The rules* say they gotta fall in my/our** favor eventually, right? Because it’s getting to be about time to do so…***
The Perseids meteor shower is predicted to peak the night of August 12th and morning of the 13th, precise time about 03:00 UTC on the 13th, which places it as 11 PM on the 12th for those of us on the east coast of the US. ‘Peak’ is often a very broad term in meteorology, uh, meteoronomy, shootingstaragy, whatever – activity may be very strong or barely any noticeable difference during such showers, and may last from a half hour to a few days, and may not even be all that close to that time. On average, more meteors are visible at peak times – usually, often enough, though it only takes a couple of more meteors to skew an average in this manner. Math isn’t going to help us out much here.
What may help us out significantly is that there will be no moon in the sky at all during the night – in fact, it will be eclipsing the sun over in Europe not long before. Also, this peak time (for EDT timezone anyway) falls right before meteors tend to become more visible, which is after midnight. S’okay, the Earth rotates, right? And it also trundles in a big circle around the Sun, in a plane that largely coincides with the rotation. This means that, every day, any point on Earth is either facing into the wind of its orbit, turning against the orbital motion, or falling behind and thus moving in accordance with this motion. Since meteor showers come from passing through a trail of debris left behind by comets as they orbited the sun in their own manner, ‘facing into the wind’ means the path of the Earth and the rotation double up to increase the speed of intersecting dust, making meteors brighter and more frequent, but shorter. At any local midnight, the point on Earth where we stand starts ‘facing into the wind,’ so meteors increase, though we may not be in the thickest part of the debris trail just then. Conversely, before that time, meteors may be much fewer, but also last longer since their speed is slower relative to the Earth.
The debris trail is large enough that the shower may last several days, so whatever clear night you have surrounding that date, go for it. At least this one is during the summer for the northern hemisphere, so you shouldn’t have to bundle up, unlike far too many of the other showers.
Where to look? Seriously, any place the sky is dark enough – it’s a debris trail, it’s scattered and messy, so meteors might appear anywhere in the sky, but your better bet is someplace where other light is minimal and thus you can see more of the dimmer ones.
Now, the radiant is between the constellations Perseus and Camelopardis, just south of Cassiopeia, which at peak time will be medium low to the northeast for mid-latitudes US – lower for southerners, higher for northerners. But the radiant is another average thingy – it means that, if you traced all the trails of the meteors you see during a shower, they would favor lines that point towards the radiant – indeed, that’s about where the bulk of the debris trail lies. That doesn’t mean you’ll necessarily see more if you look there, only that most of the paths converge there – you might see them anywhere (well, in the sky at least,) and the slower ones more away from that point, so again, wherever you have the best visibility.
How to photograph them? Well, you’re asking the wrong guy, because my luck has been abysmal in this regard – up until this storm, right? Anyway, camera on tripod, focus on infinity (I often use the lights on radio towers to focus on when they’re available, since they’re bright enough and far enough away.) Turn autofocus off so it doesn’t keep trying to focus on those dark skies every time you trip the shutter. A remote release is recommended, and an intervalometer can help automate the shutter releases so you don’t have to do it manually. Shutter speed and aperture are going to be guided by the light in the sky, so test exposures are in order. The longer the shutter is open, the more chance you have of capturing a meteor, but also, the more residual light is admitted, brightening the sky, and the longer the star trails will become, making meteors harder to see. So start with ISO 400 or 800 (too high produces noise, especially in long exposures,) f5.6 to f8, 20 seconds shutter speed. Take a look at the resulting exposure – you should have plenty of stars visible but the background should not be very bright. Note, too, the closer you aim towards the North Star/Polaris, the shorter your star trails will be, and the longer your exposure before they get too streaky. Adjust as needed.
The more sky you can see, the better, but bear in mind, the shorter the focal length (the wider the view,) the shorter and less-noticeable the meteor trails become. I’d suggest 18-50mm (or equivalent.) Having a foreground interest makes for much better images, so pick a lake, find that dark old house or tree, that mountain peak – try for what would be scenic in daytime. You have a few days to think about this or scout locations, especially to see how dark it gets at night. Also, aiming away from commercial airline paths is much better, but these taper off seriously after 10-11 PM locally, in most locations (we sit directly under a major N/S route here, so I’m always ending exposures before aircraft enter the frame – red and white lines add absolutely nothing to the image.)
Don’t chase them. You may see a meteor or two in a particular direction, which is not where you’d aimed or the darkest sky. This doesn’t mean this is the spot to see them – they occur everywhere. Just be consistent, since the more time you’re adjusting the camera, the more time you’re not photographing. Believe me, you’re fairly likely to see one blaze outside the field of view of the camera, because the field of view is fairly small no matter what. This is the primary frustration of meteor storms: if you see nothing, well, bad night, but if you miss one, you’re more annoyed. It can happen easily, and there’s no good way to combat it except having a lot more cameras running simultaneously – which isn’t a bad idea, but it means more attending to them and less sky-watching. Better to at least witness that spectacular meteor.
Also, I’ve done a page explaining how to edit out the sensor noise from long exposures, those persistent pixels that occur because of small imperfections of the camera. This doesn’t remove all noise, but it gets those bright annoying pixels out of there.
So, good luck with it, should you decide to try your hand. As always, my brilliant successes will be available here.
* There are no ‘rules’ of averages, just statistics.
** You may have been having far better luck than I.
*** See asterisk one – there is no ‘due.’ Also, witnessing over 300 the night of the 2001 Leonids may have completely fucked my own personal averages, and I’m not due for any more…


























































Knowing it’s in good shape? There’s no easy test (especially if there are no batteries handy,) but check the movement of the settings and the lens rings, look for excessive wear or evidence that it wasn’t stored well, like unclear glass or mildew residues, especially in the finer cracks of the body where people’s cleaning efforts often miss. If the camera is working, set for 1/2 second shutter speed, preferably with a lens attached and set to f16, and trip the shutter a few times. The double-click of the shutter opening and closing should be consistent and easy to time by ear, and you should see the aperture quickly close down and open again each time – these are the things that tend to stick if improperly stored.
What film? Depends on what you want to do. The common print films are not only the easiest to find, you’re more likely to find places to develop it and make prints. The quality, however, tended towards the lower end, and the longevity, even with proper storage, was never that good. One thing to know is, film not only ages, it’s susceptible to heat, so the rolls someone finds in an old camera bag are not going to produce the same results as new. Should you find someone clearing out their stock that they maintained in a refrigerator or freezer, however, go for it. And you can still buy it new.





















You might think you wouldn’t need exposure compensation when the sky is right around that 18% grey middle tone that meters are calibrated for, but the key factor is, the sky is significantly brighter than the subjects against it, especially without direct light on them to brighten them up a bit, so without compensation, the frames were looking like this. And yes, the sky looks exactly the same hue as above – the overcast is never perfectly uniform, so the frame at left was actually brighter than the frame above, since the frame above has been lightened by 2/3 of a stop; the difference is plainly visible in the osprey. This is exactly why exposure compensation is usually linked by default to the dial that sits under your thumb, so this can be adjusted on the fly as you might switch from aiming into the sky to aiming against dark foliage – you just have to remember to keep adjusting this compensation, better than I did for this frame.



