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Active July 23-August 20
Radiant RA 03h 04m Dec +58°
The
undoubted stand-out for meteor observers in the summer of 2007 is a
very favourable return of the Perseids, peaking on Aug 13d 02h UT in
dark, moonless skies. At this time, just as dawn is approaching for
observers in the British Isles, the Perseid radiant will be high in the
eastern sky and from locations away from artificial light pollution
rates of around a meteor per minute should be attained. In most years,
the Perseids produce corrected ZHR around 80 at maximum, with rates at
half that level on Aug 11-12 and 13-14. Indeed, watches on any night in
the 10-day interval centred on Perseid maximum are likely to be very
productive for the patient observer: this is a great time for new
observers to try their hand at meteor work!
All else being equal, best
rates are found when the Perseid radiant – near the ‘Sword Handle’ on
the Perseus-Cassiopeia border – is highest in the sky during the
pre-dawn hours. Even in early evening, however, the radiant is already
quite favourably placed:
Local Time (53oN) Radiant Altitude Local Time Radiant Altitude
21h 28.1° 01h 52.8°
22h 32.8° 02h 59.3°
23h 38.4° 03h 67.1°
00h 44.7°
Observers
should bear in mind the nightly eastwards ‘drift’ of the Perseid
radiant e to Earth’s orbital motion. In early August, the radiant is 15
degrees west of its position at maximum (given above), to the north of
Andromeda.
New Moon falls on August 12, and the Perseid maximum night
of Aug 12-13 (a Sunday to Monday) will be free from lunar interference.
Productive watches become possible from about Aug 6-7 onwards, with the
waning crescent Moon retreating into the morning sky and rising later
from night to night.
Perseid meteors are produced by debris from Comet
109P/Swift-Tuttle. Incoming meteoroids have atmospheric entry
velocities of 60 km/s, resulting in very fast meteors. A healthy
proportion of Perseids are bright, making the shower a good target for
photography. Perseids brighter than about magnitude 0 can be captured
at film speeds of ISO 400 or greater with a camera fitted with either a
50 mm standard lens or 28 mm wideangle lens at f/2.8 or faster, using
time exposures aimed towards Cygnus or the Square of Pegasus. These
need not be driven – ‘static’ cameras yield images with meteors
appearing as longer streaks cutting across the short arcs of star
trails. Users of conventional film can try exposures of 10-15 minutes’
duration. Some observers enjoyed success with digital exposures of 30
seconds’ duration in 2005: obviously, these demand availability of
sufficient memory as a night’s operation may amount to as many as 500
images!
Being fast meteors, Perseids – particularly the brighter examples – often leave behind persistent ionisation trains.
As one of the year’s most consistent very active showers (alongside the
Quadrantids and Geminids), the Perseids justifiably enjoy favour with
even casual observers. The 2005 return was well-observed from the UK,
showing a typical strong peak with ZHR 70-80 and the usual abundance of
bright events. It appears that the enhanced Perseid activity attending
the 1992 perihelion return of the parent comet is now behind us, but
the shower’s regular, fairly dependable performance makes this a
continued highlight of the meteor observer’s year. Circumstances of the
shower could hardly be more favourable for the UK in 2007, both in
terms of the absence of moonlight, and the timing of maximum: observers
should make the most of this opportunity – moonlight will severely
restrict viewing in 2008.
Observations of these, and other
less-active showers, together with sporadic activity, will be welcomed
by the Meteor Section. Observing instructions can be found on the
website at http://www.britastro.org/meteor
Send reports and enquiries to the Meteor Section Director:
Neil Bone, ‘The Harepath’, Mile End Lane, Apuldram, Chichester, West Sussex, PO20 7DZ
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