ALPO Meteors SectionCoordinator: Robert Lunsford |
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Contents:
Viewing Meteor Activity
Since meteors are a transient phenomena one cannot go outside at night and expect
to see meteor activity. This is especially true during the evening hours when the
Earth is moving in the opposite direction from the sky seen above during those
hours. At this time of night meteoroids (meteors in space) must catch up to the
Earth in order to enter the Earth's atmosphere. Therefore meteor rates are lowest
near 1800 (6:00pm) local time. Conditions for viewing meteor activity improves as
the night progresses. At midnight a great majority of the meteors seen strike the
Earth from a perpendicular angle instead of from behind. These conditions offer
better rates than witnessed early in the evening but the general activity is still
low when compared to the morning hours. During the dark morning hours the Earth
is rotating toward the direction it moves in space, known as the apex. During this
time the Earth slams head-on into meteoroids and many more will be seen. This is
much like a vehicle driving through the rain. More raindrops will strike the front
windshield compared to the rear window. The peak meteor activity occurs near 0600.
In addition to the diurnal cycle there are also annual variations in the meteor
activity. As seen from the mid-northern hemisphere the second half of the year
is much more active than the first six months. The reason for this are several.
First of all the sporadic (random) meteor activity is stronger during this period.
Also most of the major annual showers active during the second half of the year
have radiants located north of the celestial equator, favoring northern obserevers.
The cycle seen from the mid-southern hemisphere is opposite with the better activity
occurring during the first half of the year. Observers at the equator enjoy fair,
but not exceptional activity all year long.
During certain times of the year the major meteor showers are active and increase
the nightly activity severalfold. This is especially true if the moon is near its
new phase and not brightening the nighttime sky. The list of these showers is
provided below (see the class I showers).
This is also the best time to see fireballs, which are exceptionally bright meteors
that can light the nighttime scene. These meteors can range from the light of the
brightest planet Venus (magnitude -5) to that beyond the light produced by the
full moon (magnitude >-13).
To keep current on the upcoming meteor activity the Meteors Section invites you
to subscribe to their quarterly newsletter, available for the price of postage
(currently 42 cents per issue). To subscribe contact our section coordinator
Robert Lunsford.
The Taurids are not well known outside the astronomical community. They are not
a strong shower and rarely produce in excess of ten meteors per hour, even at
maximum activity. The Taurids are known for producing bright, often fireball
class meteors during the last half of October and the first half of November.
They appear to move slowly compared to most meteors. The sight of a bright
Taurid, often fragmenting in flight, is unforgettable.
The Taurids are one of the few meteor showers that produce activity all night
long. They are best seen near midnight when the radiant, the area of the sky
where the meteors seem to originate, lies highest above the horizon. The radiant
lies in the constellation of Aries during October and crosses into Taurus in
November. During the time of maximum activity in early November, the large Taurid
radiant is located in western Taurus, just south of the brilliant naked eye star
cluster known as the Pleiades or the Seven Sisters. Any true Taurid meteor will
trace back to this area of the sky.
There are actually two branches of the Taurid meteor shower. A southern branch
peaks a week before the northern branch (November 5) and is located roughly five
degrees further south. Together they can produce 5-10 meteors per hour during the
first two weeks in November. Lesser rates can be seen in October and during the
second half of November. It is difficult to differentiate between the two branches
unless you face directly at this area of the sky.
Occasionally there are years when an extraordinary number of Taurid fireballs
are observed. 2005 was one such year and there are predictions that 2008 may be
another. These events are associated with the parent comet 1P/Encke and possible
concentrations of material that happen to encounter the Earth in these years. We
urge you to monitor the skies for the next two weeks to view the Taurid meteor
shower. If you are lucky then perhaps a brilliant Taurid fireball will light up
the skies above while you are out observing!
Activity Period: the dates when the ZHR (Zenith Hourly Rates) are equal to or greater than one.
Maximum: the date on which the maximum activity is expected to occur.
S.L.: the equivalent solar longitude of the date of maximum activity.
Solar longitude is measured in degrees (0-359) with 0 occurring at the exact moment
of the spring equinox, 90 at the summer solstice, 180 at the autumnal equinox, and
270 at the winter solstice.
Radiant: the area in the sky where shower meteors seem to appear from. This position
is given in right ascension (celestial longitude) and declination (celestial latitude).
Velocity: the velocity at which shower meteors strike the Earth's atmosphere.
The velocity depends on the angle meteoroids (meteors in space) intersect the Earth.
Meteoroids orbiting in the opposite direction of the Earth and striking the atmosphere
head-on are much faster than those orbiting in the same direction as the Earth. This
velocity is measured in kilometers per second.
r: The Population Index, An estimate of the ratio of the number of meteors
in subsequent magnitude classes. Simply stated: the lower the "r" value, the resulting
overall mean magnitude of each shower will be brighter. "r" usually ranges from 2.0 (bright)
to 3.5 (faint).
ZHR: Zenith Hourly Rate, the average maximum number of shower meteors visible
per hour if the radiant is located exactly overhead and the limiting magnitude equals +6.5.
Actual counts rarely reach this figure as the zenith angle of the radiant is usually less and
the limiting magnitude is usually lower. ZHR is a useful tool when comparing the actual observed
rates between individual observers as it sets observing conditions for all to the same standards.
Class: A scale developed by Robert Lunsford to group meteor showers by their intensity:
Class I: the strongest annual showers with ZHR's normally ten or better.
Class II: reliable minor showers with ZHR's normally three or better.
Class III: showers with widely variable rates. They may be strong one year and totally
inactive the next.
Class IV: weak minor showers with ZHR's rarely exceeding three. The study of these
showers is best left to experienced observers who use plotting and angular velocity
estimates to determine shower association. Observers with less experience are urged to
limit their shower associations to showers with a rating of I to III. These showers
are also good targets for video and photographic work.
Moon: the age of the moon in days where 0 is new, 7 is first quarter, 14 is full,
and 21 is last quarter. Meteor activity is best seen in the absence of moonlight so
showers reaching maximum activity when the moon is less than 10 days old or more than 25
are much more favorably observed than those situated closer to the full moon.
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