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): 
8*\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 PrintoutU
(( Stars Plotted) Type any Key to ContinueU
+Type F8 again to clear all starmap overlays
?-(Type any key to printout or <ESC> to bypass)U
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"Standard 9-Pin Dot Matrix PrintoutI(Some 24 pin and laser printers may emulate a standard 9-Pin printer.  IfI distortion occurs, change the printer aspect ratio in the startup file.)3 The "Small Scale 3-D" printout has been requested./ Do you want the printout to be in 3-D? (Y/N): 
0.01|
    [ Eye spacing: 
Astronomical Units ]
Light Years ]
 Title Line:
 O.K.? (Y/N): 
@$(Type any key when printer is ready)
(Processing Printer Output)U
(PRINTING--TYPE <ESC> TO ABORT)
 Long:
 deg 
 min, 
 min /U
UUUUUUU
@!(Printout Aborted--Reset Printer)
 Form Feed? (Y/N): 
>Z+Yt
>Z+Yt
   0 5 ? D I S X b g 
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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
%No star identified at cursor locationU
@4View Direction (Use Arrow Keys, <Enter>, or <ESC>): 
?3333333
	b	x	
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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
2Select Comet From List or Type <ESC> 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: "  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: 
Node: 
| (1950.0)
          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 Observations2 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:  
Sunset: 
 +++ 
 --- 
Morning Twilight: 
Evening Twilight: 	Sunrise: <                     Rise    20-Deg   Trans    20-Deg    Set>                   -------------------------------------------
Observing Time: 
       
Advance the Date?  
>C4Nt
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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: 
              Node: 
 | (1950.0)
          q: 
                 i: 
Absolute Magnitude:
   Magnitude Coefficient:
Time of Observations: 
  (Starting JD=%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: 
comet|
 O.K.? (Y/N): 
  	  Exists.5  It will be overwritten.                            
NY0  Will Be Created                               U
 ASCII Format File Path: 
 File Name: 
comet|
 O.K.? (Y/N): 
  	  Exists.5  It will be overwritten.                            
NY0  Will Be Created                               U
    <
 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
	dayta.day
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): 
12: Printed Page Format -- H. Horizontal, V. Vertical (H/V): 
 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 4 Printed Page Format -- H. Horizontal, V. Vertical: 
 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)
!'!,!>!C!H!c!h!z!
"""'"B"G"Y"^"c"m"r"|"
",#1#;#@#J#O#a#f#k#
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Location: 
 Longitude: 
 deg 
 min 
/ Latitude: 
) / Julian Day:
    U
	dayta.dayU
!Sunlight Data for Day & Night of 
                 Sunrise: 
 +++ 
 --- 
           Solar Transit: 
                  Sunset: 
   Evening Twilight Ends: 
 Morning Twilight Begins: 
          (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
>D8Yu
  --- 
  +++ U
         Year 
        Month 
          Day < Use P)rimary, A)lternate, or N)ew observing site? (P/A/N): 
 O.K.? (Y/N): 
C8<Pu
5<Nu1
New Moons from DEC 
 through JAN 
 Moon Phases Near 
Planet Position DataN          RA     DEC    Az     Alt   Elong ||  Rise 20-Deg  Trans 20-Deg   SetP         ----------------------------------||-----------------------------------
        
     
      
       
H Positive elongations = evening sky / Negative elongations = morning skyE                P-print screen, <ESC>-skip comets, <ENTER>-continue: 
Location of all comets in J           RA     DEC    MAG       Rise    20-Deg   Trans    20-Deg    SetL           -----------------------------------------------------------------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: 
>D8Au
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BSelect Data File for Orbital Elements (or <ESC> to start new file)
Select Comet Data File
*.cfl
current.cfl
CURRENT.CFL
recent.cfl
RECENT.CFL
Name for new comet data file: 
 O.K.? (Y/N): 
           
