(meteorobs) Eta Aquariids 2007
meteors at eclipse.net
meteors at eclipse.net
Wed Apr 25 12:06:16 EDT 2007
And certainly, the moon, 86% illuminated, will be a hindrance to
observations everywhere :(
> Dear all,
>
> I am Mikiya Sato. I was not sending mail for a long time, sorry!
>
> I calculated the trail of Eta Aquariids in 2007, as already announced
> by CBET 944 and Quanzhi's mail.
> Two parts of a trail that was ejected from 1P/Halley in -835 (836 BC)
> will approach to the Earth, about May 6.6.
> The outline is as follows.
>
> E.Y DATE (UT) TIME LS Delta-r Ej.V fM RP-Alp. Del. Vg(km/s)
> -835 May.06.56 13:28 45.553 +0.00068 -20.29 0.018 337.72 -0.91 65.93
> -835 May.06.62 14:57 45.613 -0.00010 -20.26 0.046 337.76 -0.89 65.95
> *Ej.V: Ejection Velocity (m/s)
>
> This trail is very old and the shape is very complex due to
> perturbations of Jupiter. So the peak will not be sharp,
> a long peak might be observed.
>
> But, it is difficult to guess the activity because the detail
> of other years was not calculated.
> Moreover, the fM value of this Aquariids is smaller than the
> value of another trails of last Orionids. And the usual ZHR of
> Eta Aquariids is very high (about 60? at the southern hemisphere),
> so the peak might not be separated if the activity of this peak
> is a low level.
>
> However, it is a good opportunity that the influence of the dust
> trail from 1P/Halley can be observed. In Japan, the observation
> condition is not so good.
> So, I hope to be observed at the wide region in the world.
>
> Please refer to the following my web for a figure etc.
>
> http://fas.kaicho.net/tenshow/meteor/1p2007/EAqr2007.htm
>
> Best wishes,
>
> Mikiya Sato
> mail at kaicho.net
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