Meteor Activity Outlook for October 29-November 4, 2011

The following is a slightly edited version of Bob Lunsford’s excellent weekly summary of meteor activity. The original version can be found at the American Meteor Society’s site.

As seen from the northern hemisphere, meteor rates continue to be strong in November. While no major activity is expected this month, the two Taurid radiants plus the Leonids keep the skies active. The addition of strong sporadic rates make November one of the better months to view meteor activity from north of the equator. Skies are fairly quiet as seen from the southern hemisphere this month. Activity from the three showers mentioned above may be seen from south of the equator, but the sporadic rates are much lower than those seen in the northern hemisphere.

During this period the moon reaches its first quarter phase on Wednesday November 2nd. At this time the moon will lie ninety degrees east of the sun and will set near midnight local daylight time (LDT). This weekend the waxing crescent moon will set during the early evening hours and will not interfere with meteor observing during the more active morning hours. The estimated total hourly rates for evening observers this week is near four as seen from the northern hemisphere and three as seen from the southern hemisphere. For morning observers the estimated total hourly rates should be near eighteen as seen from mid-northern latitudes and thirteen from mid-southern latitudes. 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 this week due to moonlight.

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 October 29/30. These positions do not change greatly day to day so the listed coordinates may be used during this entire period.

The following showers are expected to be active this week:

The Northern Taurids (NTA) are active from a large radiant centered at 03:12 (048) +21, which lies in eastern Aries, very close to the position of the fourth magnitude star Delta Arietis. The radiant is best placed near 0200 LDT, when it lies highest above the horizon. Meteors from the Northern Taurids strike the atmosphere at 29km/sec., which would produce meteors of slow velocity. Expected rates would be near two per hour, no matter your location.

The center of the Southern Taurid (STA) radiant now lies 03:15 (049) +12. This position lies in southeastern Aries, eight degrees south of the fourth magnitude star Delta Arietis The radiant is best placed near the meridian at 0200 LDT, but activity may be seen all night long. Striking the atmosphere at 29 km/sec., the average Southern Taurid meteor travels slowly through the skies. Rates should be near two per hour no matter your location.

A new radiant has been discovered in Taurus which is active during this period. The Eta Taurids (ETT) are active from October 24 through November 3, with maximum occurring on the 24th. The radiant position currently lies at 04:04 (061) +24, which lies in western Taurus, four degrees east of the famous Pleiades star cluster. The radiant is best placed near 0300 LDT, when it lies highest above the horizon. Meteors from the Eta Taurids strike the atmosphere at 47km/sec., which would produce meteors of average velocity. Expected rates would be less than one per hour, no matter your location.

The Orionids (ORI) have now passed maximum and hourly rates are now falling with each passing night. Rates are expected to be less than five per hour this week. The radiant is currently located at 06:49 (102) +16. This position lies in southern Gemini, two degrees southeast of the second magnitude star Alhena (Gamma Geminorum). The radiant is best placed near 0500 LDT, when it lies highest above the horizon. At 67km/sec., the average Orionid is swift.

Recent studies by Sirko Molau and Juergen Rendtel have revealed a radiant in Canis Minor that is active this time of year. Old radiant positions placed it within the borders of Cancer. The Beta Cancrids (BCN) are active from October 25 through November 3, with maximum occurring on the 27th. The radiant position currently lies at 07:32 (113) -03, which lies in central Canis Minor, five degrees south of the brilliant zero magnitude star Procyon (Alpha Canis Minoris. The radiant is best placed near 0600 LDT, when it lies highest above the horizon. Meteors from the Beta Cancrids strike the atmosphere at 65km/sec., which would produce meteors of swift velocity. Expected rates would be less than one per hour, no matter your location.

As seen from the mid-northern hemisphere (45N) one would expect to see approximately ten sporadic meteors per hour during the last hour before dawn as seen from rural observing sites. Evening rates would be near three per hour. As seen from the mid-southern hemisphere (45S), morning rates would be near five 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.

The list below presents a condensed version of the expected activity this week. Rates and positions are exact for Saturday night/Sunday morning.

Shower Name                 RA     DEC   Vel     Rates
                                         km/s   NH    SH
NTA Northern Taurids      03h 12m  +21    29     2     2
STA Southern Taurids      03h 15m  +12    27     2     2 
ETT Eta Taurids           04h 04m  +24    47    <1    <1 
ORI Orionids              06h 49m  +16    61     3     3
BCN Beta Cancrids         07h 32m  -03    65    <1    <1

RA - Right Ascension
DEC - Declination
Vel - Velocity relative to Earth (in km per sec)
Rates - Rate of visible meteors per hour from a dark site
NH - Northern Hemisphere
SH - Southern Hemisphere

Meteor Activity Outlook for October 12-28, 2011

Sorry, I’m a few days late posting this…

The following is a slightly edited version of Bob Lunsford’s excellent weekly summary of meteor activity. The original version can be found at the American Meteor Society’s site.

Meteor activity in general increases in October when compared to September. A major shower (the Orionids) is active most of the month along with many minor showers. Both branches of the Taurids become more active as the month progresses, providing slow, graceful meteors to the nighttime scene. The Orionids are the big story of the month reaching maximum activity on the 22nd. This display can be seen equally well from both hemispheres which definitely helps out observers located in the sporadic-poor southern hemisphere this time of year.

During this period the moon reaches its new phase on Wednesday October 26th. At this time the moon will lie near the sun and will be invisible at night. This weekend the waning crescent moon will rise during the late morning hours and will not interfere with meteor observing. The estimated total hourly rates for evening observers this week is near four as seen from the northern hemisphere and three as seen from the southern hemisphere. For morning observers the estimated total hourly rates should be near thirty three as seen from mid-northern latitudes and twenty eight from mid-southern latitudes. 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.

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 October 22/23. These positions do not change greatly day to day so the listed coordinates may be used during this entire period.

The following showers are expected to be active this week:

A new radiant has been discovered by Sirko Molau and Juergen Rendtel in Draco which is active during this period. The October Ursa Minorids (OUI) are active from October 16-28, with maximum occurring on the 24th. The current radiant position lies at 18:18 (275) +75. This position lies in eastern Draco two degrees north of the faint star Chi Draconis. Older radiant positions were a bit further west in Ursa Minor.  The radiant is best placed just as soon as it becomes dark, when it lies highest in a dark sky. Meteors from the October Ursa Minorids strike the atmosphere at 28km/sec., which would produce meteors of slow velocity. Expected rates would be less than one per hour, as seen from the northern hemisphere. Activity from this shower is not visible in the southern hemisphere due to the high northerly location of the radiant.

The Northern Taurids (NTA) are now active from a large radiant centered at 02:48 (042) +20, which lies in central Aries, six degrees west of the fourth magnitude star Delta Arietis. The radiant is best placed near 0200 local daylight time (LDT), when it lies highest above the horizon. Meteors from the Northern Taurids strike the atmosphere at 29km/sec., which would produce meteors of slow velocity. Expected rates would be near two per hour, no matter your location.

