Here is August and here is the best summer meteor shower – the Perseids. This year combines a very favourable Moon phase at the shower’s peak with an expected outburst in activity! ZHR may reach as many as 200 meteors per hour! Excellent prospects for meteor observers. Here are the details.

Perseids 2016 LIVE!

Perseids at a glance

The Perseids are one of the strongest annual meteor showers. As most other meteors, the Perseids are caused by small dust particles called meteoroids. Meteoroids usually originate from comets. As a comet revolves around the Sun it periodically heats up and ices on its surface begin to sublimate, releasing tiny mineral grains and clumps which were trapped in the ice. During tens to hundreds of successive revolutions around the Sun, a comet produces a long stream of meteoroids. If the Earth passes through this stream, meteoroids bombard our atmosphere, hitting it at tens of kilometers per second and creating beautiful streaks of light we know as meteors.

The Perseids are caused by the meteoroids from the periodic comet 109P/Swift-Tuttle, which revolves around the Sun every 130 years. The Perseids have been observed for centuries, but were officially recognized as a major meteor shower in the middle of the 19th century. They have been regularly observed for the past 150 years and are best known for a series of strong outbursts in the first half of the 1990s, which reached ZHRs up to about 500 meteors per hour.

Perseid meteoroids hit our atmosphere at 59 km/s, so the Perseids are swift meteors and often very colorful. Many brighter shower members leave persistent trains. Fireballs may leave persistent trains that last for tens of seconds or even minutes! Interestingly enough, the meteoroids that cause ordinary bright Perseids are only a few millimeters across! Even the meteoroids that produce fireballs are only centimeters across.

Perseids 2016 – an outburst and enhanced overall activity?

The 2016 Perseids may turn out to be something special – offering two nights of enhanced activity compared to the usual annual peak. The annual peak is expected on August 12 between 13h and 15h30 UTC with ZHR~80-100. Predictions by a number of independent teams indicate several outbursts as well as enhanced activity overall.

  • NASA (Cooke & Moser, 2016): a major outburst with a peak ZHR of ~210 is expected just past midning UTC on August 12, caused by meteoroids in the 1 and 4 revolution old trails, with an additional enhancement around 4h UTC by 7-rev trail meteoroids. The second maximum coincides with the annual peak, caused by 12-rev meteoroids, enhancing the peak rate by 30-40% to ZHR ~130. Details here.
  • Vaubaillon: indicates the Earth will cros the 2-rev trail on August 12 between 0 and 4h UTC, enhancing the rates.
  • Maslov and Lyytinen: indicate the Earth will cross a denser part of the Perseid meteoroid stream shifted closer by Jupiter this year. Expected ZHR of the annual peak is 150-160. An additional enhancement by ZHR about 10 is expected by the 1-rev trail late on August 11, centered on 22:34 UTC.

How to observe the Perseids?

The Perseids all appear to radiate from (fly out of) a point – the radiant – in the constellation of Perseus. The radiant drifts eastward each successive night. At the beginning of the shower’s activity it is located in the western part of Cassiopeia, drifting through it and into Perseus by early August and towards the border with Camelopardalis in late August. Check the radiant position before observation.

The first Perseids appear in mid July, but the shower begins picking up strength in the first week of August. By August 7 you may be able to see about 10 to 15 Perseids per hour just before dawn, if your sky is dark. By August 10 the rate increases to about 20-30 Perseids per hour. The peak is reached on August 11/12! The numbers then decline by half every night, so the night after the peak you may see about 40-50 meteors per hour and on August 14/15 there will be about 25-30 Perseids per hour. The final Perseids may be seen around August 25. These rates are expected under dark skies – light pollution will diminish the number of meteors significantly. But the rate also changes during the night. As the radiant rises, so does the number of meteors! The radiant is at its lowest during the evening hours and climbs high in the sky in the morning. The final hour before dawn will usually produce the most Perseids. So do persist until dawn!

Position of Perseid radiant on August 12 at 3 am from 45°N, looking east.

Position of Perseid radiant on August 12 at 3 am from 45°N, looking east.

To observe the Perseids, you need to dress warmly, bring a reclining chair and watch the sky. You need no other equipment. Find a dark observing spot, preferably with a low horizon and look in any (the darkest) direction. Use this light pollution map to find dark locations near you. Also remember that the Perseids are not the only active meteor shower in this period. Other active showers include the Kappa Cygnids, Southern delta Aquariids and Alpha Capricornids. Check the 2016 IMO Shower Calendar for more information.

But you can also contribute valuable observational data! If you decide to do so, use the IMO major meteor shower observing technique. This way your data will be in a standard format, that can readily be used for analysis. Send us your data as soon after the observations as possible.

