Bi2L Δημοσιεύτηκε Ιούλιος 1, 2008 Δημοσιεύτηκε Ιούλιος 1, 2008 α-Capricornids (CAP) Active: July 3 — August 15Maximum: July 29 (λsol = 127°)ZHR = 4Radiant: α = 307° δ = -10°Radiant drift: see Table 6vinf = 23 km/s; r = 2.5TFC: α = 255° to 000° δ = 00° to +15° choose pairs separated by about 30° in α (β < 40° N)IFC: α = 300° δ = +10° (β > 45° N) α = 320° δ = -05° (β 0° to 45° N) α = 300° δ = -25° (β < 0°) The α-Capricornids and SDA were both definitely detected visually in former years, standing out against the much weaker other radiants supposed active in Capricornus-Aquarius then. Whether the CAP can still be detected separately from the new ANT radiant area remains to be discovered, as its radiant now partly overlaps that of the large ANT oval region. In their favour, CAP meteors are noted for being bright, at times even of fireball-class, which, combined with their low apparent velocity, can make some of these objects among the most impressive and attractive an observer could wish for. A minor enhancement of CAP ZHRs to ~ 10 was noted in 1995 by European IMO observers. More recent results suggest the maximum may continue for an extra day, so perhaps from July 29 — 30 this year. Βασίλης ΜεταλληνόςOO 16 1600 f4ΟΟ 12.5 1525 f4.8 NEQ6TOA130 1000 f7.7 ΕΜ200ED80 600 f7.5, Vixen9x63Canon eos 6D, Sony a7s2, Wat120n+,Asi1202009年7月22號日食 - 2017 Aug 21www.metallinos.net
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