(meteorobs) Meteor Activity Outlook for January 10-16, 2015
Richard Kramer
kramer at sria.com
Thu Jan 8 17:26:35 EST 2015
Robert,
This week's Outlook is all jammed together and
very difficult to read. Apparently, you sent it in a different way this week.
Regards,
Richard
At 05:03 PM 1/8/2015, you wrote:
>During this period the moon reaches its last
>quarter phase on Tuesday January 13th. At this
>time the moon is located 90 degrees west of the
>sun and rises near midnight local standard time
>(LST). At this time evening skies are dark but
>the light of the half illuminated moon will
>interfere with observing during the morning
>hours. This weekend the waning gibbous moon will
>hamper viewing meteor activity after 2200 (10pm)
>LST. The estimated total hourly meteor rates
>for evening observers this week is near 3 as
>seen from the northern hemisphere (45N) and 2 as
>seen from southern tropical latitudes (25S). For
>morning observers the estimated total hourly
>rates should be near 10 as seen from the
>northern hemisphere and 8 as seen from south of
>the equator. 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 during the morning hours are reduced due
>to interfering moonlight. 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 January 10/11.
>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 center of the large
>Anthelion (ANT) radiant is currently located at
>08:12 (123) +18. This position lies in western
>Cancer, 4 degrees west of the 4th magnitude star
>Asellus Australis (Delta Cancri). Due to the
>large size of this radiant, Anthelion activity
>may also appear from western Leo, Gemini, Canis
>Minor, northwestern Hydra as well as Cancer.
>This radiant is best placed near midnight LST,
>when it lies on the meridian and is located
>highest in the sky. Rates at this time should be
>near 2 per hour as seen from the northern
>hemisphere and 1 per hour from south of the
>equator. With an entry velocity of 30 km/sec.,
>the average Anthelion meteor would be of slow
>velocity. The December Leonis Minorids (DLM) are
>active from a radiant located at 12:04 (181)
>+21. This position lies in western Coma
>Berenices, 7 degrees northeast of the 2nd
>magnitude star Denebola (Beta Leonis). These
>meteors are best seen near 0400 LST when the
>radiant lies highest above the horizon. This
>shower peaked on December 21st so current rates
>would be less than 1 per hour no matter your
>location. At 63 km/sec. the December Leonis
>Minorids produce mostly swift meteors. The Canum
>Venaticids (CVN) are a new shower discovered by
>Peter Brown and his associates at the University
>of Western Ontario, using meteor orbits obtained
>by radar. This activity was verified by the IMO
>video network which has 271 possible candidates
>in its database. This shower is best seen from
>January 13-18, with maximum activity occurring
>on the 15th. At maximum the radiant is located
>at 14:00 (210) +38, which places it in eastern
>Canes Venatici, 6 degrees west of the 3rd
>magnitude star Seginus (Gamma Boötis). These
>meteors encounter the atmosphere at 56 km/sec.,
>which would produce mostly medium-swift meteors.
>These meteors are best seen during the last few
>hours before dawn, when the radiant lies highest
>in a dark sky. This activity would be difficult
>to view from the southern hemisphere as the
>radiant lies low in the north at dawn. The X
>Corona Borealids (XCB) are another new shower
>discovered by Peter Brown and his associates at
>the University of Western Ontario. This shower
>is best seen from January 11-18, with maximum
>activity occurring on the 15th. At maximum the
>radiant is located at 16:36; (249) +30, which
>actually places it within the borders of
>Hercules, 2 degrees southwest of the 3rd
>magnitude star Zeta Herculis. These meteors
>encounter the atmosphere at 49 km/sec., which
>would produce meteors of average velocity. These
>meteors are best seen during the last few hours
>before dawn, when the radiant lies highest in a
>dark sky. This activity would be difficult to
>view from the southern hemisphere as the radiant
>lies low in the north at dawn. As seen from the
>mid-northern hemisphere (45N) one would expect
>to see approximately 7 sporadic meteors per hour
>during the last hour before dawn as seen from
>rural observing sites. Evening rates would be
>near 2 per hour. As seen from the tropical
>southern latitudes (25S), morning rates would be
>near 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. Rates
>during the morning hours are reduced due to
>interfering moonlight. The list below offers the
>information from above in tabular form. Rates
>and positions are exact for Saturday
>night/Sunday morning except where noted in the
>shower descriptions. Anthelion (ANT) - 08:12
>(123) +18 Velocity - 30km/sec. Northern
>Hemisphere - 2 per hr. Southern Hemisphere - 1
>per hr. Dec. Leonis Minorids (DLM) - 11:14 (169)
>+27 Velocity - 64km/sec. Northern Hemisphere -
>1 per hr. Southern Hemisphere - 1 per hr.
>Canum Venaticids (CVN) - 14:00 (210)
>+38 Velocity - 56km/sec. Northern Hemisphere -
><1 per hr. Southern Hemisphere - <1 per hr X
>Coronae Borealids (XCB) - 16:36 (249)
>+30 Velocity - 49km/sec. Northern Hemisphere -
><1 per hr. Southern Hemisphere - <1 per
>hr Clear Skies! Robert Lunsford American
>Meteor
>Society
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