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For objects that do not have enough data necessary to
create orbital elements you can use TheSky's tools to help find the
objects in many ways. By accessing the
MPC's NEO
Confirmation Page you can get the positions for newly discovered
objects and have TheSky slew the telescope to coordinates. Here is
how.
REMEMBER: Whenever an object has orbital
elements available use them instead! By supplying orbital elements
to TheSky can do all the work for you. See the
tracking
rates page on Tom's Corner for complete details on how to do this.
The following screen shot shows the Minor Planet
Center's NEO Confirmation
Page. The very bottom of the page has objects listed which
need follow-up work so that orbital elements can be provided.
Screen shot of NEO page

Grab Text at the bottom!
By highlighting the text at the bottom of the page that
contains name, position, date, and magnitude you can easily Add the
object to TheSky. By doing this you can find the object by name,
label it, and slew to it with minimal effort. And best of all you
don't have to do any manual entering of data.
Simply drag the mouse over the text first then copy that
text to the clipboard. See the following. Once the TEXT has
been high lighted Right Mouse Click and choose COPY.
Drag the text using the mouse

Grab only the relevant text!
Now use WordPad, NotePad or any other TEXT editor to
edit the text by pasting it from the clipboard..
Open WordPad for example and Edit Paste the text using the Edit |
Paste Special "UNFORMATTED" Text mode! You DO NOT want the
text formatted for you. Here is the text grabbed from the NEO page
above and then after it was Edit Pasted Special into WordPad.
76R001 [2005 June 27.2 UT. R.A. = 16 08.1, Decl.
= +08 27, V = 18.7] Added June 27.50 UT [1 nighter]
SW40Nt [2005 June 27.1 UT. R.A. = 16 08.9, Decl.
= -12 14, V = 20.5] Added June 27.51 UT [1 nighter]
JMYI251 [2005 June 25.9 UT. R.A. = 18 05.2,
Decl. = -03 24, V = 19.2] Updated June 27.55 UT
5M9CBCE [2005 June 18.3 UT. R.A. = 21 45.0,
Decl. = -04 28, V = 20.3] Updated June 21.66 UT
5M3C619 [2005 June 16.4 UT. R.A. = 02 11.3,
Decl. = +32 30, V = 18.4] Updated June 27.63 UT
To clean up the text just remove the
extra line between objects but this is not actually necessary.
However, YOU MUST keep the fields in the same columns! In the
example above there needs to be a space after the first two entries to
line up the columns as shown below.
76R001 [2005 June 27.2 UT. R.A. = 16
08.1, Decl. = +08 27, V = 18.7] Added June 27.50 UT [1 nighter]
SW40Nt [2005 June 27.1 UT. R.A. = 16 08.9, Decl. = -12 14, V =
20.5] Added June 27.51 UT [1 nighter]
JMYI251 [2005 June 25.9 UT. R.A. = 18 05.2, Decl. = -03 24, V = 19.2]
Updated June 27.55 UT
5M9CBCE [2005 June 18.3 UT. R.A. = 21 45.0, Decl. = -04 28, V = 20.3]
Updated June 21.66 UT
5M3C619 [2005 June 16.4 UT. R.A. = 02 11.3, Decl. = +32 30, V = 18.4]
Updated June 27.63 UT
Now just attach the header text I have
created to the top of the object data text so it can be compiled in
TheSky directly.
>LABEL 1,8
>SEARCH 1,8
>PARSE "Date U.T." 9,28
>RAHOURS 36,37
>RAMINUTES 39,42
>DECSIGN 53,53
>DECDEGREES 54,55
>DECMINUTES 57,58
>MAGNITUDE 65,68
>OBJECT TYPE 55
>IDENTIFIER NEO's from MPC
>PARSE "Description" 71,200
JMYI251 [2005 June 25.9 UT. R.A. = 18 05.2,
Decl. = -03 24, V = 19.2] Updated June 27.55 UT
SW40Nt [2005 June 27.1 UT. R.A. = 16 08.9, Decl. = -12 14, V =
20.5] Added June 27.51 UT [1 nighter]
76R001 [2005 June 27.2 UT. R.A. = 16 08.1, Decl. = +08 27, V =
18.7] Added June 27.50 UT [1 nighter]
5M9CBCE [2005 June 18.3 UT. R.A. = 21 45.0, Decl. = -04 28, V = 20.3]
Updated June 21.66 UT
5M3C619 [2005 June 16.4 UT. R.A. = 02 11.3, Decl. = +32 30, V = 18.4]
Updated June 27.63 UT
The above header simply tells TheSky
where the data is. That is what columns are what. This way
you can just compile the text into an SDB file (Sky Database File) for
plotting, searching, and slewing to the objects easy enough.
DOWNLOAD the above SDB and Text file
Place the two files in the Sky Database
Folder. It is located under \TheSky\User\SDB's. Once the two
files are there they can be added to the existing list of Databases
using TheSky's Database Manager. Data | Sky Database Manager's Add
button.
Add the SDB file to the
existing list

Your list may vary!
NOTE: Because the SDB was compiled using
Object Type "REFERENCE POINT" they must be set to visible to see them! Use the View |
Display Explorer to enable object type Reference Points. Just
enter Reference point in the Go to: field and you will be taken there.
See below.
Turn on Reference Points

Once the SDB has been added and Reference Points are set
to visible as per the above the data can then be searched, labeled, and
plotted in TheSky. Use Edit | Find then go down to NEO's from MPC
located under the list of Sky Databases (SDB's)
and you will see a list of all objects by name. You can also search by
name but you must use the SDB name first then the NEO name. As in
"NEO's from MPC" space then the name. Just as it is in the
following. Picking the NEO by name off the SDB list is easiest.
Edit | Find | SDB's | NEO's from MPC

Center the object you want!
The object can be slewed to just as easy as it is found
provided the telescope has been initialized.
Once found you can slew to the NEO

Use the Object Information Dialog's
Slew to button
NOTE: The Set Tracking
Rates option does not apply! Because the data does not
contain anything but RA and DEC a rate cannot be computed.
However, if you wish to CHANGE the default Paramount tracking rates that
can be done manually. The More Settings dialog is where.
Choose Telescope | Options | More Settings to access the settings for RA
and DEC rates.
Change RA rate to a non-sidereal rate

Make the rate change here
&
Same for the Declination axis

Enter non-sidereal DEC rate here
NOTE: It is easy to forget you have made
changes to the tracking rates! DON'T forget to put them back to
ZERO when you are finished. OR make sure you change them
accordingly when slewing to different objects that are moving at
different rates!
NEO shown in TheSky and Labeled

Note date/time and position for the NEO
NOTE: Don't forget to convert
Universal Time to local time! This is often an area of
confusion. The data provided is in Universal Time not local time
so you must do the conversion or you will be several hours off. I
have done this myself so I am speaking from experience. Nothing
like running a script to image Rosetta the night AFTER it was visible!
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