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Following early January’s Quadrantids, the opening months
of the year are generally regarded as a rather thin time for meteor observing,
with only minor shower and low background sporadic activity in evidence. Even the
most dedicated observers find the minimal rates - sometimes only one or two
meteors per hour - in February and early March rather a trial on their
patience.
Virginids
Active March and April
Radiant RA 14h 04m
Dec -09o
13h 36m
-11o
Activity begins to pick up a little from late March with
the arrival of the Virginids. The shower is part of an essentially year-long ‘drizzle’
of meteor activity from close to the ecliptic plane. In common with other
near-ecliptic showers, the Virginids show a split radiant, presumably a consequence
of gravitational perturbations by the planets. Activity comes from radiants in
the Virgo ‘Bowl’, and to the east of Spica, fairly low in the southern spring
sky for UK-based observers. A result of the low radiant elevation is that
Virginid meteors can, on occasion, have long, slow ‘grazing’ trajectories up
from the horizon towards the zenith.
Observed
Virginid rates are typically low, usually no better than 2-3 meteors/hr in late
March and early April. The meteors can, however, sometimes be reasonably bright
by way of reward for the patient observer. Watches in the post-midnight hours
are likely to be most productive, and the dark of the Moon interval from about
28 March until mid-April will be the most favourable time to observe this
low-activity, poorly-covered shower.
Lyrids
Active April 19-25
Radiant RA 18h 98m Dec +32o
Usually, the shower which ‘re-opens’ the more active part
of the meteor observer’s year, the Lyrids are unfortunately-timed in 2008. The
Moon is only three days past Full at their April 21-22 maximum, and rises
before the radiant has really climbed into the northeastern sky.
Eta Aquarids
Active April 24-May 20
Radiant RA 22h 20m Dec -01o
An excellent shower for observers at southerly latitudes,
the Eta Aquarids present a considerable challenge for those in the British
Isles. The shower radiant, near the ‘Water Jar’ asterism in Aquarius, is only
just beginning to climb in the eastern sky as dawn breaks in early May.
Radiant elevation at 53oN
Local Time
Alt
02
3.9o
03
12.8o
04
21.0o
Observations are hampered by the bright twilit skies. By
the time nautical twilight has set in (Sun less than 12o below the
horizon), faint stars and meteors are hard to see; astronomical twilight (Sun
12-18o below the horizon) allows brighter meteors to be seen. The
observing window becomes more limited the farther north one goes:
Latitude Onset
of Twilight (May 4): Astronomical Nautical
57oN
All night 0208
55oN
0052 0229
53oN
0131 0245
51oN
0157 0300
The Eta Aquarids are, like October’s Orionids, produced by
debris shed from Comet 1P/Halley, and are extremely swift meteors, often
leaving short-duration persistent trains. Peak activity occurs over several
nights close to May 4, and observers seeking a challenge might wish to make use
of the last hour or so of darkness on mornings around the Bank Holiday weekend
to obtain watch time on this elusive shower: many very experienced
northern-hemisphere meteor-watchers have never seen an Eta Aquarid! The Moon is
New on May 5, and won’t interfere.
Alpha Scorpiids
Active April 20-May 19
Radiant RA 16h 31m Dec -24o
16h
04m -24o
Ophiuchids
Active May 19-July
Radiant RA 17h 56m Dec -23o
17h
20m -20o
Continuing the near-ecliptic trickle of low activity
through early summer, these two showers offer only low rates for observers
willing to persevere with the permanently twilit skies. As with the earlier Virginids,
the meteors can sometimes be long, slow and reasonably bright as they climb
from the low southern sky.
Capricornids
Active July-August
Radiant RA 20h 44m Dec -15o
21h 00m -15o
July finally sees a significant upturn in overall meteor
activity, including improved background sporadic rates. The Capricornids,
active from early in the month, are a rather poorly-defined shower from the
near-ecliptic region, with possible maxima on July 8, 15 and 26. The first two
of these are favoured by an absence of moonlight in 2008, but observed rates
are never likely to be higher than one or two per hour.
Alpha Cygnids
Active July-August
Radiant RA 21h 00m
Dec +48o
Throughout July and August, a steady trickle of one or two meteors/hr is
reported from an apparently stationary radiant near Deneb, high in the UK
summer sky. In theory, meteor shower radiants should move eastwards by roughly
a degree per day, thanks to Earth’s orbital motion, and there are therefore
some doubts as to whether the Alpha Cygnids are a genuine shower, or simply the
result of observers aligning sporadic activity to a radiant close to a
conveniently bright star.
Late July brings us into the most substantial active
meteor period for the summer, with the combined output of the Delta Aquarids,
Alpha Capricornids, Iota Aquarids, Piscis
Australids and Perseids making for productive watches as the skies begin
to darken once again following the Summer Solstice. The Moon is at Last Quarter
on July 25, and as it retreats further into the morning sky during early
August, observers can look forward to some excellent watches, weather
permitting.
Delta Aquarids
Active July 15-August 20
Radiant RA 22h 36m Dec -17o
23h 04m
+02o
The Delta Aquarids are the most productive of several
showers with radiants south of the Square of Pegasus, still rather low in
British skies on a July-August night. The shower has two branches, the southern
being the more active: peak for this branch is on July 28-29, and shouldn’t be
too badly affected by moonlight (the Moon is a waning crescent, rising around
00h local time) .
