Satellite flare
This article is licensed under the GNU Free Documentation License. It uses material from the Wikipedia article "Satellite_flare"
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A simulated animation of a typical iridium flare.
Iridium Flare and comet 17P/Holmes
A 30-second exposure of a flare produced by an Iridium satellite.
Iridium flare observed on November 26th, 2006 from Tübingen, Germany

Satellite flare (also known as satellite glint) is the phenomenon caused by the reflective surfaces on satellites (such as antennas or solar panels) reflecting sunlight directly onto the Earth below and appearing as a brief, bright "flare".

Iridium satellite flare

The Iridium communication satellites have a peculiar shape with three polished door-sized antennas, 120 degrees apart and at 40 degree angles with the main bus. The forward antenna faces the direction in which the satellite is travelling. Occasionally an antenna will reflect sunlight directly down to the Earth, creating a predictable and quickly moving illuminated spot of about 10 km diameter. To an observer this looks like an extremely bright flare in the sky with a duration of a few seconds.

Ranging up to -8 magnitude (rarely to a brilliant -9.5)1, some of the flares are so bright that they can be seen at daytime; but they are most impressive at night. This flashing has been some annoyance to astronomers, as the flares occasionally disturb observations and can damage sensitive equipment.citation needed

When not flaring, the satellites are often visible crossing the night sky at a typical magnitude of 6, similar to a dim star.

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