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S K Y G L O B E 3.0
A Shareware Product of Klassm Software
Copyright (c) 1992 Mark A Haney
Congratulations! You have a fully registered copy of Skyglobe, the fun
and easy educational astronomy program. Skyglobe is distributed as
Shareware to reach the widest possible audience, so let's take care
of the legalities first.
Skyglobe is copyrighted material. You are granted permission to use
Skyglobe, and to make as many backup copies for your own purposes as
you want.
You are encouraged to distribute copies of Skyglobe, subject to the
following conditions:
1) All files, except for the file SKYGLOBE.REG, are
distributed together and unaltered.
2) No charge is made for the software.
(A small fee for media and handling is permissible.)
Anyone who receives a copy of Skyglobe from you should register
their copy if they decide to keep it and use it.
As I am now a member of the Association of Shareware Professionals,
I have included a copy of their standard Shareware and license wording
at the end of this file.
Skyglobe was originally developed with registered Shareware. Thank you
for supporting the Shareware concept by registering your copy of
S K Y G L O B E ! ! !
_______
____|__ | (R)
--| | |-------------------
| ____|__ | Association of
| | |_| Shareware
|__| o | Professionals
-----| | |---------------------
|___|___| MEMBER
February 9, 1992
SKYGLOBE 3.0 ORDER FORM
Your friends can use this form to register a copy of SkyGlobe 3.0.
Registration ($20) will entitle you to the following:
1) A copy of SkyGlobe with your Home Town as the default city.
2) A Handy SkyGlobe Reference Card.
Shipping Address: Name:
........................................
Street:
......................................
City, ST, ZIP
................................
Home Town:
(Up to three permitted) .............................................
Disk Type: 5 1/4" 3 1/2"
(circle one)
Default Video Mode: CGA Hercules EGA VGA
(circle one)
Please make checks ($20) payable to Klassm Software.
MI residents must add 4% sales tax, for a total of $20.80.
For your convenience, I now accept VISA/MasterCard, with a form below.
International customers need pay only $20, which includes airmail
shipping. For those of you without VISA/MasterCard, US dollar checks
drawn on a US bank are safest for me. However, to avoid excessive bank
charges, you might try international money orders or US currency. As a
last resort, I can accept foreign currency, or international checks
denominated in the currency of the issuing bank. Unfortunately, I am
not able to accept Eurocheques. Thank you for your cooperation.
Mail to: Klassm Software
284 142nd AVE
Caledonia, MI 49316-9604
Credit Card Authorization Form:
Card #__ __ __ __ __ __ __ __ __ __ __ __ __ __ __ __
Signature:_______________________________________________
Date of Authorization:___________ Amount:__________ Expiration:______
Thanks, and I hope you enjoy SkyGlobe!
-3-
Quick Starting Instructions
These instructions will enable you to get SkyGlobe up and
running as quickly as possible. Then you can return to the
manual to learn about SkyGlobe's advanced features.
SKYGLOBE.EXE is the only file that is absolutely necessary
in order to run SkyGlobe. If you wish to see more than 7000 stars,
you will need the files SKY8000.DAT and SKY10000.DAT as well.
Make certain these files are in the currently active directory,
type SKYGLOBE, and press the Enter key.
As a fully registered user of SkyGlobe, all you need to do is
type GO and press Enter. SkyGlobe will determine your choice of
video adapter and location from the file SKYGLOBE.REG. You can
override the video settings from the command line by using a command
such as SKYGLOBE E, for instance, to start SkyGlobe in EGA mode. Other
choices are V for VGA, C for CGA, H for Hercules, S for SVGA, and S2
for alternate SVGA mode.
When you type GO and press Enter, you will be quickly presented
with a view of the Southern sky for the current time and date. In the
middle of the top of the screen will be a welcome and copyright message,
which will disappear when you press your first command key. Most of the
commands in SkyGlobe require only a single keypress.