      
      ---  
      +++  	    ---  	    +++  U
@3333333
?/Out of Range / Procedure Aborted / Type Any Key5
plcrunch.dat
 is missing -- Type any keyU
	@3333333
@fffff
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&.'='O'
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/	0=0I0_0
0-1d1
dsconfig.filU
dsconfig.fil
c:\ds3d\
c:\ds3d\dsdata\
c:\ds3d\dsfiles\
 Observing Site:
 Name of your 
 observing site: 
 Longitude: 
 Deg  
 Min  (East/West) 
 Latitude: 
 Min( 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
#Are you using a hard drive? (Y/N): 
BK (The program disk, must be left in one disk drive and be accessible at allN  times.  Other data or output files may share space on the same disk, but theN  program disk may not be swapped out to allow other disks to share the drive.O  While the program is running none of the drives referenced here should remainO  empty.  If the proper file is not present in the drive indicated, you will be
  prompted for a disk change.)
 Which Drive will be used for
 Main Program Files: 
@"   (DS3D.EXE, DS3D.OVR, and *.BGI)
 Supplementary Files: !   (TEXT.TXT, 4X6.FON, and *.DAT)
 Star Data Files: 
   (SST01,SST02,...)
 Comet Data and Output Files:     (*.CFL, *.EPH, DAYTA.DAY,...)
 O.K.? (Y/N): 
 Default Directories: I   Drive letter and directory path where main program files may be found:0     (DS3D.EXE, DS3D.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,...)
|	 Floppy? H   Drive letter and directory path for comet data and output data files:$     (*.CFL, *.EPH, DAYTA.DAY,...): 
\C Testing Directories for Minimum Content and Correct File Placement
 Main Directory = 
 Supplementary Directory = 
 Data Directory = 
SST01
 Output Directory = 
dsconfig.fil6 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 continue
 Star Data Installed:1   Highest numbered star data file installed: SST<   (77 files containing nearly 250,000 stars are available.)	 Printer:F   Some 24 pin printers introduce a 20% elongation of graphics images.9   Should the output be corrected for elongation? (Y/N): F   (Try a "Day and Time Mode" printout and check the boundary circle.)
01/ (THE UNREGISTERED VERSION IS LIMITED TO SST01)
 (Type any key to continue)U
,This copy of Deep Space 3-D is registered to
N To legally share copies of DEEP SPACE 3-D with friends or colleagues you mustL remove the registration imprint, restoring it to "UNREGISTERED" status.  ToH deregister a copy of the program at this time, place the DEEP SPACE 3-DO program disk in a floppy drive and answer the following queries.  (The imprintM of registration may also be removed by deleting the file DSCONFIG.FIL on the
 program disk.)F Do you wish to deregister a copy of the program at this time? (Y/N): 
NY: Drive letter containing the DEEP SPACE 3-D program disk: 
A@% Proceed with deregistration? (Y/N): 
:dsconfig.fil
 The copy of DEEP SPACE 3-D in %: is restored to UNREGISTERED status.A (Type <ESC> to quit or any other key to unregister another copy)K Do you wish to deregister the currently running copy at this time? (Y/N): 
dsconfig.filG The current copy of DEEP SPACE 3-D is restored to UNREGISTERED status.- Please start the program from the beginning.H This copy of Deep Space 3-D is UNREGISTERED.  It is a fully functioningM trial copy for individual use only.  Additional database files are availableJ to registered users.  They cannot be accessed by the program until it hasN been "imprinted" with the REGISTERED USER NAME and REGISTRATION NUMBER.  GiveK your name exactly as you want it spelled when you become a registered userM and you will be issued an REGISTRATION NUMBER that will be recognized by theL program in connection with your name.  You may imprint any copy of the diskK for your own use, but disks must be returned to unregistered status before, they are shared with friends or colleagues.F Do you wish to imprint this copy of the program at this time? (Y/N): 
(Type <ESC> to quit)
 REGISTERED USER NAME: 
  REGISTRATION NUMBER: 
 O.K.? (Y/N): 
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./ Highest numbered star data file installed: SST: (77 files containing nearly 250,000 stars are available.)U
 D E E P   S P A C E   3 - D 4Copyright (c) 1987, 1988, 1989, 1990  David Chandler
 REGISTERED USER: 
 UNREGISTERED VERSION 0Star data is adapted from the "Skymap" data base3courtesy of the National Space Science Data Center.
Version 2.1 (512k minimum)
Release Date: Aug 28, 1990
(Type any key to continue), To the users of DEEP SPACE 3-D Version 2.1:N Deep Space 3-D comes as a 2-disk "core" program, which is SHAREWARE, and lotsM of additional databases which are made available only to registered users.  M You are encouraged to pass around UNREGISTERED copies of the original 2-DiskK set: DEEP SPACE 3-D, and DS SUPPLEMENT, but they must be restored to theirN original "unregistered" condition.  (There is an option at the Main Menu thatM imprints or removes your REGISTERED USER NAME.)  Upon registration, you willK receive the disk STAR DATA #0, a 3-D viewer, and access to additional data; disks for a total of nearly 250,000 stars and 1100 comets.J SHAREWARE is not the same as public domain.  It is a means of letting youM "test drive" a fully functioning program before making a final purchase.  WeL are confident that as you become familiar with DEEP SPACE 3-D you will wantJ to become a registered user.  Please respect our interests and share only
 unregistered copies.D For more information, choose the HELP MENU option at the Main Menu.J Written comments and "bug reports" are welcome from all users.  Write to:@               David Chandler, P.O. Box 309, La Verne, CA 91750.
 (Type any key to continue)U
(Type Any Key to Continue)U
text.txt
Topics"Send to Printer or Screen? (P/S): 
SP$(Type Any Key When Printer Is Ready)
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(, is needed) -- Type any key or <ESC> to quit
(Insert -) -- Type any key or <ESC> to create new file$) -- Type any key or <ESC> to bypassU
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