Mónika Landy-Gyebnár captured this multi-bursting South Taurid fireball on October 26, 2022, at 03:43 CEST (1:43 UT) from Hárskút, Hungary. She commented “First it was very bright (-2 magnitudes) and green then quickly faded, still remained visible for 5 minutes, twisted and drifted away, upwards. Then the thin clouds covered it. ©Mónika Landy-Gyebnár

As seen from the northern hemisphere, June is another slow month for meteor activity. There are no major showers active in June and only the Anthelion source can be counted on for continuous activity. Sporadic rates continue to remain low as seen from the mid-northern hemisphere (45 N) with only half the rates seen from the mid-southern hemisphere. For the upper half of the northern hemisphere the nights are short to non-existent this time of year. As seen from the southern tropics (25 S) sporadic rates continue to be strong this month with morning hourly rates near 10.

During this period, the moon reaches its full phase on Sunday June 4th. On that date it will lie above the horizon all night long. As the week progresses, the moon rises approximately 45 minutes later each night. Toward the end of this period the evening hours are free of interfering moonlight. Unfortunately, during the evening hours meteor rates are low this time of year. The estimated total hourly rates for evening observers this week should be near 2 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 4 as seen from mid-northern latitudes (45N) and 6 as seen from tropical southern locations (25S). The actual rates seen 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 this period due to bright 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 brighter 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 June 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. I have also included charts of the sky that display the radiant positions for evening, midnight, and morning. The center of each chart is the sky directly overhead at the appropriate hour. These charts are oriented for facing south but can be used for any direction by rotating the charts to the desired direction. 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 its 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 sporadic. Meteor activity is not seen from radiants that are located far 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.

Radiant Positions at 23:00 LST

Radiant Positions at 23:00 Local Summer Time

Radiant Positions at 01:00 LST

Radiant Positions at 01:00 Local Summer Time

Radiant Positions at 03:00 LST

Radiant Positions at 03:00 Local Summer Time

These sources of meteoric activity are expected to be active this week.

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The center of the large Anthelion (ANT) radiant is currently located at 17:44 (266) -23. This position lies on the Ophiuchus/Sagittarius border, 4 degrees northeast of the 3rd magnitude star known as theta Ophiuchi. Due to the large size of this radiant, Anthelion activity may also appear from western Sagittarius as well as southern Ophiuchus. This radiant is best placed near 0100 LST, when it lies on the meridian and is located highest in the sky. Rates at this time should be less than 1 per hour as seen from the Northern Hemisphere and 1 per hour as seen from south of the equator. With an entry velocity of 30 km/sec., the average Anthelion meteor would be of slow velocity.

The Daytime Arietids (ARI) are active from May 29-June 17 with maximum activity occurring on June 5th. These meteors are difficult to catch as the radiant only lies 30 degrees west of the sun. Therefore, the only time these meteors are visible is during the last dark hour before dawn. Any member of this shower will be see shooting from low in the eastern sky just prior to dawn. The radiant is currently located at 02:44 (041) +24. This area of the sky is located in northern Aries, 4 degrees southwest of the 4th magnitude star known as Bharani (41Aa Arietis). Current rates are expected to be less than 1 no matter your location. With an entry velocity of 39 km/sec., the average meteor from this source would be of medium velocity. For radio observers, this is the best time of the year to hear meteors. Radio rates will be increasing now and will peak during the second week of June when this shower and the Daytime zeta Perseids reach maximum activity.

As seen from the mid-northern hemisphere (45N) one would expect to see approximately 3 sporadic meteors per hour during the last hour before dawn as seen from rural observing sites. Evening rates would be near 1 per hour. As seen from the tropical southern latitudes (25S), morning rates would be near 5 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 are reduced due to intense moonlight.

The list below offers the information in tabular form. 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 Summer Time North-South
Anthelion (ANT) 17:44 (266) -23 30 02:00 <1 – 1 II
Daytime Arietids (ARI) Jun 07 02:44 (041) +24 39 11:00 <1 – <1 I

 

Class Explanation: A scale to group meteor showers by their intensity:

  • Class I: the strongest annual showers with Zenith Hourly Rates normally ten or better.
  • Class II: reliable minor showers with ZHR’s normally two to ten.
  • Class III: showers that do not provide annual activity. These showers are rarely active yet have the potential to produce a major display on occasion.
  • Class IV: weak minor showers with ZHR’s rarely exceeding two. The study of these showers is best left to experienced observers who use plotting and angular velocity estimates to determine shower association. These weak showers are also good targets for video and photographic work. Observers with less experience are urged to limit their shower associations to showers with a rating of I to III.

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