The center of the Southern Taurid (STA) radiant now lies 02:51 (043) +11. This position lies on the Aries/Cetus border, three degrees east of the fourth magnitude star Mu Ceti. The radiant is best placed near the meridian at 0200 LDT, but activity may be seen all night long. Striking the atmosphere at 29 km/sec., the average Southern Taurid meteor travels slowly through the skies. Rates should be near two per hour no matter your location.

A new radiant has been discovered in Taurus which is active during this period. The Eta Taurids (ETT) are active from October 24 through November 3, with maximum occurring on the 24th. At maximum, the  radiant position lies at 03:42 (056) +24, which lies in western Taurus in the area of sky occupied by the famous Pleiades star cluster. The radiant is best placed near 0300 LDT, when it lies highest above the horizon. Meteors from the Eta Taurids strike the atmosphere at 47km/sec., which would produce meteors of average velocity. Expected rates would be less than one per hour, no matter your location.

The Orionids (ORI) reach maximum activity on morning of October 22nd. Rates are expected to peak between 10-20 shower members per hour on that morning. Moonlight from the waning crescent moon will reduce activity slightly. The radiant is currently located at 06:28 (97) +16. This position lies in western Gemini, close to the second magnitude star Alhena (Gamma Geminorum). The radiant is best placed near 0500 LDT, when it lies highest above the horizon. At 67km/sec., the average Orionid is swift.

The Epsilon Geminids (EGE) are active from October 16th through the 27th. Maximum activity occurred on the 19th. The radiant is currently located at 07:02 (105) +27. This position lies in central Gemini, three degrees northeast of the third magnitude star Epsilon Geminorum. This position is also close to the Orionid radiant so care must taken for correct shower association, especially since they have similar velocities. The Orionids will be more numerous. Current rates are near one per hour. The radiant is best placed near 0600 LDT, when it lies highest above the horizon. At 70km/sec., the average Epsilon Geminid is swift.

Recent studies by Sirko Molau and Juergen Rendtel have revealed a radiant in Canis Minor that is active this time of year. Old radiant positions placed it within the borders of Cancer. The Beta Cancrids (BCN) are active from October 25 through November 3, with maximum occurring on the 27th. The radiant position at maximum lies at 07:22 (111) -06, which lies in southwestern Canis Minor, three degrees west of the brilliant zero magnitude star Procyon (Alpha Canis Minoris. The radiant is best placed near 0600 LDT, when it lies highest above the horizon.Meteors from the Beta Cancrids strike the atmosphere at 65km/sec., which would produce meteors of swift velocity. Expected rates would be less than one per hour, no matter your location.

The Leonis Minorids (LMI) are active from October 16-27 with maximum activity occurring on October 23rd. ZHR’s are usually low but the radiant is far removed from the Orionids and Epsilon Geminids so that any possible shower members should be easily identified. Hourly rates should be near one this weekend. This radiant is currently located at 10:43 (161) +36, which places it in northeastern Leo Minor, two degrees east of the fourth magnitude star Beta Leonis Minoris . The radiant is best placed just before dawn when it lies highest in a dark sky. This shower is better situated for observers situated in the northern hemisphere where the radiant rises far higher into the sky before the start of morning twilight. At 60km/sec., the average Leonis Minorid is swift.

As seen from the mid-northern hemisphere (45N) one would expect to see approximately ten sporadic meteors per hour during the last hour before dawn as seen from rural observing sites. Evening rates would be near three per hour. As seen from the mid-southern hemisphere (45S), morning rates would be near five 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.

The list below presents a condensed version of the expected activity this week. Rates and positions are exact for Saturday night/Sunday morning.

Shower Name                 RA     DEC   Vel     Rates
                                         km/s   NH    SH
OUI Oct Ursa Minorids     18h 18m  +75    28    <1    <1
NTA Northern Taurids      02h 48m  +20    29     2     2
STA Southern Taurids      02h 51m  +11    27     2     2 
ETT Eta Taurids           03h 42m  +24    47    <1    <1 
ORI Orionids              06h 28m  +16    61    15    15
EGE Epsilon Geminids      07h 02m  +27    70     1     1
BCN Beta Cancrids         07h 22m  -06    65    <1    <1
LMI Leo Minorids          10h 43m  +36    60     2     2

RA - Right Ascension
DEC - Declination
Vel - Velocity relative to Earth (in km per sec)
Rates - Rate of visible meteors per hour from a dark site
NH - Northern Hemisphere
SH - Southern Hemisphere

Sep 18 – 31 Meteors

It has been a long time since I posted my nightly video meteor results. Part of the problem was our annual monsoon season here in Tucson. But the main problem was a series of mechanical and software issues that I just didn’t have the time to solve until a few weeks ago.

The 2011 monsoon was very similar to last years ‘nonsoon’. Though every night saw lots of clouds and rain threatened, little rain actually fell. That wouldn’t have been too much of a problem for my video set-up except for the fact that my ‘all-weather’ camera enclosure is no longer ‘all-weather’. So I decided to leave my camera off on those nights when it looked like it might rain. Since I was going to be down for weather reasons anyway I went ahead and upgraded to the latest version of the automatic meteor detection software, MetRec. That didn’t go so well and resulted in finally upgrading from an old PIII computer to a Pentium 4 machine. Now, knock on wood, everything seems to be working.

September is a month of high meteor rates. Sporadic meteors rates are near their annual peak. Though no major showers are active, a number of minor showers are consistent contributors to the high rates. Below are a collection of some of the best meteors from the last two weeks of September.

Long-lasting (~3.5+ sec) SPO seen on 2011 Sep 18 @ 05:47 UT.

Bright (~-2 mag) SPO on 2011 Sep 22 @ 06:58 UT.

Another SPO from 2011 Sep 23 (08:17 UT).

A third SPO from 2011 Sep 23 (10:00 UT).

Almost 2 sec in duration SPO on 2011 Sep 25 @ 06:07 UT.

Nu Eridanid fireball (~-4 to -5 mag) on 2011 Sep 26 @ 08:33 UT.

SPO racing north out of Auriga on 2011 Sep 26 @ 12:07 UT.

