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Space Debris: Assessing The Risk

Date:
March 28, 2005
Source:
European Space Agency
Summary:
Assessing the risk that space debris pose to operational spacecraft and satellites is a challenge and depends on whether you are worried about being hit by a known, tracked debris object or by an unknown object. At least the known objects are, well, known. These include old spacecraft, other satellites, rocket bodies and large fragments from past break-ups.

Front view of penetration of Hubble Space Telescope (HST) solar array. Clear hole size: 2.5 mm. The HST solar array was retrieved in March 2002 after 8.25 years in space.
Credit: European Space Agency

Assessing the risk that space debris pose to operational spacecraft and satellites is a challenge and depends on whether you are worried about being hit by a known, tracked debris object or by an unknown object. At least the known objects are, well, known. These include old spacecraft, other satellites, rocket bodies and large fragments from past break-ups.

"It's now standard practice that near-Earth satellites carry an allowance of fuel simply for taking evasive manoeuvres during the craft's operational lifetime," says Dr Heiner Klinkrad, a debris specialist at ESOC in Darmstadt, Germany.

Small objects, big threat

However, assessing the risk due to smaller debris objects and meteoroids is an entirely different matter, as these are difficult or impossible to track.

Smaller debris range from microscopic particles of dust, which are relatively harmless, up to objects about 1 cm in diameter. Objects in this range are a threat, but protective shielding, including Whipple Shield technology, is sufficiently robust to defeat these. Shielding, however, can only be used on some missions, such as the International Space Station (ISS).

Deadly objects in 1- to 10-cm range

Objects from 1 to 10 cm in size cause the real worry. These are too small and numerous to be individually tracked but could cripple or kill any craft they hit.

To assess risk in the deadly 1- to 10-cm range, scientists at ESA and other space organizations use sophisticated probability models and software. Risk is predicted based on a spacecraft's cross-sectional area, its orbital altitude and flight path and other factors.

For example, for a satellite with a 100-m2 cross-sectional area (including solar panels) orbiting at 400 km altitude, the mean time between impact with a debris object 10 cm in size has been calculated to be on the order of 15 000 years.

Collision events once per decade

While this figure may at first glance seem comfortably large for any particular satellite, there are many satellites in orbit. "If you calculate the combined profile area of all satellites in orbit, you find that the average time between destructive collisions is about 10 years," says Klinkrad.

Considering that even a single 10-cm debris collision event could wipe out a multi-million-Euro spacecraft or hit the (manned) ISS, a risk of even one impact per decade suddenly becomes very serious.

Destructive collisions do happen

In 1993, the first servicing mission found a hole over 1 cm in diameter in a high-gain antenna mounted on the Hubble Space Telescope.

In July 1996, France's Cerise military reconnaissance satellite was struck and severely damaged by, ironically, a catalogued Ariane upper-stage explosion fragment; a 4.2-metre portion of Cerise's gravity gradient stabilisation boom was torn off.

Will there be more collisions in the current decade? Nobody can predict with certainty, but it is obvious that steps toward mitigation are required.

ESA space debris research

In addition to a debris warning system developed at ESOC, additional ESA space debris research is done at the European Space Research and Technology Centre (ESTEC), in The Netherlands, mainly focusing on the space segment. Activities include:

* Development and deployment of impact detectors

* Development and testing of shielding designs

* Support for shielding design verification

* Impact analysis of retrieved hardware

* Assessment of impact damage

ESA is not the only organization working on space debris. Dr Toshiya Hanada, Associate Professor at Kyushu University's Department of Mechanical and Aerospace Engineering, located near Fukuoka, Japan, works on developing optical sensors that can scan satellite solar arrays for signs of impacts and on modelling the debris field.

Dr Hanada's research team pays particular attention to geosynchronous Earth orbit. "We have developed an orbital debris evolutionary model for geosynchronous Earth orbit and conducted low-velocity impact tests, below 1.5 km/s, to model these impacts on spacecraft in GEO," he says.

Clearly, the debris issue has grabbed global attention.

Risk assessment software on tap

Back at ESOC, Dr Klinkrad explains the risk assessment software that ESA and a contractor team have developed. It is called DRAMA, for Debris Risk Assessment and Mitigation Analysis, is freely available to the space community and can be used to assess the risk of a catastrophic impact for any specific mission.

Despite such tools, the space-debris situation is unlikely to improve unless concentrated, coordinated and systematic steps are taken to mitigate the risks that are now so clearly understood.

Spacecraft operators must avoid deliberate and unintentional break-up of their craft including deliberate and unintentional explosions or collisions, as these are the major sources of untrackable yet deadly debris.


Story Source:

The above story is based on materials provided by European Space Agency. Note: Materials may be edited for content and length.


Cite This Page:

European Space Agency. "Space Debris: Assessing The Risk." ScienceDaily. ScienceDaily, 28 March 2005. <www.sciencedaily.com/releases/2005/03/050325161759.htm>.
European Space Agency. (2005, March 28). Space Debris: Assessing The Risk. ScienceDaily. Retrieved September 3, 2014 from www.sciencedaily.com/releases/2005/03/050325161759.htm
European Space Agency. "Space Debris: Assessing The Risk." ScienceDaily. www.sciencedaily.com/releases/2005/03/050325161759.htm (accessed September 3, 2014).

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