TPOVU
namenum.dat
 Records Read
conline.datU
@Too Many Stars--Choose Brighter Magnitude Limit or Smaller ScaleU
	dayta.dayU
 Comet Plot Options:" E.  Plot Earth-Based Finder Chart  R.  Comet Recovery Search Chart
 S.  View the Orbit from Space
 Choose one (E/R/S): 
 O.K.? (Y/N): 
YN3 How far (in A.U.'s) is the observer from the sun? 
5% Path to search for ephemeris files: 
Select an Ephemeris File
*.epb
*.epa
*.epc
*.ep*! Include tails on comets? (Y/N): L (Tails are drawn to an artificial length of 0.1 AU.  If the actual tail is,N  for example, twice the length shown, you know its physical length is 0.2 AU.N  The main reason to omit the tail is to conserve space if you intend to over-N  lay several comet paths.  A maximum of 500 points are allowed, including the@  heads and tails of comets and all other solar system objects.)D Indicate the sun's location for each position of the comet? (Y/N): G (Where a comet is located relative to the sun is often what determines%  whether or not it will be visible.)
Incompatible Dates
Date for start of ephemeris: 
                Date of Map: 
       Use it anyway? (Y/N): 
@4\t(
(( Stars Plotted) Type any Key to ContinueU
F1  Cursor
F2  Save/Modify
F3  Zoom Out
F3  Zoom In
F4  Constel. Lines
F4  Constel. Names
F4  Move Names
F5  Planets, etc
F6  Comet Paths
F7  Planet/Comet ID
F8  Clear Overlays
F9  Small Scale 3-D
F10 Printout
<SHFT>  next menuU
F1  Add NGC objects
F2  NGC obsrv. list
F3  NGC namesU
(( Stars Plotted) Type any Key to ContinueU
0Type "Y" to abandon map and return to main menu.&Type "Y" to clear all starmap overlays
?-(Type any key to printout or <ESC> to bypass)U
	%	B	
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3%3*3/3A3F3K3U3Z3l3q3v3
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I.ERROR--not enough room for NGC objects in RAM.U
'Erase all non-selected objects? (Y/N): U
Plotted 	 objects.U
 Include rise/set data? (Y/N): 
 Include user log? (Y/N): 
 O.K.? (Y/N): U
	     |  |
Notes
E-Edit 
<Del>-Delete 6<Enter>,<PgDn>-Continue <PgUp>-Prev. object <Esc>-QuitU
i<Eu?
computing...
ngcobjct.dat
Ran out of memory.U
< Create new observing list or Append to current list (C/A)? 
 Magnitude limit for search: 
 ("9999" represents no limit.)
Database Sub-CategoriesL(Unregistered users are limited to Messier objects and user-defined subsets)
 A. Entire database
_______________0 Choose objects from which category? (A,B,...): 
Object Types"(Use spacebar to toggle selection)
       [
 O.K.? (Y/N): 
ngclist.dat
3<Au/
category.datU
Empty
Please Choose Category:U
Category Functions
No room for a new category
 Press a key.
Please enter category name:
Category
 O.K.? (Y/N): 
 Include user notes? (Y/N): 
 Include rise/set data? (Y/N): 	dayta.dayU
Observing List Files
*.obs
 Loading...
ngclist.datU
 Name of destination file: 
 O.K.? (Y/N): 
.obsU
	dayta.day
ngclist.datU
Name for output file: 
OBSLIST
OBSLIST|
dumping...	     |  |
	dayta.day+ Printed output to printer or file? (P/F): 
PF!Press a key when printer is ready
Printing...
 	     |  |
Form Feed? (Y/N): 
Observing List Functions$ There is no current observing list.
 Press a key.U
	$	.	3	E	J	O	o	
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 Printer Type Selected: 
9-pin
24-pin
Laser! 3-D not allowed with NGC objects3 The "Small Scale 3-D" printout has been requested.
 Format (D/C): 
DC-   D = Direct (Use viewer or stare past page)'   C = Crossed (View with crossed eyes)/ Do you want the printout to be in 3-D? (Y/N): 
0.01|
    [ Eye spacing: 
 Astronomical Units ]
 Light Years ]
 Long:
 deg 
 min, 
 min /
 Title Line:
 O.K.? (Y/N): 
@$(Type any key when printer is ready)
(Processing Printer Output)U
	V	[	e	j	o	
(PRINTING--TYPE <ESC> TO ABORT)U
?UUUUUUU
[R]!(Printout Aborted--Reset Printer)
 Form Feed? (Y/N): 
!A!N!