Obs  Date(UT)      Time    TOT SPO ANT NTA STA NUE SPE DAU
TUS  2011-09-31   10h 17m   37  25  -   2   7   -   -   3
TUS  2011-09-30   07h 34m   33  26  -   4   2   -   -   1
TUS  2011-09-29   09h 44m   36  29  -   2   3   -   -   2
SDG  2011-09-27   04h 21m   28  27  1   -   0   -   -   -
TUS  2011-09-25   05h 49m   25  22  1   -   -   2   -   0
TUS  2011-09-24   09h 29m   38  28  5   -   -   4   -   1
TUS  2011-09-23   09h 39m   35  32  1   -   -   1   -   1
TUS  2011-09-22   08h 25m   33  24  3   -   -   6   -   0
TUS  2011-09-21   08h 54m   30  25  0   -   -   1   -   4
TUS  2011-09-20   10h 06m   30  25  1   -   -   1   -   3
TUS  2011-09-19   09h 41m   25  20  3   -   -   1   1   -
TUS  2011-09-18   09h 38m   39  34  3   -   -   2   0   -

SAL3 - SALSA3 camera in Tucson (Carl Hergenrother)
ALLS - Near all-sky camera in Tucson (Carl Hergenrother)
VIST - Visual observations from Tucson (Carl Hergenrother)
VISH - Visual observations from Hermosillo (Salvador Aguirre)
HERM - PARENI camera in Hermosillo (Salvador Aguirre)
SDG - Camera in San Diego operated by Bob Lunsford
Time - Total amount of time each camera looked for meteors
TOT - Total number of meteors detected
SPO - Sporadics (meteors not affiliated with any particular meteor shower)
ANT - Antihelions
NTA - Northern Taurids 
STA - Southern Taurids NUE - Nu Eridanids 
SPE - September Perseids 
DAU - Delta Aurigids

Meteor Activity Outlook for December 4-10, 2010

The Meteor Activity Outlook is a weekly summary of expected meteor activity written by Robert Lunsford, Operations Manager of the American Meteor Society and contributor to this blog. The original unedited version of this week’s Meteor Activity Outlook can be found at the American Meteor Society’s site.

No matter where you live, the first half of December provides some of the best meteor activity of the year. In the northern hemisphere the sporadic rates are still strong plus you can also count on strong activity from the Geminids, which peak on December 14. There are also several minor radiants that add a few meteors each hour. All of these centers of activity are located high in the sky during the early morning hours this time of year. Much of the activity mentioned above can also be seen from the southern hemisphere. While the sporadic rates are not as strong as those seen from the north, they are stronger than the previous months and heading for a maximum in January. The warm, but short summer nights south of the equator make for some great viewing as long as the moon does not interfere.

During this period the moon reaches its new phase on Sunday December 5th. At this time the moon lies near the sun and cannot be seen at night. Later next week the waxing crescent moon enters the evening sky but still sets long before the busy morning hours arrive. The estimated total hourly rates for evening observers this week is ~5 from the northern hemisphere and ~3 for observers south of the equator. For morning observers the estimated total hourly rates should be ~15 from the northern hemisphere and ~13 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.

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 4/5. These positions do not change greatly day to day so the listed coordinates may be used during this entire period.

The following showers are expected to be active this week:

December Phoenicids (PHO)

The December Phoenicids (PHO) are a periodic shower that rarely produces noticeable activity. The only impressive display produced by this shower occurred in 1956 when ZHR’s were near 100. Peak activity occurs on December 6. Little activity is expected away from the peak night. The radiant is currently located at 01:08 (017) -53. This position lies in eastern Phoenix, five degrees northwest of the first magnitude star Archernar (Alpha Eridani). These meteors are best seen near 2000 (8pm) LST, when the radiant lies highest above the horizon in a dark sky. Due to the southerly declination of the radiant, this shower is not visible north of the northern tropical areas. The deep southern hemisphere has the best chance of seeing any activity. At 22 km/sec. the Phoenicids produce very slow meteors.

Northern Taurids (NTA)

The center of the large Northern Taurid (NTA) radiant lies at 05:12 (078) +26. This area of the sky is located in eastern Taurus, five degrees southwest of the second magnitude star El Nath (Beta Tauri). These meteors are best seen near midnight, when the radiant lies highest above the horizon. This shower peaked on November 13, so rates are falling should be ~2 per hour. Meteors from the Northern Taurids strike the atmosphere at 29km/sec., which would produce meteors of slow velocity. This shower is also responsible for many of the fireball reports seen in November.

November Orionids (NOO)

The November Orionids (NOO) were recently discovered by analyzing video data. For years it was lost in the maze of radiants active this time of year. Due to the low activity, visual observers were unable to detect this shower. This shower is active from November 18 through December 9. Maximum activity occurs on November 30. Once you know the radiant in advance, this shower is actually quite noticeable, producing an average of 2 shower members per hour near maximum. The radiant is currently located at 06:20 (095) +15. This position lies in northeastern Orion, eight degrees northeast of the orange first magnitude star Betelgeuse (Alpha Orionis). These meteors are best seen near 0100 LST when the radiant lies on the meridian and highest above the horizon. At 44 km/sec. the November Orionids produce mostly medium velocity meteors.

Monocerotids (MON)

The Monocerotids (MON) are active from December 7th through the 18th. Peak activity occurs on December 8th. On the night of maximum activity the radiant is located at 06:37 (099) +08. This position lies in northern Monoceros, eight degrees south of the second magnitude star Alhena (Gamma Geminorum). Rates at maximum should be near two per hour no matter your location. 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.

Geminids (GEM)

Geminid (GEM) activity begins this weekend from a radiant located at 07:16 (109) +33. This position lies in northern Gemini, four degrees west of the second star Castor (Alpha Geminorum). Expected rates this weekend would only be near one per hour as maximum is still ten days away. Although Geminid meteors can be seen all night long, they are best seen near 0200 LST when the radiant lies highest above the horizon. This shower peaks on the night of December 14, when rates can surpass 60 shower members per hour as seen from dark sites. Geminid activity can be seen from the southern hemisphere but at much reduced rate. As seen from south of the equator, Geminid activity could only be seen for a few hours before and after 0200 LST. At 35 km/sec. the Geminids produce mostly meteors of medium velocity.

Puppid-Velids (PUP)

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 10. Actual hourly rates will be much less unless you happen to be observing from the deep Southern Hemisphere. The center of this activity is currently located at 08:08 (122) -45. This position lies in western Vela, two degrees north of the second magnitude star 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. At 40 km/sec. the Puppid-Velids produce meteors of average velocity.

Sigma Hydrids (HYD)

The Sigma Hydrids (HYD) are active from November 26 through December 20. Maximum activity occurs on December 6 from a radiant located at 08:16 (124) +03. This position lies on the Hydra/Canis Minor border, seven degrees southeast of the brilliant zero magnitude star Procyon (Alpha Canis Minoris). These meteors are best seen near 0300 LST when the radiant lies highest above the horizon. Current rates would be near two per hour no matter your location. At 61 km/sec. the Sigma Hydrids produce mostly swift meteors.

December Leonis Minorids (DLM)

Activity from the December Leonis Minorids (DLM) begin this weekend from a radiant located at 09:56 (149) +37. This position lies in central Leo Minor, seven degrees northeast of the fourth magnitude star Alpha Lyncis. These meteors are best seen near 0500 LST when the radiant lies highest above the horizon. This shower peaks on December 20th so current rates would be near one per hour as seen from the northern hemisphere and less than one per hour as seen from south of the equator. At 64 km/sec. the December Leonis Minorids produce mostly swift meteors.

