A typical dictionary definition of debris is "the remains of something
broken down or destroyed". To this is often added "ruins, fragments,
rubbish". A more geological orientation may elicit "an accumulation
of fragments of rocks".
Space debris is often thought of as fragments of material moving in
space. While this may be true for natural space debris, it is not
always true for artificial space debris, as we shall see. And space
debris may not always be the result of a destruction or inorganic
catabolism. Although much debris does result from catastrophic processes,
some may occur as the byproduct of another activity. And like weeds,
what some regard as debris others may regard as an opportunity, or even
an artwork.
Natural space debris is ubiquitous throughout the universe. The most
energetic events in space, supernovae, spew enormous quantities of
dust and gas into the interstellar and probably even the intergalactic
medium. Many people regard the resulting nebulae as the most
attractive and colorful of all astronomical sights.
Much closer to home, we might view solar system debris each clear
night when a meteor streaks across the sky. An occasional comet or asteroid
gives us an opportunity to view the larger debris bodies gravitationally
bound to the Sun.
From 1957 man started to add to the space debris population with the
launch of artificial satellites. These spacecraft, at the end of their useful
life, become debris. Launching rockets and other pieces of equipment (such
as shrouds) that remain in orbit are debris peripheral to the main
objective of orbiting a useful space object. Fragmentation of objects,
both derelict and functioning, is another source of man-made or
artificial space debris.
Space debris has not only been created since the start of the space
age, but it (both natural and artificial) has assumed a growing
importance because of the hazard that it may present to man and his
activities on space and even on the Earth itself.
We know little about the interstellar medium and even less about the
intergalactic medium. We do know that the former is filled with large
amounts of dust and gas. Looking in the night sky we can see that
large areas of the milky way are blocked to our view by dust. In
the southern hemisphere there is one very dark small region near the
southern cross that is called the coal-sack. This is due to dust
blocking the light of stars behind it. Although this dust is
augmented and often accompanied by large areas of gas and plasma,
we shall restrict our definition of space debris to macroscopic
particles and leave discussion of atomic and molecular debris
throughout the universe for another discussion.
Although we know nothing about larger bodies (eg meteoroids, asteroids
and comet-type bodies) in the interstellar medium, we believe them
to be present.
In the solar system itself we have two classes of body that are not
only often regarded as debris in their own right, but that also
contribute to the smaller particles (meteoroids) that constantly
pepper the Earth. Comets can be classified into long period and
short period bodies. However, it is believed that all comets
originate from a region known as the Oort cloud, a spherical shell
of space way beyond the orbit of Pluto. Perturbing forces, possibly
due to passing stars, sometimes send comets on highly eccentric
orbits (so eccentric that they can be very accurately approximated
by a parabolic orbit) into the inner solar system. Sometimes such
comets are then perturbed (or captured) into short period orbits
by close passage of a planet (usually Jupiter). Just under 200
short period comets are currently known.
Asteroids are more dense bodies than comets (with typical densities
around 3500 kg/m3) and the majority of them are found in
orbits between Mars and Jupiter, although a significant number have
been found all over the solar system. The current majority theory is that
asteroids are left over fragments from the formation of the solar
system - bodies that never accreted to a size large enough to form
a planet. However, there is some evidence to support the earlier
and minority theory that they are the result of a massive collision
between two or more larger planet sized bodies. Due to recent
concerted searches for asteroids there are currently almost 200,000
objects known in this category.
Meteoroids of all sizes are continually bombarding the Earth. Smaller
sizes are more prolific than larger sizes. Most meteoroids burn up
in the process of traversing the Earth's atmosphere, but a few of
the larger bodies reach the surface of the Earth and are then called
meteorites.
We know that there is a large amount of very fine dust in the solar
system because it scatters sunlight and thus reveals itself in the
zodiacal light. When particles this small (less than a few hundred
microns in diameter) encounter the Earth's atmosphere they do not
burn up. The ratio of their mass to cross sectional area becomes
so small that they are decelerated without undergoing substantial
heating. They then float slowly down, over a period of a few months
to a few years, to the surface of the Earth. It is estimated that
the daily influx of interplanetary dust particles (IDPs) to the
Earth could be around 1000 tons. These particles are known as
micrometeorites.
The above diagram shows artificial debris (often referred to as
orbital space debris) classified according to whether it is a
byproduct of man's space activities (eg booster in orbit) or a fragment
resulting from degradation, explosion, collision or similar event.
However, many workers in the field adopt a much more exhaustive
classification. One such scheme is shown below:
WHAT IS SPACE DEBRIS?
CLASSIFICATION OF SPACE DEBRIS
One possible classification scheme for space debris, both natural
and artificial is shown below:
Space Debris Classification Scheme
Orbital Debris Classification
After "Orbital Debris: A Technical Assessment"'NATURAL' SPACE DEBRIS
ORBITAL SPACE DEBRIS
OBSERVATION AND TRACKING
HYPERVELOCITY COLLISIONS
IMPACT PHYSICS
DEBRIS GENERATION AND EVOLUTION
REENTRY AND PLANETARY ENTRY
COLLISION AVOIDANCE
DEBRIS MITIGATION AND PROTECTION
CURRENT ISSUES
SPACE DEBRIS ORGANISATIONS
SPACE DEBRIS PEOPLE
Internationally recognised for contributions to hypervelocity
research, he helped establish the NASA hypervelocity laboratory
at the Johnson Space Center. His early work was concerned with
development of meteoroid environment models.
An international spokesman for the understanding and
mitigation of orbital debris. He was instrumental in establishing
the NASA Orbital Debris Program Office and one of the guiding
forces in the formation of the Inter-Agency Space Debris
Coordination Committee.
Involved in a diverse range of operational and observational
space debris projects including the (US) Air Force Mauii site (AMOS),
the Liquid Mirror Telescope and the CCD Debris Telescope.
Widely credited with being the first to raise awareness of the future
problems that will result from uncontrolled proliferation of space debris
- through a paper (with Burt Cours-Palais) to the Journal of Geophysical
Research. This paper described the creation of an artificial debris
belt around the Earth that would increase in time to pose a significant impediment
to satellite operations. The "Kessler Syndrome" is a term now used colloquially
to describe this problem.
ACRONYMS
COPUOS | - (UN) COmmittee on the Peaceful Uses of Outer Space | |
ESA | - European Space Agency | |
GEO | - GEosynchronous Orbit | |
IADC | - Inter-Agency Space Debris Coordination Committee | |
IAF | - International Astronautical Federation | |
LEO | - Low Earth Orbit | |
LDEF | - Long Duration Exposure Facility | |
NASA | - (US) National Aeronautics and Space Administration | |
RCS | - Radar Cross Section | |
UN | - United Nations |
JOURNALS
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