NEO
Confirmation &
Ephemeris
Grabbing the Ephemeris Text
First create an "Ephemeris" for your
observatory code using the
NEO Confirmation
Page. The following example is using Observatory ID:673.

Followed by the actual text,
Date UT * R.A. (J2000) Decl. Elong. V Motion Object Sun Moon
h "/min P.A. Azi. Alt. Alt. Phase Dist. Alt.
2005 09 27 16 00 17 31.1 -06 01 04 172.2 18.9 3.99 066.8 106 -32 +27 0.28 120 +80 !
2005 09 27 17 00 17 47.1 -05 59 32 172.2 18.9 4.53 070.5 118 -43 +38 0.28 120 +71 !
2005 09 27 18 00 18 05.2 -05 58 03 172.2 18.9 4.92 073.0 134 -53 +47 0.27 120 +59 !
2005 09 27 19 00 18 24.7 -05 56 39 172.2 18.9 5.14 074.6 158 -60 +53 0.27 121 +47 !
2005 09 27 20 00 18 44.8 -05 55 20 172.2 18.9 5.16 075.7 189 -61 +54 0.26 121 +35 !
2005 09 27 21 00 19 04.7 -05 54 06 172.2 18.9 4.98 076.1 217 -57 +49 0.26 122 +23 !
2005 09 27 22 00 19 23.5 -05 52 56 172.2 18.9 4.61 075.9 236 -48 +41 0.26 122 +12 !
2005 09 27 23 00 19 40.4 -05 51 50 172.2 18.9 4.07 074.8 250 -36 +31 0.25 122 +01 !
2005 09 28 00 00 19 54.9 -05 50 48 172.2 18.9 3.41 072.6 260 -25 +20 0.25 123 -09 !
2005 09 28 01 00 20 06.5 -05 49 47 172.2 18.9 2.67 068.1 269 -12 +07 0.25 123 -18 !
2005 09 28 02 00 20 14.8 -05 48 48 172.2 18.9 1.94 059.1 277 +00 -05 0.24 124 -25 !
2005 09 28 03 00 20 19.9 -05 47 47 172.2 18.9 1.33 040.4 286 +12 -17 0.24 124 -30 !
2005 09 28 04 00 20 21.8 -05 46 45 172.2 18.9 1.06 007.0 296 +24 -29 0.24 125 -33 !
2005 09 28 05 00 20 21.1 -05 45 41 172.2 18.9 1.21 336.4 308 +35 -41 0.23 125 -31 !
2005 09 28 06 00 20 18.1 -05 44 32 172.2 18.9 1.51 321.6 324 +43 -50 0.23 126 -27 !
2005 09 28 07 00 20 13.8 -05 43 19 172.2 18.9 1.73 316.5 344 +49 -56 0.23 126 -20 !
2005 09 28 08 00 20 08.8 -05 42 01 172.2 18.9 1.82 317.2 007 +50 -58 0.22 127 -12 !
2005 09 28 09 00 20 04.1 -05 40 38 172.2 18.9 1.78 323.0 029 +46 -53 0.22 127 -02 !
2005 09 28 10 00 20 00.5 -05 39 11 172.2 18.9 1.64 335.0 046 +38 -44 0.22 128 +09 !
2005 09 28 11 00 19 58.8 -05 37 40 172.2 18.9 1.55 354.6 060 +29 -34 0.21 128 +21 !
2005 09 28 12 00 19 59.5 -05 36 06 172.3 18.9 1.68 018.8 070 +17 -22 0.21 129 +32 !
2005 09 28 13 00 20 03.2 -05 34 29 172.3 18.9 2.08 039.3 080 +05 -10 0.21 129 +44 !
2005 09 28 14 00 20 10.2 -05 32 53 172.3 18.9 2.67 052.9 088 -07 +03 0.20 130 +56 !
2005 09 28 15 00 20 20.4 -05 31 16 172.3 18.9 3.33 061.5 097 -19 +15 0.20 130 +67 !
2005 09 28 16 00 20 33.6 -05 29 42 172.3 18.9 3.97 066.9 106 -32 +27 0.20 130 +76 !
When the Ephemeris text is listed in your
browser use your mouse to drag and highlight the text as
shown below. When highlighted RIGHT MOUSE Click and use the option to
"COPY" the text from the menu and it will be copied to the clipboard as shown below.
Ignore the heading AU52949 and "No comments so
far!" They are not needed. However, you will be saving the TEXT file
with the name "AU52949.TXT"!
Next launch any text editor like WordPad, or NotePad. I prefer WORDPAD myself
for this. The key is you MUST use the Edit |
Paste Special option! Using this Paste option the text will not be
formatted in anyway.
Microsoft WordPad

