A Speedy Comet
Events in the universe are usually measured along scales of millions or billions
of years, so most of what humans observe in the night sky seems constant. Perhaps
that is why comets have always fascinated astronomers. Their relatively rapid
orbits around the Sun result in a visible change from one night to the next.
Comet 103P/Hartley (Fig. 1) is a small, faint comet that orbits
the Sun approximately once every 6.5 years. Because of its close approach to
Earth during October 2010, its motion against the stars could be observed during the
same night. The fortuitous combination of this close approach and clear skies
on two weekend nights (i.e., not having to worry about waking up for work the next
morning) provided an ideal opportunity to capture the comet's motion
photographically (Fig. 2).
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Technical Notes
- Camera: Canon 5D Mark II digital SLR camera with Canon 70-200 mm f/2.8 telephoto
zoom lens (zoomed out to 200 mm) and Canon 1.4X teleconverter, effective aperture f/4.
- Telescope mount: camera mounted directly on Losmandy GM-8 equatorial mount with
digital clock drive, tracking unguided.
- Exposure: sequence of 8 exposures of 28 s at ISO 3200 (Fig. 1) and 210 exposures of
60 s at ISO 1600 starting every 2 min (Fig. 2).
- Processing: aligned and stacked with Nebulosity program (Fig. 1); color correction,
contrast adjustment, and cropping with Photoshop; time-lapse frames assembled with
Quicktime 7 (Fig. 2).
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