During this period the moon reaches its first quarter phase on Tuesday December 6th. At this time the moon will be located 90 degrees east of the sun and will set between 2300 and midnight local standard time (LST). As the week progresses the waxing gibbous moon will begin to interfere with early morning meteor observations as the bright moonlight will obscure the fainter meteors. The estimated total hourly meteor rates for evening observers this week is near 5 as seen from mid-northern latitudes (45N) and 4 as seen from tropical southern locations (25S). For morning observers the estimated total hourly rates should be near 30 as seen from mid-northern latitudes (45N) and 25 as seen from tropical southern locations (25S). 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. Note that the hourly rates listed below are estimates as viewed from dark sky sites away from urban light sources. Observers viewing from urban areas will see less activity as only the brightest meteors will be visible from such locations.
The radiant (the area of the sky where meteors appear to shoot from) positions and rates listed below are exact for Saturday night/Sunday morning December 3/4. 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.
These sources of meteoric activity are expected to be active this week.
The December Phoenicids (PHO) are a periodic shower that rarely produces noticeable activity. The only impressive display produced so far by this shower occurred in 1956 when ZHR’s were near 100. These meteors at active from November 28-December 9 with a peak on December 6. The radiant is currently located at 01:04 (016) -53. This position lies in southeastern Phoenix, 5 degrees south of the 3rd magnitude star known as beta Phoenicis. For those viewing from the northern tropics southward, this position also lies 5 degrees northwest of the bright 1st magnitude star known as Achernar (alpha Eridani). This area of the sky is best placed as soon as evening twilight ends. These meteors are best seen from the southern hemisphere where the radiant lies much higher in the sky. For those viewing from the northern hemisphere, only those in the northern tropics have any real chance of seeing activity from this source. At only 18 km/sec. the Phoenicids produce extremely slow meteors.
The December Phi Cassiopeiids (DPC) were discovered by Dr. Peter Jenniskens and are active from November 26 through December 5th. Maximum activity occurs on December 1st when the radiant is located at 01:33 (023) +53. This area of the sky is located in southern Cassiopeia, 3 degrees southeast of the faint star known as Theta Cassiopeiae. These meteors are best seen near 2100 Local Standard Time (LST). Meteors from the December Phi Cassiopeiids strike the atmosphere at 17km/sec., which would produce meteors of very slow velocity. Expected rates would be near less than 1 no matter your location. It has been suggested that these meteors are a continuation of the Andromedids, but for now they remain separate.
The last of the Northern Taurids (NTA) are expected this week from a large radiant located near 05:11 (078) +26. This position lies in northern Taurus, 4 degrees southwest of 2nd magnitude star known as El Nath (beta Tauri). Rates at this time should be near 2 per hour as seen from the northern hemisphere and 1 as seen south of the equator. These meteors may be seen all night long but the radiant is best placed near midnight LST when it lies on the meridian and is located highest in the sky. With an entry velocity of 27 km/sec., the average Northern Taurid meteor would be of slow velocity.
The November Orionids (NOO) are active from a radiant located at 06:20 (095) +15. This area of the sky is located in extreme northeastern Orion, 3 degrees southwest of the 2nd magnitude star known as Alhena (gamma Geminorum). This location is close to the Northern Taurids , but far enough east to be distinguishable. The faster velocity of the November Orionids should help distinguish these meteors from the slower Taurids. The radiant is best placed for viewing near 0100 LST when it lies on the meridian and is highest above the horizon. Hourly rates are expected to be near 2 shower members per hour, no matter your location. With an entry velocity of 44 km/sec., the November Orionids would be of medium speed.
The Monocerotids (MON) are active from November 27th through December 17th with the peak activity occurring on December 9th. The radiant is currently located at 06:26 (097) +09. This position lies in northwest Monoceros, 7 degrees east of the 1st magnitude orange star known as Betelgeuse (Alpha Orionis). This position is only 6 degrees south of the radiant of the November Orionids so care must be take to distinguish between the two. Current rates should be near 1 per hour no matter your location. Rates at maximum may reach 2 per hour. The Monocerotids are best seen near 0100 LST when the radiant lies highest above the horizon. At 41 km/sec. the Monocerotids produce mostly meteors of medium velocity.
The Geminids (GEM) are increasing in strength with each passing night. The peak will occur on Tuesday evening/Wednesday morning December 13/14. This weekend the radiant is located near 06:56 (104) +34. This position lies in northern Gemini, near the spot occupied by the 4th magnitude star known as Theta Geminorum. Rates this weekend should be near 2 per hour as seen from mid-northern latitudes and 1 as seen from the southern tropics. At 34 km/sec. the Geminids produce mostly meteors of medium velocity.
The Puppid-Velids (PUP) are a vast complex of weak radiants located in the constellations of Puppis and Vela. Visual plots and photographic studies have revealed many radiants in this area during November and December. The combined strength of these radiants can produce a ZHR of ten. Actual hourly rates will be much less unless you happen to be observing from the deep Southern Hemisphere. Activity from this source begins around December 1st. The center of this activity is currently located at 08:04 (121) -45. This position lies on the Puppis/Vela border, 3 degrees northwest of the 2nd magnitude star known as gamma Velorum. Peak rates occur near December 7. These meteors are best seen near 0300 LST when the radiant lies highest above the horizon in a dark sky. Observers located in the Southern Hemisphere have an advantage viewing this shower as the radiant will rise higher into their sky allowing more activity to be seen. Since the radiant lies low in the south for most northern hemisphere observers, meteors seen from north of the equator tend to be long in length and long-lasting. At 40 km/sec. the Puppid-Velids produce meteors of average velocity.