Use Paste Special
You do not want the text to be formatted.
The header text will not work if you have altered the data in any way.
Just one column shift causes the header to be inaccurate.
And then Select the

Unformatted Text Option
The text from the NEO Confirmation page will look as follows,
Date UT * R.A. (J2000) Decl. Elong. V Motion Object Sun Moon Uncertainty
h "/min P.A. Azi. Alt. Alt. Phase Dist. Alt.
2005 07 12 21 21 01 49.5 +45 54 17 109.0 17.4 39.28 151.2 175 -10 +71 0.33 118 +31 Map/Offsets
2005 07 12 22 21 03 37.2 +45 19 53 109.4 17.4 39.17 151.4 185 -10 +60 0.33 119 +41 Map/Offsets
2005 07 12 23 21 05 22.7 +44 45 31 109.9 17.4 39.02 151.7 196 -09 +48 0.34 119 +50 Map/Offsets
Now by attaching the header text that follows you have everything you
will need to plot this Ephemeris data in TheSky. The text will be compiled
into an SDB file TheSky database file using TheSky's Database Compiler.
Here is the header text that defines the fields of information for the text.
You can highlight the following text and copy it to the clipboard to save it.
Or
DOWNLOAD header text here! Choose Save As to save the text header to
your hard disk. Or just mouse drag the text that follows and copy it to
the clipboard.
>SEARCH 1,18
>RAHOURS 19,20
>RAMINUTES 22,23
>RASECONDS 25,29
>SEARCH 1,18
>DECSIGN 30,30
>DECDEGREES 31,32
>DECMINUTES 34,35
>DECSECONDS 37,38
>MAGNITUDE 47,50
>OBJECT TYPE 55
>IDENTIFIER NEO's from MPC
>PARSE "Date U.T." 1,18
>PARSE "Elong." 40,44
>PARSE "Motion arc secs/min" 53,58
>PARSE "P.A." 60,65
>PARSE "Object Alt. Az." 66,78
>PARSE "Sun Alt." 78,84
>PARSE "Moon Phase Dist. Alt." 85,102
>PARSE "Uncertainty" 103,114
Now add the header text (EDIT COPY | EDIT PASTE) to the Ephemeris data as shown below.
>SEARCH 1,18
>RAHOURS 19,20
>RAMINUTES 22,23
>RASECONDS 25,29
>SEARCH 1,18
>DECSIGN 30,30
>DECDEGREES 31,32
>DECMINUTES 34,35
>DECSECONDS 37,38
>MAGNITUDE 47,50
>OBJECT TYPE 55
>IDENTIFIER NEO AU52949
>PARSE "Date U.T." 1,18
>PARSE "Elong." 40,44
>PARSE "Motion arc secs/min" 53,58
>PARSE "P.A." 60,65
>PARSE "Object Alt. Az." 66,78
>PARSE "Sun Alt." 78,84
>PARSE "Moon Phase Dist. Alt." 85,102
>PARSE "Uncertainty" 103,114
;Date UT * R.A. (J2000) Decl. Elong. V Motion Object Sun Moon Uncertainty
h "/min P.A. Azi. Alt. Alt. Phase Dist. Alt.
2005 07 12 21 21 01 49.5 +45 54 17 109.0 17.4 39.28 151.2 175 -10 +71 0.33 118 +31 Map/Offsets
2005 07 12 22 21 03 37.2 +45 19 53 109.4 17.4 39.17 151.4 185 -10 +60 0.33 119 +41 Map/Offsets
2005 07 12 23 21 05 22.7 +44 45 31 109.9 17.4 39.02 151.7 196 -09 +48 0.34 119 +50 Map/Offsets
... and so on
The new text file is both the header text and the
ephemeris text data combined. Save the new TEXT file with the name of the
NEO for convenience. Using WORDPAD use File Save As and enter the name
AU52949.TXT making it easy to identify. Place the text file in any
folder you like. Better yet use the My Documents Folder and create a NEW
SDB folder named something like "NEO SDB's". You must remember where you
have placed the files because you will need to load them from TheSky.
Once the new combined text files have been saved they will
need to be compiled using TheSky's Data | Import.
Data | Import