Let's try a few of the commands. First press 'A' to start the
Automatic increment of time. The Time, as indicated in the upper-
lefthand corner of the screen, will begin to change by five minutes.
Press 'Shift-A' to reverse direction, then press 'A' again to stop
the movement. Press 'B' for Brightness a few times and watch more
stars appear. Most actions in SkyGlobe are reversed by using the
Shift key. Press 'Shift-B', and watch the dimmest stars vanish. Try
'Z' and 'Shift-Z' to Zoom in and out.
Want to change the time? Try 'M', 'H', 'D' and 'T' for Month,
Hour, Day and Time (in minutes). Change the number of Constellation
Lines displayed by pressing 'C'. Use the cursor keys to change the
Viewing Direction and Elevation. And if you ever need to use your
computer for something besides SkyGlobe, press 'Q' to return to DOS.
I hope this quick introduction has gotten you started with
SkyGlobe. More detailed descriptions of the commands appear in
the following pages. Have fun!
-4-
SkyGlobe Command Descriptions
As a registered user of SkyGlobe, you received a Handy Reference Card
that will remind you of SkyGlobe commands. The inside of the Reference
Card contains two lists of the 300 brightest stars, as well as lists
of the constellations and Messier Objects. These lists will help you
when using the Find object command.
Time and Date Commands
SkyGlobe provides many ways to change the Time or Date of the
displayed sky view. You can change the Time forward or backward by a
minute or an hour. The Date can be changed forward or backward by a
day, a month, a year, or a century. Except for tiny changes due to
leap years, only the planets change from year to year.
Use the table below:
Forward Backward
1 Minute Press 'T' Press 'Shift-T'
1 Hour 'H' 'Shift-H'
1 Day 'D' 'Shift-D'
1 Month (30 days) 'M' 'Shift-M'
1 Year 'Y' 'Shift-Y'
1 Century 'J' 'Shift-J'
One of SkyGlobe's most useful features is the Auto-Increment mode.
This gives you the ability to simulate the passage of time on your com-
puter. To enter or exit this mode, press 'A'. The sky view will begin
to change in a manner that depends on the Auto-Increment parameters.
Use 'Alt-A' to change the increment type from Time to Date and
back. Use 'Shift-A' to change the direction of increment from Forward to
Backward and back. You can also change the speed of increment. Press '>'
to increase the speed, and '<' to slow back down. Only the active
increment type, either Time or Date, is affected by the '>' key '<' keys.
V3.0 of SkyGlobe adds two new features to the Auto-Increment mode.
Press 'R' to enter (or disable) Real-Time mode. This will synchronize
the Time and Date to the system clock. You still have control over all
commands except those related to Time and Date. Press 'Shift-R', and
the Increment speed will be set to one Sidereal day, or 1436 minutes.
This has the effect of seeming to freeze the star and constellation
display, while allowing the planets to continue their progress along
the ecliptic. This is useful for learning about retrograde motion, as
well as teaching something about the relative speeds of motions of the
planets.
-5-
Where Are We Looking?
Now let's learn about how SkyGlobe interprets directions. The
program assumes you are standing outside and that your eyes are
facing the direction your feet are pointing. This is the View Dir-
ection. The display shows this direction in degrees, ranging from
0 for due north, through 180 degrees for due south, to 350 degrees
for 10 degrees west of north. The View Direction is also indicated
by abbreviations in the parameter display, as well as along the
Horizon line by initials.
The View Elevation ranges from 0 degrees to 90. The Horizon ap-
pears as a straight line at the 0 degree setting. It might help to
imagine that you are extremely short for this one, so that the ground
covers the lower half of your eyes, but is transparent. The 90 degree
setting is like looking straight overhead at the Zenith.