The Sigma Hydrids (HYD) are active from November 26 through December 21, with maximum activity occurring on December 6. The radiant is currently located at 08:08 (122) +03 , which places it in extreme eastern Canis Minor, 8 degrees east of the brilliant zero magnitude star known as Procyon (Alpha Canis Minoris). These meteors are best seen near 0400 LST when the radiant lies highest above the horizon. This source is the strongest in the sky for the first week of December. Hourly rates are expected to be near 5 per hour no matter your location. With an entry velocity of 62 km/sec., most activity from this radiant would be of swift speed.
The December Leonis Minorids (DLM) are a shower of long duration active from December 6th through January 18th. Maximum occurs near December 21st when rates may reach 3 an hour. During this period I would expect an hourly rates of less than 1 from a radiant located at 09:52 (148) +35. This position lies in western Leo Minor, 2 degrees west of the faint star known as 21 Leo Minoris. These meteors are best seen near 0400 LST when the radiant lies highest above the horizon. At 63 km/sec. the December Leonis Minorids produce mostly swift meteors.
The Psi Ursa Majorids (PSU) were discovered by observers in Japan using data from SonotaCo. This shower is active from December 1-16 with maximum activity occurring on December 4. At maximum the radiant is located at 11:16 (169) +44. This position lies in southern Ursa Major, one degree southeast of the third magnitude star known as Psi Ursae Majoris. This area of the sky is best placed during the last hour before dawn, when it lies highest above the horizon in a dark sky. Current rates would most likely be less than one per hour and may reach 1 per hour at maximum. Observers south of the equator would see rates less than 1 per hour due to the lower radiant elevation. At 61km/sec., the average Psi Ursa Majorid meteor would be swift.
The December Kappa Draconids (DKD) are another shower discovered in Japan by observers using data from SonotaCo. This short-lived shower is only active from December 2-6 with maximum activity occurring on December 3rd. On the night of maximum the radiant will be located at 12:22 (185) +70. This position lies in extreme western Draco, close to the faint star Kappa Draconis. While the radiant lies above the horizon all night for most of the northern hemisphere, it is best placed during the last hour before dawn, when it lies highest above the horizon in a dark sky. Rates could reach 3 per hour on the morning of the 3rd. Away from that morning I would expect hourly rates of less than 1. Due to the high northerly declination of the radiant these meteors are not visible from most of the southern hemisphere. At 41km/sec., the average December Kappa Draconid meteor would be of medium velocity.
The December Sigma Virginids (DSV) was discovered by John Greaves using the data of SonotaCo. IMO video cameras confirmed that this source is active during most of December and into the first week of January. Visual observers have their best chance at catching these meteors from December 17-31. Peak rates occur near December 24th. The current radiant location is at 12:40 (190) +08 which place it in northern Virgo some 2 degrees south of the faint star known as Rho Virginis. Current hourly rates would be less than 1 shower member no matter you location. These meteors are best seen during the last dark hour before dawn, when the radiant lies highest above the horizon in a dark sky. At 68 km/sec. the December Sigma Virginids would produce mostly swift meteors.
The December Alpha Draconids (DAD) were discovered by the Japanese observers using data from SonotaCo and is active from December 5-13. They are predicted to peak on December 7th from a radiant located at 13:01 (210) +60. This position actually lies in northeastern Ursa Major, 4 degrees northeast of the second magnitude star known as Alioth (Epsilon Ursae Majoris). These meteors are best seen during the last dark hour before dawn, when the radiant lies highest above the horizon in a dark sky. This shower is not well seen from the southern hemisphere. Current rates would most likely be near 1 per hour as seen from the northern hemisphere. Observers south of the equator would see rates less than 1 per hour due to the lower radiant elevation. Recent analysis by the IMO has revealed that this shower actually has two activity periods. The one listed above and another lasting from December 26-January 1st.
As seen from the mid-northern hemisphere (45N) one would expect to see approximately 12 sporadic meteors per hour during the last hour before dawn as seen from rural observing sites. Evening rates would be near 4 per hour. As seen from the tropical southern latitudes (25S), morning rates would be near 8 per hour as seen from rural observing sites and 3 per hour during the evening hours. Locations between these two extremes would see activity between the listed figures.
The table below presents a list of radiants that are expected to be active this week. Rates and positions are exact for Saturday night/Sunday morning except where noted in the shower descriptions.
|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|
|Phoenicids (PHO)||Dec 06||01:04 (016) -53||18||20:00||<1 – <1||III|
|Dec. Phi Cassiopeiids (DPC)||Dec 05||01:33 (023) +53||19||21:00||<1 – <1||IV|
|Northern Taurids (NTA)||Nov 11||05:11 (078) +26||30||00:00||3 – 2||II|
|November Orionids (NOO)||Nov 29||06:20 (095) +15||44||01:00||2 – 2||II|
|Monocerotids (MON)||Dec 09||06:26 (097) +09||41||01:00||1 – 1||II|
|Geminids (GEM)||Dec 13||06:56 (104) +34||34||02:00||3 – 1||I|
|Puppid-Velids (PUP)||Dec 07||08:04 (121) -45||42||03:00||1 – 5||II|
|Sigma Hydrids (HYD)||Dec 07||08:08 (122) +03||61||03:00||5 – 5||II|
|Dec. Leonis Minorids (DLM)||Dec 21||09:52 (148) +35||63||05:00||<1 – <1||IV|
|Psi Ursa Majorids (PSU)||Dec 05||11:24 (171) +43||61||06:00||1 – <1||IV|
|Dec. Sigma Virginids (DSV)||Dec 24||12:40 (190) +08||68||08:00||<1 – <1||IV|
|Dec. Alpha Draconids (DAD)||Dec 07||13:01 (210) +60||41||08:00||1 – <1||IV|