Select Object Type Reference Point
and Load to memory as shown
Next click the Browse button highlighted
above to locate the TEXT file you have created. See below. You will
have to locate the FOLDER that contains the text file. In my example My
Documents | NEO SDB's folder as shown.
Find the text file you created

with the header and ephemeris data
Once you have found the file note the
Identifier is "NEO AU52949". This is being filled in from the header
text above. The folder name being used is also displayed. If you do
not see the identifier "NEO's from MPC" display you HAVE NOT loaded the correct
text file. That is the text file does not have the header.
Check Identifier field first

Also check "Load To Memory"
Now just use the COMPILE button located on
the Import dialog to create the SDB file. You will be asked to Add to Auto
Load Database List answer yes.
Auto Load?

Answer "Yes"
You will know if the data is successfully
compiled. The Import dialog shows how many objects were found in the data
and the purple dots represent the location of the objects in the sky.
The more objects you have the easy the purple dot distribution is to see!
Data has been compiled

Now the Ephemeris can be accessed
Now, because the ephemeris data has been
compiled as object type "Reference Point" these must be set to visible to see
them! Use
the View | Display Explorer to check this. Just
type in "Reference Point" in the field "Go to:" and you are taken directly to
the object type "Reference Point". See below. Place a check next to
"Reference
Point" to make them visible.
View | Display Explorer

Enable Reference Point
Because the text header has a "SEARCH" field
specified you can use the Find dialog to show the individual SDB entries. This
makes centering on them easy. Check mark the options "Frame Object" and
"Object information" on the top of the Find dialog. Next go down under the
Sky Databases (SDBs) entry and expand the SDB file named "NEO
AU52949". Here are the individual entries
from the Ephemeris in the list. When you click on an entry in the list you are taken directly to
the object and its' data is displayed for when you have Frame object and Object
Information checked on the Find dialog! See below.
Edit | Find

Search the SDB by name
If you do not see the reference point on
TheSky display after it has been centered, showing
the position, you
have not enabled Object Type Reference Points see above.
You can also go DIRECTLY to the coordinates
of the minor planet if you like. This assumes you know them. Right
Mouse Click on TheSky display and the following menu shows. By choosing
the Move To option you can go directly to any ALT. AZ. or RA and DEC
coordinates.
Right Mouse Click TheSky display

Choose Move To
Enter coordinates here

Note SLEW button too!
When the telescope is connected the option to
"Slew To" the coordinates is available. There maybe times when it is
easier to just slew to the coordinates directly like this or you can simply use
the Data | User-Defined data area to quickly add the object.
Add the NEO here

Another Option
You
can quickly Center on the object added using the Center button above.
You can label the data as you see fit.
Any or all of the fields can be included. Using the Display Explorer
expand the NEO SDB file listed under the Sky Databases (SDB's). Here you
will see the fields associated to the data. Check mark those that apply.
See below.
Label Date/UT and Motion (rate)

The labels show the fields you have selected
The EXTENDED labels must by enabled to see
them. Use View | Labels | Extended Labels and make sure they are on.
Extended Labels