Psi Ursa Majorids (PSU)

Another shower verified by video means are the Psi Ursa Majorids (PSU). This shower is active from November 29-December 13 with maximum activity occurring on December 5. The radiant is currently located at 11:12 (168) +43. This position lies in southern Ursa Major, one degree south of the third magnitude star 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. At 61km/sec., the average Psi Ursa Majorid meteor would be swift.

December Kappa Draconids (KDR)

Another shower verified by video means are the December Kappa Draconids (KDR). This shower is active from November 30-December 6 with maximum activity occurring on December 3. Activity from this source is not expected this weekend. On the night of maximum the radiant will be located at 12:30 (187) +69. This position lies in extreme western Draco, very 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. Current rates would most likely be less than one per hour. At 43km/sec., the average December Kappa Draconid meteor would be of medium velocity.

Shower Name                 RA     DEC   Vel     Rates
                                         km/s   NH    SH
PHO December Phoencids    01h 08m  -53    18    <1    <1
NTA Northern Taurids      05h 12m  +26    29     2     2
NOO November Orionids     06h 20m  +15    44     2     2
MON Monocerotids          06h 37m  +08    41     2     2
GEM Geminids              07h 16m  +33    35     1    <1
PUP Puppid-Velids         08h 08m  -45    40    <1     5
HYD Sigma Hydrids         08h 16m  +03    61     2     2
DLM Dec Leonis Minorids   09h 56m  +37    71    <1    <1
PSU Psi Ursa Majorids     11h 12m  +43    61    <1    <1
KDR Dec Kappa Draconids   12h 30m  +69    43    <1    <1

RA - Right Ascension
DEC - Declination
Vel - Velocity relative to Earth (in km per sec)
Rates - Rate of visible meteors per hour from a
        dark site
NH - Northern Hemisphere
SH - Southern Hemisphere

Meteor Activity Outlook for November 27-December 3, 2010

The Meteor Activity Outlook is a weekly summary of expected meteor activity written by Robert Lunsford, Operations Manager of the American Meteor Society and contributor to this blog. The original unedited version of this week’s Meteor Activity Outlook can be found at the American Meteor Society’s site.

No matter where you live, the first half of December provides some of the best meteor activity of the year. In the northern hemisphere the sporadic rates are still strong plus you can also count on strong activity from the Geminids, which peak on December 14. There are also several minor radiants that add a few meteors each hour. All of these centers of activity are located high in the sky during the early morning hours this time of year. Much of the activity mentioned above can also be seen from the southern hemisphere. While the sporadic rates are not as strong as those seen from the north, they are stronger than the previous months and heading for a maximum in January. The warm, but short summer nights south of the equator make for some great viewing as long as the moon does not interfere.

During this period the moon reaches its last quarter phase on Saturday November 27th. At this time the moon lies ninety degrees west of the sun and rises near midnight LST (Local Standard Time). Thus morning observers will have moonlight to contend with this weekend. Successful observations can still be undertaken as long as the moon is kept out of your field of view. The light of the last quarter moon is much less intense than that of a full moon and many meteors can still be seen, especially under transparent skies. As the week progresses the waning crescent moon becomes less of a problem as it grows dimmer and rises later and later during the early morning hours. The estimated total hourly rates for evening observers this week is ~5 from the northern hemisphere and ~3 for observers south of the equator. For morning observers the estimated total hourly rates should be ~15 from the northern hemisphere and ~13 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. Morning rates are reduced due to moonlight.

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 November 27/28. These positions do not change greatly day to day so the listed coordinates may be used during this entire period.

The following showers are expected to be active this week:

December Phoenicids (PHO)

The December Phoenicids (PHO) are a periodic shower that rarely produces noticeable activity. The only impressive display produced by this shower occurred in 1956 when ZHR’s were near 100. Peak activity occurs on December 6. Little activity is expected away from the peak night. The radiant is currently located at 00:50 (012) -52. This position lies in central Phoenix some ten degrees southeast of the second magnitude star Ankaa (Alpha Phoenicis). These meteors are best seen near 2100 (9pm) LST, when the radiant lies highest above the horizon in a dark sky. Due to the southerly declination of the radiant, this shower is not visible north of the northern tropical areas. The deep southern hemisphere has the best chance of seeing any activity. At 22 km/sec. the Phoenicids produce very slow meteors.

Andromedids (AND)

Sirko Molau and Juergen Rendtel’s studies of video radiants has revealed that activity from the famous Andromedid shower, noted for intense storms during the 19th century, may still be seen throughout November. The current
position of the large radiant is 01:44 (026) +45. This position lies in eastern Andromeda, three degrees south of the fourth magnitude star 51 Andromedae. Visual activity is expected to be low, but detectable. An inconspicuous maximum occurs on November 12. The Andromedid meteors are best seen near 2200 (10pm) LST (Local Standard Time) when the radiant lies on the meridian. At 19km/sec., the average Andromedid will appear as a very slow moving meteor. Sirko mentions that these meteors are “conspicuously slow and of almost constant activity” during this period.

Northern Taurids (NTA)

The center of the large Northern Taurid (NTA) radiant lies at 04:49 (072) +25. This area of the sky is located in central Taurus, eight degrees north of the orange first magnitude star Aldebaran (Alpha Tauri). These meteors are best seen near 0100 LST, when the radiant lies highest above the horizon. This shower peaked on November 13, so rates are falling should be ~2 per hour. Meteors from the Northern Taurids strike the atmosphere at 29km/sec., which would produce meteors of slow velocity. This shower is also responsible for many of the fireball reports seen in November.

November Orionids (NOO)

The November Orionids (NOO) were recently discovered by analyzing video data. For years it was lost in the maze of radiants active this time of year. Due to the low activity, visual observers were unable to detect this shower. This shower is active from November 18 through December 9. Maximum activity occurs on November 30. Once you know the radiant in advance, this shower is actually quite noticeable, producing an average of 2 shower members per hour near maximum. The radiant is currently located at 05:58 (090) +15. This position lies in northeastern Orion, seven degrees north of the orange first magnitude star Betelgeuse (Alpha Orionis). These meteors are best seen near 0200 LST when the radiant lies on the meridian and highest above the horizon. At 44 km/sec. the November Orionids produce mostly medium velocity meteors.

Puppid-Velids (PUP)

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 10. Actual hourly rates will be much less unless you happen to be observing from the deep Southern Hemisphere. The center of this activity is currently located at 07:52 (118) -45. This position lies in eastern Puppis, four degrees northwest of the second magnitude star 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. At 40 km/sec. the Puppid-Velids produce meteors of average velocity.

Psi Ursa Majorids (PSU)

Another shower verified by video means are the Psi Ursa Majorids (PSU). This shower is active from November 29-December 13 with maximum activity occurring on December 5. The radiant is currently located at 10:38 (159) +45. This position lies in southwestern Ursa Major, five degrees west of the third magnitude star Kappa 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. At 61km/sec., the average Psi Ursa Majorid meteor would be swift.