Lines And Labels
One of the most useful features of SkyGlobe is its ability to
quickly and easily change the lines and labels that help our eyes
and minds make sense of the vastness of the sky. This can be very
helpful to the novice just learning the stars. Use the 'C' key
to increase the number of Constellation Lines displayed. As always,
use the Shift key to reduce the number of lines. The Constellation
Lines have been grouped by importance, with some constellations
having several classes of lines. The constellations also have
abbreviations available for display. Use 'F9' to display these three-
letter abbreviations. The 1000 brightest stars can be labelled by
using 'F8' to see more labels, and keep pressing it until the labels
disappear if you want to see fewer, or use 'Shift-F8'.
V3.0 of SkyGlobe has added the capability to display either an
outline or a filled region to represent the Milky Way. Press 'K' or
'Shift-K' to scroll through the levels of display, which affect the
types, brightnesses, and colors of the lines and regions.
Messier Objects
Labels for the Messier Object can be turned on or off with the
'F4' key. Use the Reference Card to learn the names of the important
objects.
-6-
Moving Around
SkyGlobe provides many convenient methods for rapidly changing
the sky view. The up and down arrow keys change the View Elevation
by 5 degrees. The right and left arrow keys work with the View
Direction. When the View Elevation is near the Horizon these keys
work about as you expect, but nearer to the Zenith they rotate the
view more than they move it. This is correct when you remember that
the View Direction stands for where your feet are pointing. PgUp and
PgDn change Elevation in multiple jumps. Use Alt or Ctrl with the
arrow keys to change the direction in smaller amounts. Finally, you can
change the View Direction instantly to compass points by pressing
'N', 'S', 'E' or 'W'.
What Do We See?
Lots and lots of stars! You can change the number of stars
displayed by pressing 'B' for Brightness to increase the number, or
'Shift-B' to decrease it. The number of stars added or deleted from
the display depends on the number currently displayed.
SkyGlobe allows you to adjust the magnification of your sky
view. At a nominal magnification of 1, with the Inflated projection
chosen, (this is the new program default) half of the celestial sphere
is visible. Since the eye can focus on far less area than this, a
certain amount of distortion is evident at low magnifications. Still,
you can use these views to quickly find areas of interest. The center
of the screen is always the most accurate portion. Use 'Z' to increase
the magnification and 'Shift-Z' to decrease it.
Keeping Track
SkyGlobe has two handy on-screen displays to help the user. The
left-hand display will help you keep track of settings such as the Zoom
Index, and will remind you of the Viewing Location. By pressing 'F2' you
can see the Auto-Increment parameters, the Print parameters and other
miscellaneous information. This display can be blanked by pressing 'F2'
yet again, or use 'Shift-F2' to peel off one screen at a time.
A Help screen appears on the right-hand side of the screen. This
display will remind you of the single-key commands of SkyGlobe. Press
'F1', and the function key assignments appear (on non-CGA machines) One
more 'F1', and the list of alternate function keys shows up. Press 'F1'
again to turn off the Help display.
-7-
The Planets
You can use SkyGlobe to learn something about the way the
planets move around the Sun. The very word 'Planet' is derived from
the Greek word for wanderer. The ancients, who spent more time out-
of-doors than we do, noticed that a few bright 'stars' seemed to
move against the 'fixed' background of the rest of the heavens.
(Here I mean fixed with respect to each other; they were acquainted
with the slow progression from one season to the next of the whole
'sphere'.) They soon worked out the repetitive patterns the diff-
erent 'stars' followed. We will learn how to simulate this motion
shortly, but first we need to talk about some SkyGlobe features that
are relevant.
Although the stars don't really change from one year to the next,
the planets do. Notice the year displayed on the Date display in the
upper left-hand corner. If this Time and Date are not displayed, press
'F2' to turn this display on. Use 'Y' or 'Sh-Y' to increase or decrease
the year. These planetary positions are now calculated on the fly in
SkyGlobe 3.0. This is a bit slower and less accurate than previous ver-
sions of SkyGlobe, but the added flexibility of dispensing with the
data files is more than worth it. You can use 'F3' to turn on the planet
display, and to turn on planet labels. EGA/VGA color users see the planets
in more or less appropriate colors. You may need to change the Time or
Date to see your favorite planet.
