January sees a peak of sporadic activity for the
southern hemisphere while rates seen north of the equator begin a steady downward
turn that continues throughout the first half of the year. The sporadic activity
is good for both hemispheres, but not as good as it was for northern observers in
December. Once the Quadrantids have passed the shower activity for January is very
quiet.
During this period the moon progresses from its
new phase to nearly half illuminated. The waxing crescent moon will be limited
to the evening sky and will not interfere with the choice morning hours.
The estimated total hourly rates for evening observers this week is near three no
matter your location. For morning observers the estimated total hourly rates should
be near fifteen from the northern hemisphere and sixteen as seen from the southern
hemisphere. The actual rates will also depend on factors such as personal light and
motion perception, local weather conditions, alertness and experience in watching
meteor activity. Evening rates are reduced by moonlight.
The radiant positions and rates listed below are exact
for Saturday night/Sunday morning January 16/17. These positions do not change
greatly day to day so the listed coordinates may be used during this entire period.
Most star atlases (available at science stores and planetariums) will provide
maps with grid lines of the celestial coordinates so that you may find out exactly
where these positions are located in the sky. A planisphere or computer planetarium
program is also useful in showing the sky at any time of night on any date of the
year. Activity from each radiant is best seen when it is positioned highest in the
sky, either due north or south along the meridian, depending on your latitude. It
must be remembered that meteor activity is rarely seen at the radiant position.
Rather they shoot outwards from the radiant so it is best to center your field of
view so that the radiant lies at the edge and not the center. Viewing there will
allow you to easily trace the path of each meteor back to the radiant (if it is
a shower member) or in another direction if it is a sporadic. Meteor activity is
not seen from radiants that are located below the horizon. The positions below
are listed in a west to east manner in order of right ascension (celestial longitude).
The positions listed first are located further west therefore are accessible earlier
in the night while those listed further down the list rise later in the night.
The wide Antihelion (ANT) radiant is now centered at 08:36 (129) +17.
This area of the sky lies in central Cancer, close to the faint star Theta Cancri.
This radiant is best placed near 0100 local standard time (LST)
when it lies on the meridian and is located highest in the sky. Due to the large
size of this radiant, any meteor radiating from eastern Gemini, northwest Hydra,
western Leo, or Cancer could be a candidate for this shower. Rates at this time should be near
two per hour as seen from the northern hemisphere and one per hour for observers
located south of the equator. With an entry velocity of 30 km/sec., the average
Antihelion meteor would be of medium-slow speed.
Studies of the IMO’s video database by Sirko Molau has shown a radiant active in
Cancer this time of year. This radiant is different from the nearby Antihelion
source but the meteors have essentially the same entry velocity. Activity from
the Southern Delta Cancrids (SCC) begin to appear on January 14th and peak
four nights later. On the 14th the radiant is located at 08:39 (130) +10. This
position lies in southern Cancer, just north of the five faint stars that make up
the head of Hydra. These meteors are best seen near 0100 LST when the radiant lies highest
above the horizon. Hourly rates from this shower will be less than one per hour no
matter your location. At 29km/sec. the Southern Delta Cancrids produce meteors of
medium-slow velocity.
The December Leonis Minorids (DLM) are active from a radiant located at 12:22
(186) +18. This position lies in southwestern Coma Berenices near the faint star
11 Comae Berenices. These meteors are best seen near 0500 LST when the radiant lies
highest above the horizon. This shower peaked on December 20th so current rates
would be near less than one per hour no matter your location. At 64km/sec. the
December Leonis Minorids produce mostly swift meteors.
As seen from the mid-northern hemisphere (45N) one would expect to see approximately
thirteen Sporadic meteors per hour during the last hour before dawn as seen
from rural observing sites. Evening rates would be near two per hour. As seen from
the mid-southern hemisphere (45S), morning rates would be near fifteen per hour
as seen from rural observing sites and two per hour during the evening hours. Locations
between these two extremes would see activity between the listed figures. Moonlight
interferes with evening rates during this period.
The table below presents a condensed version of the expected activity this week.
Rates and positions are exact for Saturday night/Sunday morning.
| SHOWER | DATE OF MAXIMUM ACTIVITY | CELESTIAL POSITION | ENTRY VELOCITY | CULMINATION | HOURLY RATE | CLASS* | RA (RA in Deg.) DEC | Km/Sec | Local Standard Time | North-South | Antihelion (ANT) | – | 08:04 (122) +19 | 30 | 01:00 | 2 – 1 | II | Southern Delta Cancrids (SCC) | Jan 18 | 08:39 (130) +10 | 29 | 01:00 | <1 - <1 | IV | December Leonis Minorids (DLM) | Dec 20 | 12:22 (186) +18 | 64 | 05:00 | <1 - <1 | II |
You saw something bright and fast? Like a huge shooting star? Report it: it may be a fireball. 
You counted meteors last night? Share your results with us! 
You took a photo of a meteor or fireball? You have a screenshot of your cam? Share it with us! 
You caught a meteor or fireball on video? Share your video with us!