Leonids (LEO)

This week is your last chance to see the Leonids (LEO) for 2010. This shower peaked on the Thursday morning November 18 and current rates are well below 1 per hour no matter your location. The radiant is located at 10:41 (160) +19. This position lies in central Leo, four degrees east of the second magnitude star Algeiba (Gamma Leonis). The area of the sky does not clear the eastern horizon until the late evening hours so no Leonid activity can be seen during the early evening hours. These meteors are best seen during the last hour before the onset of morning twilight, when the radiant lies highest above the horizon in a dark sky. At 71km/sec., the average Leonid is swift with a high percentage of trains.

December Kappa Draconids (KDR)

Another shower verified by video means are the December Kappa Draconids (KDR). This shower is active from November 30-December 6 with maximum activity occurring on December 3. Activity from this source is not expected this weekend. On the night of maximum the radiant will be located at 12:22 (185) +72. This position lies in extreme western Draco, two degrees northwest of 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. Current rates would most likely be less than one per hour. At 43km/sec., the average December Kappa Draconid meteor would be of medium velocity.

Shower Name                 RA     DEC   Vel     Rates
                                         km/s   NH    SH
PHO December Phoencids    00h 50m  -52    18    <1    <1
AND Andromedids           01h 44m  +45    19    <1    <1
NTA Northern Taurids      04h 49m  +25    29     2     2
NOO November Orionids     05h 58m  +15    44     2     2
PUP Puppid-Velids         07h 52m  -45    40    <1     2
PSU Psi Ursa Majorids     19h 38m  +45    61    <1    <1
LEO Leonids               10h 41m  +19    71    <1    <1
KDR Dec Kappa Draconids   12h 22m  +72    43    <1    <1

RA - Right Ascension
DEC - Declination
Vel - Velocity relative to Earth (in km per sec)
Rates - Rate of visible meteors per hour from a
        dark site
NH - Northern Hemisphere
SH - Southern Hemisphere

Meteor Activity Outlook for November 6-12, 2010

The Meteor Activity Outlook is a weekly summary of expected meteor activity written by Robert Lunsford, Operations Manager of the American Meteor Society and contributor to this blog. The original unedited version of this week’s Meteor Activity Outlook can be found at the American Meteor Society’s site.

As seen from the northern hemisphere, meteor rates continue to be strong in November. While no major activity is expected this month, the two Taurid radiants plus the Leonids keep the skies active. The addition of strong sporadic rates make November one of the better months to view meteor activity from north of the equator. Skies are fairly quiet as seen from the southern hemisphere this month. Activity from the three showers mentioned above may be seen from south of the equator, but the sporadic rates are much lower than those seen in the northern hemisphere.

During this period the moon reaches its new phase on Saturday November 6th. At this time the moon lies near the sun and cannot be seen at night. This will be the best time to view meteor activity this month. The Taurids will be producing many slow meteors all night long while the sporadic rates will also remain high. The estimated total hourly rates for evening observers this week is near six from the northern hemisphere and four for observers south of the equator. For morning observers the estimated total hourly rates should be near twenty four from the northern hemisphere and fourteen 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.

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 November 6/7. These positions do not change greatly day to day so the listed coordinates may be used during this entire period.

The following showers are expected to be active this week:

Andromedids (AND)

Sirko Molau and Juergen Rendtel’s studies of video radiants has revealed that activity from the famous Andromedid shower, noted for intense storms during the 19th century, may still be seen throughout November. The current
position of the large radiant is 01:27 (022) +27. This position lies in a sparse area of northeastern Pisces. The nearest bright star is third magnitude Alpha Trianguli, which lies five degrees to the northeast. Visual activity is expected to be low, but detectable. An inconspicuous maximum occurs on November 12. The Andromedid meteors are best seen near 2200 (10pm) LST (Local Standard Time) when the radiant lies on the meridian. At 19km/sec., the average Andromedid will appear as a very slow moving meteor. Sirko mentions that these meteors are “conspicuously slow and of almost constant activity” during this period.

Northern Taurids (NTA)

The center of the large Northern Taurid (NTA) radiant lies at 03:38 (055) +22. This area of the sky is located in western Taurus, two degrees southwest of the famous naked eye open cluster known as the Pleiades. These meteors are best seen near 0100 LST, when the radiant lies highest above the horizon. This shower peaks on November 13, so rates are slowly increasing. Current rates would be near three per hour, no matter your location. Meteors from the Northern Taurids strike the atmosphere at 29km/sec., which would produce meteors of slow velocity. This shower is also responsible for many of the fireball reports seen in November.

Southern Taurids (STA)

The center of the large Southern Taurid (STA) radiant lies at 03:42 (056) +14. This area of the sky is located in western Taurus, ten degrees south of the Pleiades. The radiant is also best placed near the meridian near 0100 LDT. We are now well past the October 10 maximum for this shower but rates will still remain near two per hour, no matter your location. Striking the atmosphere at 29 km/sec., the average Southern Taurid meteor travels slowly through the skies. This shower is also responsible for many of the fireball reports seen in October.

Orionids (ORI)

The Orionids (ORI) reached maximum activity on October 22nd. Some activity may still be seen during the morning hours from a radiant located at 07:14 (109) +16. This position lies in southern Gemini, close to the faint magnitude star Lambda Geminorum. The radiant is best placed on the meridian near 0400 LDT. Current rates should be near two per hour no matter your location. At 67km/sec., the average Orionid is swift.

Leonids (LEO)

The Leonids (LEO) are just now coming to life from a radiant located at 09:50 (148) +25. This position lies in western Leo only one degree north of the third magnitude star Epsilon Leonis. Maximum activity is still more than a week away so current rates would most likely be less than one per hour. At 71km/sec., the average Leonid is swift with a high percentage of trains. These meteors are best seen during the last hour before the onset of morning twilight, when the radiant lies highest above the horizon in a dark sky.

Shower Name                 RA     DEC   Vel     Rates
                                         km/s   NH    SH
AND Andromedids           01h 27m  +27    19    <1    <1
NTA Northern Taurids      03h 38m  +22    29     3     3
STA Southern Taurids      03h 42m  +14    29     2     2
ORI Orionids              07h 14m  +16    67     2     2
LEO Leonids               09h 50m  +25    71    <1    <1

RA - Right Ascension
DEC - Declination
Vel - Velocity relative to Earth (in km per sec)
Rates - Rate of visible meteors per hour from a
        dark site
NH - Northern Hemisphere
SH - Southern Hemisphere

Meteor Activity Outlook for October 30-November 5, 2010

The Meteor Activity Outlook is a weekly summary of expected meteor activity written by Robert Lunsford, Operations Manager of the American Meteor Society and contributor to this blog. The original unedited version of this week’s Meteor Activity Outlook can be found at the American Meteor Society’s site.

As seen from the northern hemisphere, meteor rates continue to be strong in November. While no major activity is expected this month, the two Taurid radiants plus the Leonids keep the skies active. The addition of strong sporadic rates make November one of the better months to view meteor activity from north of the equator. Skies are fairly quiet as seen from the southern hemisphere this month. Activity from the three showers mentioned above may be seen from south of the equator, but the sporadic rates are much lower than those seen in the northern hemisphere.