How to photograph the Perseids

The first Perseids appear in mid July, but the shower begins picking up strength in the first week of August. By August 7 you may be able to see about 10 to 15 Perseids per hour just before dawn, if your sky is dark. By August 10 the rate increases to about 20-30 Perseids per hour. The peak is reached on August 11/12! The numbers then decline by half every night, so the night after the peak you may see about 40-50 meteors per hour and on August 14/15 there will be about 25-30 Perseids per hour. The final Perseids may be seen around August 25. These rates are expected under dark skies – light pollution will diminish the number of meteors significantly. But the rate also changes during the night. As the radiant rises, so does the number of meteors! The radiant is at its lowest during the evening hours and climbs high in the sky in the morning. The final hour before dawn will usually produce the most Perseids. So do persist until dawn!

Meteor photography is a lot of fun, particularly during a major meteor shower! Chances of photographing a bright meteor are really good. With modern cameras it is also really easy. You will need a photo tripod, a remote/programmable release and a suitable camera. With modern cameras the selection has expanded from DSLRs also to mirrorless and other types of cameras. The only requirements are: good performance at medium to high ISO (>800-1600), a reasonably fast and wide field lens (f/3.5 or faster is preferable). Put the camera on the tripod and aim it at the sky – it does not matter which part, meteors appear everywhere. Set the exposure to at least 15 s, but you can go up to several minutes if the sky is dark or if the lens is slow or if you are using comparatively low ISO. Continue making successive photos throughout the night. On the peak night you are bound to catch some good meteors!

Expect an 18-mm lens at f/3.5 and ISO 1600 to detect meteors down to about magnitude 0, while a 50-mm lens at f/1.4 and ISO 3200 may detect meteors down to magnitude +3 or even +4. Of course to look really good on a photo the meteor must be at least two or three magnitudes brighter.

A final piece of advice to always keep in mind: properly focus the lens – check your focus every once in a while. There is no worse feeling than getting an out of focus shot of a beautiful
meteor! Also bring backup batteries.

When things go right. Jure Atanackov captured this brilliant -9 magnitude Perseid fireball in constellation Cetus on August 12, 2010 with a Nikon D80 camera set to ISO 1600 and an 18-mm f/3.5 lens (100 sec exposure). Such meteors are rare, but the excitement of catching a brilliant fireball is tremendous!

When things go right. Jure Atanackov captured this brilliant -9 magnitude Perseid fireball in constellation Cetus on August 12, 2010 with a Nikon D80 camera set to ISO 1600 and an 18-mm f/3.5 lens (100 sec exposure). Such meteors are rare, but the excitement of catching a brilliant fireball is tremendous!
A -3 magnitude Perseid shoots into Ursa Minor on August 12, 2013 at 23:18 UT. Photo taken by Klemen Čotar from Medvedje Brdo, Slovenia. Nikon D3000, 18-mm f/3.5, ISO 1600, 148 s exposure.

A -3 magnitude Perseid shoots into Ursa Minor on August 12, 2013 at 23:18 UT. Photo taken by Klemen Čotar from Medvedje Brdo, Slovenia. Nikon D3000, 18-mm f/3.5, ISO 1600, 148 s exposure.
A +1 magnitude Perseid in Cygnus on August 12, 2013 at 23:59 UT. Photo taken by Rok Pucer and Jure Atanackov from Medvedje Brdo, Slovenia. Canon EOS 6D, 35-mm f/1.4, ISO 3200, 10 s exposure.

A 1 magnitude Perseid in Cygnus on August 12, 2013 at 23:59 UT. Photo taken by Rok Pucer and Jure Atanackov from Medvedje Brdo, Slovenia. Canon EOS 6D, 35-mm f/1.4, ISO 3200, 10 s exposure.
Almost got away: a -7 magnitude Perseid in Cetus on August 13, 2013 at 1:17 UT. Photo taken by Danaja Dvornik from Medvedje Brdo, Slovenia. Nikon D3100, 10-mm f/2.8, ISO 1600, 69 s exposure.

Almost got away: a -7 magnitude Perseid in Cetus on August 13, 2013 at 1:17 UT. Photo taken by Danaja Dvornik from Medvedje Brdo, Slovenia. Nikon D3100, 10-mm f/2.8, ISO 1600, 69 s exposure.
Not a Perseid! A -8 magnitude sporadic fireball in Taurus on August 11, 2005 at 1:59 UT. Photo taken by Peter Atanackov and Simon Krulec from Trije Kralji na Pohorju, Slovenia. Canon EOS 300D, 21-mm f/3.5, ISO 3200, 41 s exposure.

Not a Perseid! A -8 magnitude sporadic fireball in Taurus on August 11, 2005 at 1:59 UT. Photo taken by Peter Atanackov and Simon Krulec from Trije Kralji na Pohorju, Slovenia. Canon EOS 300D, 21-mm f/3.5, ISO 3200, 41 s exposure.

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