"O"q"
#H#k#{#
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...4.G.L.Q.V.[.`.}.
/ /%/Y/
&l8CU
laserdot.datU
&f1XU
(s0p16.67h8.5v0s0b0T
(s0p10.00h12.0v0s0b3T
(s0p10.00h12.0v0s3b3TU
*c766a8b100g2P
*c8a766b100g2PU
ngcsymbl.dat
extsymbl.dat
&f1XU
ngcsymbl.dat
extsymbl.dat
"#"("-"G"T"_"l"q"v"
#$#4#A#N#Y#f#q#
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Name for map file: 
.m01	dayta.day
.m02U
 Limiting magnitude: 
 O.K.? (Y/N): 
0 Do you wish to save the map as a file?  (Y/N): 
NY7 Do you wish to display a previously saved map? (Y/N): ? Do you want lines for only the labeled constellations? (Y/N): ! The current magnitude limit is: 
@< Do you wish to alter the number of stars displayed? (Y/N): U
.d01	dayta.day
 Path to search: 
Select Map File
*.m01
 does not exist.2 Type <ESC> to quit or any other key to try again.
.d01U
namenum.dat
------
  R.A.:
   (No Name)  R.A.:
m  Dec.:
'   Mag:
  Dist:
(Comet Relative to the Horizon)
	dayta.dayU
	dayta.dayU
%Nothing identified at cursor locationU
@4View Direction (Use Arrow Keys, <Enter>, or <ESC>): 
@3333333
?3333333
 O!h!
"!"c"4#
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first name
no name
second nameU
Edit log
End edit
CategoryU
PGup/dn scrollU
8Your log file is full.  Some of this log can't be saved.G Your log file is full.  Some of this log can't be saved.  Press a key.U
	saving...U
Save log? (Y/N):U
r<Yu	
< r	<~w
	C	H	
ngcobjct.datU
category.datU
userlog.dat
building userlog.dat...U
ngclist.datU
ngclist.datU
category.datU
Press a key.U
sacindex.dat
sacindx2.dat
sacnotes.dat
sacrest.dat
"  L_
"  PA (dgr):
  CLASS:
# of stars: 
  brightest star: 
ngclist.datU
	 	*	/	E	O	T	j	t	y	
Absolute Magnitude: 
Coefficient of log(r) 
(Use 10 if unknown): 
 O.K.? (Y/N): 
@%For what date is the magnitude known?
YYYY: 
DD.D: 
Magnitude on that day: 
Coefficient of log(r) 
(Use 10 if unknown): 
 O.K.? (Y/N): 
deleteU
5Select Comet From List or Type <INSERT> for New Entry
#New Comet Data (Type <ESC> to Quit)
Name: $ (Time of Perihelion Passage)   T:  
YYYY 
  MM 	  DD.DDD # (Eccentricity)                 e: # (Perihelion Distance)          q: # (Argument of Perihelion)    Peri: # (Longitude of Ascen. Node)  Node: # (Inclination)                  i: 
BJ# (Equinox:  B=B1950.0, J=J2000.0): "  Format of Magnitude Information:   A. Absolute magnitude is known.  B. Apparent magnitude is known for some date
  C. No magnitude data is known
  D. LEAVE MAGNITUDE UNCHANGED
  Magnitude Format Option: 
 O.K.? (Y/N): 
          T: 
Peri: 
          e: 	(J2000.0)
(1950.0)
Node: 
          q: 
 A.U.'s
   i: 
          Absolute Magnitude: 
   Magnitude Coefficient: 
Period: 
 Days
 YearsCE-Edit, C-Copy, <ESC>-quit, <DEL>-delete comet, <Enter>-continue): 
 EC<83>U
=Copy Comet to Which CFL File? (Type <ESC> to create new file)
*.cfl
Name for new comet data file: 
 O.K.? (Y/N): 
delete
Dates and Times of Observations
     (Type <Esc> to quit)      2 Your choice for method of day and time selection:J   A. Choose Day and Time for Symmetry around Perihelion (for orbit plots)=   B. Use Day and Time of Most Recent "What's Up" Computation9      (For Compatibility with Current Day-and-Time Chart)8   C. Determine Search Area for Attempted Comet Recovery
   D. Other (Direct Entry)
     Your Choice: 
      
 O.K.? (Y/N): 
YNK (If the ephemeris is saved to a file, the method of day and time selectionD will be reflected in the file extension: .epa, .epb, .epc, or .epd)
 This comet has a period of 
 years.  Do you want a full	 orbit? (
 positions at 
 day intervals
, no tail.) 
