds of stars
like dust, one of which is our own sun.
41Measuring in meters, this power of ten is equal
to 100,000 light years. We are looking at a swirl
of a hundred billion stars in our Milky Way
galaxy, all bound to the spiral by gravity.
42Measuring in meters, this power of ten is equal
to 1 million light years. We see the spiral
structure of our own galaxy, the Milky Way. The
two satellite galaxies traveling with it are the
Clouds of Magellan and the Clouds.
43Measuring in meters, this power of ten is equal
to 10 million light years. Each sphere of light
is seen as the result of billions of star light.
These galaxies are within our own cosmic region.
44Measuring in meters, this power of ten is equal
to 100 million light years. We see the The Virgo
Cluster of galaxies, made up of a couple of
thousand galaxies of all sorts and sizes,
circulating in mutual orbit.
45Measuring in meters, this power of ten is equal
to a billion light years. The Virgo Supercluster
of galaxies is seen in the center of this image,
but like most of space, the scene is fairly
empty. Distant galaxies are strung out in
clusters that appear as sprinklings of dust.