[neo_followup] Improved 1964-054A = OGO-1 data, ephems
Bill Gray
pluto at projectpluto.com
Thu Aug 27 17:23:08 EDT 2020
Just got my first post-perigee data. The object was a few
arcminutes off prediction (8' north, 6' east), corresponding
to an AMR of 0.046. So modify my earlier message : if you
turn on SRP and constrain A=0.046, you'll nail the object
within an arcsecond or two. More later...
-- Bill
On 8/27/20 11:30 AM, Bill Gray wrote:
> Hello all,
>
> I found quite a bit of additional data for this object in
> my inbox this morning (thank you!). At present, I've got
> 46 observations from the current orbit :
>
> https://www.projectpluto.com/temp/ogo1.txt
>
> A correction to my previous e-mail : you can just download
> the above file and feed it into Find_Orb, either "current"
> Windows or Linux, or on-line, or the old Windows GUI version,
> and compute ephemerides for your location that should be good
> to within a few arcminutes. That's about the level of effect
> I expect the upcoming perigee (occurring as I write) to have.
>
> You can still turn on solar radiation pressure (by hitting
> the '*' key) and constrain the area/mass ratio to be A=0.03,
> and get suitably adjusted results. But unless you have a
> small field of view, the non-SRP version should at least let
> you find the object.
>
> The good news is that, if the nominal AMR makes a five
> arcminute difference (300") and the object is measured to an
> arcsecond, it means the effects of atmospheric drag during
> that pass will be measured to about one part in 300. Which
> is pretty good. And we'll probably get enough data to
> _really_ nail down the re-entry time and location.
> (Currently looks to be at about 21:00 UTC on the 29th over
> French Polynesia, but a little more or less drag could
> make that prediction look stupid.)
>
> This may be a useful exercise to prepare for something
> like the 1972 fireball that zipped through the atmosphere,
> lost lots of speed, and probably was left in Earth orbit
> and crashed at the next perigee.
>
> -- Bill
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