5%Number of days between calculations: 
Number of calculations: 
@	dayta.day
Starting Date   YYYY: 
DD: &Presumed Uncertainty in arrival time: 
 DaysL (The stated uncertainty will be rounded to a multiple of the step interval)< Use P)rimary, A)lternate, or N)ew observing site? (P/A/N): 
?'Sun and Comet Data for Starting Date:  
, 	     |  |
Observing Time: 
       
Advance the Date?  
,<Cu(
@<Nu<
C          R.A.(H,M)   DEC(D,M)    R     DELTA   ELONG   PHASE    PA
@	      MAG?      R.A.(H,M)   DEC(D,M)    R     DELTA   ELONG   PHASE    PAU
          T: 
      Peri: 
          e: 	(J2000.0)
(1950.0)
              Node: 
          q: 
                 i: 
Absolute Magnitude:
   Magnitude Coefficient:
Time of Observations: 
  (Starting JD=
Period: 
 Days  
 Years  %Ephemeris computed for equinox 2000.0U
 Output Options
 Printer (Y/N, Default = N): 
NY0 Disk File--Star Map Format (Y/N, Default = Y): 
YN- Disk File--ASCII Format (Y/N, Default = N): 
 O.K.? (Y/N): U
 Map Format File Path: 
 File Name: 
 O.K.? (Y/N): 
  	  Exists.5  It will be overwritten.                            
NY0  Will Be Created                               U
 ASCII Format File Path: 
 File Name: 
 O.K.? (Y/N): 
  	  Exists.5  It will be overwritten.                            
NY0  Will Be Created                               U
    <
cometq
 Form Feed? 
 (Type any key)U
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 Map LocationK You have two options for specifying the location of the center of the map:$           A. Select a Constellation(           B. Specify the Coordinates : 
              Your Option: 
Constellations
r<Dun
Data is available for:
Use this data? 
SPECIAL MATCH THE SKY MODEH One good way to point out constellations to beginners (especially youngK children) is to make a set of constellation charts at the same exact scaleI as what they will see in the sky.  Constellations are BIG in the sky butH usually appear small on star charts.  Getting used to the difference in/ scale can be a problem in itself for children.L MATCH THE SKY charts should be designed to be held 12 to 18 inches in frontI of the eyes.  They show only a small portion of the sky, so they fail toJ show the constellations in context.  Context is important in learning theN constellations, so these charts should supplement rather than replace smaller
 scale charts.
 Viewing distance (in inches): 
 Format -- H)oriz., V)ert.: 
  N)orth up, S)outh up: 
 Magnitude Limit: 
54(Magnitude 4.5 or 5 is recommended for this purpose)
 O.K.? (Y/N): 
,                               Map SelectionM A. STAR ATLAS MODE--(Equatorial Coordinates) / This mode is best for viewing8    a given constellation or a given section of the sky.M B. DAY AND TIME MODE--(Horizon Coordinates) / This mode shows the portion of.    the sky visible at a given place and time.I C. SOLAR SYSTEM MODE--(Ecliptic Coordinates) / The ecliptic plane is theL    plane of the solar system.  This mode is useful for studies of planetary;    motion, comet orbits, and other solar system phenomena.I D. MILKY WAY MODE--(Galactic Coordinates) / The Milky Way traces out theL    plane of the galaxy as seen in the sky.  This mode is useful for studies=    of celestial objects relative to the plane of the galaxy.G E. SPECIAL "MATCH THE SKY MODE" / This mode generates specially scaledL    maps that can be held at arm's length to match the sky exactly--a useful(    aid for learning the constellations.
 Choose one (A,B,C,D,E): 
ABCDE
 OK? (Y/N): 
Equatorial Coordinates'   R.A. of center of view (0 to 24):   
 hr  
 min& Dec. of center of view (-90 to 90):  
 deg 
 O.K.? (Y/N): 	dayta.day
 Limiting magnitude: 
Ecliptic Coordinates
Galactic Coordinates+ Longitude of center of view (0 to 360):   
 deg  * Latitude of center of view (-90 to 90):  ! Scale for 8 x 10 inch printout: 
 degrees per 
 inches.
