What are Iridium
Flares?
Recently I’ve become obsessed with observing and
photographing Iridium flares. A lot of
people have asked me what they are. I knew the basics, but this question led me
to find out more about them.
Basically, an Iridium flare is when the sun catches the
reflective panel on an Iridium satellite, and this causes it to glint in the
sky. The flare can last anywhere from 5
to 20 seconds and may as bright as magnitude -8; that is 30 times brighter than
Venus! Each satellite has 3 reflective panels, each called a main mission
antenna, which are arranged in a kind of triangular structure and angled at 40o.
Each panel measures just 188cm x 86cm x 4cm but they are highly reflective
aluminium plates which have been treated with silver coated Teflon.
Structure of an Iridium Satellite:
(Image: www.satobs.org)
When in orbit, the satellites are in a vertical position. When
one of the main mission antennae catches the Sun, it produces a bright but
small reflection which projects onto the surface of the Earth. This reflection
is only 10s of kilometres in size, so this means that Iridium Flares are very
location specific.
So what are these Iridium satellites? They are a network of
66 active satellites which are used for worldwide voice and data communication
from satellite phones. This means the
network of satellites needs to provide full global coverage, so their orbits
cover all parts of the Earth. This is called the Iridium Satellite
Constellation” (ISC). The ISC launched
in 1998 with financial backing from Motorola.
Unfortunately they went bankrupt 9 months later, partly due to the huge
costs involved with getting all 66 satellites functional before the satellite
phone network could properly function.
Another factor was that the handsets were very bulky and would only work
outside, therefore the popularity of mobile telephones overtook satellite
phones. At one point it was looking like
the satellites would have to be de-orbited. Fortunately, the scheme was
restarted in 2001 by Iridium Satellite LCC, who later merged with GHQ in 2009
to form Iridium Communications Ltd. The
system was largely used by the US Department of Defence.
The Iridium Satellite Constellation was originally planned
to consist of 77 satellites, the atomic number of Iridium. However, it actually
consists of 66 satellites, in 6 polar low-Earth orbital planes. All satellite calls are routed via space. As
well as communicating with the hand-held devices, each satellite is in communication
with up to 4 adjacent satellites. This effectively forms a mesh network. In addition there are 4 Earth base stations,
which are in communication with any satellites within range. They can only communicate if there is clear
sky between the device and the satellite, therefore they don’t work well
indoors or in areas of dense forest.
Iridium are currently developing a second generation
network, called Iridium NEXT. This will consist of 66 new satellites plus 6
spare in orbit and 9 spare on the ground. These are due to launch in 2015 via
Space X Falcon 9 launchers. Each
satellite will also contain cameras and additional sensors. The current ISC will remain in service until
the NEXT network is fully functional, estimated to be during the 2020s.
There are currently over 8,000 satellites in orbit, around
3,000 of which are defunct. With such
high numbers in orbit it’s hardly surprising that on 10th February,
2009 there was a collision between Iridium 33 and Kosmos 2251. They collided at
a speed of over 26,000 miles per hour!
So how can you observe an Iridium Flare? There are many
flare prediction programs available, either online or in the form of smart
phone apps. I use either www.heavensabove.com
or the SatTrack app. As they are so
location specific, it is necessary to first input your exact latitude and
longitude. Then you will see a list of
upcoming flares, along with their predicted magnitude and exact location in the
sky. If you are very lucky, you may get
multiple satellites glinting at once, producing a double or even a triple
flare. There are some Iridium satellites
which are out of commission and which are tumbling; flares from these cannot be
predicted. The angle of the flare is dependant on the orbit of that particular
satellite. If you want to photograph an Iridium Flare, you need to be
organised. First of all, I manually focus my camera on a bright star or planet.
Then using a remote shutter cable I start the exposure between 10 - 30 seconds
before the peak of the flare (depending on the magnitude) and continue to
expose for the same length of time after the peak. This will give you a really
nice, symmetrical flare on your photo. The
result will depend on how dark the sky is at the time of the flare and will be
affected by moonlight, etc. It took me quite a few attempts before getting decent
results but it was worth persevering!
Some Iridium Flare Photos by
Mary
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