During this period the moon wanes from its last quarter phase to nearly new at the end of the period. This weekend the half illuminated last quarter moon will rise near 0100 LDT (Local Daylight Time) and will remain in the sky the remainder of the night. While the moon at this phase is still bright, it is nowhere as bright as the full moon encountered the previous week. Successful meteor observations can be undertaken by simply keeping the moon far from your field of view. The observing situation improves further as the week progresses as the moon wanes and rises later and later during the morning hours. The estimated total hourly rates for evening observers this week is near six from the northern hemisphere and three for observers south of the equator. For morning observers the estimated total hourly rates should be near twenty from the northern hemisphere and twelve 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. Morning rates are reduced this week due to lunar interference.

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 October 30/31. These positions do not change greatly day to day so the listed coordinates may be used during this entire period.

The following showers are expected to be active this week:

Northern Taurids (NTA)

The center of the large Northern Taurid (NTA) radiant lies at 03:12 (048) +21. This area of the sky is located in eastern Aries, ten degrees southwest of the famous naked eye open cluster known as the Pleiades. The radiant is best placed near 0200 local daylight time (LDT), when it lies highest above the horizon. This shower peaks on November 13, so rates are slowly increasing. Current rates would be near two per hour, no matter your location. Meteors from the Northern Taurids strike the atmosphere at 29km/sec., which would produce meteors of slow velocity. This shower is also responsible for many of the fireball reports seen in November.

Southern Taurids (STA)

The center of the large Southern Taurid (STA) radiant lies at 03:16 (049) +12. This area of the sky is located in eastern Aries, fifteen degrees southwest of the Pleiades. The radiant is also best placed near the meridian near 0200 LDT. We are now well past the October 10 maximum for this shower but rates will still remain near two per hour, no matter your location. Striking the atmosphere at 29 km/sec., the average Southern Taurid meteor travels slowly through the skies. This shower is also responsible for many of the fireball reports seen in October.

Eta Taurids (ETT)

Studies of the IMO video database by Sirko Molau and Juergen Rendtel has revealed a radiant located in Taurus this time of year. The Eta Taurids (ETT) are active from October 25 through November 3, with maximum occurring on October 25th. The current radiant position lies at 04:04 (061) +24, which lies in western Taurus, three degrees east of the Pleiades star cluster. The radiant is best placed near 0300 LDT, when it lies highest above the horizon. Meteors from the Eta Taurids strike the atmosphere at 47km/sec., which would produce meteors of average velocity. Expected rates would be less than one per hour, no matter your location.

Orionids (ORI)

The Orionids (ORI) reached maximum activity on October 22nd. Some activity may still be seen during the morning hours from a radiant located at 06:48 (102) +16. This position lies in southwestern Gemini, close to the second magnitude star Alhena (Gamma Geminorum). The radiant is best placed on the meridian near 0500 LDT. Current rates should be near three per hour no matter your location. At 67km/sec., the average Orionid is swift.

Beta Cancrids (BCN)

Another shower derived from the IMO video database is the Beta Cancrids (BCN). This shower is active from October 25-November 3 with a peak on the 27th. This shower has been known from visual observations for some time. Video analysis have confirmed the activity but from a slightly different portion of the sky. The radiant was suspected to be active from the Cancer/Gemini border when in fact the position actually lies in the constellation of Monoceros, to the south. The radiant is located at 07:32 (113) -10, which is fifteen degrees south of the brilliant zero magnitude star Procyon (Alpha Canis Minoris). The radiant is best placed during the last dark hour before dawn when it lies highest above the horizon in a dark sky. Rates should less than one per hour. With an entry velocity of 65 km/sec., most activity from this radiant would be swift.

Shower Name                 RA     DEC   Vel     Rates
                                         km/s   NH    SH
NTA Northern Taurids      02h 28m  +18    29     1     1
STA Southern Taurids      01h 20m  +06    30     2     2
ETT Eta Taurids           04h 04m  +24    47    <1    <1
ORI Orionids              06h 08m  +16    67     3     3
BCN Beta Cancrids         07h 32m  -10    65    <1    <1

RA - Right Ascension
DEC - Declination
Vel - Velocity relative to Earth (in km per sec)
Rates - Rate of visible meteors per hour from a
        dark site
NH - Northern Hemisphere
SH - Southern Hemisphere

Meteor Activity Outlook for October 23-29, 2010

The Meteor Activity Outlook is a weekly summary of expected meteor activity written by Robert Lunsford, Operations Manager of the American Meteor Society and contributor to this blog. The original unedited version of this week’s Meteor Activity Outlook can be found at the American Meteor Society’s site.

Meteor activity in general increases in October when compared to September. A major shower (the Orionids) is active most of the month along with several minor showers. Both branches of the Taurids become more active as the month progresses, providing slow, graceful meteors to the nighttime scene. The Orionids are usually the big story of the month but this year the Orionid peak coincides with the full moon, which will severely reduce the number of meteors seen. Orionid activity can be seen before and after maximum when the moon is not so troublesome. Unfortunately on these nights the Orionid rates will be low, most likely less than five per hour.

During this period the moon is full on the 23rd and wanes toward last quarter, which is reached on the 30th. The bright moon will make observing meteors difficult as only the brightest ones can be seen in the lunar glare. Those viewing under transparent skies will have better success as the moonlight will be less scattered. The estimated total hourly rates for evening observers this week is near four from the northern hemisphere and two for observers south of the equator. For morning observers the estimated total hourly rates should be near twelve from the northern hemisphere and nine 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. Rates are reduced this week due to lunar interference.

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 October 23/24. These positions do not change greatly day to day so the listed coordinates may be used during this entire period.

The following showers are expected to be active this week. The detailed descriptions will be continued next week when the moonlight is not as intense.

Shower Name                 RA     DEC   Vel     Rates
                                         km/s   NH    SH
OUI October Ursa Minorids 18h 12m  +74    28    <1    <1
NTA Northern Taurids      02h 52m  +20    29     1    <1
STA Southern Taurids      02h 32m  +11    30     2     2
ETT Eta Taurids           04h 00m  +24    47    <1    <1
ORI Orionids              06h 32m  +16    67     5     5
EGE Epsilon Geminids      07h 04m  +27    70    <1    <1
BCN Beta Cancrids         07h 12m  -03    65    <1    <1
LMI Leonis Minorids       10h 48m  +36    60    <1    <1

RA - Right Ascension
DEC - Declination
Vel - Velocity relative to Earth (in km per sec)
Rates - Rate of visible meteors per hour from a
        dark site
NH - Northern Hemisphere
SH - Southern Hemisphere

Meteor Activity Outlook for October 16-22, 2010

The Meteor Activity Outlook is a weekly summary of expected meteor activity written by Robert Lunsford, Operations Manager of the American Meteor Society and contributor to this blog. The original unedited version of this week’s Meteor Activity Outlook can be found at the American Meteor Society’s site.