Now that we have seen the planets, let's see how they move. Change
the Viewing Direction to South and the Time to 12:00 noon. Turn off
Daylight Time by pressing 'V'. Set Auto-Increment Type to Date by
pressing 'Alt-A' if needed. Now press 'A' and watch the show. If you
want to see how the planets stick near the ecliptic, make sure its
display is turned, by pressing 'F6' if needed. Since your location
may not fall exactly on the Standard Time meridian, the Sun may not
be due South for you at Civil noon. Also notice how it wanders from
side to side throughout the year.
Notice how Mercury and Venus stay close to the Sun. Mars has
positively weird behavior, since it is outside the Earth's orbit, but
relatively close by. It also has an eccentric orbit. The other outside
planets drift more slowly against the background of the stars. You
may see more clearly how the moon goes through its phases, being al-
ways in New Moon phase when near the Sun. Move to Midnight, and the
Moon will be in Full phase when it shows up in the South. Since the
orbit of the Moon is inclined at about 5 degrees to the ecliptic, it
wanders above and below it each month. This motion, which rotates
through an 18 year cycle, accounts for the periodicity of eclipses.
SkyGlobe 3.0 uses calculated planetary positions to allow for planet
display without the need for data tables. For instance, take a look
at the solar eclipse of July 11, 1991. Slowly step through the hours,
and watch how the moon gradually overtakes the Sun. Currently the years
are limited to the range 1900-2099, but this range will be greatly ex-
panded shortly.
-8-
What Is A Toggle?
Many of the display features in SkyGlobe can be instantly
turned off or turned back on by pressing a single function key.
A list follows.
F5-Horizon line F9-Constellation Labels
F6-Ecliptic line F10-Constellation Lines
We haven't yet discussed a few features mentioned in the above
function key list. SkyGlobe can display Right Ascension, Declination
and Ecliptic lines to help you orient yourself on the celestial sphere.
Notice how the Ecliptic passes through the constellations of the
Zodiac, and how Orion lies right across the celestial equator.
Try looking north with Auto-Increment mode on. Watch how the sphere
appears to rotate, and how Polaris, very near the celestial pole,
seems almost motionless.
Using the Alt-key in conjunction with the function keys can be
used to control some of the more obscure parameters in SkyGlobe 3.0.
Alt-F1 reduces the display to stars and constellation lines only.
Alt-F2 reduces the display to stars only.
Alt-F3 gradually changes the background color from black to blue.
Alt-F5 turns off the mouse position display, independently of the
F2 Parameter Index. This makes mouse centering impossible.
Alt-F6 toggles the Precession flag. With current range of only 200
years, this in not all that valuable, but it does work.
Alt-F7 toggles the printer port from LPT1 to LPT2.
Alt-F8 controls whether line feeds are added to carriage returns
while printing.
Special Command Modes
The SPACE bar, Home and End keys, and Alt and Ctrl keys, have special
meaning in V3.0, as described on the Reference Card. The SPACE bar acti-
vates Turbo mode, which takes the next keypress and continually feeds it
into the program, until the SPACE bar is pressed again. The Home and End
keys, for many commands, take the next keypress, and either minimize or
maximize the program parameter altered by that key. The Alt and Ctrl keys
often work as very small positive and negative increments for the command
with which they are used. To illustrate this, press Home, followed by 'Z',
to reset the Zoom Index to 1. You will have noticed that you were prompted
to enter the command to be used with the Home feature. Now, press the SPACE
bar. You will be prompted to enter the Turbo key. Let's use the Alt feature
here. Hold down the Alt key, and press 'Z'. The display will slowly begin
to expand, and a message on the bottom of the screen will remind you to
press the SPACE bar when you wish to exit Turbo mode.
