The Moon
Luna
Moon Facts
- The Moon is the only natural satellite of Earth:
- distance from Earth: 384,400 km
- diameter: 3476 km
- mass: 7.35e22 kg
- Called Luna by the Romans, Selene and
Artemis
by the Greeks.
- The Moon, of course, has been known since prehistoric times.
It is the second brightest object in
the sky after the Sun.
- Due to its size and composition, the Moon is sometimes classified as a
terrestrial "planet" along with
Mercury,
Venus,
Earth and
Mars.
- The Moon was first visited by the Soviet spacecraft
Luna 2 in 1959. It is the only
extraterrestrial body to have been visited by humans
(picture 4, 3).
The first landing was on July 20, 1969
(do you remember where you were?);
the last was in December 1972.
The Moon is also the only body from which
samples have been returned to Earth. In the summer of 1994,
the Moon was very extensively mapped by the little spacecraft
Clementine.
- The Moon's rotation is locked in phase with its orbit so that the same side is
always facing toward the Earth.
Actually, the Moon appears to wobble a bit (due to its slightly non-circular
orbit) so that a few degrees of the far side can be
seen from time to time, but the
majority of the far side (picture 2)
was completely unknown until the Soviet spacecraft
Luna 3 photographed it in 1959.
- The Moon is receding away from the Earth at about 3.5 centimeters per year.
The gravitational coupling between the Moon and the Earth in
addition to causing the tides also
transfers rotational energy from the Earth to the Moon.
This slows down the Earth's rotation
(by about 1.48 milliseconds/century)
and accelerates the Moon into a higher orbit (the opposite
effect happens to Phobos and
Triton).
- The Moon has no atmosphere. Recent evidence from
Clementine that suggested that there
might be water ice in some craters near the Moon's poles has turned out to be
inconclusive. But the possibility still exists that ice may exist
mixed with lunar soil.
- The Moon's crust averages 68 km thick and varies from
essentially 0 under Mare Crisium to 107 km north of the crater Korolev
on the lunar farside. Below the crust is a mantle
and possibly a small core.
Unlike the Earth's mantle, however, the Moon's is almost certainly not hot enough
to be molten.
Curiously, the Moon's center of mass is offset
from its geometric center by about 2 km in the direction toward the Earth.
Also, the crust is thinner on the near side.
- There are two primary types of terrain on the Moon: the heavily cratered
and very old
highlands
and the relatively smooth and younger maria.
The maria (which comprise about 16% of the Moon's surface)
are huge impact craters that were later flooded by molten lava.
Most of the surface is covered with regolith,
a mixture of fine dust and rocky debris produced by meteor impacts.
For some unknown reason, the maria are concentrated on the near side.
- In addition to the familiar features on the near side, the Moon also has
South Pole-Aitken
on the far side which is 2250 km in diameter and 12 km deep making it the
the largest impact basin in the solar system and Orientale
on the western limb which is a splendid example of a multi-ring crater.
- A total of 382 kg of rock samples were returned to the Earth by the
Apollo and
Luna programs. These provide most of our
detailed knowledge of the Moon.
They are particularly valuable in that they can be dated.
Even today, 20 years after the last Moon landing,
scientist still study these precious samples.
(picture 18)
- Most rocks on the surface of the Moon seem to be between 4.6 and 3 billion years
old. This is a fortuitous match with the oldest terrestrial
rocks which are rarely
more than 3 billion years old. Thus the Moon provides evidence about the
early history of the Solar System not available on the Earth.
- Prior to the study of the Apollo samples, there was no concensus about the origin
of the Moon. There were three principal theories: co-accretion which
asserted that the Moon and the Earth formed at the same time from the
Solar Nebula;
fission which asserted that the Moon split off of the Earth; and
capture which held that the Moon formed elsewhere and was subsequently
captured by the Earth.
None of these work very well.
But the new and detailed information from the Moon rocks
led to the impact theory: that
the Earth collided with a very large object and that
the Moon formed from the ejected material. There are still details to be
worked out, but the impact theory is now widely accepted.
- The Moon has no global magnetic field. But some of its surface rocks exhibit
remanent magnetism indicating that there may have been a global magnetic field
early in the Moon's history.
- With no atmosphere and no magnetic field, the Moon's surface is exposed directly
to the solar wind. Over its 4 billion year
lifetime many hydrogen ions from the solar wind have become embedded in
the Moon's regolith. Thus samples of regolith returned by the Apollo
missions proved valuable in studies of the solar wind.
This lunar hydrogen may also be of use someday as rocket fuel.
Pictures
- (above) Nice image of full moon
106k gif
the farside
342k gif
Apollo 17 landing site
94k jpg
Buzz Aldrin, second man on the Moon 98k jpg
- The moon
106k gif
- Apollo 17 landing site
291k gif
- GOES satellite image of Earth showing Moon in same frame
92k gif
- Classic image of the Earth and moon, taken from Voyager, low resolution.
35k gif
Earth and Moon taken from Galileo
54k gif;
36k gif
- False-Color mosiac of the moon, showing part of the dark side
94k gif
- Black and white image of the moon showing the North polar regions
153k gif
- Close up view of the north pole of the moon
136k gif
Earth rise over the moon
150k gif
- The east side of the moon (hidden part)
105k gif
- Moon in 2nd Galileo flyby with grid overlaid P-41475
154K gif
Moon from Galileo (unusual perspectives)
38k gif;
13k jpg;
Color image of the Moon from Galileo
62k jpg
Highland Anorthosite, 4.4 billion years old
197k gif
- Apollo images
ftp directory
- Clementine images
ftp directory;
image browser;
a few processed images from usgs
- ... more Moon images
Movies
- Earth-Moon animation
382K fli;
373K pics;
140K quicktime
- Astronauts walking near US flag and lunar lander
118k mpg
- A dramatic view the the moon with Venus in the distance
82k mpeg
- Galileo Moon Encounter
8000k AVI
- Time-lapse sequence of Earth moon system from Galileo
382k FLI
- Clementine images showing the Apollo 16 lunar landing site
212k MPEG
More about the Moon
Open Issues
- Is there water on the Moon? Even small quantities would be enormously valuable
to future astronauts.
- Why are the maria concentrated on the near side?
- Why is the Moon's center of mass off center? Because of the tidal lock with
the Earth?
- Only twelve men have ever on walked the surface of the Moon. Who will be the 13th?
Who will be the first woman?
Express to Mars
... Earth
... Moon
... Mars
...
Bill Arnett; last updated:
1995 September 11