Beta Taurids | |
---|---|
Discovery date | 1947[1] |
Parent body | 2P/Encke (Taurid Complex) 2004 TG10[2] |
Radiant | |
Constellation | Taurus (near Zeta Tauri) |
Properties | |
Occurs during | June 5 – July 18[1] |
Date of peak | June 28–29[3][1] |
Zenithal hourly rate | 25 (radar)[1] |
Notable features | Daytime shower |
The Beta Taurids (β–Taurids) are an annual meteor shower belonging to a class of "daytime showers" that peak after sunrise. The Beta Taurids are best observed by radar and radio-echo techniques.
The Beta Taurids are normally active from June 5 to July 18.[1] They emanate from an average radiant of right ascension 5h18m, declination +21.2 and exhibit maximum activity around June 28–29 (Solar Longitude=98.3 deg).[a] The maximum hourly rate typically reaches about 25 as seen on radar.[1] Non-radio observers are faced with a very difficult prospect, because the Beta Taurid radiant is just 10–15 degrees west of the Sun on June 28.[4][b]
These Beta Taurids are the same meteoroid stream as the Taurids (which form a meteor shower in late October). The Earth intersects this stream of debris twice, once in late October and once in late June, forming two separate meteor showers. However, because the October event occurs at night, it is far more visible and better known than the Beta Taurids, which peak during daylight hours.
Asteroids associated with the β–Taurids include 2201 Oljato, 5143 Heracles, 6063 Jason, (8201) 1994 AH2 and 1991 BA.[5]
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