-9-
Finding Stars And Constellations
Let's say you wish to find a planet, or perhaps your favorite
constellation. Press 'F' to access the Find menu. Use the cursor keys
to navigate the menus, using PgDn and PgUp to choose other pages for
other types of Objects. The display will be re-centered at the chosen
object, if it is visible from your latitude. If necessary, the time will
be incremented until the object is above the horizon. The next time
you use the menus, the last chosen object will be under the cursor.
I would like to say a few words here about nomenclature. The
names of the constellations are well standardized. Many of the
strange names in the southern sky are Latinized names of scientific
implements, since these constellations were named, (by the Western
world, that is), in the beginning of the Industrial Age. Most of the
northern constellation names go back much further. We use the genitive,
or possessive, form of the constellation name to denote star names.
For example, Alpha Centauri means the first star of Centaurus. The
stars were generally enumerated in order of brightness. Since star
brightnesses change with time, this correlation is not always exact.
Many stars also have popular names, which are not standardized nearly
as well as constellations. Most of the names are Arabic in origin.
This reflects the fact that the Arabic world maintained and developed
astronomical knowledge while Europe was struggling through the Dark
Ages. You may want to take my lists with a grain of salt. Fifty-seven
stars have been chosen for celestial navigation purposes by the various
authorities, and labels for these stars appear in a different color
in EGA and VGA color modes.
-10-
Changing Viewing Locations
One of the most popular pastimes for new astronomers is seeing
what the sky looks like from other places. Perhaps you're thinking
of moving, and want to make sure the stars will still be interesting
to view from your prospective new home. (They will be!) Rather than
quitting the program and choosing a different location from the menu,
simply press 'L'. Once you make your new choice you will return to
the program with all your other parameters just the way you left them.
Since SkyGlobe 3.0 now has over 230 locations, there are two pages
of locations to choose from. Use the 'End' key to quickly go to the
spot that changes between pages.
If you wish to move a small amount in a compass direction, try
'Alt-N', 'Alt-S', 'Alt-E' or 'Alt-W'. Then you can change locations
without ever taking your eyes off the current display. The east and
west moves simply have the effect of changing the local time by 1
minute. The north-south changes are 1/4 degree, about 17 miles. You
may instantly change your location between the North and South Hemi-
spheres by pressing 'Alt-F' to Flip between the two.
Changing Your Environment
No, this section has nothing to do with blowing up oil wells.
SkyGlobe 3.0 adds the capability to customize many program settings.
The file SKYGLOBE.REG allows you to specify three custom locations.
These locations will occupy the top three spots in the Location menu.
When your order was filled, your Home Town was placed in the top
spot, while Caledonia and Roscommon occupy the next two. If you move,
or you wish to change the second and third cities, you may use any
text editor to do so. But please be careful! Before you make any
changes, you should make a copy of the file. Then make certain you
don't change the lengths of any field or the whole file. The location
name, latitude, and longitude fields should be self-explanatory. The
first three characters refer to North-South, West-East, and Daylight
Time, respectively. Use 'N' or 'S', 'W' or 'E', and 'Y' or 'N' to
specify the hemispheres, and whether Daylight Time is used. The next
two characters refer to the time zone used. This number refers to the
number of half-hours around from the Greenwich meridian the standard
meridian for the time zone is. Use 10 for Eastern Time, 12 for Central,
14 for Mountain, and 16 for Pacific. European continental time is 46,
not -2 or anything. SKYGLOBE.REG also allows for the specification of
either DOT or LAS default printer types, and either HER, CGA, EGA, or
VGA default video types. If your order didn't say, I let the program
make its best guess. This can be overridden on the command line.
Use of the number keys allows for the saving of current program
settings. Up to 10 different settings may be saved, one of which will
be used as the new program default. These keys will create the file
SKYGLOBE.CF#, where # is a digit 0 through 9. When SkyGlobe is started,
it looks for the .CF0 file to get its initial settings. If you would
rather use the default settings, delete or REName this file. If you
want to use one of the other files, just use SKYGLOBE #, such as
SKYGLOBE 4 to use SKYGLOBE.CF4. This scheme allows for the use of
batch files, such as ECLIPSE.BAT=SKYGLOBE 1, where SKYGLOBE.CF1 has
been set up for July 11, 1991. These parameters can be mixed with video
choices, as long as you separate the parameters with spaces.
