A Bad Time for Flares but a Good Time for Debris

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A Bad Time for Flares but a Good Time for Debris
Number: 111
1st Author: William Pesnell
2nd Author:
Published:
Next Nugget: 112
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Introduction

During the current solar minimum the Sun has had few sunspots, irradiances are at measured lows, weak magnetic fields are measured throughout the heliosphere, and very few flares are being seen. What do we have plenty of? Orbital debris!

The breakup of five satellites in low-Earth orbit (LEO) has significantly increased the number of objects tracked by NORAD. With low solar activity for the past several years, the thermosphere of the Earth has contracted, reducing the frictional drag force that normally cleans some of this debris.

One satellite, the Fengyun-1C, was deliberately destroyed in January 2007, leaves about 2630 pieces still in orbit. A unique event, the collision of Iridium 33 with Cosmos 2251 in February 2009, left 1120 pieces of debris in orbit. Two other breakups left pieces in LEO, the explosion of an Arabsat Briz-M booster on February 2007 (67 pieces tracked, many others untracked) and the breakup of Cosmos 2421 for unknown reasons in March 2008 left at least 40 objects that are still in orbit. In only two years almost 4000 pieces of debris were injected into the already crowded environment of low-Earth orbit. Because there are typically 10,000-20,000 objects being tracked in LEO, the breakup of these five satellites increased the number by 20-40%!

The orbital lifetime of these objects increases with decreasing solar activity. NASA’s Orbital Debris Program Office says some of this debris would fall out of orbit in about five years if solar activity returns to the levels of Solar Cycle 23 but if solar activity remains low it could remain aloft for many more years. The current lack of solar activity means the Sun is dimmer in the extreme ultraviolet, which allows the thermosphere to cool and decreases the atmospheric density. Satellites and debris in LEO then see a smaller frictional drag force. The drag force tends to first make the orbit of the object more circular by decreasing the apogee and then contracts the orbit until it falls out of orbit.

Unless they are carefully crafted, satellite orbits precess around the Earth. This means the orbital elements change in well-understood ways. You can obtain Two-Line Elements that describe how the orbits of most satellites move in space. Here is RHESSI’s TLE for September 2009:

RHESSI

1 27370U 02004A 09255.68332445 .00000190 00000-0 22237-4 0 1386

2 27370 38.0400 351.8236 0015470 241.3408 118.5797 15.02191210416891

Although I won’t explain all the terms, the finite number of digits in each parameter limits the accuracy of predicted close approaches between satellites. Timing errors of several seconds result in several km of uncertainty in the predicted trajectory. After an explosive on-orbit breakup, debris moves into new orbital elements. It is lofted to higher apogees and lower perigees. The inclinations are almost randomized, with some of the debris moving into retrograde orbits.

RHESSI is currently at an altitude of about 550 km (a loss of about 40 km since launch.) It is below most of the orbits where the destroyed satellites orbited, but that does not protect from debris. Pieces of Cosmos 2251 moved into orbits with perigees below RHESSI.

Conclusion

We may forget this solar minimum when sunspots and active regions reappear but the debris will be there for years to come. An increase in the lifetime of orbital debris is a natural consequence of solar minimum. But a radical increase in the number of debris objects is not normal. We should protect our assets in space by cluttering LEO no more than is necessary to place satellites in orbit and maintain their usefulness.

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