Here is exactly how. This is more work
but certainly a workable option. Add all of the NEO ephemeris' texts into
a single text file. By adding the NEO name to the end of each entry you
can distinguish each position with the name of the NEO it belongs to. See
below.
NOTE: Only two entries per NEO are shown
for clarity!
>SEARCH 105,114
>RAHOURS 19,20
>RAMINUTES 22,23
>RASECONDS 25,29
>SEARCH 1,18
>DECSIGN 30,30
>DECDEGREES 31,32
>DECMINUTES 34,35
>DECSECONDS 37,38
>MAGNITUDE 47,50
>OBJECT TYPE 55
>IDENTIFIER ALL NEOS
>PARSE "Date U.T." 1,18
>PARSE "Elong." 40,44
>PARSE "Motion arc secs/min" 53,58
>PARSE "P.A." 60,65
>PARSE "Object Alt. Az." 66,78
>PARSE "Sun Alt." 78,84
>PARSE "Moon Phase Dist. Alt." 85,102
>PARSE "Uncertainty" 103,114
Date UT R.A. (J2000) Decl. Elong. V Motion
Object Sun Moon NEO
NEO
h
"/min P.A. Azi. Alt. Alt. Phase Dist. Alt. Name
;F65G0Q
2005 07 13 20 19 56 41.4 -19 37 08 174.0 20.3 0.47 272.7 162 -75 +78 0.42 105
+08 F65G0Q
2005 07 13 21 19 56 39.4 -19 37 07 174.0 20.3 0.47 272.6 214 -73 +71 0.42 105
+20 F65G0Q
;5N9E0EA
2005 07 13 20 20 17 23.4 -17 45 42 168.8 20.5 0.48 239.9 148 -71 +78 0.42 110
+08 5N9E0EA
2005 07 13 21 20 17 21.6 -17 45 56 168.8 20.5 0.48 239.8 196 -73 +71 0.42 110
+20 5N9E0EA
;UHAZ01
2005 07 13 20 13 45 22.1 +00 46 09 92.7 20.6 1.43 144.9 268 -01 +78 0.42 016 +08
UHAZ01
2005 07 13 21 13 45 25.4 +00 44 58 92.6 20.6 1.43 145.1 277 +11 +71 0.42 016 +20
UHAZ01
;5N9E167
2005 07 13 20 21 26 53.1 -14 35 05 152.0 20.9 0.56 239.9 121 -58 +78 0.42 127
+08 5N9E167
2005 07 13 21 21 26 51.1 -14 35 22 152.0 20.9 0.56 239.7 147 -67 +71 0.42 127
+20 5N9E167
;5N3E3F5
2005 07 13 20 21 35 08.0 -05 56 10 146.5 19.5 4.04 208.3 129 -51 +78 0.42 131
+08 5N3E3F5
2005 07 13 21 21 35 00.3 -05 59 44 146.6 19.4 4.05 208.2 151 -59 +71 0.42 131
+20 5N3E3F5
;5N3E3F1
2005 07 13 20 00 55 55.8 +04 46 51 96.7 18.0 1.75 093.2 100 -06 +78 0.42 177 +08
5N3E3F1
2005 07 13 21 00 56 02.8 +04 46 45 96.7 18.0 1.76 093.2 109 -18 +71 0.42 178 +20
5N3E3F1
;5N5545E
2005 07 13 20 20 17 19.3 -29 38 10 167.2 19.3 1.25 237.5 115 -80 +78 0.42 108
+08 5N5545E
2005 07 13 21 20 17 14.5 -29 38 51 167.3 19.3 1.25 237.5 223 -84 +71 0.42 107
+20 5N5545E
;5N3D9A2
2005 07 13 20 16 30 37.9 +28 27 15 113.3 19.5 2.45 223.4 221 -13 +78 0.42 063
+08 5N3D9A2
2005 07 13 21 16 30 30.3 +28 25 28 113.3 19.5 2.45 223.4 231 -05 +71 0.42 063
+20 5N3D9A2
So now the text file as all NEO's in a single place.
Just make a new field at the end of each entry and add the name of the NEO.
NOTE: There were two changes made to the HEADER text to
accommodate this new file. They are as follows. The name of the SDB
is now ALL NEOS not just the single NEO name! And secondly the SEARCH
field has been specified as columns 105,155 to allow searching by the new NEO
name field that was added!
>SEARCH 105,114
>IDENTIFIER ALL NEOS
Now new searching on the SDB file becomes ALL
NEOS and the individual entries are listed. See below.
Changes to the HEADER text

Shown here
Easy. Once you have clicked on an
Ephemeris position on TheSky display (or easier) found it in the SDB file use, the Object Information |
Telescope Tab and choose Slew.
Slew to the position here

Note Position in the dialog!
Because there is insufficient data needed
to compute the correct rates for RA and DEC, as there would be when using orbital
elements, you have no choice but to manually enter the tracking rates in the
control system. Use Telescope | Options | More Settings to
access the settings for the control system. Here you will see the NON-sidereal
rates for both RA and Dec.
NOTE: The tracking rates entered
for both RA and DEC are in arc seconds/second so adjust accordingly to match!
The value on the NEO Ephemeris page is "/min
(arc seconds/minute). That number must be divided by 60 to get the rate in
arc seconds/second.
Example. A rate of 7.3 arc
seconds/minute is equal to only 0.12166 arc seconds/second. The control
system needs the rate in arc seconds/second!
Set RA tracking rate

Default rate is zero
Set DEC tracking rate

Default rate is zero
WARNING!
DO NOT
FORGET TO SET THE RATES BACK TO ZERO OR ALTER THEM TO MATCH THE NEXT NEO!
If you forget to change the rates for the next NEO
or do not set the zero defaults you will experience tracking related problems
since the rates have been altered!
|