 Map Projection System: 
SPENG|(   (All map projections are compromises)K S. Stereographic  | Shapes preserved, sizes enlarged far from center pointJ P. Polar Equidist | More shape distortion, less size distortion than in AN E. Mercator (E-W) | Shapes preserved, sizes enlarged far from E-W center lineN N. Mercator (N-S) | Shapes preserved, sizes enlarged far from N-S center lineL G. Gnomonic       | Matches photographic plates, good for small areas only 
 Format -- H)oriz., V)ert.: 
  D)irect, R)eversed: 
  N)orth up, S)outh up: 
 Magnitude Limit (0 to 10): J (Use Mag 4 or 5 for whole sky--fainter limits for views of smaller areas.E  Entering a limiting magnitude of 10 will plot all stars available.)
 Files SST1-SST
 are installed:  
 Stars / Limiting Magnitude = K (77 star files are available for a total of 248,709 stars, 5 Megs on disk)
 " * 
 %!*!4!9!C!H!b!g!l!
"$")"."8"="O"T"Y"t"y"
#&#+#3#
$0$5$G$L$Q$[$`$r$w$|$
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&!&&&0&5&G&L&Q&l&q&{&
&('F'T'a'f'k'
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(,)1)P)\)
Location: 
 Longitude: 
 deg 
 min 
/ Latitude: 
) / Julian Day:
    U
	dayta.dayU
!Twilight Data for Night starting 
           Solar Transit: 
 --- 
                  Sunset: 
 +++ 
   Evening Twilight Ends: 
 Morning Twilight Begins: 
                 Sunrise: 
          (The sun never sets)
        (24 hours of darkness)
         (The sun never rises)
(Twilight continues all night)
Time of observation: 
 O.K.? (Y/N): 
Advance the Date?  
) / Julian Day:
    U
>nzYu
         Year 
        Month 
          Day < Use P)rimary, A)lternate, or N)ew observing site? (P/A/N): 
 O.K.? (Y/N): 
mz<Pu
5<Nu1
New Moons from DEC 
 through JAN 
 Moon Phases Near 
Planet Position DataM          RA     DEC    Long   Lat    Az     Alt   Elong   Phase  Dist   DiamO         ----------------------------------------------------------------------
        
     
      
       
@H Positive elongations = evening sky / Negative elongations = morning skyA Planet Dist. in A.U.s; Moon Dist in Earth Radii; Diam in Arc MinE         P-print screen, <ESC>-skip rise/set info, <ENTER>-continue: 
PE                P-print screen, <ESC>-skip comets, <ENTER>-continue: U
Location of all comets in U
(Type P to print screen)
delete
   	     |  |
(Type P to Print Screen): Select? (Y/N/ S(select all)/ R(reject all)/ <ESC>(quit): 
NYSRP|!(Type Any Key to Alter Selection)<                                                            E                                   P-print screen, <ENTER>-continue: 
*                               Target Date
@E A-alter date, P-print screen, <ESC>-skip planets, <ENTER>-continue: 
APK                                                                           E                                <ESC>-skip comets, <ENTER>-continue: 
>nzAu
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ESelect Data File for Orbital Elements (or <INSERT> to start new file)
Select Comet Data File
*.cfl
current.cfl
CURRENT.CFL
recent.cfl
RECENT.CFL%New comet data file (<ESC> to quit): 
 O.K.? (Y/N): 
       R.A.: 
  Dec.: 
  Mag.: 
@3333333
?/Out of Range / Procedure Aborted / Type Any Key5
plcrunch.dat
 is missing -- Type any keyU
	@3333333
@fffff
9Rise/Set Timetable Centered on Local Midnight (Times are 
I                                                                         
?I - - - - - - - - - - - - (24 Hours of Daylight) - - - - - - - - - - - - -
     U
I                                                                         
(Does Not Rise)
     U
?333333
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ds3d.exe
DSDATA\
DSFILES\
 Observing Site:
 Name of your 
 observing site: 
 Longitude: 
 Deg  
 Min  (East/West) 
 Latitude: 
 Min  (North/South) ( Altitude (approximate number of feet): 
Time ZonesM Hours from Greenwich:   10    9    8    7    6    5    4    3    2    1    0N Standard time zones:    HST  YST  PST  MST  CST  EST  AST  ---  ---  ---   UTN Daylight time zones:         HDT  YDT  PDT  MDT  CDT  EDT  ADT  ---  ---  ---
 Time Zone Name: / Time Difference from Local Time to Greenwich: 
  (East/West) 
 O.K.? (Y/N): 
PRIMARY	ALTERNATEU
( Graphics card detected by the program: J Some graphics cards cannot be autodetected by the program.  If you know aH different card is present, or if more than one card is present, you mayM make your own selection.  If you accidentally select a graphics card that isM not actually present in the machine, the program will probably crash when itG tries to enter graphics mode.  If this occurs, simply reboot and try a
 different setting.