Meteor activity in general increases in October when compared to September. A major shower (the Orionids) is active most of the month along with several minor showers. Both branches of the Taurids become more active as the month progresses, providing slow, graceful meteors to the nighttime scene. The Orionids are usually the big story of the month but this year the Orionid peak coincides with the full moon, which will severely reduce the number of meteors seen. Orionid activity can be seen before and after maximum when the moon is not so troublesome. Unfortunately on these nights the Orionid rates will be low, most likely less than five per hour.

During this period the moon waxes from just past its first quarter phase to nearly full at the end of the period. This weekend the waxing gibbous moon will set during the early morning hours and will allow a couple of hours of dark skies before the beginning of twilight. This window of opportunity will shrink as the week progresses becoming essentially zero by the end of the week. The estimated total hourly rates for evening observers this week is near three from the northern hemisphere and two for observers south of the equator. For morning observers the estimated total hourly rates should be near twenty four from the northern hemisphere and twelve 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 this week due to lunar interference.

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 October 16/17. These positions do not change greatly day to day so the listed coordinates may be used during this entire period.

The following showers are expected to be active this week:

October Ursa Minorids (OUI)

Studies of the IMO video database by Sirko Molau and Juergen Rendtel has revealed a radiant located in Draco this time of year. Earlier visual observations placed the radiant in Ursa Minor therefore this shower is known as the October Ursa Minorids (OUI). This shower is active from October 16-28 with maximum occurring on the 24th. The moon will greatly hamper observations of this shower, especially near maximum on the 24th. On Saturday evening the radiant is located at 18:44 (281) +76. This position lies in western Draco some fifteen degrees south (above) Polaris (Alpha Ursae Minoris). Although the radiant is circumpolar (never sets) for most of the northern hemisphere, it is best placed as soon as it becomes dark. Striking the atmosphere at 28 km/sec., the average October Ursa Minorid meteor travels medium-slow through the sky. This shower is best seen from high northern latitudes. It is almost impossible to see from the southern hemisphere. Even at maximum, rates should be less than one per hour no matter your location.

Northern Taurids (NTA)

Recent studies of the IMO video database has revealed that activity from the Northern Taurids (NTA) does not begin until October 19th. This is nearly one month after pervious published dates. Maximum activity does not occur until November 13th so current rates will be low, lower than its southern counterpart until late in the month. The current radiant position lies near 02:28 (037) +18, which is located in central Aries, six degrees southeast of the second magnitude star Hamal (Alpha Arietis). The radiant is best placed near 0200 local daylight time (LDT), when it lies highest above the horizon. Meteors from the Northern Taurids strike the atmosphere at 29km/sec., which would produce meteors of slow velocity. Expected rates would be near one per hour, no matter your location.

Southern Taurids (STA)

The center of the large Southern Taurid (STA) radiant lies at 02:32 (038) +10. This position lies on the Aries/Cetus border, three degrees west of the fourth magnitude star Mu Ceti. Since the radiant is so large, any meteor from eastern Pisces, northeastern Cetus, Aries, western Taurus, or northeastern Eridanus could be a candidate for this shower. The radiant is best placed near the meridian near 0200 LDT, but activity may be seen all night long. Although maximum activity occurred on the 10th, this is a flat plateau-like peak so activity should still be good this week. Expect to see up to three Southern Taurids per hour, no matter your location, when the radiant lies highest in the sky. Striking the atmosphere at 29 km/sec., the average Southern Taurid meteor travels slowly through the skies. This shower is also responsible for many of the fireball reports seen in October.

Sigma Arietids (SSA)

Another shower derived from the IMO video database is the Sigma Arietids (SSA). This shower is active from October 12-19 with a peak on the 19th. The radiant is located at 03:16 (049) +22. This position lies in eastern Aries, four degrees northeast of the fourth magnitude star Delta Arietis. The radiant is best placed near 0300 LDT, when it lies highest above the horizon. Rates should less than one per hour. With an entry velocity of 46 km/sec., most activity from this radiant would be of medium velocity. These meteors are well seen from all but the polar regions of the Earth.

Zeta Taurids (ZTA)

Another shower derived from the IMO video database is the Zeta Taurids (ZTA). This shower is active from October 12-17 with a peak on the 16th. The radiant is located at 05:26 (081) +11. This position actually lies in Orion, three degrees northwest of the third magnitude star Lambda Orionis. The radiant is best placed near 0500 LDT, when it lies highest above the horizon. Rates should less than one per hour. With an entry velocity of 61 km/sec., most activity from this radiant would be swift. These meteors would be seen equally well from either hemisphere.

Orionids (ORI)

The Orionids (ORI) reach maximum activity on Friday October 22nd. Unfortunately a nearby full moon will spoil the display. The radiant is currently located at 06:08 (092) +16. This position lies in northeastern Orion, very close to the fourth magnitude star Nu Orionis. The radiant rises near 300 LDT and is best placed on the meridian near 0500. Current rates for all locations would be near three to five per hour as seen after midnight. At 67km/sec., the average Orionid is swift.

Epsilon Geminids (EGE)

The Epsilon Geminids (EGE) are active from October 16th through the 27th. Maximum activity occurs on the 19th. The radiant is currently located at 06:40 (100) +29. This position lies on the Gemini/Auriga border, four degrees northwest of the third magnitude star Mebsuta (Epsilon Geminorum). This position is also close to the Orionid radiant. Care must taken for correct shower association. The Orionids will be far more numerous. Current rates are probably near one per hour for the northern hemisphere and less than one as seen from south of the equator. The radiant is best placed near 0600 LDT, when it lies highest above the horizon. At 70km/sec., the average Epsilon Geminid is swift.

October  Ura Majorids (OCU)

Another shower derived from the IMO video database is the October Ursa Majorids (OCU). This shower is active from October 12-19 with a peak on the 15th. On the 12th the radiant is located at 09:52 (148) +63. This position lies in western Ursa Major, fifteen degrees west of the second magnitude star Dubhe (Alpha Ursae Majoris). The radiant is best placed during the last dark hour before dawn when it lies highest above the horizon in a dark sky. Rates should less than one per hour. With an entry velocity of 53 km/sec., most activity from this radiant would be medium-swift. With the high northern declination of the radiant, these meteors are best seen from the northern hemisphere. It would be difficult to see any of this activity from locations south of the equator.

Leonis Minorids (LMI)

The Leonis Minorids (LMI) are active from October 16-27 with maximum activity occurring on October 23rd. ZHR’s are usually low but the radiant is far removed from the Orionids and Epsilon Geminids so that any possible shower members should be easily identified. Hourly rates would be less than one this week. This radiant is currently located at 10:16 (154) +35, which places it in northeastern Leo Minor, two degrees southwest of the fourth magnitude star Beta Leonis Minoris. The radiant is best placed just before dawn when it lies highest in a dark sky. This shower is better situated for observers situated in the northern hemisphere where the radiant rises far higher into the sky before the start of morning twilight. At 60km/sec., the average Leonis Minorid is swift.