-11-
Printing
A snapshot of the screen may be printed with the use of the 'P'
command. You will be prompted to choose a printer type, and the output
will be directed to LPT1. No matter your video type, a display will be
created in VGA resolution for dot-matrix printing, or SVGA resolution
for HP-compatible laser printing.
What Else Is There?
Only a few miscellaneous tidbits remain. In VGA and SVGA color modes,
you can brighten or dim the colors with '+' and '-', and this bias can be
saved in the .CF0 file. The text color can be changed with '/'. The type
of Time display, either AM/PM or 24-hour, can be changed with '='. (I know
these particular keys are meaningless, I ran out of useful mnemonics.)
When Real-Time mode is active, an 'R' appears next to the time, or an 'S'
for Sidereal Time. Daylight time is indicated with a 'D'.
V3.0 of SkyGlobe now adds support for a mouse. The RA-Dec coordinates
of the mouse cursor, along with the name of any object underneath it, will
be displayed in the lower left-hand corner of the screen. If you wish to
re-center the display at the spot of the mouse cursor, press the button.
As long as the chosen spot is visible from your location at some time,
the spot under the mouse cursor will become the new center of the screen.
Pressing the right mouse button will return the screen to the position
before the left button was pressed.
SkyGlobe 3.0 now offers a new projection for displaying the sky,
which has become the default projection. It leaves the center, or more
accurate, portion of the original SkyGlobe projection intact, but
Inflates or stretches the edge portion, allowing for a more realistic
portrayal of shapes near the edge. Use 'I' to toggle between the new
and old projections.
Finally, press 'Q' or ESC to return to DOS.
Thanks For Your Support!
I hope you enjoy SkyGlobe! As a fully registered user, you
are encouraged to please pass it on to anyone who may find it
interesting. Registered Users will automatically hear about future
updates. Any suggestions you may have will be greatly appreciated.
I can be reached on CompuServe as 76207,3377, or in care of the
address on the order form.
Thanks, and have fun learning about the stars!
-12-
SkyGlobe and the Stars - Some Background Information
Why do we see different stars at different times? The Earth makes
one complete rotation every day. If there were no Sun we could see that
the stars appear to make one complete revolution at the same time. The
North Star, Polaris (#51), is almost directly above the North Pole on
the Earth's axis of rotation. So the stars near the North Star (about
halfway up the northern sky in mid-northern latitudes) make tiny little
circles every day. Farther away from the North Star the stars and the
constellations they form wheel across the sky in huge arcs before they
disappear below the horizon.
Why do we see different stars at different dates? Imagine midnight
in April. The Sun is behind the Earth, and you are facing away from it
if you face due south. Now imagine midnight in October, six months later.
You are still facing away from the Sun. But because the Earth has moved
halfway around the Sun in its yearly orbit, you are looking in exactly
the opposite direction to the one you were in April. So different stars
are visible at midnight, and the ones near the North Star have made half
a revolution. If there were no Sun, you could see that at noon the October
sky is the same as the midnight sky in April.
Before Standard Time Zones were instituted, the Sun was due south
at noon everywhere. That was what noon meant. Now that is true only if
you happen to live near the center of the time zone. If you live in
Michigan, the Sun is due south around 12:30 or so. In New York City,
which near the center line for the same time zone, the Sun reaches due
south a few minutes before noon, over a half hour earlier than in
Michigan. The Sun reaches due south somewhat later in Chicago than
in Michigan, but because Chicago is in the Central time zone this
occurs before 12:00PM. This has to be allowed for to make the display
correct, and is unique to each location. Daylight Saving Time is handled
in a similar manner, and is indicated on the Time Display by the letter
D before the time if Daylight is in use.