 Graphics Card Setting:
    0. NONE
    1. CGA
    2. MCGA
    3. EGA
    4. EGA64
    5. EGAMono
    6. VGA
    7. HERCULES
 Selection: 
 O.K.? (Y/N): 
--MISSING--U
 Default Directories: I   Drive letter and directory path where main program files may be found:,     (DS.EXE, DS.OVR, *.BGI, & DSCONFIG.FIL)J   Drive letter and directory path where supplementary files may be found:
     (TEXT.TXT, *.DAT)F   Drive letter and directory path where star data files may be found:
     (SST01,SST02,...)H   Drive letter and directory path for comet data and output data files:$     (*.CFL, *.EPH, DAYTA.DAY,...): 
 O.K.? (Y/N): 
\C Testing Directories for Minimum Content and Correct File Placement
 Main Directory = 
 Supplementary Directory = 
 Data Directory = 
 Output Directory = 6 One or more essential files are missing or misplaced.N Check to see that all files are in the correct directories before continuing.
 Type any key to continueU
 Star Data Installed:1   Highest numbered star data file installed: SST<   (77 files containing nearly 250,000 stars are available.)
@2 Default Magnitude Limit for Non-Stellar Objects: 
BJB Default Equinox for New Orbital Elements (B=B1950.0, J=J2000.0): E (Through 1991 choose B1950.0; Starting January 1992, choose J2000.0)
NTL9 Printer:  N. Nine pin, T. Twenty-four pin, or L. Laser: G (Deep Space 3-D supports Epson-compatible dot matrix graphics printersF  and HP Laserjet II-compatible laser printers using HP PCL commands.)
 O.K.? (Y/N): 
01/ (THE UNREGISTERED VERSION IS LIMITED TO SST01)
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,This copy of Deep Space 3-D is registered to
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YNH This copy of Deep Space 3-D is UNREGISTERED.  It is a fully functioningL trial copy for individual use only.  All features work normally, but accessL to the databases is limited to one file of stars (SST01), the Messier list,K and two comet files (CURRENT.CFL and RECENT.CFL).  Star files up to SST77,N the full Saguaro Database (the entire NGC plus additional entries), and filesG of all known comets are available to registered users.  They cannot beJ accessed by the program until it has been "imprinted" with the REGISTERED# USER NAME and REGISTRATION NUMBER.
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 REGISTERED USER NAME: 
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THANK YOU FOR REGISTERING!N Please keep a copy of your REGISTRATION NUMBER and the exact spelling of yourI REGISTERED USER NAME for future reference.  They may be used repeatedly.
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 D E E P   S P A C E   3 - D 'Copyright (c) 1987-1991  David Chandler!P.O. Box 309, La Verne, CA  91750
 REGISTERED USER: 
 UNREGISTERED VERSION .Star data is adapted from the Skymap data base3courtesy of the National Space Science Data Center.3Non-stellar data is adapted from the SAC data base,)(A project of the Saguaro Astronomy Club)
Version 3.0 (August 4, 1991)
(Type any key to continue), To the users of DEEP SPACE 3-D Version 3.0:J Deep Space 3-D comes as a "core" program, which is SHAREWARE, and lots ofM additional databases which are made available only to registered users.  YouF are encouraged to share the original archived version of the program.L Registered users will receive the disk STAR DATA #0 (which brings your starK database up to about 19,600 stars), a 3-D viewer, access to the entire NGCJ catalog, and the option to purchase additional star and comet data disks.G (Choose the CATALOG option at the Main Menu for ordering information.)M SHAREWARE does not mean "Public Domain."  It is a means of letting you "testK drive" a fully functioning program before making a final purchase.  We areM confident you will want the full benefits of the registered version once you& see what DEEP SPACE 3-D has to offer." Send comments and bug reports to:G   David Chandler Co., PO. Box 309, La Verne, CA 91750 / (714) 988-5678
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