Re: (meteorobs) Perseid stream spread (was: NAMN Notes: July 1999)

• To: meteorobs@jovian.com
• Subject: Re: (meteorobs) Perseid stream spread (was: NAMN Notes: July 1999)
• From: GeoZay@aol.com
• Date: Tue, 13 Jul 1999 21:02:49 EDT
• Reply-To: meteorobs@jovian.com
• Sender: owner-meteorobs@jovian.com

In a message dated 99-07-13 20:22:36 EDT, you write:

<< 
 
 Wayne makes the point (I think) that there are a number of other radiants
 which are much larger, even based on true radar and photographic studies!
 However, many of those are Ecliptic radiants, subject to a wide variety of
 well-understood perturbations, and some actually represent more radiant
 "complexes" than true single-stream radiants.
 
 Last I looked though, Perseus was pretty far off the Ecliptic! ;> So my
 question is, "Why is the Perseid radiant so large in diameter"?
 
 Clear skies, and thanks for the clarifying questions, guys!
  >>
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