The sky can be viewed as a sphere with the Earth at the center, and
the stars as fixed points on the sphere. Any attempt to represent this
3-dimensional space on a 2-dimensional surface inevitably introduces
some distortion. SkyGlobe uses a unique projection that can be calculated
very rapidly and provides quite accurate rendering of shapes as they
appear in the sky, even near the edge of the display. The old ortho-
graphic projection used in earlier versions of SkyGlobe (and still
available through the use of the 'I' command) had fairly severe dis-
tortions near the edges, and was only slightly faster.
-13-
Background Continued
Another issue that must be dealt with is double stars. Perhaps as
many as half of all stars are actually multiple star systems. The naked
eye frequently interprets two dim stars close together as one brighter
star. Many 'stars' that serve as end-points on constellation lines fit
into this category. If these stars were left dim and separate they would
appear 'invisible' at low brightnesses and make constellation shapes
unrecognizable. At higher brightnesses and low magnifications these stars
would be plotted on top of one another as points, still artificially dim.
The solution is to combine magnitudes for these stars. The ordering of
stars in SkyGlobe reflects this combination, so at medium brightnesses
and magnifications the display is as realistic as possible. The dimmer
star is retained at its actual brightness, so at very high magnifications
and brightnesses you will see one artificially bright star and one correct
dim star.
SkyGlobe contains coordinates for 7000 stars in the file SKY7000.EXE.
This represents all the stars visible to the naked eye. These coordinates
were obtained from Sky Catalogue 2000.0 with permission from the publisher,
Sky Publishing Corp. This permission is gratefully appreciated. The files
SKY8000.DAT and SKY10000.DAT contain another 8000 and 10000 stars,
respectively.
SkyGlobe was programmed mostly in assembly language for maximum speed.
Since there is necessarily a tradeoff between speed and accuracy, the
precision of the star coordinates was carefully matched to the resolution
of the graphics display and the projection algorithm chosen.
Of course, no program is perfect. Any suggestions or bug reports
would be greatly appreciated, and if you have any problems getting this
new version up and running on your system, don't hesitate to contact me.
I can be reached at the address on the order form and Reference Card, or
on CompuServe at 76207,3377.
Thank you for supporting Shareware and...
S K Y G L O B E ! ! !
-14-
Some Frequently Asked Questions
How can I speed up SkyGlobe?
There are really two answers to this question. SkyGlobe always
does what you ask it to do as fast as it can. (We think it's pretty
fast!) The trick is to ask it to do things in a way that seems faster.
The first method involves asking SkyGlobe to do less work. Try
turning off everything you can do without, especially the Milky Way,
planets, and horizon line. Other possibilities: ecliptic, right
ascension and declination lines, extra constellation lines, and
dim stars. In addition, determining the location of the mouse
cursor tends to be a slow operation, so you may want to turn it
off by using 'F2' or 'Shift-F2'.
The second method applies only to Auto-Increment mode. SkyGlobe
starts off changing the view five minutes at a time. You can increase
this rate by pressing '>'. Another way is to change the increment type
to Date mode by pressing 'Alt-A', Then increase the Date increment rate
by pressing '>'.
Why doesn't anything happen when I press 'V'?
Either the date is not appropriate for Daylight Saving Time, or
you chose a location that does not use it.
Why do I get garbage when I try to print?
When you print the screen by choosing 'P', you will be prompted
to choose the appropriate printer type, either 9-pin, 24-pin, or
HP-compatible laser printing. The only difference between the two
dot-matrix modes is the line-spacing, and it is possible that the
9-pin choice will work better for some 24-pin printers. If you try
print in laser mode on a dot-matrix printer, or vice versa, the results
will be unsatisfactory. Printing on other devices, such as ink-jet or
bubble-jet printers, should work, as long as you choose the correct
mode that is emulated by your printer. If your printer is not connected
to LPT1, you will not be able to print.
Why does the screen go blank when I try to start SkyGlobe?