Radiant elevation at 53oN
Local Time
D-Aq N D-Aq S
22
14.1o 2.1o
23 22.4o 9.1o
00 29.7o 14.8o
01 38.5o 18.5o
02 38.5o 20.0o
03
38.7o 19.1o 28-29 July
The Delta Aquarids’ northern branch, with its radiant near
the ‘Water Jar’, is better-placed (higher in the sky) for UK observers, and
peaks on August 6-7, with the Moon well out of the way (setting in early
evening).
Radiant elevation at 53oN
Local Time
D-Aq N D-Aq S
22 19.1o 6.4o
23 26.9o 12.7o
00 33.2o 17.2o
01 37.5o 19.7o
02 37.5o 19.7o
03 33.3o 17.5o 6-7 August
Peak Zenithal Hourly Rate (ZHR, allowing for sky
transparency and radiant elevation) for the Northern Delta Aquarids is about
10, perhaps corresponding to observed rates of 5-6 per hour under good
conditions. Most Delta Aquarids are medium-velocity meteors in the magnitude +2
to +4 range; the shower is not particularly noted for an abundance of bright
events.
Alpha Capricornids
Active July 15-August 20
Radiant RA 20h 36m
Dec -10o
Although comparatively weak (ZHR 5), the Alpha
Capricornids are a distinctive shower, producing long, slow meteors which can
sometimes be notably bright. Observers conducting watches in early August can
expect to record one or two ‘Alpha Caps’ per hour, and the nominal peak on
August 2-3 is well-placed with respect to moonlight - the Moon is New on August
1 and therefore won’t interfere. The radiant is close to the wide naked-eye
pair of Alpha and Beta Capricorni, fairly low in the southern sky on an August
night.
Iota Aquarids
Active July-August
Radiant RA 22h 10m Dec -15o
22h 04m
-06o
Like the Delta Aquarids, a shower with a double radiant.
At peak, on August 6-7, the Iota Aquarid radiants lie roughly 10 degrees east
of those of the Delta Aquarids, and care must be taken to distinguish the two
showers. Iota Aquarid meteors are mostly faint and quite swift
Piscis Australids
Active July 15-August 20
Radiant RA 22h 40m Dec -30o
Further complicating the radiant profusion in the low
summer sky, the Piscis Australids are a rather minor stream, producing slow,
long meteors. The radiant’s low altitude from UK locations means that rather few
of these are reported by BAA observers.
Perseids
Active July 23-August 20
Radiant RA 03h 04m Dec +58o
Always the summer’s main attraction for meteor observers,
the Perseids are expected to peak around August 12d 09h UT, making the Monday
night to Tuesday morning of Aug 11-12 probably the shower’s most productive in
2008. Good observed rates can be expected particularly in the early hours after
the waxing gibbous Moon has set (around 23h 20m local time on Aug 11-12). Observers
watching late on Aug 11-12 should experience increasing activity towards dawn: from
a clear, dark location rates of a meteor per minute might be seen in the latter
parts of the night as the shower radiant (near the Double Cluster on the
Perseus/Cassiopeia border) climbs high into the eastern sky. Activity should be
starting to decline by the time darkness falls on Aug 12-13. Moonlight becomes a nuisance after maximum,
but even as late as Aug 13-14 it should still be possible to follow the
Perseids’ immediate decline from peak, with at least a couple of hours of dark
sky between moonset and dawn.
Perseid Radiant at 53oN
Local Time
Altitude
21h
28.1o
22h
32.8o
23h
38.4o
00h
44.7o
01h 52.8o
02h
59.3o
03h
67.1o
Perseid activity is evident as early as the third week of
July. The main part of the shower, including its steady rise through the first
9 days or so of August, will enjoy dark skies. Activity takes a marked ‘kick’
around August 8-9, and watches between this date and August 14-15,
particularly, should be very rewarding.
The Perseids are
associated with Comet 109P/Swift-Tuttle, which was last at perihelion in 1992.
Enhanced activity accompanied that return, and was evident for several years,
up to at least 1997. The 2005 and 2007 Perseids - our most recent well-covered
returns of the shower - proved fairly ‘normal’, with a single sharp peak to ZHR
ca. 80 in 2005 (perhaps slightly lower - ca. 70 - in 2007), and the usual slow
rise to and steep decline from maximum. As always the 2008 return of the shower
requires careful scrutiny on all possible clear nights (and not just at
maximum!).
The Perseids are
well known for the abundance of fast, bright meteors close to their maximum.
Perseid meteoroids enter the atmosphere at a velocity of 60 km/sec, and the
resulting meteors often leave behind persistent ionisation trains.
The large numbers of bright events in the
five-day interval centred on Perseid maximum makes this an excellent target for
photography. Conventional film remains the medium of choice for most observers.
Exposures, which can be with a static (undriven) camera, of 10-15 minutes’
duration, using ISO 400 film and a 50 mm or wideangle 28 mm lens at f/2.8 or
faster, can capture meteors of magnitude 0 and brighter. Ideal aiming
directions are about 20-30 degrees to one side of the radiant at 50 degrees
altitude above the horizon - Cygnus in early evening, the Square of Pegasus
later in the night, or towards the north celestial pole, for example
Observations of any of the above showers, made by the BAA Meteor
Section’s standard methods - outlined elsewhere on these pages - will be
welcomed by the Director.
- Neil Bone
‘The Harepath’, Mile End Lane, Apuldram, Chichester, West
Sussex, PO20 7DZ
(01243) 782679
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