StellarWindowUsers' GuideStar display and setting


Click the ‘Tool’ icon located on the toolbar to open the setting dialog. Select “Stars” in the left column to open the star setting pane.

Star display modes

The main StellarWindow star catalog is called the “Hipparcos and Tycho2 Catalog” containing approximately 2.6 million stars covering up to those of the 16th magnitude. There are two different display modes to display these stars: Photo Simulation Mode and Actual View Mode. When using StellarWindow in the Standard Mode, the Photo Simulation Mode is set by default while the Actual View Mode is set when using StellarWindow in the Light Mode.

Actual View Mode
With this mode, the magnitudes of the stars recorded in the star chart are accurately reproduced to enable the actual view of the starry sky to be reproduced. An applicable darkest magnitude*1can be specified optionally. It is reported that setting the darkest magnitude within the range of 2 to 3 is suitable to reproduce the actual starry sky observed in Tokyo. The tones of the Milky Way photos (designed to be used as the screen background) and the photos of nebulas and star clusters are quite dark as a result of the reproduction of the actual view. The Actual View Mode is the default display mode when using StellarWindow in the Light Mode. In addition to achieve light operations, this mode is also useful to reproduce the actual starry sky and to use StellarWindow solely to perform celestial body searches.

Photo Simulation Mode
In order to reproduce a photo of the starry sky, this mode simulates the photo shooting process of the starry sky by means of calculations. While an optional darkest magnitude cannot be specified with this mode *2, a parameter ranging from 1.0 to 2.0*3 can be selected to specify the amount of stars subject to display. The default parameter is set at 1.4. The larger this figure becomes the greater the amount of stars becomes apparently. It is also the case that the larger this figure becomes the brighter the stars become apparently. After changing the parameter value, click the “Recalculation” button to confirm the new value. It may take some time to complete the recalculation procedure. The photos of the Milky Way, nebulas and star clusters are displayed with almost no darkening effect. The Photo Simulation Mode is the default display mode when using Stellar- Window in the Standard Mode.

Overlay display of star names and Bayer codes

By default, the names and Bayer codes of the stars displayed do not appear on the screen. Tick the boxes “Overlay star name” and “Overlay Bayer code” locating on the “Display setting” screen so that the common names and Bayer codes of the stars displayed are overlaid on the images appearing on the main screen.
Light green are set as the default overlay display colors to describe star names and Bayer codes. As shown in the screenshot below, optional colors can be selected by clicking the “Color well” located on the setting screen.

Screenshot showing the stars’ names and Bayer codes overlaid on the images
As the initial setting, no information is overlaid on the images appearing on the screen. The display setting for star names and Bayer codes can be carried out separately.

 Light greenare set as the default overlay display colors to describe star names and Bayer codes. As shown in the screenshot below, optional colors can be selected by clicking the “Color well” located on the setting screen.

Click the Color well button to open the color selection dialog.
Using the color selection dialog, the desired color can be selected by clicking the color spectrum or inputting a numeric figure ranging from ‘0’ to ‘255’ applicable individually to the shades of red, green and blue.

Memory saving setting (for experienced users)

The amount of stars to be loaded into the star chart can be restricted for the purpose of memory saving. This is able to save a maximum of approximately 80MB memory capacity. In the Light Mode, the maximum memory saving setting is enabled by default while this is not the case of the Standard Mode.


Memory saving setting
The memory saving setting screen. It is recommended only for experienced users to change the memory saving setting.

When specifying the darkest magnitude of stars subject to display, the memory capacity required is exhibited in the bottom of the setting screen. Click the “Setting” button so that the darkest magnitude specified is recorded. Restart StellarWindow to enable the new memory saving setting.


*1 Setting of the darkest magnitude
A magnitude of the darkest stars can be specified optionally. The smaller the magnitude becomes the brighter the stars become. The default darkest magnitude is set at 7.0. Stars darker than those of the 7th magnitude (=stars of magnitudes that are larger than 7.0) are therefore not displayed. It may be necessary to specify a magnitude smaller than 7.0 when reproducing the actual view of the starry sky observed in a big city such as Tokyo.

*2 Darkest magnitude setting applicable to the Photo Simulation Mode
While there is no direct setting dialog,the darkest magnitude applicable when using the Photo Simulation Mode can be specified through a different setting feature. To achieve this, enable the memory saving feature (explained later in this
section) and specify the darkest magnitude so that any stars of magnitudes darker than the darkest magnitude specified are not loaded. In this manner, the darkest magnitude applicable to the memory saving feature works as that applicable to photo simulation calculations. This allows the user using a PC with a limited memory capacity or low specifications to use the Photo Simulation Mode.

*3 Parameters designed to determine the amount of stars subject to display
In principle, parameters designed to determine the amount of stars to be displayed on the screen are in proportion with the photo shooting exposure time. StellarWindows’ photo simulation calculation process however adopts photology differing from that applicable to the actual photo shooting (i.e. stars that are too bright are peaked out with StellarWindow). These parameters are therefore not strictly in proportion with the photo shooting exposure time.

 
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