As seen from the mid-northern hemisphere (45N) one would expect to see approximately fifteen 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 four per hour as seen from rural observing sites and one per hour during the evening hours. Locations between these two extremes would see activity between the listed figures. Evening rates are reduced due to moonlight.

The list below presents a condensed version of the expected activity this week. Rates and positions are exact for Saturday night/Sunday morning.

Shower Name                 RA     DEC   Vel     Rates
                                         km/s   NH    SH
OUI October Ursa Minorids 18h 44m  +76    28    <1    <1
NTA Northern Taurids      02h 28m  +18    29     1     1
STA Southern Taurids      02h 32m  +10    30     3     3
SSA Sigma Arietids        03h 16m  +22    46    <1    <1
ZTA Zeta Taurids          05h 26m  +11    61    <1    <1
ORI Orionids              06h 08m  +16    67     2     2
EGE Epsilon Geminids      06h 40m  +29    70     1    <1 
OCU October Ursa Majorids 09h 12m  +64    53     1    <1
LMI Leonis Minorids       10h 16m  +35    60    <1    <1

RA - Right Ascension
DEC - Declination
Vel - Velocity relative to Earth (in km per sec)
Rates - Rate of visible meteors per hour from a
        dark site
NH - Northern Hemisphere
SH - Southern Hemisphere

Meteor Activity Outlook for November 21-27, 2009

The Meteor Activity Outlook is a weekly summary of expected meteor activity written by Robert Lunsford, Operations Manager of the American Meteor Society and contributor to this blog. The original unedited version of this week’s Meteor Activity Outlook can be found at the American Meteor Society’s site.

As seen from the northern hemisphere, meteor rates continue to be strong in November. While no major showers are active this month, the two Taurid radiants plus the Leonids keep the skies active. The addition of strong sporadic rates make November one of the better months to view meteor activity from north of the equator. Skies are fairly quiet as seen from the southern hemisphere this month. Activity from the three showers mentioned above may be seen from south of the equator, but the sporadic rates are much lower than those seen in the northern hemisphere.

During this period the moon reaches its first quarter phase on Tuesday November 24th. On that date the moon lies ninety degrees east of the sun and will set near midnight local standard time (LST). This weekend the waxing crescent moon will set long before the more active morning hours arrive, allowing dark skies for those who venture out during the morning hours. As the week progresses the moon sets later each night narrowing the window of opportunity to view under dark conditions. The estimated total hourly rates for evening observers this week is near four as seen from the northern hemisphere and three from the southern hemisphere. For morning observers the estimated total hourly rates should be near twenty from the northern hemisphere and ten 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. Rates are reduced during the evening hours due to moonlight.

The radiant positions and rates listed below are exact for Saturday night/Sunday morning November 21/22. These positions do not change greatly day to day so the listed coordinates may be used during this entire period.

The following showers are expected to be active this week.

Andromedids (AND)

Sirko Molau’s studies of video radiants has revealed that activity from the famous Andromedid shower, noted for intense storms during the 19th century, may still be seen throughout November. This position lies in eastern Andromeda, two degrees south of the fourth magnitude star Nu Andromedae. The nearest bright star is second magnitude Almach (Gamma Andromedae), which lies four degrees to the northeast. Visual activity is expected to be low, but detectable. The Andromedid radiant is best placed near 2200 (10pm) local standard time (LST) when it lies on the meridian. At 19km/sec., the average Andromedid will appear as a very slow moving meteor. Sirko mentions that these meteors are “conspicuously slow and of almost constant activity” during this period.

Northern Taurids (NTA)

The Northern Taurids (NTA) are active from a large radiant centered at 04:29 (067) +24, which lies in northern Taurus, eight degrees north of the orange first magnitude star Aldebaran (Alpha Tauri). The radiant is best placed near 0100 LST, when it lies highest above the horizon, but activity may be seen all night long. Meteors from the Northern Taurids strike the atmosphere at 29km/sec., which would produce meteors of slow velocity. Expected rates would be ~3 per hour as seen from the northern hemisphere and ~2 per hour as seen south of the equator.

November Orionids (NOO)

The November Orionids (NOO) were recently discovered by analyzing video data. This shower is active from November 18 through December 9. Maximum activity occurs on November 30. The radiant is currently (11/18) located at 05:44 (086) +15. This position lies on the Orion/Taurus border, six degrees north of the third magnitude star Lambda Orionis. These meteors are also best seen near 0300 LST when the radiant lies on the meridian and highest above the horizon. At 44 km/sec. the November Orionids produce mostly medium velocity meteors.

Alpha Monocerotids (AMO)

The Alpha Monocerotids (AMO) are active from November 15-25, with maximum occurring on the 21st. This shower has produced outbursts in the past but none are expected for many years to come. Rates are expected to be < 1 shower member per hour, even on the night of maximum activity. The radiant is currently located at 07:52 (118) +01. This position lies in southeastern Canis Minor, five degrees southeast of the zero magnitude star Procyon (Alpha Canis Minoris). These meteors are also best seen near 0500 LST when the radiant lies highest above the horizon in a dark sky. At 65 km/sec. the Alpha Monocerotids produce mostly swift meteors.

Leonids (LEO)

The Leonids (LEO) reached maximum activity on the morning of November 17th with ZHR’s exceeding 100 as seen over Asia. Current rates would be near one per hour no matter your location. The radiant is currently located at 10:27 (157) +20. This position lies in western Leo, just one degree northeast of the famous second magnitude double star Algeiba (Gamma Leonis). At 70km/sec., the average Leonid is swift with a high percentage of trains. The radiant does not rise until the late evening hours so it is advised to wait until after midnight before beginning serious observations. The radiant is most favorably located during the last dark hour before the onset of morning twilight when it lies highest in a dark sky.

As seen from the mid-northern hemisphere (45N) one would expect to see ~16 Sporadic meteors per hour during the last hour before dawn as seen from rural observing sites. Evening rates would be ~3 per hour. As seen from the mid-southern hemisphere (45S), morning rates would be ~6 per hour as seen from rural observing sites and ~2 per hour during the evening hours. Locations between these two extremes would see activity between the listed figures.

The table below presents a condensed version of the expected activity this week. Rates and positions are exact for Saturday night/Sunday morning but may be used all week long.

Shower Name                RA     DEC   Vel     Rates
                                        km/s   NH    SH
AND Andromedids          01h 38m  +39    19    <1    <1
NTA Northern Taurids     04h 29m  +24    29     3     2
AMO Alpha Monocerotids   07h 52m  +01    65    <1    <1
LEO Leonids              10h 27m  +20    70     1     1

RA - Right Ascension
DEC - Declination
Vel - Velocity relative to Earth (in km per sec)
Rates - Rate of visible meteors per hour from a
        dark site
NH - Northern Hemisphere
SH - Southern Hemisphere
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