If you attempt to start SkyGlobe in a video mode that is not
supported by your system, the usual result is a blank screen, perhaps
with the DOS prompt changing color. You will usually be able to get
back to DOS by pressing 'Q'. If you are attempting to use SVGA, you
may want to try SKYGLOBE S2 instead of SKYGLOBE S. The normal mode
used for SVGA is the VESA standard, and you may need to load the VESA
driver that came with your video card before starting SkyGlobe. The
S2 mode is a commonly used non-VESA mode supported by many cards. More
SVGA support for other cards will be available soon; contact Klassm
Software for an update if you are still having trouble. Otherwise,
try working your way up from CGA to EGA to VGA mode, to see if the
program will work in one of these modes, with SKYGLOBE C, SKYGLOBE E,
and SKYGLOBE V. For a Hercules monochrome system, try SKYGLOBE H.
DEFINITION OF SHAREWARE
Shareware distribution gives users a chance to try software
before buying it. If you try a Shareware program and continue
using it, you are expected to register. Individual programs
differ on details -- some request registration while others
require it, some specify a maximum trial period. With
registration, you get anything from the simple right to continue
using the software to an updated program with printed manual.
Copyright laws apply to both Shareware and commercial software,
and the copyright holder retains all rights, with a few specific
exceptions as stated below. Shareware authors are accomplished
programmers, just like commercial authors, and the programs are
of comparable quality. (In both cases, there are good programs
and bad ones!) The main difference is in the method of
distribution. The author specifically grants the right to copy
and distribute the software, either to all and sundry or to a
specific group. For example, some authors require written
permission before a commercial disk vendor may copy their
Shareware.
Shareware is a distribution method, not a type of software. You
should find software that suits your needs and pocketbook,
whether it's commercial or Shareware. The Shareware system makes
fitting your needs easier, because you can try before you buy.
And because the overhead is low, prices are low also. Shareware
has the ultimate money-back guarantee -- if you don't use the
product, you don't pay for it.
DISCLAIMER - AGREEMENT
Users of SkyGlobe 3.0 must accept this disclaimer of warranty:
"SkyGlobe 3.0 is supplied as is. The author disclaims all
warranties, expressed or implied, including, without limitation,
the warranties of merchantability and of fitness for any purpose.
The author assumes no liability for damages, direct or conse-
quential, which may result from the use of SkyGlobe 3.0."
SkyGlobe 3.0 is a "shareware program" and is provided at no charge
to the user for evaluation. Feel free to share it with your
friends, but please do not give it away altered or as part of
another system. The essence of "user-supported" software is to
provide personal computer users with quality software without
high prices, and yet to provide incentive for programmers to
continue to develop new products. If you find this program
useful and find that you are using SkyGlobe 3.0 and continue to use
SkyGlobe 3.0 after a reasonable trial period, you must make a reg-
istration payment of $20 to Klassm Software. The $20
registration fee will license one copy for use on any one
computer at any one time. You must treat this software just like
a book. An example is that this software may be used by any
number of people and may be freely moved from one computer
location to another, so long as there is no possibility of it
being used at one location while it's being used at another.
Just as a book cannot be read by two different persons at the
same time.
Commercial users of SkyGlobe 3.0 must register and pay for their
copies of SkyGlobe 3.0 within 30 days of first use or their license
is withdrawn. Site-License arrangements may be made by con-
tacting Klassm Software.
Anyone distributing SkyGlobe 3.0 for any kind of remuneration must
first contact Klassm Software at the address below for authorization.
This authorization will be automatically granted to distributors
recognized by the (ASP) as adhering to its guidelines for
shareware distributors, and such distributors may begin offering
SkyGlobe 3.0 immediately (However Klassm Software must still be
advised so that the distributor can be kept up-to-date with the
latest version of SkyGlobe 3.0.).
You are encouraged to pass a copy of SkyGlobe 3.0 along to your
friends for evaluation. Please encourage them to register their
copy if they find that they can use it. All registered users
will receive a copy of the latest version of the SkyGlobe 3.0
system.